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 Pineda et al. (2017).


Data Set Characteristics

Data ProductDescriptionData Access
Spectra Herschel HIFI

MAGCLOUDSCPLUS Documentation

Documentation
MAGCLOUDSCPLUS Delivery Document