4.6 Article

The GALEX Arecibo SDSS Survey VI. Second data release and updated gas fraction scaling relations

Journal

ASTRONOMY & ASTROPHYSICS
Volume 544, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201219261

Keywords

galaxies: fundamental parameters; ultraviolet: galaxies; radio lines: galaxies; surveys; catalogs

Funding

  1. National Science Foundation [AST-1100968]
  2. Ana G. Mendez-Universidad Metropolitana
  3. Universities Space Research Association
  4. Alfred P. Sloan Foundation
  5. National Science Foundation
  6. US Department of Energy
  7. National Aeronautics and Space Administration
  8. Japanese Monbukagakusho
  9. Max Planck Society
  10. Higher Education Funding Council for England

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We present the second data release from the GALEX Arecibo SDSS Survey (GASS), an ongoing large Arecibo program to measure the Hi properties for an unbiased sample of similar to 1000 galaxies with stellar masses greater than 10(10) M-circle dot and redshifts 0.025 < z < 0.05. GASS targets are selected from the Sloan Digital Sky Survey (SDSS) spectroscopic and Galaxy Evolution Explorer (GALEX) imaging surveys, and are observed until detected or until a gas mass fraction limit of a few per cent is reached. This second data installment includes new Arecibo observations of 240 galaxies, and marks the 50% of the complete survey. We present catalogs of the HI, optical and ultraviolet parameters for these galaxies, and their Hi-line profiles. Having more than doubled the size of the sample since the first data release, we also revisit the main scaling relations of the Hi mass fraction with galaxy stellar mass, stellar mass surface density, concentration index, and NUV-r color, as well as the gas fraction plane introduced in our earlier work.

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