J/ApJ/901/3         Blazar Radio and Optical Survey (BROS)   (Itoh+, 2020)

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., Ohta K., Doi A., Morokuma T., Kawabata K.S., Tanaka Y.T. <Astrophys. J., 901, 3-3 (2020)> =2020ApJ...901....3I 2020ApJ...901....3I (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; BL Lac objects ; Radio sources Keywords: blazars - radio active galactic nuclei - catalogs 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 88211 sources located at decl. δ>-40° and outside the galactic plane (|b|>10°). We list compact flat-spectrum radio sources of α>-0.6 (α is defined as Fν∝να) from 0.15GHz TGSS to 1.4GHz 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. Description: BROS (Blazar Radio and Optical Survey) is a new blazar candidate catalog, which includes 88,211 sources located at declination DE>-40° and outside the Galactic Plane |b|>10°. We list compact flat-spectrum radio sources of alpha>-0.6 from 0.15GHz TGSS and 1.4GHz NVSS catalogs. We further identify optical counterparts of the selected sources by cross-matching with the Pan-STARRS1 photometric data. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 325 88211 BROS Catalog -------------------------------------------------------------------------------- See also: II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/A+A/598/A78 : The GMRT 150MHz all-sky radio survey (TGSS) (Intema+, 2017) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- BROS-ID source ID (BROS-ID) 19- 31 F13.9 deg RAdeg Right ascension (J2000) from TGSS-NVSS catalog (spindx-RA) 33- 45 F13.9 deg DEdeg Declination (J2000) from TGSS-NVSS catalog (spindx-Dec) 47- 59 F13.9 Jy FTGSS TGSS 150MHz total flux (spindx-TGSS-Flux) 61- 71 F11.9 Jy e_FTGSS TGSS 150MHz total flux error (spindx-TGSS-Flux-error) 73- 84 F12.9 Jy FNVSS NVSS 1.4GHz total flux (spindx-NVSS-Flux) 86- 96 F11.9 Jy e_FNVSS NVSS 1.4GHz total flux error (spindx-NVSS-Flux-error) 98-105 F8.5 --- SpIndex Spectral index between 0.15GHz and 1.4GHz (spindx-Spectral-Index) 107-115 F9.6 --- e_SpIndex Spectral index error (spindx-Spectral-Index-error) 117 A1 --- Flag [QEGB] Source type flag (SourceFlag) (1) 119-126 F8.6 --- Rcomp Radio compactness defined as totalflux/peakflux (NVSS) (radio-Compactness) 128-136 F9.7 --- e_Rcomp Radio compactness error (radio-Compactness-error) 138-145 F8.3 --- Ocomp ?=-999 Optical compactness defined as MPSF-MKron (PS1, i- band) (optical-Compactness) 147-155 F9.4 --- e_Ocomp ?=-999 Optical compactness error (optical-Compactness-error) 157-167 F11.6 arcsec Sep ?=-999 Source separation angle between TGSS-NVSS and PS1 catalog position (PS1-BROS-separation) 169-182 F14.9 deg RAPdeg ?=-999 r-band R.A. position (PS1-r-RA) 184-197 F14.9 deg DEPdeg ?=-999 r-band Decl. position (PS1-r-Dec) 199-207 F9.4 mag gmagK ?=-999 g-band Kron magnitude (PS1-g-Kronmag) 209-218 F10.5 mag e_gmagK ?=-999 g-band Kron magnitude error (PS1-g-Kronmag-error) 220-228 F9.4 mag gmagP ?=-999 g-band PSF magnitude (PS1-g-PSFmag) 230-240 F11.5 mag e_gmagP ?=-999 g-band PSF magnitude error (PS1-g-PSFmag-error) 242-250 F9.4 mag rmagK ?=-999 r-band Kron magnitude (PS1-r-Kronmag) 252-261 F10.5 mag e_rmagK ?=-999 r-band Kron magnitude error (PS1-r-Kronmag-error) 263-271 F9.4 mag rmagP ?=-999 r-band PSF magnitude (PS1-r-PSFmag) 273-283 F11.5 mag e_rmagP ?=-999 r-band PSF magnitude error (PS1-r-PSFmag-error) 285-293 F9.4 mag imagK ?=-999 i-band Kron magnitude (PS1-i-Kronmag) 295-304 F10.5 mag e_imagK ?=-999 i-band Kron magnitude error (PS1-i-Kronmag-error) 306-314 F9.4 mag imagP ?=-999 i-band PSF magnitude (PS1-i-PSFmag) 316-325 F10.5 mag e_imagP ?=-999 i-band PSF magnitude error (PS1-i-PSFmag-error) -------------------------------------------------------------------------------- Note (1): Source type flag as follows: Q = source have a PS1 candidate and not classified as GPS source E = source, which is located in a quasar-like (elliptical-like) population G = GPS source B = source that do not have a PS1-candidate and not classified as GPS source -------------------------------------------------------------------------------- Acknowledgements: Ryosuke Itoh, itoh(at)bao.city.ibara.okayama.jp
(End) Patricia Vannier [CDS] 10-Mar-2021
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line