Herschel ATLAS : the cosmic star formation history of quasar host galaxies
- Author
- S Serjeant, F Bertoldi, AW Blain, DL Clements, A Cooray, L Danese, J Dunlop, L Dunne, S Eales, J Falder, E Hatziminaoglou, DH Hughes, E Ibar, MJ Jarvis, A Lawrence, MG Lee, M Michalowski, M Negrello, A Omont, M Page, C Pearson, PP van der Werf, G White, A Amblard, R Auld, Maarten Baes (UGent) , DG Bonfield, D Burgarella, S Buttiglione, A Cava, A Dariush, G de Zotti, S Dye, D Frayer, Jacopo Fritz (UGent) , J Gonzalez-Nuevo, D Herranz, RJ Ivison, G Lagache, L Leeuw, M Lopez-Caniego, S Maddox, E Pascale, M Pohlen, E Rigby, G Rodighiero, S Samui, B Sibthorpe, DJB Smith, P Temi, M Thompson, I Valtchanov and A Verma
- Organization
- Abstract
- 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 > I-AB > -32 We use the science demonstration observations of the first similar to 16 deg(2) 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 > 5 sigma at 250, 350 and 500 mu m. 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 > I-AB > -24 have a comoving star formation rate (derived from 100 mu m rest-frame luminosities) peaking between redshifts of 1 and 2, while high-luminosity quasars with I-AB -26 have a maximum contribution to the star formation density at z similar to 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 > I-AB > -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.
- Keywords
- infrared: galaxies, quasars: general, galaxies: active, galaxies: formation, submillimeter: galaxies, galaxies: starburst, SPECTRAL ENERGY-DISTRIBUTIONS, SUPERMASSIVE BLACK-HOLES, ACTIVE GALACTIC NUCLEI, MM MAMBO/IRAM-30 M, SUBMILLIMETER GALAXIES, DUST EMISSION, SURVEY SBQS, EVOLUTION, CONSTRAINTS, DETECTIONS
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Citation
Please use this url to cite or link to this publication: http://hdl.handle.net/1854/LU-1236067
- MLA
- Serjeant, S., et al. “Herschel ATLAS : The Cosmic Star Formation History of Quasar Host Galaxies.” ASTRONOMY & ASTROPHYSICS, vol. 518, 2010, doi:10.1051/0004-6361/201014565.
- APA
- Serjeant, S., Bertoldi, F., Blain, A., Clements, D., Cooray, A., Danese, L., … Verma, A. (2010). Herschel ATLAS : the cosmic star formation history of quasar host galaxies. ASTRONOMY & ASTROPHYSICS, 518. https://doi.org/10.1051/0004-6361/201014565
- Chicago author-date
- Serjeant, S, F Bertoldi, AW Blain, DL Clements, A Cooray, L Danese, J Dunlop, et al. 2010. “Herschel ATLAS : The Cosmic Star Formation History of Quasar Host Galaxies.” ASTRONOMY & ASTROPHYSICS 518. https://doi.org/10.1051/0004-6361/201014565.
- Chicago author-date (all authors)
- Serjeant, S, F Bertoldi, AW Blain, DL Clements, A Cooray, L Danese, J Dunlop, L Dunne, S Eales, J Falder, E Hatziminaoglou, DH Hughes, E Ibar, MJ Jarvis, A Lawrence, MG Lee, M Michalowski, M Negrello, A Omont, M Page, C Pearson, PP van der Werf, G White, A Amblard, R Auld, Maarten Baes, DG Bonfield, D Burgarella, S Buttiglione, A Cava, A Dariush, G de Zotti, S Dye, D Frayer, Jacopo Fritz, J Gonzalez-Nuevo, D Herranz, RJ Ivison, G Lagache, L Leeuw, M Lopez-Caniego, S Maddox, E Pascale, M Pohlen, E Rigby, G Rodighiero, S Samui, B Sibthorpe, DJB Smith, P Temi, M Thompson, I Valtchanov, and A Verma. 2010. “Herschel ATLAS : The Cosmic Star Formation History of Quasar Host Galaxies.” ASTRONOMY & ASTROPHYSICS 518. doi:10.1051/0004-6361/201014565.
- Vancouver
- 1.Serjeant S, Bertoldi F, Blain A, Clements D, Cooray A, Danese L, et al. Herschel ATLAS : the cosmic star formation history of quasar host galaxies. ASTRONOMY & ASTROPHYSICS. 2010;518.
- IEEE
- [1]S. Serjeant et al., “Herschel ATLAS : the cosmic star formation history of quasar host galaxies,” ASTRONOMY & ASTROPHYSICS, vol. 518, 2010.
@article{1236067, abstract = {{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 > I-AB > -32 We use the science demonstration observations of the first similar to 16 deg(2) 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 > 5 sigma at 250, 350 and 500 mu m. 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 > I-AB > -24 have a comoving star formation rate (derived from 100 mu m rest-frame luminosities) peaking between redshifts of 1 and 2, while high-luminosity quasars with I-AB -26 have a maximum contribution to the star formation density at z similar to 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 > I-AB > -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.}}, articleno = {{L7}}, author = {{Serjeant, S and Bertoldi, F and Blain, AW and Clements, DL and Cooray, A and Danese, L and Dunlop, J and Dunne, L and Eales, S and Falder, J and Hatziminaoglou, E and Hughes, DH and Ibar, E and Jarvis, MJ and Lawrence, A and Lee, MG and Michalowski, M and Negrello, M and Omont, A and Page, M and Pearson, C and van der Werf, PP and White, G and Amblard, A and Auld, R and Baes, Maarten and Bonfield, DG and Burgarella, D and Buttiglione, S and Cava, A and Dariush, A and de Zotti, G and Dye, S and Frayer, D and Fritz, Jacopo and Gonzalez-Nuevo, J and Herranz, D and Ivison, RJ and Lagache, G and Leeuw, L and Lopez-Caniego, M and Maddox, S and Pascale, E and Pohlen, M and Rigby, E and Rodighiero, G and Samui, S and Sibthorpe, B and Smith, DJB and Temi, P and Thompson, M and Valtchanov, I and Verma, A}}, issn = {{0004-6361}}, journal = {{ASTRONOMY & ASTROPHYSICS}}, keywords = {{infrared: galaxies,quasars: general,galaxies: active,galaxies: formation,submillimeter: galaxies,galaxies: starburst,SPECTRAL ENERGY-DISTRIBUTIONS,SUPERMASSIVE BLACK-HOLES,ACTIVE GALACTIC NUCLEI,MM MAMBO/IRAM-30 M,SUBMILLIMETER GALAXIES,DUST EMISSION,SURVEY SBQS,EVOLUTION,CONSTRAINTS,DETECTIONS}}, language = {{eng}}, pages = {{5}}, title = {{Herschel ATLAS : the cosmic star formation history of quasar host galaxies}}, url = {{http://doi.org/10.1051/0004-6361/201014565}}, volume = {{518}}, year = {{2010}}, }
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