Blazar Radio and Optical Survey (BROS): A Catalog of Blazar Candidates Showing Flat Radio Spectrum and Their Optical Identification in Pan-STARRS1 Surveys

  • Itoh R
  • Utsumi Y
  • Inoue Y
  • et al.
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Abstract

Utilizing the latest and the most sensitive radio and optical catalogs, we completed a new blazar candidate catalog, Blazar Radio and Optical Survey (BROS), which includes 88,211 sources located at decl. δ  > −40° and outside the galactic plane ( ). We list compact flat-spectrum radio sources of α  > −0.6 ( α is defined as F ν ∝ ν α ) from 0.15 GHz TGSS to 1.4 GHz NVSS catalogs. We further identify optical counterparts of the selected sources by cross-matching with Pan-STARRS1 photometric data. Color–color and color–magnitude plots for the selected BROS sources clearly show two distinct populations, a “quasar-like” population consisting of both flat-spectrum radio quasars and BL Lac type objects. On the other hand, an “elliptical-like” population of mostly BL Lac type objects is buried in the elliptical galaxy. The latter population is also reported in previous catalogs, but the BROS catalog provided a new larger sample of this population, due to the lower radio flux threshold of our selection. Model calculations show that the “elliptical-like” population consists of elliptical galaxies located at redshift z  ≲ 0.5, which is also supported by the logN-logS distribution of the power-law index of 1.49 ± 0.05. This BROS catalog is useful for identifying the electromagnetic counterparts of ultra-high-energy cosmic rays and PeV neutrinos recently detected by IceCube, as well as nearby BL Lac objects detectable by future high-sensitivity TeV telescopes, such as the Cherenkov Telescope Array.

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Itoh, R., Utsumi, Y., Inoue, Y., Ohta, K., Doi, A., Morokuma, T., … Tanaka, Y. T. (2020). Blazar Radio and Optical Survey (BROS): A Catalog of Blazar Candidates Showing Flat Radio Spectrum and Their Optical Identification in Pan-STARRS1 Surveys. The Astrophysical Journal, 901(1), 3. https://doi.org/10.3847/1538-4357/abab07

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