PPT-WFIRST

Instrument reference information July 1 2015 The information in this file is excerpted from the SDT report dated March 10 2015 Spergel et al arXiv150303757 and from the February 13 2015 SDT briefing to Paul Hertz Both are accessible from the WFIRST site . Figure 1. Fruit • HO-46-WFirst Season’s Care Page 2 of 3 Purdue University Cooperative Extension Service Revised 12/01 Fruit • HO-46-W Mulching After plants have become dormant, wh 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 . -- Preliminary “existence proof”. Qian Gong & 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. Figure of Merit . David . Bennett. University of Notre Dame. WFIRST. WFIRST Microlensing Figure of Merit. Primary FOM1 - # of planets detected for a particular mass and separation range. Cannot be calculated analytically – must be simulated. 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. Status Report -- . ExoPAG. Feng Zhao. AFTA Coronagraph Instrument Manager. 1/5 2014. 1. Copyright 2013 California Institute of Technology. Government sponsorship acknowledged. Outline. Introduction. Newly selected architecture description. Is . cosmic acceleration . caused by . a new energy component or by . the breakdown . of General Relativity (GR) . on cosmological . scales. ?. If . the cause is a new . energy component. , is its energy density . Measurement Method. Aparna. Bhattacharya. NASA GSFC, Notre Dame, UMBC. Collaborator. : . David Bennett. . J.Anderson. , . N. . Koshimoto. ,. V.Batista. , J.-P. Beaulieu, . I.A.Bond. , . A.Gould. , . 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. David . Spergel. Princeton University. Center for Computational Astrophysics, Flatiron Institute. Outline. Next generation CMB experiments: Simons Observatory CMB-S4. Next generation optical/IR surveys: WFIRST. Status Report -- . ExoPAG. Feng Zhao. AFTA Coronagraph Instrument Manager. 1/5 2014. 1. Copyright 2013 California Institute of Technology. Government sponsorship acknowledged. Outline. Introduction. Newly selected architecture description. California Institute of Technology. Copyright 2011 California Institute of Technology. Government sponsorship acknowledged.. The Missions. Euclid. Mapping the geometry of the Dark Universe. . 2004. : Dark Universe Mission proposed as a Theme to ESA’s Cosmic Vision programme.