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The Fermi Large Area Telescope (LAT) is currently the most important facility for investigating the GeV $\gamma$-ray sky. With Fermi LAT more than three thousand $\gamma$-ray sources have been discovered so far. 1144 ($\sim40\%$) of the…

High Energy Astrophysical Phenomena · Physics 2016-09-07 G. Chiaro , D. Salvetti , G. La Mura , M. Giroletti , D. J. Thompson , D. Bastieri

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

We present an analysis of the optical spectra available in the Sloan Digital Sky survey data release nine (SDSS DR9) for the blazars listed in the ROMA-BZCAT and for the gamma-ray blazar candidates selected according to their IR colors.…

High Energy Astrophysical Phenomena · Physics 2015-03-16 F. Massaro , N. Masetti , R. D'Abrusco , A. Paggi , S. Funk

\textbf{Context.} Deep optical surveys open the avenue for find large numbers of BL Lac objects that are hard to identify because they lack the unique properties classifying them as such. While radio or X-ray surveys typically reveal dozens…

Astrophysics of Galaxies · Physics 2014-09-30 S. D. Kügler , K. Nilsson , J. Heidt , J. Esser , T. Schultz

A majority of blazars exhibit variable emission across the entire electromagnetic spectrum, observed over various time scales. In particular, discernible periodic patterns are detected in the $\gamma$-ray light curves of a few blazars, such…

High Energy Astrophysical Phenomena · Physics 2025-06-18 Alba Rico , A. Domínguez , P. Peñil , M. Ajello , S. Buson , S. Adhikari , M. Movahedifar

The latest source catalog of the Fermi-LAT telescope contains more than 7000 $\gamma$-ray sources at GeV energies, with the two dominant source classes thought to be blazars and rotation-powered pulsars. Our target is the identification of…

High Energy Astrophysical Phenomena · Physics 2024-02-09 Martin G. F. Mayer , Werner Becker

Recent works have developed samples of blazars from among the Fermi-LAT unassociated sources via machine learning comparisons with known blazar samples. Continued analysis of these new blazars tests the predictions of the blazar sequence…

High Energy Astrophysical Phenomena · Physics 2023-07-17 Stephen Kerby , Abraham D. Falcone

A direct search of $\gamma$-ray emission centered on multi-frequency selected candidates is a valuable complementary approach to the standard search adopted in current $\gamma$-ray Fermi-LAT catalogs. Our candidates are part of the 2WHSP…

High Energy Astrophysical Phenomena · Physics 2017-02-15 Bruno Arsioli , Yu-Ling Chang

Blazars represent the most abundant class of high-energy extragalactic $\gamma$-ray sources. The subset of blazars known as BL Lac objects is on average closer to Earth and characterized by harder spectra at high energy than the whole…

High Energy Astrophysical Phenomena · Physics 2016-05-26 M. Di Mauro , F. Donato , G. Lamanna , D. A. Sanchez , P. D. Serpico

The Large Area Telescope (LAT) aboard the Fermi satellite allows us to study the high-energy gamma-ray sky with unprecedented sensitivity. However, the origin of 31% of the detected gamma-ray sources remains unknown. This population of…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Hannes-S. Zechlin , Dieter Horns

We present the results of our analysis devoted to the research of sources emitting in the energy bands surveyed by both the Swift-BAT and the Fermi-LAT telescopes. We cross-correlate the Fermi-LAT 1-year point source catalogue (1FGL) of…

High Energy Astrophysical Phenomena · Physics 2015-05-27 A. Maselli , G. Cusumano , E. Massaro , A. Segreto , V. La Parola , A. Tramacere , I. Donnarumma

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

Blazars are the dominant type of extragalactic sources at microwave and at $\gamma$-ray energies. In the most energetic part of the electromagnetic spectrum (E>100GeV) a large fraction of high Galactic latitude sources are blazars of the…

High Energy Astrophysical Phenomena · Physics 2015-06-24 B. Arsioli , B. Fraga , P. Giommi , P. Padovani , P. M. Marrese

We aim to test if a blazar candidate of uncertain-type (BCU) in the third Fermi active galactic nuclei catalog (3LAC) can be potentially classified as a BL Lac object or a flat spectrum radio quasar (FSRQ) by performing a statistical…

High Energy Astrophysical Phenomena · Physics 2017-03-29 Ting-Feng Yi , Jin Zhang , Rui-Jing Lu , Rui Huang , En-Wei Liang

We report on the results of an optical spectroscopic survey at high Galactic latitude (b\geq30{\deg}) of a sample of WISE-selected targets, grouped by WISE W1 ({\lambda}_eff = 3.4 \mum) flux, which we use to characterize the sources WISE…

Blazars are the brightest and most abundant persistent sources in the extragalactic gamma-ray sky. Due to their significance, they are often observed across various energy bands to explore potential correlations between emissions at…

High Energy Astrophysical Phenomena · Physics 2024-01-22 P. Giommi , N. Sahakyan , D. Israyelyan , M. Manvelyan

The Fermi fourth catalog of active galactic nuclei (AGNs) data release 3 (4LAC-DR3) contains 3407 AGNs, out of which 755 are flat spectrum radio quasars (FSRQs), 1379 are BL Lacertae objects (BL Lacs), 1208 are blazars of unknown (BCUs)…

High Energy Astrophysical Phenomena · Physics 2023-04-12 Aditi Agarwal

The fourth-DR3 version (4FGL-DR3) of the Fermi/LAT catalogue of $\gamma$-ray sources contains $\sim$ 1000 objects at a galactic latitude |b| > 10$^{\circ}$ which are not identified with an optical counterpart (UGS). We performed a…

High Energy Astrophysical Phenomena · Physics 2024-02-20 Alberto Ulgiati , Simona Paiano , Aldo Treves , Renato Falomo , Boris Sbarufatti , Fabio Pintore , Thomas D. Russell , Giancarlo Cusumano

Since 2008 August the Fermi Large Area Telescope (LAT) has provided continuous coverage of the gamma-ray sky yielding more than 5000 gamma-ray sources, but 54% of the detected sources remain with no certain or unknown association with a low…

High Energy Astrophysical Phenomena · Physics 2020-12-01 Chiaro G. , Kovacevic M. , La Mura G

We cross correlate the Fermi 11 months survey catalogue (1FGL) with the 20 GHz Australia Telescope Compact Array radio survey catalogue (AT20G) composed by 5890 sources at declination <0 deg. Among the 738 Fermi sources distributed in the…

High Energy Astrophysical Phenomena · Physics 2015-05-18 G. Ghirlanda , G. Ghisellini , F. Tavecchio , L. Foschini