Sample records for academies keck futures
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Advances in instrumentation at the W. M. Keck Observatory
Adkins, Sean M.; Armandroff, Taft E.; Johnson, James; Lewis, Hilton A.; Martin, Christopher; McLean, Ian S.; Wizinowich, Peter
2012-09-01
In this paper we describe both recently completed instrumentation projects and our current development efforts in terms of their role in the strategic plan, the key science areas they address, and their performance as measured or predicted. Projects reaching completion in 2012 include MOSFIRE, a near IR multi-object spectrograph, a laser guide star adaptive optics facility on the Keck I telescope, and an upgrade to the guide camera for the HIRES instrument on Keck I. Projects in development include a new seeing limited integral field spectrograph for the visible wavelength range called the Keck Cosmic Web Imager (KCWI), an upgrade to the telescope control systems on both Keck telescopes, a near-IR tip/tilt sensor for the Keck I adaptive optics system, and a new grating for the OSIRIS integral field spectrograph.
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Morrissey, Patrick; KCWI Team
2013-01-01
The Keck Cosmic Web Imager (KCWI) is a new facility instrument being developed for the W. M. Keck Observatory and funded for construction by the Telescope System Instrumentation Program (TSIP) of the National Science Foundation (NSF). KCWI is a bench-mounted spectrograph for the Keck II right Nasmyth focal station, providing integral field spectroscopy over a seeing-limited field up to 20"x33" in extent. Selectable Volume Phase Holographic (VPH) gratings provide high efficiency and spectral resolution in the range of 1000 to 20000. The dual-beam design of KCWI passed a Preliminary Design Review in summer 2011. The detailed design of the KCWI blue channel (350 to 700 nm) is now nearly complete, with the red channel (530 to 1050 nm) planned for a phased implementation contingent upon additional funding. KCWI builds on the experience of the Caltech team in implementing the Cosmic Web Imager (CWI), in operation since 2009 at Palomar Observatory. KCWI adds considerable flexibility to the CWI design, and will take full advantage of the excellent seeing and dark sky above Mauna Kea with a selectable nod-and-shuffle observing mode. The KCWI team is lead by Caltech (project management, design and implementation) in partnership with the University of California at Santa Cruz (camera optical and mechanical design) and the W. M. Keck Observatory (program oversight and observatory interfaces).
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New developments in instrumentation at the W. M. Keck Observatory
Adkins, Sean M.; Armandroff, Taft E.; Fitzgerald, Michael P.; Johnson, James; Larkin, James E.; Lewis, Hilton A.; Martin, Christopher; Matthews, Keith Y.; Prochaska, J. X.; Wizinowich, Peter
2014-07-01
The W. M. Keck Observatory continues to develop new capabilities in support of our science driven strategic plan which emphasizes leadership in key areas of observational astronomy. This leadership is a key component of the scientific productivity of our observing community and depends on our ability to develop new instrumentation, upgrades to existing instrumentation, and upgrades to supporting infrastructure at the observatory. In this paper we describe the as measured performance of projects completed in 2014 and the expected performance of projects currently in the development or construction phases. Projects reaching completion in 2014 include a near-IR tip/tilt sensor for the Keck I adaptive optics system, a new center launch system for the Keck II laser guide star facility, and NIRES, a near-IR Echelle spectrograph for the Keck II telescope. Projects in development include a new seeing limited integral field spectrograph for the visible wavelength range called the Keck Cosmic Web Imager, a deployable tertiary mirror for the Keck I telescope, upgrades to the spectrograph detector and the imager of the OSIRIS instrument, and an upgrade to the telescope control systems on both Keck telescopes.
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Energy Technology Data Exchange (ETDEWEB)
Ade, P. A. R. [School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA (United Kingdom); Aikin, R. W.; Bock, J. J.; Brevik, J. A.; Filippini, J. P.; Golwala, S. R.; Hildebrandt, S. R.; Hui, H. [Department of Physics, California Institute of Technology, Pasadena, CA 91125 (United States); Barkats, D. [Joint ALMA Observatory, ESO, Santiago (Chile); Benton, S. J. [Department of Physics, University of Toronto, Toronto, ON (Canada); Bischoff, C. A.; Bradford, K. J.; Buder, I. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, MA 02138 (United States); Bullock, E. [Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, MN 55455 (United States); Dowell, C. D. [Jet Propulsion Laboratory, Pasadena, CA 91109 (United States); Duband, L. [Université Grenoble Alpes, CEA INAC-SBT, F-38000 Grenoble (France); Fliescher, S. [Department of Physics, University of Minnesota, Minneapolis, MN 55455 (United States); Halpern, M.; Hasselfield, M. [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC (Canada); Hilton, G. C., E-mail: avieregg@kicp.uchicago.edu [National Institute of Standards and Technology, Boulder, CO 80305 (United States); Collaboration: bicep2 and Keck Array Collaborations; and others
2015-06-20
bicep2 and the Keck Array are polarization-sensitive microwave telescopes that observe the cosmic microwave background (CMB) from the South Pole at degree angular scales in search of a signature of inflation imprinted as B-mode polarization in the CMB. bicep2 was deployed in late 2009, observed for three years until the end of 2012 at 150 GHz with 512 antenna-coupled transition edge sensor bolometers, and has reported a detection of B-mode polarization on degree angular scales. The Keck Array was first deployed in late 2010 and will observe through 2016 with five receivers at several frequencies (95, 150, and 220 GHz). bicep2 and the Keck Array share a common optical design and employ the field-proven bicep1 strategy of using small-aperture, cold, on-axis refractive optics, providing excellent control of systematics while maintaining a large field of view. This design allows for full characterization of far-field optical performance using microwave sources on the ground. Here we describe the optical design of both instruments and report a full characterization of the optical performance and beams of bicep2 and the Keck Array at 150 GHz.
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Energy Technology Data Exchange (ETDEWEB)
Ade, P.A.R.; Aikin, R.W.; Barkats, D.; Benton, S.J.; Bischoff, C.A.; Bock, J.J.; Bradford, K.J.; Brevik, J.A.; Buder, I.; Bullock, E.; Dowell, C.D.; Duband, L.; Filippini, J.P.; Fliescher, S.; Golwala, S.R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S.R.; Hilton, G.C.; Hui, H.; Irwin, K.D.
2015-06-18
bicep2/KECK ARRAY. IV. OPTICAL CHARACTERIZATION AND PERFORMANCE OF THE bicep2 AND KECK ARRAY EXPERIMENTS P. A. R. Ade1, R. W. Aikin2, D. Barkats3, S. J. Benton4, C. A. Bischoff5, J. J. Bock2,6, K. J. Bradford5, J. A. Brevik2, I. Buder5, E. Bullock7Show full author list Published 2015 June 18 • © 2015. The American Astronomical Society. All rights reserved. The Astrophysical Journal, Volume 806, Number 2 Article PDF Figures Tables References Citations 273 Total downloads Cited by 6 articles Turn on MathJax Share this article Get permission to re-use this article Article information Abstract bicep2 and the Keck Array are polarization-sensitive microwave telescopes that observe the cosmic microwave background (CMB) from the South Pole at degree angular scales in search of a signature of inflation imprinted as B-mode polarization in the CMB. bicep2 was deployed in late 2009, observed for three years until the end of 2012 at 150 GHz with 512 antenna-coupled transition edge sensor bolometers, and has reported a detection of B-mode polarization on degree angular scales. The Keck Array was first deployed in late 2010 and will observe through 2016 with five receivers at several frequencies (95, 150, and 220 GHz). bicep2 and the Keck Array share a common optical design and employ the field-proven bicep1 strategy of using small-aperture, cold, on-axis refractive optics, providing excellent control of systematics while maintaining a large field of view. This design allows for full characterization of far-field optical performance using microwave sources on the ground. Here we describe the optical design of both instruments and report a full characterization of the optical performance and beams of bicep2 and the Keck Array at 150 GHz.
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Faculty Unions, Business Models, and the Academy's Future
Rhoades, Gary
2011-01-01
In this article, the author addresses questions about the future of faculty unions, business models, and the academy by providing some current and historical context regarding the causes of and conflicts about faculty unions. He also reviews trends in college and university management over the past three decades, using California, Ohio, and…
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Automating OSIRIS Data Reduction for the Keck Observatory Archive
Holt, J.; Tran, H. D.; Goodrich, R.; Berriman, G. B.; Gelino, C. R.; KOA Team
2014-05-01
By the end of 2013, the Keck Observatory Archive (KOA) will serve data from all active instruments on the Keck Telescopes. OSIRIS (OH-Suppressing Infra-Red Imaging Spectrograph), the last active instrument to be archived in KOA, has been in use behind the (AO) system at Keck since February 2005. It uses an array of tiny lenslets to simultaneously produce spectra at up to 4096 locations. Due to the complicated nature of the OSIRIS raw data, the OSIRIS team developed a comprehensive data reduction program. This data reduction system has an online mode for quick real-time reductions, which are used primarily for basic data visualization and quality assessment done at the telescope while observing. The offline version of the data reduction system includes an expanded reduction method list, does more iterations for a better construction of the data cubes, and is used to produce publication-quality products. It can also use reconstruction matrices that are developed after the observations were taken, and are more refined. The KOA team is currently utilizing the standard offline reduction mode to produce quick-look browse products for the raw data. Users of the offline data reduction system generally use a graphical user interface to manually setup the reduction parameters. However, in order to reduce and serve the 200,000 science files on disk, all of the reduction parameters and steps need to be fully automated. This pipeline will also be used to automatically produce quick-look browse products for future OSIRIS data after each night's observations. Here we discuss the complexities of OSIRIS data, the reduction system in place, methods for automating the system, performance using virtualization, and progress made to date in generating the KOA products.
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Drummond, Jack D.; Conrad, Al; Reddy, Vishnu; de Kleer, Katherine R.; Adamkovics, Mate; de Pater, Imke; Merline, William J.; Tamblyn, Peter
2016-10-01
Adaptive optics (AO) images of asteroid (16) Psyche obtained at 4 epochs with the NIRC2 camera at the 10m W. M. Keck Observatory (Keck II) on UT 2015 December 25 lead to triaxial ellipsoid diameters of 279±4 x 230±2 x 195±14 km, and a rotational pole at RA=29° and Dec=-2°. Adding 6 more epochs obtained nearly simultaneously with the OSIRIS system at Keck I, as well as two more epochs from Keck II in 2009, yields diameters of 273±2 x 232±2 x 165±3 km, and a pole at RA=37° and Dec=+1°. (Errors are formal fit parameter uncertainties; an additional 4% uncertainty is possible from systematic biases.) The differing perspectives between 2015 (sub-Earth latitude Θ=-50°) and 2009 (Θ=-6°) improves primarily the c dimension and the location of the rotational pole, but illustrates how well images from even a single night can determine the size, shape, and pole of an asteroid. The 2015 observations were obtained as part of a campaign to study Psyche with many techniques over a few months, including radar from Arecibo and images from Magellan.These handful of images show the same rugged outline as the radius vector model available on the DAMIT website, constructed from many lightcurves and scaled by previous Keck AO images. In fact Psyche has rotated some 125,350 times between the first lightcurve in 1955 and our 2015 AO images, exactly 60 years apart to the day. Since the asteroid has such a high obliquity, these lightcurves have scanned well into both northern and southern hemispheres. The difference between the pole derived from our images and the radius vector model pole is only 7°, and the mean diameters of Psyche are 219 and 211 km, respectively.
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Remote observing with the Keck Telescopes from the U.S. mainland
Kibrick, Robert I.; Allen, Steve L.; Conrad, Albert
2000-06-01
We describe the current status of efforts to establish a high-bandwidth network from the U.S. mainland to Mauna Kea and a facility in California to support Keck remote observing and engineering via the Internet. The California facility will be an extension of the existing Keck remote operations facility located in Waimea, Hawaii. It will be targeted towards short-duration observing runs which now comprise roughly half of all scheduled science runs on the Keck Telescope. Keck technical staff in Hawaii will support remote observers on the mainland via video conferencing and collaborative software tools. Advantages and disadvantages of remote operation from California versus Hawaii are explored, and costs of alternative communication paths examined. We describe a plan for a backup communications path to protect against failure of the primary network. Alternative software models for remote operation are explored, and recent operational results described.
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Anatomy of the academy: Dissecting the past, resecting the future
Daniel R. Williams
2000-01-01
Offered the opportunity to write about whatever topic moves me, I decided my millennial issue is to examine the place of leisure studies in higher education. Having recently left the academy after putting in 15 years at three different universities (most recently, the University of Illinois), affords me certain liberty to explore my thoughts on the future of the field...
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Performance of the Keck Observatory adaptive-optics system.
van Dam, Marcos A; Le Mignant, David; Macintosh, Bruce A
2004-10-10
The adaptive-optics (AO) system at the W. M. Keck Observatory is characterized. We calculate the error budget of the Keck AO system operating in natural guide star mode with a near-infrared imaging camera. The measurement noise and bandwidth errors are obtained by modeling the control loops and recording residual centroids. Results of sky performance tests are presented: The AO system is shown to deliver images with average Strehl ratios of as much as 0.37 at 1.58 microm when a bright guide star is used and of 0.19 for a magnitude 12 star. The images are consistent with the predicted wave-front error based on our error budget estimates.
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Keck-I MOSFIRE Spectroscopy of the z ~ 12 Candidate Galaxy UDFj-39546284
Capak, P.; Faisst, A.; Vieira, J. D.; Tacchella, S.; Carollo, M.; Scoville, N. Z.
2013-08-01
We report the results of deep (4.6 hr) H-band spectroscopy of the well studied z ~ 12 H-band dropout galaxy candidate UDFj-39546284 with MOSFIRE on Keck-I. These data reach a sensitivity of 5-10 × 10-19 erg s-1 cm-2 per 4.4 Å resolution element between sky lines. Previous papers have argued that this source could either be a large equivalent width line emitting galaxy at 2 dropout candidates in our mask and find no significant detections. The data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
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Long wavelength infrared camera (LWIRC): a 10 micron camera for the Keck Telescope
Energy Technology Data Exchange (ETDEWEB)
Wishnow, E.H.; Danchi, W.C.; Tuthill, P.; Wurtz, R.; Jernigan, J.G.; Arens, J.F.
1998-05-01
The Long Wavelength Infrared Camera (LWIRC) is a facility instrument for the Keck Observatory designed to operate at the f/25 forward Cassegrain focus of the Keck I telescope. The camera operates over the wavelength band 7-13 {micro}m using ZnSe transmissive optics. A set of filters, a circular variable filter (CVF), and a mid-infrared polarizer are available, as are three plate scales: 0.05``, 0.10``, 0.21`` per pixel. The camera focal plane array and optics are cooled using liquid helium. The system has been refurbished with a 128 x 128 pixel Si:As detector array. The electronics readout system used to clock the array is compatible with both the hardware and software of the other Keck infrared instruments NIRC and LWS. A new pre-amplifier/A-D converter has been designed and constructed which decreases greatly the system susceptibility to noise.
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Conrad, A. R.; Lupton, W. F.
1992-01-01
Each Keck instrument presents a consistent software view to the user interface programmer. The view consists of a small library of functions, which are identical for all instruments, and a large set of keywords, that vary from instrument to instrument. All knowledge of the underlying task structure is hidden from the application programmer by the keyword layer. Image capture software uses the same function library to collect data for the image header. Because the image capture software and the instrument control software are built on top of the same keyword layer, a given observation can be 'replayed' by extracting keyword-value pairs from the image header and passing them back to the control system. The keyword layer features non-blocking as well as blocking I/O. A non-blocking keyword write operation (such as setting a filter position) specifies a callback to be invoked when the operation is complete. A non-blocking keyword read operation specifies a callback to be invoked whenever the keyword changes state. The keyword-callback style meshes well with the widget-callback style commonly used in X window programs. The first keyword library was built for the two Keck optical instruments. More recently, keyword libraries have been developed for the infrared instruments and for telescope control. Although the underlying mechanisms used for inter-process communication by each of these systems vary widely (Lick MUSIC, Sun RPC, and direct socket I/O, respectively), a basic user interface has been written that can be used with any of these systems. Since the keyword libraries are bound to user interface programs dynamically at run time, only a single set of user interface executables is needed. For example, the same program, 'xshow', can be used to display continuously the telescope's position, the time left in an instrument's exposure, or both values simultaneously. Less generic tools that operate on specific keywords, for example an X display that controls optical
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Near-Infrared Keck Interferometer and IOTA Closure Phase Observations of Wolf-Rayet stars
Rajagopal, J.; Wallace, D.; Barry, R.; Richardson, L. J.; Traub, W.; Danchi, W. C.
We present first results from observations of a small sample of IR-bright Wolf-Rayet stars with the Keck Interferometer in the near-infrared, and with the IONIC beam three-telescope beam combiner at the Infrared and Optical Telescope Array (IOTA) observatory. The former results were obtained as part of shared-risk observations in commissioning the Keck Interferometer and form a subset of a high-resolution study of dust around Wolf-Rayet stars using multiple interferometers in progress in our group. The latter results are the first closure phase observations of these stars in the near-infrared in a separated telescope interferometer. Earlier aperture-masking observations with the Keck-I telescope provide strong evidence that dust-formation in late-type WC stars are a result of wind-wind collision in short-period binaries.Our program with the Keck interferometer seeks to further examine this paradigm at much higher resolution. We have spatially resolved the binary in the prototypical dusty WC type star WR 140. WR 137, another episodic dust-producing star, has been partially resolved for the first time, providing the first direct clue to its possible binary nature.We also include WN stars in our sample to investigate circumstellar dust in this other main sub-type of WRs. We have been unable to resolve any of these, indicating a lack of extended dust.Complementary observations using the MIDI instrument on the VLTI in the mid-infrared are presented in another contribution to this workshop.
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The Operation and Architecture of the Keck Observatory Archive
Berriman, G. B.; Gelino, C. R.; Laity, A.; Kong, M.; Swain, M.; Holt, J.; Goodrich, R.; Mader, J.; Tran, H. D.
2014-05-01
The Infrared Processing and Analysis Center (IPAC) and the W. M. Keck Observatory (WMKO) are collaborating to build an archive for the twin 10-m Keck Telescopes, located near the summit of Mauna Kea. The Keck Observatory Archive (KOA) takes advantage of IPAC's long experience with managing and archiving large and complex data sets from active missions and serving them to the community; and of the Observatory's knowledge of the operation of its sophisticated instrumentation and the organization of the data products. By the end of 2013, KOA will contain data from all eight active observatory instruments, with an anticipated volume of 28 TB. The data include raw science and observations, quick look products, weather information, and, for some instruments, reduced and calibrated products. The goal of including data from all instruments is the cumulation of a rapid expansion of the archive's holdings, and already data from four new instruments have been added since October 2012. One more active instrument, the integral field spectrograph OSIRIS, is scheduled for ingestion in December 2013. After preparation for ingestion into the archive, the data are transmitted electronically from WMKO to IPAC for curation in the physical archive. This process includes validation of the science and content of the data and verification that data were not corrupted in transmission. The archived data include both newly-acquired observations and all previously acquired observations. The older data extends back to the date of instrument commissioning; for some instruments, such as HIRES, these data can extend as far back as 1994. KOA will continue to ingest all newly obtained observations, at an anticipated volume of 4 TB per year, and plans to ingest data from two decommissioned instruments. Access to these data is governed by a data use policy that guarantees Principal Investigators (PI) exclusive access to their data for at least 18 months, and allows for extensions as granted by
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Latest Results from the Multi-Object Keck Exoplanet Tracker
Van Eyken, Julian C.; Ge, J.; Wan, X.; Zhao, B.; Hariharan, A.; Mahadevan, S.; DeWitt, C.; Guo, P.; Cohen, R.; Fleming, S. W.; Crepp, J.; Warner, C.; Kane, S.; Leger, F.; Pan, K.
2006-12-01
The W. M. Keck Exoplanet Tracker is a precision Doppler radial velocity instrument based on dispersed fixed-delay interferometry (DFDI) which takes advantage of the new technique to allow multi-object RV surveying. Installed at the 2.5m Sloan telescope at Apache Point Observatory, the combination of Michelson interferometer and medium resolution spectrograph allows design for simultaneous Doppler measurements of up to 60 targets, while maintaining high instrument throughput. Using a single-object prototype of the instrument at the Kitt Peak National Observatory 2.1m telescope, we previously discovered a 0.49MJup planet, HD 102195b (ET-1), orbiting with a 4.11d period, and other interesting targets are being followed up. From recent trial observations, the Keck Exoplanet Tracker now yields 59 usable simultaneous fringing stellar spectra, of a quality sufficient to attempt to detect short period hot-Jupiter type planets. Recent engineering improvements reduced errors by a factor of 2, and typical photon limits for stellar data are now at the 30m/s level for magnitude V 10.5 (depending on spectral type and v sin i), with a best value of 6.9m/s at V=7.6. Preliminary RMS precisions from solar data (daytime sky) are around 10m/s over a few days, with some spectra reaching close to their photon limit of 6-7m/s on the short term ( 1 hour). A number of targets showing interesting RV variability are currently being followed up independently. Additional engineering work is planned which should make for further significant gains in Doppler precision. Here we present the latest results and updates from the most recent engineering and observing runs with the Keck ET.
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Joint Analysis of BICEP2/Keck Array and Planck Data
DEFF Research Database (Denmark)
Ade, P. A. R.; Aghanim, N.; Ahmed, Z.
2015-01-01
We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg2 patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck...... GHz to a lensed-ΛCDM model that includes dust and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r), using a prior on the frequency spectral behavior of polarized dust emission from previous Planck analysis of other regions of the sky. We...... present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for r, and yields an upper limit r 0.05
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Two Decades (almost) of Keck Observations of Io
De Pater, I.; Davies, A. G.; de Kleer, K.
2015-12-01
We have regularly observed Io with the 10-m Keck Telescope since 1998, initially using the speckle imaging technique, and switching to Adaptive Optics techniques when this became available in 2001. In this talk we will discuss several eruptions that we witnessed, and present 20-30 year timelines of thermal emission from Pele, Pillan, Janus Patera, Kanehekili Fluctus, and Loki Patera, updating timelines in recent publications [1, 2] with additional Keck adaptive optics data obtained between 2002 and 2015. These new timelines are the most comprehensive plots ever produced of the volcanic thermal emission variability for these or any other locations on Io, utilizing data from multiple ground- and space-based assets. Our continuing multi-decadal observing program forms the basis for charting the variability of Io's volcanic activity, of great importance for understanding the evolution of the Galilean satellite system, and with the expectation of new missions to the jovian system in the next decade. Acknowledgements: This research is in part supported by NSF grant AST-1313485 to UC Berkeley. AGD is supported by a grant from the NASA OPR Program. References: [1] Davies et al. (2012) Icarus, 221, 466-470. [2] Rathbun and Spencer (2010) Icarus, 209, 625-630.
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Keck/HIRES Spectroscopy of V838 Monocerotis in October 2005
Kamiński, T.; Schmidt, M.; Tylenda, R.; Konacki, M.; Gromadzki, M.
2009-05-01
V838 Monocerotis (V838 Mon) erupted at the beginning of 2002 becoming an extremely luminous star with L sime 106 L sun. Among various scenarios proposed to explain the nature of the outburst, the most promising is a stellar merger event. In this paper, we investigate the observational properties of the star and its surroundings in the post outburst phase. We have obtained a high-resolution optical spectrum of V838 Mon in 2005 October using the Keck I telescope. We have identified numerous atomic features and molecular bands present in the spectrum and provided an atlas of those features. In order to improve the spectrum interpretation, we have performed simple modeling of the molecular bands. Our analysis indicates that the spectrum is dominated by molecular absorption features arising in photospheric regions with temperatures of ~2400 K and in colder outer layers, where the temperature decreases to ~500 K. A number of resonance lines of neutral alkali metals are observed to show P Cygni profiles. Particularly interesting are numerous prominent emission lines of [Fe II]. All of them show practically the same profile, which can be well described by a Lorentzian profile. In the blue part of the spectrum, photospheric signatures of the B-type companion are easily seen. We have fitted the observed spectrum with a synthetic one and the obtained parameters are consistent with the B3V type. We have also estimated radial and rotational velocities of the companion. The data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
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Design and Implementation of Data Reduction Pipelines for the Keck Observatory Archive
Gelino, C. R.; Berriman, G. B.; Kong, M.; Laity, A. C.; Swain, M. A.; Campbell, R.; Goodrich, R. W.; Holt, J.; Lyke, J.; Mader, J. A.; Tran, H. D.; Barlow, T.
2015-09-01
The Keck Observatory Archive (KOA), a collaboration between the NASA Exoplanet Science Institute and the W. M. Keck Observatory, serves science and calibration data for all active and inactive instruments from the twin Keck Telescopes located near the summit of Mauna Kea, Hawaii. In addition to the raw data, we produce and provide quick look reduced data for four instruments (HIRES, LWS, NIRC2, and OSIRIS) so that KOA users can more easily assess the scientific content and the quality of the data, which can often be difficult with raw data. The reduced products derive from both publicly available data reduction packages (when available) and KOA-created reduction scripts. The automation of publicly available data reduction packages has the benefit of providing a good quality product without the additional time and expense of creating a new reduction package, and is easily applied to bulk processing needs. The downside is that the pipeline is not always able to create an ideal product, particularly for spectra, because the processing options for one type of target (eg., point sources) may not be appropriate for other types of targets (eg., extended galaxies and nebulae). In this poster we present the design and implementation for the current pipelines used at KOA and discuss our strategies for handling data for which the nature of the targets and the observers' scientific goals and data taking procedures are unknown. We also discuss our plans for implementing automated pipelines for the remaining six instruments.
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Twenty Years of Precise Radial Velocities at Keck and Lick Observatories
Wright, J. T.
2015-10-01
The precise radial velocity survey at Keck Observatory began over 20 years ago. Its survey of thousands of stars now has the time baseline to be sensitive to planets with decade-long orbits, including Jupiter analogs. I present several newly-finished orbital solutions for long-period giant planets. Although hot Jupiters are generally ``lonely'' (i.e. they are not part of multiplanet systems), those that are not appear to often have giant companions at 5 AU or beyond. I present two of the highest period-ratios among planets in a two-planet system, and some of the longest orbital periods ever measured for exoplanets. In many cases, combining Keck radial velocities from those from other long-term surveys at Lick Observatory, McDonald Observatory, HARPS, and, of course, OHP spectrographs, produces superior orbital fits, constraining both period and eccentricity better than could be possible with any single set alone. Stellar magnetic activity cycles can masquerade as long-period planets. In most cases this effect is very small, but a loud minority of stars, including, apparently, HD 154345, show very strong RV-activity correlations.
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Developing Youth Football Academies in Greece: Managing Issues and Challenges
Chris Trikalis; Zisis Papanikolaou; Sofia Trikali
2014-01-01
Present study firstly investigated the goals and objectives of youth football academies in Greece, according to the different sector that they operate (public, private, voluntary) and secondly created proposals for future youth football academies development. Research was conducted in Greece, at the period of 2010-2011. Fourteen youth football academies participated in this study and divided into three categories (five academies in commercial sector, four academies in public sector, and five ...
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Huang, Yvonne J.; Marsland, Benjamin J.; Bunyavanich, Supinda; O’Mahony, Liam; Leung, Donald Y. M.; Muraro, Antonella; Fleisher, Thomas A.
2018-01-01
PRACTALL is a joint initiative of the American Academy of Allergy, Asthma & Immunology and the European Academy of Allergy and Clinical Immunology to provide shared evidence-based recommendations on cutting-edge topics in the field of allergy and immunology. PRACTALL 2017 is focused on what has been established regarding the role of the microbiome in patients with asthma, atopic dermatitis, and food allergy. This is complemented by outlining important knowledge gaps regarding its role in allergic disease and delineating strategies necessary to fill these gaps. In addition, a review of progress in approaches used to manipulate the microbiome will be addressed, identifying what has and has not worked to serve as a baseline for future directions to intervene in allergic disease development, progression, or both. PMID:28257972
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International Nuclear Information System (INIS)
Griest, Kim; Whitmore, Jonathan B.; Wolfe, Arthur M.; Prochaska, J. Xavier; Howk, J. Christopher; Marcy, Geoffrey W.
2010-01-01
We report on an attempt to accurately wavelength calibrate four nights of data taken with the Keck HIRES spectrograph on QSO PHL957, for the purpose of determining whether the fine structure constant was different in the past. Using new software and techniques, we measured the redshifts of various Ni II, Fe II, Si II, etc. lines in a damped Lyα system at z = 2.309. Roughly half the data were taken through the Keck iodine cell which contains thousands of well calibrated iodine lines. Using these iodine exposures to calibrate the normal Th-Ar Keck data pipeline output, we found absolute wavelength offsets of 500 m s -1 to 1000 m s -1 with drifts of more than 500 m s -1 over a single night, and drifts of nearly 2000 m s -1 over several nights. These offsets correspond to an absolute redshift of uncertainty of about Δz ∼ 10 -5 (Δλ ∼ 0.02 A), with daily drifts of around Δz ∼ 5 x 10 -6 (Δλ ∼ 0.01 A), and multiday drifts of nearly Δz ∼ 2 x 10 -5 (∼0.04 A). The causes of the wavelength offsets are not known, but since claimed shifts in the fine structure constant would result in velocity shifts of less than 100 m s -1 , this level of systematic uncertainty may make it difficult to use Keck HIRES data to constrain the change in the fine structure constant. Using our calibrated data, we applied both our own fitting software and standard fitting software to measure Δα/α, but discovered that we could obtain results ranging from significant detection of either sign, to strong null limits, depending upon which sets of lines and which fitting method were used. We thus speculate that the discrepant results on Δα/α reported in the literature may be due to random fluctuations coming from underestimated systematic errors in wavelength calibration and fitting procedure.
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Huang, Yvonne J; Marsland, Benjamin J; Bunyavanich, Supinda; O'Mahony, Liam; Leung, Donald Y M; Muraro, Antonella; Fleisher, Thomas A
2017-04-01
PRACTALL is a joint initiative of the American Academy of Allergy, Asthma & Immunology and the European Academy of Allergy and Clinical Immunology to provide shared evidence-based recommendations on cutting-edge topics in the field of allergy and immunology. PRACTALL 2017 is focused on what has been established regarding the role of the microbiome in patients with asthma, atopic dermatitis, and food allergy. This is complemented by outlining important knowledge gaps regarding its role in allergic disease and delineating strategies necessary to fill these gaps. In addition, a review of progress in approaches used to manipulate the microbiome will be addressed, identifying what has and has not worked to serve as a baseline for future directions to intervene in allergic disease development, progression, or both. Copyright © 2017. Published by Elsevier Inc.
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TWO EXOPLANETS DISCOVERED AT KECK OBSERVATORY
International Nuclear Information System (INIS)
Valenti, Jeff A.; Fischer, Debra; Giguere, Matt; Isaacson, Howard; Marcy, Geoffrey W.; Howard, Andrew W.; Johnson, John A.; Henry, Gregory W.; Wright, Jason T.
2009-01-01
We present two exoplanets detected at Keck Observatory. HD 179079 is a G5 subgiant that hosts a hot Neptune planet with M sin i = 27.5 M + in a 14.48 days, low-eccentricity orbit. The stellar reflex velocity induced by this planet has a semiamplitude of K = 6.6 m s -1 . HD 73534 is a G5 subgiant with a Jupiter-like planet of M sin i = 1.1 M Jup and K = 16 m s -1 in a nearly circular 4.85 yr orbit. Both stars are chromospherically inactive and metal-rich. We discuss a known, classical bias in measuring eccentricities for orbits with velocity semiamplitudes, K, comparable to the radial velocity uncertainties. For exoplanets with periods longer than 10 days, the observed exoplanet eccentricity distribution is nearly flat for large amplitude systems (K > 80 m s -1 ), but rises linearly toward low eccentricity for lower amplitude systems (K > 20 m s -1 ).
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The connection: schooling, youth development, and community building-The Futures Academy case.
Taylor, Henry Louis; McGlynn, Linda Greenough
2009-01-01
Universities, because of their vast human and fiscal resources, can play the central role in assisting in the development of school-centered community development programs that make youth development their top priority. The Futures Academy, a K-8 public school in the Fruit Belt, an inner-city neighborhood in Buffalo, New York, offers a useful model of community development in partnership with the Center for Urban Studies at the State University of New York at Buffalo. The goal of the project is to create opportunities for students to apply the knowledge and skills they learn in the classroom to the goal of working with others to make the neighborhood a better place to live. The efforts seek to realize in practice the Dewey dictum that individuals learn best when they have "a real motive behind and a real outcome ahead."
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Wirth, K. R.; Garver, J. I.; Greer, L.; Pollock, M.; Varga, R. J.; Davidson, C. M.; Frey, H. M.; Hubbard, D. K.; Peck, W. H.; Wobus, R. A.
2015-12-01
The Keck Geology Consortium, with support from the National Science Foundation (REU Program) and ExxonMobil, is a collaborative effort by 18 colleges to improve geoscience education through high-quality research experiences. Since its inception in 1987 more than 1350 undergraduate students and 145 faculty have been involved in 189 yearlong research projects. This non-traditional REU model offers exceptional opportunities for students to address research questions at a deep level, to learn and utilize sophisticated analytical methods, and to engage in authentic collaborative research that culminates in an undergraduate research symposium and published abstracts volume. The large numbers of student and faculty participants in Keck projects also affords a unique opportunity to study the impacts of program design on undergraduate research experiences in the geosciences. Students who participate in Keck projects generally report significant gains in personal and professional dimensions, as well as in clarification of educational and career goals. Survey data from student participants, project directors, and campus advisors identify mentoring as one of the most critical and challenging elements of successful undergraduate research experiences. Additional challenges arise from the distributed nature of Keck projects (i.e., participants, project directors, advisors, and other collaborators are at different institutions) and across the span of yearlong projects. In an endeavor to improve student learning about the nature and process of science, and to make mentoring practices more intentional, the Consortium has developed workshops and materials to support both project directors and campus research advisors (e.g., best practices for mentoring, teaching ethical professional conduct, benchmarks for progress, activities to support students during research process). The Consortium continues to evolve its practices to better support students from underrepresented groups.
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Ioachimescu, Octavian C; Wickwire, Emerson M; Harrington, John; Kristo, David; Arnedt, J Todd; Ramar, Kannan; Won, Christine; Billings, Martha E; DelRosso, Lourdes; Williams, Scott; Paruthi, Shalini; Morgenthaler, Timothy I
2014-03-15
Sleep medicine remains an underrepresented medical specialty worldwide, with significant geographic disparities with regard to training, number of available sleep specialists, sleep laboratory or clinic infrastructures, and evidence-based clinical practices. The American Academy of Sleep Medicine (AASM) is committed to facilitating the education of sleep medicine professionals to ensure high-quality, evidence-based clinical care and improve access to sleep centers around the world, particularly in developing countries. In 2002, the AASM launched an annual 4-week training program called Mini-Fellowship for International Scholars, designed to support the establishment of sleep medicine in developing countries. The participating fellows were generally chosen from areas that lacked a clinical infrastructure in this specialty and provided with training in AASM Accredited sleep centers. This manuscript presents an overview of the program, summarizes the outcomes, successes, and lessons learned during the first 12 years, and describes a set of programmatic changes for the near-future, as assembled and proposed by the AASM Education Committee and recently approved by the AASM Board of Directors. Ioachimescu OC; Wickwire EM; Harrington J; Kristo D; Arnedt JT; Ramar K; Won C; Billings ME; DelRosso L; Williams S; Paruthi S; Morgenthaler TI. A dozen years of American Academy of Sleep Medicine (AASM) international mini-fellowship: program evaluation and future directions.
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CHANDRA, KECK, AND VLA OBSERVATIONS OF THE CRAB NEBULA DURING THE 2011-APRIL GAMMA-RAY FLARE
Energy Technology Data Exchange (ETDEWEB)
Weisskopf, Martin C.; Tennant, Allyn F.; O' Dell, Stephen L. [NASA Marshall Space Flight Center, Astrophysics Office (ZP12), Huntsville, AL 35812 (United States); Arons, Jonathan [Astronomy Department and Theoretical Astrophysics Center, University of California, Berkeley, 601 Campbell Hall, Berkeley, CA 94720 (United States); Blandford, Roger; Funk, Stefan; Romani, Roger W. [W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305 (United States); Buehler, Rolf [DESY, Platanenallee 6, D-15738 Zeuthen (Germany); Caraveo, Patrizia; De Luca, Andrea [INAF-IASF Milano, via E. Bassini 15, I-20133 Milano (Italy); Cheung, Chi C. [National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001 (United States); Costa, Enrico [INFN Roma Tor Vergata, via della Ricerca Scientifica 1, I-00133 Roma (Italy); Ferrigno, Carlo [ISDC, Data Center for Astrophysics of the University of Geneva, chemin d' cogia 16, CH-1290 Versoix (Switzerland); Fu, Hai [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Habermehl, Moritz; Horns, Dieter [Institut fuer Experimentalphysik, Universitaet Hamburg, Luruper Chaussee 149, D-22761 Hamburg (Germany); Linford, Justin D. [Department of Physics and Astronomy, University of New Mexico, MSC07 4220, Albuquerque, NM 87131-0001 (United States); Lobanov, Andrei [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); Max, Claire [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Mignani, Roberto [Mullard Space Science Laboratory, University College London, Holmbury St. Mary Dorking, Surrey RH5 6NT (United Kingdom); and others
2013-03-01
We present results from our analysis of Chandra X-Ray Observatory, W. M. Keck Observatory, and Karl G. Jansky Very Large Array (VLA) images of the Crab Nebula that were contemporaneous with the {gamma}-ray flare of 2011 April. Despite hints in the X-ray data, we find no evidence for statistically significant variations that pinpoint the specific location of the flares within the Nebula. The Keck observations extend this conclusion to the 'inner knot', i.e., the feature within an arcsecond of the pulsar. The VLA observations support this conclusion. We also discuss theoretical implications of the {gamma}-ray flares and suggest that the most dramatic {gamma}-ray flares are due to radiation-reaction-limited synchrotron emission associated with sudden, dissipative changes in the current system sustained by the central pulsar.
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Keck i LWS Mid-Ir Images and Photometry of 9P/TEMPEL 1
Fernandez, Y. R.; Lisse, C. M.; A'Hearn, M. F.; Belton, M. J. S.
2010-01-01
This data set contains raw and reduced mid-infrared images and photometry of comet 9P/Tempel 1, the target of the Deep Impact mission. Images were acquired on the night of 21 August 2000, about 7.5 months after perihelion, by Y. Fernandez, C. Lisse, M. A'Hearn and M. Belton using the Long Wavelength Spectrometer instrument at the Keck I telescope.
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Keck Spectroscopy of Globular Clusters in the Elliptical Galaxy NGC 3610
Strader, Jay; Brodie, Jean P.; Schweizer, Francois; Larsen, Soeren S.; Seitzer, Patrick
2002-01-01
We present moderate-resolution Keck spectra of nine candidate globular clusters in the possible merger-remnant elliptical galaxy NGC 3610. Eight of the objects appear to be bona fide globular clusters of NGC 3610. We find that two of the clusters belong to an old metal-poor population, five to an old metal-rich population, and only one to an intermediate-age metal-rich population. The estimated age of the intermediate-age cluster is 1-5 Gyr, which is in agreement with earlier estimates of the...
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Back to the future: virtualization of the computing environment at the W. M. Keck Observatory
McCann, Kevin L.; Birch, Denny A.; Holt, Jennifer M.; Randolph, William B.; Ward, Josephine A.
2014-07-01
Over its two decades of science operations, the W.M. Keck Observatory computing environment has evolved to contain a distributed hybrid mix of hundreds of servers, desktops and laptops of multiple different hardware platforms, O/S versions and vintages. Supporting the growing computing capabilities to meet the observatory's diverse, evolving computing demands within fixed budget constraints, presents many challenges. This paper describes the significant role that virtualization is playing in addressing these challenges while improving the level and quality of service as well as realizing significant savings across many cost areas. Starting in December 2012, the observatory embarked on an ambitious plan to incrementally test and deploy a migration to virtualized platforms to address a broad range of specific opportunities. Implementation to date has been surprisingly glitch free, progressing well and yielding tangible benefits much faster than many expected. We describe here the general approach, starting with the initial identification of some low hanging fruit which also provided opportunity to gain experience and build confidence among both the implementation team and the user community. We describe the range of challenges, opportunities and cost savings potential. Very significant among these was the substantial power savings which resulted in strong broad support for moving forward. We go on to describe the phasing plan, the evolving scalable architecture, some of the specific technical choices, as well as some of the individual technical issues encountered along the way. The phased implementation spans Windows and Unix servers for scientific, engineering and business operations, virtualized desktops for typical office users as well as more the more demanding graphics intensive CAD users. Other areas discussed in this paper include staff training, load balancing, redundancy, scalability, remote access, disaster readiness and recovery.
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Neptune’s zonal winds from near-IR Keck adaptive optics imaging in August 2001
Martin, S.C.; De Pater, I.; Marcus, P.
2011-01-01
We present H-band (1.4–1.8 ?m) images of Neptune with a spatial resolution of ?0.06?, taken with the W.M. Keck II telescope using the slit-viewing camera (SCAM) of the NIRSPEC instrument backed with Adaptive Optics. Images with 60-second integration times span 4 hours each on UT 20 and 21 August,
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Strategic Plan for the Spanish Academy of Dermatology and Venerology (AEDV): FuturAEDV 2013-2017.
Ribera Pibernat, M; Moreno Jiménez, J C; Valcuende Cavero, F; Soto de Delás, J; Vázquez Veiga, H; Lázaro Ochaíta, P; Giménez Arnau, A
2014-09-01
The Spanish Academy of Dermatology and Venereology (AEDV) has decided that a Strategic Plan is needed to help the association adapt to new circumstances and anticipate future developments. 1) To position the AEDV as a medical association that can exert an influence in everything related to dermatology. 2) To contribute to the development of the specialty, strengthening the prestige and reputation of dermatology and dermatologists. 3) To establish a model for operating and strategic thinking that can be handed on to successive Boards of Directors and will enable the Academy to identify future challenges. The approach used to develop the Strategic Plan was as follows: analysis of trends in the health care system; assessment of the current situation of AEDV and of dermatology in general through an internal analysis based on surveys and interviews with academics; analysis of strengths, weaknesses, opportunities, and threats; preparation of a mission statement; and identification, development, and implementation of a strategy map prioritizing strategic lines of action. The strategy map set out 16 general goals grouped into 4 main topics (achieving the vision, internal and external customers, internal processes, and innovation) and detailed in an action plan with 19 initiatives, each with specific actions. The plan will be monitored by the Strategic Plan Monitoring Committee, which is made up of the members of the Standing Committee and the chairs of the 9 Technical Committees responsible for implementing the initiatives. The Functional Plan should guide the management of AEDV until 2017, and its implementation will enable the association to contribute to the development and prestige of the specialty and position itself as a reference in terms of its functional model. Copyright © 2014 Elsevier España, S.L.U. y AEDV. All rights reserved.
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Kibrick, Robert I.; Wirth, Gregory D.; Allen, Steven L.; Deich, William T. S.; Goodrich, Robert W.; Lanclos, Kyle; Lyke, James E.
2011-03-01
For over a decade, the W. M. Keck Observatory's two 10-meter telescopes have been operated remotely from its Waimea headquarters. Over the last 9 years, WMKO remote observing has expanded to allow observing teams at dedicated sites located across California to observe via the Internet either in collaboration with colleagues in Waimea or entirely from California; this capability was extended to Swinburne University in Melbourne, Australia in 2010 and to Yale University in New Haven, Connecticut in early 2011. All Keck facility science instruments are currently supported. Observers distributed between as many as four sites can collaborate in the interactive operation of each instrument by means of shared VNC desktops and multipoint video and/or telephone conferencing. Automated routers at primary remote observing sites ensure continued connectivity during Internet outages. Each Keck remote observing facility is similarly equipped and configured so observers have the same operating environment. This architecture provides observers the flexibility to conduct observations from the location best suited to their needs and to adapt to last-minute changes. It also enhances the ability of off-site technical staff to provide remote support.
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Addressing chronic operational issues at the W. M. Keck Observatory
Nordin, Tom; Matsuda, Richard
2016-07-01
The W. M. Keck Observatory (WMKO) has a good track record at addressing large critical faults which impact observing. Our performance tracking and correcting chronic minor faults has been mixed, yet this class of problems has a significant negative impact on scientific productivity and staff effectiveness. We have taken steps to address this shortcoming. This paper outlines the creation of a program to identify, categorize and rank these chronic operational issues, track them over time, and develop management options for their resolution. The success of the program at identifying these chronic operational issues and the advantages of dedicating observatory resources to this endeavor are presented.
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THE TEAM KECK REDSHIFT SURVEY 2: MOSFIRE SPECTROSCOPY OF THE GOODS-NORTH FIELD
Energy Technology Data Exchange (ETDEWEB)
Wirth, Gregory D.; Kassis, Marc; Lyke, Jim; Rizzi, Luca; Campbell, Randy; Goodrich, Robert W. [W. M. Keck Observatory, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743 (United States); Trump, Jonathan R.; Barro, Guillermo; Guo, Yicheng; Koo, David C.; Liu, Fengshan; Faber, S. M., E-mail: gregory.wirth@gmail.com [University of California Observatories, Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)
2015-11-15
We present the Team Keck Redshift Survey 2 (TKRS2), a near-infrared spectral observing program targeting selected galaxies within the CANDELS subsection of the GOODS-North Field. The TKRS2 program exploits the unique capabilities of the Multi-Object Spectrometer For Infra-Red Exploration (MOSFIRE), which entered service on the Keck I telescope in 2012 and contributes substantially to the study of galaxy spectral features at redshifts inaccessible to optical spectrographs. The TKRS2 project targets 97 galaxies drawn from samples that include z ≈ 2 emission-line galaxies with features observable in the JHK bands as well as lower-redshift targets with features in the Y band. We present a detailed measurement of MOSFIRE’s sensitivity as a function of wavelength, including the effects of telluric features across the YJHK filters. The largest utility of our survey is in providing rest-frame-optical emission lines for z > 1 galaxies, and we demonstrate that the ratios of strong, optical emission lines of z ≈ 2 galaxies suggest the presence of either higher N/O abundances than are found in z ≈ 0 galaxies or low-metallicity gas ionized by an active galactic nucleus. We have released all TKRS2 data products into the public domain to allow researchers access to representative raw and reduced MOSFIRE spectra.
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Mentoring the Afghan Army at the Officer Academy in Kabul
DEFF Research Database (Denmark)
Mynster Christensen, Maya
Capacity building of host nation militaries is a central component of current multinational military operations, which is likely to become increasingly vital to future military interventions in conflict settings. Focusing on the mentoring of the Afghan National Army at the British-led officer...... academy in Kabul, this policy brief stresses the urgency with which Western militaries should improve military capacity building efforts. Based on qualitative data collected at the British Royal Military Academy Sandhurst and the Afghan National Army Officer Academy, the brief outlines five clusters...
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Creation of an instrument maintenance program at W. M. Keck Observatory
Hill, G. M.; Kwok, S. H.; Mader, J. A.; Wirth, G. D.; Dahm, S. E.; Goodrich, R. W.
2014-08-01
Until a few years ago, the W. M. Keck Observatory (WMKO) did not have a systematic program of instrument maintenance at a level appropriate for a world-leading observatory. We describe the creation of such a program within the context of WMKO's lean operations model which posed challenges but also guided the design of the system and resulted in some unique and notable capabilities. These capabilities and the flexibility of the system have led to its adoption across the Observatory for virtually all PM's. The success of the Observatory in implementing the program and its impact on instrument reliability are presented. Lessons learned are reviewed and strategic implications discussed.
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Brown dwarf distances and atmospheres: Spitzer Parallaxes and the Keck/NIRSPEC upgrade
Martin, Emily C.
2018-01-01
Advances in infrared technology have been essential towards improving our understanding of the solar neighborhood, revealing a large population of brown dwarfs, which span the mass regime between planets and stars. My thesis combines near-infrared (NIR) spectroscopic and astrometric analysis of nearby low-mass stars and brown dwarfs with instrumentation work to upgrade the NIRSPEC instrument for the Keck II Telescope. I will present results from a program using Spitzer/IRAC data to measure precise locations and distances to 22 of the coldest and closest brown dwarfs. These distances allow us to constrain absolute physical properties, such as mass, radius, and age, of free-floating planetary-mass objects through comparison to atmospheric and evolutionary models. NIR spectroscopy combined with the Spitzer photometry reveals a detailed look into the atmospheres of brown dwarfs and gaseous extrasolar planets. Additionally, I will discuss the improvements we are making to the NIRSPEC instrument at Keck. NIRSPEC is a NIR echelle spectrograph, capable of R~2000 and R~25,000 observations in the 1-5 μm range. As part of the upgrade, I performed detector characterization, optical design of a new slit-viewing camera, mechanical testing, and electronics design. NIRSPEC’s increased efficiency will allow us to obtain moderate- and high-resolution NIR spectra of objects up to a magnitude fainter than the current NIRSPEC design. Finally, I will demonstrate the utility of a NIR laser frequency comb as a high-resolution calibrator. This new technology will revolutionize precision radial velocity measurements in the coming decade.
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Red Science: China's Scientific Capital and the Future of the Chinese Academy of Sciences
Directory of Open Access Journals (Sweden)
Arturo Salazar
2008-10-01
Full Text Available The Chinese Academy of Sciences (CAS produces the scientific and technological breakthroughs that place China among the major players in scientific innovation. However, the control that the Chinese government exerts over the Academy and the tradition of guanxi among its members prevent the CAS from take-off and securing a free environment to conduct original research. The article assesses the economic logic of scientific control and its effects within the Chinese Academy of Sciences. The paper’s aim is to derive to what extent the CAS will remain as China’s main provider of scientific innovation. The “national innovation systems” approach and the cultural traditions rooted in Confucianism are revised in detail to provide an accurate perspective. The paper concludes that the CAS’ international reputation as a center of scientific and technological innovation might be at stake unless the Chinese government makes some critical reforms.
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Williamson, Norma Velia
2011-01-01
Because educators vicariously touch the future through their students, the author believes that they sometimes have the uncanny ability to see the future. One common future forecast is the phenomenal growth of green jobs in the emerging green economy, leading to the creation of the "Reach of the Sun" Solar Energy Academy at La Mirada…
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Brooks, Norman H.
1990-01-01
This research biennial report for 1987-89 covers the activities of both the Environmental Engineering Science program and the Environmental Quality Laboratory for the period October 1987-November 1989. Environmental Engineering Science is the degree-granting academic program housed in the Keck Laboratories, with associated research projects. The Environmental Quality Laboratory is a research center focusing on large scale problems of environmental quality and natural resources. All the facult...
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Currie, T.; Fukagawa, M.; Thalmann, C.; Matsumura, S.; Plavchan, P.
2012-01-01
We present previously unpublished 2005 July H-band coronagraphic data of the young, planet-hosting star HR 8799 from the newly released Keck/NIRC2 archive. Despite poor observing conditions, we detect three of the planets (HR 8799 bcd), two of them (HR 8799 bc) without advanced image processing.
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Carnegie Science Academy Web Site
Kotwicki, John; Atzinger, Joe; Turso, Denise
1997-11-01
The Carnegie Science Academy is a professional society "For Teens...By Teens" at the Carnegie Science Center in Pittsburgh. The CSA Web Site [ http://csa.clpgh.org ] is designed for teens who have an interest in science and technology. This online or virtual science academy provides resources for teens in high school science classes. The Web site also allows students around the world to participate and communicate with other students, discuss current events in science, share opinions, find answers to questions, or make online friends. Visitors can enjoy the main components of the site or sign up for a free membership which allows access to our chat room for monthly meeting, online newsletter, members forum, and much more. Main components to the site include a spot for cool links and downloads, available for any visitor to download or view. Online exhibits are created by students to examine and publish an area of study and also allow teachers to easily post classroom activities as exhibits by submitting pictures and text. Random Access, the interactive part of the academy, allows users to share ideas and opinions. Planet CSA focuses on current events in science and the academy. In the future the CSA Web site will become a major resource for teens and science teachers providing materials that will allow students to further enhance their interest and experiences in science.
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Energy Technology Data Exchange (ETDEWEB)
Philipp, Hugh T., E-mail: htp2@cornell.edu; Tate, Mark W.; Purohit, Prafull; Shanks, Katherine S.; Weiss, Joel T. [Laboratory of Atomic and Solid State Physics, Cornell University, Ithaca, NY (United States); Chamberlain, Darol; Gruner, Sol M. [Laboratory of Atomic and Solid State Physics, Cornell University, Ithaca, NY (United States); Cornell High Energy Synchrotron Source (CHESS), Cornell University, Ithaca, NY (United States)
2016-07-27
Modern storage rings are readily capable of providing intense x-ray pulses, tens of picoseconds in duration, millions of times per second. Exploiting the temporal structure of these x-ray sources opens avenues for studying rapid structural changes in materials. Many processes (e.g. crack propagation, deformation on impact, turbulence, etc.) differ in detail from one sample trial to the next and would benefit from the ability to record successive x-ray images with single x-ray sensitivity while framing at 5 to 10 MHz rates. To this end, we have pursued the development of fast x-ray imaging detectors capable of collecting bursts of images that enable the isolation of single synchrotron bunches and/or bunch trains. The detector technology used is the hybrid pixel array detector (PAD) with a charge integrating front-end, and high-speed, in-pixel signal storage elements. A 384×256 pixel version, the Keck-PAD, with 150 µm × 150 µm pixels and 8 dedicated in-pixel storage elements is operational, has been tested at CHESS, and has collected data for compression wave studies. An updated version with 27 dedicated storage capacitors and identical pixel size has been fabricated.
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Millan-Gabet, Rafael; Che, Xiao; Monnier, John D.; Sitko, Michael L.; Russell, Ray W.; Grady, Carol A.; Day, Amanda N.; Perry, R. B.; Harries, Tim J.; Aarnio, Alicia N.; Colavita, Mark M.; Wizinowich, Peter L.; Ragland, Sam; Woillez, Julien
2016-01-01
We present near- and mid-infrared (MIR) interferometric observations made with the Keck Interferometer Nuller and near-contemporaneous spectro-photometry from the infrared telescope facilities (IRTFs) of 11 well-known young stellar objects, several of which were observed for the first time in these spectral and spatial resolution regimes. With au-level spatial resolution, we first establish characteristic sizes of the infrared emission using a simple geometrical model consisting of a hot inne...
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The Keck/OSIRIS Nearby AGN Survey (KONA). I. The Nuclear K-band Properties of Nearby AGN
Müller-Sánchez, F.; Hicks, E. K. S.; Malkan, M.; Davies, R.; Yu, P. C.; Shaver, S.; Davis, B.
2018-05-01
We introduce the Keck OSIRIS Nearby AGN survey (KONA), a new adaptive optics-assisted integral-field spectroscopic survey of Seyfert galaxies. KONA permits at ∼0.″1 resolution a detailed study of the nuclear kinematic structure of gas and stars in a representative sample of 40 local bona fide active galactic nucleus (AGN). KONA seeks to characterize the physical processes responsible for the coevolution of supermassive black holes and galaxies, principally inflows and outflows. With these IFU data of the nuclear regions of 40 Seyfert galaxies, the KONA survey will be able to study, for the first time, a number of key topics with meaningful statistics. In this paper we study the nuclear K-band properties of nearby AGN. We find that the K-band (2.1 μm) luminosities of the compact Seyfert 1 nuclei are correlated with the hard X-ray luminosities, implying a non-stellar origin for the majority of the continuum emission. The best-fit correlation is log L K = 0.9log L 2–10 keV + 4 over three orders of magnitude in both K-band and X-ray luminosities. We find no strong correlation between 2.1 μm luminosity and hard X-ray luminosity for the Seyfert 2 galaxies. The spatial extent and spectral slope of the Seyfert 2 galaxies indicate the presence of nuclear star formation and attenuating material (gas and dust), which in some cases is compact and in some galaxies extended. We detect coronal-line emission in 36 galaxies and for the first time in 5 galaxies. Finally, we find 4/20 galaxies that are usually classified as Seyfert 2 based on their optical spectra exhibit a broad component of Brγ emission, and one galaxy (NGC 7465) shows evidence of a double nucleus. Based on observations at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The observatory was made possible by the generous financial support of the W. M
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Deep Keck u-Band Imaging of the Hubble Ultra Deep Field: A Catalog of z ~ 3 Lyman Break Galaxies
Rafelski, Marc; Wolfe, Arthur M.; Cooke, Jeff; Chen, Hsiao-Wen; Armandroff, Taft E.; Wirth, Gregory D.
2009-10-01
We present a sample of 407 z ~ 3 Lyman break galaxies (LBGs) to a limiting isophotal u-band magnitude of 27.6 mag in the Hubble Ultra Deep Field. The LBGs are selected using a combination of photometric redshifts and the u-band drop-out technique enabled by the introduction of an extremely deep u-band image obtained with the Keck I telescope and the blue channel of the Low Resolution Imaging Spectrometer. The Keck u-band image, totaling 9 hr of integration time, has a 1σ depth of 30.7 mag arcsec-2, making it one of the most sensitive u-band images ever obtained. The u-band image also substantially improves the accuracy of photometric redshift measurements of ~50% of the z ~ 3 LBGs, significantly reducing the traditional degeneracy of colors between z ~ 3 and z ~ 0.2 galaxies. This sample provides the most sensitive, high-resolution multi-filter imaging of reliably identified z ~ 3 LBGs for morphological studies of galaxy formation and evolution and the star formation efficiency of gas at high redshift.
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Recruit Fitness as a Predictor of Police Academy Graduation.
Shusko, M; Benedetti, L; Korre, M; Eshleman, E J; Farioli, A; Christophi, C A; Kales, S N
2017-10-01
Suboptimal recruit fitness may be a risk factor for poor performance, injury, illness, and lost time during police academy training. To assess the probability of successful completion and graduation from a police academy as a function of recruits' baseline fitness levels at the time of academy entry. Retrospective study where all available records from recruit training courses held (2006-2012) at all Massachusetts municipal police academies were reviewed and analysed. Entry fitness levels were quantified from the following measures, as recorded at the start of each training class: body composition, push-ups, sit-ups, sit-and-reach, and 1.5-mile run-time. The primary outcome of interest was the odds of not successfully graduating from an academy. We used generalized linear mixed models in order to fit logistic regression models with random intercepts for assessing the probability of not graduating, based on entry-level fitness. The primary analyses were restricted to recruits with complete entry-level fitness data. The fitness measures most strongly associated with academy failure were lesser number of push-ups completed (odds ratio [OR] = 5.2, 95% confidence interval [CI] 2.3-11.7, for 20 versus 41-60 push-ups) and slower run times (OR = 3.8, 95% CI 1.8-7.8, [1.5 mile run time of ≥15'20″] versus [12'33″ to 10'37″]). Baseline pushups and 1.5-mile run-time showed the best ability to predict successful academy graduation, especially when considered together. Future research should include prospective validation of entry-level fitness as a predictor of subsequent police academy success. © The Author 2017. Published by Oxford University Press on behalf of the Society of Occupational Medicine.
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Operating a wide-area remote observing system for the W. M. Keck Observatory
Wirth, Gregory D.; Kibrick, Robert I.; Goodrich, Robert W.; Lyke, James E.
2008-07-01
For over a decade, the W. M. Keck Observatory's two 10-meter telescopes have been operated remotely from its Waimea headquarters. Over the last 6 years, WMKO remote observing has expanded to allow teams at dedicated sites in California to observe either in collaboration with colleagues in Waimea or entirely from the U.S. mainland. Once an experimental effort, the Observatory's mainland observing capability is now fully operational, supported on all science instruments (except the interferometer) and regularly used by astronomers at eight mainland sites. Establishing a convenient and secure observing capability from those sites required careful planning to ensure that they are properly equipped and configured. It also entailed a significant investment in hardware and software, including both custom scripts to simplify launching the instrument interface at remote sites and automated routers employing ISDN backup lines to ensure continuation of observing during Internet outages. Observers often wait until shortly before their runs to request use of the mainland facilities. Scheduling these requests and ensuring proper system operation prior to observing requires close coordination between personnel at WMKO and the mainland sites. An established protocol for approving requests and carrying out pre-run checkout has proven useful in ensuring success. The Observatory anticipates enhancing and expanding its remote observing system. Future plans include deploying dedicated summit computers for running VNC server software, implementing a web-based tracking system for mainland-based observing requests, expanding the system to additional mainland sites, and converting to full-time VNC operation for all instruments.
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DEEP KECK u-BAND IMAGING OF THE HUBBLE ULTRA DEEP FIELD: A CATALOG OF z ∼ 3 LYMAN BREAK GALAXIES
International Nuclear Information System (INIS)
Rafelski, Marc; Wolfe, Arthur M.; Cooke, Jeff; Chen, H.-W.; Armandroff, Taft E.; Wirth, Gregory D.
2009-01-01
We present a sample of 407 z ∼ 3 Lyman break galaxies (LBGs) to a limiting isophotal u-band magnitude of 27.6 mag in the Hubble Ultra Deep Field. The LBGs are selected using a combination of photometric redshifts and the u-band drop-out technique enabled by the introduction of an extremely deep u-band image obtained with the Keck I telescope and the blue channel of the Low Resolution Imaging Spectrometer. The Keck u-band image, totaling 9 hr of integration time, has a 1σ depth of 30.7 mag arcsec -2 , making it one of the most sensitive u-band images ever obtained. The u-band image also substantially improves the accuracy of photometric redshift measurements of ∼50% of the z ∼ 3 LBGs, significantly reducing the traditional degeneracy of colors between z ∼ 3 and z ∼ 0.2 galaxies. This sample provides the most sensitive, high-resolution multi-filter imaging of reliably identified z ∼ 3 LBGs for morphological studies of galaxy formation and evolution and the star formation efficiency of gas at high redshift.
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KECK NIRSPEC RADIAL VELOCITY OBSERVATIONS OF LATE-M DWARFS
Energy Technology Data Exchange (ETDEWEB)
Tanner, Angelle; White, Russel [Department of Astronomy, Georgia State University, One Park Place, Atlanta, GA 30303 (United States); Bailey, John [Department of Astronomy, University of Michigan, 830 Dennison Building, 500 Church Street, Ann Arbor, MI 48109-1042 (United States); Blake, Cullen [Department of Astrophysical Sciences, Princeton University, Peyton Hall, Ivy Lane, Princeton, NJ 08544 (United States); Blake, Geoffrey [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Cruz, Kelle [Department of Physics and Astronomy, Hunter College, 695 Park Avenue, New York, NY 10065 (United States); Burgasser, Adam J. [Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093 (United States); Kraus, Adam [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)
2012-11-15
We present the results of an infrared spectroscopic survey of 23 late-M dwarfs with the NIRSPEC echelle spectrometer on the Keck II telescope. Using telluric lines for wavelength calibration, we are able to achieve measurement precisions of down to 45 m s{sup -1} for our late-M dwarfs over a one- to four-year long baseline. Our sample contains two stars with radial velocity (RV) variations of >1000 m s{sup -1}. While we require more measurements to determine whether these RV variations are due to unseen planetary or stellar companions or are the result of starspots known to plague the surface of M dwarfs, we can place upper limits of <40 M{sub J} sin i on the masses of any companions around those two M dwarfs with RV variations of <160 m s{sup -1} at orbital periods of 10-100 days. We have also measured the rotational velocities for all the stars in our late-M dwarf sample and offer our multi-order, high-resolution spectra over 2.0-2.4 {mu}m to the atmospheric modeling community to better understand the atmospheres of late-M dwarfs.
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KECK NIRSPEC RADIAL VELOCITY OBSERVATIONS OF LATE-M DWARFS
International Nuclear Information System (INIS)
Tanner, Angelle; White, Russel; Bailey, John; Blake, Cullen; Blake, Geoffrey; Cruz, Kelle; Burgasser, Adam J.; Kraus, Adam
2012-01-01
We present the results of an infrared spectroscopic survey of 23 late-M dwarfs with the NIRSPEC echelle spectrometer on the Keck II telescope. Using telluric lines for wavelength calibration, we are able to achieve measurement precisions of down to 45 m s –1 for our late-M dwarfs over a one- to four-year long baseline. Our sample contains two stars with radial velocity (RV) variations of >1000 m s –1 . While we require more measurements to determine whether these RV variations are due to unseen planetary or stellar companions or are the result of starspots known to plague the surface of M dwarfs, we can place upper limits of J sin i on the masses of any companions around those two M dwarfs with RV variations of –1 at orbital periods of 10-100 days. We have also measured the rotational velocities for all the stars in our late-M dwarf sample and offer our multi-order, high-resolution spectra over 2.0-2.4 μm to the atmospheric modeling community to better understand the atmospheres of late-M dwarfs.
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Martin, N. F.; Ibata, R. A.; Chapman, S. C.; Irwin, M.; Lewis, G. F.
2007-09-01
We present the results of a spectroscopic survey of the recently discovered faint Milky Way satellites Boötes, Ursa Major I, Ursa Major II and Willman 1 (Wil1). Using the DEep Imaging Multi-Object Spectrograph mounted on the Keck II telescope, we have obtained samples that contain from ~15 to ~85 probable members of these satellites for which we derive radial velocities precise to a few kms-1 down to i ~ 21-22. About half of these stars are observed with a high enough signal-to-noise ratio to estimate their metallicity to within +/-0.2 dex. The characteristics of all the observed stars are made available, along with those of the Canes Venatici I dwarf galaxy that have been analysed in a companion paper. From this data set, we show that Ursa Major II is the only object that does not show a clear radial velocity peak. However, the measured systemic radial velocity (vr = 115 +/- 5kms-1) is in good agreement with simulations in which this object is the progenitor of the recently discovered Orphan Stream. The three other satellites show velocity dispersions that make them highly dark matter dominated systems (under the usual assumptions of symmetry and virial equilibrium). In particular, we show that despite its small size and faintness, the Wil1 object is not a globular cluster given its metallicity scatter over -2.0 systemic velocity of -12.3 +/- 2.3kms-1 which implies a mass-to-light ratio of ~700 and a total mass of ~5 × 105Msolar for this satellite, making it the least massive satellite galaxy known to date. Such a low mass could mean that the 107Msolar limit that had until now never been crossed for Milky Way and Andromeda satellite galaxies may only be an observational limit and that fainter, less massive systems exist within the Local Group. However, more modelling and an extended search for potential extratidal stars are required to rule out the possibility that these systems have not been significantly heated by tidal interaction. The data presented herein
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Academy Trust | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Journal of Biosciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
Department of Physiology, Kangwon National University School of Medicine Chuncheon 200-701, South Korea; Department of Microbiology, Inje University College of Medicine Busan 614-735, South Korea; Department of Pulmonary, Critical Care and Sleep Medicine, University of Southern California, Keck School of ...
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Metallicity and Kinematics of M31's Outer Stellar Halo from a Keck Spectroscopic Survey
Reitzel, David B.; Guhathakurta, Puragra
2002-07-01
We present first results from a spectroscopic survey designed to examine the metallicity and kinematics of individual red giant branch stars in the outer halo of the Andromeda spiral galaxy (M31). This study is based on multislit spectroscopy with the Keck II 10 m telescope and Low Resolution Imaging Spectrograph of the Ca II near-infrared triplet in 99 M31 halo candidates in a field at R=19 kpc on the southeast minor axis with brightnesses from 20intermediate-velocity stars (-160~2 dex range over which the abundance measurement methods are calibrated. The mean/median metallicity of the M31 halo is about =-1.9 to -1.1 dex (depending on the details of metallicity calibration and sample selection) and possibly higher: the high-metallicity end of the distribution is poorly constrained by our data since the selection function for the secure M31 sample excludes over 80% of the giants in solar/supersolar metallicity range. Possible reasons are explored for the apparent discrepancy between the mean [Fe/H] found in our spectroscopic survey (corrected for metallicity selection bias) and the slightly higher mean values found in earlier photometric studies. Field halo red giants in M31 appear to be somewhat more metal-rich on average than their Milky Way counterparts. The M31 halo [Fe/H] distribution is comparable to that of M31 globular clusters, Galactic globular clusters, and Local Group dwarf satellite galaxies. The data in this 19 kpc outer halo field are broadly consistent with a scenario in which the halo is built from the accretion of small stellar subsystems. There are four stars in the secure M31 sample that have particularly strong Ca II lines, indicating solar metallicity, at a common velocity of ~-340 km s-1 close to the galaxy's systemic velocity, similar to what might be expected for M31 disk giants on the minor axis. An extrapolation of the inner disk brightness profile, however, falls far short of accounting for these four stars-the disk would instead have to
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The W. M. Keck Telescope segmented primary mirror active control system software
Energy Technology Data Exchange (ETDEWEB)
Cohen, R.W. (Lawrence Berkeley Lab., CA (USA) California Association for Research in Astronomy, Kamuela, HI (USA)); Andreae, S.; Biocca, A.K.; Jared, R.C.; Llacer, J.; Meng, J.D.; Minor, R.H.; Orayani, M. (Lawrence Berkeley Lab., CA (USA))
1989-07-01
The active control system (ACS) uses both parallel and distributed processing techniques to measure and control the positions of the 36 segments of the Keck Observatory Telescope primary mirror. The main function of the software is to maintain the mirror figure; to accomplish this goal the software uses a predictive, feed-forward'' mechanism which effectively increases the system bandwidth for the most important sources of perturbation. The software executes on a set of twelve 68000-family processors under the supervision of a VAX workstation. An array of nine parallel I/O processors collect and process data from 168 displacement sensors and transmit motion commands to 108 actuators. Three additional processors simultaneously compute actuator commands, monitor system performance, compute sensor control parameters and communicate with other observatory computers. The software is highly optimized for speed. 6 refs., 7 figs.
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Constraints on cosmological birefringence from PLANCK and Bicep2/Keck data
Energy Technology Data Exchange (ETDEWEB)
Gruppuso, A. [INAF-IASF Bologna, Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna, Istituto Nazionale di Astrofisica, via Gobetti 101, I-40129 Bologna (Italy); Gerbino, M.; Pagano, L.; Melchiorri, A. [Dipartimento di Fisica and INFN, Università di Roma ' ' La Sapienza' ' , P.le Aldo Moro 2, 00185, Rome (Italy); Natoli, P.; Mandolesi, N.; Molinari, D., E-mail: gruppuso@iasbo.inaf.it, E-mail: martina.gerbino@roma1.infn.it, E-mail: ntlpla@unife.it, E-mail: luca.pagano@roma1.infn.it, E-mail: mandolesi@iasfbo.inaf.it, E-mail: alessandro.melchiorri@roma1.infn.it, E-mail: molinari@iasfbo.inaf.it [Dipartimento di Fisica e Scienze della Terra and INFN, Università degli Studi di Ferrara, Via Saragat 1, I-44100 Ferrara (Italy)
2016-06-01
The polarization of cosmic microwave background (CMB) can be used to constrain cosmological birefringence, the rotation of the linear polarization of CMB photons potentially induced by parity violating physics beyond the standard model. This effect produces non-null CMB cross correlations between temperature and B mode-polarization, and between E- and B-mode polarization. Both cross-correlations are otherwise null in the standard cosmological model. We use the recently released 2015 PLANCK likelihood in combination with the Bicep2/Keck/Planck (BKP) likelihood to constrain the birefringence angle α. Our findings, that are compatible with no detection, read α = 0.0° ± 1.3° (stat) ± 1° (sys) for PLANCK data and α = 0.30° ± 0.27° (stat) ± 1° (sys) for BKP data. We finally forecast the expected improvements over present constraints when the PLANCK BB, TB and EB spectra at high ℓ will be included in the analysis.
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epubworkshop | Indian Academy of Sciences
Indian Academy of Sciences (India)
Toggle navigation. Logo of the Indian Academy of Sciences. Indian Academy of Sciences. Home · About IASc · History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair · Jubilee Chair · Academy – Springer Nature chair · Academy Trust · Contact details · Office Staff · Office complaint ...
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International Nuclear Information System (INIS)
Jiang Linhua; Egami, Eiichi; Walth, Gregory; Kashikawa, Nobunari; Matsuda, Yuichi; Shimasaku, Kazuhiro; Nagao, Tohru; Ota, Kazuaki; Ouchi, Masami
2011-01-01
We present Keck spectroscopic observations of z > 6 Lyman-break galaxy (LBG) candidates in the Subaru Deep Field (SDF). The candidates were selected as i'-dropout objects down to z' = 27 AB magnitudes from an ultra-deep SDF z'-band image. With the Keck spectroscopy we identified 19 LBGs with prominent Lyα emission lines at 6 ≤ z ≤ 6.4. The median value of the Lyα rest-frame equivalent widths (EWs) is ∼50 Å, with four EWs >100 Å. This well-defined spectroscopic sample spans a UV-continuum luminosity range of –21.8 ≤ M UV ≤ –19.5 (0.6 ∼ 5 L* UV ) and a Lyα luminosity range of (0.3-3) × 10 43 erg s –1 (0.3-3 L* Lyα ). We derive the UV and Lyα luminosity functions (LFs) from our sample at (z) ∼ 6.2 after we correct for sample incompleteness. We find that our measurement of the UV LF is consistent with the results of previous studies based on photometric LBG samples at 5 6.
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Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. BEDARTHA GOSWAMI. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 51-60 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Inferring interdependencies from short ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. SERGEY P KUZNETSOV. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 117-132 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Chaos in three coupled rotators: ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. PRIYANKA SHUKLA. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 133-143 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Grad-type fourteen-moment theory for ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. F FAMILY. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 221-224 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Transport in ratchets with single-file constraint.
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. GIOVANNA ZIMATORE. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 35-41 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. RQA correlations on real business cycles ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. SUDHARSANA V IYENGAR. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 93-99 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Missing cycles: Effect of climate ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. NORBERT MARWAN. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 51-60 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Inferring interdependencies from short time ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. JANAKI BALAKRISHNAN. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 93-99 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Missing cycles: Effect of climate change ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. PAUL SCHULTZ. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 51-60 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Inferring interdependencies from short time ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. F REVUELTA. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 145-155 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Rate calculation in two-dimensional barriers with ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. JOYDEEP SINGHA. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 195-203 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Spatial splay states in coupled map lattices ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series. MURILO S BAPTISTA. Articles written in Indian Academy of Sciences Conference Series. Volume 1 Issue 1 December 2017 pp 17-23 Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016. Interpreting physical flows in networks as a ...
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Indian Academy of Sciences Indian National Science Academy The ...
Indian Academy of Sciences (India)
The three national Science Academies offer several two-month Summer Fellowships to enable students/teachers to work with scientists associated with the three Academies during 2012. A list of those who have consented to guide students/teachers to work on short-term projects is displayed on the online announcement.
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Berriman, G. Bruce; Cohen, Richard W.; Colson, Andrew; Gelino, Christopher R.; Good, John C.; Kong, Mihseh; Laity, Anastasia C.; Mader, Jeffrey A.; Swain, Melanie A.; Tran, Hien D.; Wang, Shin-Ywan
2016-08-01
The Keck Observatory Archive (KOA) (https://koa.ipac.caltech.edu) curates all observations acquired at the W. M. Keck Observatory (WMKO) since it began operations in 1994, including data from eight active instruments and two decommissioned instruments. The archive is a collaboration between WMKO and the NASA Exoplanet Science Institute (NExScI). Since its inception in 2004, the science information system used at KOA has adopted an architectural approach that emphasizes software re-use and adaptability. This paper describes how KOA is currently leveraging and extending open source software components to develop new services and to support delivery of a complete set of instrument metadata, which will enable more sophisticated and extensive queries than currently possible. In August 2015, KOA deployed a program interface to discover public data from all instruments equipped with an imaging mode. The interface complies with version 2 of the Simple Imaging Access Protocol (SIAP), under development by the International Virtual Observatory Alliance (IVOA), which defines a standard mechanism for discovering images through spatial queries. The heart of the KOA service is an R-tree-based, database-indexing mechanism prototyped by the Virtual Astronomical Observatory (VAO) and further developed by the Montage Image Mosaic project, designed to provide fast access to large imaging data sets as a first step in creating wide-area image mosaics (such as mosaics of subsets of the 4.7 million images of the SDSS DR9 release). The KOA service uses the results of the spatial R-tree search to create an SQLite data database for further relational filtering. The service uses a JSON configuration file to describe the association between instrument parameters and the service query parameters, and to make it applicable beyond the Keck instruments. The images generated at the Keck telescope usually do not encode the image footprints as WCS fields in the FITS file headers. Because SIAP
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The Future of Student Engagement
Buskist, William; Groccia, James E.
2018-01-01
This chapter underscores the importance of conceptualizing student engagement as a responsibility shared by all members of the academy and describes how Groccia's multidimensional model can serve as blueprint for future thinking and research on student engagement.
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Stern, Daniel; C3R2 Team
2017-01-01
A primary objective of both WFIRST and Euclid is to provide a 3D map of the distribution of matter across a significant fraction of the universe from the weak lensing shear field, but to do so requires robust distances to billions of galaxies. I will report on a multi-semester program, expected to total approximately 40 nights with Keck over the next two years. This program, supporting both the NASA PCOS and COR science goals, will obtain the necessary galaxy spectroscopy to calibrate the color-redshift relation for the Euclid mission, and make significant progress towards the WFIRST requirements. The program, called C3R2 or Complete Calibration of the Color-Redshift Relation, already encompasses 10 allocated nights of NASA Keck Key Strategic Mission Support (PI D. Stern), 12 allocated nights from Caltech (PI J. Cohen), 3 allocated nights from the University of Hawaii (PI D. Sanders), and 1.5 allocated nights from UC-Riverside (PI B. Mobasher). We are also pursuing opportunities at additional 8- to 10-meter class telescopes, including Magellan, VLT and GCT. I will present the motivation for this program, the plans, and current results.
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ayurvis.pdf | dvdocs | academy | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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astrophys.pdf | dvdocs | academy | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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GMCrops-interAcademy-report-updated.pdf | inter academy ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Directory of Open Access Journals (Sweden)
Nodar Z. Mossaki
2015-03-01
Full Text Available The article analyzes the system of training of officers in military academies in Iraq – in Zakho, Qalacholan, ar-Rustamiyah and an-Nasiriyah. The author describes the history of creation, process of evolution, challenges and features of training in these colleges. Particular attention paid to military academies in the territory of Iraqi Kurdistan, which actually do not obey the central government of Iraq, however, have the highest level of training. Currently, Iraq's military academies operate on the basis of the NATO standards. Iraqi military academies paid miuch attention to the specifics of the military and political situation in Iraq – counterinsurgency and counterterrorism operations, patrolling cities, fighting in an urban environment etc. Significant place in the curriculum take the courses contributing to the formation of pro-Western sentiment.
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office.html | Indian Academy of Sciences
Indian Academy of Sciences (India)
Toggle navigation. Logo of the Indian Academy of Sciences. Indian Academy of Sciences. Home · About IASc · History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair · Jubilee Chair · Academy – Springer Nature chair · Academy Trust · Contact details · Office Staff · Office complaint ...
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Avison, Kevin
2008-01-01
This article examines the curious position of the Academy model in the English school system and how a potential Hereford Steiner Waldorf Academy might figure in this. It sketches the background to the Steiner movement in the UK and goes on to set out the key aspirations and concerns of Steiner educators regarding an Academy. The article provides…
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American Academy of Cosmetic Dentistry
... AACD AACD 2018: A Masterpiece of Comprehensive Cosmetic Dentistry Education 34th Annual Scientific Session | April 18-21 ... 222.9540 Contact Us © 2017American Academy of Cosmetic Dentistry American Academy of Cosmetic Dentistry (AACD) © 2017American Academy ...
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epubworkshop | Indian Academy of Sciences
Indian Academy of Sciences (India)
How to combat infectious diseases: The role of Science Academies · Academy Public Lecture and INSA–Leopoldina Lecture by Prof. Jörg Hacker, President, German Academy of Sciences Leopoldina. 4 December, 2017, 4 PM Faculty Hall, Indian Institute ...
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Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Executive Energy Leadership Academy | NREL
Executive Energy Leadership Academy Executive Energy Leadership Academy NREL's Executive Energy Leadership Academy is a nationally renowned program that provides non-technical business, governmental, and foreground. Leadership Program The Leadership Program is designed for community and industry leaders with an
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Science Academies' Summer Research Fellowship Programme for ...
Indian Academy of Sciences (India)
IAS Admin
2013-11-30
Nov 30, 2013 ... Science Academies' Summer Research Fellowship Programme for. Students and Teachers – 2014. Sponspored by. Indian Academy of Sciences, Bangalore. Indian National Science Academy, New Delhi. The National Academy of Sciences, India, Allahabad. The three national science academies offer ...
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Kos16.pdf | multimedia | academy | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Directory of Open Access Journals (Sweden)
Simon Drees
2016-07-01
Full Text Available The ASPIRE-to-Excellence Academy was recently founded at the 2015 Association for Medical Education in Europe (AMEE conference in Glasgow. The academy is new pillar of the ASPIRE-to-Excellence initiative by AMEE, which aims at promoting and encouraging medical schools in achieving excellence in the categories of assessment, student engagement, social accountability or faculty development. The Academy panel consists of the members of the ASPIRE Board and representatives from schools which have been recognised with an ASPIRE-to-excellence award in one or more of the categories. Major goal of the ASPIRE-to-Excellence Academy is to foster collaboration between excellent medical schools and to allow them to exchange experiences and Best Practices. The Academy members are organising workshops and symposia at international conferences to inform medical schools about the ASPIRE-to-Excellence programme and the areas for recognition in excellence as well as to support medical school in preparing their applications.
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32 CFR 575.1 - Military Academy.
2010-07-01
... 32 National Defense 3 2010-07-01 2010-07-01 true Military Academy. 575.1 Section 575.1 National... MILITARY ACADEMY § 575.1 Military Academy. (a) Organization and administration. (1) The United States Military Academy is under the general direction and supervision of the Department of the Army. The...
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Biomicrofluidics: Recent trends and future challenges
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences ... Biomicrofluidics is an active area of research at present, exploring the synergy of microfluidics with cellular and molecular biology, ... Future directions of research on these topics are also discussed.
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European Academy of decommisioning
International Nuclear Information System (INIS)
Slugen, V.; Hinca, R.
2014-01-01
According to analyses presented at EC meeting focused on decommissioning organized at 11.9.2012 in Brussels, it was stated that at least 500 new international experts for decommissioning will be needed in Europe up to 2025, which means about 35 per year.Having in mind the actual EHRO-N report from 2013 focused on operation of nuclear facilities and an assumption that the ratio between nuclear experts, nuclearized and nuclear aware people is comparable also for decommissioning (16:74:10), as well as the fact that the special study branch for decommissioning in the European countries almost does not exist, this European Decommissioning Academy (EDA) could be helpful in the overbridging this gap.For the first run of the EDA scheduled on 2014 we would like to focus on VVER decommissioning issues because this reactor type is the most distributed design in the world and many of these units are actually in decommissioning process or will be decommissioned in the near future in Europe.A graduate of the European Decommissioning Academy (EDA) should have at least bachelor level from technical or natural science Universities or Colleges and at least one year working experiences in the area of NPP decommissioning or nuclear power engineering. This study creates prerequisites for acquiring and completion of professional and specialized knowledge in the subjects which are described. (authors)
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Liu, Michael C.; Dupuy, Trent J.; Leggett, S. K.
2010-10-01
Highly unequal-mass ratio binaries are rare among field brown dwarfs, with the mass ratio distribution of the known census described by q (4.9±0.7). However, such systems enable a unique test of the joint accuracy of evolutionary and atmospheric models, under the constraint of coevality for the individual components (the "isochrone test"). We carry out this test using two of the most extreme field substellar binaries currently known, the T1 + T6 epsilon Ind Bab binary and a newly discovered 0farcs14 T2.0 + T7.5 binary, 2MASS J12095613-1004008AB, identified with Keck laser guide star adaptive optics. The latter is the most extreme tight binary resolved to date (q ≈ 0.5). Based on the locations of the binary components on the Hertzsprung-Russell (H-R) diagram, current models successfully indicate that these two systems are coeval, with internal age differences of log(age) = -0.8 ± 1.3(-1.0+1.2 -1.3) dex and 0.5+0.4 -0.3(0.3+0.3 -0.4) dex for 2MASS J1209-1004AB and epsilon Ind Bab, respectively, as inferred from the Lyon (Tucson) models. However, the total mass of epsilon Ind Bab derived from the H-R diagram (≈ 80 M Jup using the Lyon models) is strongly discrepant with the reported dynamical mass. This problem, which is independent of the assumed age of the epsilon Ind Bab system, can be explained by a ≈ 50-100 K systematic error in the model atmosphere fitting, indicating slightly warmer temperatures for both components; bringing the mass determinations from the H-R diagram and the visual orbit into consistency leads to an inferred age of ≈ 6 Gyr for epsilon Ind Bab, older than previously assumed. Overall, the two T dwarf binaries studied here, along with recent results from T dwarfs in age and mass benchmark systems, yield evidence for small (≈100 K) errors in the evolutionary models and/or model atmospheres, but not significantly larger. Future parallax, resolved spectroscopy, and dynamical mass measurements for 2MASS J1209-1004AB will enable a more
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... and Irma. Proceedings of the National Academy of Sciences (PNAS) PNAS is one of the world’s most- ... Exchange Evolution Resources Biographical Memoirs National Academy of Sciences About The NAS Mission History Organization Leadership and ...
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The Teachers Academy for Mathematics and Science
Energy Technology Data Exchange (ETDEWEB)
1992-01-01
In his State of the Union address on January 31, 1990, President Bush set a goal for US students to be number one in the world in mathematics and science achievement by the year 2000. The Teachers Academy for Mathematics and Science in Chicago is an experiment of unprecedented boldness and scale that can provide a means to the President's goal, both for the Chicago area and as a national model. This document covers organization and governance, program activities, future training goals, and evaluation programs.
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CHARACTERIZATION OF THE INNER DISK AROUND HD 141569 A FROM KECK/NIRC2 L-BAND VORTEX CORONAGRAPHY
Energy Technology Data Exchange (ETDEWEB)
Mawet, Dimitri; Bottom, Michael; Matthews, Keith [Department of Astronomy, California Institute of Technology, 1200 East California Boulevard, MC 249-17, Pasadena, CA 91125 (United States); Choquet, Élodie; Serabyn, Eugene [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Absil, Olivier; Huby, Elsa; Gonzalez, Carlos A. Gomez; Wertz, Olivier; Carlomagno, Brunella; Christiaens, Valentin; Defrère, Denis; Delacroix, Christian; Habraken, Serge; Jolivet, Aissa [Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, 19 Allée du Six Août, B-4000 Liège (Belgium); Femenia, Bruno [W. M. Keck Observatory, 65-1120 Mamalahoa Hwy., Kamuela, HI 96743 (United States); Lebreton, Jérémy [NASA Exoplanet Science Institute, California Institute of Technology, 770 South Wilson Avenue, Pasadena, CA 91125 (United States); Forsberg, Pontus; Karlsson, Mikael [Department of Engineering Sciences, Ångström Laboratory, Uppsala University, Box 534, SE-751 21 Uppsala (Sweden); Milli, Julien, E-mail: dmawet@astro.caltech.edu [European Southern Observatory, Alonso de Cordóva 3107, Vitacura, Santiago (Chile); and others
2017-01-01
HD 141569 A is a pre-main sequence B9.5 Ve star surrounded by a prominent and complex circumstellar disk, likely still in a transition stage from protoplanetary to debris disk phase. Here, we present a new image of the third inner disk component of HD 141569 A made in the L ′ band (3.8 μ m) during the commissioning of the vector vortex coronagraph that has recently been installed in the near-infrared imager and spectrograph NIRC2 behind the W.M. Keck Observatory Keck II adaptive optics system. We used reference point-spread function subtraction, which reveals the innermost disk component from the inner working distance of ≃23 au and up to ≃70 au. The spatial scale of our detection roughly corresponds to the optical and near-infrared scattered light, thermal Q , N , and 8.6 μ m PAH emission reported earlier. We also see an outward progression in dust location from the L ′ band to the H band (Very Large Telescope/SPHERE image) to the visible ( Hubble Space Telescope ( HST )/STIS image), which is likely indicative of dust blowout. The warm disk component is nested deep inside the two outer belts imaged by HST-NICMOS in 1999 (at 406 and 245 au, respectively). We fit our new L ′-band image and spectral energy distribution of HD 141569 A with the radiative transfer code MCFOST. Our best-fit models favor pure olivine grains and are consistent with the composition of the outer belts. While our image shows a putative very faint point-like clump or source embedded in the inner disk, we did not detect any true companion within the gap between the inner disk and the first outer ring, at a sensitivity of a few Jupiter masses.
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Reder, Leonard J.; Booth, Andrew; Hsieh, Jonathan; Summers, Kellee R.
2004-09-01
This paper presents a discussion of the evolution of a sequencer from a simple Experimental Physics and Industrial Control System (EPICS) based sequencer into a complex implementation designed utilizing UML (Unified Modeling Language) methodologies and a Computer Aided Software Engineering (CASE) tool approach. The main purpose of the Interferometer Sequencer (called the IF Sequencer) is to provide overall control of the Keck Interferometer to enable science operations to be carried out by a single operator (and/or observer). The interferometer links the two 10m telescopes of the W. M. Keck Observatory at Mauna Kea, Hawaii. The IF Sequencer is a high-level, multi-threaded, Harel finite state machine software program designed to orchestrate several lower-level hardware and software hard real-time subsystems that must perform their work in a specific and sequential order. The sequencing need not be done in hard real-time. Each state machine thread commands either a high-speed real-time multiple mode embedded controller via CORBA, or slower controllers via EPICS Channel Access interfaces. The overall operation of the system is simplified by the automation. The UML is discussed and our use of it to implement the sequencer is presented. The decision to use the Rhapsody product as our CASE tool is explained and reflected upon. Most importantly, a section on lessons learned is presented and the difficulty of integrating CASE tool automatically generated C++ code into a large control system consisting of multiple infrastructures is presented.
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Nuclear energy - the future climate
International Nuclear Information System (INIS)
Ash, Eric Sir
2000-01-01
In June 1999, a report entitled Nuclear Energy-The Future Climate was published and was the result of a collaboration between the Royal Society and the Royal Academy of Engineering. The report was the work of a group of nine people, made up of scientists, engineers and an economist, whose purpose was to attempt a new and objective look at the total energy scene and specifically the future role of nuclear energy. This paper discusses the findings of that report. (author)
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International Nuclear Information System (INIS)
Golder, T.; Laktasic, S.
1987-01-01
In order to provide and maintain a high level of nuclear security at DOE installations, the Office of Safeguards and Security (OSS) is charged with the deployment of highly trained security staff at each DOE site. Faced with this mission, OSS must ensure that both Safeguards and Security personnel are adequately trained to meet present as well as potential future insider and outside threats. A major step toward meeting this goal was to begin to standardize training, establish an elite training cadre, and create a central training facility to implement training for safeguards and security personnel. These requirements were actualized by the creation of the Central Training Academy. After a 9 month start-up and 2 years of initial operation, the CTA can now provide a historical perspective on its evolution, early program development, and future plans and challenges. Central to future program planning at the Academy is the development and implementation of an internal DOE needs assessment process which is the focus of this study. Once institutionalized, the system would allow for the Academy to accurately assess and translate OSS needs into requirements for both OSS Safeguards and Security personnel and place the Academy in position to develop and tailor Tactical and Specialized programs that reflect and respond to changing threats and technological advances
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Automatic Image Processing Workflow for the Keck/NIRC2 Vortex Coronagraph
Xuan, Wenhao; Cook, Therese; Ngo, Henry; Zawol, Zoe; Ruane, Garreth; Mawet, Dimitri
2018-01-01
The Keck/NIRC2 camera, equipped with the vortex coronagraph, is an instrument targeted at the high contrast imaging of extrasolar planets. To uncover a faint planet signal from the overwhelming starlight, we utilize the Vortex Image Processing (VIP) library, which carries out principal component analysis to model and remove the stellar point spread function. To bridge the gap between data acquisition and data reduction, we implement a workflow that 1) downloads, sorts, and processes data with VIP, 2) stores the analysis products into a database, and 3) displays the reduced images, contrast curves, and auxiliary information on a web interface. Both angular differential imaging and reference star differential imaging are implemented in the analysis module. A real-time version of the workflow runs during observations, allowing observers to make educated decisions about time distribution on different targets, hence optimizing science yield. The post-night version performs a standardized reduction after the observation, building up a valuable database that not only helps uncover new discoveries, but also enables a statistical study of the instrument itself. We present the workflow, and an examination of the contrast performance of the NIRC2 vortex with respect to factors including target star properties and observing conditions.
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KECK-I MOSFIRE SPECTROSCOPY OF THE z {approx} 12 CANDIDATE GALAXY UDFj-39546284
Energy Technology Data Exchange (ETDEWEB)
Capak, P. [Spitzer Science Center, 314-6 Caltech, Pasadena, CA 91125 (United States); Faisst, A.; Tacchella, S.; Carollo, M. [Institute for Astronomy, Swiss Federal Institute of Technology (ETH Zurich), CH-8093 Zurich (Switzerland); Vieira, J. D.; Scoville, N. Z. [California Institute of Technology, 314-6 Caltech, Pasadena, CA 91125 (United States)
2013-08-10
We report the results of deep (4.6 hr) H-band spectroscopy of the well studied z {approx} 12 H-band dropout galaxy candidate UDFj-39546284 with MOSFIRE on Keck-I. These data reach a sensitivity of 5-10 Multiplication-Sign 10{sup -19} erg s{sup -1} cm{sup -2} per 4.4 A resolution element between sky lines. Previous papers have argued that this source could either be a large equivalent width line emitting galaxy at 2 < z < 3.5 or a luminous galaxy at z {approx} 12. We find a 2.2{sigma} peak associated with a line candidate in deep Hubble Space Telescope Wide-Field Camera 3 Infrared grism observations, but at a lower flux than expected. After considering several possibilities, we conclude these data cannot conclusively confirm or reject the previous line detection, and significantly deeper spectroscopic observations are required. We also search for low-redshift emission lines in 10 other 7 < z < 10 z, Y, and J-dropout candidates in our mask and find no significant detections.
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Bazyka, D
2017-12-01
the first academic supervisors in studies of Chornobyl health effects and got professor certificates in this new area. First PhD theses were successfully passed by Dr. E. Gorbov, and Dr. of Sciences - by Dr. D. Bazyka. Basics of future aca demic research directions were elaborated that time by Drs. O. Kovalenko, Zh. Minchenko, V. Talko, I. Holyavka, D. Belyi, D. Yakimenko, E. Mikhai lovska, V. Malyzhev, V. Sushko, A. Cheban, K. Lo ganovsky, K. Bruslova, I. Dyagil, T. Liubarets, O. Kucher, G. Chobotko, and others. Later the major ity of these studies formed a background for Chornobyl legislation, regulatory directives, pre sented as dissertations.A quarter of century passed. The Center as a part of the National Academy of Medical Sciences resisted the challenges and moved forward, was recognized worldwide and fulfilled its main mission - providing highly qualified health care to radiation exposed. Staff numbers decreased (1,091), but work amount has increased. Since 2000, new premises were installed - a hospital with the biggest in Ukraine outpatient clin ic, new laboratory facilities, the last of which was in troduced in 2013. The Academy became a national one and since 2011 the Center was recognized as a national research institution (NRCRM), staff mem bers received 3 State Awards of Ukraine in the Field of Science and Technology, numerous personal awards.During this period, NRCRM staff conducted and published priority research data on radiation risks and molecular mechanisms of leukemia, including chronic lymphocytic, myelodysplastic syndrome, multiple myeloma, thyroid cancer, breast cancer in Chornobyl accident cleanup workers. Studies of the mechanisms of non tumor pathology - cardio vascular, cerebrovascular, cognitive disorders are in process. Of high importance are studies of possible transgenerational effects of radiation. The devel oped new technologies and protocols for the advanced care of radiation exposed were intro duced to the general health care system
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Patrika | Publications | Indian Academy of Sciences
Indian Academy of Sciences (India)
Patrika. Newsletter of the Indian Academy of Sciences. Patrika is a newsletter brought out by the Indian Academy of Sciences every year. It records all the major activities, events and initiatives of the academy. Issue 65. March 2017. In English | In Hindi. Issue 64. September 2016. In English | In Hindi. Issue 63. March 2016.
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Energy Technology Data Exchange (ETDEWEB)
Jiang Linhua; Egami, Eiichi; Walth, Gregory [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Kashikawa, Nobunari [Optical and Infrared Astronomy Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan); Matsuda, Yuichi [Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Shimasaku, Kazuhiro [Department of Astronomy, University of Tokyo, Hongo, Tokyo 113-0033 (Japan); Nagao, Tohru [Research Center for Space and Cosmic Evolution, Ehime University, Bunkyo-cho, Matsuyama 790-8577 (Japan); Ota, Kazuaki [Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502 (Japan); Ouchi, Masami [Institute for Cosmic Ray Research, University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa City, Chiba 77-8582 (Japan)
2011-12-10
We present Keck spectroscopic observations of z > 6 Lyman-break galaxy (LBG) candidates in the Subaru Deep Field (SDF). The candidates were selected as i'-dropout objects down to z' = 27 AB magnitudes from an ultra-deep SDF z'-band image. With the Keck spectroscopy we identified 19 LBGs with prominent Ly{alpha} emission lines at 6 {<=} z {<=} 6.4. The median value of the Ly{alpha} rest-frame equivalent widths (EWs) is {approx}50 A, with four EWs >100 A. This well-defined spectroscopic sample spans a UV-continuum luminosity range of -21.8 {<=} M{sub UV} {<=} -19.5 (0.6 {approx} 5 L*{sub UV}) and a Ly{alpha} luminosity range of (0.3-3) Multiplication-Sign 10{sup 43} erg s{sup -1} (0.3-3 L*{sub Ly{alpha}}). We derive the UV and Ly{alpha} luminosity functions (LFs) from our sample at (z) {approx} 6.2 after we correct for sample incompleteness. We find that our measurement of the UV LF is consistent with the results of previous studies based on photometric LBG samples at 5 < z < 7. Our Ly{alpha} LF is also generally in agreement with the results of Ly{alpha}-emitter surveys at z {approx} 5.7 and 6.6. This study shows that deep spectroscopic observations of LBGs can provide unique constraints on both the UV and Ly{alpha} LFs at z > 6.
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Talent Management in Academies
Davies, Brent; Davies, Barbara J.
2010-01-01
Purpose: Academies are semi-autonomous schools set up outside the normal local government structures with sponsors from business and charity groups to create new and innovative ways of creating and sustaining school transformation. The aim of this paper is to assist in a strategic conversation within the academy movement on talent development.…
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A Keck/DEIMOS spectroscopic survey of the faint M31 satellites AndIX, AndXI, AndXII and AndXIII†
Collins, M. L. M.; Chapman, S. C.; Irwin, M. J.; Martin, N. F.; Ibata, R. A.; Zucker, D. B.; Blain, A.; Ferguson, A. M. N.; Lewis, G. F.; McConnachie, A. W.; Peñarrubia, J.
2010-10-01
We present the first spectroscopic analysis of the faint M31 satellite galaxies, AndXI and AndXIII, as well as a re-analysis of existing spectroscopic data for two further faint companions, AndIX (correcting for an error in earlier geometric modelling that caused a misclassification of member stars in previous work) and AndXII. By combining data obtained using the Deep Imaging Multi-Object Spectrograph (DEIMOS) mounted on the Keck II telescope with deep photometry from the Suprime-Cam instrument on Subaru, we have identified the most probable members for each of the satellites based on their radial velocities (precise to several down to i ~ 22), distance from the centre of the dwarf spheroidal galaxies (dSphs) and their photometric [Fe/H]. Using both the photometric and spectroscopic data, we have also calculated global properties for the dwarfs, such as systemic velocities, metallicities and half-light radii. We find each dwarf to be very metal poor ([Fe/H] ~ -2 both photometrically and spectroscopically, from their stacked spectrum), and as such, they continue to follow the luminosity-metallicity relationship established with brighter dwarfs. We are unable to resolve dispersion for AndXI due to small sample size and low signal-to-noise ratio, but we set a 1σ upper limit of σv financial support of the W.M. Keck Foundation. Based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. ‡ E-mail: mlmc2@ast.cam.ac.uk
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HDE 245059: A WEAK-LINED T TAURI BINARY REVEALED BY CHANDRA AND KECK
International Nuclear Information System (INIS)
Baldovin-Saavedra, C.; Audard, M.; Duchene, G.; Guedel, M.; Skinner, S.L.; Paerels, F. B. S.; Ghez, A.; McCabe, C.
2009-01-01
We present the Chandra High Energy Transmission Grating Spectrometer and Keck observations of HDE 245059, a young weak-lined T Tauri star (WTTS), member of the pre-main-sequence group in the λ Orionis Cluster. Our high spatial resolution, near-infrared observations with Keck reveal that HDE 245059 is in fact a binary separated by 0.''87, probably composed of two WTTS based on their color indices. Based on this new information we have obtained an estimate of the masses of the binary components; ∼3 M sun and ∼2.5 M sun for the north and south components, respectively. We have also estimated the age of the system to be ∼2-3 Myr. We detect both components of the binary in the zeroth-order Chandra image and in the grating spectra. The light curves show X-ray variability of both sources and in particular a flaring event in the weaker southern component. The spectra of both stars show similar features: a combination of cool and hot plasma as demonstrated by several iron lines from Fe XVII to Fe XXV and a strong bremsstrahlung continuum at short wavelengths. We have fitted the combined grating and zeroth-order spectrum (considering the contribution of both stars) in XSPEC. The coronal abundances and emission measure distribution for the binary have been obtained using different methods, including a continuous emission measure distribution and a multi-temperature approximation. In all cases we have found that the emission is dominated by plasma between ∼8 and ∼15 MK a soft component at ∼4 MK and a hard component at ∼50 MK are also detected. The value of the hydrogen column density was low, N H ∼ 8 x 10 19 cm -2 , likely due to the clearing of the inner region of the λ Orionis cloud, where HDE 245059 is located. The abundance pattern shows an inverse first ionization potential effect for all elements from O to Fe, the only exception being Ca. To obtain the properties of the binary components, a 3-T model was fitted to the individual zeroth-order spectra
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European Decommissioning Academy (EDA). Ready to start
International Nuclear Information System (INIS)
Slugen, Vladimir
2015-01-01
According to analyses presented at EC meeting focused on decommissioning organized at 11 September 2012 in Brussels, it was stated that at least 2,000 new international experts for decommissioning will be needed in Europe up to 2025, which means about 150 each year. The article describes the European Decommissioning Academy (EDA) which is prepared for the first term in June 2015 in Slovakia. The main goal is a creation of new nuclear experts generation for decommissioning via the Academy, which will include lessons, practical exercises in laboratories as well as 2 days on-site training at NPP V-1 in Jaslovske Bohunice (Slovakia). Four days technical tour via most interesting European decommissioning facilities in Switzerland and Italy are planned as well. After the final exam, there is the option to continue in knowledge collection via participation at the 2nd Eastern and Central European Decommissioning (ECED) conference in Trnava (Slovakia). We would like to focus on VVER decommissioning issues because this reactor type is the most distributed design in the world and many of these units are actually in decommissioning process or will be decommissioned in the near future.
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Journal of Chemical Sciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
Indian Academy of Sciences. Home · About IASc · History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair · Jubilee Chair · Academy – Springer Nature chair · Academy Trust · Contact details · Office Staff · Office complaint redressal committee · Positions Available · Citizens Charter ...
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cur | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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jarc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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j | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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May, Cattleya; Cutting, Katharine N
2014-01-01
The Institute for Healthcare Improvement is an independent not-for-profit organization based in Cambridge, Massachusetts. It is a leading innovator in health and health care improvement with a global following.One important part of the IHI is the development and evolution of the "Open School." Launched in September 2008, the online community currently includes hundreds of thousands of students worldwide. The goals of the Open School are consistent with the IHI initial concepts: to build will for change, seek out innovation, share expertise, and build leaders. Each year, the Open School awards scholarships to select students to attend a Leadership Academy.The Student Quality Leadership Academy allows students to network with other future nurses, physicians, and health care administrators and explores how they feel about leadership. This is important to nursing as we will need to replace many leadership positions in the future, but often new nurses are uncertain about leadership roles.
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Most recent entry 16 January 2017. The Academy regrets to report the passing of: Roshko, Prof. Anatol C V Vishveshwara (see YouTube video: Eureka with C. V. Vishveshwara) Mandayam Anandampillai Lakshmi Thathachar Chokkappa Kempanna. © 2017 Indian Academy of Sciences, Bengaluru. Contact | Site index.
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Rakic, Olivera; Schaye, Joop; Steidel, Charles C.; Rudie, Gwen C.
2012-06-01
We study the interface between galaxies and the intergalactic medium by measuring the absorption by neutral hydrogen in the vicinity of star-forming galaxies at z ≈ 2.4. Our sample consists of 679 rest-frame UV-selected galaxies with spectroscopic redshifts that have impact parameters advantage of all available Lyman series lines. The median optical depth, and hence the median density of atomic hydrogen, drops by more than an order of magnitude around 100 kpc, which is similar to the virial radius of the halos thought to host the galaxies. The median remains enhanced, at the >3σ level, out to at least 2.8 Mpc (i.e., >9 comoving Mpc), but the scatter at a given distance is large compared with the median excess optical depth, suggesting that the gas is clumpy. Within 100 (200) kpc, and over ±165 km s-1, the covering fraction of gas with Lyα optical depth greater than unity is 100+0 - 32% (66% ± 16%). Absorbers with τLyα > 0.1 are typically closer to galaxies than random. The mean galaxy overdensity around absorbers increases with the optical depth and also as the length scale over which the galaxy overdensity is evaluated is decreased. Absorbers with τLyα ~ 1 reside in regions where the galaxy number density is close to the cosmic mean on scales >=0.25 Mpc. We clearly detect two types of redshift space anisotropies. On scales 3σ significance), an effect that we attribute to large-scale infall (i.e., the Kaiser effect). Based on data obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, and was made possible by the generous financial support of the W. M. Keck Foundation.
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Sadhana | Indian Academy of Sciences
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences. Indian Academy of ... 2013 pp 571-589. An evolutionary approach for colour constancy based on gamut mapping constraint satisfaction ... A new colour constancy algorithm based on automatic determination of gray framework parameters using neural network · Mohammad Mehdi ...
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Authentic Assessment in the First Steiner Academy
Burnett, John
2009-01-01
In August 2008, the then Schools Minister, Andrew Adonis, gave the go-ahead for the privately funded Hereford Waldorf School to reopen as a tax-payer-funded Academy, sponsored by the Steiner Waldorf Schools Fellowship of Great Britain. Accordingly, the Steiner Academy Hereford opened in September 2008. In common with the 132 other Academies opened…
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THE W. M. KECK OBSERVATORY INFRARED VORTEX CORONAGRAPH AND A FIRST IMAGE OF HIP 79124 B
Energy Technology Data Exchange (ETDEWEB)
Serabyn, E.; Liewer, K. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Huby, E.; Absil, O.; Carlomagno, B.; Defrère, D.; Delacroix, C.; Gonzalez, C. Gomez; Habraken, S.; Jolivet, A.; Piron, P. [Space Sciences, Technologies, and Astrophysics (STAR) Institute, Université de Liège, 19c allée du Six Août, B-4000 Liège (Belgium); Matthews, K.; Mawet, D.; Bottom, M. [California Institute of Technology, Division of Physics, Mathematics and Astronomy, Pasadena, CA 91125 (United States); Femenia, B.; Wizinowich, P.; Campbell, R.; Lilley, S. [W. M. Keck Observatory, 65-1120 Mamalahoa Hwy, Kamuela, HI (United States); Karlsson, M.; Forsberg, P., E-mail: gene.serabyn@jpl.nasa.gov [Department of Engineering Sciences, Ångström Laboratory, Uppsala University, Box 534, SE-751 21 Uppsala (Sweden); and others
2017-01-01
An optical vortex coronagraph has been implemented within the NIRC2 camera on the Keck II telescope and used to carry out on-sky tests and observations. The development of this new L ′-band observational mode is described, and an initial demonstration of the new capability is presented: a resolved image of the low-mass companion to HIP 79124, which had previously been detected by means of interferometry. With HIP 79124 B at a projected separation of 186.5 mas, both the small inner working angle of the vortex coronagraph and the related imaging improvements were crucial in imaging this close companion directly. Due to higher Strehl ratios and more relaxed contrasts in L ′ band versus H band, this new coronagraphic capability will enable high-contrast, small-angle observations of nearby young exoplanets and disks on a par with those of shorter-wavelength extreme adaptive optics coronagraphs.
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Tender Notices | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
... Tender for works related to expansion to main building of Indian Academy of ... for building Hostel Block at Indian Academy of Sciences Fellows Residency, ... the Three Science Academies of India on the teaching of the theory of evolution
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 30 December 1961. Specialization: String Theory Address during Associateship: Institute of Physics, Sachivalaya Marg, Bhubaneswar 751 005. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 27 August 1960. Specialization: Polymer Science Address during Associateship: IPC Department, Indian Institute of Science, Bangalore 560 012. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will ...
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conf | Indian Academy of Sciences
Indian Academy of Sciences (India)
Academy Public Lecture and INSA–Leopoldina Lecture by Prof. Jörg Hacker, President, German Academy of Sciences Leopoldina. 4 December, 2017, 4 PM Faculty Hall, Indian Institute. Associates – 2017. Posted on 30 August 2017. Click here to see the list · 83rd Annual Meeting. Posted on 01 December 2017.
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Nuclear Academy for journalists
International Nuclear Information System (INIS)
Szoenyi, Z.; Bujdoso, E.; Komornik, F.
2000-01-01
Hungarian Atomic Energy Authority launched a comprehensive nuclear training program for journalists in 1999. The aim of the ''Nuclear Academy'' was to gain the journalists for the objective interpretation and - for this reason - to provide them a large-scale knowledge and experience in connection with nuclear energy. The Academy consisted of ten all day long programs monthly, containing lectures, discussions, debates and technical visits to the Paks NPP, research and training reactors, scientific institutions and facilities of waste disposal, etc. Two international outlooks were important events of the training: the journalists visited the Mohovce NPP (Slovakia) and the International Atomic Energy Agency (IAEA) in Vienna.The successful attendants took over diplomas at the closing ceremony in June 2000, which diplomas authorise them to use the ''Nuclear Journalist'' title. The slogan of the Academy was: ''Gain and provide objective information''. (author)
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Canter, Anna Rudolph
2004-12-01
the changes faculty members and administrators have made over time. Chapter Five, "The Students of the Science Academy of South Texas," focuses on the students at the Science Academy, who administrators and teachers describe as "the whole reason we are here." Chapter Six offers concluding thoughts and ideas for future research.
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Information and Announcements Science Academies' Refresher ...
Indian Academy of Sciences (India)
IAS Admin
2015-09-20
Sep 20, 2015 ... Indian National Science Academy, New Delhi, The National Academy ... Advances in Chemistry for College/University teachers and research scholars will be ... Course will cover both basic and advanced topics in Chemistry ...
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Sadhana | Indian Academy of Sciences
Indian Academy of Sciences (India)
Toggle navigation. Logo of the Indian Academy of Sciences. Indian Academy of Sciences. Home · About IASc · History · Memorandum of Association ... Volume 31 Issue 5 October 2006 pp 621-633. Minimizing total costs of forest roads with computer-aided design model · Abdullah E Akay · More Details Abstract Fulltext PDF.
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de Pater, Imke
2015-11-01
We present highlights of our observations of Pele and Pillan on Io, and a multi-decade timeline of thermal emission intensities in both regions. Io was regularly observed by Galileo NIMS during 1996-2001. Since 2001 the satellite has been imaged semi-regularly with NIRC2, coupled to an adaptive optics system, on the 10-m Keck telescope. In 1997, Galileo NIMS observed a large and highly-variable eruption close to Pillan Mons; this eruption lasted several months [1]. Since that time no eruptions had been seen (but time coverage was scarce), until our Keck images on 14 August 2007 revealed an active and highly-energetic eruption at a location close to that of the 1997 eruptions. A one-temperature blackbody fit to the data revealed a (blackbody) temperature of 840 ± 40 K over an area of 17 km2, with a total power output of ~500 GW. Using Davies’ (1996) Io Flow Model [2] we find that the oldest lava present is less than 1-2 hours old, having cooled down from the eruption temperature of >1400 K to ~710 K. This young, hot lava suggests that an episode of lava fountaining was underway. Since 2007, several eruptions have been seen in the Pillan region. The 18 February 2015 eruption was discovered during a mutual occultation event with the NASA IRTF. This event was (serendipitously) subsequently imaged with the Large Binocular Telescope Interferometer (LBTI) on 8 March 2015 during a mutual event occultation, and again with the IRTF on 15 March. The site was imaged with the Keck and Gemini-N telescopes between 27 March and May 5, during which time the intensity gradually decreased. Interestingly, the precise location of the eruption had shifted to the north-west from Pillan Patera, where the initial (18 Feb) eruption had taken place. In contrast to the episodicity of Pillan, Pele has been remarkably consistent in its thermal emission during the Galileo era [1] through February 2002, when a blackbody temperature of 940 ± 40 K and an area of 6.5 km2 was measured. Since that
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Indian Academy of Sciences: Home
Indian Academy of Sciences (India)
Founded in 1934 by Sir C V Raman the Indian Academy of Sciences, Bangalore was registered as a Society on 27 April 1934 with the main objective of promoting the progress and upholding the cause of science. The Academy began functioning with 65 Founding Fellows and the formal inauguration took place at the ...
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Planning Guide for Career Academies
Dayton, Charles
2010-01-01
A career academy is a small learning community within a high school, which selects a subset of students and teachers for a two-, three-, or four-year period. Students enter through a voluntary process; they must apply and be accepted, with parental knowledge and support. A career academy involves teachers from different subjects working together…
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American Academy of Dental Sleep Medicine
... New Research AADSM Highlights Members More news... Dental Sleep Medicine: An area of dental practice that focuses on ... SomnoMed Silver Sponsors Copyright © American Academy of Dental Sleep Medicine, All Rights Reserved. American Academy of Dental Sleep ...
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
The process of election of Fellows is described in the statutes. Nomination forms are provided only to the Fellows and are not made available on the Academy website. Those pursuing research in India are eligible to be nominated. The last date for receipt of new nominations is 31st May. The Academy offers only fellowship ...
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Overview | Journals | Indian Academy of Sciences
Indian Academy of Sciences (India)
2017-12-21
Dec 21, 2017 ... ... Academy of Sciences Parts A and B began publication that very year. The Academy today publishes 12 journals, several of which grew out of ... which is among the oldest English language journals in genetics, having been ...
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Energy Technology Data Exchange (ETDEWEB)
Fischer, P. D.; Brown, M. E.; Trumbo, S. K. [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Hand, K. P., E-mail: pfischer@caltech.edu [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
2017-01-01
We present spatially resolved spectroscopic observations of Europa’s surface at 3–4 μ m obtained with the near-infrared spectrograph and adaptive optics system on the Keck II telescope. These are the highest quality spatially resolved reflectance spectra of Europa’s surface at 3–4 μ m. The observations spatially resolve Europa’s large-scale compositional units at a resolution of several hundred kilometers. The spectra show distinct features and geographic variations associated with known compositional units; in particular, large-scale leading hemisphere chaos shows a characteristic longward shift in peak reflectance near 3.7 μ m compared to icy regions. These observations complement previous spectra of large-scale chaos, and can aid efforts to identify the endogenous non-ice species.
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Consumer Sleep Technology: An American Academy of Sleep Medicine Position Statement.
Khosla, Seema; Deak, Maryann C; Gault, Dominic; Goldstein, Cathy A; Hwang, Dennis; Kwon, Younghoon; O'Hearn, Daniel; Schutte-Rodin, Sharon; Yurcheshen, Michael; Rosen, Ilene M; Kirsch, Douglas B; Chervin, Ronald D; Carden, Kelly A; Ramar, Kannan; Aurora, R Nisha; Kristo, David A; Malhotra, Raman K; Martin, Jennifer L; Olson, Eric J; Rosen, Carol L; Rowley, James A
2018-05-15
Consumer sleep technologies (CSTs) are widespread applications and devices that purport to measure and even improve sleep. Sleep clinicians may frequently encounter CST in practice and, despite lack of validation against gold standard polysomnography, familiarity with these devices has become a patient expectation. This American Academy of Sleep Medicine position statement details the disadvantages and potential benefits of CSTs and provides guidance when approaching patient-generated health data from CSTs in a clinical setting. Given the lack of validation and United States Food and Drug Administration (FDA) clearance, CSTs cannot be utilized for the diagnosis and/or treatment of sleep disorders at this time. However, CSTs may be utilized to enhance the patient-clinician interaction when presented in the context of an appropriate clinical evaluation. The ubiquitous nature of CSTs may further sleep research and practice. However, future validation, access to raw data and algorithms, and FDA oversight are needed. © 2018 American Academy of Sleep Medicine.
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Citizens Charter | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Science Education Panel: The Academy has been undertaking several programmes for improving the state of science education in the country. ... Panels on Scientific Values and Women in Science: As part of the Academy initiatives on topics of importance to scientists, two new panels were set up by the Academy - on ...
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Information and Announcements Science Academies 81st Refresher ...
Indian Academy of Sciences (India)
IAS Admin
2016-09-25
Sep 25, 2016 ... are in (a) mechanics, (b) heat, (c) electricity both DC and AC, (d) magnetism, (e) relaxation, (f) phase sensitive detection technique, and (g) non-linear dynamics. This course is sponsored by Indian Academy of Sciences,. Bangalore, Indian National Science Academy, New Delhi and National Academy of ...
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European Decommissioning Academy
International Nuclear Information System (INIS)
Slugen, V. S.; Hornacek, M.
2016-01-01
Full text: Experiences from the first run of the European Decommissioning Academy (EDA) are reported in details. EDA was created at the Slovak University of Technology in Bratislava Slovakia, based on discussion and expressed needs declared at many international meetings including ECED2013. The first run successfully passed 15 participants during 7–26 June 2015. Academy was focused on decommissioning issues via lessons, practical exercises in laboratories, on-site training prepared at NPP V-1 in Jaslovské Bohunice, Slovakia as well as four day technical tour to other European decommissioning facilities in Switzerland and Italy. Detailed information can be found at http://kome.snus.sk/inpe/. (author
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KECK II OBSERVATIONS OF HEMISPHERICAL DIFFERENCES IN H2O2 ON EUROPA
International Nuclear Information System (INIS)
Hand, K. P.; Brown, M. E.
2013-01-01
We present results from Keck II observations of Europa over four consecutive nights using the near-infrared spectrograph. Spectra were collected in the 3.14-4.0 μm range, enabling detection and monitoring of the 3.5 μm feature due to hydrogen peroxide. Galileo Near-Infrared Mapping Spectrometer results first revealed hydrogen peroxide on Europa in the anti-Jovian region of the leading hemisphere at a percent by number abundance of 0.13% ± 0.07% relative to water. We find comparable results for the two nights over which we observed the leading hemisphere. Significantly, we observed a small amount of hydrogen peroxide (∼0.04%) during observations of Europa's anti-Jovian and sub-Jovian hemispheres. Almost no hydrogen peroxide was detected during observations of just the trailing hemisphere. We conclude that the Galileo observations likely represent the maximum hydrogen peroxide concentration, the exception potentially being the cold water ice regions of the poles, which are not readily observable from the ground. Our mapping of the peroxide abundance across Europa requires revisions to previous estimates for Europa's global surface abundance of oxidants and leads to a reduction in the total oxidant delivery expected for the subsurface ocean if an exchange of surface material with the ocean occurs.
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Academy named after newsreader's wife.
2010-06-24
AN ADMIRAL nurse academy named in honour of Bonnie Suchet, the wife of former newsreader John Suchet, has opened. The 'virtual' academy, set up by charity dementia UK, Canterbury Christ Church University and the Avante Partnership, will provide continuing professional development and a networking environment for n nurses through its website. Ms Suchet has Alzheimer's disease and is in a care home.
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Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; Events. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June ...
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currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June ...
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Polish Academy of Sciences Great Dictionary of Polish [Wielki słownik języka polskiego PAN
Directory of Open Access Journals (Sweden)
Piotr Žmigrodzki
2014-12-01
Full Text Available The paper describes a lexicographical project involving the development of the newest general dictionary of the Polish language: the Polish Academy of Sciences Great Dictionary of Polish [Wielki słownik języka polskiego PAN]. The project is coordinated by the Institute of Polish Language at the Polish Academy of Sciences and carried out in collaboration with linguists and lexicographers from several other Polish academic centres. The paper offers a brief description of the genesis of the project and the scope of information included in the dictionary, the organisation of work, the life of the dictionary on the Web as well as the plans for the future.
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Committee on Scientific Values | Initiatives | Indian Academy of ...
Indian Academy of Sciences (India)
Academy Committee on Scientific Values. The Council of the Academy had in 2003 constituted a Committee to consider and submit a report on ethical guidelines which the fellowship of the Academy should follow. The Committee submitted its report to the Council, which at its meeting in December 2005 approved this report ...
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VizieR Online Data Catalog: Brown dwarf surface gravities with Keck/NIRSPEC (Martin , 2017)
Martin, E. C.; Mace, G. N.; McLean, I. S.; Logsdon, S. E.; Rice, E. L.; Kirkpatrick, J. D.; Burgasser, A. J.; McGovern, M. R.; Prato, L.
2017-10-01
In this paper, we follow up on prior NIR spectroscopy by our group and use a modified Allers & Liu (A13, 2013ApJ...772...79A) method to determine surface gravities for 228 M, L, and T dwarfs. We present medium-resolution (R~20000) J-band spectra of 85 M dwarfs, 92 L dwarfs, and 51 T dwarfs obtained as part of the Keck NIRSPEC Brown Dwarf Spectroscopic Survey (BDSS). Ninety-seven spectra were published previously in McLean+ (2003ApJ...596..561M), Burgasser+ (2003ApJ...592.1186B), McGovern+ (2004ApJ...600.1020M), Rice+ (2010ApJS..186...63R), Kirkpatrick+ (2010, J/ApJS/190/100), Luhman (2012ARA&A..50...65L), Thompson+ (2013PASP..125..809T), Mace+ (2013, J/ApJS/205/6), Mace+ (2013ApJ...777...36M), and Kirkpatrick+ (2014, J/ApJ/783/122), and the remaining 131 are presented here for the first time. Observation information (spanning 1999 Apr to 2015 Mar) for all of the targets in our sample is listed in Table 1. (4 data files).
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A DEEP KECK/NIRC2 SEARCH FOR THERMAL EMISSION FROM PLANETARY COMPANIONS ORBITING FOMALHAUT
Energy Technology Data Exchange (ETDEWEB)
Currie, Thayne; Cloutier, Ryan [University of Toronto, 50 St George St., Toronto, ON M5S 1A1 (Canada); Debes, John H. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Kenyon, Scott J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kaisler, Denise [Citrus College, 1000 West Foothill Boulevard, Glendora, CA 91741 (United States)
2013-11-01
We present deep Keck/NIRC2 1.6 and 3.8 μm imaging of Fomalhaut to constrain the near-infrared brightness of Fomalhaut b, recently confirmed as a likely planet, and search for additional planets at r {sub proj} = 15-150 AU. Using advanced/novel point spread function subtraction techniques, we identify seven candidate substellar companions Fomalhaut b-like projected separations. However, multi-epoch data show them to be background objects. We set a new 3σ upper limit for Fomalhaut b's H-band brightness of m(H) ∼23.15 or 1.5-4.5 M{sub J} . We do not recover the possible point source reported from Spitzer/IRAC data: at its location detection limits are similar to those for Fomalhaut b. Our data when combined with other recent work rule out planets with masses and projected separations comparable to HR 8799 bcde and M > 3 M{sub J} planets at r {sub proj} > 45 AU. The James Webb Space Telescope will likely be required to shed substantial further light on Fomalhaut's planetary system in the next decade.
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series; Volume 1; Issue 1. Chimera-like states generated by large perturbation of synchronous state of coupled metronomes. SERGEY BREZETSKIY DAWID DUDKOWSKI PATRYCJA JAROS JERZY WOJEWODA KRZYSZTOF CZOLCZYNSKI YURI MAISTRENKO ...
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STEM Summer Academy on the Navajo Reservation
Alexander, C. J.
2012-12-01
Navajo contributors. In 2012, the Academy was conducted with 45 children and 4 instructors. Following up on lessons learned in previous reports, it is clear that community involvement and buy-in is critical to the success of the program. This means that the US Rosetta Project modified its goals and curriculum to accommodate the teaching desires of teachers in the district, and the capabilities of the medicine men that agreed to participate. The use of NASA material and imagery can be shown to have a positive impact on the accessibility of the overall STEM material. Metrics used in the program will be discussed. Future work to extract STEM language elements to enhance the program will include organized Elder's Round Tables for discussion, and recording, of language with first speakers. Work on this project was supported by NASA at California Institute of Technology/Jet Propulsion Laboratory.
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1173.pdf | may102008 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
How to combat infectious diseases: The role of Science Academies · Academy Public Lecture and INSA–Leopoldina Lecture by Prof. Jörg Hacker, President, German Academy of Sciences Leopoldina. 4 December, 2017, 4 PM Faculty Hall, Indian Institute ...
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Double Consciousness and the Future of Service-Learning
Hickmon, Gabrielle
2015-01-01
The author begins this essay by reflecting on an article penned twenty years earlier, "Does Service-Learning Have a Future?" (Zlotkowski, 1995) that called educators to attend seriously to the academic aspects of service-learning (SL), to situate the pedagogy strongly within the academy as a means of legitimizing and expanding the work.…
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Considerations about the European Decommissioning Academy (EDA)
International Nuclear Information System (INIS)
Slugen, V.; Hinca, R.
2014-01-01
According to analyses presented at EC meeting focused on decommissioning organized at 11.9.2012 in Brussels, it was stated that at least 500 new international experts for decommissioning will be needed in Europe up to 2025, which means about 35 per year.Having in mind the actual EHRO-N report from 2013 focused on operation of nuclear facilities and an assumption that the ratio between nuclear experts, nuclearized and nuclear aware people is comparable also for decommissioning (16:74:10), as well as the fact that the special study branch for decommissioning in the European countries almost does not exist, this European Decommissioning Academy (EDA) could be helpful in the overbridging this gap.For the first run of the EDA scheduled on 2014 we would like to focus on VVER decommissioning issues because this reactor type is the most distributed design in the world and many of these units are actually in decommissioning process or will be decommissioned in the near future in Europe.A graduate of the European Decommissioning Academy (EDA) should have at least bachelor level from technical or natural science Universities or Colleges and at least one year working experiences in the area of NPP decommissioning or nuclear power engineering. This study creates prerequisites for acquiring and completion of professional and specialized knowledge in the subjects which are described. (authors)
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75 FR 39561 - National Fire Academy Board of Visitors
2010-07-09
...] National Fire Academy Board of Visitors AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The National Fire Academy Board of... the docket to read background documents or comments received by the National Fire Academy Board of...
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Associateship | Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Associateship. Associate of the Indian Academy of Sciences. This programme was initiated by the Academy in 1983 to identify and encourage promising young scientists. The Associateship is tenable for a maximum period of five years until the age of 35 or a minimum period of three years. During this period the Associates ...
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Thakore, Bhoomi K; Naffziger-Hirsch, Michelle E; Richardson, Jennifer L; Williams, Simon N; McGee, Richard
2014-08-02
Approaches to training biomedical scientists have created a talented research community. However, they have failed to create a professional workforce that includes many racial and ethnic minorities and women in proportion to their representation in the population or in PhD training. This is particularly true at the faculty level. Explanations for the absence of diversity in faculty ranks can be found in social science theories that reveal processes by which individuals develop identities, experiences, and skills required to be seen as legitimate within the profession. Using the social science theories of Communities of Practice, Social Cognitive Career Theory, identity formation, and cultural capital, we have developed and are testing a novel coaching-based model to address some of the limitations of previous diversity approaches. This coaching intervention (The Academy for Future Science Faculty) includes annual in-person meetings of students and trained faculty Career Coaches, along with ongoing virtual coaching, group meetings and communication. The model is being tested as a randomized controlled trial with two cohorts of biomedical PhD students from across the U.S., one recruited at the start of their PhDs and one nearing completion. Stratification into the experimental and control groups, and to coaching groups within the experimental arms, achieved equal numbers of students by race, ethnicity and gender to the extent possible. A fundamental design element of the Academy is to teach and make visible the social science principles which highly influence scientific advancement, as well as acknowledging the extra challenges faced by underrepresented groups working to be seen as legitimate within the scientific communities. The strategy being tested is based upon a novel application of the well-established principles of deploying highly skilled coaches, selected and trained for their ability to develop talents of others. This coaching model is intended to be a
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Department of Transportation — IRIS is a suite of front-end web applications utilizing a centralized back-end Oracle database. The system fully supports the FAA Academy's Distance Learning Program...
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Role of the Academy | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
The Academy has laid the responsibility on all its Fellows, individually and ... the principle of social responsibility for all scientific effort, individual or corporate, ... to provide publication opportunities to Indian scientists at the international level; ...
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Home; Journals; Indian Academy of Sciences Conference Series; Volume 1; Issue 1. Missing cycles: Effect of climate change on population dynamics. JANAKI BALAKRISHNAN SUDHARSANA V IYENGAR JÜRGEN KURTHS. Proceedings of the Conference on Perspectives in Nonlinear Dynamics - 2016 Volume 1 Issue 1 ...
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Planned obsolescence publishing, technology, and the future of the academy
Fitzpatrick, Kathleen
2011-01-01
Academic institutions are facing a crisis in scholarly publishing at multiple levels: presses are stressed as never before, library budgets are squeezed, faculty are having difficulty publishing their work, and promotion and tenure committees are facing a range of new ways of working without a clear sense of how to understand and evaluate them. Planned Obsolescence is both a provocation to think more broadly about the academy’s future and an argument for reconceiving that future in more communally-oriented ways. Facing these issues head-on, Kathleen Fitzpatrick focuses on the technological changes—especially greater utilization of internet publication technologies, including digital archives, social networking tools, and multimedia—necessary to allow academic publishing to thrive into the future. But she goes further, insisting that the key issues that must be addressed are social and institutional in origin. Springing from original research as well as Fitzpatrick’s own hands-on experiments in ne...
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Annual Meetings | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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pju | splpubs | pubs | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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B | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Leadership Academies: Elixir for Common School Ills.
School Administrator, 1989
1989-01-01
Describes a model leadership academy program at Topeka (Kansas) Public Schools in cooperation with Kansas State University. Created in 1987, the academy was designed to serve the school system's unique needs while fostering innovative educational experiences for administrator preparation. Includes four references. (MLH)
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Academy of Program/Project & Engineering Leadership Annual Publications
National Aeronautics and Space Administration — Academy of Program/Project & Engineering Leadership's Annual Report highlights the Academy's efforts to serve the NASA workforce's needs in adapting to the...
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Role of the Academy | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
... individual or corporate, is entirely consistent with individual freedom and that the quest for knowledge and ... within the Academy a fuller representation of the Indian scientific community in its corporate body so that the ... Math and Finance ...
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A search for lithium in Pleiades brown dwarf candidates using the Keck hires echelle
Marcy, Geoffrey W.; Basri, Gibor; Graham, James R.
1994-01-01
We report Keck Observatory high-resolution echelle spectra of lithium at 670.8 nm in two of the lowest luminosity brown dwarf candidates in the Pleiades. These objects have estimated masses of 0.055 to 0.059 solar mass from their location on a color-magnitude diagram relative to theoretical isochrones. Stellar interior models predict that Li has not burned in them. However, we find no evidence of the Li line, at limits 100 to 1000 times below the initial abundance. This indicates that Li has in fact been depleted, presumably by nuclear processing as occurs in Pleiades stars. Interior models suggest that such large Li depletion occurs only for objects with M greater than 0.09 solar mass at the age of the Pleiades. Thus, it is unlikely that the candidates are brown dwarfs. The brown dwarf candidates present a conflict: either they have masses greater than suggested from their placement on the H-R diagram, or they do have the very low suggested masses but are nonetheless capable of destroying Li, in only 70 Myr. Until this dilemma is resolved, the photometric identification of brown dwarfs will remain difficult. Resolution may reside in higher T(sub eff) derived from optical and IR colors or in lower T(sub eff) in the interior models.
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Annual Meetings · Mid Year Meetings · Discussion Meetings · Public Lectures · Lecture Workshops · Refresher Courses · Symposia · Live Streaming. Home; Journals; Indian Academy of Sciences Conference Series; Volume 1; Issue 1. Organizing Commitee. Proceedings of the Conference on Perspectives in Nonlinear ...
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publications.html | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; publications.html. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from ...
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associates.html | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; associates.html. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 ...
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Journal of the Cameroon Academy of Sciences
African Journals Online (AJOL)
Revue de L'academie des Sciences du Cameroun The Journal of the Cameroon Academy of Sciences is a multi-disciplinary publication devoted to all aspects of fundamental and applied research. It also publishes topical reviews on science and technology in development, arts, humanities and culture.
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Selling Academies: Local Democracy and the Management of "Consultation"
Hatcher, Richard
2008-01-01
Academies (state schools owned and run by private sponsors on a non-profit basis) are a key element in Labour's education agenda. Proposals to set up Academies, in most cases by taking over existing schools, have provoked local campaigns of opposition in many areas. Replacing a Local Authority with an Academy entails a process of consultation.…
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Energy Technology Data Exchange (ETDEWEB)
Merchant Boesgaard, Ann; Lum, Michael G. [Institute for Astronomy, University of Hawai' i at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Deliyannis, Constantine P., E-mail: boes@ifa.hawaii.edu, E-mail: mikelum@ifa.hawaii.edu, E-mail: cdeliyan@indiana.edu [Department of Astronomy, Indiana University 727 East 3rd Street, Swain Hall West 319, Bloomington, IN 47405-7105 (United States)
2015-02-01
The study of star clusters has advanced our understanding of stellar evolution, Galactic chemical evolution, and nucleosynthesis. Here we investigate the composition of turn-off stars in the intriguing open cluster, NGC 6791, which is old, but super-metal-rich with high-resolution (R = 46,000) Keck/HIRES spectra. We find [Fe/H] = +0.30 ± 0.02 from measurements of some 40 unblended, unsaturated lines of both Fe I and Fe II in eight turn-off stars. Our O abundances come from the O I triplet near 7774 Å and we perform a differential analysis relative to the Sun from our Lunar spectrum also obtained with Keck/HIRES. The O results are corrected for small nLTE effects. We find consistent ratios of [O/Fe]{sub n} with a mean of –0.06 ± 0.02. This is low with respect to field stars that are also both old and metal-rich and continue the trend of decreasing [O/Fe] with increasing [Fe/H]. The small range in our oxygen abundances is consistent with a single population of stars. Our results for the alpha elements [Mg/Fe], [Si/Fe], [Ca/Fe], and [Ti/Fe] are near solar and compare well with those of the old, metal-rich field stars. The two Fe-peak elements, Cr and Ni, are consistent with Fe. These turn-off-star abundances provide benchmark abundances to investigate whether there are any observable abundance differences with the giants that might arise from nuclear-burning and dredge-up processes. Determinations of upper limits were found for Li by spectrum synthesis and are consistent with the upper limits in similar stars in the relatively old, super-metal-rich cluster NGC 6253. Our results support the prediction from standard theory that higher-metallicity stars deplete more Li. Probably no stars in NGC 6791 have retained their initial Li.
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report2.pdf | cvnit | academy | Indian Academy of Sciences
Indian Academy of Sciences (India)
Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more. ... Posted on 21 December 2017. ASTROPHYSICS: An Observational View of the Universe. Math Art and Design: MAD about Math, Math Education and Outreach.
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Indian Academy of Sciences Conference Series | Indian Academy of ...
Indian Academy of Sciences (India)
Aim and Scope. The scope of the Indian Academy of Sciences Conference Series is to publish invited and peer reviewed original research, review, perspective, and commentary articles arising from presentations at select and topical Scientific Conferences. Upto four issues are published a year, each edited in consultation ...
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Ade, P A R; Ahmed, Z; Aikin, R W; Alexander, K D; Barkats, D; Benton, S J; Bischoff, C A; Bock, J J; Bowens-Rubin, R; Brevik, J A; Buder, I; Bullock, E; Buza, V; Connors, J; Crill, B P; Duband, L; Dvorkin, C; Filippini, J P; Fliescher, S; Grayson, J; Halpern, M; Harrison, S; Hilton, G C; Hui, H; Irwin, K D; Karkare, K S; Karpel, E; Kaufman, J P; Keating, B G; Kefeli, S; Kernasovskiy, S A; Kovac, J M; Kuo, C L; Leitch, E M; Lueker, M; Megerian, K G; Netterfield, C B; Nguyen, H T; O'Brient, R; Ogburn, R W; Orlando, A; Pryke, C; Richter, S; Schwarz, R; Sheehy, C D; Staniszewski, Z K; Steinbach, B; Sudiwala, R V; Teply, G P; Thompson, K L; Tolan, J E; Tucker, C; Turner, A D; Vieregg, A G; Weber, A C; Wiebe, D V; Willmert, J; Wong, C L; Wu, W L K; Yoon, K W
2016-01-22
We present results from an analysis of all data taken by the BICEP2 and Keck Array cosmic microwave background (CMB) polarization experiments up to and including the 2014 observing season. This includes the first Keck Array observations at 95 GHz. The maps reach a depth of 50 nK deg in Stokes Q and U in the 150 GHz band and 127 nK deg in the 95 GHz band. We take auto- and cross-spectra between these maps and publicly available maps from WMAP and Planck at frequencies from 23 to 353 GHz. An excess over lensed ΛCDM is detected at modest significance in the 95×150 BB spectrum, and is consistent with the dust contribution expected from our previous work. No significant evidence for synchrotron emission is found in spectra such as 23×95, or for correlation between the dust and synchrotron sky patterns in spectra such as 23×353. We take the likelihood of all the spectra for a multicomponent model including lensed ΛCDM, dust, synchrotron, and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r) using priors on the frequency spectral behaviors of dust and synchrotron emission from previous analyses of WMAP and Planck data in other regions of the sky. This analysis yields an upper limit r_{0.05}<0.09 at 95% confidence, which is robust to variations explored in analysis and priors. Combining these B-mode results with the (more model-dependent) constraints from Planck analysis of CMB temperature plus baryon acoustic oscillations and other data yields a combined limit r_{0.05}<0.07 at 95% confidence. These are the strongest constraints to date on inflationary gravitational waves.
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Office Staff | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Administration; Editorial Staff - Academy; Editorial Staff - Current Science ... Coordinator, Summer Research Fellowship Programme (Science Education Panel), .... Joint Statement by the Three Science Academies of India on the teaching of the ...
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.pdf | Volumes | public | Indian Academy of Sciences
Indian Academy of Sciences (India)
Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more... Introducing: Summer Schools. Posted on 21 December 2017. ASTROPHYSICS: An Observational View of the ... Academy Public Lecture. Posted on 19 January 2018. Seasonal and Pandemic Influenza by Prof.
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Chain Effects: The Impact of Academy Chains on Low Income Students
Hutchings, Merryn; Francis, Becky; De Vries, Robert
2014-01-01
The authors analysed school performance data to review how well disadvantaged pupils achieve in academy chains. They included chains only if they had at least three academies in 2013, and two sponsored secondary academies for the whole period from September 2010 to July 2013. This means that academies are included in our analysis only when there…
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Obstacles Facing the Iranian Basketball Academy
Hamta Hadian; Mohamad Reza Boroumand; Saeed Amirnejad; Masoud Najafi
2016-01-01
This study, which is a strategic study with a mixed research approach aimed to identify obstacles facing the academies of Iranian Basketball Federation. The population comprises board of directors and committees responsible for Education and Talent Spotting Association, academy administrators, physical education instructors, qualified experts, professors, coaches, referees and heads of delegations who were asked via interviews and questionnaire (exploratory manner) to state internal and exter...
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journals | pubs | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Startup - Philippines Community Electronic Centres Academy | CRDI ...
International Development Research Centre (IDRC) Digital Library (Canada)
... involved in setting up such an academy, such as formulating operational guidelines, competency standards and an accreditation program. The team will also pilot a CeC training course using the train-the-trainers approach, form a mentors' network and engage in social marketing, advocacy and promotion of the academy.
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
All correspondence regarding subscription within India should be addressed to the Circulation Department, Indian Academy of Sciences, at the address below, or by e-mail to orders@ias.ac.in. See the Academy journals page for the latest subscription information (PDF file) and 2018 subscription prices (Library, Personal).
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Bulkeley, Kelly
2017-10-01
This article describes the future prospects of scientific dream research. Three frontiers of investigation hold special promise: neuroscientific studies of the brain-mind system's activities during sleep (such as during lucid dreaming); systematic analyses of large collections of dream reports from diverse populations of people; and psychotherapeutic explorations of the multiple dimensions of personal and collective meaning woven into the dream experiences of each individual. Several helpful books on the science of sleep and dreaming are mentioned for further study. © 2017 New York Academy of Sciences.
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Contact details | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Academy Fellows' Residency, Jalahalli. Indian Academy of Sciences (Next to ISRO Housing Colony, Near HMT School) Jalahalli West Bengaluru 560 031 Tel.: +91-80-2838 1934. Location on Google Map · Sketch Map ...
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PEMANFAATAN WEB KHAN ACADEMY DALAM PEMBELAJARAN MATEMATIKA
Directory of Open Access Journals (Sweden)
Joko Soebagyo
2016-02-01
Full Text Available Artikel ini bertujuan untuk mengobservasi pemanfaatan web Khan Academy siswa SMK Swasta di Jakarta Utara. Observasi dilakukan untuk mengamati aktivitas siswa dalam menggunakan web khan academy selama proses pembelajaran matematika. Pemanfaatan teknologi dalam proses pembelajaran matematika sudah sepatutnya dilakukan oleh pihak-pihak yang ikut bertanggungjawab atas keberhasilan belajar matematika perserta didik. Teknologi merupakan hal yang tidak bisa dipisahkan dalam kehidupan sehari-hari dan salah satu bentuk teknologi yang sering dimanfaatkan saat ini adalah website dimana akitifitas pekerjaan, pendidikan, hiburan dan hubungan sosial, semuanya dapat dialami melalui website. Dibutuhkan sebuah website yang bias mengakomodir siswa dalam proses pembelajaran matematika baik di dalam kelas maupun di luar kelas. Kriteria web yang baik haruslah memberikan kemudahan dalam pemanfaatannya, salah satu web tersebut adalah web khan academy. This paper aims to observe the use of web Khan Academy Private vocational students in North Jakarta. Observations carried out to observe the activities of the students in using web khan academy during the learning process of mathematics. The use of technology in the learning process of mathematics has been duly carried out by parties who share responsibility for the success of students studying mathematics participants. Technology is something that can not be separated in everyday life and one form of technology that is often used today is a website where the activity, employment, education, entertainment and social relationships, all of which can be experienced through the website. It takes a biased website to accommodate students in mathematics learning process both in the classroom and outside the classroom. Criteria for good web should provide ease of use, one of the web is a web khan academy.
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78 FR 25289 - Board of Visitors for the National Fire Academy Teleconference
2013-04-30
...] Board of Visitors for the National Fire Academy Teleconference AGENCY: Federal Emergency Management... National Fire Academy (Academy) and advise the Administrator of the Federal Emergency Management Agency.... SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet via teleconference on...
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Duplessis, Gilda
2008-01-01
Immediately after the devastation of Hurricane Katrina, the author and her partner made a decision to rebuild their child care center as two apartments. However, the city of New Orleans would only approve the location for one dwelling with a child care center. This article describes the author's experiences in rebuilding Gilda's Academy, her child…
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THE INNER KILOPARSEC OF Mrk 273 WITH KECK ADAPTIVE OPTICS
Energy Technology Data Exchange (ETDEWEB)
U, Vivian; Sanders, David; Kewley, Lisa [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96822 (United States); Medling, Anne; Max, Claire [Department of Astronomy and Astrophysics, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Armus, Lee [Spitzer Science Center, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Iwasawa, Kazushi [ICREA and Institut del Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès, 1, E-08028 Barcelona (Spain); Evans, Aaron [Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904 (United States); Fazio, Giovanni, E-mail: vivianu@ucr.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States)
2013-10-01
There is X-ray, optical, and mid-infrared imaging and spectroscopic evidence that the late-stage ultraluminous infrared galaxy merger Mrk 273 hosts a powerful active galactic nucleus (AGN). However, the exact location of the AGN and the nature of the nucleus have been difficult to determine due to dust obscuration and the limited wavelength coverage of available high-resolution data. Here we present near-infrared integral-field spectra and images of the nuclear region of Mrk 273 taken with OSIRIS and NIRC2 on the Keck II Telescope with laser guide star adaptive optics. We observe three spatially resolved components, and analyze the nuclear molecular and ionized gas emission lines and their kinematics. We confirm the presence of the hard X-ray AGN in the southwest nucleus. In the north nucleus, we find a strongly rotating gas disk whose kinematics indicate a central black hole of mass 1.04 ± 0.1 × 10{sup 9} M{sub ☉}. The H{sub 2} emission line shows an increase in velocity dispersion along the minor axis in both directions, and an increased flux with negative velocities in the southeast direction; this provides direct evidence for a collimated molecular outflow along the axis of rotation of the disk. The third spatially distinct component appears to the southeast, 640 and 750 pc from the north and southwest nuclei, respectively. This component is faint in continuum emission but shows several strong emission line features, including [Si VI] 1.964 μm which traces an extended coronal-line region. The geometry of the [Si VI] emission combined with shock models and energy arguments suggest that [Si VI] in the southeast component must be at least partly ionized by the SW AGN or a putative AGN in the northern disk, either through photoionization or through shock-heating from strong AGN- and circumnuclear-starburst-driven outflows. This lends support to a scenario in which Mrk 273 may be a dual AGN system.
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KECK/LRIS SPECTROSCOPIC CONFIRMATION OF COMA CLUSTER DWARF GALAXY MEMBERSHIP ASSIGNMENTS
International Nuclear Information System (INIS)
Chiboucas, Kristin; Tully, R. Brent; Marzke, Ronald O.; Trentham, Neil; Ferguson, Henry C.; Hammer, Derek; Carter, David; Khosroshahi, Habib
2010-01-01
Keck/LRIS multi-object spectroscopy has been carried out on 140 of some of the lowest and highest surface brightness faint (19 < R < 22) dwarf galaxy candidates in the core region of the Coma Cluster. These spectra are used to measure redshifts and establish membership for these faint dwarf populations. The primary goal of the low surface brightness sample is to test our ability to use morphological and surface brightness criteria to distinguish between Coma Cluster members and background galaxies using high resolution Hubble Space Telescope/Advanced Camera for Surveys images. Candidates were rated as expected members, uncertain, or expected background. From 93 spectra, 51 dwarf galaxy members and 20 background galaxies are identified. Our morphological membership estimation success rate is ∼100% for objects expected to be members and better than ∼90% for galaxies expected to be in the background. We confirm that low surface brightness is a very good indicator of cluster membership. High surface brightness galaxies are almost always background with confusion arising only from the cases of the rare compact elliptical (cE) galaxies. The more problematic cases occur at intermediate surface brightness. Many of these galaxies are given uncertain membership ratings, and these were found to be members about half of the time. Including color information will improve membership determination but will fail for some of the same objects that are already misidentified when using only surface brightness and morphology criteria. cE galaxies with B-V colors ∼0.2 mag redward of the red sequence in particular require spectroscopic follow up. In a sample of 47 high surface brightness, ultracompact dwarf candidates, 19 objects have redshifts which place them in the Coma Cluster, while another 6 have questionable redshift measurements but may also prove to be members. Redshift measurements are presented and the use of indirect means for establishing cluster membership is
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e-Books | Publications | Indian Academy of Sciences
Indian Academy of Sciences (India)
e-Books. of the Indian Academy of Sciences. The following publications of the Academy are now available in e-Book (ePub) format. More details about the format can be seen here. Organic Chemistry Masterclasses Articles by Prof. S Ranganathan in Resonance Download ePub | Read online. Linear Algebra and Analysis ...
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Public Lectures | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Public and special lectures. Academy Public Lectures · Public and special lectures in Mid-Year and Annual Meetings · Platinum Jubilee Lectures. Academy's annual and mid-year meetings include a special lecture by a senior Fellow in the morning of each meeting day and one public lecture by an eminent person, from ...
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Minimally invasive glaucoma surgery: current status and future prospects
Directory of Open Access Journals (Sweden)
Richter GM
2016-01-01
Full Text Available Grace M Richter,1,2 Anne L Coleman11UCLA Stein Eye Institute, Department of Ophthalmology, University of California, Los Angeles, CA, USA; 2USC Eye Institute, Department of Ophthalmology, Keck School of Medicine of University of Southern California, Los Angeles, CA, USAAbstract: Minimally invasive glaucoma surgery aims to provide a medication-sparing, conjunctival-sparing, ab interno approach to intraocular pressure reduction for patients with mild-to-moderate glaucoma that is safer than traditional incisional glaucoma surgery. The current approaches include: increasing trabecular outflow (Trabectome, iStent, Hydrus stent, gonioscopy-assisted transluminal trabeculotomy, excimer laser trabeculotomy; suprachoroidal shunts (Cypass micro-stent; reducing aqueous production (endocyclophotocoagulation; and subconjunctival filtration (XEN gel stent. The data on each surgical procedure for each of these approaches are reviewed in this article, patient selection pearls learned to date are discussed, and expectations for the future are examined. Keywords: MIGS, microincisional glaucoma surgery, trabecular stent, Schlemm’s canal, suprachoroidal shunt, ab interno
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Journal of Biosciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
2016-08-26
Aug 26, 2016 ... Home; Journals; Journal of Biosciences; Search ... part of the email address of all email addresses used by the office of Indian Academy of Sciences, including those of the staff, the journals, various programmes, and Current Science, has changed from 'ias.ernet.in' (or 'academy.ias.ernet.in') to 'ias.ac.in'.
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Parent Academy: Evaluation Report and Executive Summary
Husain, Fatima; Jabin, Nico; Haywood, Sarah; Kasim, Adetayo; Paylor, Jonathan
2016-01-01
The Parent Academy was a series of classes for pupils' parents, designed to improve the English and mathematics attainment of pupils in Years 3 to 6 in English primary schools. Parents were offered the opportunity to participate in 12 Parent Academy classes, 6 on English and 6 on mathematics, delivered fortnightly by tutors with teaching…
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Live Streaming | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Live Streaming. Watch Academy events live here! There are no live events currently happening. Watch out this space for updates or suscribe to our YouTube channel by clicking here. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year ...
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Hydrocarbons cocktails of the future
International Nuclear Information System (INIS)
Anon.
2004-01-01
This publication of the Areva Group, a world nuclear industry leader, provides information on the energy in many domains. This issue deals with the CO 2 pollution exchange, the carbon sinks to compensate the CO 2 , the green coal as an innovative solution, an outsize dam in China, the solar energy progresses in France and the french medicine academy in favor of Nuclear. A special chapter is devoted to the hydrocarbons of the future, artificial chemical combination created from constituents of hydrocarbons and derived from various sources. (A.L.B.)
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How Academies use science to enhance global security and well-being.
Boright, John
2017-01-01
Science academies were originally created to facilitate science communication and later to recognize excellence. But in the last 20 years some 150 academies of science, engineering,and medicine around the world have united to cooperate in contributing to human welfare, by: 1. Providing evidence-based inputs to national, regional, and global policies addressing human needs, and 2. Conducting cooperative programs to increase the capacity of academies to provide such advice, and to better connect academies to publics and to policy makers. Examples: At the global level, 112 academies of science produce brief common statements on major global issues. They have also created an organization to provide in-depth reports on major issues such as a transition to sustainable energy systems, boosting agricultural productivity in Africa, and a guide to responsible conduct in the global research enterprise. Regional networks of those academies, in Africa, the Americas, Asia, and Europe conduct program on topics such as water, energy, engagement of women in science, and science education. They also help and mentor new academies.
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70am | annmeet | meetings | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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absfeb2015.htm | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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san boq.pdf | office | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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00001061.pdf | 6 | bms | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Science Academies' Refresher Course on Innovations in Genetics ...
Indian Academy of Sciences (India)
PG and Research Department of Botany, Vivekananda College of Arts and Sciences for Women. (Autonomous), Elayampalayam ... Academy of Sciences, Bengaluru. Indian National Science Academy, New Delhi ... R Uma Shaankar, Department of Crop physiology and School of Ecology and Conservation, University of ...
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Bulletin of Materials Science | Indian Academy of Sciences
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences. Indian Academy of ... using Scherrer's formula. Volume 27 Issue 2 April 2004 pp 213-216 High Pressure Studies. High pressure effect on MoS2 and MoSe2 single crystals grown by CVT method.
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Resonance – Journal of Science Education | Indian Academy of ...
Indian Academy of Sciences (India)
2016 Nobel Prize in Chemistry: Conferring Molecular Machines as Engines of Creativity ... Science Academies' 92nd Refresher Course in Experimental Physics ... Science Academies' Refresher Course on Advances in Molecular Biology.
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77 FR 21576 - Board of Visitors for the National Fire Academy
2012-04-10
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Teleconference Meeting. SUMMARY: The Board... National Fire Academy (Academy) and advise the Administrator of the Federal Emergency Management Agency...
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backissues.htm | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci; backissues.htm. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from ...
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Journal of | Journals | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; Journals; Journal of. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from ...
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contents.htm | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci; contents.htm. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from ...
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Feofilova, E P
2004-01-01
This review deals with the historical development of mycology at the Winogradsky Institute of Microbiology (Russian Academy of Sciences). Starting from the works of Academician G.A. Nadson, the review considers from the historical perspective the main achievements of the researchers of the Institute in the field of mycology, including such important subfields as the cytology, genetics, physiology, and biochemistry of mycelial fungi and yeast. The review concerns itself with the major theoretical ideas generated by the team of the Laboratory of Experimental Mycology in the course of their studies of micro- and macromycetes. Special attention is also given to recent developments in biotechnology and medicine, including the development of new drug preparations from biologically active substances of fungi.
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The Teachers Academy for Mathematics and Science. Executive summary and program activities update
Energy Technology Data Exchange (ETDEWEB)
1992-09-01
In his State of the Union address on January 31, 1990, President Bush set a goal for US students to be number one in the world in mathematics and science achievement by the year 2000. The Teachers Academy for Mathematics and Science in Chicago is an experiment of unprecedented boldness and scale that can provide a means to the President`s goal, both for the Chicago area and as a national model. This document covers organization and governance, program activities, future training goals, and evaluation programs.
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Visible Leading: Principal Academy Connects and Empowers Principals
Hindman, Jennifer; Rozzelle, Jan; Ball, Rachel; Fahey, John
2015-01-01
The School-University Research Network (SURN) Principal Academy at the College of William & Mary in Williamsburg, Virginia, has a mission to build a leadership development program that increases principals' instructional knowledge and develops mentor principals to sustain the program. The academy is designed to connect and empower principals…
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Bulletin of Materials Science | Indian Academy of Sciences
Indian Academy of Sciences (India)
All correspondence regarding subscription within India should be addressed to: The Circulation Department Indian Academy of Sciences C V Raman Avenue P.B. No. 8005. Bengaluru 560 080, India. Download the Order form (2018): Institutions and Individuals. DD should be arranged in favour of "Indian Academy of ...
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... Certification Meetings & Events Employee Resources Research Academia Practice Management Reimbursement Coding Compliance Resources and Tools Publications & News News Audiology Today Journal of the American Academy of Audiology Books Brochures Multimedia Guidelines and Standards ...
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resources.html | epubworkshop | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Other | Resources | public | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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salary.pdf | office | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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National Academy of Sciences - National Research Council, Washington, DC. Inst. of Lab. Animal Resources.
This volume contains the prepared papers and discussions of a National Academy of Sciences - National Research Council Symposium on the Future of Animals, Cells, Models, and Systems in Research, Development, Education, and Testing. The purpose of the symposium was to examine the past, present, and future contributions of animals to human health…
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KECK OBSERVATIONS OF THE GALACTIC CENTER SOURCE G2: GAS CLOUD OR STAR?
Energy Technology Data Exchange (ETDEWEB)
Phifer, K.; Meyer, L.; Ghez, A. M.; Witzel, G.; Yelda, S.; Boehle, A.; Morris, M. R.; Becklin, E. E. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Do, T. [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H4 (Canada); Lu, J. R. [Institute for Astronomy, University of Hawaii, Hilo, HI 96720 (United States); Matthews, K., E-mail: ghez@astro.ucla.edu [Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States)
2013-08-10
We present new observations and analysis of G2-the intriguing red emission-line object which is quickly approaching the Galaxy's central black hole. The observations were obtained with the laser guide star adaptive optics systems on the W. M. Keck I and II telescopes (2006-2012) and include spectroscopy (R {approx} 3600) centered on the hydrogen Br{gamma} line as well as K' (2.1 {mu}m) and L' (3.8 {mu}m) imaging. Analysis of these observations shows the Br{gamma} line emission has a positional offset from the L' continuum. This offset is likely due to background source confusion at L'. We therefore present the first orbital solution derived from Br{gamma} line astrometry, which, when coupled with radial velocity measurements, results in a later time of closest approach (2014.21 {+-} 0.14), closer periastron (130 AU, 1600 R{sub s}), and higher eccentricity (0.9814 {+-} 0.0060) compared to a solution using L' astrometry. It is shown that G2 has no K' counterpart down to K' {approx} 20 mag. G2's L' continuum and the Br{gamma} line emission appears unresolved in almost all epochs, which implies that the bulk of the emission resides in a compact region. The observations altogether suggest that while G2 has a gaseous component that is tidally interacting with the central black hole, there is likely a central star providing the self-gravity necessary to sustain the compact nature of this object.
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... Examine Oral Systemic Health Nov 14, 2017 General Dentistry and American Family Physician Collaborate to Examine Oral ... Oral Health Oct 23, 2017 Academy of General Dentistry Foundation Celebrates 45 Years Raising Awareness for Oral ...
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Living Spaces for Talk with/in the Academy
Directory of Open Access Journals (Sweden)
Donna Patterson
2004-09-01
Full Text Available Exploring to find the question is always already exploring to find the method. What's (really happening when we talk in academic spaces? What talk(s belong in the Academy? Where does the ‘talk’ happen and how is it (invisible? Based on ‘talk’ of reflective practice shared between two colleagues, this article examines issues of ethics, methodology and usefulness as they pertain to the terra (incognito of idea talk with/in the Academy. Through a dialogue about methods and method in which we emphasize permission to dwell, we hope to further inquiry into the role of talk with/in the Academy.
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... Award Recipients Nov 07, 2017 View all news Optometry and Vision Science Journal Optometry and Vision Science is the official journal of the American Academy of Optometry. AAO members receive a complimentary online subscription. Learn ...
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International Nuclear Information System (INIS)
Yamashita, Yuji; Tanaka, Satoru
2012-01-01
We made a descriptive inference about the role of the U.S. National Academies in the U.S. radioactive waste disposal projects on the basis of literature-based information and compared the U.S. National Academies with the Science Council of Japan to determine their implications on the progress of social acceptability of radioactive waste disposal projects in Japan. The descriptive inference was made as follows. We described the organizational characteristics of the U.S. National Academies and the U.S. federal governments related to the projects. We outlined the related bills and demonstrated chronologically the activities related to the projects by the U.S. National Academies and the U.S. Government. As a consequence, we identified some specific roles that the U.S. National Academies played in the U.S. radioactive waste disposal projects. The U.S. National Academies have acted not only as a scientific and engineering adviser for the governments but also as an anchor for some political decision making or judicial actions. Furthermore, we analyzed the credibility of the Science Council of Japan and the U.S. National Academies from the viewpoint that a reliable third party must exhibit fairness, expertise and continuity. From the results of the comparison, it was found that the Science Council of Japan has the possibility to become a reliable third party that can help the radioactive waste disposal projects in Japan. (author)
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CosmoAcademy Training and Certification for Scientists and Engineers
Noel-Storr, Jacob; Buxner, Sanlyn; Grier, Jennifer A.; Gay, Pamela L.; CosmoQuest Team
2016-10-01
CosmoQuest is a virtual research facility bringing together scientists, citizens, and learners of all ages. CosmoQuest offers classes, training, and learning opportunities online through CosmoAcademy, offering opportunities for all kinds of learners to become more connected to the science of the Universe. In this poster we describe CosmoAcademy opportunities for Subject Matter Experts (SMEs), scientists and engineers who are interested in broadening their impact of their work by providing learning opportunities for those outside of the scientific community. CosmoAcademy offers SME programs at a variety of levels and across a variety of topics in formal and informal education and outreach -- ranging from sharing the results of your work on social media, through delivering an online class series, to partnering with teachers and schools. SMEs may combine sequences of training to earn certification at various levels for their participation in the CosmoAcademy programs. SMEs who have been trained may also apply to teach CosmoAcademy classes for the community on subjects of their expertise to build a rich and engaging learning resource for members of society who wish to understand more about the Universe.
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The Future Nuclear Arms Control Agenda and Its Potential Implications for the Air Force
2015-08-01
US AIR FORCE INSTITUTE FOR NATIONAL SECURITY STUDIES USAF ACADEMY, COLORADO INSS OCCASIONAL PAPER AUGUST 2015 70 Dr. Lewis A. Dunn The Future...Implications for the Air Force Dr. Lewis A. Dunn INSS Occasional Paper 70 August 2015 USAF Institute for National Security Studies USAF
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Indian Academy of Sciences (India)
Brahma
The Academy reserves the right to reject/not to accept any quotation without assigning any reason thereof. ❖ Those interested may ... The sealed covers must be superscribed "TENDER FOR HOUSEKEEPING –. 2016-17" and submitted to:.
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DOD Service Academies. Update on Extent of Sexual Harassment. Report to Congressional Requesters.
General Accounting Office, Washington, DC. National Security and International Affairs Div.
This report provides an update on the nature and extent of sexual harassment at the three Department of Defense (DOD) service academies. It is based on a stratified random survey of 430 Military Academy cadets, 470 Naval Academy midshipmen, and 428 Air Force Academy cadets, which oversampled women to ensure that a statistically significant number…
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Journal of Earth System Science | Indian Academy of Sciences
Indian Academy of Sciences (India)
... Chinese Academy of Sciences (CAS), Lanzhou 730000, China. University of Chinese Academy of Sciences, Beijing 100049, China. Geography and Environment College of Northwest Normal University, Lanzhou 730070, China. School of Urban Economics and Tourism Culture, Lanzhou City University, Lanzhou 730070, ...
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Memorandum of Association | About IASc | Indian Academy of ...
Indian Academy of Sciences (India)
Memorandum of Association. Registered on 27 April 1934 under the Societies Registration Act, 1860. I. The name of the Association shall be `The Indian Academy of Sciences'. II. The objects of the Academy are: To promote the progress and uphold the cause of science, both in pure and applied branches. To co-operate ...
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EDUCAUSE, 2015
2015-01-01
The four guiding principles behind the blended, competency-based, personalized learning model of Valor Collegiate Academies, a charter organization serving grades 5-12 in Nashville, TN: (1) Reflect the diversity of both our country and local community; (2) Personalize a student's experience to meet his/her unique academic and non-academic needs;…
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National Academy of Sciences survey on risks associated with nuclear power
International Nuclear Information System (INIS)
Buchanan, J.R.
1980-01-01
A critical review of the literature pertaining to the risks associated with nuclear electric power was sponsored by the Committee on Science and Public Policy of the National Academy of Sciences. Although the full report (consisting of over 25 chapters) has not yet been published, this paper presents highlights from the Summary and Synthesis Chapter, which was released separately. Of the risks whose magnitudes can be estimated with reasonable accuracy, the most serious is the exposure of future generations to 14 C from reactors and reprocessing plants. Prospects are good for reducing this risk considerably, since carbon can be collected and stored as waste
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303.pdf | mar2015 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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1413.pdf | aug2014 | jessci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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783.pdf | jun2015 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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807.pdf | jun2015 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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959.pdf | jul2014 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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791.pdf | jun2014 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Journal of Astrophysics and Astronomy | Indian Academy of Sciences
Indian Academy of Sciences (India)
2016-01-27
Jan 27, 2016 ... Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi 830011, China. Department of Physics and GXU-NAOC, Centre for Astrophysics and Space Sciences, Guangxi University, Nanning 530004, China. University of Chinese Academy of Sciences, Beijing 100049 ...
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1197.pdf | aug2014 | jessci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Visc | chemistry | resources | sci ed | initiat | Indian Academy of ...
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Resonance – Journal of Science Education | Indian Academy of ...
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences. Indian Academy of ... Volume 17; Issue 8. UNIX: Genesis and Design Features ... Keywords. Operating system design; UNIX shell; UNIX kernel; file systems; process management; interprocess communication; versioning; documentation and high level language C; tools and utilities.
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75 FR 2153 - National Fire Academy Board of Visitors
2010-01-14
...] National Fire Academy Board of Visitors AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Teleconference Federal Advisory Committee Meeting. SUMMARY: The National Fire Academy Board of Visitors will meet by teleconference on February 2, 2010. DATES: The teleconference will...
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75 FR 44276 - National Fire Academy Board of Visitors
2010-07-28
...] National Fire Academy Board of Visitors AGENCY: Federal Emergency Management Agency, DHS. ACTION: Notice of cancellation of meeting. SUMMARY: The National Fire Academy Board of Visitors public teleconference [email protected] . SUPPLEMENTARY INFORMATION: The Federal Emergency Management Agency (FEMA) published a Notice...
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Raman Chair | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Raman Chair. The Raman Chair was instituted in 1972 by the Government of India to commemorate the memory of the founder of the Academy, Sir C. V. Raman. Eminent scientists are invited by the Council of the Academy to occupy the Chair, for periods of between six weeks and six months. Raman Professors who have ...
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Contact details | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
Contact. Change in email domain name. The domain part of the email address of all email addresses used by the office of Indian Academy of Sciences, including those of the staff, the journals, various programmes, and Current Science, has changed from 'ias.ernet.in' (or 'academy.ias.ernet.in') to 'ias.ac.in'. Thus, for ...
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Raman Chair | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
The Raman Chair was instituted in 1972 by the Government of India to commemorate the memory of the founder of the Academy, Sir C. V. Raman. Eminent scientists are invited by the Council of the Academy to occupy the Chair, for periods of between six weeks and six months. Raman Professors who have occupied the ...
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Towards A Regional Science Academy: A Manifesto
Directory of Open Access Journals (Sweden)
Karima Kourtit
2016-04-01
Full Text Available This Manifesto provides a joint proposal to create a Regional Science Academy as a think-tank support platform for a strategic development of the spatial sciences. The Regional Science Academy is a strategic spatial knowledge catalyst: it acts as a global intellectual powerhouse for new knowledge network initiatives and scholarly views on regions and cities as vital centrepieces of interconnected spatial systems. This contribution highlights its role and presents various activity plans.
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Introduction to NASA's Academy of Aerospace Quality
Smith, Alice; Smith, Jeffrey
2016-01-01
The NASA Academy of Aerospace Quality (AAQ) is an internet-based public domain forum of quality assurance-related educational modules for students and faculty at academic institutions targeting those involved in aerospace research, technology development, and payload design and development including Cube Sats, Small Sats, Nano Sats, Rockets and High Altitude Balloons. The target users are university project and research teams but the academy has also been used by K-12 teams, independent space...
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The G4R GMES Academy - linking research, academia, service providers and local authorities.
Zeil, Peter; Tramutoli, Valerio
2013-04-01
The GMES Academy intends to enhance the role of the academic and R&D communities in the evolution of EO & GI services. The GMES4Regions G4R initiative, aiming to strengthen the link between GMES (Global Monitoring for Environment and Security) and European regions, inaugurated the GMES Academy at the University Mozarteum of Salzburg (Austria) on 13th - 14th September 2012. This academy has been created with the objective of fostering a dialogue among the private sector, Local and Regional Administration (LRA) and the academic and research community, in order to improve the development of Earth Observation (EO) and Geographic Information (GI) services. On this occasion, Z_GIS, the Interfaculty Department of Geoinformatics of Salzburg University, hosted the round table "Fostering Downstream Services for the Regions - contributions from Research & Academia," during which the participants had the opportunity to discuss with representatives of the European Commission (EC) and the European Space Agency (ESA) the future role of the academic community in this domain. Stakeholders from the academic and R&D world adopted the 'Salzburg Declaration on GMES related Research', calling for strengthening connections between research activities and educational programmes to improve GMES services. The Declaration calls mainly for: • fostering education and training on GMES • ensuring cooperation among the academic and research community through the GMES Academy • maintaining a political commitment towards the implementation of such academic initiatives. The GMES Academy is established as a platform with six components: GATEWAY - the directory of Universities and Research Centres BRIDGE - an inventory of research briefs documenting the latest offerings from research to effective applications FACILITATOR - a portal to seek or propose internships or contract research across Europe and addressing outreach and advocacy: LINK - Access to the repository of on-going GMES related
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Guhathakurta, Puragra; Toloba, Elisa; Peng, Eric W.; Li, Biao; Gwyn, Stephen; Ferrarese, Laura; Cote, Patrick; Chu, Jason; Sparkman, Lea; Chen, Stephanie; Yagati, Samyukta; Muller, Meredith; Next Generation Virgo Survey Collaboration
2015-01-01
We present results from an ongoing study of globular cluster (GC) satellites of low-luminosity dwarf elliptical (dE) galaxies in the Virgo cluster. Our 21 dE targets and candidate GC satellites around them in the apparent magnitude range g ~ 20-24 were selected from the Next Generation Virgo Survey (NGVS) and followed up with medium-resolution Keck/DEIMOS spectroscopy (resolving power: R ~ 2000; wavelength coverage: 4800-9500 Angstrom). In addition, the remaining space available on the nine DEIMOS multi-slit masks were populated with "filler" targets in the form of distant Milky Way halo star candidates in a comparable apparent magnitude range. A combination of radial velocity information (measured from the Keck/DEIMOS spectra), color-color information (from four-band NGVS photometry), and sky position information was used to sort the sample into the following categories: (1) GC satellites of dEs, (2) other non-satellite GCs in the Virgo cluster (we dub them "orphan" GCs), (3) foreground Milky Way stars that are members of the Sagittarius stream, the Virgo overdensity, or the field halo population, and (4) distant background galaxies. We stack the GC satellite population across all 21 host dEs and carry out dynamical modeling of the stacked sample in order to constrain the average mass of dark matter halos that these dEs are embedded in. We study rotation in the system of GC satellites of dEs in the handful of more populated systems in our sample - i.e., those that contain 10 or more GC satellites per dE. A companion AAS poster presented at this meeting (Chu, J. et al. 2015) presents chemical composition and age constraints for these GC satellites relative to the nuclei of the host dEs based on absorption line strengths in co-added spectra. The orphan GCs are likely to be intergalactic GCs within the Virgo cluster (or, equivalently, GCs in the remote outer envelope of the cluster's central galaxy, the giant elliptical M87).This project is funded in part by the
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Resonance – Journal of Science Education | Indian Academy of ...
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences. Indian Academy of Sciences ... Home; Journals; Resonance – Journal of Science Education; Volume 1; Issue 1. Factoring Fermat Numbers. C E Veni ... C E Veni Madhavan1. Department of Computer Science and Automation, Indian Institute of Science, Bangalore 560 012.
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Hartmann, Karin; Escribano, Luis; Grattan, Clive; Brockow, Knut; Carter, Melody C; Alvarez-Twose, Ivan; Matito, Almudena; Broesby-Olsen, Sigurd; Siebenhaar, Frank; Lange, Magdalena; Niedoszytko, Marek; Castells, Mariana; Oude Elberink, Joanna N G; Bonadonna, Patrizia; Zanotti, Roberta; Hornick, Jason L; Torrelo, Antonio; Grabbe, Jürgen; Rabenhorst, Anja; Nedoszytko, Boguslaw; Butterfield, Joseph H; Gotlib, Jason; Reiter, Andreas; Radia, Deepti; Hermine, Olivier; Sotlar, Karl; George, Tracy I; Kristensen, Thomas K; Kluin-Nelemans, Hanneke C; Yavuz, Selim; Hägglund, Hans; Sperr, Wolfgang R; Schwartz, Lawrence B; Triggiani, Massimo; Maurer, Marcus; Nilsson, Gunnar; Horny, Hans-Peter; Arock, Michel; Orfao, Alberto; Metcalfe, Dean D; Akin, Cem; Valent, Peter
2016-01-01
Cutaneous lesions in patients with mastocytosis are highly heterogeneous and encompass localized and disseminated forms. Although a classification and criteria for cutaneous mastocytosis (CM) have been proposed, there remains a need to better define subforms of cutaneous manifestations in patients with mastocytosis. To address this unmet need, an international task force involving experts from different organizations (including the European Competence Network on Mastocytosis; the American Academy of Allergy, Asthma & Immunology; and the European Academy of Allergology and Clinical Immunology) met several times between 2010 and 2014 to discuss the classification and criteria for diagnosis of cutaneous manifestations in patients with mastocytosis. This article provides the major outcomes of these meetings and a proposal for a revised definition and criteria. In particular, we recommend that the typical maculopapular cutaneous lesions (urticaria pigmentosa) should be subdivided into 2 variants, namely a monomorphic variant with small maculopapular lesions, which is typically seen in adult patients, and a polymorphic variant with larger lesions of variable size and shape, which is typically seen in pediatric patients. Clinical observations suggest that the monomorphic variant, if it develops in children, often persists into adulthood, whereas the polymorphic variant may resolve around puberty. This delineation might have important prognostic implications, and its implementation in diagnostic algorithms and future mastocytosis classifications is recommended. Refinements are also suggested for the diagnostic criteria of CM, removal of telangiectasia macularis eruptiva perstans from the current classification of CM, and removal of the adjunct solitary from the term solitary mastocytoma. Copyright © 2015 American Academy of Allergy, Asthma & Immunology. Published by Elsevier Inc. All rights reserved.
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Maximilien Brice
2011-01-01
4th February 2011 - Austrian Academy of Sciences President H. Denk visiting CMS underground area with Collaboration Spokesperson G. Tonelli, Austrian Academy of Sciences Secretary General A. Suppan, CERN Head of International Relations F. Pauss and Director, High Energy Physics Laboratory, Austrian Academy of Sciences C Fabjan.
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Resonance – Journal of Science Education | Indian Academy of ...
Indian Academy of Sciences (India)
... Jubilee Chair · Academy – Springer Nature chair · Academy Trust · Contact details · Office Staff · Office complaint ... Know Your Personal Computer Introduction to Computers .... Algorithms Data Types and their Representation in Memory ... The Immune System and Bodily Defence Why Do We Need an Immune System?
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contents.htm | may102003 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page. New Fellows and Honorary Fellows. Posted on 4 January 2017. List of Fellows and Honorary ...
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Journal of Astrophysics and Astronomy | Indian Academy of Sciences
Indian Academy of Sciences (India)
Download the Order Form (2018): Institution and Personal. All correspondence regarding subscription within India should be addressed to the Circulation Department of the Academy (orders@ias.ac.in). DD should be prepared in favour of "Indian Academy of Sciences" payable at Bengaluru. Payment can also be made ...
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1518.pdf | dec102003 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page. New Fellows and Honorary Fellows. Posted on 4 January 2017. List of Fellows and Honorary ...
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Self-Efficacy and social support of Academy cricketers | Cowan ...
African Journals Online (AJOL)
South African Journal for Research in Sport, Physical Education and Recreation ... This article aims to provide an initial insight into the role that South African provincial cricket academies play in talent development of cricketers by reflecting on possible changes in academy cricketers' self-efficacy and perceived social ...
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Academy Distance Learning Tools (IRIS) -
Department of Transportation — IRIS is a suite of front-end web applications utilizing a centralized back-end Oracle database. The system fully supports the FAA Academy's Distance Learning Program...
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Academie prix - Les Grands Prix de l'Academie des sciences 2002
2002-01-01
"Le physicien americain Richard Garwin a recu mardi, a Paris, la Grande Medaille de l'Academie des sciences, pour son "inventivite remarquable", aux cotes des laureats des soixante-seize Prix allant de 230 a 76.250 euros, pour un montant global de plus de 827.000 euros, decernes cette annee par la societe savante" (1/2 page).
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jgen- | jgen | General | Resources | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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ComputerScience.html | pubs | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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furnishing.doc | tendernotices | office | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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index body.html | epsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Systemic Mentoring for Competitiveness: The Model of the Timbuktu Academy
Bagayoko, Diola
2010-02-01
The Timbuktu Academy is a comprehensive, systemic mentoring program at Southern University and A&M College in Baton Rouge (SUBR), Louisiana. We define systemic mentoring as one that is woven into the core functions of an organization. For most universities, those functions include instruction, research, and service. While the Academy has programs for pre-college and graduate students, its Ten-Strand Systemic Mentoring Model was specifically tailored to undergraduate education. We discuss basic considerations that led to the paradigm, programs, activities, and results of the Timbuktu Academy. The proper implementation of the Ten-Strand Systemic Mentoring Model couples teaching and superior learning, on the one hand, and integrates research and education, on the other hand. For undergraduate education, key strands include support (financially or otherwise), scientific advisement, research participation (academic year or summer), immersion in a professional culture, monitoring, and guidance to graduate school. From the summer of 1994 to 2009, the Academy has engaged 2,093 pre-college scholars in its summer programs. To date, the Academy has assisted in the production of one hundred seventy (170) minority undergraduate scholars who have earned a Bachelor of Science degree. Seventy (70) of 83 physics graduates, twenty (20) of 29 chemistry graduates, and twenty-two (22) of 49 engineering graduates have earned graduate degrees or are successfully enrolled in graduate school, with emphasis on the pursuit of the Ph.D. For the above model and results, the Timbuktu Academy received the 2002 U.S. Presidential Award for Excellence in Science, Mathematics, and Engineering Mentoring. Its director was among the first individual recipients of this award in 1996. The handouts accompanying this presentation are intended to facilitate the adaptive replication of the Timbuktu Academy by individuals, departments, colleges and universities, and other organizations. )
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Sustainable Materials Management Web Academy
The Sustainable Materials Management (SMM) Web Academy series is a free resource for SMM challenge participants, stakeholders, and anyone else interested in learning more about SMM principles from experts in the field.
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Specialization: Medical Biostatistics, Medical Research Methodology, Medical ... Address: Centre for Advanced Research & Development, SBM Jain College of ... Joint Statement by the Three Science Academies of India on the teaching of the ...
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Dual Enrollment Academy Programs
Gonzalez, Nicolas; Chavez, Guadalupe
2009-01-01
Dual Enrollment Engineering (DEEA) and Medical Science (DEMSA) Academies are two-year dual enrollment programs for high school students. Students explore engineering and medical careers through college coursework. Students prepare for higher education in engineering and medical fields while completing associate degrees in biology or engineering…
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E1419.pdf | dec2000 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Amir.pdf | supp | jul2015 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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pg319.pdf | Pdf2010Jun | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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contjun2000.html | jun2000 | jessci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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patrika 54.pdf | Patrika | publ...ns | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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JB 480.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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articles30.htm | may25 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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JB 660.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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Journal of Astrophysics and A | Journals | Indian Academy of Sciences
Indian Academy of Sciences (India)
Ethical Guidelines and Procedures document. Posted on 17 January 2017. A revised version of the document 'Scientific Values: Ethical Guidelines and Procedures' has been produced by the Academy's Panel on Scientific Values. For more details, see the Academy Committee on Scientific Values page.
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150 years of the New York Academy of Medicine: a series of exhibitions.
Black, L F; North, M J
1996-01-01
As the New York Academy of Medicine celebrates its 150th year as a leader in the field of urban health, it is instructive to review the events and decisions that influenced and shaped it. Since its inception, the Academy has taken an active role in lobbying state and local governments to enact more-effective public health laws and in educating the public about improving health conditions. During 1996 and 1997, the Academy Library's Historical Collections is mounting a series of six exhibitions that are intended to tell the story of public health in New York as influenced by the New York Academy of Medicine. The story will be told using printed books, pamphlets, posters, photographs, and manuscripts drawn from the Library's collections, as well as the Academy's archives. Each exhibition will highlight the Academy's accomplishments in the subject areas presented. In this article, we summarize all six of the exhibitions and offer an in-depth look at the first two exhibitions.
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de Wet, A. P.; Bleacher, J. E.; Garry, W. B.
2012-01-01
Water has clearly played an important part in the geological evolution of Mars. There are many features on Mars that were almost certainly formed by fluvial processes -- for example, the channels Kasei Valles and Ares Vallis in the Chryse Planitia area of Mars are almost certainly fluvial features. On the other hand, there are many channel features that are much more difficult to interpret -- and have been variously attributed to volcanic and fluvial processes. Clearly unraveling the details of the role of water on Mars is extremely important, especially in the context of the search of extinct or extant life. In this project we built on our recent work in determining the origin of one channel on the southwest rift apron of Ascraeus Mons. This project, funded by the Keck Geology Consortium and involving 4 undergraduate geology majors took advantage of the recently available datasets to map and analyze similar features on Ascraeus Mons and some other areas of Mars. A clearer understanding of how these particular channel features formed might lead to the development of better criteria to distinguish how other Martian channel features formed. Ultimately this might provide us with a better understanding of the role of volcanic and fluvial processes in the geological evolution of Mars.
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Marketingová komunikace společnosti Driving Academy
Pařízek, Tomáš
2015-01-01
Title: Marketing communications of Driving Academy Co. Goal: This thesis aims to present marketing communications of Driving Academy, Inc., summarize used communications tools and propose plan of marketing communications for 2016. Methods: For the collection of information was used qualitative research in the form of descriptive case study. The study consists of qualitative interviews, analysis of texts and documents. Results: The result of this work is plan of marketing communications for 20...
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Wei, Chiming; Lyubchenko, Yuri L; Ghandehari, Hamid; Hanes, Justin; Stebe, Kathleen J; Mao, Hai-Quan; Haynie, Donald T; Tomalia, Donald A; Foldvari, Marianna; Monteiro-Riviere, Nancy; Simeonova, Petia; Nie, Shuming; Mori, Hidezo; Gilbert, Susan P; Needham, David
2006-12-01
The Second Annual Meeting of the American Academy of Nanomedicine (AANM) was held at the National Academy of Science Building in Washington, DC, September 9-10, 2006. The program included two Nobel Prize Laureate Lectures, two Keynote Lectures, and 123 invited outstanding State-in-Art lectures presenting in 23 special concurrent symposia. In addition, there were 22 poster presentations in the meeting addressing different areas in nanomedicine research. All of the presenters at the meeting are outstanding investigators and researchers in the field. The Second Annual Meeting of the AANM was a great success. The meeting provides investigators from different world areas a forum and an opportunity for discussion. We believe that nanomedicine research will develop rapidly in the future. The AANM invites basic and clinical researchers from the world to join this exciting research.
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Indian Academy of Sciences (India)
Manjunath
2016-12-26
Dec 26, 2016 ... various parameters such as Impact Factors, Citation Indices, etc., provided by international agencies. Needless to mention, these Journals are priced ... available in the Academy website: www.ias.ac.in) and we would generally like to recommend all. Journals for your library. The prices are inclusive of ...
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Sadhana | Indian Academy of Sciences
Indian Academy of Sciences (India)
https://www.ias.ac.in/article/fulltext/sadh/038/01/0123-0131 ... play a key role in telemedicine applications that help in accurate diagnosis and research. ... Department of Electronics Engineering, Sinhgad Academy of Engineering, Pune 411048 ...
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fell all.php3 | php | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1089.pdf | jul2014 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
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630.pdf | sep102009 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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37.pdf | jan102006 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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867.pdf | aug2012 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1417.pdf | nov252004 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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contents.htm | nov102005 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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Other Women in Science Groups | Indian Academy of Sciences
Indian Academy of Sciences (India)
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897.pdf | apr102004 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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The Politics of the Academies Programme: Natality and Pluralism in Education Policy-Making
Gunter, Helen M.; McGinity, Ruth
2014-01-01
Our investigations into the politics of the Academies Programme in England have generated thinking that draws on data about the conversion process from two projects. We engage with an early City Academy that replaced two "failing" schools, and a recent Academy that replaced a "successful" high school. We deploy Hannah Arendt's…
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Health Policy, Ethics, and the Kansas Legislative Health Academy
Maree, Gina; Schrandt, Suzanne; Soderquist, Chris; Steffensmeier, Tim; St. Peter, Robert
2015-01-01
We describe a unique program, the Kansas Legislative Health Academy, that brings together state legislators from across the political spectrum to build their capacity in advancing policies that can improve the health of Kansans. To that end, the academy helps legislators develop new skills to deliberate the ethics of health policy, use systems thinking to understand the long- and short-term effects of policy action and inaction, and engage in acts of civic leadership. The academy also seeks to foster an environment of respectful open dialogue and to build new cross-chamber and cross-party relationships. Among the most important outcomes cited by program participants is the value of sustained, personal interaction and problem solving with individuals holding differing political views. PMID:25607945
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Health policy, ethics, and the Kansas Legislative Health Academy.
Blacksher, Erika; Maree, Gina; Schrandt, Suzanne; Soderquist, Chris; Steffensmeier, Tim; St Peter, Robert
2015-03-01
We describe a unique program, the Kansas Legislative Health Academy, that brings together state legislators from across the political spectrum to build their capacity in advancing policies that can improve the health of Kansans. To that end, the academy helps legislators develop new skills to deliberate the ethics of health policy, use systems thinking to understand the long- and short-term effects of policy action and inaction, and engage in acts of civic leadership. The academy also seeks to foster an environment of respectful open dialogue and to build new cross-chamber and cross-party relationships. Among the most important outcomes cited by program participants is the value of sustained, personal interaction and problem solving with individuals holding differing political views.
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Skevaki, Chrysanthi L; Maggina, Paraskevi; Santos, Alexandra F; Rodrigues-Alves, Rodrigo; Antolin-Amerigo, Dario; Borrego, Luis Miguel; Bretschneider, Isabell; Butiene, Indre; Couto, Mariana; Fassio, Filippo; Gardner, James; Xatzipsalti, Maria; Hovhannisyan, Lilit; Hox, Valerie; Makrinioti, Heidi; O Neil, Serena E; Pala, Gianni; Rudenko, Michael; Santucci, Annalisa; Seys, Sven; Sokolowska, Milena; Whitaker, Paul; Heffler, Enrico
2011-12-01
This year is the 10th anniversary of the European Academy of Allergy and Clinical Immunology (EAACI) Junior Members and Affiliates (JMAs). The aim of this review is to highlight the work and activities of EAACI JMAs. To this end, we have summarized all the initiatives taken by JMAs during the last 10 yr. EAACI JMAs are currently a group of over 2380 clinicians and scientists under the age of 35 yr, who support the continuous education of the Academy's younger members. For the past decade, JMAs enjoy a steadily increasing number of benefits such as free online access to the Academy's journals, the possibility to apply for Fellowships and the Mentorship Program, travel grants to attend scientific meetings, and many more. In addition, JMAs have been involved in task forces, cooperation schemes with other scientific bodies, organization of JMA focused sessions during EAACI meetings, and participation in the activities of EAACI communication platforms. EAACI JMA activities represent an ideal example of recruiting, training, and educating young scientists in order for them to thrive as future experts in their field. This model may serve as a prototype for other scientific communities, several of which have already adapted similar policies. © 2011 John Wiley & Sons A/S.
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DEFF Research Database (Denmark)
Nazaroff, William W.; Clausen, Geo; Wargocki, Pawel
2014-01-01
The 13th International Conference on Indoor Air Quality and Climate (Indoor Air 2014) was convened in Hong Kong during the week of 7–12 July 2014. Professor Yuguo Li served as the Conference President. One of many highlights was the presentation of awards from the ISIAQ Academy of Fellows, which...
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Man and technology in the future
International Nuclear Information System (INIS)
1993-01-01
The Royal Swedish Academy of Engineering Sciences has set up a committee known as The Committee of Man, Technology and Society. The members of this committee form an interdisciplinary group for the study of the interaction between scientific and technological advances and the way in which society evolves. Most of the committees activities have focused on the present relationship between man, technology and society. Attempts have been made to assess the future influence on society of key developments in biotechnology, electronic communication and systems analysis. In order to pursue this path still further, the committee decided to arrange an international symposium on the topic Man and Technology in the Future at the village of Forsmark on the Baltic coast of Sweden. The proceedings consists of 13 lectures centered on energy systems - and the connected waste problems, biotechnology, and telecommunications. Separate abstracts were prepared for 5 of the lectures in this volume
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About | Indian Academy of Sciences
Indian Academy of Sciences (India)
The 82nd Annual Meeting of the Indian Academy of Sciences is being held at ... by newly elected Fellows and Associates over a wide range of scientific topics. ... Indian Institute of Science Education and Research (IISER), Bhopal: Indian ...
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MODELS OF THE η CORVI DEBRIS DISK FROM THE KECK INTERFEROMETER, SPITZER, AND HERSCHEL
Energy Technology Data Exchange (ETDEWEB)
Lebreton, J.; Beichman, C.; Millan-Gabet, R. [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Bryden, G.; Mennesson, B. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91107 (United States); Defrère, D. [Department of Astronomy, University of Arizona, 993 N. Cherry Avenue, Tucson, AZ, 85721 (United States); Boccaletti, A., E-mail: lebretoj@gmail.com [LESIA, Observatoire de Paris, CNRS, University Pierre et Marie Curie Paris 6 and University Denis Diderot Paris 7, 5 place Jules Janssen, F-92195 Meudon (France)
2016-02-01
Debris disks are signposts of analogs to small-body populations of the solar system, often, however, with much higher masses and dust production rates. The disk associated with the nearby star η Crv is especially striking, as it shows strong mid- and far-infrared excesses despite an age of ∼1.4 Gyr. We undertake constructing a consistent model of the system that can explain a diverse collection of spatial and spectral data. We analyze Keck Interferometer Nuller measurements and revisit Spitzer and additional spectrophotometric data, as well as resolved Herschel images, to determine the dust spatial distribution in the inner exozodi and in the outer belt. We model in detail the two-component disk and the dust properties from the sub-AU scale to the outermost regions by fitting simultaneously all measurements against a large parameter space. The properties of the cold belt are consistent with a collisional cascade in a reservoir of ice-free planetesimals at 133 AU. It shows marginal evidence for asymmetries along the major axis. KIN enables us to establish that the warm dust consists of a ring that peaks between 0.2 and 0.8 AU. To reconcile this location with the ∼400 K dust temperature, very high albedo dust must be invoked, and a distribution of forsterite grains starting from micron sizes satisfies this criterion, while providing an excellent fit to the spectrum. We discuss additional constraints from the LBTI and near-infrared spectra, and we present predictions of what James Webb Space Telescope can unveil about this unusual object and whether it can detect unseen planets.
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report reco | 1-Overview | 5-Publications | Indian Academy of Sciences
Indian Academy of Sciences (India)
An important aspect is continuous teacher training and upgradation of ... a wide variety of options of a more vocational or practical nature are available; we are ... programmes in selected institutions, the Academy also urges the introduction of .... the Three Science Academies of India on the teaching of the theory of evolution
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Music Performance Anxiety among Students of the Academy in Lithuania
Paliaukiene, Vilma; Kazlauskas, Evaldas; Eimontas, Jonas; Skeryte-Kazlauskiene, Monika
2018-01-01
Music performance anxiety (MPA) affects amateurs, students and professional musicians. We aimed to analyse MPA among students of music performance in a higher education academy in Lithuania. A sample of 258 music performance arts students of the Lithuanian Music and Theatre Academy participated in this study. The Kenny Music Performance Anxiety…
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Journal of the Cameroon Academy of Sciences: About this journal
African Journals Online (AJOL)
Journal of the Cameroon Academy of Sciences: About this journal. Journal Home > Journal of the Cameroon Academy of Sciences: About this journal. Log in or Register to get access to full text downloads. Username, Password, Remember me, or Register · Journal Home · ABOUT THIS JOURNAL · Advanced Search ...
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
2016-09-22
Sep 22, 2016 ... From the discovery of the Higgs Boson, to how supersymmetry solves the ... Is the discovery of the 125 GeV resonance at the LHC suggestive of a new ... Soap Bubbles and Drones: National Science Day at the Academy!!!
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The Bulgarian Academy of Sciences.
1960-05-24
Academy of Sciences of Peru , and the international Committee on Ap- plied Mechanics.’ :■’.....;.;■ . Has given scientific reports at...of cholera in hogs (spontaneous and experimental), the pathomorphology and pathophysiology of infectious anemia in horses, the morphophysiology of
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Visc | chemistry | resources | sci ed | initiat | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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44.pdf | jul102004 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1383.pdf | may252007 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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fell detail.php3 | php | Indian Academy of Sciences
Indian Academy of Sciences (India)
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17mymprog.html | myrmeet | meetings | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1651.pdf | dec252008 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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contents.htm | jan102006 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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314.pdf | feb102006 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1524.pdf | nov102005 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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Marketing mix - project of a textbook for business academies
Zatloukalová, Zuzana
2010-01-01
The thesis deals with project of a textbook for business academies. The theme of the chapter of the textbook is marketing mix. The project is made in such a way the students get total information on these problems. The extant of the theme is intended for students of higher classes. The project consists of theoretical part (textbook, exercise book) and practical part (teaching at business academy).
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html xml pdf.ppt | presentations | epubworkshop | Indian Academy of ...
Indian Academy of Sciences (India)
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1015.pdf | oct252006 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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1253.pdf | may102003 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
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Brightside Academy: Pittsburgh, Pennsylvania
Horn, Sarah
2009-01-01
Since its inception in 1992, Brightside Academy has been providing quality care to children six weeks to 12 years old. Operating 49 locations in Pennsylvania, Ohio, and New York, the company is committed to strengthening learners and respecting families. Currently, the organization provides early education for 6,700 children on a daily basis. 90%…
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An American Academy for Training Safeguards Inspectors - An Idea Revisited
International Nuclear Information System (INIS)
Durst, Philip Casey; Bean, Robert
2010-01-01
In 2009, we presented the idea of an American academy for training safeguards inspectors for the International Atomic Energy Agency (IAEA), due to the declining percentage of Americans in that international organization. In this paper we assert that there is still a compelling need for this academy. While the American Safeguards Academy would be useful in preparing and pre-training American inspectors for the IAEA, it would also be useful for preparing Americans for domestic safeguards duties in the U.S. Department of Energy (DOE), U.S. DOE National Laboratories, and the U.S. Nuclear Regulatory Commission (NRC). It is envisioned that such an academy would train graduate and post-graduate university students, DOE National Laboratory interns, and nuclear safeguards professionals in the modern equipment, safeguards measures, and approaches currently used by the IAEA. It is also envisioned that the Academy would involve the domestic nuclear industry, which could provide use of commercial nuclear facilities for tours and demonstrations of the safeguards tools and methods in actual nuclear facilities. This would be in support of the U.S. DOE National Nuclear Security Administration's Next Generation Safeguards Initiative (NGSI). This training would also help American nuclear safeguards and non-proliferation professionals better understand the potential limitations of the current tools used by the IAEA and give them a foundation from which to consider even more effective and efficient safeguards measures and approaches.
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2010-08-25
... preparation for, teaching these subjects. The Congressional Academies for Students of American History and... in historical methodology or the teaching of history. We published a notice of proposed waiver and... or the teaching of history. The Secretary certifies that the waiver and extension of project period...
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Do AAO-HNSF CORE Grants Predict Future NIH Funding Success?
Eloy, Jean Anderson; Svider, Peter F; Kanumuri, Vivek V; Folbe, Adam J; Setzen, Michael; Baredes, Soly
2014-08-01
To determine (1) whether academic otolaryngologists who have received an American Academy of Otolaryngology- Head and Neck Surgery Foundation (AAO-HNSF) Centralized Otolaryngology Research Efforts (CORE) grant are more likely to procure future National Institutes of Health (NIH) funding; (2) whether CORE grants or NIH Career Development (K) awards have a stronger association with scholarly impact. Historical cohort. Scholarly impact, as measured by the h-index, publication experience, and prior grant history, were determined for CORE-funded and non-CORE-funded academic otolaryngologists. All individuals were assessed for NIH funding history. Of 192 academic otolaryngologists with a CORE funding history, 39.6% had active or prior NIH awards versus 15.1% of 1002 non-CORE-funded faculty (P productivity than those with CORE funding history. Both cohorts had higher scholarly impact values than previously published figures among academic otolaryngologists, highlighting that both CORE grants and NIH K-grants awards are effective career development resources. © American Academy of Otolaryngology—Head and Neck Surgery Foundation 2014.
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In Brief: Science academies' statement on climate change
Showstack, Randy
2009-06-01
“It is essential that world leaders agree on emissions reductions needed to combat negative consequences of anthropogenic climate change,” national science academies from 13 countries declared in a joint statement issued on 11 June. The statement, issued by the academies of the G8 countries—including England, France, Russia, and the United States—and five other countries (Brazil, China, India, Mexico, and South Africa), came in advance of a G8 meeting in Italy in July and prior to United Nations Framework Convention on Climate Change (UNFCCC) negotiations in Denmark in December. “The G8+5 should lead the transition to an energy-efficient and low-carbon world economy, and foster innovation and research and development for both mitigation and adaptation technologies,” the statement noted. The academies urged governments to agree at the UNFCCC negotiations to adopt a long-term global goal and short-term emissions reduction targets so that by 2050 global emissions would be reduced by about 50% from 1990 levels.
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INDIAN ACADEMY OF SCIENCES BANGALORE
Indian Academy of Sciences (India)
... in larger structures. They combine small size and complex organizational ... The uniqueness of the physics, chemistry, structural response and dynamics of the ... They are emerging as key components in information technology devices with ..... country based on recommendations received from Fellows of the Academy.
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Academy Engages Incarcerated Youths
Zehr, Mary Ann
2010-01-01
It's not easy to keep young people on task for learning in a youth prison, but David Domenici, the principal of the Maya Angelou Academy, a charter-like school serving incarcerated juveniles, is trying to do it while at the same time creating a model program for improving educational services for young offenders. Located at the New Beginnings…
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The Role of the Company Officer at the United States Naval Academy
National Research Council Canada - National Science Library
Moxey, Tyrel
2001-01-01
... contributing or not contributing to the mission of the United States Naval Academy. The author conducted 30 questionnaires on the 30 Company Officers stationed at the Naval Academy during this period...
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77 FR 69648 - Board of Visitors for the National Fire Academy
2012-11-20
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Teleconference Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet via teleconference on Wednesday, December...
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Zeng Jing
2017-01-01
[Purpose/significance] The provincial academy of sciences is an important part of national-wide scientific academies and regional innovation system. Promoting the transformation of the intellectual property is an important work for provincial academy of sciences. Nobody has ever revealed the status of the intellectual property resources and its management strategy of the provincial academy of sciences. [Method/process] With the methods of bibliometrics and investigations, this paper revealed ...
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The Northern Manitoba Mining Academy
Alexandre, Paul
2017-04-01
The Northern Manitoba Mining Academy (NMMA, miningacademy.ca) is a new educational institution located in Flin Flon, Manitoba. It is associated with the University College of the North and is specifically intended to serve the needs of the Northern Manitoban communities with regards to job creation by providing training in a variety of mining, construction, and exploration related areas. NMMA's mission is to provide innovative and responsible solutions for the creation of a knowledgeable, skilled, and sustainable workforce within a vibrant, mineral-rich resource industry. It facilitates strategic training initiatives and research activities in order to strengthen the social, economic, and environmental benefits of a robust mining and resources sector. In terms of education, NMMA offers its own programs, mostly short courses in health and safety, courses organized by the University College of the North (wilderness safety, prospecting, and exploration), and courses organized in association with provincial Industries-Based Safety Programs and Associations (a variety of construction-related trades). However, the programming is not limited to those courses already on the syllabus: the Academy operates on open-doors policy and welcomes people with their unique and diverse needs; it prides itself in its ability to tailor or create specific on-demand courses and deliver them locally in the North. The Northern Manitoba Mining Academy also provides access to its world-class facilities for field-based undergraduate courses, as well as graduate students and researchers doing field work. Full sample preparation facilities are offered to students and scientists in all natural and environmental sciences.
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International Nuclear Information System (INIS)
Sozzetti, Alessandro; Torres, Guillermo; Latham, David W.; Stefanik, Robert P.; Korzennik, Sylvain G.; Boss, Alan P.; Carney, Bruce W.; Laird, John B.
2009-01-01
We present an analysis of three years of precision radial velocity (RV) measurements of 160 metal-poor stars observed with HIRES on the Keck 1 telescope. We report on variability and long-term velocity trends for each star in our sample. We identify several long-term, low-amplitude RV variables worthy of followup with direct imaging techniques. We place lower limits on the detectable companion mass as a function of orbital period. Our survey would have detected, with a 99.5% confidence level, over 95% of all companions on low-eccentricity orbits with velocity semiamplitude K ∼> 100 m s -1 , or M p sin i ∼> 3.0 M J (P/yr) (1/3) , for orbital periods P ∼ p p ≅ 1%. Our results can usefully inform theoretical studies of the process of giant-planet formation across two orders of magnitude in metallicity.
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From Living Space to Cultural Space: How a Modern University Academy System Is Possible
Zhang, Yingqiang; Fang, Hualiang
2018-01-01
The reforms on the modern university academy system that preserve certain elements of China's ancient traditional academies have currently encountered a series of difficulties. The crux of the problem is that living and educational spaces were integrated in the traditional academy, while modern school education institution has separated the two.…
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International Nuclear Information System (INIS)
Melbourne, J.; Matthews, K.; Soifer, B. T.
2009-01-01
A simple optical to mid-IR color selection, R - [24]>14, i.e., f ν (24 μm)/f ν (R) ∼> 1000, identifies highly dust obscured galaxies (DOGs) with typical redshifts of z ∼ 2 ± 0.5. Extreme mid-IR luminosities (L IR > 10 12-14 ) suggest that DOGs are powered by a combination of active galactic nuclei (AGNs) and star formation, possibly driven by mergers. In an effort to compare their photometric properties with their rest-frame optical morphologies, we obtained high-spatial resolution (0.''05-0.''1) Keck Adaptive Optics K'-band images of 15 DOGs. The images reveal a wide range of morphologies, including small exponential disks (eight of 15), small ellipticals (four of 15), and unresolved sources (two of 15). One particularly diffuse source could not be classified because of low signal-to-noise ratio. We find a statistically significant correlation between galaxy concentration and mid-IR luminosity, with the most luminous DOGs exhibiting higher concentration and smaller physical size. DOGs with high concentration also tend to have spectral energy distributions (SEDs) suggestive of AGN activity. Thus, central AGN light may be biasing the morphologies of the more luminous DOGs to higher concentration. Conversely, more diffuse DOGs tend to show an SED shape suggestive of star formation. Two of 15 in the sample show multiple resolved components with separations of ∼1 kpc, circumstantial evidence for ongoing mergers.
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0227-.pdf | 03 | 084 | jgen | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution
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tutorial2.pdf | apr102000 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution
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0117-0126 | 01 | 084 | pram | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution
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0084-0088;.pdf | 01 | 006 | reso | Volumes | public | Indian Academy ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution
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78 FR 72094 - Board of Visitors for the National Fire Academy
2013-12-02
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for... Academy (NFA) and advise the Administrator of the Federal Emergency Management Agency (FEMA), through the...
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78 FR 59045 - Board of Visitors for the National Fire Academy
2013-09-25
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for... National Fire Academy (NFA) and advise the Administrator of the Federal Emergency Management Agency (FEMA...
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77 FR 5818 - Board of Visitors for the National Fire Academy
2012-02-06
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee management; notice of open federal advisory committee teleconference meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet by teleconference on February 21, 2012...
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77 FR 41196 - Board of Visitors for the National Fire Academy
2012-07-12
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Teleconference Meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet by teleconference on July 26, 2012. The...
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76 FR 36933 - Board of Visitors for the National Fire Academy
2011-06-23
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Teleconference Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet by teleconference on July 12, 2011. The...
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The art of creating a school: The Illinois Mathematics and Science Academy, 1979-1986
Coates, Judith Mary
The Illinois Mathematics and Science Academy is a three-year, public, residential learning environment for high school aged, gifted students. Established in 1986, it was one of only four such high schools in the United States. It continues to be successful and is often cited for its exemplary educational practices. The Academy is located in Aurora, Illinois and attracts gifted students from across the state. This study analyzes the Illinois Mathematics and Science Academy's stages of development over a seven year period prior to its opening in September of 1986. Through documentary research, this dissertation analyzes the methods, procedures, and marketing strategies utilized by the individuals and organizations who successfully managed the development of the Academy. Some of these methods and strategies include: defining a purpose, rallying community support, acquiring legislative approval, recruiting faculty and students, identifying a site, etc. The research identifies political, social, ideological, technological, utilitarian, environmental and educational needs unmet at the time by existing high schools, and illustrates how the Academy positioned itself to address those unmet needs. The information provides historical facts about the Academy and reveals some common and unique methodologies used to research, organize, manage, and implement the developmental process used to establish the school. The seven year period of development documented in the research begins at the definitive moment that the idea for establishing the new Academy occurred, and concludes with the first day the Academy opened its doors to its first class of students. The study uses a considerable volume of direct quotations from the individuals involved in the Academy's establishment to authenticate the historical facts. Quotations are cited from students, teachers, community members, board members, legislators, business owners, scientists, etc. Using the Academy's process of development as
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Female health and physical fitness at the Naval Academy
Stamper, Trevis L.
1998-01-01
Approved for public release; distribution is unlimited Stress related health disorders may he an indication that some female midshipmen at the Naval Academy are making exceptional efforts to meet specified physical performance standards. The stress at the service academies is much higher than in many civilian occupations and may increase the risk of females developing gender related health problems such as amenorrhea, bone loss, and eating disorders. The purpose of this research is to shed...
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Directory of Open Access Journals (Sweden)
Güven Bakırezer
2018-01-01
Full Text Available After declaring a state of emergency on 20 July, 2016 as a response to the failed coup attempt of 15 July, 2016, the Turkish government launched a nation-wide academic purge, especially targeting the Academics for Peace. This group of academics signed a peace petition in January 2016 to address civilian deaths in the South-Eastern part of the country and to urge the government to take responsibility and restart the peace process. Having the largest number of peace petitioners among Turkey’s provincial universities, Kocaeli University was the first to dismiss all 19 of the peace academics from their positions on 1 September, 2016. Already active in defending the universal values of academia in other venues, these dismissed peace academics founded the Kocaeli Academy of Solidarity in pursuit of an alternative academy that aims to bring together university students, NGO members and ordinary citizens in the city in a cooperative understanding of education and research. After weekly seminars over eight months, a summer school of five days, and with applications in for funding its projects, particularly amongst others the School of Life, Kocaeli Academy for Solidarity has a strong determination to demonstrate a new democratic model of education and research.
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 22 January 1952. Specialization: Surface Chemical Physics Address during Associateship: Chemical Engineering Division, National Chemical Laboratory, Pune 411 008. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year ...
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; Fellowship. Fellow Profile. Elected: 1955 Section: Medicine. Iyengar, Nuggehalli Keshava D. Phil. Date of birth: 29 July 1910. Date of death: 29 November 1970. Specialization: Forensic Sciences. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018.
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 16 August 1968. Specialization: Molecular Biology Address during Associateship: Eukaryotic Gene Expression Lab., National Institute of Immunology, Aruna Asaf Ali Marg, New Delhi 110 016. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018.
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair ... Elected: 1999 Section: Mathematical Sciences. Misra ... Address: Department of Mathematics, Indian Institute of Science, Bengaluru 560 012, Karnataka ... Math Art and Design: MAD about Math, Math Education and Outreach.
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair ... Elected: 2006 Section: Animal Sciences ... Address: Professor, National Centre for Biological Sciences, GKVK Campus, Bengaluru 560 065, Karnataka ... Math Art and Design: MAD about Math, Math Education and Outreach.
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Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
History · Memorandum of Association · Role of the Academy · Statutes · Council · Raman Chair · Jubilee ... Elected: 1988 Section: Mathematical Sciences ... Address: Professor, Department of Mathematics and Computer Science, Emory University, 400 ... Math Art and Design: MAD about Math, Math Education and Outreach.
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The Effect of Using Cooking Academy Game towards Students’ Writing Ability
Directory of Open Access Journals (Sweden)
Nofrika Sari
2016-11-01
Full Text Available This study is an experimental research that discussed the impact of the use of cooking academy game in teaching writing on the students’ ability in writing procedure text at class VII Junior Secondary School I Pangkalan Baru Lima Puluh Kota. This study was aimed to determine the effects of the use of cooking academy game towards the student's ability in writing procedure text. In this study, the population is the students of class VII, while sample are two classes: one class for the experimental class and another class for control. Samples were drawn randomly. Data were collected by giving pre-test and post-test on the sample. Data were, then, analyzed applying t-test formula. The results showed that students who were taught to write text using the procedure of cooking academy game has the ability to write higher than students who are not taught by using games cooking academy.
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Four-year-BS-position-paper.pdf | misc docs | academy | Indian ...
Indian Academy of Sciences (India)
Home; academy; misc docs; Four-year-BS-position-paper.pdf. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of ...
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Rein and Zheng Elected to American Academy of Microbiology | Poster
By Nancy Parrish, Staff Writer Earlier this year, Alan Rein, Ph.D., and Zhi-Ming (Thomas) Zheng, M.D., Ph.D., were elected to fellowship in the American Academy of Microbiology, the honorific leadership group within the American Society for Microbiology (ASM). They were among 88 microbiologists who were elected to the academy “through a highly selective, peer-review process,
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articles32.htm | sep25 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci; sep25; articles32.htm. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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index body.html | sep2000 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; jess; sep2000; index body.html. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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index body.html | sep2002 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; jess; sep2002; index body.html. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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ilc-25.pdf | dec2005 | jess | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; jess; dec2005; ilc-25.pdf. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held ...
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577.pdf | 10sep2010 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci; 10sep2010; 577.pdf. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held ...
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articles16.htm | jul10 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; currsci; jul10; articles16.htm. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held ...
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HUBBLE AND KECK TELESCOPE OBSERVATIONS OF ACTIVE ASTEROID 288P/300163 (2006 VW139)
International Nuclear Information System (INIS)
Agarwal, Jessica; Jewitt, David; Weaver, Harold; Mutchler, Max; Larson, Stephen
2016-01-01
We present Hubble Space Telescope (HST) and Keck 10 m telescope observations of active asteroid 288P/300163 (2006 VW139) taken to examine ejected dust. The nucleus is a C-type object with absolute magnitude H V = 17.0 ± 0.1 and estimated diameter ∼2.6 km (for assumed visual geometric albedo p V = 0.04). Variations in the brightness of the nucleus at the 10%–15% level are significant in both 2011 December and 2012 October but we possess too few data to distinguish variations caused by activity from those caused by rotation. The dust scattering cross-section in 2011 December is ∼40 km 2 , corresponding to a dust mass ∼9 × 10 6 kg (88 μm mean particle radius assumed). The FWHM of the debris sheet varies from ∼100 km near the nucleus to ∼1000 km 30″ (40,000 km) east of it. Dust dynamical models indicate ejection speeds between 0.06 and 0.3 m s −1 , particle sizes between 10 and 300 μm and an inverse square-root relation between particle size and velocity. Overall, the data are most simply explained by prolonged, low velocity ejection of dust, starting in or before 2011 July and continuing until at least 2011 October. These properties are consistent with the sublimation of near-surface ice aided by centrifugal forces. The high spatial resolution of our HST images (52 km pixel −1 ) reveals details that remained hidden in previous ground-based observations, such as the extraordinarily small vertical extent of the dust sheet, ejection speeds well below the nucleus escape speed, and the possibility of a binary nucleus
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HUBBLE AND KECK TELESCOPE OBSERVATIONS OF ACTIVE ASTEROID 288P/300163 (2006 VW139)
Energy Technology Data Exchange (ETDEWEB)
Agarwal, Jessica [Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, D-37077 Göttingen (Germany); Jewitt, David [Department Earth, Planetary and Space Sciences, UCLA, 595 Charles Young Drive East, Box 951567 Los Angeles, CA 90095-1567 (United States); Weaver, Harold [The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723 (United States); Mutchler, Max [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Larson, Stephen, E-mail: agarwal@mps.mpg.de [Lunar and Planetary Laboratory, University of Arizona, 1629 E. University Blvd. Tucson AZ 85721-0092 (United States)
2016-01-15
We present Hubble Space Telescope (HST) and Keck 10 m telescope observations of active asteroid 288P/300163 (2006 VW139) taken to examine ejected dust. The nucleus is a C-type object with absolute magnitude H{sub V} = 17.0 ± 0.1 and estimated diameter ∼2.6 km (for assumed visual geometric albedo p{sub V} = 0.04). Variations in the brightness of the nucleus at the 10%–15% level are significant in both 2011 December and 2012 October but we possess too few data to distinguish variations caused by activity from those caused by rotation. The dust scattering cross-section in 2011 December is ∼40 km{sup 2}, corresponding to a dust mass ∼9 × 10{sup 6} kg (88 μm mean particle radius assumed). The FWHM of the debris sheet varies from ∼100 km near the nucleus to ∼1000 km 30″ (40,000 km) east of it. Dust dynamical models indicate ejection speeds between 0.06 and 0.3 m s{sup −1}, particle sizes between 10 and 300 μm and an inverse square-root relation between particle size and velocity. Overall, the data are most simply explained by prolonged, low velocity ejection of dust, starting in or before 2011 July and continuing until at least 2011 October. These properties are consistent with the sublimation of near-surface ice aided by centrifugal forces. The high spatial resolution of our HST images (52 km pixel{sup −1}) reveals details that remained hidden in previous ground-based observations, such as the extraordinarily small vertical extent of the dust sheet, ejection speeds well below the nucleus escape speed, and the possibility of a binary nucleus.
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76 FR 58028 - Board of Visitors for the National Fire Academy
2011-09-19
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet on October 14 and 15, 2011. The meeting will be open to...
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The physical characteristics of match-play in English schoolboy and academy rugby union.
Read, Dale B; Jones, Ben; Phibbs, Padraic J; Roe, Gregory A B; Darrall-Jones, Joshua; Weakley, Jonathon J S; Till, Kevin
2018-03-01
The aim was to compare the physical characteristics of under-18 academy and schoolboy rugby union competition by position (forwards and backs). Using a microsensor unit, match characteristics were recorded in 66 players. Locomotor characteristics were assessed by maximum sprint speed (MSS) and total, walking, jogging, striding and sprinting distances. The slow component (<2 m · s -1 ) of PlayerLoad TM (PL slow ), which is the accumulated accelerations from the three axes of movement, was analysed as a measure of low-speed activity (e.g., rucking). A linear mixed-model was assessed with magnitude-based inferences. Academy forwards and backs almost certainly and very likely covered greater total distance than school forwards and backs. Academy players from both positions were also very likely to cover greater jogging distances. Academy backs were very likely to accumulate greater PL slow and the academy forwards a likely greater sprinting distance than school players in their respective positions. The MSS, total, walking and sprinting distances were greater in backs (likely-almost certainly), while forwards accumulated greater PL slow (almost certainly) and jogging distance (very likely). The results suggest that academy-standard rugby better prepares players to progress to senior competition compared to schoolboy rugby.
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Training activities and injuries in English youth academy and schools rugby union.
Palmer-Green, Deborah S; Stokes, Keith A; Fuller, Colin W; England, Michael; Kemp, Simon P T; Trewartha, Grant
2015-02-01
All rugby training activities carry an injury risk, but in the training environment these injury risks should be more controllable than during matches. To (1) describe the incidence, severity, anatomic location, and type of youth rugby training injuries; (2) determine the injury events and type of training activities associated with injuries; and (3) compare 2 levels of play (professional academy vs school) within English youth rugby union. Cohort study; Level of evidence, 2. A 2-season (2006-2007 and 2007-2008) study recorded exposure to training activities and time-loss injuries in male youth rugby union players (age range, 16-18 years) from 12 English Premiership academies (250 player-seasons) and 7 schools (222 player-seasons). Players from the Premiership academies, associated with the top-level professional clubs in England, represented the elite level of youth rugby; the school players were from established rugby-playing schools but were overall considered at a lower level of play. There was a trend for training injury incidence to be lower for the academy group (1.4/1000 player-hours; 95% CI, 1.0-1.7) compared with the school group (2.1/1000 player-hours; 95% CI, 1.4-2.9) (P = .06). Injuries to the ankle/heel and thigh were most common in academy players and injuries to the lumbar spine and ankle/heel region most common in school players. The training activities responsible for injury differed between the 2 groups: technical skills (scrummaging) for school players and contact skills (defense and ruck/maul drills) for academy players. For injury risk management in youth rugby, coaches of school players should focus on the development of the correct technique during practice of technical skills such as scrummaging, weight training, and skills training, and coaches of academy players should consider the extent to which contact drills are necessary during training. © 2014 The Author(s).
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Journals | Indian Academy of Sciences
Indian Academy of Sciences (India)
Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more. ... Posted on 21 December 2017. ASTROPHYSICS: An Observational View of the Universe. Math Art and Design: MAD about Math, Math Education and Outreach.
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more. ... Posted on 21 December 2017. ASTROPHYSICS: An Observational View of the Universe. Math Art and Design: MAD about Math, Math Education and Outreach.
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
2016-11-06
Nov 6, 2016 ... The Indian Academy of Sciences, Bengaluru, through many scientific meetings, symposia, and public lectures it organizes, aims to facilitate scientific exchange among researchers and to highlight novel findings both within the scientific community and the public. The Mid-Year Meetings held during July at ...
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Specialization: Stochastic Modelling Address during Associateship: Statistics & Mathematics Unit, Indian Statistical Institute, 203, B.T. Road, Kolkata 700 108. Contact: Email: krishanu@isical.ac.in. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th ...
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
The 25 July 2016 issue of Current Science includes a compilation of nine articles ... These articles, authored by various medical experts, both from India and outside, ... India's current position on the regulation of Ayurvedic practice, research and ... journal of science education brought out by the Indian Academy of Sciences.
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
The Indian Academy of Sciences, Bengaluru, through many scientific meetings, symposia, and public lectures it organizes, aims to facilitate scientific exchange among researchers and to highlight novel findings both within the scientific community and the public. The Mid-Year Meetings held during July at Bengaluru and the ...
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epsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Recent Lecture workshops. Recent advances in chemical sciences, 13–15 June 2017, St. Thomas College, Pala MORE · Action Plan for Harnessing Science and Technology towards Indigenous Self-Reliance. Posted on 12 July 2017. Submitted by the Science Academies to The Honorable Prime Minister of India. MORE ...
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 21 September 1953. Specialization: Plant Genetics Address during Associateship: Scientist, National Botanical Research, Institute, Rana Prathap Marg, Lucknow 226 001. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year ...
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Science Academies' Summer Research Fellowship Programme
Indian Academy of Sciences (India)
Home; Journals; Resonance – Journal of Science Education; Volume 22; Issue 11. Science Academies' Summer Research Fellowship Programme for Students and Teachers - 2018. Information and Announcements Volume 22 Issue 11 November 2017 pp 1100-1100 ...
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Change, organisational culture and the development of the South African Military Academy to 2009
Directory of Open Access Journals (Sweden)
G E (Deon Visser
2011-12-01
Full Text Available This article investigates the impact of change and organisational culture on the growth and development of the South African Military Academy. It explores the impact of Nationalist Party rule since 1948 and black majority rule since 1994 on the institutional culture of the South African military and how that influenced the development of the Military Academy. This is intertwined with an investigation of the nature and impact of the diverging military and academic subcultures at the Academy. The article contends that, together with the historical exclusion of blacks and women from the military, the marginalisation of white English-speaking citizens by Nationalist Party rule denied the Academy the exploitation of a significant portion of the country’s human resource potential in the interest of institutional development. The same happened with the introduction of racial quotas and the marginalisation of whites since 1994. The Military Academy has, furthermore, historically been too reflective of the organisational culture of the South African National Defence Force and its predecessors instead of informing that culture to meet the challenges of military professionalism. The Academy has a potentially vital educational role to play in the South African and Sub-Saharan African militaries, but requires some changes in its organisational culture to fulfil that mission. Keywords: South African Military Academy, organisational culture, military culture, military education, Stellenbosch University Disciplines: Military History, Industrial Psychology
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77 FR 57102 - Board of Visitors for the National Fire Academy
2012-09-17
...] Board of Visitors for the National Fire Academy AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The Board of Visitors for the National Fire Academy (Board) will meet on October 5 and 6, 2012. The meeting will be open to the...
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967.pdf | 10apr2010 | currsci | Indian Academy of Sciences
Indian Academy of Sciences (India)
2010-04-10
Apr 10, 2010 ... error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 ...
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James.T.pdf | chemistry | resources | sci ed | initiat | Indian Academy ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JB 204.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JESS-D-12-00167.pdf | forthcoming | jess | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JB 742.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JB 92.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JESS-D-12-00365.pdf | forthcoming | jess | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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JB 230.pdf | forthcoming | jbsc | Volumes | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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What expects of academies. Activity of code and standard Div. in JSME, AESJ and JEA
International Nuclear Information System (INIS)
Miyano, Hiroshi
2005-01-01
The present states of establishment activities of standards by the three academies in the title are summarized from the viewpoint of 'explanation accountability'. Their roles and directions to go forward are also summarized. To be concrete, the trends of these establishment academies of standards relating to the nuclear industry are summarized. By focusing on the three indispensable conditions (neutrality, impartiality and transparency) for the establishment academy of standards and their implementation, the verifications of these conditions and 'explanation accountability' in these three academies are described. (K. Kato)
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The User-Driven Creative Academy
DEFF Research Database (Denmark)
Nielsen, Louise Møller; Poulsen, Søren Bolvig
2016-01-01
Users have always been a point of focus in design, but in the beginning of the new millennium userdriven approaches and user-oriented projects were taken to a new level of recognition. As part of this development, the User Driven Creative Academy (U-CrAc) was created at Aalborg University...
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
Special Issue on Theoretical Chemistry/Chemical Dynamics · The Ooty Radio Telescope Upgrade · Of Prisms, Soap Bubbles and Drones: National Science Day at the Academy!!! Science with the Square Kilometre Array: An Indian Perspective — A Special Issue of the Journal of Astrophysics and Astronomy · The 82nd ...
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Associateship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Date of birth: 15 January 1966. Specialization: Computer Science Address during Associateship: Machine Intelligence Unit, Indian Statistical Institute, 203, B T Road, Calcutta 700 035. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year ...
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INSPIRED High School Computing Academies
Doerschuk, Peggy; Liu, Jiangjiang; Mann, Judith
2011-01-01
If we are to attract more women and minorities to computing we must engage students at an early age. As part of its mission to increase participation of women and underrepresented minorities in computing, the Increasing Student Participation in Research Development Program (INSPIRED) conducts computing academies for high school students. The…
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Symposia | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Annual meetings of Academy include one or two symposia, one of which is usually on a topic of interest to or pursued in .... Impact of science and technology on medicine - a cardiac illustration ... Planetary studies ... Elementary particle physics
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Russian Academy of Engineering: a strong power for integration of engineering community
Directory of Open Access Journals (Sweden)
GUSEV Boris Vladimirovich
2015-04-01
Full Text Available Russian Academy of Engineering is legal successor of the Engineering Academy of USSR, founded by 20 ministries and departments of USSR and RSFSR on May 13, 1990. The Engineering Academy of USSR since the very beginning of its functioning, has launched its task-oriented activity on strengthening of links between science and industry, on solving the problems of using the results of basic (fundamental research and their accelerated adaptation into the industry. In the post-Soviet period, on the basis of the Academy, the Ministry of Justice of the Russian Federation, on December 24, 1991, registered the All-Russian Public Organization Russian Academy of Engineering (RAE. At the present time, RAE includes over 1350 full and corresponding members, prominent Russian scientists, engineers and industry organizers, over 200 member societies which include major Russian science & technology organizations, and over 40 regional engineering-technical structures, departments of RAE. RAE carries out large-scale work on the development of science & technology areas in science, creating new machinery and technologies, organization of efficient functioning of the Russian Engineering community. During the 25-year period of work, about 4,5 thousand new technologies were developed, over 6,5 thousand monographs were published. Over 4 thousand patents were obtained. 209 members of RAE became laureates of State Prize of USSR and RF, 376 members of RAE became laureates of Government Prize of USSR and RF. Annual value of science & research, project and other works in the area of engineering amounts from 0,5 to 1 billion roubles. This information and reference edition of the Encyclopedia of the Russian Academy of Engineering is dedicated to the 25th anniversary of the Russian Academy of Engineering. The Encyclopedia includes creative biographies of more than 1750 full and corresponding members of RAE, prominent scientists, distinguished engineers and organizers of industry
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Urban Teacher Academy Project Toolkit: A Guide to Developing High School Teaching Career Academies.
Berrigan, Anne; Schwartz, Shirley
There is an urgent need not only to attract more people into the teaching profession but also to build a more diverse, highly qualified, and culturally sensitive teaching force that can meet the needs of a rapidly changing school-age population. This Toolkit takes best practices from high school teacher academies around the United States and…
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2011-02-22
... for Teaching of American History and Civics (Presidential Academies) that offer workshops for both... DEPARTMENT OF EDUCATION Presidential Academies for Teaching of American History and Civics; Office of Innovation and Improvement; Overview Information; Presidential Academies for Teaching of American...
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An Exploratory Assessment of the United States Naval Academy Ethical Decision Making Instrument
National Research Council Canada - National Science Library
Beyer, Jr, Wayne R
2007-01-01
...). The study answered two questions regarding moral development at the Naval Academy. The first question involved determining if there is a difference in moral thinking between year groups at the Naval Academy...
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Opening Doors of Opportunity to Develop the Future Nuclear Workforce - 13325
International Nuclear Information System (INIS)
Mets, Mindy
2013-01-01
The United States' long-term demand for highly skilled nuclear industry workers is well-documented by the Nuclear Energy Institute. In addition, a study commissioned by the SRS Community Reuse Organization concludes that 10,000 new nuclear workers are needed in the two-state region of Georgia and South Carolina alone. Young adults interested in preparing for these nuclear careers must develop specialized skills and knowledge, including a clear understanding of the nuclear workforce culture. Successful students are able to enter well-paying career fields. However, the national focus on nuclear career opportunities and associated training and education programs has been minimal in recent decades. Developing the future nuclear workforce is a challenge, particularly in the midst of competition for similar workers from various industries. In response to regional nuclear workforce development needs, the SRS Community Reuse Organization established the Nuclear Workforce Initiative (NWI R ) to promote and expand nuclear workforce development capabilities by facilitating integrated partnerships. NWI R achievements include a unique program concept called NWI R Academies developed to link students with nuclear career options through firsthand experiences. The academies are developed and conducted at Aiken Technical College and Augusta Technical College with support from workforce development organizations and nuclear employers. Programs successfully engage citizens in nuclear workforce development and can be adapted to other communities focused on building the future nuclear workforce. (authors)
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Opening Doors of Opportunity to Develop the Future Nuclear Workforce - 13325
Energy Technology Data Exchange (ETDEWEB)
Mets, Mindy [Nuclear Workforce Initiative Program, SRS Community Reuse Organization, P.O. Box 696, Aiken, SC 29802 (United States)
2013-07-01
The United States' long-term demand for highly skilled nuclear industry workers is well-documented by the Nuclear Energy Institute. In addition, a study commissioned by the SRS Community Reuse Organization concludes that 10,000 new nuclear workers are needed in the two-state region of Georgia and South Carolina alone. Young adults interested in preparing for these nuclear careers must develop specialized skills and knowledge, including a clear understanding of the nuclear workforce culture. Successful students are able to enter well-paying career fields. However, the national focus on nuclear career opportunities and associated training and education programs has been minimal in recent decades. Developing the future nuclear workforce is a challenge, particularly in the midst of competition for similar workers from various industries. In response to regional nuclear workforce development needs, the SRS Community Reuse Organization established the Nuclear Workforce Initiative (NWI{sup R}) to promote and expand nuclear workforce development capabilities by facilitating integrated partnerships. NWI{sup R} achievements include a unique program concept called NWI{sup R} Academies developed to link students with nuclear career options through firsthand experiences. The academies are developed and conducted at Aiken Technical College and Augusta Technical College with support from workforce development organizations and nuclear employers. Programs successfully engage citizens in nuclear workforce development and can be adapted to other communities focused on building the future nuclear workforce. (authors)
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Southampton: A Case Study on Why Academies Are Not the Answer
Harris, Richard
2009-01-01
The author recounts the arrival of two Oasis Community Learning Academies in Southampton through a process of failed political courage to continue supporting the Local Authority. He tells of the subsequent impact when children and parents react against the regime in one of the Academies. In conclusion he challenges the Labour Government over the…
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Primary School Autonomy in the Context of the Expanding Academies Programme
Boyask, Ruth
2018-01-01
The transnational trend towards school autonomy has been enacted in England through the academies programme. The programme is poised to enter its third phase of expansion in light of government commitment to the conversion of all state-funded schools to academies. This article considers the moral implications of the expansion of the programme that…
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
2016-06-20
Jun 20, 2016 ... Only on two occasions the meetings travelled to the Royal Cities of Mysore and Hyderabad –during the Diamond and Platinum Jubilee years of the ... the International Year of Pulses, this edition of the Academy meeting has arranged a special lecture on a possible second Green Revolution through pulses.
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Driving Organizational Change From the Bedside: The AACN Clinical Scene Investigator Academy.
Lacey, Susan R; Goodyear-Bruch, Caryl; Olney, Adrienne; Hanson, Dave; Altman, Marian S; Varn-Davis, Natasha S; Brinker, Debbie; Lavandero, Ramón; Cox, Karen S
2017-08-01
Staff nurses are pivotal in leading change related to quality improvement efforts, although many lack skills to steer change from the bedside. The American Association of Critical-Care Nurses (AACN) staff nurse leadership program, Clinical Scene Investigator (CSI) Academy, teaches and empowers staff nurses in leadership skills and change concepts to translate evidence into practice affecting patient outcomes. To describe the curriculum of the AACN CSI Academy that provides staff nurses with the leadership skills required to create unit-based change projects that positively impact patient/family outcomes. The curriculum of the Academy included leadership topics, communication, change concepts, quality improvement methods, project management, and data management and analysis. Each team of participants collected project data to show improvements in patient care. The program evaluation used many data sources to assess the program effectiveness, relating to the professional growth of the participant nurses. The participants assessed project patient outcomes, sustainability, and spread. The first cohort of CSI participants included 164 direct care nurses from 42 hospitals in 6 cities. They rated the Academy highly in the program evaluation, and they reported that the Academy contributed to their professional development. The individual hospital quality improvement projects resulted in positive patient and estimated fiscal outcomes that were generally sustained 1 year after the program. With the skills, tools, and support obtained from participation in the CSI Academy, staff nurses can make substantial contributions to their organizations in clinical and possibly fiscal outcomes. ©2017 American Association of Critical-Care Nurses.
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International Nuclear Information System (INIS)
Naegel, W.
1997-01-01
On October 9, 1997, a seminar on energy sources was held in Duesseldorf within the framework of the programme of the academy for nature conservation and environmental protection (NUA) of North Rhine-Westphalia. The topic of the meeting, 'local governments' contributions to establishing a future-oriented energy policy from below' gathered representatives and lecturers from local authorities, electric utilities, planning and consultancy firms, political bodies and environmental associations. Papers presented to the seminar have been indexed and analysed for separate retrieval from the database. (orig./CB) [de
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Transport | Information | Indian Academy of Sciences
Indian Academy of Sciences (India)
Local Transport. The Academy office has made airport pick-up / drop-off arrangements as per the timings of the arrival / departure communicated by the Fellows / Speakers / Editorial Board Memebers. Detailed information on this will be sent separately to the participants ...
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76 FR 6149 - National Fire Academy Board of Visitors; Notice of Meeting
2011-02-03
...] National Fire Academy Board of Visitors; Notice of Meeting AGENCY: Federal Emergency Management Agency, DHS. ACTION: Committee Management; Notice of Open Federal Advisory Committee Meeting. SUMMARY: The National Fire Academy Board of Visitors will meet on February 22, 2011. DATES: The teleconference will take...
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Hanford Patrol Academy demolition sites closure plan
Energy Technology Data Exchange (ETDEWEB)
1993-09-30
The Hanford Site is owned by the U.S. Government and operated by the U.S. Department of Energy, Richland Operations Office. Westinghouse Hanford Company is a major contractor to the U.S. Department of Energy, Richland Operations Office and serves as co-operator of the Hanford Patrol Academy Demolition Sites, the unit addressed in this paper. This document consists of a Hanford Facility Dangerous Waste Part A Permit Application, Form 3 (Revision 4), and a closure plan for the site. An explanation of the Part A Form 3 submitted with this closure plan is provided at the beginning of the Part A section. This Hanford Patrol Academy Demolition Sites Closure Plan submittal contains information current as of December 15, 1994.
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Countermovement-Jump-Phase Characteristics of Senior and Academy Rugby League Players.
McMahon, John J; Murphy, Shannon; Rej, Sophie J E; Comfort, Paul
2017-07-01
Gross measures of countermovement-jump (CMJ) performance are commonly used to track maturational changes in neuromuscular function in rugby league (RL). The purpose of this study was to conduct both a gross and a more detailed temporal-phase analysis of the CMJ performances of senior and academy RL players, to provide greater insight into how neuromuscular function differs between these groups. Twenty senior and 14 academy (under-19) male RL players performed 3 maximal-effort CMJs on a force platform, with forward dynamics subsequently employed to allow gross performance measures and entire kinetic- and kinematic-time curves to be compared between groups. Jump height (JH), reactive strength index modified, concentric displacement, and relative concentric impulse (C-IMP) were the only gross measures that were greater for senior players (d = 0.58-0.91) than for academy players. The relative force- and displacement-time curves were similar between groups, but the relative power- and velocity-time curves were greater (d = 0.59-0.97) for the senior players at 94-96% and 89-100% of the total movement time, respectively. The CMJ distinguished between senior and academy RL players, with seniors demonstrating greater JH through applying a larger C-IMP and thus achieving greater velocity throughout the majority of the concentric phase and at takeoff. Therefore, academy RL players should train to improve triple (ie, ankle, knee, and hip) extension velocity during the CMJ to bring their JH scores in line with those attained by senior players.
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Home | Indian Academy of Sciences
Indian Academy of Sciences (India)
The Indian Academy of Sciences has published a new eBook in the Masterclass series, titled 'Linear Algebra and Analysis ', directed primarily at students and teachers of the undergraduate level. The eBook is a compilation of ten pedagogical articles on the topic– eight of which are sourced from Resonance, the Journal of ...
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Subjective education in analytic training: drawing on values from the art academy.
Dougherty, Mary
2008-11-01
Kernberg and others have observed that psychoanalytic education has tended to promote the acquisition of theoretical knowledge and clinical technique within an atmosphere of indoctrination rather than of exploration. As a corrective, he proposed four models that correspond to values in psychoanalytic education: the art academy, the technical trade school, the religious seminary and the university. He commended models of the university and art academy to our collective attention because of their combined effectiveness in providing for the objective and subjective education of candidates: the university model for its capacity to provide a critical sense of a wide range of theories in an atmosphere tolerating debate and difference, and the art academy model for its capacity to facilitate the expression of individual creativity. In this paper, I will explore the art academy model for correspondences between artistic and analytic trainings that can enhance the development of the creative subjectivity of psychoanalytic candidates. I will draw additional correspondences between analytic and artistic learning that can enhance psychoanalytic education.
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Overview | Publications | Indian Academy of Sciences
Indian Academy of Sciences (India)
Decadal vision document - Towards Ayurvedic Biology, 2006, PDF. Dragonflies and Damselflies of Peninsular India - a field guide, 2005, HTML. Report of Academy committee on scientific value, 2005, PDF. Decadal vision document - Astronomy & Astrophysics, 2004, PDF. Report on university education in science, 1994 ...
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Study of Gender Differences in Performance at the U.S. Naval Academy and U.S. Coast Guard Academy
National Research Council Canada - National Science Library
Sanders, Pride L
2005-01-01
.... The SAT scores for men and women at the two academies also were compared. The population included the Classes of 1997 through 2003, totaling 1,184 cadets from USCGA and 6,598 midshipmen from USNA...
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A Controversial Reform in Indigenous Education: The Cape York Aboriginal Australian Academy
McCollow, John
2012-01-01
This article examines a controversial initiative in Indigenous education: the establishment of the Cape York Aboriginal Australian Academy (CYAAA). The article provides a brief description of the Academy's three campuses and their communities and considers: the circumstances of its creation, including the role of Noel Pearson and Cape York…
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796.pdf | sept 25 2004 | curr sci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; curr sci; sept 25 2004; 796.pdf. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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621.pdf | Pdf2006Oct | sadha-na | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; sadha-na; Pdf2006Oct; 621.pdf. 404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be ...
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Jupiter Environmental Research & Field Studies Academy.
Huttemeyer, Bob
1996-01-01
Describes the development and workings of the Jupiter Environmental Research and Field Studies Academy that focuses on enabling both teachers and students to participate in real-life learning experiences. Discusses qualifications for admittance, curriculum, location, ongoing projects, students, academics, preparation for life, problem solving, and…
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Discussion Meetings | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
Academy supports discussion meetings of small groups of scientists from within India and outside organized by a ... Conference on Physics and Chemistry of Spintronic Materials ... Recent advances in operator theory and operator algebras
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American Academy of Allergy, Asthma, and Immunology
... reasons to celebrate its journals. Learn More about the American Academy Of Allergy, Asthma & Immunology Life Spectrum of Asthma Meeting School-based Asthma Management Program – (SAMPRO TM ) This central resource focuses on ...
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d8j-79.pdf | oct2009 | jessci | Indian Academy of Sciences
Indian Academy of Sciences (India)
Academy Public Lecture and INSA–Leopoldina Lecture by Prof. Jörg Hacker, President, German Academy of Sciences Leopoldina. 4 December, 2017, 4 PM Faculty Hall, Indian Institute. Associates – 2017. Posted on 30 August 2017. Click here to see the list · 83rd Annual Meeting. Posted on 01 December 2017.
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Summer Academy : for social media trainers in local regional governments and business
Liefers, Jan; Huttenga, Nancy; Goubin, Eric; Lemal, Marijke
2013-01-01
One of the work packages which Hanzehogeschool emphatically has a role, is Research and Training. In the Summer Academy teachers are trained by translating their knowledge back to their own schools. The Summer Academy is given on 27-30 May 2013, as part of "Opening Up". This project aims to find
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"I Love My Work, but This Is Not My Life": Women of Color in the Academy
Mena, Jasmine A.
2016-01-01
The present study used critical ethnography and intersectionality theory to better understand the experiences of Women of Color (WOC) in the academy. WOC experience numerous and significant challenges in the academy that have the potential to stifle their career growth. Claiming increased acceptance and diversity in the academy without a…
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[Navy medical academy (to the 75th anniversary of establishment)].
Chernikov, O G; Zaimagov, S V
2016-02-01
The article is devoted to the history of the creation in 1940 of the Naval Medical Academy on the basis of the 3rd Leningrad Medical Institute and the Institute for sanitary-chemical protection of the People's Commissariat of the USSR. The structure of this institution included, faculties management staff of the medical service, medical and sanitation, Higher Naval Medical School, the Marine Research Institute Medical, higher courses for officers of the medical service, clinical naval hospital. During the period of its activity (1940-1956), the staff of the Naval Medical Academy made a great contribution to the naval medicine and practical public health. The merit of the Academy is not only a beautifully staged academic, medical, research process, but also in the creation of the spirit of the high sea camaraderie, accomplishment and pride for the work which its graduates have dedicated their lives.
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[I. P. Pavlov--a Full Member (Academician) of Russian Academy of Sciences (100-years anniversary)].
Kosmachevskaia, E A; Gromova, L I
2008-01-01
I. P. Pavlov, the great Russian physiologist, the founder of a leading scientific school of physiology, first Russian scientist to be awarded the Nobel Prize. Pavlov's work received wide international recognition. He was elected full or honorary member of more than 120 academies, scientific societies and universities. In 1907 he was elected a Full Member (Academician) of Russian Academy of Sciences and headed the Physiological Laboratory of the Academy. In 1925, at his petition, the Laboratory was transformed into the Physiological Institute, remaining his head until 1936, when he had died. Since 1950 this is the Pavlov Institute of Physiology of the Russian Academy of Sciences.
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The Enlightenments of Educational Ideas of Ancient Academy on Modern Higher Education
Huang, Xia; Shen, Xi
2013-01-01
The ancient academy in China demonstrated some unique educational values, such as the school-running idea of independence and autonomy and the governance by famous experts, the instruction idea of being free and open and focusing on academy and morality cultivation, and the management concept of mind-oriented administration and student autonomy.…
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jbsc 040 05 0891-0907.pdf | Downloads | public | Indian Academy of ...
Indian Academy of Sciences (India)
error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog. Academy News. IAS Logo. 29th Mid-year meeting. Posted on 19 January 2018. The 29th Mid-year meeting of the Academy will be held from 29–30 June 2018 in Infosys, Mysuru ...
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Accommodation | Information | Indian Academy of Sciences
Indian Academy of Sciences (India)
Accommodation. The Academy has made arrangements to accommodate all participants who have requested for it. Details of accommodation have been sent to all registered participants. Volunteers at the airport will assist the participants in reaching their respective places of accommodation. For any queries ...
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
... Sharat Chandra (both of Indian Institute of Science, Bengaluru) and Suresh Jayakar ... In 1985, the Indian Academy of Sciences, Bengaluru, revived publication of ... It publishes papers and review articles on current topics, commentaries and ...
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Mr. B. Paton, President of the National Academy of Sciences, Ukraine
Patrice Loïez
2002-01-01
Photo 05: The Ambassador of Ukraine to Switzerland, H.E. Dr Yevhen Bersheda speaking on the occasion of the visit of the President of the National Academy of Sciences, Ukraine. Seated, clockwise from bottom left, Michel della Negra, Spokesman CMS; Roger Cashmore, Research Director; Academician Anatoli Shpak, Vice-President, National Academy of Sciences; John Ellis, Adviser for Non-Memebr State Relations; Viatcheslav Borschchov, CERN/SRTIIE; Teyana Levchuk, Interpreter; Dmytro Akimov, Director-General, Golden Fortune Foundation; Gennady Zinovjev, CERN/Ukraine Coordinator; Nicolas Koulberg, Coordinator for Russia and Eastern countries; J rgen Schukraft, Spokesman ALICE. Photo 21 : Dr Boris Paton, President of the National Academy of Sciences, Ukraine (left) and Prof. Roger Cashmore, Research Director for Collider Programmes frame the statue of the Goddess of Fortune which was given to CERN by the President.
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A Cook's Tour: The Journey to Become a Model Culinary Arts Academy
Bantang, Susan C.
2008-01-01
This article is about how the West Boca Raton Community High School's Culinary Arts Academy achieved national model status as it works to prepare the next generation of culinary artists. The culinary academy, established in 2004, adopted national standards that have served as a foundation for its excellence. In November 2007, the National Career…
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tendernotices | office | Indian Academy of Sciences
Indian Academy of Sciences (India)
Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more. ... Posted on 21 December 2017. ASTROPHYSICS: An Observational View of the Universe. Math Art and Design: MAD about Math, Math Education and Outreach.
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Information and Announcements Science Academies' Refresher ...
Indian Academy of Sciences (India)
IAS Admin
2015-11-15
Nov 15, 2015 ... Course Director: Professor Alok K Gupta, University of Allahabad, Allahabad 211 002, U.P.. Course Coordinator: Dr T D Mahabaleswara, Coordinator (RC&LW), Science Education Panel,. Indian Academy of Sciences, C V Raman Avenue, Sadashivanagar P O, Bangalore 560 080 (Email: sep@ias.ernet.in).
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Interrogating Gender and the Tourism Academy Through Epistemological Lens
DEFF Research Database (Denmark)
Chambers, Donna; Munar, Ana Maria; Khoo-Lattimore, Catheryn
2017-01-01
This introductory essay argues for the adoption of feminist epistemologies to unpack the role, nature and effects of gender (in) equality in our tourism academy. Our focus on tourism academia recognizes the importance of tourism to social life and the crucial role that tourism academics play...... in knowledge production. We therefore argue for a shift in the focus of extant gender research in tourism away from tourism as a phenomenon to ourselves as tourism academics. We provide an overview of the five papers in this special issue which explore the gendered nature of our academy in diverse contexts...
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A Value-Engaged Approach for Evaluating the Bunche-Da Vinci Learning Academy
Greene, Jennifer C.
2005-01-01
In 2001, the Bunche Academy was chosen by its district to join in partnership with the Da Vinci Learning Corporation to embark on an ambitious whole-school reform initiative, especially designed by the corporation for low-performing schools. In this chapter, the author describes how, as illustrated in the Bunche-Da Vinci Learning Academy context,…
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Energy Technology Data Exchange (ETDEWEB)
Bussmann, R. S.; Gurwell, M. A. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Fu Hai; Cooray, A. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Smith, D. J. B.; Bonfield, D.; Dunne, L. [Centre for Astrophysics, Science and Technology Research Institute, University of Hertfordshire, Hatfield, Herts AL10 9AB (United Kingdom); Dye, S.; Eales, S. [School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD (United Kingdom); Auld, R. [Cardiff University, School of Physics and Astronomy, Queens Buildings, The Parade, Cardiff CF24 3AA (United Kingdom); Baes, M.; Fritz, J. [Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent (Belgium); Baker, A. J. [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019 (United States); Cava, A. [Departamento de Astrofisica, Facultad de CC. Fisicas, Universidad Complutense de Madrid, E-28040 Madrid (Spain); Clements, D. L.; Dariush, A. [Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Coppin, K. [Department of Physics, McGill University, Ernest Rutherford Building, 3600 Rue University, Montreal, Quebec, H3A 2T8 (Canada); Dannerbauer, H. [Universitaet Wien, Institut fuer Astronomie, Tuerkenschanzstrasse 17, 1180 Wien, Oesterreich (Austria); De Zotti, G. [Universita di Padova, Dipto di Astronomia, Vicolo dell' Osservatorio 2, IT 35122, Padova (Italy); Hopwood, R., E-mail: rbussmann@cfa.harvard.edu [Department of Physics and Astronomy, Open University, Walton Hall, Milton Keynes, MK7 6AA (United Kingdom); and others
2012-09-10
We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 {mu}m and the Keck adaptive optics (AO) system at the K{sub S}-band of a gravitationally lensed submillimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey. The SMA data (angular resolution Almost-Equal-To 0.''6) resolve the dust emission into multiple lensed images, while the Keck AO K{sub S}-band data (angular resolution Almost-Equal-To 0.''1) resolve the lens into a pair of galaxies separated by 0.''3. We present an optical spectrum of the foreground lens obtained with the Gemini-South telescope that provides a lens redshift of z{sub lens} = 0.595 {+-} 0.005. We develop and apply a new lens modeling technique in the visibility plane that shows that the SMG is magnified by a factor of {mu} = 4.1 {+-} 0.2 and has an intrinsic infrared (IR) luminosity of L{sub IR} = (2.1 {+-} 0.2) Multiplication-Sign 10{sup 13} L{sub Sun }. We measure a half-light radius of the background source of r{sub s} = 4.4 {+-} 0.5 kpc which implies an IR luminosity surface density of {Sigma}{sub IR} (3.4 {+-} 0.9) Multiplication-Sign 10{sup 11} L{sub Sun} kpc{sup -2}, a value that is typical of z > 2 SMGs but significantly lower than IR luminous galaxies at z {approx} 0. The two lens galaxies are compact (r{sub lens} Almost-Equal-To 0.9 kpc) early-types with Einstein radii of {theta}{sub E1} 0.57 {+-} 0.01 and {theta}{sub E2} = 0.40 {+-} 0.01 that imply masses of M{sub lens1} = (7.4 {+-} 0.5) Multiplication-Sign 10{sup 10} M{sub Sun} and M{sub lens2} = (3.7 {+-} 0.3) Multiplication-Sign 10{sup 10} M{sub Sun }. The two lensing galaxies are likely about to undergo a dissipationless merger, and the mass and size of the resultant system should be similar to other early-type galaxies at z {approx} 0.6. This work highlights the importance of high spatial resolution imaging in developing models of strongly lensed galaxies
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
... Center for Agricultural Resources Research, Institute of Genetics and Developmental Biology, Chinese Academy of Sciences, Shijiazhuang, 050021, Hebei, People's Republic of China; Tianxing Biotechnology, Handian Industrial Zone, 256200 Zouping, Shandong, People's Republic of China; Tobacco Research Institute, ...
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Science Academies' Refresher Course on Theoretical Structural ...
Indian Academy of Sciences (India)
Home; Journals; Resonance – Journal of Science Education; Volume 22; Issue 8. Science Academies' Refresher Course on Theoretical Structural Geology, Crystallography, Mineralogy, Thermodynamics, Experimental Petrology and Theoretical Geophysics. Information and Announcements Volume 22 Issue 8 August 2017 ...
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Science Academies' Refresher Course on Advanced Quantum ...
Indian Academy of Sciences (India)
IAS Admin
2016-10-10
Sponsored by Indian Academy of Sciences, Bengaluru. Indian National ... brief statement (between 250 and 500 words) as to why they think the Course will help to improve their classroom ... Last date for receipt of applications: October 10, 2016.
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Journal of Biosciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
History · Memorandum of Association · Role of the Academy · Statutes · Council ... Darwin proposed the theory of sexual selection to explain the differences between the ... First, classical Darwinism failed to recognize social competition as an ...
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Apprenticeship at the Academy of Music
Nielsen, Klaus
2006-01-01
Inspired by studies of apprenticeship and theories of situated learning, this study argues that learning should be understood in relation to ongoing social practice. Using interview material and participant observation studying piano students' learning at the Academy of Music in Aarhus, it describes how transparency and access to the music culture…
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Action Learning Drives the Emerald Academy
Nalborczyk, Sarah; Sandelands, Luke
2012-01-01
This account examines the action learning process adopted by Emerald Group Publishing Ltd., embedded in the organization through the in-company Emerald Academy. In case study format, the paper emphasizes that in order to align learning with organizational objectives joined up thinking and practice is needed beyond the learning and development…
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Kawane, Shannon E.
1999-01-01
This thesis addresses several issues identified in the analysis and design phases of the Instructional Systems Development process to develop an IMI leadership program for the Naval Academy. The overarching goal is to provide the Naval Academy with a study that uses current research and existing innovative leadership programs to answer questions that need to be resolved in developing a program consistent with the Naval Academy's leadership training philosophy. The results suggest that an IMI ...
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Science Academies Refresher Course on Crustal Strength ...
Indian Academy of Sciences (India)
2017-05-26
May 26, 2017 ... Sponsored by Indian Academy of Sciences, Bengaluru. Indian National Science ... Only 25 outstations and 10 Local ... a brief statement (between 250 and 500 words) as to why they think the Course will help to improve their.
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Project Lifescape | Initiatives | Indian Academy of Sciences
Indian Academy of Sciences (India)
This project is part of the Academy initiative to enhance the quality of science education. It is pursued in ... database through a website. Project Lifescape has also initiated work using some Indian languages. ... and Outreach. Math and Finance ...
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What Is Hospitality in the Academy? Epistemic Ignorance and the (Im)possible Gift
Kuokkanen, Rauna
2008-01-01
The academy is considered by many as the major Western institution of knowledge. This article, however, argues that the academy is characterized by prevalent "epistemic ignorance"--a concept informed by Spivak's discussion of "sanctioned ignorance." Epistemic ignorance refers to academic practices and discourses that enable the continued exclusion…
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Kok, Laura M; Nelissen, Rob G H H; Huisstede, Bionka M A
2015-09-01
CANS (complaints of arm, neck, and/or shoulder not caused by a systemic disease or acute trauma) are a recognized problem in specific occupational groups such as musicians. This study aimed to compare the prevalence, characteristics, and consequences of CANS between music academy students and a control group of peer-age medical students. A cross-sectional study among music academy students and medical students. Data were collected using a web-based questionnaire on musculoskeletal conditions of the upper extremity in the two cohorts. Students of three music academies (n=345) and one medical university (n=2,870) received the questionnaire, of which 25% (n=87) and 18% (n=503) responded, respectively. The 12-month prevalence of CANS was nearly twice as high among music academy students as the control group (80.7% vs 41.5%, pMusic academy students reported 2.6 times the point prevalence as medical students (47.0% vs 18.2%, pmusic students, compared to 10.3% of the medical students (pMusic academy students presented more complaints per anatomic localization and a higher number of involved anatomic localizations. Music students rated the influence of CANS on daily functioning as more severe (5.0 vs 3.1, pmusic academy students (46.3%) visited a healthcare professional compared to medical students (29.8%, p=0.013). The prevalence of CANS is high in music academy students compared to medical students. This emphasizes the necessity of effective (preventive) interventions in these high-demanding professionals.
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Moderating effect of age on the association between future time perspective and preventive coping.
Chen, Tao; Liu, Lu-Lu; Cui, Ji-Fang; Chen, Xing-Jie; Shi, Hai-Song; Neumann, David L; Shum, David H K; Wang, Ya; Chan, Raymond C K
2017-09-01
The present study aimed to investigate the moderating effect of age on the relationship between future time perspective (FTP) and future-oriented coping. A total of 1,915 participants aged 9-84 years completed measures of FTP and future-oriented coping. Moderation analyses were conducted to examine whether age played a role in the association between FTP and future-oriented coping (proactive and preventive). Results showed that proactive and preventive coping were negatively correlated with age, and age moderated the association between FTP and preventive coping but not proactive coping. Furthermore, the strength of the positive association between FTP and preventive coping was strongest among the older participants, moderate among the middle-aged participants, and weakest among the younger participants. These results suggest that the association between FTP and preventive coping varies across the lifespan. © 2017 The Institute of Psychology, Chinese Academy of Sciences and John Wiley & Sons Australia, Ltd.
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National Research Council Canada - National Science Library
Kawane, Shannon
1999-01-01
... a program consistent with the Naval Academy's leadership training philosophy. The results suggest that an IMI program can be developed that is consistent with the Naval Academy's leadership development program...
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Science Academies' Refresher Course on Quantum Mechanics
Indian Academy of Sciences (India)
Home; Journals; Resonance – Journal of Science Education; Volume 21; Issue 7. Science Academies' Refresher Course on Quantum Mechanics. Information and Announcements Volume 21 Issue 7 July 2016 pp 669-670. Fulltext. Click here to view fulltext PDF. Permanent link:
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Science Academies' Refresher Course in Developmental Biology
Indian Academy of Sciences (India)
Home; Journals; Resonance – Journal of Science Education; Volume 20; Issue 8. Science Academies' Refresher Course in Developmental Biology. Information and Announcements Volume 20 Issue 8 August 2015 pp 756-756. Fulltext. Click here to view fulltext PDF. Permanent link:
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
Life Science and Technology A1201, Beijing University of Chemical Technology, Beijing 102200, People's Republic of China; Department of Food Crop Science, Cotton Research Institute, Shanxi Agriculture Science Academy, Yuncheng, Shanxi 044000, People's Republic of China; Foreign Language College, Anhui ...
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
Faculty of Geology, Lomonosov Moscow State University, GSP-1, 1 Leninskiye Gory, Moscow 119991, Russia; Earth Cryosphere Institute, Siberian Branch of Russian Academy of Sciences, Tyumen, 86 Malygina, Tyumen 625000, Russia; State Research Center for Applied Microbiology and Biotechnology, Obolensk, ...
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The CSI Academy: Encouraging Diverse Students to Consider Science Careers and Science Teaching
Kaye, Karen; Turner, John F.; Emigh, James
2011-01-01
The CSI academies employed a multi-layered, collaborative approach to encourage diverse students to consider STEM careers, including science teaching. The academies recruited a diverse group of high school students. This was due, in large part, to the creation of a unique selection process that identified students with unrealized potential. The…
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Cisco Networking Academy: Next-Generation Assessments and Their Implications for K-12 Education
Liu, Meredith
2014-01-01
To illuminate the possibilities for next-generation assessments in K-12 schools, this case study profiles the Cisco Networking Academy, which creates comprehensive online training curriculum to teach networking skills. Since 1997, the Cisco Networking Academy has served more than five million high school and college students and now delivers…
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US and Russian academies forge ties for nuclear security
International Nuclear Information System (INIS)
Eldridge, Christopher A.
2005-01-01
In response to the growing threats of nuclear terrorism and proliferation, the US National Academies (NA) and the Russian Academy of Sciences (RAS) initiated a series of joint projects in early 2002 that bring their concerted expertise to bear on the challenges of cooperation between their two countries on nuclear non-proliferation. The IAEA has lent its talent and support to this inter-academy collaboration by hosting workshops that were jointly organized by the NA and RAS with financial support from the US-based Nuclear Threat Initiative. The two workshops, held at IAEA headquarters in September 2003, shed valuable light on both the obstacles and opportunities being faced. The first workshop explored ways of overcoming impediments to cooperation between the US and Russia on nuclear non-proliferation. Participants included current and former US and Russian government officials with responsibility for cooperative programs as well as experts from non-governmental organizations in the two countries. The second workshop convened a multinational group of experts on nuclear materials protection, control, and accounting (MPC and A) to discuss practices and procedures in light of the evolving threats of nuclear proliferation and terrorism
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Workshop Report: The Future of ROK Navy-US Navy Cooperation
2007-10-01
at the Korea Naval Academy in the southeastern port city of Chinhae, President Kim said, "We will soon have a strategic mobile fleet that protects...CHINA INDIA* Dhaka ngkok MAIMYS *Kua -4 zz z < <zt C z4 wi ohm,; -0 CL SCl) ._ ൈ a)) U)c Cu somm ... U- /) ’- ,+ • - ) o C7C am U D-a-- w • • - • C...This is the reason why the surrounding nations show a very keen concern on the sea boundary issues. The ROK’s economic fate in the future depends on
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Service Academy 2005 Sexual Harassment and Assault Survey
National Research Council Canada - National Science Library
Cook, Paul J; Jones, Alan M; Lipari, Rachel N; Lancaster, Anita R
2005-01-01
This report provides the results for the Service Academy 2005 Sexual Harassment and Assault Survey that the Defense Manpower Defense Center conducted in response to Section 527 of the National Defense...
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Unsafe in the Camouflage Tower: Sexual Victimization and Perceptions of Military Academy Leadership
Snyder, Jamie A.; Fisher, Bonnie S.; Scherer, Heidi L.; Daigle, Leah E.
2012-01-01
Few studies have examined sexual victimization among cadets and midshipmen at the three U.S. Military Academies. Self-report data from the 2005 Service Academy Sexual Assault Survey of Cadets and Midshipmen (n = 5,220) were used to examine the extent of unwanted sexual attention, sexual harassment, unwanted sexual contact, sexual coercion, and…
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48th Annual Meeting of the Academy
Indian Academy of Sciences (India)
1982-10-08
Oct 8, 1982 ... It was in early 1977 that the Academy decided to .... To obviate against these disadvantages, the screening of ... as done in a'few places in the West, by using urine as the body ..... teachers and who came as vacation workers,.
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
The National Key Facility for Crop Gene Resources and Genetic Improvement, Institute of Crop Science, Chinese Academy of Agricultural Sciences, Beijing 100081, People's Republic of China; College of Tobacco Science, Henan Agricultural University, Zhengzhou 450002, People's Republic of China; Institute of Cotton ...
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Journal of Biosciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
Logo of the Indian Academy of Sciences ... Home; Journals; Journal of Biosciences; Volume 28; Issue 1 ... Department of Safety and Environmental Management, College of Engineering and Mineral Resources, Morgantown, WV 26506, USA; Health Effects Laboratory Division, National Institute for Occupational Safety and ...
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Annual Meetings | Events | Indian Academy of Sciences
Indian Academy of Sciences (India)
two days in early July) is held in Bangalore, while the location of the Annual meeting of the Academy (three days around the 7th of November) changes each year. During these meetings, there are symposia on special topics as well as ...
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Proceedings – Mathematical Sciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
Author Affiliations. XIAOXIANG JIAO1 MINGYAN LI2. School of Mathematical Sciences, University of Chinese Academy of Sciences, Beijing 101408, China; School of Mathematics and Statistics, Zhengzhou University, Zhengzhou 450001, China ...
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About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
404! error. The page your are looking for can not be found! Please check the link or use the navigation bar at the top. YouTube; Twitter; Facebook; Blog ... Theory Of Evolution. Posted on 23 January 2018. Joint Statement by the Three Science Academies of India on the teaching of the theory of evolution more.
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[SLEEP OF ELITE YOUNG ATHLETE AT THE ACADEMY FOR SPORT EXCELLENCE AT THE WINGATE INSTITUTE].
Navot Mintzer, Dalya; Shargal, Eyal; Fuxman, Yair; Wissblat, Dorit; Baharav, Anda
2016-06-01
Sleep duration and quality have a critical role in cognitive and athletic performances. A relationship was demonstrated between sleep deprivation, reduced performance and elevated injury risk. The recommended sleep duration for teenagers is at least 9 hours a day but most sleep less. To estimate sleep duration among elite adolescent athletes at the Academy for Sport Excellence at the Wingate Institute, by quantifying the changes after joining the academy and the relation to school performances and the usage of medical services. Data from medical records, including sleep screening questionnaires and a number of the athletes' medical appointments were analyzed. Athletes reported that sleep duration was less than recommended before joining the academy. After joining the academy the average sleep duration decreased (7.37 vs 7.7 hours, P = 0.05) and daytime sleepiness was elevated (13/24 v 11/24 Epworth-Sleepiness-Scale (ESS), P = 0.002). Correlations between changes in sleep duration and changes in school achievements before and after joining the academy were demonstrated (P = 0.027). No correlation was found between sleep duration at the academy and usage of medical services. Elite adolescent athletes do not sleep enough and are tired during the day. Reduction in sleep duration and elevation in sleepiness were observed with the transition to practice, study and life at the Academy for Sport Excellence. In accordance with previous studies, our findings showed elite young athletes are in a state of continuous sleep deprivation that interferes with their school achievements. Further research is needed to evaluate the importance of sleep duration and quality in performance for the health of young athletes.
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President Barack Obama addresses the 146th annual meeting of the National Academy of Sciences.
2009-06-16
On April 27, 2009, President Barack Obama addressed members of the National Academy of Sciences (NAS) gathered at its 146th annual meeting in Washington, D.C. In his speech, the president shared his plans to give science and technology a central role in the nation's future and an immediate place in America's economic renewal. He outlined steps he is taking to increase research spending, achieve energy independence, and improve science education. Included was what Mr. Obama cited as the largest commitment to scientific research in American history-devoting more than 3% of our gross domestic product to research and development. "Next, we are restoring science to its rightful place," Mr. Obama told a packed NAS auditorium audience. "Under my administration, the days of science taking a backseat to ideology are over." He appealed to scientists' sense of personal responsibility to reach and educate young Americans: "I want to challenge you to use your love and knowledge of science to spark a sense of wonder and excitement in a new generation." President Obama was welcomed to the National Academy of Sciences by President Ralph J. Cicerone and John P. Holdren, Assistant to the President for Science and Technology and Director of the White House Office of Science and Technology Policy. The following is a transcript of that speech.
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Biomechanics in dermatology: Recent advances and future directions.
Lewinson, Ryan T; Haber, Richard M
2017-02-01
Biomechanics is increasingly being recognized as an important research area in dermatology. To highlight only a few examples, biomechanics has contributed to the development of novel topical therapies for aesthetic and medical purposes, enhanced our understanding of the pathogenesis of plantar melanoma, and provided insight into the epidemiology of psoriatic disease. This article summarizes the findings from recent studies to demonstrate the important role that biomechanics may have in dermatologic disease and therapy and places these biomechanical findings in a clinical context for the practicing physician. In addition, areas for future biomechanics research and development in dermatology are discussed. Copyright © 2016 American Academy of Dermatology, Inc. Published by Elsevier Inc. All rights reserved.
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On Detecting New Worlds: The Art of Doppler Spectroscopy with Iodine Cells
Wang, Sharon Xuesong
2016-08-01
20-50 cm/s. The strategies proposed and tested in this thesis will improve the RV precision of HET/HRS and Keck/HIRES, including their decade worth of archival data. This thesis also documents my work on characterizing exoplanet orbits using RV data and the discovery of HD 37605c. It concludes with a summary of major findings and an outline of future plans to use future precise Doppler spectrometers to move towards the goal of 10 cm/s and detecting Earth 2.0.
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Science Academies' Refresher Course on Theoretical Structural ...
Indian Academy of Sciences (India)
A course on Theoretical Structural Geology, Crystallography, Mineralogy, Thermodynamics, Exper- imental Petrology and Theoretical Geophysics will be conducted in the Jallahalli Campus under the aegis of Indian Academy of Sciences during 20th November to 4th December, 2017. University lec- turers, Research ...
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
Author Affiliations. JAMILEH MALBIN1 MOHAMMAD-SADEGH FALLAH2 3 ZOHREH SHARIFI2 MAHSA SHAFAEI4 HAMIDEH BAGHERIAN2 TAHEREH POUR MOSTAFAEI2 RAMIZ ALIEV1 SIROUS ZAINALI2 5. Azerbaijan National Academy of Science (ANAS), Genetic Resources Institute, Baku AZ1005, Azerbaijan ...
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Partial Support of MAST Academy Outreach Program
1993-05-25
Another very positive aspect of the student-mentor relationship occured when young women served their internship with a woman scientist or the... siences has indirectly led to the initiation of similar programs in other academic areas. APPENDIX A JOB DESCRIPTIONS FOR MAST ACADEMY OUTREACH PROGRAM
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Millan-Gabet, Rafael; Che, Xiao; Monnier, John D.; Sitko, Michael L.; Russell, Ray W.; Grady, Carol A.; Day, Amanda N.; Perry, R. B.; Harries, Tim J.; Aarnio, Alicia N.; Colavita, Mark M.; Wizinowich, Peter L.; Ragland, Sam; Woillez, Julien
2016-08-01
We present near- and mid-infrared (MIR) interferometric observations made with the Keck Interferometer Nuller and near-contemporaneous spectro-photometry from the infrared telescope facilities (IRTFs) of 11 well-known young stellar objects, several of which were observed for the first time in these spectral and spatial resolution regimes. With au-level spatial resolution, we first establish characteristic sizes of the infrared emission using a simple geometrical model consisting of a hot inner rim and MIR disk emission. We find a high degree of correlation between the stellar luminosity and the MIR disk sizes after using near-infrared data to remove the contribution from the inner rim. We then use a semi-analytical physical model to also find that the very widely used “star + inner dust rim + flared disk” class of models strongly fails to reproduce the spectral energy distribution (SED) and spatially resolved MIR data simultaneously; specifically a more compact source of MIR emission is required than results from the standard flared disk model. We explore the viability of a modification to the model whereby a second dust rim containing smaller dust grains is added, and find that the 2-rim model leads to significantly improved fits in most cases. This complexity is largely missed when carrying out SED modeling alone, although detailed silicate feature fitting by McClure et al. recently came to a similar conclusion. As has been suggested recently by Menu et al., the difficulty in predicting MIR sizes from the SED alone might hint at “transition disk”-like gaps in the inner au; however, the relatively high correlation found in our MIR disk size versus stellar luminosity relation favors layered disk morphologies and points to missing disk model ingredients instead.
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Energy Technology Data Exchange (ETDEWEB)
Millan-Gabet, Rafael [California Institute of Technology, NASA Exoplanet Science Institute, Pasadena, CA 91125 (United States); Che, Xiao; Monnier, John D.; Aarnio, Alicia N. [University of Michigan Astronomy Department, 1085 S. University Avenue 303B West Hall University of Michigan, Ann Arbor, MI 48109-1107 (United States); Sitko, Michael L.; Day, Amanda N. [Department of Physics, University of Cincinnati, Cincinnati OH 45221 (United States); Russell, Ray W. [The Aerospace Corporation, Los Angeles, CA 90009 (United States); Grady, Carol A. [Eureka Scientific, 2452 Delmer, Suite 100, Oakland, CA 96002 (United States); Perry, R. B. [NASA Langley Research Center, MS 160, Hampton, VA 23681 (United States); Harries, Tim J. [Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter EX4 4QL (United Kingdom); Colavita, Mark M. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Wizinowich, Peter L.; Ragland, Sam; Woillez, Julien, E-mail: R.Millan-Gabet@caltech.edu [Keck Observatory, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743 (United States)
2016-08-01
We present near- and mid-infrared (MIR) interferometric observations made with the Keck Interferometer Nuller and near-contemporaneous spectro-photometry from the infrared telescope facilities (IRTFs) of 11 well-known young stellar objects, several of which were observed for the first time in these spectral and spatial resolution regimes. With au-level spatial resolution, we first establish characteristic sizes of the infrared emission using a simple geometrical model consisting of a hot inner rim and MIR disk emission. We find a high degree of correlation between the stellar luminosity and the MIR disk sizes after using near-infrared data to remove the contribution from the inner rim. We then use a semi-analytical physical model to also find that the very widely used “star + inner dust rim + flared disk” class of models strongly fails to reproduce the spectral energy distribution (SED) and spatially resolved MIR data simultaneously; specifically a more compact source of MIR emission is required than results from the standard flared disk model. We explore the viability of a modification to the model whereby a second dust rim containing smaller dust grains is added, and find that the 2-rim model leads to significantly improved fits in most cases. This complexity is largely missed when carrying out SED modeling alone, although detailed silicate feature fitting by McClure et al. recently came to a similar conclusion. As has been suggested recently by Menu et al., the difficulty in predicting MIR sizes from the SED alone might hint at “transition disk”-like gaps in the inner au; however, the relatively high correlation found in our MIR disk size versus stellar luminosity relation favors layered disk morphologies and points to missing disk model ingredients instead.
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International Nuclear Information System (INIS)
Millan-Gabet, Rafael; Che, Xiao; Monnier, John D.; Aarnio, Alicia N.; Sitko, Michael L.; Day, Amanda N.; Russell, Ray W.; Grady, Carol A.; Perry, R. B.; Harries, Tim J.; Colavita, Mark M.; Wizinowich, Peter L.; Ragland, Sam; Woillez, Julien
2016-01-01
We present near- and mid-infrared (MIR) interferometric observations made with the Keck Interferometer Nuller and near-contemporaneous spectro-photometry from the infrared telescope facilities (IRTFs) of 11 well-known young stellar objects, several of which were observed for the first time in these spectral and spatial resolution regimes. With au-level spatial resolution, we first establish characteristic sizes of the infrared emission using a simple geometrical model consisting of a hot inner rim and MIR disk emission. We find a high degree of correlation between the stellar luminosity and the MIR disk sizes after using near-infrared data to remove the contribution from the inner rim. We then use a semi-analytical physical model to also find that the very widely used “star + inner dust rim + flared disk” class of models strongly fails to reproduce the spectral energy distribution (SED) and spatially resolved MIR data simultaneously; specifically a more compact source of MIR emission is required than results from the standard flared disk model. We explore the viability of a modification to the model whereby a second dust rim containing smaller dust grains is added, and find that the 2-rim model leads to significantly improved fits in most cases. This complexity is largely missed when carrying out SED modeling alone, although detailed silicate feature fitting by McClure et al. recently came to a similar conclusion. As has been suggested recently by Menu et al., the difficulty in predicting MIR sizes from the SED alone might hint at “transition disk”-like gaps in the inner au; however, the relatively high correlation found in our MIR disk size versus stellar luminosity relation favors layered disk morphologies and points to missing disk model ingredients instead.
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Women Achievers | Women in Science | Initiatives | Indian Academy ...
Indian Academy of Sciences (India)
... demonstrations and creation of infrastructural facilities a clear visible impact of this ... and skill to address such challenges as hunger, disease and poverty. ... the Academy had essential support from Italian scientists and political leaders.
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Oral History Archives | Fellowship | Indian Academy of Sciences
Indian Academy of Sciences (India)
Home; Fellowship; Oral History Archives. Oral history archive ... video documentaries of some of the leading scientists of the country from among Academy's fellowship. ... Math Art and Design: MAD about Math, Math Education and Outreach.
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Paul Abraham: A Forgotten Scholar of the Prussian Academy of Sciences and Humanities
Thiel, Jens
2004-01-01
Paul Abraham, one of the Berlin Academy's most experienced researchers, was deported to Auschwitz in 1943. The fate of this Jewish scholar reveals much about the inner life of the Academy, and its treatment of Jewish staff, during the World War II. This paper describes his life, against a backdrop of war, revolution, and dictatorship, and in the…
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Cognitive style and plebe turnover at the U.S. Naval Academy.
Mitchell, Tom; Cahill, Alice M
2005-08-01
Students entering (N = 1,134) the U.S. Naval Academy class of 2000 were administered the Kirton Adaption-Innovation Inventory on the first day of Plebe Summer, a 7-wk. nonacademic training program completed by all entering students in the summer prior to the freshman year. The mean score on Innovation cognitive style for this sample of plebes was approximately a standard deviation lower than those of five other undergraduate student samples from nonmilitary universities. Furthermore, the 98 plebes who voluntarily withdrew before completing the program scored higher on the average on Innovation than those who remained. Findings suggest that, in terms of Person-Organization fit, plebes with a more innovative cognitive style may, perhaps, be less compatible with the regimentation-style climate of the Academy than those with an Adaptive cognitive style. Further research, however, is needed to specify the relationship between Academy students' cognitive style and other important organizational outcomes.
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Africa Agribusiness Academy (AAA) Year Report 2014
Nijhoff, G.H.; Vugt, van S.M.
2015-01-01
The Africa Agribusiness Academy (AAA) supports African SME agrifood companies in growing their business. An AAA member companies can enhance knowledge, skills and expertise, and get support in accessing finance and markets. By the end of 2014, AAA had 200 members in five countries: Tanzania, Kenya,
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Savage, Grant T; Duncan, W Jack; Knowles, Kathy L; Nelson, Kathleen; Rogers, David A; Kennedy, Karen N
2014-05-01
The study describes the genesis of the University of Alabama at Birmingham's Healthcare Leadership Academy (HLA), highlights the HLA's outcomes, discloses how the HLA has changed, and delineates future directions for academic health center (AHC) interprofessional leadership training. While interprofessional training is recognized as an important component of the professional education for health professionals, AHCs have not focused on interprofessional leadership training to prepare future AHC leaders. As professional bureaucracies, AHCs require leadership distributed across different professions; these leaders not only should be technical experts, but also skilled at interprofessional teamwork and collaborative governance. The HLA is examined using the case method, which is supplemented with a descriptive analysis of program evaluation data and outcomes. The HLA has created a networked community of AHC leaders; the HLA's interprofessional team projects foster innovative problem solving. Interprofessional leadership training expands individuals' networks and has multiple organizational benefits. © 2014.
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Site Index | About IASc | Indian Academy of Sciences
Indian Academy of Sciences (India)
History · Memorandum of Association · Role of the Academy · Statutes ... Proceedings – Mathematical Sciences · Resonance – Journal of Science Education · Sadhana ... Math Art and Design: MAD about Math, Math Education and Outreach.
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The Academy of Arts and Sciences in Krakow (1872–1918 and its Czech members (in Polish
Directory of Open Access Journals (Sweden)
Halina LICHOCKA
2015-12-01
Full Text Available The article shows that the Czech humanists formed the largest group among the foreign members of the Academy of Arts and Sciences in Krakow. It is mainly based on the reports of the activities of the Academy. The Academy of Arts and Sciences in Krakow was established by transforming the Krakow Learned Society. The Statute of the newly founded Academy was approved by a decision of the Emperor Franz Joseph I on February 16, 1872. The Emperor nominated his brother Archduke Karl Ludwig as the Academy’s Protector. The Academy was assigned to take charge of research matters related to different fields of science: philology (mainly Polish and other Slavic languages; history of literature; history of art; philosophical; political and legal sciences; history and archaeology; mathematical sciences, life sciences, Earth sciences and medical sciences. In order to make it possible for the Academy to manage so many research topics, it was divided into three classes: a philological class, a historico‑philosophical class, and a class for mathematics and natural sciences. Each class was allowed to establish its own commissions dealing with different branches of science. The first members of the Academy were chosen from among the members of the Krakow Learned Society. It was a 12‑person group including only local members, approved by the Emperor. It was also them who elected the first President of the Academy, Józef Majer, and the Secretary General, Józef Szujski, from this group. By the end of 1872, the organization of the Academy of Arts and Sciences in Krakow was completed. It had its administration, management and three classes that were managed by the respective directors and secretaries. It also had three commissions, taken over from the Krakow Learned Society, namely: the Physiographic Commission, the Bibliographic Commission and the Linguistic Commission. At that time, the Academy had only a total of 24 active members who had the right
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Pediatrics in the year 2020 and beyond: preparing for plausible futures.
Starmer, Amy J; Duby, John C; Slaw, Kenneth M; Edwards, Anne; Leslie, Laurel K
2010-11-01
Although the future of pediatrics is uncertain, the organizations that lead pediatrics, and the professionals who practice within it, have embraced the notion that the pediatric community must anticipate and lead change to ultimately improve the health of children and adolescents. In an attempt to proactively prepare for a variety of conceivable futures, the board of directors of the American Academy of Pediatrics established the Vision of Pediatrics 2020 Task Force in 2008. This group was charged to think broadly about the future of pediatrics, to gather input on key trends that are influencing the future, to create likely scenarios of the future, and to recommend strategies to best prepare pediatric clinicians and pediatric organizations for a range of potential futures. The work of this task force led to the development of 8 "megatrends" that were identified as highly likely to have a profound influence on the future of pediatrics. A separate list of "wild-card" scenarios was created of trends with the potential to have a substantial influence but are less likely to occur. The process of scenario-planning was used to consider the effects of the 8 megatrends on pediatrics in the year 2020 and beyond. Consideration of these possible scenarios affords the opportunity to determine potential future pediatric needs, to identify potential solutions to address those needs, and, ultimately, to proactively prepare the profession to thrive if these or other future scenarios become realities.
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Watson, Nathaniel F.; Badr, M. Safwan; Belenky, Gregory; Bliwise, Donald L.; Buxton, Orfeu M.; Buysse, Daniel; Dinges, David F.; Gangwisch, James; Grandner, Michael A.; Kushida, Clete; Malhotra, Raman K.; Martin, Jennifer L.; Patel, Sanjay R.; Quan, Stuart F.; Tasali, Esra
2015-01-01
The American Academy of Sleep Medicine and Sleep Research Society recently released a Consensus Statement regarding the recommended amount of sleep to promote optimal health in adults. This paper describes the methodology, background literature, voting process, and voting results for the consensus statement. In addition, we address important assumptions and challenges encountered during the consensus process. Finally, we outline future directions that will advance our understanding of sleep n...
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International Nuclear Information System (INIS)
Schenker, Matthew A; Ellis, Richard S; Konidaris, Nick P; Stark, Daniel P
2013-01-01
Earlier work has raised the potential importance of nebular emission in the derivation of the physical characteristics of high-redshift Lyman break galaxies. Within certain redshift ranges, and especially at z ≅ 6-7, such lines may be strong enough to reduce estimates of the stellar masses and ages of galaxies compared with those derived assuming the broadband photometry represents stellar light alone. To test this hypothesis at the highest redshifts where such lines can be probed with ground-based facilities, we examine the near-infrared spectra of a representative sample of 28 3.0 < z < 3.8 Lyman break galaxies using the newly commissioned MOSFIRE near-infrared spectrograph at the Keck I telescope. We use these data to derive the rest-frame equivalent widths (EWs) of [O III] emission and show that these are comparable with estimates derived using the spectral energy distribution (SED) fitting technique introduced for sources of known redshift by Stark et al. Although our current sample is modest, its [O III] EW distribution is consistent with that inferred for Hα based on SED fitting of Stark et al.'s larger sample of 3.8 < z < 5 galaxies. For a subset of survey galaxies, we use the combination of optical and near-infrared spectroscopy to quantify kinematics of outflows in z ≅ 3.5 star-forming galaxies and discuss the implications for reionization measurements. The trends we uncover underline the dangers of relying purely on broadband photometry to estimate the physical properties of high-redshift galaxies and emphasize the important role of diagnostic spectroscopy
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Science Academies Refresher Course on Traditional and Modern
Indian Academy of Sciences (India)
Home; Journals; Resonance – Journal of Science Education; Volume 17; Issue 9. Science Academies Refresher Course on Traditional and Modern Approaches in Plant Taxonomy'. Information and Announcements Volume 17 Issue 9 September 2012 pp 921-921 ...
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Indian Academy of Sciences, Bangalore Indian National Science ...
Indian Academy of Sciences (India)
2009-09-30
.in),. (www.insaindia.org) or (www.nasi.org.in); however a copy of the application together with enclosures must be sent by post to The Coordinator, Science Education Programme, Indian. Academy of Sciences, C.V. Raman ...
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Ruane, G.; Mawet, D.; Kastner, J.; Meshkat, T.; Bottom, M.; Femenía Castellá, B.; Absil, O.; Gomez Gonzalez, C.; Huby, E.; Zhu, Z.; Jenson-Clem, R.; Choquet, É.; Serabyn, E.
2017-08-01
Distinct gap features in the nearest protoplanetary disk, TW Hya (distance of 59.5 ± 0.9 pc), may be signposts of ongoing planet formation. We performed long-exposure thermal infrared coronagraphic imaging observations to search for accreting planets, especially within dust gaps previously detected in scattered light and submillimeter-wave thermal emission. Three nights of observations with the Keck/NIRC2 vortex coronagraph in L‧ (3.4-4.1 μm) did not reveal any statistically significant point sources. We thereby set strict upper limits on the masses of non-accreting planets. In the four most prominent disk gaps at 24, 41, 47, and 88 au, we obtain upper mass limits of 1.6-2.3, 1.1-1.6, 1.1-1.5, and 1.0-1.2 Jupiter masses (M J), assuming an age range of 7-10 Myr for TW Hya. These limits correspond to the contrast at 95% completeness (true positive fraction of 0.95) with a 1% chance of a false positive within 1″ of the star. We also approximate an upper limit on the product of the planet mass and planetary accretion rate of {M}{{p}}\\dot{M}≲ {10}-8 {M}{{J}}2 {{yr}}-1 implying that any putative ˜0.1 M J planet, which could be responsible for opening the 24 au gap, is presently accreting at rates insufficient to build up a Jupiter mass within TW Hya’s pre-main-sequence lifetime.
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Energy Technology Data Exchange (ETDEWEB)
Mennesson, B.; Serabyn, E.; Colavita, M. M. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena CA 91109-8099 (United States); Absil, O. [Departement d' Astrophysique, Geophysique et Oceanographie, Universite de Liege, 17 Allee du Six Aout, B-4000 Sart Tilman (Belgium); Lebreton, J.; Augereau, J.-C. [IPAG, UMR 5274, CNRS and Universite Joseph Fourier, BP 53, F-38041 Grenoble (France); Millan-Gabet, R. [Michelson Science Center, California Institute of Technology, 770 South Wilson Avenue, Pasadena CA 91125 (United States); Liu, W. [Infrared Processing and Analysis Center, California Institute of Technology, Mail Code 100-22, Pasadena, CA 91125 (United States); Hinz, P. [Steward Observatory, University of Arizona, 933 N Cherry Avenue, Tucson, AZ 85721 (United States); Thebault, P. [Observatoire de Paris, Section de Meudon, F-92195 Meudon Principal Cedex (France)
2013-02-15
We report on high-contrast mid-infrared observations of Fomalhaut obtained with the Keck Interferometer Nuller (KIN) showing a small resolved excess over the level expected from the stellar photosphere. The measured null excess has a mean value of 0.35% {+-} 0.10% between 8 and 11 {mu}m and increases from 8 to 13 {mu}m. Given the small field of view of the instrument, the source of this marginal excess must be contained within 2 AU of Fomalhaut. This result is reminiscent of previous VLTI K-band ({approx_equal}2{mu}m) observations, which implied the presence of a {approx}0.88% excess, and argued that thermal emission from hot dusty grains located within 6 AU from Fomalhaut was the most plausible explanation. Using a parametric two-dimensional radiative transfer code and a Bayesian analysis, we examine different dust disk structures to reproduce both the near- and mid-infrared data simultaneously. While not a definitive explanation of the hot excess of Fomalhaut, our model suggests that the most likely inner few AU disk geometry consists of a two-component structure, with two different and spatially distinct grain populations. The 2-11 {mu}m data are consistent with an inner hot ring of very small ({approx_equal}10-300 nm) carbon-rich grains concentrating around 0.1 AU. The second dust population-inferred from the KIN data at longer mid-infrared wavelengths-consists of larger grains (size of a few microns to a few tens of microns) located further out in a colder region where regular astronomical silicates could survive, with an inner edge around 0.4 AU-1 AU. From a dynamical point of view, the presence of the inner concentration of submicron-sized grains is surprising, as such grains should be expelled from the inner planetary system by radiation pressure within only a few years. This could either point to some inordinate replenishment rates (e.g., many grazing comets coming from an outer reservoir) or to the existence of some braking mechanism preventing the grains
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Pramana – Journal of Physics | Indian Academy of Sciences
Indian Academy of Sciences (India)
Author Affiliations. I N Askerzade1 2. Department of Physics, Ankara University, Tandogan 06100, Ankara, Turkey; Institute of Physics, Azerbaijan National Academy of Sciences, Baku 370143, Azerbaijan ...
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The influence of leadership on morale at the United States Naval Academy
Miller, Christopher A.
2006-01-01
The purpose of this thesis is to quantitatively analyze the relationship between midshipmen leadership and morale at the United States Naval Academy. The goal is to determine if there is a specific set of leadership characteristics that directly contribute to positive company morale within the Brigade of Midshipmen. The study is quantitative and uses the Naval Academy Brigade Climate survey as its primary instrument. The results of this effort indicate that leadership characteristics that are...
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Journal of Genetics | Indian Academy of Sciences
Indian Academy of Sciences (India)
Joint Laboratory of the Hungarian Academy of Sciences and the Semmelweis University Budapest, Szentkirályi u. 46., H-1085 Budapest, Hungary; Department of Histology and Embryology, University School of Medicine, ul. Chalubińskiego 6a, 50-356 Wroclaw, Poland; Joint Research Laboratory for Pediatrics and ...
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Sagar Sengupta | Speakers | Indian Academy of Sciences
Indian Academy of Sciences (India)
Sagar Sengupta. Sagar Sengupta. NII, New Delhi. Sagar Sengupta is Staff Scientist at National Institute of Immunology, New Delhi. He is a Fellow of all three National Science Academies in India. He is a recipient of the 2011 National Bioscience Award for Career Development by Department of Biotechnology, India.
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Journal of Chemical Sciences | Indian Academy of Sciences
Indian Academy of Sciences (India)
Surface Engineering & Tribology Group, CSIR-Central Mechanical Engineering Research Institute, Mahatma Gandhi Avenue, Durgapur 713 209, India; Academy of Scientific and Innovative Research(AcSIR), CSIR-Central Mechanical Engineering Research Institute (CMERI) campus, Mahatma Gandhi Avenue, Durgapur ...
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Aping the Ape: Kafka's "Report to an Academy"
Directory of Open Access Journals (Sweden)
Ziad Elmarsafy
1995-06-01
Full Text Available The "Report to an Academy" narrates a curious situation: an ape presents (or rather, performs a report to an academy. What he presents is an autobiography. Like so much in Kafka, the "Report" is a parable about writing in general and about the writer's identity in particular. This essay attempts to address these issues through a close reading of Kafka's text against Blanchot's L'espace littéraire . Central to this endeavour is an analysis of the ape's use of the first-person pronoun as someone who fashions himself while, at the same time, presenting a theatrical autobiography featuring the self in question. My reading then moves on to analyze the act of writing as a negotiation of the passage between self and other, framed as it is by the theatrical context of Kafka's parable.
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Bulletin of Materials Science | Indian Academy of Sciences
Indian Academy of Sciences (India)
Transparent conducting amorphous p-type CuFeO 2 (CFO) thin film was ... Key Lab of Novel Thin Film Solar Cells, Chinese Academy of Sciences, Hefei 230031, China; University of Science and Technology of China, Hefei 230026, China ...
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School 2.0: The Science Leadership Academy
Lehmann, Christopher
2007-01-01
This article features the Science Leadership Academy, a new public partnership school in Philadelphia that incorporates core values of inquiry, research, collaboration, presentation, and reflection. Founded by the School District of Philadelphia and The Franklin Institute, SLA is one of four partnership high schools that opened in September 2006…
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Science Academies' Refresher Course in Experimental Physics
Indian Academy of Sciences (India)
2017-12-18
Dec 18, 2017 ... laws and principles and yield reasonably accurate results. The Refresher Course is jointly spon- sored by the Indian Academy of Sciences, ... Selected participants will be provided local hospitality during the Course in addition to course material. Outstation participants will be given three-tier A/c train fare.
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Resonance – Journal of Science Education | Indian Academy of ...
Indian Academy of Sciences (India)
37th International Mathematical Olympiad / Indian Statistical Institute · More Details .... Instructional School on Linear Algebra - Sponsored by Indian Academy of Sciences ...... Refresher Course on Mountain Hydrology and Climate Change.
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Journal of Earth System Science | Indian Academy of Sciences
Indian Academy of Sciences (India)
Solute transport; convection–dispersion equation; boundary layer theory; ... to convection–dispersion equation (CDE) based on boundary layer theory has been ... Sciences and Natural Resources Research, Chinese Academy of Sciences, ...
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Khan Academy ehk Kuidas õppeaineid integreeriti / Kärt Matiisen
Matiisen, Kärt
2012-01-01
Kose gümnaasiumi 7. klassi matemaatikarühma uute õppemeetodite leidmise projektist ja erinevate õppeainete integreerimisest, mille käigus loodi subtiitrid Khan Academy ingliskeelsetele matemaatika õppetükkidele