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Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field

, , , , , , , , , , , , , , and . (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.

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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.ALMACAL III: A combined ALMA and MUSE Survey for Neutral, Molecular, and Ionised Gas in an HI-Absorption-Selected System, , , , , , , and . (2017)cite arxiv:1712.00014Comment: 17 pages, 9 figures, 9 tables, accepted for publication in MNRAS.ALMACAL I: First dual-band number counts from a deep and wide ALMA submm survey, free from cosmic variance, , , , and . (2015)cite arxiv:1508.05099Comment: Submitted to ApJ.Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.ALMACAL II: Extreme star-formation-rate densities in a pair of dusty starbursts at $z = 3.442$ revealed by ALMA 20-milliarcsec resolution imaging, , , , and . (2016)cite arxiv:1607.06464Comment: Submitted to ApJ. Comments are welcome.Parsec-scale HI absorption structure in a low-redshift galaxy seen against a Compact Symmetric Object, , , , and . (2016)cite arxiv:1607.05995Comment: 14 pages and 10 figures. Accepted for publication in MNRAS.