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ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions

, , , , , , , , , , , , , , , , , and . (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.

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Metal deficiency in cluster star-forming galaxies at z=2, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1410.1437Comment: 18 pages, 18 figures, Submitted to ApJ.The hidden AGN main sequence: Evidence for a universal SMBH accretion to star formation rate ratio since z~2 producing a M_BH-M* relation, , , , , , , , and . (2012)cite arxiv:1204.2824Comment: 6 Pages, 3 Figures, Submitted to ApJL.The FMOS-COSMOS survey of star-forming galaxies at z~1.6. IV: Excitation state and chemical enrichment of HII regions, , , , , , , , , and 14 other author(s). (2016)cite arxiv:1604.06802Comment: 22 pages, 17 Figures, submitted to ApJ.ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra, , , , , , , , , and 62 other author(s). (2022)cite arxiv:2208.08517Comment: AJ, submitted, 26 pages, 15 figures, 9 tables, one of a suite of 8 papers detailing targeting for DESI.