Red and Reddened Quasars in the Sloan Digital Sky Survey
arXiv:astro-ph/0305305 · doi:10.1086/377014
Abstract
We investigate the continuum and emission line properties of 4576 SDSS quasars as a function of their optical/UV SEDs. The optical/UV color distribution of our sample is roughly Gaussian, but with a red tail; we distinguish between 1) intrinsically blue (optically flat) quasars, 2) intrinsically red (optically steep) quasars, and 3) the 273 (6%) of our quasars whose continua are inconsistent with a single power-law and appear redder due to SMC-like dust reddening rather than synchrotron emission. The color distribution suggests that the population of moderately dust reddened broad-line quasars is smaller than that of unobscured quasars, but we estimate that a further 10% of the luminous quasar population is missing from the SDSS sample because of dust extinction with E(B-V)<0.5. We also investigate the emission and absorption line properties of these quasars as a function of color with regard to Boroson & Green type eigenvectors. Intrinsically red (optically steep) quasars tend to have narrower Balmer lines and weaker CIV, CIII], HeII and 3000A bump emission as compared with bluer (optically flatter) quasars. The change in strength of the 3000A bump appears to be dominated by the Balmer continuum and not by FeII emission. The dust reddened quasars have even narrower Balmer lines and weaker 3000A bumps, in addition to having considerably larger equivalent widths of [OII] and [OIII] emission. The fraction of broad absorption line quasars (BALQSOs) increases from ~3.4% for the bluest quasars to perhaps as large as 20% for the dust reddened quasars, but the intrinsic color distribution is affected by dust reddening. (abridged)
arXiv comment37 pages, 10 figures (3 color), 2 tables, accepted by AJ. For a version with higher quality figures, see ftp://astro.princeton.edu/gtr/redqsos/RichardsGT_redqsos.revised3.preprint.ps
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- Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.1292
- DESI Mg II Absorbers: Extinction Characteristics & Quasar Redshift Accuracy
- Supernovae Light Curves: An Argument for a New Distance Modulus
- Aplicando modelos de granos de polvo con propiedades meteoriticas al continuo ionizante de algunos Nucleos Activos de Galaxias
- Evidence for the connection between star formation rate and evolutionary phases of quasars
- A quasar shedding its dust cocoon at redshift 2
- The Compact Star-Forming Galaxies at in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
- There Are (super)Giants in the Sky: Searching for Misidentified Massive Stars in Algorithmically-Selected Quasar Catalogs
- Constraining the AGN tori at cosmic noon using high-resolution JWST imaging and simultaneous SED fitting
- Near infrared imaging of the broad absorption line quasar BAL QSO 0134+3253
- Revealing a strongly reddened, faint active galactic nucleus population by stacking deep co-added images
- Giant radio quasars: composite optical spectra