Mariangela Bernardi et al. 2003 The Astronomical Journal 125 1849 doi:10.1086/374256
Mariangela Bernardi1,2, Ravi K. Sheth3,4, James Annis3, Scott Burles3, Daniel J. Eisenstein5, Douglas P. Finkbeiner6,7,8, David W. Hogg9, Robert H. Lupton7, David J. Schlegel7, Mark SubbaRao1, Neta A. Bahcall7, John P. Blakeslee10, J. Brinkmann11, Francisco J. Castander12,13, Andrew J. Connolly4, István Csabai10,14, Mamoru Doi15,16, Masataka Fukugita17,18, Joshua Frieman1,3, Timothy Heckman10, Gregory S. Hennessy19, Željko Ivezić7, G. R. Knapp7, Don Q. Lamb1, Timothy McKay20, Jeffrey A. Munn19, Robert Nichol2, Sadanori Okamura15,21, Donald P. Schneider22, Aniruddha R. Thakar10 and Donald G. York1
Show affiliationsA magnitude-limited sample of nearly 9000 early-type galaxies, in the redshift range 0.01 ≤ z ≤ 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. The sample was used to study how early-type galaxy observables, including luminosity L, effective radius Ro, surface brightness Io, color, and velocity dispersion σ, are correlated with one another. Measurement biases are understood with mock catalogs that reproduce all of the observed scaling relations and their dependences on fitting technique. At any given redshift, the intrinsic distribution of luminosities, sizes, and velocity dispersions in our sample are all approximately Gaussian. A maximum likelihood analysis shows that σ ∝ L0.25±0.012, Ro ∝ L0.63±0.025, and Ro ∝ I-0.75±0.02 in the r* band. In addition, the mass-to-light ratio within the effective radius scales as Mo/L ∝ L0.14±0.02 or Mo/L ∝ M
, and galaxies with larger effective masses have smaller effective densities: Δo ∝ M
. These relations are approximately the same in the g*, i*, and z* bands. Relative to the population at the median redshift in the sample, galaxies at lower and higher redshifts have evolved only little, with more evolution in the bluer bands. The luminosity function is consistent with weak passive luminosity evolution and a formation time of about 9 Gyr ago.
galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: fundamental parameters; galaxies: photometry; galaxies: stellar content
Issue 4 (2003 April)
Received 2002 September 27, accepted for publication 2003 January 23
Mariangela Bernardi et al. 2003 The Astronomical Journal 125 1849
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