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VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA, , , , , , , , , and 11 other author(s). (2016)cite arxiv:1611.05867Comment: Accepted for publication in A&A. Abstract abridged for arXiv. 13 pages, including 5 figures and 2 tables.Witnessing the birth of the red sequence: the physical scale and morphology of dust emission in hyper-luminous starbursts in the early Universe, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1709.04191Comment: Submitted to ApJ. Comments welcome.A submillimeter galaxy illuminating its circumgalactic medium: Ly-alpha scattering in a cold, clumpy outflow, , , , , , , , , and 10 other author(s). (2014)cite arxiv:1402.6335Comment: Submitted to ApJ.The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1504.02479Comment: Submitted to ApJ.A deep ALMA image of the Hubble Ultra Deep Field, , , , , , , , , and 26 other author(s). (2016)cite arxiv:1606.00227Comment: 25 pages, 14 figures, submitted to MNRAS.Witnessing the birth of the red sequence: ALMA high-resolution imaging of CII and dust in two interacting ultra-red starbursts at z = 4.425, , , , , , , , , and 12 other author(s). (2016)cite arxiv:1601.07549Comment: Submitted to ApJ.A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time, , , , , , , and . (2019)cite arxiv:1902.09172Comment: 21 pages, 10 figures, 8 table, accepted for publication in A&A.The average submillimetre properties of Lyman-alpha Blobs at z=3, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1605.04912v1.pdfComment: Accepted MNRAS 16 May 2016.H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum, , , , , , , , , and 15 other author(s). (2012)cite arxiv:1212.2211Comment: 15 pages, 12 figures, ApJ submitted.The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5, , , , , , , and . (2017)cite arxiv:1706.00426Comment: 17 pages, 12 figures, 5 tables, submitted to MNRAS.