M. A. DiPompeo

Quasar probabilities and redshifts from WISE mid-IR through GALEX UV photometry

Extreme deconvolution (XD) of broad-band photometric data can both separate stars from quasars and generate probability density functions for quasar redshifts, while incorporating flux uncertainties and missing data. Mid-infrared photometric colors are now widely used to identify hot dust intrinsic to quasars, and the release of all-sky WISE data has led to a dramatic increase in the number of IR-selected quasars. Using forced-photometry on public WISE data at the locations of SDSS point sources, we incorporate this all-sky data into the training of the XDQSOz models originally developed to select quasars from optical photometry. The combination of WISE and SDSS information is far more powerful than SDSS alone, particularly at

THE PROPERTIES OF POST-STARBURST QUASARS BASED ON OPTICAL SPECTROSCOPY

z>2

The orientation dependence of quasar single-epoch black hole mass scaling relationships

. The use of SDSS

THE VIEWING ANGLES OF BROAD ABSORPTION LINE VERSUS UNABSORBED QUASARS

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A spectroscopic survey of WISE-selected obscured quasars with the southern african large telescope

WISE photometry is comparable to the use of SDSS

Weighing obscured and unobscured quasar hosts with the cosmic microwave background

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An Infrared Excess Identified in Radio-loud Broad Absorption Line Quasars

ultraviolet

The rest‐frame ultraviolet properties of radio‐loud broad absorption line quasars

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Very Large Telescope Spectropolarimetry of Broad Absorption Line QSOs

near-IR data. We release a new public catalogue of 5,537,436 (total; 3,874,639 weighted by probability) potential quasars with probability

SPECTROPOLARIMETRY OF RADIO-SELECTED BROAD ABSORPTION LINE QUASARS

P_{\textrm{QSO}} > 0.2