4.6 Article

A CATALOG OF BULGE plus DISK DECOMPOSITIONS AND UPDATED PHOTOMETRY FOR 1.12 MILLION GALAXIES IN THE SLOAN DIGITAL SKY SURVEY

Journal

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 196, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0067-0049/196/1/11

Keywords

galaxies: evolution; galaxies: fundamental parameters

Funding

  1. Natural Science and Engineering Research Council of Canada
  2. Canadian Foundation for Innovation
  3. British Columbia
  4. Alfred P. Sloan Foundation
  5. National Aeronautics and Space Administration
  6. National Science Foundation
  7. U.S. Department of Energy
  8. Japanese Monbukagakusho
  9. Max Planck Society

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We perform two-dimensional, point-spread-function-convolved, bulge+disk decompositions in the g and r bandpasses on a sample of 1,123,718 galaxies from the Legacy area of the Sloan Digital Sky Survey Data Release Seven. Four different decomposition procedures are investigated which make improvements to sky background determinations and object deblending over the standard SDSS procedures that lead to more robust structural parameters and integrated galaxy magnitudes and colors, especially in crowded environments. We use a set of science-based quality assurance metrics, namely, the disk luminosity-size relation, the galaxy color-magnitude diagram, and the galaxy central (fiber) colors to show the robustness of our structural parameters. The best procedure utilizes simultaneous, two-bandpass decompositions. Bulge and disk photometric errors remain below 0.1 mag down to bulge and disk magnitudes of g similar or equal to 19 and r similar or equal to 18.5. We also use and compare three different galaxy fitting models: a pure Sersic model, an n(b) = 4 bulge + disk model, and a Sersic (free n(b)) bulge + disk model. The most appropriate model for a given galaxy is determined by the F-test probability. All three catalogs of measured structural parameters, rest-frame magnitudes, and colors are publicly released here. These catalogs should provide an extensive comparison set for a wide range of observational and theoretical studies of galaxies.

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