Identifying quasars with astrometric and mid-infrared methods from APOP and ALLWISE

Abstract

Context. Quasars are spatially stationary, and they are essential objects in astrometry when defining reference frames. However, the census of quasars is far from complete. Mid-infared colors can be used to find quasar candidates because active galactic nuclei (AGNs) show a peculiar appearance in mid-infrared color, but these methods are incapable of separating quasars from AGNs.
Aims: The aim of our study is to use astrometric and mid-infrared methods to select quasars and get a reliable quasar candidates catalog.
Methods: We used a near-zero proper motion criterion in conjuction with WISE [W1-W2] color to select quasar candidates. The [W1-W2] color criterion is defined by the linear boundary of two samples: LAMOST DR5 quasars, which serve as the quasar sample, and LAMOST DR5 stars and galaxies, which serve as the non-quasar sample. The contamination and completeness are evaluated.
Results: We present a catalog of 662 753 quasar candidates, with a completeness of about 75% and a reliability of 77.2%.

The catalog of AGN candidates is only available in electronic form at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/618/A144