1. ALMA observations of cold molecular gas in AGN hosts at z ~ 1.5 – evidence of AGN feedback?
- Author
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Kakkad, D, Mainieri, V, Brusa, M, Padovani, P, Carniani, S, Feruglio, C, Sargent, M, Husemann, B, Bongiorno, A, Bonzini, M, Piconcelli, E, Silverman, JD, and Rujopakarn, W
- Subjects
quasars: emission lines ,submillimetre: ISM ,13. Climate action ,galaxies: high-redshift ,Astrophysics::High Energy Astrophysical Phenomena ,galaxies: star formation ,galaxies: active ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics::Galaxy Astrophysics ,ISM: molecules - Abstract
Similarly to the cosmic star formation history, the black hole accretion rate density of the Universe peaked at 199 per cent 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., MB acknowledges support from the FP7 Career Integration Grant ‘eEASY: supermassive black holes through cosmic time from current surveys to eROSITA-Euclid Synergies’ (CIG 321913). SC acknowledges financial support from the Science and Technology Facilities Council (STFC). CF acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant agreement no. 664931. MTS acknowledges support from a Royal Society Leverhulme Trust Senior Research Fellowship (LT150041). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00171.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.