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Measuring star formation with resolved observations: the test case of M33, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1502.01347Comment: 15 pages, 9 figures, 1 table. Accepted for publication in A&A.The Mass Spectra of Giant Molecular Clouds in the Local Group. \pasp, (December 2005)Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1902.10437Comment: 23 pages, 9 figures, accepted for publication in A&A.The JCMT Nearby Galaxies Legacy Survey X. Environmental Effects on the Molecular Gas and Star Formation Properties of Spiral Galaxies, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1512.05768Comment: Accepted for publication in MNRAS, 25 pages, 14 figures.The molecular gas mass of M33, , , , , , , , , and 8 other author(s). (2016)cite arxiv:1609.03791Comment: Accepted for publication in Astronomy and Astrophysics.The Scale Dependence of the Molecular Gas Depletion Time in M33, , , , and . \apj, (October 2010)CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope, , , , , , , , , and 63 other author(s). (2021)cite arxiv:2107.10364Comment: 61 pages, 16 figures. Submitted to the Astrophysical Journal July 17, 2021.The Effect of Projection on Derived Mass-Size and Linewidth-Size Relationships, , , , , and . \apj, (April 2010)