PPT-Status of the Evaluated Gamma-ray Activation File (EGAF)

Richard B Firestone Lawrence Berkeley National Laboratory Berkeley CA 94720 About EGAF The EGAF database is the result of an IAEA CRP to evaluate thermal neutron capture cross sections s g. Overview. Key Data. Grant Agreement . n°. 312382. Starting date: 1. st. September 2013. Duration: 48 months (end date 31. st. August 2017). Total Budget: 14.837.981 euro. Consortium Composition. BUS 374. D. r. Rajiv Krishnan Kozhikode. Reputation: Quality expectations based on accumulated evidence of past demonstration of quality. Status: Quality expectations based on network of affiliations in an exchange network. 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . Opening in the lens. Aperture. f-number or stop. = focal length/Aperture diameter. Each stop represents either half or double the amount of light exposing the film or chip. The circle of confusion is defined as the largest blur spot that is indistinguishable from the point source that is being rendered. . Polarimeter. for Solar flares . (. GRIPS. ). Recently funded NASA LCAS balloon mission. 3D position-sensitive germanium spectrometer. High spectral resolution (~2 keV FWHM at 662 keV). Compton-scatter track reconstruction. Manel. Martinez. 4. 3. rd. . Winter Meeting. March 2015-Benasque. Outline. 1) Introduction. 2) Basics on VHE Gamma Astronomy physics. 3) VHE gamma observatories. 4) CTA. 5. ) Conclusions. 1) INTRODUCTION. Haoyuan. Li. UC Berkeley . Outline. Outline. . |. . Motivation| . Design | . Results| Status| Future. Motivation. System Design. Evaluation Results. Release Status. Future Directions. Outline| . Motivation. BUS 374. D. r. Rajiv Krishnan Kozhikode. Reputation: Quality expectations based on accumulated evidence of past demonstration of quality. Status: Quality expectations based on network of affiliations in an exchange network. January 17, 2012. Signal arrives. Activation. How long?. For . efficent. simulation:. Cumulative Distribution . Function. F(t. ) = probability that the activation time is ≤ . t. Project Goal. Using a CDF. By Cary Grant from. and. James Schwartz. Why yet another session on Model Review?. Why are we hearing about model review again at another User Group? Maybe since some have not heard about it and the topic values a bit of repetition, plus there are some new twists that have been added.. These statements have not been evaluated by the Food and Drug Administration These products are not intended to diagnose treat cure or prevent any disease Always consult your doctor before taking any . Matthew Erenpreiss. Ohio Department of Natural Resources. Division of Geological Survey. Utica . Shale Play Book Study Workshop. Canonsburg, PA. July 14, 2015. Outline. Background. Spectral Gamma-Ray Scanner. Francesco Loparco*. Salvatore De Gaetano, Mario Nicola . Mazziotta. . on behalf of the Fermi LAT Collaboration. *e-mail: francesco.loparco@ba.infn.it. The gamma-ray Moon. 1. The Moon is among the brightest sources in the gamma-ray sky. Flashes. Gamma Ray . Astronomy. . Beginning. started . as a small budget research program in 1959. monitor. ing. compliance with the 1963 Partial Test Ban Treaty by the Soviet Union, and other nuclear-capable states.