AAS 201st Meeting, January, 2003
Session 52. Galaxy Evolution and Surveys: Observations and Interpretation
Poster, Tuesday, January 7, 2003, 9:20am-6:30pm, Exhibit Hall AB

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[52.07] Evolution of Field Galaxies from 0.5 < z < 1.0 in ACS GTO Cluster Fields

N. Cross, N. Ben\'itez (JHU), C. Gronwall (Pennsylvania State Univ.), J.P. Blakeslee, F. Menanteau (JHU), R. Bouwens (UCO/Lick Observatory), D.R. Ardila (JHU), F. Bartko (Bartko Sci. & Tech.), T.J. Broadhurst (Racah Inst. Physics, Hebrew U.), R.A. Brown, C. Burrows (STScI), E. Cheng (GSFC), M. Clampin (STScI), P.D. Feldman, H.C. Ford (JHU), M. Franx (Leiden Obs.), D.A. Golimowski (JHU), G. Hartig (STScI), G.D. Illingworth (UCO/Lick Obs.), L. Infante (Pontificia Univ. Catolica de Chile), R.A. Kimble (GSFC), J. Krist (STScI), M. Lesser (Steward Obs.), A.R. Martel, G.R. Meurer (JHU), G. Miley (Leiden Obs.), M. Postman (STScI), P. Rosati (ESO), M. Sirianni (JHU), W.B. Sparks (STScI), H.D. Tran, Z.I. Tsvetanov (JHU), R.L. White (STScI), W. Zheng (JHU), ACS Science Team

We present data from the ACS Science Team demonstrating how galaxies evolve in terms of luminosity, scale-size, morphological type and color in the range 0.5 <z< 1.0. The galaxies are foreground or background galaxies from clusters imaged by ACS in GTO time. We will show the bivariate space density for each combination of luminosity, scale-size, morphological type and color. Finally we will measure the changes in these distributions with redshift.

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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.