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 Pineda et al. (2017).