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ALMA observations of a z~3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment

, , , , , , , , , , , , , , , , and . (2016)cite arxiv:1601.00682Comment: MNRAS, submitted: 9 pages, 3 figures, 2 tables.

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Star Formation and Supercluster Environment of 107 Nearby Galaxy Clusters, , , , and . (2016)cite arxiv:1612.04813Comment: 6 pages, 3 figures, 2 tables; Accepted for publication in ApJ.A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN, , , , , , , and . (Feb 26, 2015)Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1404.0677Comment: 28 pages (8 in appendices), 12 figures (3 in appendices), accepted for publication in MNRAS.The Bolometric Quasar Luminosity Function at z = 0-7, , , , , , and . (2020)cite arxiv:2001.02696Comment: Submitted to MNRAS. The code and data are available at https://bitbucket.org/ShenXuejian/quasarlf/src/master/. Comments are welcomed!.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.ALMA observations of a z~3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1601.00682Comment: MNRAS, submitted: 9 pages, 3 figures, 2 tables.