Herschel: Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO (MAGCLOUDSCPLUS)
MAGCLOUDSCPLUS Overview MAGCLOUDSCPLUS Data Access

Overview

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.

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Data Set Characteristics

Data ProductDescriptionData Access
Spectra Herschel HIFI

MAGCLOUDSCPLUS Documentation

Documentation
MAGCLOUDSCPLUS Delivery Document