Most Distant Galaxy Candidates in the Hubble Ultra Deep Field
HUDF, Ultra deep field
The image is 3 arcminutes square.
This image was created from HST data from the following proposal: 9978:: HUDF Team (STScI). The science teams are:
— A.J. Bunker (Univ.of Exeter U.K./ Inst. of Astrophysics, Univ. of Cambridge, U.K.), E.R. Stanway (Inst. of Astrophysics, Univ. of Cambridge, U.K.), R.S. Ellis (California Inst. of Tech.), and
R.G. McMahon (Inst. of Astrophysics, Univ. of Cambridge, U.K.)
— M. Stiavelli, S. M. Fall, and N. Panagia (STScI)
— H. Yan (Spitzer Science Center, California Inst. of Tech.) and R.A. Windhorst (Arizona State Univ.)
— R.J. Bouwens and G.D. Illingworth (Univ. of California, Santa Cruz), R.I. Thompson (Steward Obs./Univ. of Arizona), J.P. Blakeslee (Johns Hopkins Univ.), M.E. Dickinson (National Optical Astronomy Obs.), T.J. Broadhurst (The Hebrew Univ., Israel), D.J. Eisenstein and X. Fan (Steward Obs./Univ. of Arizona), M. Franx (Leiden Observatory, Netherlands), G. Meurer (Johns Hopkins Univ.), and P. van Dokkum (Yale Univ.)
— S. Malhotra, J.E. Rhoads, N. Pirzkal and C. Xu (STScI)
F435W (B), F606W (V), F775W (i), F850LP (z)
Blue: F435W (B)
Green: F606W (V), F775W (i)
Red: F850LP (z)
NASA, ESA, R. Windhorst (Arizona State University) and H. Yan (Spitzer Science Center, Caltech)