Herschel data from the "Characterizing the transition from diffuse atomic to
dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO"
(MAGCLOUDSCPLUS) Open Time Key Program (KPOT_jpineda_1) are available here using
spatial and visualization tools. MAGCLOUDSCPLUS surveyed 54 lines of sight
toward the Large and Small Magellanic Clouds in the [C II] 158 micron, [C I] 609
micron, [C I] 370 micron, and 12CO J = 7 → 6 lines using Herschel's HIFI
instrument.
If you use MAGCLOUDSCPLUS data, please cite both the journal article Pineda et al.
(2017) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA516.
Jump to documentation.
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