Evolution of Field Galaxies from 0.5 < z < 1.0 in ACS GTO Cluster Fields
Cross, N., Benitez, N., Gronwall, C., Blakeslee, J.P., Menanteau, F., Bouwens, R., Ardila, D.R., Bartko, F., Broadhurst, T.J., Brown, R.A., Burrows, C., Cheng, E., Clampin, M., Feldman, P.D., Ford, H.C., Franx, M., Golimowski, D.A., Hartig, G.F., Illingworth, G.D., Infante, L., Kimble, R.A., Krist, J.E., Lesser, M., Martel, A.R., Meurer, G.R., Miley, G., Postman, M., Rosati, P., Sirianni, M., Sparks, W.B., Tran, H.D, Tsvetanov, Z.I., White, R.L., and Zheng, W.
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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