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Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe, , , , , , , , , and 20 other author(s). (2021)cite arxiv:2106.13719Comment: 26 pages, 1 table, 17 figures, submitted to ApJ, Table 2 will become available on publication of the paper.The Herschel Reference Survey: Dust in Early-Type Galaxies and Across the Hubble Sequence, , , , , , , , , and 17 other author(s). (2011)cite arxiv:1112.1408Comment: 35 Pages, 12 Figures. Submitted to ApJ December 2011.The Ionized Gas in Nearby Galaxies as Traced by the NII 122 and 205 m Transitions, , , , , , , , , and 13 other author(s). (2016)cite arxiv:1605.03180Comment: 18 pages, 9 figures, accepted for publication in The Astrophysical Journal.The dust content of the Crab Nebula, , , , , , , , , and . (2019)cite arxiv:1906.02203Comment: 33 pages, 17 figures, Manuscript accepted for publication in MNRAS. Accepted on 31/05/2019. Deposited on 31/05/2019.Normal, Dust-Obscured Galaxies in the Epoch of Reionization, , , , , , , , , and 19 other author(s). (2021)cite arxiv:2109.10378Comment: 16 pages, 7 figures, 4 tables, published in Nature.Dust Properties in HII Regions in M33, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1606.03624Comment: Accepted for publication in A&A, 29 pages, 16 figures.An Overview of the Dwarf Galaxy Survey, , , , , , , , , and 31 other author(s). (2013)cite arxiv:1305.2628Comment: Article accepted for PASP (april 25 2013).The reliability of CII as a star formation rate indicator, , , , and . ArXiv e-prints, (June 2011)Linking dust emission to fundamental properties in galaxies: The low-metallicity picture, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1507.05432Comment: 44 pages (20 pages main body plus 5 Appendices), 11 figures, 9 tables, accepted for publication in A&A.Star-forming dwarf galaxies in the Virgo cluster: the link between molecular gas, atomic gas, and dust, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1602.09077Comment: 19 pages, 11 figures, accepted for publication in Astronomy & Astrophysics.