Hubble Galaxy at Redshift z = 0.65

About the data

The science findings are based on various Hubble archival observations of galaxy surveys, including COSMOS, CDF–S, UDS, GOODS, and CANDELS.

The images were created from Hubble data from proposal 12060 , PIs: S. Faber (University of California, Santa Cruz) and H. Ferguson (STScI), et al.

The science team includes: C. Papovich (Mitchell Inst./Texas A&M U.), I. Labbé (Leiden Obs.), R. Quadri and V. Tilvi (Mitchell Inst./Texas A&M U.), E.F. Bell (U. Michigan, Ann Arbor), K. Glazebrook (CAS/Swinburne U.), L. Spitler (Macquarie U., Sydney/ AAO), C.M.S. Straatman (Leiden Obs.), K.-V. Tran (Mitchell Inst./Texas A&M U.), P. Behroozi (STScI), M. Cowley (CAS/Swinburne U.), R. Davé (U. Western Cape/South African Astronomical Obs./African Inst. for Mathematical Sciences, Cape Town), A. Dekel (Hebrew U. of Jerusalem), M. Dickinson (NOAO), H.C. Ferguson (STScI), S.L. Finkelstein (U. Texas, Austin), E. Gawiser (Rutgers U.), H. Inami (NOAO), G. Kacprzak (CAS/Swinburne U.), L. Kawinwanichakij (Mitchell Inst./Texas A&M U.), D. Kocevski (U. Kentucky), A. Koekemoer (STScI), D. Koo (Lick Obs./U. California, Santa Cruz), P. Kurczynski (Rutgers U.), J.M. Lotz (STScI), Y. Lu (Kavli Institute/Stanford U.), R.A. Lucas (STScI), D. Mcintosh (U. Missouri, Kansas City), N. Mehrtens (Mitchell Inst./Texas A&M U.), B. Mobasher (U. California, Riverside), A. Monson (Carnegie Obs.), G. Morrison (IfA/U. Hawaii/CFHT), T. Nanayakkar (CAS/Swinburne U.), S.E. Persson (Carnegie Obs.), B. Salmon (Mitchell Inst./Texas A&M U.), R. Simons (JHU), A. Tomczak (Mitchell Inst./Texas A&M U.), P. van Dokkum (Yale U.), B. Weiner (Steward Obs./U. Arizona), and S.P. Willner (Harvard-Smithsonian Center for Astrophysics).