The GALEX Arecibo SDSS Survey (GASS)
was a survey of HIemissions
from over a thousand galaxies.
Galaxies were chosen from SDSS and GALEX,
so that cross correlations can be made.
Observations were made in 2008-2009 at Arecibo,
using the 21-cm line to detect HI.
Three data releases followed, the final one 2013.
A later extension covering over a thousand additional galaxies was
xGASS (for Extended GALEX Arecibo SDSS Survey).
Follow-up surveys estimating galaxies' molecular hydrogen
were COLD GASS and xCOLD GASS.