The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of
600 deg^2 in five photometric bands (100, 160, 250, 350 and 500 microns) with
the Photoconductor Array Camera and Spectrometer (PACS) and Spectral and
Photometric Imaging Receiver (SPIRE) cameras. DR1 of H-ATLAS includes the survey of
three fields on the celestial equator, covering a total area of 161.6 deg^2 and
previously observed in the Galaxy and Mass Assembly (GAMA) spectroscopic
survey.
If you use H-ATLAS data, please cite the journal articles Valiante et al.
(2016) and Bourne et al.
(2016), as well as the dataset Digital Object Identifier (DOI): 10.26131/IRSA84.
Jump to documentation.
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H-ATLAS Overview
H-ATLAS Primary Data Access
H-ATLAS Cutouts
H-ATLAS Catalogs
