D. Salvetti

Blazar flaring patterns (B-FlaP) classifying blazar candidate of uncertain type in the third Fermi-LAT catalogue by artificial neural networks

The Fermi Large Area Telescope (LAT) is currently the most important facility for investigating the GeV

A CANDIDATE OPTICAL COUNTERPART TO THE MIDDLE AGED γ -RAY PULSAR PSR J1741–2054

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Searching for the optical counterparts of two young γ-ray pulsars

-ray sky. With Fermi LAT more than three thousand

Large Binocular Telescope observations of PSR J2043+2740*

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A systematic analysis of the XMM-Newton background: IV

-ray sources have been discovered so far. 1144 (

Observations of one young and three middle-aged γ-ray pulsarswith the Gran Telescopio Canarias

sim40%

Characterising the Fermi-LAT BCUs: Optical Spectroscopy and Neural Networks

) of the sources are active galaxies of the blazar class, and 573 (

3FGLzoo: classifying 3FGL unassociated Fermi-LAT γ-ray sources by artificial neural networks

sim20%

A multiwavelength investigation of candidate millisecond pulsars in unassociated γ-ray sources

) are listed as Blazar Candidate of Uncertain type (BCU), or sources without a conclusive classification. We use the Empirical Cumulative Distribution Functions (ECDF) and the Artificial Neural Networks (ANN) for a fast method of screening and classification for BCUs based on data collected at

Optical Counterparts of Undetermined Type γ-Ray Active Galactic Nuclei with Blazar-Like Spectral Energy Distributions

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