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Molecular gas in three z~7 quasar host galaxies

, , , , , , , , and . (2017)cite arxiv:1707.05238Comment: 12 pages, 6 figures. Accepted for publication in ApJ.

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Molecular gas in three z~7 quasar host galaxies, , , , , , , , and . (2017)cite arxiv:1707.05238Comment: 12 pages, 6 figures. Accepted for publication in ApJ.An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1705.03503Comment: 26 pages; 15 figures. Accepted for publication in ApJ. Redshift catalogs, spectra and SED templates available from: http://astro.dur.ac.uk/~ams/zLESS/.An ALMA survey of Sub-millimetre Galaxies in the Extended Chandra Deep Field South: Detection of C II at z=4.4, , , , , , , , , and 12 other author(s). (2012)cite arxiv:1209.1390Comment: Accepted for publication in MNRAS. 10 pages, 5 figures, 2 tables.The Starburst-Driven Molecular Wind in NGC 253 and the Suppression of Star Formation, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1307.6259Comment: Appearing in the July 25 2013 issue of Nature.The Multi-Phase Cold Fountain in M82 Revealed by a Wide, Sensitive Map of the Molecular ISM, , , , , , , , , and . (2015)cite arxiv:1509.02932Comment: 36 pages including 25 figures and 4 appendices. Accepted for publication in the Astrophysical Journal. For a high resolution version please visit http://www.astronomy.ohio-state.edu/~leroy.42/ms_m82.pdf.Faint CO Line Wings in Four Star-Forming (Ultra)luminous Infrared Galaxies, , , , , and . (2015)cite arxiv:1508.03223Comment: 9 pages, 5 figures, 1 appendix; accepted for publication in the Astrophysical Journal.CO(1-0) in z>2 Quasar Host Galaxies: No Evidence for Extended Molecular Gas Reservoirs, , , , , , , , , and 1 other author(s). (2011)cite arxiv:1106.2553Comment: 6 pages, 4 figures, 1 table, to appear in ApJL (EVLA Special Issue; accepted June 10, 2011).dtv-Atlas Pädagogik, and . Dt. Taschenbuch-Verl., München, (2008)An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1504.04376Comment: 22 pages, 14 figures, 2 tables. Accepted for publication in the Astrophysical Journal. The new MAGPHYS model libraries used in this paper will appear in www.iap.fr/magphys. The SMG SED templates shown in Section 6.1 are available at http://astronomy.swinburne.edu.au/~ecunha/ecunha/SED_Templates.html.Imaging the Molecular Interstellar Medium in a Gravitationally Lensed Star-forming Galaxy at z=5.7, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1905.12738Comment: 13 pages, 10 figures, accepted for publication in Astronomy and Astrophysics.