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The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization
Journal article   Open access

The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization

Yue Shen, Patrick B Hall, Keith Horne, Guangtun Zhu, Ian McGreer, Torben Simm, Jonathan R Trump, Karen Kinemuchi, W. N Brandt, Paul J Green, …
The Astrophysical journal. Supplement series, v 241(2), p34
15 Apr 2019
url
https://doi.org/10.3847/1538-4365/ab074fView
Published, Version of Record (VoR)Maybe Open Access (Publisher Bronze) Open

Abstract

black hole physics galaxies: active line: profiles quasars: general surveys
We present a detailed characterization of the 849 broad-line quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Our quasar sample covers a redshift range of 0.1 < z < 4.5 and is flux-limited to iPSF < 21.7 without any other cuts on quasar properties. The main sample characterization includes: (1) spectral measurements of the continuum and broad emission lines for individual objects from the coadded first-season spectroscopy in 2014, (2) identification of broad and narrow absorption lines in the spectra, and (3) optical variability properties for continuum and broad lines from multi-epoch spectroscopy. We provide improved systemic redshift estimates for all quasars and demonstrate the effects of the signal-to-noise ratio on the spectral measurements. We compile measured properties for all 849 quasars along with supplemental multi-wavelength data for subsets of our sample from other surveys. The SDSS-RM sample probes a diverse range in quasar properties and shows well-detected continuum and broad-line variability for many objects from first-season monitoring data. The compiled properties serve as the benchmark for follow-up work based on SDSS-RM data. The spectral fitting tools are made public along with this work.

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Astronomy & Astrophysics
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