{ "id": "1703.08183", "version": "v1", "published": "2017-03-23T18:00:03.000Z", "updated": "2017-03-23T18:00:03.000Z", "title": "ALMA observations of cold molecular gas in AGN hosts at z~1.5 - Evidence of AGN feedback?", "authors": [ "D. Kakkad", "V. Mainieri", "M. Brusa", "P. Padovani", "S. Carniani", "C. Feruglio", "M. Sargent", "B. Husemann", "A. Bongiorno", "M. Bonzini", "E. Piconcelli", "J. D. Silverman", "W. Rujopakarn" ], "comment": "12 pages, 5 figures, 3 tables, accepted for publication in MNRAS", "doi": "10.1093/mnras/stx726", "categories": [ "astro-ph.GA", "astro-ph.HE" ], "abstract": "Similarly to the cosmic star formation history, the black hole accretion rate density of the Universe peaked at 199% probability of lower depletion time scales and lower molecular gas fractions in AGN hosts with respect to the non-AGN comparison sample. We discuss the implications of these observations on the impact that AGN feedback may have on star formation efficiency of z>1 galaxies.", "revisions": [ { "version": "v1", "updated": "2017-03-23T18:00:03.000Z" } ], "analyses": { "keywords": [ "cold molecular gas", "agn hosts", "agn feedback", "alma observations", "black hole accretion rate density" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable" } } }