PPT-Developing WFIRST Exoplanet Mass

Measurement Method Aparna Bhattacharya NASA GSFC Notre Dame UMBC Collaborator David Bennett JAnderson N Koshimoto VBatista JP Beaulieu IABond AGould . only 2 50-day observing windows per year. The bulge must be observed whenever it can be. Significant “edge effect” penalties for regular interruptions. 0.5 year . SNe. program. Must sample high-. 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. PUMP How the magnetic sector mass spectrograph works: qvB = mv), B the magnetic field, m is the mass of the Classically, the speed of the ion, v, is related 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. 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 . At SDT7 3/1-2/2012 consensus for concepts w/out overlap w/ other mission, aka “DRM2” was:. 1.1m aperture, unobscured three. mirror anastigmat telescope. Single. channel instrument. Imaging. with filter wheel. ). 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. 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. Atomic Mass. What is an elements atomic mass?. The weighted average of its naturally occurring isotopes. .. When looking at an element on the periodic table of elements, where is atomic mass found?. Usually the top left hand corner of each elements box. However, on the periodic table that you will use for your AP Exam(s), this number will be located below each elements chemical symbol.. Jennifer Yee. &. Etienne . Bachelet. Big Picture. Using simulated WFIRST light curves, explore the kinds of . microlensing. planets WFIRST will find.. Goals. Identify planetary perturbations in light curves.