PPT-WFIRST IFU

Preliminary existence proof Qian Gong amp Dave Content GSFC optics branch Code 551 summary Started work last summer on an existence proof IFU for IDRM Could work equally well for DRM1 or DRM2. Microlensing. Planetary Systems.. Scott Gaudi. Matthew Penny. (OSU). WFIRST . Microlensing. Survey.. Microlensing. Survey Dataset. . Properties.. . ~. 3. sq. deg.. ~432 days.. ~80% of the area will have 2 million seconds of integration time.. NASA’s . Dark Energy Program. Linda . Sparke. (NASA HQ) . January 5, 2014. PhysPAG. @ AAS. © . 2013, . government sponsorship acknowledged. . 2004:. Dark Universe Mission Theme proposed to ESA’s Cosmic Vision programme. Chris Hirata. May 10, . 2011. f. or the /. usr. /WFIRST/HLS/WL group. General Notes. Exposure Time Calculations. Maturity greatly improved from previous version, with some losses. Assumed for numbers presented here: WFIRST 1c configuration. This is . Instrument. reference information. July. . 1, . 2015. The information in this file is excerpted from the SDT report dated March 10, 2015 (. Spergel. et al. arXiv:1503.03757) and from the February 13, 2015 SDT briefing to Paul Hertz. Both are accessible from the WFIRST site: . Imaging Science with the WFIRST Coronagraph. AAS Conference 2015. N. Jeremy Kasdin. Bruce Macintosh, Olivier . Guyon. , Tom Green, Wes . Traub. , Jim . Breckinridge. and. The WFIRST/AFTA Coronagraph Engineering team. . Chris Haines . (Universidad de Chile). Paula . Merluzzi. , Gianni . Busarello. , . Amata. . Mercurio. . (Naples). , . Nobuhiro. Okabe . (IPMU). , Luis . Campusano. . (. U.Chile. ). ESO: Dissecting Galaxies Near and Far, 26th March 2015. ). Presentation to P. Hertz April 19, 2013. . Neil . Gehrels. (GSFC). SDT . Co-Chair. David . Spergel. (Princeton) . . SDT Co-Chair. Kevin Grady (GSFC) Study Manager . & . Project Team. Perspective. 2020?. 2013. 2004. Ichi . Tanaka. Subaru Telescope. Preface. Question:“. How you want to use 8-m Telescope . in 2020s when TMT/GMT/JWST/WISH . etc are there?”. “Attractiveness” of the instrument itself is the key for success.. with WFIRST . DRM1 and DRM2. C Baltay. June 1, 2012. Supernova Surveys . using . Slitless. Spectroscopy. Use Imager for . SNe. discovery and to get . lightcurves. Use . slitless. spectroscopy to type supernovae and get redshifts. The Ohio State University. (with the WFIRST SDTs and on behalf of the WFIRST . μSIT. ). Completing the Census of . Exoplanetary. Systems . with WFIRST.. 21. st. International . Microlnesing. Conference. Cynthia Spry, MA,MS,RN,CNOR(E),CSPDT. Independent Consultant. 1. Disclosure. 3M. Aesculap. Boston Scientific. Ecolab. oneSource. IMS. 2. Objectives. Identify the current focus on instructions for use (IFU). IFU Performance requirement document XIFU-RD-SYS-00278-CNES 2.0 [RD2] Athena Science Requirement Document Athena_SciRd_v2.1_20180625 2.1 [RD3] On the Athena effective area science requirements at 7 a 15Weillustratetheuseofrevisiondiagramsbypresentingtwooperationalsystemmodelsusingasingleserverandaserverpoolrespectively2FormulationTogetstartedweneedtoestablishsomepreciseterminologyPer-hapsthevery2r www.drsvenkatesan.com. Dr.S.Venkatesan. MD. Professor of cardiology. Madras medical college . Chennai.India. .. www.drsvenkatesan.com. www.drsvenkatesan.com. www.drsvenkatesan.com. History of Erosions.