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VERITAS: Status and Highlights

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arxiv 1111.1225 v1 pith:IUGP6CKR submitted 2011-11-04 astro-ph.HE astro-ph.IM

J. Holder , E. Aliu , T. Arlen , T. Aune , M. Beilicke , W. Benbow , M. Böttcher , A. Bouvier
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J. H. Buckley V. Bugaev K. Byrum A. Cannon A. Cesarini J. L. Christiansen L. Ciupik E. Collins-Hughes M. P. Connolly W. Cui R. Dickherber C. Duke V. V. Dwarkadas M. Errando A. Falcone J. P. Finley G. Finnegan L. Fortson A. Furniss N. Galante D. Gall K. Gibbs G. H. Gillanders S. Godambe S. Griffin J. Grube R. Guenette G. Gyuk D. Hanna H. Huan G. Hughes C. M. Hui T. B. Humensky A. Imran P. Kaaret N. Karlsson M. Kertzman Y. Khassen D. Kieda H. Krawczynski F. Krennrich M. J. Lang M. Lyutikov A. S Madhavan G. Maier P. Majumdar S. McArthur A. McCann M. McCutcheon P. Moriarty R. Mukherjee P. D Nunez R. A. Ong M. Orr A. N. Otte N. Park J. S. Perkins A. Pichel F. Pizlo M. Pohl H. Prokoph J. Quinn K. Ragan L. C. Reyes P. T. Reynolds A. C. Rovero J. Ruppel A. C. Sadun D. B. Saxon M. Schroedter G. H. Sembroski G. D. Şentürk A. W. Smith D. Staszak G. Tešić M. Theiling S. Thibadeau K. Tsurusaki J. Tyler A. Varlotta V. V. Vassiliev S. Vincent M. Vivier S. P. Wakely J. E. Ward T. C. Weekes A. Weinstein T. Weisgarber D. A. Williams B. Zitzer
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classification astro-ph.HEastro-ph.IM
keywords gamma-rayarraygalaxyhighlightspulsarsincesourcesstatus
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The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emission above 100 GeV from 40 astrophysical sources. These include blazars, pulsar wind nebulae, supernova remnants, gamma-ray binary systems, a starburst galaxy, a radio galaxy, the Crab pulsar, and gamma-ray sources whose origin remains unidentified. In 2009, the array was reconfigured, greatly improving the sensitivity. We summarize the current status of the observatory, describe some of the scientific highlights since 2009, and outline plans for the future.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Multiwavelength Study of a Long-Duration VHE Flare from BL Lacertae with VERITAS

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    BL Lacertae produced its first long-duration very-high-energy flare, detected for ~11 days and still visible ~40 days after the triggering GeV flare, with SED modeling favoring an SSC+external-Compton interpretation.

  2. Longtime Monitoring of TeV Radio Galaxies with HAWC

    astro-ph.HE 2025-06 conditional novelty 5.0 of 10

    HAWC detects M87 at 5.21 sigma over 7.5 years and finds a low-state power-law spectrum extending to 26.5 TeV, with only marginal detection of 3C 264.

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