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Sökning: onr:"swepub:oai:research.chalmers.se:47ed38e7-365f-49ef-9357-b3b853dfdd3c" > The mean star forma...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004272naa a2200613 4500
001oai:research.chalmers.se:47ed38e7-365f-49ef-9357-b3b853dfdd3c
003SwePub
008171108s2017 | |||||||||||000 ||eng|
024a https://research.chalmers.se/publication/2529952 URI
024a https://research.chalmers.se/publication/5048252 URI
024a https://doi.org/10.1093/MNRAS/STX21212 DOI
024a https://doi.org/10.1093/mnras/stx21212 DOI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Stanley, Flora,d 1990u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)floras
2451 0a The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
264 c 2017-08-17
264 1b Oxford University Press (OUP),c 2017
338 a electronic2 rdacarrier
520 a We investigate the mean star formation rates (SFRs) in the host galaxies of similar to 3000 optically selected quasi-stellar objects (QSOs) from the Sloan Digital Sky Survey within the Herschel-ATLAS fields, and a radio-luminous subsample covering the redshift range of z = 0.2-2.5. Using Wide-field Infrared Survey Explorer (WISE) and Herschel photometry (12-500 mu m) we construct composite spectral energy distributions (SEDs) in bins of redshift and active galactic nucleus (AGN) luminosity. We perform SED fitting to measure the mean infrared luminosity due to star formation, removing the contamination from AGN emission. We find that the mean SFRs show a weak positive trend with increasing AGN luminosity. However, we demonstrate that the observed trend could be due to an increase in black hole (BH) mass (and a consequent increase of inferred stellar mass) with increasing AGN luminosity. We compare to a sample of X-ray selected AGN and find that the two populations have consistent mean SFRs when matched in AGN luminosity and redshift. On the basis of the available virial BH masses, and the evolving BH mass to stellar mass relationship, we find that the mean SFRs of our QSO sample are consistent with those of main sequence star-forming galaxies. Similarly the radio-luminous QSOs have mean SFRs that are consistent with both the overall QSO sample and with star-forming galaxies on the main sequence. In conclusion, on average QSOs reside on the main sequence of star-forming galaxies, and the observed positive trend between the mean SFRs and AGN luminosity can be attributed to BH mass and redshift dependencies.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a galaxies: active
653 a galaxies: star formation
653 a galaxies: evolution
653 a quasars: general
700a Alexander, D. M.4 aut
700a Harrison, C. M.4 aut
700a Rosario, D. J.4 aut
700a Wang, L.4 aut
700a Aird, J. A.4 aut
700a Bourne, N.4 aut
700a Dunne, L.4 aut
700a Dye, S.4 aut
700a Eales, S.4 aut
700a Knudsen, Kirsten Kraiberg,d 1976u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)kraiberg
700a Michalowski, M. J.4 aut
700a Valiante, E.4 aut
700a De Zotti, G.4 aut
700a Furlanetto, C.4 aut
700a Ivison, R. J.4 aut
700a Maddox, S.4 aut
700a Smith, M. W. L.4 aut
710a Chalmers tekniska högskola4 org
773t Monthly Notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 472:2, s. 2221-2240q 472:2<2221-2240x 0035-8711x 1365-2966
856u http://publications.lib.chalmers.se/records/fulltext/252995/local_252995.pdfx primaryx freey FULLTEXT
856u http://dro.dur.ac.uk/23390/1/23390.pdf
8564 8u https://research.chalmers.se/publication/252995
8564 8u https://research.chalmers.se/publication/504825
8564 8u https://doi.org/10.1093/MNRAS/STX2121
8564 8u https://doi.org/10.1093/mnras/stx2121

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