The FIRST-2MASS Red Quasar Survey
Eilat Glikman (1) David J. Helfand (2) Richard L. White (3) Robert H., Becker (4,5) Michael D. Gregg (4,5), Mark Lacy (6) ((1) Caltech, (2), Columbia University, (3) STScI, (4) UC Davis, (5) IGPP-LLNL, (6) Spitzer, Science Center)

TL;DR
This study introduces an efficient radio and infrared color selection method to identify red quasars, revealing a significant population missed by optical surveys and estimating their contribution to the overall quasar population.
Contribution
The paper presents a novel combined radio and infrared color selection technique that effectively finds red quasars, expanding the known quasar population beyond optical survey limits.
Findings
Approximately 50% success rate in identifying red quasars with the new criteria
Red quasars constitute 25-60% of the quasar population at certain magnitudes
Over 10% of quasars are missed in optical surveys due to reddening
Abstract
Combining radio observations with optical and infrared color selection -- demonstrated in our pilot study to be an efficient selection algorithm for finding red quasars -- we have obtained optical and infrared spectroscopy for 120 objects in a complete sample of 156 candidates from a sky area of 2716 square degrees. Consistent with our initial results, we find our selection criteria -- J-K>1.7, R-K>4.0 -- yield a ~50% success rate for discovering quasars substantially redder than those found in optical surveys. Comparison with UVX- and optical color-selected samples shows that >~ 10% of the quasars are missed in a magnitude-limited survey. Simultaneous two-frequency radio observations for part of the sample indicate that a synchrotron continuum component is ruled out as a significant contributor to reddening the quasars' spectra. We go on to estimate extinctions for our objects assuming…
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