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An Infrared Excess Identified in Radio-Loud Broad Absorption Line Quasars
M. A. DiPompeo, J. C. Runnoe, M. S. Brotherton +1
If broad absorption line (BAL) quasars represent a high covering fraction evolutionary state (even if this is not the sole factor governing the presence of BALs), it is expected th…
The Properties of Post-Starburst Quasars Based on Optical Spectroscopy
Sabrina L. Cales, Michael S. Brotherton, Zhaohui Shang +8
We present optical spectroscopy of a sample of 38 post-starburst quasars (PSQs) at z ~ 0.3, 29 of which have morphological classifications based on Hubble Space Telescope imaging.…
The orientation dependence of quasar single-epoch black hole mass scaling relationships
Jessie C. Runnoe, Michael Brotherton, Zhaohui Shang +2
Black hole masses are estimated for radio-loud quasars using several self-consistent scaling relationships based on emission-line widths and continuum luminosities. The emission li…
The rest-frame ultraviolet properties of radio-loud broad absorption line quasars
M. A. DiPompeo, M. S. Brotherton, S. L. Cales +1
We recently presented radio observations of a large sample of radio-loud broad absorption line (BAL) quasars from the SDSS and FIRST surveys, as well as a well matched sample of un…
The Optical and Ultraviolet Emission-Line Properties of Bright Quasars with Detailed Spectral Energy Distributions
Baitian Tang, Zhaohui Shang, Qiusheng Gu +2
We present measurements and statistical properties of the optical and ultraviolet emission lines present in the spectra of 85 bright quasars which have detailed spectral energy dis…
Updating quasar bolometric luminosity corrections. II. Infrared bolometric corrections
Jessie C. Runnoe, Michael S. Brotherton, Zhaohui Shang
We present infrared bolometric luminosity corrections derived from the detailed spectral energy distributions of 62 bright quasars of low- to moderate-redshift (z=0.03-1.4). At 1.5…