The Herschel Gould Belt Survey is one of the largest Herschel Key Projects (KPGT_pandre_1).
It conducted extensive far-infrared and submillimeter mapping of nearby
molecular clouds with both the SPIRE and PACS instruments. It covered the bulk
of the nearest (d ≤ 0.5 kpc) cloud complexes in the Galaxy, which are mostly
located in the Gould Belt, a giant (700 pc by 1000 pc), flat structure inclined
by 20d to the Galactic plane.
If you use HGBS data, please cite both the journal article Andre et al.
(2010) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA72.
Jump to documentation.
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HGBS Overview
HGBS Primary Data Access
HGBS Cutouts
