Mining for Dust in Type 1 Quasars
Coleman M. Krawczyk, Gordon T. Richards, S. C. Gallagher, Karen M., Leighly, Paul C. Hewett, Nicholas P. Ross, P. B. Hall

TL;DR
This study analyzes dust extinction in approximately 35,000 quasars across a wide redshift range, revealing that a small but significant fraction exhibit reddening consistent with SMC-like dust, and that intrinsic spectral properties vary with continuum color.
Contribution
It introduces a hierarchical Bayesian approach to quantify dust reddening distributions in quasars, linking spectral properties with dust and orientation effects, which is novel in large quasar samples.
Findings
2.5% of non-BAL quasars show E(B-V)>0.1
Quasars are intrinsically bluer than the mean composite
Redder quasars have narrower Balmer lines and stronger ionizing lines
Abstract
We explore the extinction/reddening of ~35,000 uniformly selected quasars with 0<z<5.3 in order to better understand their intrinsic optical/ultraviolet spectral energy distributions. Using rest-frame optical-UV photometry taken from the Sloan Digital Sky Survey's (SDSS) 7th data release, cross-matched to WISE in the mid-infrared, 2MASS and UKIDSS in the near-infrared, and GALEX in the UV, we isolate outliers in the color distribution and find them well described by an SMC-like reddening law. A hierarchical Bayesian model with a Markov Chain Monte Carlo sampling method was used to find distributions of powerlaw indices and E(B-V) consistent with both the broad absorption line (BAL) and non-BAL samples. We find that, of the ugriz color-selected type 1 quasars in SDSS, 2.5% (13%) of the non-BAL (BAL) sample are consistent with E(B-V)>0.1 and 0.1% (1.3%) with E(B-V)>0.2. Simulations show…
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