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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.The nature of the ISM in galaxies during the star-formation activity peak of the Universe, , , , and . (2013)cite arxiv:1310.1476Comment: 18 pages, 14 figures, submitted to MNRAS.A PDR-Code Comparison Study, , , , , , , , , and 14 other author(s). (2007)cite arxiv:astro-ph/0702231 Comment: 28 pages, 16 figures, see all benchmark data under: http://www.ph1.uni-koeln.de/pdr-comparison.ALMA view of the $^12$C/$^13$C isotopic ratio in starburst galaxies, , , , , , , , , and 9 other author(s). (2019)cite arxiv:1906.06638Comment: Accepted for publication in A&A.Ly$\alpha$ Cooling Radiation from High-Redshift Halos, , and . \apjl, (July 2000)Star formation near an obscured AGN: Variations in the initial mass function, and . (2011)cite arxiv:1109.6593 Comment: 25 pages, 17 figures. Accepted for publication in Astronomy and Astrophysics.ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1608.02941Comment: Accepted for publication in ApJ.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.Effects of turbulence and rotation on protostar formation as a precursor to seed black holes, , , , , and . (Aug 6, 2014)Facial recognition system for driver vigilance monitoring., , , , and . SMC (4), page 3787-3792. IEEE, (2004)