Unveiling the nature of the unidentified gamma-ray sources I: a new method for the association of gamma-ray blazars
R. D'Abrusco, F. Massaro, A. Paggi, N. Masetti, G. Tosti, M., Giroletti, H.A. Smith

TL;DR
This paper introduces a refined 3D color space method using PCA for identifying gamma-ray blazar candidates with high efficiency and completeness, improving association accuracy in gamma-ray source catalogs.
Contribution
A new PCA-based 3D color locus method for gamma-ray blazar identification, enhancing previous 2D approaches with higher completeness and efficiency.
Findings
Achieved ~81% completeness in blazar candidate identification.
Attained ~97% efficiency in the new association method.
Produced a catalog of gamma-ray blazar candidates with multi-frequency data.
Abstract
We present a new method for identifying blazar candidates by examining the locus, i.e. the region occupied by the Fermi gamma-ray blazars in the three-dimensional color space defined by the WISE infrared colors. This method is a refinement of our previous approach that made use of the two-dimensional projection of the distribution of WISE gamma-ray emitting blazars (the Strip) in the three WISE color-color planes (Massaro et al. 2012a). In this paper, we define the three-dimensional locus by means of a Principal Component (PCs) analysis of the colors distribution of a large sample of blazars composed by all the ROMA-BZCAT sources with counterparts in the WISE All-Sky Catalog and associated to gamma-ray source in the second Fermi LAT catalog (the WISE Fermi Blazars sample, WFB). Our new procedure yields a total completeness of c~81% and total efficiency of e~97%. We also obtain local…
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