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Title: THE BLACK HOLE MASS-GALAXY LUMINOSITY RELATIONSHIP FOR SLOAN DIGITAL SKY SURVEY QUASARS

Abstract

We investigate the relationship between the mass of the central supermassive black hole, M {sub BH}, and the host galaxy luminosity, L {sub gal}, in a sample of quasars from the Sloan Digital Sky Survey Data Release 7. We use composite quasar spectra binned by black hole mass and redshift to assess galaxy features that would otherwise be overwhelmed by noise in individual spectra. The black hole mass is calculated using the photoionization method, and the host galaxy luminosity is inferred from the depth of the Ca II H+K features in the composite spectra. We evaluate the evolution in the M {sub BH}-L {sub gal} relationship by examining the redshift dependence of Δ log M {sub BH}, the offset in M {sub BH} from the local M {sub BH}-L {sub gal} relationship. There is little systematic trend in Δ log M {sub BH} out to z = 0.8. Using the width of the [O III] emission line as a proxy for the stellar velocity dispersion, σ{sub *}, we find agreement of our derived host luminosities with the locally observed Faber-Jackson relation. This supports the utility of the width of the [O III] line as a proxy for σ{sub *} inmore » statistical studies.« less

Authors:
;  [1];  [2]
  1. Department of Astronomy, University of Texas, Austin, TX 78712 (United States)
  2. Department of Physics, Emory University, Atlanta, GA 30322 (United States)
Publication Date:
OSTI Identifier:
22364334
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 799; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BLACK HOLES; CALCIUM IONS; GALAXIES; LUMINOSITY; MASS; OXYGEN IONS; PHOTOIONIZATION; QUASARS; RED SHIFT; STAR EVOLUTION

Citation Formats

Salviander, S., Shields, G. A., and Bonning, E. W., E-mail: triples@astro.as.utexas.edu, E-mail: shields@astro.as.utexas.edu, E-mail: erin.bonning@emory.edu. THE BLACK HOLE MASS-GALAXY LUMINOSITY RELATIONSHIP FOR SLOAN DIGITAL SKY SURVEY QUASARS. United States: N. p., 2015. Web. doi:10.1088/0004-637X/799/2/173.
Salviander, S., Shields, G. A., & Bonning, E. W., E-mail: triples@astro.as.utexas.edu, E-mail: shields@astro.as.utexas.edu, E-mail: erin.bonning@emory.edu. THE BLACK HOLE MASS-GALAXY LUMINOSITY RELATIONSHIP FOR SLOAN DIGITAL SKY SURVEY QUASARS. United States. doi:10.1088/0004-637X/799/2/173.
Salviander, S., Shields, G. A., and Bonning, E. W., E-mail: triples@astro.as.utexas.edu, E-mail: shields@astro.as.utexas.edu, E-mail: erin.bonning@emory.edu. Sun . "THE BLACK HOLE MASS-GALAXY LUMINOSITY RELATIONSHIP FOR SLOAN DIGITAL SKY SURVEY QUASARS". United States. doi:10.1088/0004-637X/799/2/173.
@article{osti_22364334,
title = {THE BLACK HOLE MASS-GALAXY LUMINOSITY RELATIONSHIP FOR SLOAN DIGITAL SKY SURVEY QUASARS},
author = {Salviander, S. and Shields, G. A. and Bonning, E. W., E-mail: triples@astro.as.utexas.edu, E-mail: shields@astro.as.utexas.edu, E-mail: erin.bonning@emory.edu},
abstractNote = {We investigate the relationship between the mass of the central supermassive black hole, M {sub BH}, and the host galaxy luminosity, L {sub gal}, in a sample of quasars from the Sloan Digital Sky Survey Data Release 7. We use composite quasar spectra binned by black hole mass and redshift to assess galaxy features that would otherwise be overwhelmed by noise in individual spectra. The black hole mass is calculated using the photoionization method, and the host galaxy luminosity is inferred from the depth of the Ca II H+K features in the composite spectra. We evaluate the evolution in the M {sub BH}-L {sub gal} relationship by examining the redshift dependence of Δ log M {sub BH}, the offset in M {sub BH} from the local M {sub BH}-L {sub gal} relationship. There is little systematic trend in Δ log M {sub BH} out to z = 0.8. Using the width of the [O III] emission line as a proxy for the stellar velocity dispersion, σ{sub *}, we find agreement of our derived host luminosities with the locally observed Faber-Jackson relation. This supports the utility of the width of the [O III] line as a proxy for σ{sub *} in statistical studies.},
doi = {10.1088/0004-637X/799/2/173},
journal = {Astrophysical Journal},
number = 2,
volume = 799,
place = {United States},
year = {Sun Feb 01 00:00:00 EST 2015},
month = {Sun Feb 01 00:00:00 EST 2015}
}