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Date and Time of the Query: 2019-06-16 T21:40:41 PDT
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For refcode 2002ApJ...571..136I:
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Copyright by American Astronomical Society. Reproduced by permission
2002ApJ...571..136I The DEEP Groth Strip Survey. X. Number Density and Luminosity Function of Field E/S0 Galaxies at z < 1 Myungshin Im, Luc Simard, S. M. Faber, David C. Koo, Karl Gebhardt, Christopher N. A. Willmer, Andrew Phillips, Garth Illingworth, Nicole P. Vogt, and Vicki L. Sarajedini Received 2000 June 9; accepted 2000 November 3 ABSTRACT We present the luminosity function and color-redshift relation of a magnitude-limited sample of 145 mostly red field E/S0 galaxies at z <~ 1 from the DEEP Groth Strip Survey (GSS). Using nearby galaxy images as a training set, we develop a quantitative method to classify E/S0 galaxies based on smoothness, symmetry, and bulge-to-total light ratio. Using this method, we identify 145 E/S0's at 16.5 < I < 22 within the GSS, for which 44 spectroscopic redshifts (z_spec_) are available. Most of the galaxies with spectroscopic redshifts (86%) form a "red envelope" in the redshift-color diagram, consistent with predictions of spectral synthesis models in which the dominant stellar population is formed at redshifts z >~ 1.5. We use the tight correlation between V - I and z_spec_ for this red subset to estimate redshifts of the remaining E/S0's to an accuracy of ~10%, with the exception of a small number (16%) of blue interlopers at low redshift that are quantitatively classified as E/S0's but are not contained within the red envelope. Constructing a luminosity function of the full sample of 145 E/S0's, we find that there is about 1.1-1.9 mag brightening in rest-frame B-band luminosity back to z ~ 0.8 from z = 0, consistent with other studies. Together with the red colors, this brightening is consistent with models in which the bulk of stars in red field E/S0's formed before z_for_ >~ 1.5 and have been evolving rather quiescently, with few large starbursts since then. Evolution in the number density of field E/S0 galaxies is more difficult to measure, and uncertainties in the raw counts and their ratio to local samples might amount to as much as a factor of 2. Within that uncertainty, the number density of red E/S0's to z ~ 0.8 seems relatively static, being comparable to or perhaps moderately less than that of local E/S0's, depending on the assumed cosmology. A doubling of E/S0 number density since z = 1 can be ruled out with high confidence (97%) if {OMEGA}_m_ = 1. Taken together, our results are consistent with the hypothesis that the majority of luminous field E/S0's were already in place by z ~ 1, that the bulk of their stars were already fairly old, and that their number density has not changed by large amounts since then. Subject headings: cosmology: observations - galaxies: evolution - galaxies: luminosity function, mass function
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