Dissecting GAs Stripping Phenomena in galaxies with MUSE (GASP)

GASP (Gas Stripping Phenomena in galaxies) is an ESO Large Program (196.B-0578) using MUSE in wide-field mode with natural seeing to study a sample of 144 galaxies at z=0.04-0.07 in different environments. The release includes reduced data cubes and fits images with maps of Hα and Hβ emission-line fluxes, Hα radial velocity, average star formation rate in four age bins, luminosity-weighted stellar age and stellar mass density, as well as the integrated 1D spectrum of each galaxy.