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dc.contributor.authorShen, Yue
dc.contributor.authorGreene, Jenny E.
dc.contributor.authorHo, Luis C.
dc.contributor.authorBrandt, W. N.
dc.contributor.authorDenney, Kelly D.
dc.contributor.authorHorne, Keith Douglas
dc.contributor.authorJiang, Linhua
dc.contributor.authorKochanek, Christopher S.
dc.contributor.authorMcGreer, Ian D.
dc.contributor.authorMerloni, Andrea
dc.contributor.authorPeterson, Bradley M.
dc.contributor.authorPetitjean, Patrick
dc.contributor.authorSchneider, Donald P.
dc.contributor.authorSchulze, Andreas
dc.contributor.authorStrauss, Michael A.
dc.contributor.authorTao, Charling
dc.contributor.authorTrump, Jonathan R.
dc.contributor.authorPan, Kaike
dc.contributor.authorBizyaev, Dmitry
dc.date.accessioned2016-02-11T16:10:12Z
dc.date.available2016-02-11T16:10:12Z
dc.date.issued2015-06-01
dc.identifier.citationShen , Y , Greene , J E , Ho , L C , Brandt , W N , Denney , K D , Horne , K D , Jiang , L , Kochanek , C S , McGreer , I D , Merloni , A , Peterson , B M , Petitjean , P , Schneider , D P , Schulze , A , Strauss , M A , Tao , C , Trump , J R , Pan , K & Bizyaev , D 2015 , ' The Sloan Digital Sky Survey Reverberation Mapping project: : no evidence for evolution in the M•-σ* Relation to z~1 ' Astrophysical Journal , vol 805 , no. 2 . DOI: 10.1088/0004-637X/805/2/96en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 240938622
dc.identifier.otherPURE UUID: a50a9037-274a-42ca-baa7-9970fab11d12
dc.identifier.otherScopus: 84930676853
dc.identifier.urihttp://hdl.handle.net/10023/8205
dc.descriptionSupport for the work of Y.S. was provided by NASA through Hubble Fellowship grant number HST-HF-51314, awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. L.C.H. acknowledges support from the Chinese Academy of Sciences through grant No. XDB09030102 (Emergence of Cosmological Structures) from the Strategic Priority Research Program and from the National Natural Science Foundation of China through grant No. 11473002. W.N.B. acknowledges support from NSF grant AST-1108604. B.M.P. acknowledges support from the NSF through grant AST-1008882.en
dc.description.abstractWe present host stellar velocity dispersion measurements for a sample of 88 broad-line quasars at 0.1 <z <1 (46 at z > 0.6) from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. High signal-to-noise ratio coadded spectra (average S/N ≈ 30 per 69 km s-1 pixel) from SDSS-RM allowed for the decomposition of the host and quasar spectra and for measurements of the host stellar velocity dispersions and black hole (BH) masses using the single-epoch (SE) virial method. The large sample size and dynamic range in luminosity (L5100 = 1043.2-44.7 ergs-1) lead to the first clear detection of a correlation between SE virial BH mass and host stellar velocity dispersion far beyond the local universe. However, the observed correlation is significantly flatter than the local relation, suggesting that there are selection biases in high-z luminosity-threshold quasar samples for such studies. Our uniform sample and analysis enable an investigation of the redshift evolution of the M-σ∗ relation relatively free of caveats by comparing different samples/analyses at disjoint redshifts. We do not observe evolution of the M-σ∗ relation in our sample up to z ∼ 1, but there is an indication that the relation flattens toward higher redshifts. Coupled with the increasing threshold luminosity with redshift in our sample, this again suggests that certain selection biases are at work, and simple simulations demonstrate that a constant M-σ∗ relation is favored to z ∼ 1. Our results highlight the scientific potential of deep coadded spectroscopy from quasar monitoring programs, and offer a new path to probe the co-evolution of BHs and galaxies at earlier times.en
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2015. The American Astronomical Society. All rights reserved. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.1088/0004-637X/805/2/96en
dc.subjectBlack hole physicsen
dc.subjectGalaxies: activeen
dc.subjectQuasars: generalen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNuclear and High Energy Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe Sloan Digital Sky Survey Reverberation Mapping project: : no evidence for evolution in the M•-σ* Relation to z~1en
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttp://dx.doi.org/10.1088/0004-637X/805/2/96
dc.description.statusPeer revieweden


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