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We describe further results of a program aimed to yield ~10^4 fully characterized optical identifications of ROSAT X-ray sources. Our program employs X-ray data from the ROSAT All-Sky Survey (RASS), and both optical imaging and…

The parsec-scale radio properties of 232 active galactic nuclei (AGNs), most of which are blazars, detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope have been observed contemporaneously by the Very Long…

High Energy Astrophysical Phenomena · Physics 2015-06-11 J. D. Linford , G. B. Taylor , F. K. Schinzel

The uncharted territory of the high-redshift ($z\gtrsim3$) Universe holds the key to understand the evolution of quasars. In an attempt to identify the most extreme members of the quasar population, i.e., blazars, we have carried out a…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Vaidehi S. Paliya , M. Ajello , H. -M. Cao , M. Giroletti , Amanpreet Kaur , Greg Madejski , Benoit Lott , D. Hartmann

The REX (Radio-Emitting X-ray sources) is a catalogue produced by cross-matching X-ray data from the ROSAT-PSPC archive of pointed observations and radio data from the NRAO VLA Sky Survey, aimed at the selection of blazars. From the REX…

High Energy Astrophysical Phenomena · Physics 2020-01-08 B. Balmaverde , A. Caccianiga , R. Della Ceca , A. Wolter , A. Belfiore , L. Ballo , M. Berton , I. Gioia , T. Maccacaro , B. Sbarufatti

We have observed with ROSAT six blazars from the sample of 31 polarized objects constructed by Impey and Tapia (1988). Results of the spectral analysis in the ROSAT band of three objects, PKS 0301-243, PKS 1055+018 and PG 1424+240 are…

Astrophysics · Physics 2009-10-22 L. Maraschi , G. Fossati , G. Tagliaferri , A. Treves

The fourth catalog of active galactic nuclei (AGNs) detected by the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) between 2008 August 4 and 2016 August 2 contains 2863 objects located at high Galactic latitudes (|b|>10{\deg}).…

High Energy Astrophysical Phenomena · Physics 2020-10-29 LAT collaboration

We present the X-ray analysis of the largest flux-limited complete sample of blazar candidates at z>4 selected from the Cosmic Lens All Sky Survey (CLASS). After obtaining a nearly complete (24/25) X-ray coverage of the sample (from…

Astrophysics of Galaxies · Physics 2019-09-25 L. Ighina , A. Caccianiga , A. Moretti , S. Belladitta , R. Della Ceca , L. Ballo , D. Dallacasa

One of the main scientific objectives of the ongoing Fermi mission is unveiling the nature of the unidentified gamma-ray sources (UGSs). Despite the large improvements of Fermi in the localization of gamma-ray sources with respect to the…

High Energy Astrophysical Phenomena · Physics 2015-06-04 F. Massaro , R. D'Abrusco , G. Tosti , M. Ajello , A. Paggi. D. Gasparrini

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

We present simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard X-ray, and gamma-ray bands. Our unique data set has allowed us to demonstrate that the…

Active galactic Nuclei (AGNs) with their relativistic jets pointed towards the observer, form a subclass of luminous gamma-ray sources commonly known as blazars. The study of blazars is essential to improve our understanding on the AGNs…

High Energy Astrophysical Phenomena · Physics 2019-03-05 Abhishek Desai , Stefano Marchesi , Meenakshi Rajagopal , Marco Ajello

We present a systematic search for radio active galactic nuclei (AGNs) in dwarf galaxies using recent observations taken by the Very Large Array Sky Survey (VLASS). To select these objects, we first establish a criterion to identify…

Astrophysics of Galaxies · Physics 2024-11-25 John-Michael Eberhard , Amy E. Reines , Hansung B. Gim , Jeremy Darling , Jenny E. Greene

Our understanding of blazars has been greatly increased in recent years by extensive multi-wavelength observations, particularly in the radio, X-ray and gamma-ray regions. Over the past decade the Whipple 10m telescope has contributed to…

Astrophysics · Physics 2010-11-24 I. de la Calle Perez , the VERITAS Collaboration

Extremely high-peaked BL Lac objects - also named extreme blazars - are among the most energetic and persistent extragalactic accelerators in the Universe, defined by a synchrotron emission peaking above $10^{17}$ Hz in X-rays. Such…

High Energy Astrophysical Phenomena · Physics 2026-05-06 K. Abe , S. Abe , J. Abhir , A. Abhishek , V. A. Acciari , F. Acero , A. Aguasca-Cabot , I. Agudo , C. Alispach , D. Ambrosino , F. Ambrosino , T. Aniello , S. Ansoldi , L. A. Antonelli , C. Aramo , A. Arbet-Engels , C. Arcaro , T. T. H. Arnesen , P. Aubert , A. Babić , C. Bakshi , A. Baktash , M. Balbo , A. Bamba , A. Baquero Larriva , U. Barres de Almeida , J. A. Barrio , L. Barrios Jiménez , I. Batkovic , J. Baxter , J. Becerra González , W. Bednarek , E. Bernardini , J. Bernete , A. Berti , C. Bigongiari , A. Biland , E. Bissaldi , O. Blanch , G. Bonnoli , P. Bordas , Ž. Bošnjak , A. Briscioli , E. Bronzini , G. Brunelli , J. Buces , A. Bulgarelli , I. Burelli , L. Burmistrov , A. Campoy-Ordaz , M. Cardillo , S. Caroff , A. Carosi , R. Carosi , R. Carraro , M. Carretero-Castrillo , F. Cassol , A. J. Castro-Tirado , D. Cerasole , G. Ceribella , A. Cerviño Cortínez , Y. Chai , G. Chon , L. Chytka , G. M. Cicciari , A. Cifuentes Santos , J. L. Contreras , J. Cortina , S. Covino , H. Costantini , M. Croisonnier , M. Dalchenko , G. D'Amico , P. Da Vela , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , R. Del Burgo , M. Delfino , C. Delgado , J. Delgado Mengual , D. della Volpe , B. De Lotto , L. Del Peral , R. de Menezes , G. De Palma , V. de Souza , C. Díaz , L. Di Bella , A. Di Piano , F. Di Pierro , R. Di Tria , L. Di Venere , A. Dinesh , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , L. Eisenberger , D. Elsässer , G. Emery , L. Feligioni , J. Escudero , L. Fariña , F. Ferrarotto , A. Fiasson , L. Foffano , L. Font , F. Frías García-Lago , S. Fröse , Y. Fukazawa , S. Gallozzi , R. Garcia López , S. Garcia Soto , C. Gasbarra , D. Gasparrini , S. Gasparyan , M. Gaug , J. Giesbrecht Paiva , N. Giglietto , F. Giordano , P. Gliwny , N. Godinovic , T. Gradetzke , R. Grau , J. Green , G. Grolleron , S. Gunji , P. Günther , J. Hackfeld , D. Hadasch , A. Hahn , G. Harutyunyan , M. Hashizume , T. Hassan , K. Hayashi , L. Heckmann , M. Heller , J. Herrera Llorente , N. Hiroshima , D. Hoffmann , D. Horns , J. Houles , D. Hrupec , R. Imazawa , T. Inada , S. Inoue , K. Ioka , M. Iori , D. Israyelyan , T. Itokawa , A. Iuliano , J. Jahanvi , I. Jimenez Martinez , J. Jimenez Quiles , I. Jorge Rodrigo , J. Jormanainen , J. Jurysek , M. Kagaya , S. Kankkunen , V. Karas , H. Katagiri , T. Kayanoki , D. Kerszberg , T. Kiyomoto , G. W. Kluge , Y. Kobayashi , K. Kohri , J. Konrad , P. Kornecki , P. M. Kouch , G. Koziol , H. Kubo , J. Kushida , B. Lacave , M. Lainez , A. Lamastra , L. Lemoigne , E. Lindfors , M. Linhoff , S. Lombardi , F. Longo , R. López-Coto , M. López-Moya , A. López-Oramas , S. Loporchio , J. Lozano Bahilo , F. Lucarelli , H. Luciani , L. Lulić , P. L. Luque-Escamilla , E. Lyard , P. Majumdar , M. Makariev , M. Mallamaci , D. Mandat , G. Maneva , M. Manganaro , S. Mangano , K. Mannheim , S. Marchesi , F. Marini , M. Mariotti , P. Marquez , G. Marsella , J. Martí , D. Martin , O. Martinez , G. Martínez , M. Martínez , M. Massa , P. Maruševec , D. Mazin , S. Menchiari , J. Méndez-Gallego , S. Menon , E. Mestre Guillen , D. Miceli , T. Miener , J. M. Miranda , R. Mirzoyan , M. Molero Gonzalez , E. Molina , H. A. Mondal , T. Montaruli , A. Moralejo , A. Morselli , V. Moya , A. L. Müller , H. Muraishi , S. Nagataki , T. Nakamori , C. Nanci , A. Negro , A. Neronov , V. Neustroev , D. Nieto Castaño , M. Nievas Rosillo , C. Nigro , L. Nikolic , K. Noda , V. Novotny , S. Nozaki , M. Ohishi , A. Okumura , R. Orito , L. Orsini , J. Otero-Santos , P. Ottanelli , S. Paiano , M. Palatiello , G. Panebianco , D. Paneque , R. Paoletti , J. M. Paredes , M. Pech , M. Pecimotika , M. Peresano , F. Perrotta , M. Persic , F. Pfeifle , M. Pihet , G. Pirola , C. Plard , F. Podobnik , M. Polo , C. Pozo-Gonzaléz , P. G. Prada Moroni , E. Prandini , S. Rainò , R. Rando , W. Rhode , M. Ribó , J. Rico , G. Rodriguez Fer dez , M. D. Rodríguez Frías , A. Roy , A. Ruina , E. Ruiz-Velasco , N. Sahakyan , T. Saito , S. Sakurai , D. A. Sanchez , H. Sano , E. Santos Moura , T. Šarić , Y. Sato , F. G. Saturni , V. Savchenko , F. Schiavone , K. Schmitz , F. Schmuckermaier , F. Schussler , T. Schweizer , M. Seglar Arroyo , A. Sciaccaluga , G. Silvestri , A. Simongini , J. Sitarek , V. Sliusar , I. Sofia , D. Sobczynska , A. Stamerra , J. Strišković , D. Strom , M. Strzys , Y. Suda , A. Sunny , H. Tajima , M. Takahashi , R. Takeishi , S. J. Tanaka , D. Tateishi , T. Tavernier , P. Temnikov , Y. Terada , K. Terauchi , T. Terzic , M. Teshima , M. Tluczykont , T. Tomura , D. F. Torres , F. Tramonti , P. Travnicek , G. Tripodo , A. Tutone , S. Ubach , M. Vacula , M. Vázquez Acosta , S. Ventura , G. Verna , I. Viale , A. Viana , A. Vigliano , C. F. Vigorito , E. Visentin , V. Vitale , G. Voutsinas , I. Vovk , T. Vuillaume , R. Walter , C. Walther , F. Wersig , M. Will , T. Yamamoto , R. Yamazaki , Y. Yao , P. K. H. Yeung , T. Yoshida , T. Yoshikoshi , W. Zhang , N. Zywucka , F. D'Ammando , D. Linder , F. Wierda

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

We analyse a group of radio sources, a subset of the 200 mJy sample, all of which have core-jet radio structures measured with VLBI and have flat spectra stretching from the radio to the millimetre/sub-millimetre band. Thus the objects have…

Astrophysics · Physics 2009-11-10 S. Anton , I. W. A. Browne

We utilize machine learning methods to distinguish BL Lacertae objects (BL Lac) from Flat Spectrum Radio Quasars (FSRQ) within a sample of likely X-ray blazar counterparts to Fermi 3FGL unassociated gamma-ray sources. From our previous…

High Energy Astrophysical Phenomena · Physics 2021-03-03 Amanpreet Kaur , Abraham D. Falcone , Michael C. Stroh

Results are presented of extended and refined optical identification of 181 radio/X-ray sources in the RASS-Green Bank (RGB) catalog which have been spectroscopically observed in the Sloan digital sky survey (SDSS) DR5. For 72 sources, the…

High Energy Astrophysical Phenomena · Physics 2009-09-24 Deliang Wang , Jianguo Wang , Xiaobo Dong

The fourth Fermi Large Area Telescope Source Catalog (4FGL) lists over 5000 gamma-ray sources with statistical significance above 4$\sigma$. About 23% of the sources listed in this catalog are unidentified/unassociated gamma-ray sources…

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