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BL Lacertae, the prototype of the BL Lacertae (BL Lac) category of blazars, underwent a giant $\gamma-$ray flare in April 2021. The Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope (hereafter Fermi-LAT) observed a peak…

High Energy Astrophysical Phenomena · Physics 2022-12-21 Ashwani Pandey , C. S. Stalin

Many blazars detected by the Fermi satellite, observed spectroscopically in the optical, are line-less, and have been classified as BL Lac objects. Optical-UV photometry of nearly one hundred of them allowed to determine the redshift for a…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 G. Ghisellini , F. Tavecchio , L. Foschini , T. Sbarrato , G. Ghirlanda , L. Maraschi

We investigate the variability properties of blazars in the GeV band using the data of the Fermi/LAT telescope. We find that blazars exhibit variability on the scales down to the minimal timescale resolvable by Fermi, which is a function of…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Ievgen Vovk , Andrii Neronov

We construct a large sample of gamma-ray blazars with low-frequency radio data using the recent released TGSS AD1 catalog at 150 MHz. The radio/gamma connections of blazars are compared from 143 GHz to 150 MHz. The radio flux density at all…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Xu-Liang Fan , Qingwen Wu

We report on optical spectroscopy of 165 Flat Spectrum Radio Quasars (FSRQs) in the Fermi 1LAC sample, which have helped allow a nearly complete study of this population. Fermi FSRQ show significant evidence for non-thermal emission even in…

A comprehensive study of multifrequency correlations can shed light on the nature of variation for blazars. In this work, we collect the long-term radio, optical and $\gamma$-ray light curves of PKS 1502+106. After performing the localized…

High Energy Astrophysical Phenomena · Physics 2020-01-06 Xi Shao , Yunguo Jiang , Xu Chen

The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope routinely detects the highly dust-absorbed, reddened, and MeV-peaked flat spectrum radio quasar PKS 1830-211 (z=2.507). Its apparent isotropic gamma-ray luminosity…

High Energy Astrophysical Phenomena · Physics 2015-06-23 The Fermi LAT Collaboration , A. A. Abdo , M. Ackermann , M. Ajello , A. Allafort , M. A. Amin , L. Baldini , G. Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , R. D. Blandford , E. Bonamente , A. W. Borgland , J. Bregeon , M. Brigida , R. Buehler , D. Bulmash , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , E. Cavazzuti , C. Cecchi , E. Charles , C. C. Cheung , J. Chiang , G. Chiaro , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , R. H. D. Corbet , S. Cutini , F. D'Ammando , A. de Angelis , F. de Palma , C. D. Dermer , P. S. Drell , A. Drlica-Wagner , C. Favuzzi , J. Finke , W. B. Focke , Y. Fukazawa , P. Fusco , F. Gargano , D. Gasparrini , N. Gehrels , N. Giglietto , F. Giordano , M. Giroletti , T. Glanzman , I. A. Grenier , J. E. Grove , S. Guiriec , D. Hadasch , M. Hayashida , E. Hays , R. E. Hughes , Y. Inoue , M. S. Jackson , T. Jogler , G. Jòhannesson , A. S. Johnson , T. Kamae , J. Knödlseder , M. Kuss , J. Lande , S. Larsson , L. Latronico , F. Longo , F. Loparco , B. Lott , M. N. Lovellette , P. Lubrano , G. M. Madejski , M. N. Mazziotta , J. Mehault , P. F. Michelson , T. Mizuno , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , R. Nemmen , E. Nuss , M. Ohno , T. Ohsugi , D. Paneque , J. S. Perkins , M. Pesce-Rollins , F. Piron , G. Pivato , T. A. Porter , S. Rainò , R. Rando , M. Razzano , A. Reimer , O. Reimer , L. C. Reyes , S. Ritz , C. Romoli , M. Roth , P. M. Saz Parkinson , C. Sgrò , E. J. Siskind , G. Spandre , P. Spinelli , H. Takahashi , Y. Takeuchi , T. Tanaka , J. G. Thayer , J. B. Thayer , D. J. Thompson , L. Tibaldo , M. Tinivella , D. F. Torres , G. Tosti , E. Troja , V. Tronconi , T. L. Usher , J. Vandenbroucke , V. Vasileiou , G. Vianello , V. Vitale , A. P. Waite , M. Werner , B. L. Winer , K. S. Wood

We analyze average gamma-ray variability statistics for the sample of blazars detected by CGRO/EGRET. We re-reduce all the available EGRET observations and analyze light curves by Monte Carlo modeling of the variability statistics including…

Astrophysics · Physics 2007-05-23 P. Magdziarz , R. Moderski , G. M. Madejski

We have been using the 0.76-m Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory to optically monitor a sample of 157 blazars that are bright in gamma rays, being detected with high significance ($\ge 10\sigma$) in one year by…

High Energy Astrophysical Phenomena · Physics 2015-01-27 Daniel P. Cohen , Roger W. Romani , Alexei V. Filippenko , S. Bradley Cenko , Benoit Lott , WeiKang Zheng , Weidong Li

We report the first results obtained from our campaign to characterize the intranight-optical variability (INOV) properties of {\it Fermi}~detected blazars, using the observations from the recently commissioned 1.3 m J C Bhattacharya…

High Energy Astrophysical Phenomena · Physics 2018-12-31 Vaidehi S. Paliya , C. S. Stalin , M. Ajello , A. Kaur

We present the observational results of multi-colour optical monitoring of eight red blazars from 2003 September to 2004 February. The aim of our monitoring is to investigate the spectral variability as well as the flux variations at short…

Astrophysics · Physics 2009-11-11 Minfeng Gu , C. -U. Lee , Soojong Pak , H. S. Yim , A. B. Fletcher

Multi-wavelength analyses of spectra of active galactic nuclei (AGNs) provide useful information on the physical processes in the accretion disk and jets of black holes. This, however, is limited to bright sources and may not represent the…

High Energy Astrophysical Phenomena · Physics 2021-06-09 Houdun Zeng , Vahé Petrosian , Tingfeng Yi

We present the results of our power spectral density analysis for the BL Lac object OJ\,287, utilizing the {\it Fermi}-LAT survey at high-energy $\gamma$-rays, {\it Swift}-XRT in X-rays, several ground-based telescopes and the {\it Kepler}…

High Energy Astrophysical Phenomena · Physics 2018-08-29 A. Goyal , L. Stawarz , S. Zola , V. Marchenko , M. Soida , K. Nilsson , S. Ciprini , A. Baran , M. Ostrowski , P. J. Wiita , Gopal-Krishna , A. Siemiginowska , M. Sobolewska , S. Jorstad , A. Marscher , M. F. Aller H. D. Aller T. Hovatta , D. B. Caton , D. Reichart , K. Matsumoto , K. Sadakane , K. Gazeas , M. Kidger , V. Piirola , H. Jermak , F. Alicavus , K. S. Baliyan , A. Baransky , A. Berdyugin , P. Blay , P. Boumis , D. Boyd , Y. Bufan , M. Campas Torrent , F. Campos , J. Carrillo Gomez , J. Dalessio , B. Debski , D. Dimitrov , M. Drozdz , H. Er , A. Erdem , A. Escartin Perez , V. Fallah Ramazani , A. V. Filippenko , E. Gafton , F. Garcia , V. Godunova , F. Gomez Pinilla , M. Gopinathan , J. B. Haislip , S. Haque , J. Harmanen , R. Hudec , G. Hurst , K. M. Ivarsen , A. Joshi , M. Kagitani , N. Karaman , R. Karjalainen , N. Kaur , D. Kozie l-Wierzbowska , E. Kuligowska , T. Kundera , S. Kurowski , A. Kvammen , A. P. LaCluyze , B. C. Lee , A. Liakos , J. Lozano de Haro , I. Mohammed , J. P. Moore , M. Mugrauer , R. Naves Nogues , A. W. Neely , W. Ogloza , S. Okano , U. Pajdosz , J. C. Pandey , M. Perri , G. Poyner , J. Provencal , T. Pursimo , A. Raj , B. Rajkumar , R. Reinthal , T. Reynolds , J. Saario , S. Sadegi , T. Sakanoi , J. L. Salto Gonzalez , Sameer , A. Heung , O. Simon , M. Siwak , T. Schweyer , F. C. Soldan Alfaro , E. Sonbas , J. Strobl , L. O. Takalo , L. Tremosa Espasa , J. R. Valdes , V. V. Vasylenko , F. Verrecchia , J. R. Webb , M. Yoneda , M. Zejmo , W. Zheng , P. Zielinski , J. Janik , V. Chavushyan , C. C. Cheung , M. Giroletti

Flat-spectrum radio quasars (FSRQs) whose brightness is dominated by a relativistically beamed core, are frequently found in 'blazar state' commonly inferred from a high optical polarization ( > 3%), and/or a large continuum variability.…

Astrophysics of Galaxies · Physics 2022-10-05 Krishan Chand , Gopal-Krishna

We perform a blind search for the variability of the gamma-ray sky in the energy range E>1 GeV using 308 weeks of the Fermi-LAT data. We use the technique based on the comparison of the weekly photon counts and exposures in sky pixels by…

High Energy Astrophysical Phenomena · Physics 2015-12-22 M. S. Pshirkov , G. I. Rubtsov

High-energy blazar light curves, in X-rays and beyond, have historically preferred a log-normal flux distribution, signifying multiplicative processes either in the jet itself or due to connection(s) with accretion. Here we present 18 year…

High Energy Astrophysical Phenomena · Physics 2026-01-27 Agniva Roychowdhury

We have presented a multiwavelength temporal and spectral study of the Blazar PKS 0346-27 for the period 2019 January-2021 December (MJD 58484-59575) using data from Fermi-LAT (gamma-rays), Swift-XRT (X-rays) and Swift-UVOT (ultra-violet…

High Energy Astrophysical Phenomena · Physics 2023-01-25 Sushanth Reddy Kamaram , Raj Prince , Suman Pramanick , Debanjan Bose

We have analyzed a large sample of clean blazars detected by Fermi Large Area Telescope (LAT). Using literature and calculation, we obtained intrinsic $\gamma$-ray luminosity excluding beaming effect, black hole mass, broad-line luminosity…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Dingrong Xiong , Xiong Zhang

We compiled the radio, optical, and X-ray data of blazars from the Sloan Digital Sky Survey (SDSS) database, and presented the distribution of luminosities and broad band spectral indices. The distribution of luminosities shows that the…

High Energy Astrophysical Phenomena · Physics 2015-03-20 Huaizhen Li , Luoen Chen , Yunguo Jiang , Tingfeng Yi

We present the analysis results of flux and spectral variability of the blazar OP 313 across intra-night to short-term timescales using BVRI photometric data, gathered over 25 nights from Nov 2024 to May 2025, using two optical telescopes…

High Energy Astrophysical Phenomena · Physics 2025-09-11 P. U. Devanand , Alok C. Gupta , Karan Dogra , Shubham Kishore , Tushar Tripathi
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