Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3

Baldry et al. 2018, published in MNRAS, Vol. 474, pp. 3875-3888 (links: ADS, DOI)

Abstract

We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multi-wavelength photometric survey in three equatorial regions each of 60.0 deg² (G09, G12, G15), and two southern regions of 55.7 deg² (G02) and 50.6 deg² (G23). DR3 consists of: the first release of data covering the G02 region and of data on H-ATLAS sources in the equatorial regions; and updates to data on sources released in DR2. DR3 includes 154809 sources with secure redshifts across four regions. A subset of the G02 region is 95.5% redshift complete to r<19.8 over an area of 19.5 deg², with 20086 galaxy redshifts, that overlaps substantially with the XXL survey (X-ray) and VIPERS (redshift survey). In the equatorial regions, the main survey has even higher completeness (98.5%), and spectra for about 75% of H-ATLAS filler targets were also obtained. This filler sample extends spectroscopic redshifts, for probable optical counterparts to H-ATLAS sub-mm sources, to 0.8 mag deeper (r<20.6) than the GAMA main survey. There are 25814 galaxy redshifts for H-ATLAS sources from the GAMA main or filler surveys. GAMA DR3 is available at the survey website (www.gama-survey.org/dr3/).

Data:

GAMA DR3.

H-ATLAS-GAMA sample as used in Figures 9-13. The selection is m₂₅₀<12.72, m_r<20.6, match-reliability R>0.8, star-galaxy separation (eq. 1), and reduced area to match selection of filler targets (within blue solid line of Fig. 8). Bourne et al. 2016 describe the H-ATLAS DR1 used for this sample.

Links: - return to my home page; return to my research page; list of publications.