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Prospects for Galaxy Clusters and AGN with WFIRST Gillian Wilson (UC Riverside) + Ian Dell’Antonio, Mark Lacy, Douglas Clowe, Megan Donahue, Ranga Ram Chary, Marc Postman, Gus Evrard, Priya Natarajan, Jane Rigby, Elena Pierpaoli, Keiichi Umetsu, Tod Lauer, Massimo MenegheM, Michael Cooper Features of Clusters Bullet Cluster Clowe+04 •  Nearly representa?ve census of maBer (gas, stars, dark maBer) within ~10 Mpc scales •  Host the most massive galaxies and supermassive black holes •  Natural laboratories for studying high-‐density galaxy environments (100s-‐1000s) Why WFIRST will Revolu’onize Cluster Science: 1) Resolu?on •  Higher resolu?on than LSST/Euclid The CLASH HST Gallery A383 (0.189)" A209 (0.209)" A1423 (0.214)" A2261 (0.224)" RXJ2129 (0.234)" A611 (0.288)" MS2137 (0.315)" RXJ2248 (0.348)" MACS1931 (0.352)" MACS1115 (0.353)" RXJ1532 (0.363)" MACS1720 (0.391)" MACS0416 (0.396)" MACS0429 (0.399)" MACS1206 (0.440)" MACS0329 (0.450)" RXJ1347 (0.451)" MACS1311 (0.494)" MACS1149 (0.544)" MACS1423 (0.545)"MACS0717 (0.548)" MACS2129 (0.570)"MACS0647 (0.591)"MACS0744 (0.686)" CLJ1226 (0.890)" 25 clusters at 0.2 < z < 0.9 Postman+12 Why WFIRST will Revolu’onize Cluster Science: 2) Large FOV •  Higher resolu?on than LSST/Euclid •  Larger field of view than HST/JWST CLASH Ensemble Mass Profile Umetsu+15 At z < 0.5, HST and JWST don’t give you virial radius in single poin?ng WFIRST wide-‐field imaging will allow HST-‐level PSF and galaxy densi?es over ~degree scales Subaru FOV WFIRST FOV Umetsu+12 MACSJ1206.2-‐0847 z=0.44 Why WFIRST will Revolu’onize Cluster Science: 2) Large FOV •  HLS will return CLASH-‐depth for 40,000 clusters extending far beyond virial radius •  GO Program could do Fron?er Field-‐depth for >100 clusters Why WFIRST will Revolu’onize Cluster Science: 3) Can Discover Clusters at z > 1 •  Higher resolu?on than LSST/Euclid •  Larger field of view than HST/JWST •  Low sky background in space SpARCS J003645-441050 SpARCS J161314+564930 SpARCS J003442-430753 z = 0.869 z = 0.871 z = 0.867 Ten clusters at z~1 from Spitzer SpARCS near-‐IR SpARCS J021524-034331 SpARCS J104737+574137 SpARCS J105111+581803 z = 1.004 z = 0.956 V5A7K6" z = 1.035 selected survey Wilson+09, Muzzin +09 SpARCS J161641+554513 SpARCS J163435+402151 SpARCS J163852+403843 SpARCS J003550-431224 z = 1.157 z = 1.180 z = 1.196 z = 1.335

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Bullet Cluster. Clowe+04. Page 3. Why WFIRST will Revolu onize Cluster Science: 1) Resolulon 25 night Gemini spectroscopic program.

Prospects for Galaxy Clusters and AGN with WFIRST PDF

24 Pages·2016·11.57 MB·English

by Lee Armus

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Bullet Cluster. Clowe+04. Page 3. Why WFIRST will Revolu onize Cluster Science: 1) Resolulon 25 night Gemini spectroscopic program.

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Author:	Lee Armus
Publication Year:	2016
Pages:	24
Language:	English
File Size:	11.57
Format:	PDF
Price:	FREE

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