Skip to content

The Broad-band Optical Properties of Galaxies with Redshifts 0.0 < z < 0.2

M. R. Blanton, D. W. Hogg, N. A. Bahcall, I. K. Baldry, J. Brinkmann, I. Csabai, D. J. Eisenstein, M. Fukugita, J. E. Gunn, Z. Ivezic, D. Q. Lamb, R. H. Lupton, J. Loveday, J. A. Munn, R. C. Nichol, S. Okamura, D. J. Schlegel, K. Shimasaku, M. A. Strauss, M. S. Vogeley, D. H. Weinberg

astro-pharXiv:astro-ph/0209479

Abstract

Using photometry and spectroscopy of 144,609 galaxies from the Sloan Digital Sky Survey, we present bivariate distributions of pairs of seven galaxy properties: four optical colors, surface brightness, radial profile shape as measured by the Sersic index, and absolute magnitude. In addition, we present the dependence of local galaxy density (smoothed on 8 h-1 Mpc scales) on all of these properties. Several classic, well-known relations among galaxy properties are evident at extremely high signal-to-noise ratio: the color-color relations of galaxies, the color-magnitude relations, the magnitude-surface brightness relation, and the dependence of density on color and absolute magnitude. We show that most of the i-band luminosity density in the universe is in the absolute magnitude and surface brightness ranges used. Some of the relationships between parameters, in particular the color--magnitude relations, show stronger correlations for exponential galaxies and concentrated galaxies taken separately than for all galaxies taken together. We provide a simple set of fits of the dependence of galaxy properties on luminosity for these two sets of galaxies.

Create a lesson