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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

Fast radio bursts (FRBs) are one of the most exciting new mysteries of astrophysics. Their origin is still unknown, but recent observations seem to link them to soft gamma repeaters and, in particular, to magnetar giant flares (MGFs). The…

High Energy Astrophysical Phenomena · Physics 2023-01-18 Giacomo Principe , Niccolò Di Lalla , Leonardo Di Venere , Michela Negro , Francesco Longo

While supernova remnants (SNRs) are widely thought to be powerful cosmic-ray accelerators, indirect evidence comes from a small number of well-studied cases. Here we systematically determine the gamma-ray emission detected by the Fermi…

High Energy Astrophysical Phenomena · Physics 2015-07-14 F. de Palma , T. J. Brandt , J. W. Hewitt , G. Johannesson , L. Tibaldo

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

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

Nearly 50% of all sources detected by the Fermi Large Area Telescope are classified as blazars or blazar candidates, one of the most elusive classes of active galaxies. Additional blazars can also be hidden within the sample of unidentified…

High Energy Astrophysical Phenomena · Physics 2020-07-13 E. J. Marchesini , A. Paggi , F. Massaro , N. Masetti , R. D'Abrusco , I. Andruchow

Dark matter annihilations taking place in nearby subhalos could appear as gamma-ray sources without detectable counterparts at other wavelengths. In this study, we consider the collection of unassociated gamma-ray sources reported by the…

High Energy Astrophysical Phenomena · Physics 2015-12-23 Bridget Bertoni , Dan Hooper , Tim Linden

We are compiling a new list of gamma-ray jetted active galactic nuclei (AGN), starting from the fourth catalog of point sources of the Fermi Large Area Telescope (LAT). Our aim is to prepare a list of jetted AGN with known redshifts and…

High Energy Astrophysical Phenomena · Physics 2021-10-06 L. Foschini , M. L. Lister , S. Antón , M. Berton , S. Ciroi , M. J. M. Marchã , M. Tornikoski , E. Järvelä , P. Romano , S. Vercellone , E. Dalla Bontà

Blazars are among the most studied sources in high-energy astrophysics as they form the largest fraction of extragalactic gamma-ray sources and are considered prime candidates for being the counterparts of high-energy astrophysical…

During its first four years of scientific observations, the Fermi Large Area Telescope (Fermi-LAT) detected 3033 $\gamma$-ray sources above a 4$\sigma$ significance level. Although most of the extra-Galactic sources are active galactic…

High Energy Astrophysical Phenomena · Physics 2019-08-15 G. La Mura , G. Chiaro , S. Ciroi , P. Rafanelli , D. Salvetti , M. Berton , V. Cracco

The classification of Gamma-Ray Bursts has long been an unresolved problem. Early long and short burst classification based on duration is not convincing due to the significant overlap in duration plot, which leads to different views on the…

High Energy Astrophysical Phenomena · Physics 2024-12-10 Jia-Ming Chen , Ke-Rui Zhu , Zhao-Yang Peng , Li Zhang

Blazars and in particular the subclass of high synchrotron peaked Active Galactic Nuclei are among the main targets for the present generation of Imaging Atmospheric Cherenkov Telescopes (IACTs) and will remain of great importance for very…

High Energy Astrophysical Phenomena · Physics 2020-01-08 G. Chiaro , M. Meyer , M. Di Mauro , D. Salvetti , G. La Mura , D. J. Thompson

Studying unidentified {\gamma}-ray sources is important as they may hide new discoveries. We conducted a multiwavelength analysis of 13 unidentified Fermi-LAT sources in the 3FGL catalog that have no known counterparts (Unidentified…

High Energy Astrophysical Phenomena · Physics 2021-07-14 Jean Damascène Mbarubucyeye , Felicia Krauß , Pheneas Nkundabakura

Classifying Active Galactic Nuclei (AGN) is a challenge, especially for BL Lac Objects (BLLs), which are identified by their weak emission line spectra. To address the problem of classification, we use data from the 4th Fermi Catalog, Data…

High Energy Astrophysical Phenomena · Physics 2023-09-12 Nathaniel Cooper , Maria Giovanna Dainotti , Aditya Narendra , Ioannis Liodakis , Malgorzata Bogdan

The Large Area Telescope (LAT) aboard the $Fermi$ spacecraft routinely observes high-energy emission from gamma-ray bursts (GRBs). Here we present the second catalog of LAT-detected GRBs, covering the first 10 years of operations, from 2008…

High Energy Astrophysical Phenomena · Physics 2019-06-28 M. Axelsson , E. Bissaldi , N. Omodei , G. Vianello

The third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC) is presented. It is based on the third Fermi-LAT catalog (3FGL) of sources detected between 100 MeV and 300 GeV with a Test Statistic (TS) greater than 25,…

High Energy Astrophysical Phenomena · Physics 2015-09-16 M. Ackermann , M. Ajello , W. Atwood , L. Baldini , J. Ballet , G. Barbiellini , D. Bastieri , J. Gonzalez , R. Bellazzini , E. Bissaldi , R. Blandford , E. Bloom , R. Bonino , E. Bottacini , T. Brandt , J. Bregeon , R. Britto , P. Bruel , R. Buehler , S. Buson , G. Caliandro , R. Cameron , M. Caragiulo , P. Caraveo , J. Casandjian , E. Cavazzuti , C. Cecchi , E. Charles , A. Chekhtman , C. Cheung , J. Chiang , G. Chiaro , S. Ciprini , R. Claus , J. Cohen-Tanugi , L. Cominsky , J. Conrad , S. Cutini , R. D'Abrusco , F. D'Ammando , A. Angelis , R. Desiante , S. Digel , L. Venere , P. Drell , C. Favuzzi , S. Fegan , E. Ferrara , J. Finke , W. Focke , A. Franckowiak , L. Fuhrmann , A. Furniss , P. Fusco , F. Gargano , D. Gasparrini , N. Giglietto , P. Giommi , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , I. Grenier , J. Grove , S. Guiriec , J. W. Hewitt , A. Hill , D. Horan , G. J'ohannesson , A. Johnson , W. Johnson , J. Kataoka , M. Kuss , G. Mura , S. Larsson , L. Latronico , C. Leto , J. Li , L. Li , F. Longo , F. Loparco , B. Lott , M. Lovellette , P. Lubrano , G. Madejski , M. Mayer , M. Mazziotta , J. McEnery , P. Michelson , T. Mizuno , A. Moiseev , M. Monzani , A. Morselli , I. Moskalenko , S. Murgia , E. Nuss , M. Ohno , T. Ohsugi , R. Ojha , N. Omodei , M. Orienti , E. Orlando , A. Paggi , D. Paneque , J. Perkins , M. Pesce-Rollins , F. Piron , G. Pivato , T. Porter , S. Rain`o , R. Rando , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , R. Romani , D. Salvetti , M. Schaal , F. Schinzel , A. Schulz , C. Sgr`o , E. Siskind , K. Sokolovsky , F. Spada , G. Spandre , P. Spinelli , L. Stawarz , D. Suson , H. Takahashi , T. Takahashi , Y. Tanaka , J. Thayer , J. Thayer , L. Tibaldo , D. Torres , E. Torresi , G. Tosti , E. Troja , Y. Uchiyama , G. Vianello , B. Winer , K. Wood , S. Zimmer

We present a framework for detecting transient gamma-ray phenomena in a controlled environment by combining end-to-end simulations of the Fermi-LAT sky with self-supervised spatio-temporal deep learning. We generate a ten-year synthetic…

The Fermi/LAT telescope is an efficient blazar-detector in the MeV/GeV range. More than 1100 (900) blazars detected above 100 MeV (10 GeV) are clearly associated to BL Lacertae or Flat Spectrum Radio Quasar objects in the Fermi/LAT 3FGL…

High Energy Astrophysical Phenomena · Physics 2017-10-02 Julien Lefaucheur , Catherine Boisson , Paolo Goldoni , Santiago Pita

The Large Area Telescope (LAT) onboard the Fermi satellite is exploring the gamma-ray sky in the energy range above 20MeV. We have developed a method to reconstruct the energy spectra of the gamma rays detected by the Fermi LAT instrument…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 M. N. Mazziotta

In the third catalog of active galactic nuclei detected by the Fermi-LAT (3LAC) Clean Sample, there are 402 blazars candidates of uncertain type (BCU). Due to the limitations of astronomical observation or intrinsic properties, it is…

High Energy Astrophysical Phenomena · Physics 2019-03-06 Shi-Ju Kang , Junhui Fan , Weiming Mao , Qingwen Wu , Jianchao Feng , Yue Yin