A dataset provided by the European Space Agency

Name OT2_clonsdal_1
Title Feedback from the most luminous dust-obscured AGNs in the universe
URL

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DOI 10.5270/esa-pg8b614
Author lonsdale, c.
Description AGN-powered feedback of energy and momentum via radiation pressure ("quasar mode") on interstellar dust and jet momentum ("radio mode") from a supermassive black hole (BH) into its host galaxy regulates the evolution of both the BH and the galaxy. Feedback is likely to be strongest in the most luminous dust-obscured QSOs, particularly those containing radio sources too luminous to be powered by starbursts. We selected a unique sample containing 147 of the most luminous obscured QSOs in the universe by identifying strong mid-infrared sources from the WISE survey covering more than half the sky having (1) convex mid-infrared spectra and (2) bright NVSS radio counterparts. The goal of our multi-telescope program is to understand the physical and evolutionary nature of these extreme feedback candidates. We have high priority (top decile) ALMA Cycle0 time for the southern sources in the sample for imaging at 345GHz, and SOAR time to obtain redshifts. This proposal requests 47.6 hours of PACS and SPIRE time to determine the relative warm to cool dust luminosities in these 147 sources, key observations for determining the relative AGN and starburst luminosties, and understanding the evolution stages, of these likely transition objects. Our goals are to discover the most obscured and powerful BHs throughout their main epoch of formation, and to test and constrain the roles of radio and radiative feedback in the quenching of star formation and the establishment of the BH-spheroid relations.
Publication Radio Jet Feedback and Star Formation in Heavily Obscured, Hyperluminous Quasars at Redshifts ˜ 0.5-3. I. ALMA Observations . Lonsdale Carol J. et al. . The Astrophysical Journal, Volume 813, Issue 1, article id. 45, 26 pp. (2015). . 813 . 10.1088\/0004-637X\/813\/1\/45 . 2015ApJ...813...45L ,
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-03-28T22:02:05Z/2013-04-27T17:22:39Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-10-27T17:18:59Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-27T17:18:59Z, OT2_clonsdal_1, SPG v14.2.0. https://doi.org/10.5270/esa-pg8b614