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WIBRALS - WISE Blazar-like Radio-Loud Source (WIBRaLS) Catalog |
HEASARC Archive |
The WISE magnitudes in the [3.4], [4.6], [12] and [22] um nominal filters are in the Vega system. The values of three WISE magnitudes, namely [3.4], [4.6], and [12], and of the colors derived using those magnitudes, have been corrected for galactic extinction according to the extinction law presented by Draine (2003, ARA&A, 41, 241). In their study, the authors adopt the nomenclature proposed in the Multi-wavelength Blazar Catalog (BZCat) that labels BL Lac objects as 'BZBs' and flat-spectrum radio quasars (FSRQs) as 'BZQs'.
The WISE blazar-like radio-loud sources: an all-sky catalog of candidate gamma-ray blazars. D'Abrusco R., Massaro F., Paggi A., Smith H.A., Masetti N., Landoni M., Tosti G. <Astrophys. J. Suppl., 215, 14 (2014)> =2014ApJS..215...14D (SIMBAD/NED BibCode)
Name
The WIBRaLS catalog source designation using the 'WB' prefix and the
truncated J2000.0 equatorial coordinates, e.g., 'WB J0004-4736'.
WISE_Name
The WISE designation of the source.
RA
The Right Ascension of the WISE source position in the selected equinox.
Dec
The Declination of the WISE source position in the selected equinox.
LII
The Galactic Longitude of the WISE source position.
BII
The Galactic Latitude of the WISE source position.
W1W2_Color
The WISE [3.4] - [4.6] um (w1 - w2) color of the
source corrected for Galactic absorption.
W1W2_Color_Error
The uncertainty in the WISE [3.4] - [4.6] um (w1 - w2)
color of the source.
W2W3_Color
The WISE [4.6] - [12] um (w2 - w3) color of the
source corrected for Galactic absorption.
W2W3_Color_Error
The uncertainty in the WISE [4.6] - [12] um (w2 - w3)
color of the source.
W3W4_Color
The WISE [12] - [22] um (w3 - w4) color of the
source corrected for Galactic absorption.
W3W4_Color_Error
The uncertainty in the WISE [12] - [22] um (w3 - w4)
color of the source.
BZB_Region_Score
The score for the BZB Region of the locus for the given
source (see Section 2.1 of the reference paper for more details).
Mixed_Region_Score
The score for the Mixed Region of the locus for the given
source (see Section 2.1 of the reference paper for more details).
BZQ_Region_Score
The score for the BZQ Region of the locus for the given
source (see Section 2.1 of the reference paper for more details).
Blazar_Type
The spectral type of the blazar (see Section 2.1 of the
reference paper for more details).
Blazar_Type_Grade
The class or grade of the blazar type, A, B, C or D.
For each distinct region of the model (BZB, BZQ, or mixed), class A sources
have a score s >= s90%, class B sources have a score s of s60% <= s <
s_90_%, and class C sources have a score of s20% <= s < s60%, where s20%
is the 20th percentile of the score distribution, s60% is the 60th
percentile of the score distribution and s90% is the 90th percentile of the
score distribution. The meaning of class D is not explicitly stated in the
paper but appears to refer to cases where an object has scores corresponding
to or just below grade C in 2 regions of the locus.
Radio_Name
The name of the final radio counterpart associated with the WISE
source, taken from either the NVSS, SUMSS or FIRST surveys, matched using the
optimal radii established in Section 2.2 of the reference paper.
Q_22
The value of the q22 parameter, defined as the logarithm of the ratio
of the WISE 22-micron to the radio flux densities. The authors in general
used the flux density at 1.4 GHz as the radio flux density Sradio. Since
flux density measurements at 1.4 GHz are not available in the SUMSS survey,
for the SUMSS counterparts, they used the flux densities at 843 MHz instead.
A well known property of blazars is the flatness of their radio spectra which
extends up to low radio frequencies well below 1 GHz. For this reason, the use
of the flux density at 843 MHz instead of the flux density at 1.4 GHz to
estimate the q22 parameter negligibly affects their analysis.
Class
Browse Object Classification