Herschel ATLAS: The cosmic star formation history of quasar host galaxies
5 páginas, 2 figuras, 1 tabla.-- Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia with important participation from NASA.-- et al.
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2010 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/46076 |
| Acceso en línea: | http://hdl.handle.net/10261/46076 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: active Infrared: galaxies Quasars: general Galaxies: formation Submillimeter: galaxies Galaxies: starburst |
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Herschel ATLAS: The cosmic star formation history of quasar host galaxiesSerjeant, StephenHerranz, DiegoLópez-Caniego, M.Galaxies: activeInfrared: galaxiesQuasars: generalGalaxies: formationSubmillimeter: galaxiesGalaxies: starburst5 páginas, 2 figuras, 1 tabla.-- Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia with important participation from NASA.-- et al.We present a derivation of the star formation rate per comoving volume of quasar host galaxies, derived from stacking analyses of far-infrared to mm-wave photometry of quasars with redshifts 0 < z < 6 and absolute I-band magnitudes -22 > IAB > -32 We use the science demonstration observations of the first ~16 deg2 from the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) in which there are 240 quasars from the Sloan Digital Sky Survey (SDSS) and a further 171 from the 2dF-SDSS LRG and QSO (2SLAQ) survey. We supplement this data with a compilation of data from IRAS, ISO, Spitzer, SCUBA and MAMBO. H-ATLAS alone statistically detects the quasars in its survey area at >5σ at 250,350 and 500 μm. From the compilation as a whole we find striking evidence of downsizing in quasar host galaxy formation: low-luminosity quasars with absolute magnitudes in the range -22 > IAB > -24 have a comoving star formation rate (derived from 100 μm rest-frame luminosities) peaking between redshifts of 1 and 2, while high-luminosity quasars with IAB < -26 have a maximum contribution to the star formation density at z ~ 3. The volume-averaged star formation rate of -22 > IAB > -24 quasars evolves as (1 + z)2.3±0.7 at z < 2, but the evolution at higher luminosities is much faster reaching (1 + z)10±1 at -26 > IAB > -28. We tentatively interpret this as a combination of a declining major merger rate with time and gas consumption reducing fuel for both black hole accretion and star formation.This work was funded in part by STFC (grants PP/D002400/1 and ST/G002533/1).Peer reviewedEDP Sciences201220122010info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501http://hdl.handle.net/10261/46076reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1051/0004-6361/201014565info:eu-repo/semantics/openAccessoai:digital.csic.es:10261/460762026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| title |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| spellingShingle |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies Serjeant, Stephen Galaxies: active Infrared: galaxies Quasars: general Galaxies: formation Submillimeter: galaxies Galaxies: starburst |
| title_short |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| title_full |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| title_fullStr |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| title_full_unstemmed |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| title_sort |
Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
| dc.creator.none.fl_str_mv |
Serjeant, Stephen Herranz, Diego López-Caniego, M. |
| author |
Serjeant, Stephen |
| author_facet |
Serjeant, Stephen Herranz, Diego López-Caniego, M. |
| author_role |
author |
| author2 |
Herranz, Diego López-Caniego, M. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Galaxies: active Infrared: galaxies Quasars: general Galaxies: formation Submillimeter: galaxies Galaxies: starburst |
| topic |
Galaxies: active Infrared: galaxies Quasars: general Galaxies: formation Submillimeter: galaxies Galaxies: starburst |
| description |
5 páginas, 2 figuras, 1 tabla.-- Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia with important participation from NASA.-- et al. |
| publishDate |
2010 |
| dc.date.none.fl_str_mv |
2010 2012 2012 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 |
| format |
article |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/46076 |
| url |
http://hdl.handle.net/10261/46076 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
http://dx.doi.org/10.1051/0004-6361/201014565 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
| eu_rights_str_mv |
openAccess |
| dc.publisher.none.fl_str_mv |
EDP Sciences |
| publisher.none.fl_str_mv |
EDP Sciences |
| dc.source.none.fl_str_mv |
reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
| instname_str |
Consejo Superior de Investigaciones Científicas (CSIC) |
| reponame_str |
DIGITAL.CSIC. Repositorio Institucional del CSIC |
| collection |
DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869407460055318528 |
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15,81155 |