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The CII Deficit in LIRGs and ULIRGs is Due to High-Temperature Saturation

, and . (2015)cite arxiv:1510.00397Comment: 7 pages, 2 figures, submitted to MNRAS.

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The Flatness and Sudden Evolution of the Intergalactic Ionizing Background, , , and . (2014)cite arxiv:1410.2249Comment: 13 pages, 6 figures, submitted to MNRAS, comments welcome.Molecular Cloud Properties and CO Line Emission in z >~ 6 Galaxies, and . (2013)cite arxiv:1301.0619Comment: 18 pages, 11 figures; submitted to MNRAS; comments welcome.The CII Deficit in LIRGs and ULIRGs is Due to High-Temperature Saturation, and . (2015)cite arxiv:1510.00397Comment: 7 pages, 2 figures, submitted to MNRAS.