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Related papers: Blazars and Fast Radio Bursts with LSST

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Blazars are radio-loud active galactic nuclei well known for their non thermal emission spanning a wide range of frequencies. The Roma-BZCAT is, to date, the most comprehensive list of these sources. We performed the cross-match of several…

High Energy Astrophysical Phenomena · Physics 2015-05-04 A. Maselli , F. Massaro , R. D'Abrusco , G. Cusumano , V. La Parola , A. Segreto , G. Tosti

Precise localizations of a small number of repeating fast radio bursts (FRBs) using very long baseline interferometry (VLBI) have enabled multiwavelength follow-up observations revealing diverse local environments. However, the 2--3\% of…

High Energy Astrophysical Phenomena · Physics 2025-06-25 FRB Collaboration , Thomas C. Abbott , Daniel Amouyal , Shion E. Andrew , Kevin Bandura , Mohit Bhardwaj , Kalyani Bhopi , Yash Bhusare , Charanjot Brar , Alice Cai , Tomas Cassanelli , Shami Chatterjee , Jean-François Cliche , Amanda M. Cook , Alice P. Curtin , Evan Davies-Velie , Matt Dobbs , Fengqiu Adam Dong , Yuxin Dong , Gwendolyn Eadie , Tarraneh Eftekhari , Wen-fai Fong , Emmanuel Fonseca , B. M. Gaensler , Nina Gusinskaia , Jason W. T. Hessels , Danté M. Hewitt , Jeff Huang , Naman Jain , Ronniy. C. Joseph , Lordrick Kahinga , Victoria M. Kaspi , Afrasiyab , Khan , Bikash Kharel , Adam E. Lanman , Magnus L'Argent , Mattias Lazda , Calvin Leung , Robert Main , Lluis Mas-Ribas , Kiyoshi W. Masui , Kyle McGregor , Ryan Mckinven , Juan Mena-Parra , Daniele Michilli , Nicole Mulyk , Mason Ng , Kenzie Nimmo , Ayush Pandhi , Swarali Shivraj Patil , Aaron B. Pearlman , Ue-Li Pen , Ziggy Pleunis , J. Xavier Prochaska , Masoud Rafiei-Ravandi , Scott M. Ransom , Gurman Sachdeva , Mawson W. Sammons , Ketan R. Sand , Paul Scholz , Vishwangi Shah , Kaitlyn Shin , Seth R. Siegel , Sunil Simha , Kendrick Smith , Ingrid Stairs , David C. Stenning , Haochen Wang , Thomas Boles , Ismaël Cognard , Tammo Jan Dijkema , Alexei V. Filippenko , Marcin P. Gawroński , Wolfgang Herrmann , Charles D. Kilpatrick , Franz Kirsten , Shawn Knabel , Omar S. Ould-Boukattine , Hadrien Paugnat , Weronika Puchalska , William Sheu , Aswin Suresh , Aaron Tohuvavohu , Tommaso Treu , WeiKang Zheng

Fast Radio Bursts (FRBs) are enigmatic millisecond-duration radio transients of extra-galactic origin, whose underlying mechanisms and progenitors remain poorly understood. FRBs are broadly classified into two categories: repeating FRBs,…

We present preliminary results of a statistical analysis obtained with a sample of blazars observed at the Perugia Astronomical Observatory since 1992. We briefly show how these statistical results can be useful to discriminate faint…

Astrophysics · Physics 2007-05-23 M. Fiorucci , N. Marchili , G. Tosti , S. Ciprini , F. Marcucci , A. Tramacere

In this paper we develop a model for fast radio bursts (FRBs) based on triggered superradiance (SR) and apply it to previously published data of FRB 110220 and FRB 121102. We show how a young pulsar located at ~100 pc or more from an SR/FRB…

High Energy Astrophysical Phenomena · Physics 2018-11-28 Martin Houde , Fereshteh Rajabi , B. M. Gaensler , A. Mathews , Victor Tranchant

Using public \fermi LAT and \swift BAT observations, we constructed the first sample of blazars selected at both hard X-rays and gamma-rays. Studying its spectral properties, we find a luminosity dependence of the spectral slopes at both…

Cosmology and Nongalactic Astrophysics · Physics 2017-02-22 R. M. Sambruna , D. Donato , M. Ajello , L. Maraschi , the GSFC BAT Team

The behaviour of fast radio bursts (FRBs) at radio frequencies <400 MHz is not well understood due to very few detections, with only two known sources detected below 300 MHz. Characterising low-frequency emission of FRBs is vital for…

High Energy Astrophysical Phenomena · Physics 2025-12-03 Pragya Chawla , Akshatha Gopinath , Ninisha Manaswini , Cees Bassa , Jason Hessels , Vlad Kondratiev , Daniele Michilli , Ziggy Pleunis

We propose measuring the arrival time difference of Fast Radio Bursts (FRBs) along two adjacent sightlines as a new probe to dark matter substructures on scales down to $\sim 1\,$AU. We discuss two observational scenarios in which it may be…

Cosmology and Nongalactic Astrophysics · Physics 2024-07-16 Huangyu Xiao , Liang Dai , Matthew McQuinn

The association of persistent radio sources (PRSs) with repeating fast radio bursts (FRBs) offers unique insights into their circum-burst environments. Building upon the physical link between PRS luminosity ($L_\nu$) and FRB rotation…

High Energy Astrophysical Phenomena · Physics 2026-03-19 Yuan-Pei Yang

We examine the constraints on the luminosity-dependent density evolution model for the evolution of blazars given the observed spectrum of the diffuse gamma-ray background (DGRB), blazar source-count distribution, and the blazar spectral…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Kevork N. Abazajian , Steve Blanchet , J. Patrick Harding

Fast radio bursts (FRBs) are astrophysical transients of currently unknown origin, and so far several events have been detected at extragalactic distances. The dispersion measure (DM) of the radio signal is a probe of the integrated…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-13 Robert Reischke , Steffen Hagstotz , Robert Lilow

We describe a uniform all-sky survey of bright blazars, selected primarily by their flat radio spectra, that is designed to provide a large catalog of likely gamma-ray AGN. The defined sample has 1625 targets with radio and X-ray properties…

Do all Fast Radio Burst (FRB) sources repeat? We present evidence that FRB sources follow a Zipf-like distribution, in which the number density of sources is approximately inversely proportional to their burst rate above a fixed energy…

High Energy Astrophysical Phenomena · Physics 2025-09-12 Paz Beniamini , Pawan Kumar

We report the main results of our six year long intensive optical monitoring on blazars ON 231 (W Com), BL Lac, and 3C 273. Intensive optical monitoring is an indispensable tool to obtain well sampled light curves and thus to understand the…

Astrophysics · Physics 2010-12-13 G. Tosti , S. Ciprini , E. Massaro , M. Maesano , F. Montagni , R. Nesci

Blazars, including BL Lacs and FSRQs, are the most luminous extragalactic {\gamma}-ray sources. They account for about 56% of the sources listed in the recent Fermi-LAT catalog (4FGL-DR4). The optical and UV spectra of BL Lacs are nearly…

Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ltimately, how the energy is extracted from the central black hole in radio-loud active…

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…

Searching for fleeting radio transients like fast radio bursts (FRBs) with wide-field radio telescopes has become a common challenge in data-intensive science. Conventional algorithms normally cost enormous time to seek candidates by…

Instrumentation and Methods for Astrophysics · Physics 2025-12-23 Yao Chen , Rui Luo , Chen Wang , Yong-Kun Zhang , Shiqian Zhao , Chengbing Lyu , ZePeng Zheng , Hai Lei , DeJiang Zhou , Chenhui Niu , JinLin Han , George Hobbs , Di Li , Chengwei Liang , Siyi Tan , Ting Tian

Context. Blazars are a distinct subclass of active galactic nuclei (AGN), known for their fast variability, high polarization, and intense emission across the electromagnetic spectrum, from radio waves to gamma rays. Gamma-ray blazar…

High Energy Astrophysical Phenomena · Physics 2025-01-08 N. Álvarez Crespo , A. Domínguez , V. S. Paliya , M. Chamorro Cazorla , P. Sánchez Blázquez , A. Gil de Paz

Blazars are very broadband cosmic sources with spectra spanning over twenty orders of magnitude in frequency, down to the 100 MHz regime in the radio range, up to VHE at several tens of TeV. The modelling of their spectral energy…

High Energy Astrophysical Phenomena · Physics 2022-11-08 Hélène Sol , Andreas Zech
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