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Deep submillimeter and radio observations in the SSA22 field. I. Powering sources and Ly\alpha escape fraction of Ly\alpha blobs, , , , , , , , , и 15 other автор(ы). (2017)cite arxiv:1704.05101Comment: 22 pages, 7 figures, submitted to ApJ.Asymmetries in core-collapse supernovae from maps of radioactive \$^44\$Ti in CassiopeiaA, , , , , , , , , и 21 other автор(ы). Nature, 506 (7488): 339--342 (19.03.2014)Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters, , , , , , , , , и 2 other автор(ы). (2013)cite arxiv:1301.3922Comment: 11 pages, 5 figures, accepted for publication in 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, , , , , , , , и . (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, , , , , , , , , и 7 other автор(ы). (2016)cite arxiv:1601.00682Comment: MNRAS, submitted: 9 pages, 3 figures, 2 tables.A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN, , , , , , , и . (26.02.2015)The average submillimetre properties of Lyman-alpha Blobs at z=3, , , , , , , , , и 4 other автор(ы). (2016)cite arxiv:1605.04912v1.pdfComment: Accepted MNRAS 16 May 2016.ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions, , , , , , , , , и 8 other автор(ы). (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.Herschel protocluster survey: A search for dusty star-forming galaxies in protoclusters at z=2-3, , , , , , , , , и 8 other автор(ы). (2016)cite arxiv:1605.07370Comment: 15 pages, 5 figures, 12 tables, Accepted for publication in MNRAS.Do AGN really suppress star formation?, , , , и . (2019)cite arxiv:1912.01020Comment: IAU Proceedings No. 356 "Nuclear Activity in Galaxies Across Cosmic Time", M. Povic et al.