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ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.

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ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass, , , , , , , , , and 18 other author(s). (2016)cite arxiv:1606.05280Comment: 31 pages, 16 figures, 13 tables, incorporating the first feedback from the referee on our submitted ApJ manuscript, paper VI of the ASPECS (ALMA Spectroscopic Survey in the Hubble Ultra Deep Field) series.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.Increasing access to engineering., , , , , , and . FIE, page 1-6. IEEE Computer Society, (2012)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).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.ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim4$, , , , , , , , and . (2021)cite arxiv:2109.09754Comment: 17 pages, 8 figures, submitted to the ApJ.Extended Cold Molecular Gas Reservoirs in z~3.4 Submillimeter Galaxies, , , , and . (2011)cite arxiv:1105.4177 Comment: 6 pages, 4 figures, to appear in ApJL (EVLA Special Issue; accepted May 19, 2011).Measurement of rotation in two galaxies in the Epoch of Reionization from ALMA-detected CII emission, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1706.04614Comment: 13 pages, 5 figues, 1 table, submitted.A deep search for molecular gas in two massive Lyman break galaxies at z=3 and 4: vanishing CO-emission due to low metallicity?, , , , , , , , , and 7 other author(s). (2013)cite arxiv:1309.5448Comment: 9 pages, 3 figures, accepted for publication in Astrophysical Journal Letters.