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FERMILBLAZ - Fermi LAT Gamma-Ray Blazar Classification Catalog |
HEASARC Archive |
Looking beyond the gamma-ray features of blazars, interesting information can be obtained from a multiwavelength study of the sources and particularly from X-ray and radio flux. In this study the authors tested the possibility to use those two parameters to improve the performance of the network. They did not consider any optical spectroscopy data because, when considering uncertain sources, optical spectra are very often not available or not sufficiently descriptive of the nature of the source.
The gamma-ray flux was obtained by adding five time-integrated fluxes in five bands (0.1-0.3, 0.3-1, 1-3, 3-10, 10-100 GeV) from the 3FGL Catalog (Acero et al. 2015ApJS..218...23A, CDS Cat. J/ApJS/218/23). Radio and X-ray data were obtained from the Fermi LAT 4-Year AGN Catalog 3LAC (Ackermann et al. 2015ApJ...810...14A, CDS Cat. J/ApJ/810/14). Radio fluxes used were measured at frequencies of 1.4 and 0.8 GHz; the X-ray fluxes were measured in the 0.1-2.4keV range.
The complete list of 567 classified BCUs is presented in this table in which sources are ordered by increasing likelihood of a source being a BL Lac.
Optimizing neural network techniques in classifying Fermi-LAT gamma-ray sources. Kovacevic M., Chiaro G., Cutini S., Tosti G. <Mon. Not. R. Astron. Soc., 490, 4770-4777 (2019)> =2019MNRAS.490.4770K (SIMBAD/NED BibCode)
Name
The blazar source designation, 3FGL JHHMM.m+DDMM, constructed according to
the IAU Specifications for Nomenclature, in which the Right Ascension and
Declination have been truncated to 0.1 decimal minutes and 1', respectively.
The '3' refers to the four-year catalog (the first-year catalog was '1'; the
second-year catalog was '2') and 'FGL' represents Fermi Gamma-ray LAT.
RA
The right ascension of the source in the selected equinox. This was derived
by the HEASARC based on the provided Galactic Latitude and Longitude
coordinates to a precision of 10-3 degrees in the originating table.
Dec
The declination of the source in the selected equinox. This was derived by
the HEASARC based on the provided Galactic Latitude and Longitude coordinates
to a precision of 10-3 degrees in the originating table.
LII
The galactic longitude of the source, given to a precision of 10-3 degrees
in the originating table.
BII
The galactic latitude of the source, given to a precision of 10-3 degrees
in the originating table.
BLLac_Likelihood
The likelihood value corresponding to the source being classified as a BL Lac
source, based on the Artificial Neural Network analysis described in the
reference paper.
BLLac_Precision
The precision value corresponding to the source being classified as a BL Lac
source, based on the Artificial Neural Network analysis described in the
reference paper.
FSRQ_Precision
The precision value corresponding to the source being classified as a flat
spectrum radio quasar (FSRQ), based on the Artificial Neural Network analysis
described in the reference paper.
Source_Type
The classification for the source based on the Artificial Neural Network
analysis completed in this work and designated as follows:
BCU = Blazar candidates of uncertain type BL Lac = BL Lacertae FSRQ = Flat Spectrum Radio Quasar
BLLac_Likelihood_C16
The likelihood value corresponding to the source being classified as a BL
Lac, based on previous work by Chiaro et al. (2016MNRAS.462.3180C;
J/MNRAS/462/3180).
Source_Type_C16
The classification for the source based on previous work by Chiaro et al.
(2016MNRAS.462.3180C; J/MNRAS/462/3180), and designated as follows:
BCU = Blazar candidates of uncertain type BL Lac = BL Lacertae FSRQ = Flat Spectrum Radio Quasar
Class
The HEASARC Browse object classification, based on the source_type parameter.