A dataset provided by the European Space Agency

Name OT1_hnetzer_2
Title Black hole growth and star formation in the early universe: the z=4.8 sample
URL

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DOI https://doi.org/10.5270/esa-msd6zxr
Author netzer, h.
Description We propose to secure Herschel PACS and SPIRE observations for a unique sample of 44 z=4.8 active galactic nuclei (AGNs). This is a genuine optically-selected flux limited sample that was observed by us from the ground thus providing reliable black hole (BH) and accretion rate estimates based on the properties of the strong MgII 2800A line. Reliable BH mass estimates at z>2 can only be obtained in narrow redshift bands at around z=2.3, z=3.3, z=4.8 and z=6.5. Our z=4.8 sample is thus a corner stone for answering any question related to galaxy and BH evolution, in particular the co-evolution (if any) of BHs and star formation (SF) in the early universe. The Herschel observations will provide invaluable information about the SF rate (SFR) in the host galaxies of the z=4.8 AGNs which, when combined with observations in the other redshift bands will trace the growth of the most massive BHs and the stellar mass in their hosts. SPIRE observations will provide SFRs (or upper limits on the SFR) in all sources. PACS observations of the more luminous sources in the sample will provide a. priors for the SPIRE observations that will allow us to go below the confusion limits and b. unique information about the 17-40 micron (rest) emission by warm (200K) dust close to the centers of these sources.
Publication Star Formation and Black Hole Growth at z virgul= 4.8 . Netzer Hagai et al. . The Astrophysical Journal, Volume 791, Issue 1, article id. 34, 15 pp. (2014). . 791 . 10.1088/0004-637X/791/1/34 . 2014ApJ...791...34N ,
Extreme Star Formation in the Host Galaxies of the Fastest Growing Supermassive Black Holes at z = 4.8 . Mor Rivay et al. . The Astrophysical Journal Letters, Volume 749, Issue 2, article id. L25, 6 pp. (2012). . 749 . 10.1088/2041-8205/749/2/L25 . 2012ApJ...749L..25M ,
ALMA Observations of Quasar Host Galaxies at z ≃ 4.8 . Nguyen Nathen H. et al. . The Astrophysical Journal . null . null . 2020ApJ...895...74N ,
Instrument SPIRE_SpirePhoto_small
Temporal Coverage 2010-12-20T14:06:53Z/2012-06-03T14:24:32Z
Version SPG v14.1.0
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/h®erschel/
Date Published 2012-12-03T14:10:13Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-12-03T14:10:13Z, OT1_hnetzer_2, SPG v14.1.0. https://doi.org/10.5270/esa-msd6zxr