THE WISE BLAZAR-LIKE RADIO-LOUD SOURCES: AN ALL-SKY CATALOG OF CANDIDATE [gamma]-RAY BLAZARS
We present a catalog of radio-loud candidate [gamma]-ray emitting blazars with WISE mid-infrared colors similar to the colors of confirmed [gamma]-ray blazars. The catalog is assembled from WISE sources detected in all four WISE filters, with colors compatible with the three-dimensional locus of the...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal. Supplement series 2014-11, Vol.215 (1), p.1-15 |
---|---|
Hauptverfasser: | , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | We present a catalog of radio-loud candidate [gamma]-ray emitting blazars with WISE mid-infrared colors similar to the colors of confirmed [gamma]-ray blazars. The catalog is assembled from WISE sources detected in all four WISE filters, with colors compatible with the three-dimensional locus of the WISE [gamma]-ray emitting blazars, and which can be spatially cross-matched with radio sources from one of the three radio surveys: NVSS, FIRST, and/or SUMSS. Our initial WISE selection uses a slightly modified version of previously successful algorithms. We then select only the radio-loud sources using a measure of the radio-to-IR flux, the q sub(22) parameter, which is analogous to the q sub(24) parameter known in the literature but which instead uses the WISE band-four flux at 22 [mu]m. Our final catalog contains 7855 sources classified as BL Lacs, FSRQs, or mixed candidate blazars; 1295 of these sources can be spatially re-associated as confirmed blazars. We describe the properties of the final catalog of WISE blazar-like radio-loud sources and consider possible contaminants. Finally, we discuss why this large catalog of candidate [gamma]-ray emitting blazars represents a new and useful resource to address the problem of finding low-energy counterparts to currently unidentified high-energy sources. |
---|---|
ISSN: | 0067-0049 1538-4365 |
DOI: | 10.1088/0067-0049/215/1/14 |