Probabilistic classification of unassociated Fermi-LAT sources using machine learning methods has an implicit assumption that the distributions of associated and unassociated sources are the same as a function of source parameters, which is not the case for the Fermi-LAT catalogs. The problem of different distributions of training and testing (or target) datasets as a function of input features (covariates) is known as the covariate shift. In this paper, we, for the first time, quantitatively estimate the effect of the covariate shift on the multi-class classification of Fermi-LAT sources. We introduce sample weights proportional to the ratio of unassociated to associated source probability density functions so that associated sources in ar...
A large fraction of the gamma-ray sources presented in the Third Fermi-LAT source catalog (3FGL) is ...
The Fermi Large Area Telescope First Source Catalog (1FGL) provided spatial, spectral, and temporal ...
During its first 2 years of mission the Fermi-LAT instrument discovered more than 1,800 gamma-ray so...
Version 1: These are data products connected to https://arxiv.org/abs/2307.09584, where an analysis...
Context. Classification of sources is one of the most important tasks in astronomy. Sources detected...
We have investigated a number of factors that can have significant impacts on the classification per...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
Approximately one-third of existing $\gamma$-ray sources identified by the $\textit{Fermi Gamma-Ray ...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The small angular scale fluctuations of the (on large scale) isotropic gamma-ray background (IGRB) c...
A large fraction of the gamma-ray sources presented in the Third Fermi-LAT source catalog (3FGL) is ...
The Fermi Large Area Telescope First Source Catalog (1FGL) provided spatial, spectral, and temporal ...
During its first 2 years of mission the Fermi-LAT instrument discovered more than 1,800 gamma-ray so...
Version 1: These are data products connected to https://arxiv.org/abs/2307.09584, where an analysis...
Context. Classification of sources is one of the most important tasks in astronomy. Sources detected...
We have investigated a number of factors that can have significant impacts on the classification per...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
Approximately one-third of existing $\gamma$-ray sources identified by the $\textit{Fermi Gamma-Ray ...
The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial, spectral, and tem...
The small angular scale fluctuations of the (on large scale) isotropic gamma-ray background (IGRB) c...
A large fraction of the gamma-ray sources presented in the Third Fermi-LAT source catalog (3FGL) is ...
The Fermi Large Area Telescope First Source Catalog (1FGL) provided spatial, spectral, and temporal ...
During its first 2 years of mission the Fermi-LAT instrument discovered more than 1,800 gamma-ray so...