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In the recently published 3FGL catalogue, the Fermi/LAT collaboration reports the detection of $\gamma$-ray emission from 3034 sources obtained after four years of observations. The nature of 1010 of those sources is unknown, whereas 2023…

High Energy Astrophysical Phenomena · Physics 2017-06-21 J. Lefaucheur , S. Pita

The detection of very-high-energy (VHE; $>$100 GeV) $\gamma$-ray radiation from misaligned jetted Active Galactic Nuclei (AGN) challenges the emission models that primarily explain VHE emissions from beamed AGN, i.e., blazars. Using over 16…

High Energy Astrophysical Phenomena · Physics 2025-08-25 Gunjan Tomar , Vaidehi S. Paliya , D. J. Saikia , C. S. Stalin

Blazars, one of the most extreme class of active galaxies, constitute so far the largest known population of $\gamma$-ray sources and their number is continuously growing in the Fermi catalogs. However in the latest release of the Fermi…

Machine learning models can greatly improve the search for strong gravitational lenses in imaging surveys by reducing the amount of human inspection required. In this work, we test the performance of supervised, semi-supervised, and…

Astrophysics of Galaxies · Physics 2023-08-17 Keerthi Vasan G. C. , Stephen Sheng , Tucker Jones , Chi Po Choi , James Sharpnack

Aims. We introduce the TELAMON program which is using the Effelsberg 100-m telescope to monitor the radio spectra of active galactic nuclei (AGN) under scrutiny in astroparticle physics, specifically TeV blazars and candidate…

After 10 years of operations of the Large Area Telescope (LAT), a high-energy pair-creation telescope onboard the Fermi satellite, the Fermi Collaboration has produced two major catalogs: the 4FGL and the 3FHL. These catalogs represent the…

High Energy Astrophysical Phenomena · Physics 2021-09-21 M. Nievas Rosillo , T. Hassan

Context. Although Blazars are a small fraction of the overall AGN population they are expected to be the dominant population of extragalactic sources in the hard X-ray and gamma-ray bands and have been shown to be the largest contaminant of…

Astrophysics · Physics 2008-11-26 S. Turriziani , E. Cavazzuti , P. Giommi

BL Lac objects can be extreme in two ways: with their synchrotron emission, peaking beyond 1 keV in their spectral energy distribution, or with their gamma-ray emission, peaking at multi-TeV energies up to and beyond 10-20 TeV, like 1ES…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Luigi Costamante

The study of machine learning (ML) techniques for the autonomous classification of astrophysical sources is of great interest, and we explore its applications in the context of a multifrequency data-frame. We test the use of supervised ML…

High Energy Astrophysical Phenomena · Physics 2020-10-07 Bruno Arsioli , Pedro Dedin

Convolutional Neutral Networks have been successfully applied in searching for strong lensing systems, leading to discoveries of new candidates from large surveys. On the other hand, systematic investigations about their robustness are…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-15 Zizhao He , Xinzhong Er , Qian Long , Dezi Liu , Xiangkun Liu , Ziwei Li , Yun Liu , Wenqaing Deng , Zuhui Fan

The Fermi-Large Area Telescope (LAT) First Source Catalog (1FGL) was released in February 2010 and the Fermi-LAT 2-Year Source Catalog (2FGL) appeared in April 2012, based on data from 24 months of operation. Since their releases, many…

In this work, Machine Learning (ML) methods are used to efficiently identify the unassociated sources and the Blazar Candidate of Uncertain types (BCUs) in the Fermi-LAT Third Source Catalog (3FGL). The aims are twofold: 1) to distinguish…

High Energy Astrophysical Phenomena · Physics 2020-05-08 Hubing Xiao , Haitao Cao , Junhui Fan , Denise Costantin , Gaoyong Luo , Zhiyuan Pei

Understanding the high-energy emission processes and variability patterns are two of the most challenging research problems associated with relativistic jets. In particular, the long-term (months-to-years) flux variability at very high…

High Energy Astrophysical Phenomena · Physics 2024-01-23 Vaidehi S. Paliya

To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope. Based on the spatial overlap of…

High Energy Astrophysical Phenomena · Physics 2016-05-19 Fabio Acero , Markus Ackermann , Marco Ajello , Luca Baldini , Jean Ballet , Guido Barbiellini , Denis Bastieri , Ronaldo Bellazzini , E. Bissaldi , Roger Blandford , E. D. Bloom , Raffaella Bonino , Eugenio Bottacini , J. Bregeon , Philippe Bruel , Rolf Buehler , S. Buson , G. A. Caliandro , Rob A. Cameron , R Caputo , Micaela Caragiulo , Patrizia A. Caraveo , Jean Marc Casandjian , Elisabetta Cavazzuti , Claudia Cecchi , A. Chekhtman , J. Chiang , G. Chiaro , Stefano Ciprini , R. Claus , J. M. Cohen , Johann Cohen-Tanugi , L. R. Cominsky , B. Condon , Jan Conrad , S. Cutini , F. D'Ammando , A. Angelis , F. Palma , Rachele Desiante , S. W. Digel , L. Venere , Persis S Drell , Alex Drlica-Wagner , C. Favuzzi , E. C. Ferrara , Anna Franckowiak , Prof. Yasushi Fukazawa , Prof. Stefan Funk , P. Fusco , Fabio Gargano , Dario Gasparrini , Nicola Giglietto , Paolo Giommi , Francesco Giordano , Marcello Giroletti , Tom Glanzman , Gary Godfrey , G A. Gomez-Vargas , I. A. Grenier , M. -H. Grondin , L. Guillemot , Sylvain Guiriec , M Gustafsson , D. Hadasch , A. K. Harding , M. Hayashida , Elizabeth Hays , J. W. Hewitt , A. B. Hill , Deirdre Horan , X. Hou , Giulia Iafrate , Tobias Jogler , G. J'ohannesson , Anthony S. Johnson , T. Kamae , Hideaki Katagiri , Prof. Jun Kataoka , Junichiro Katsuta , Matthew Kerr , J. Knodlseder , Prof. Dale Kocevski , M. Kuss , Helene Laffon , J. Lande , S. Larsson , Luca Latronico , Marianne Lemoine-Goumard , J. Li , L. Li , Francesco Longo , Francesco Loparco , Michael N. Lovellette , Pasquale Lubrano , J. Magill , S. Maldera , Martino Marelli , Michael Mayer , M. N. Mazziotta , Peter F. Michelson , Warit Mitthumsiri , Tsunefumi Mizuno , Alexander A. Moiseev , Maria Elena Monzani , E. Moretti , Aldo Morselli , Igor V. Moskalenko , Prof. Simona Murgia , Prof. Rodrigo Nemmen , Eric Nuss , Takashi Ohsugi , Nicola Omodei , Monica Orienti , Elena Orlando , Jonathan F. Ormes , David Paneque , J. S. Perkins , Melissa Pesce-Rollins , Prof. Vahe' Petrosian , Frederic Piron , Giovanna Pivato , Troy Porter , S. Rain`o , Riccardo Rando , Massimiliano Razzano , Soebur Razzaque , Anita Reimer , Prof. Olaf Reimer , Matthieu Renaud , Thierry Reposeur , Mr. Romain Rousseau , P. M. Parkinson , J. Schmid , A. Schulz , C. Sgr`o , Eric J Siskind , Francesca Spada , Gloria Spandre , Paolo Spinelli , Andrew W. Strong , Daniel Suson , Hiro Tajima , Hiromitsu Takahashi , T. Tanaka , Jana B. Thayer , D. J. Thompson , L. Tibaldo , Omar Tibolla , Prof. Diego F. Torres , Gino Tosti , Eleonora Troja , Yasunobu Uchiyama , G. Vianello , B. Wells , Kent Wood , M. Wood , Manal Yassine , Stephan Zimmer

Blazars dominate the extragalactic $\gamma$-ray sky and show pronounced flares. Using public Fermi-LAT light curves for 732 blazars with secure redshifts, I implement an automated pipeline to identify and characterize $\gamma$-ray bursts…

High Energy Astrophysical Phenomena · Physics 2025-08-29 Matteo Cerruti

The extragalactic $\gamma$-rays sky observed by Fermi-Large Area Telescope (LAT) is dominated by blazars. In the fourth release of the Fermi-LAT Point Source Catalog (4FGL), are sources showing a multifrequency behavior similar to that of…

We report on observations of TeV-selected AGN made during the first 5.5 months of observations with the Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope (Fermi). In total, 28 TeV AGN were selected for study. The Fermi…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-14 S. J. Fegan , D. Sanchez

The Fermi gamma-ray space telescope has revolutionized our view of the gamma-ray sky and the high energy processes in the Universe. While the number of known gamma-ray emitters has increased by orders of magnitude since the launch of Fermi,…

High Energy Astrophysical Phenomena · Physics 2019-05-01 I. Liodakis , D. Blinov

We investigate the use of optical photometric variability to select and identify blazars in large-scale time-domain surveys, in part to aid in the identification of blazar counterparts to the ~30% of gamma-ray sources in the Fermi 2FGL…

The second Fermi-LAT source catalog (2FGL) is the deepest survey of the gamma-ray sky ever compiled, containing 1873 sources that constitute a very complete sample down to an energy flux of about 10^(-11) erg cm^(-2) s^(-1). While…

High Energy Astrophysical Phenomena · Physics 2013-07-01 M. Doert , M. Errando
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