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Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview, , , , , , , , , and 50 other author(s). (2011)cite arxiv:1107.4313Comment: 16 pages, 11 figures, AJ, in press.The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic Cloud, , , , , , , , , and 8 other author(s). (2011)cite arxiv:1107.1717Comment: Accepted for publication in the Astrophysical Journal. 21 pages and 11 figures in apjemulate style.The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1510.08084Comment: 24 pages, 14 figures, submitted for publication in ApJ.Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud, , , , , , , , , and 13 other author(s). (2014)cite arxiv:1407.7658Comment: Submitted to MNRAS.Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1406.6066Comment: 20 pages, 9 figures, accepted for publication in the ApJ.Markov model for multispectral image analysis: application to small magellanic cloud segmentation., , , and . ICIP (1), page 953-956. IEEE, (2003)