xGASS catalog : J/MNRAS/476/875


Authors : Catinella B. orcid , Saintonge A., Janowiecki S. (hide) , Saintonge A., Janowiecki S. et..al

Bibcode : 2018MNRAS.476..875C (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Galaxies, radio; H I data
UAT : Radio galaxies, H I line emission

Observation (OC)

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Inserted into VizieR : 26-Feb-2021
Last modification : 18-Aug-2024

xGASS total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe. (2018)

Keywords : galaxies evolution - galaxies: fundamental parameters - galaxies: ISM - radio lines: galaxies

Abstract:We present the extended GALEX Arecibo SDSS Survey (xGASS), a gas fraction-limited census of the atomic hydrogen (HI) gas content of 1179 galaxies selected only by stellar mass (M*=10^9^-10^11.5^M_{sun}_) and redshift (0.01<z<0.05). This includes new Arecibo observations of 208 galaxies, for which we release catalogues and HI spectra. In addition to extending the GASS HI scaling relations by one decade in stellar mass, we quantify total (atomic+molecular) cold gas fractions and molecular-to-atomic gas mass ratios, Rmol, for the subset of 477 galaxies observed with the IRAM 30m telescope. We find that atomic gas fractions keep increasing with decreasing stellar mass, with no sign of a plateau down to logM*/M_{sun}_=9. Total gas ...(more)
Abstract: (hide)
We presented xGASS, the culmination of several years of effort to gather deep HI observations for a stellar mass-selected sample of ~1200 galaxies with homogeneously measured optical and SF properties. xGASS is the combination of the original GASS survey, which started in 2008 and targeted galaxies with stellar masses larger than 10^10^M_{sun}_, and its extension to M*=10^9^M_{sun}_. Together, these surveys required ~1300h of Arecibo telescope time. Our unique approach of carrying out gas fraction-limited observations down to MHI/M*~2 per cent allowed us to obtain stringent upper limits, which are essential to interpret variations of gas content as a function of galaxy properties.


                
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