SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:lnu-42791"
 

Search: onr:"swepub:oai:DiVA.org:lnu-42791" > Discovery of TeV Ga...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist
  • Aliu, E. (author)

Discovery of TeV Gamma-Ray Emission toward Supernova Remnant SNR G78.2+2.1

  • Article/chapterEnglish2013

Publisher, publication year, extent ...

  • 2013
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:lnu-42791
  • https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-42791URI
  • https://doi.org/10.1088/0004-637X/770/2/93DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • We report the discovery of an unidentified, extended source of very-high-energy gamma-ray emission, VER J2019+407, within the radio shell of the supernova remnant SNR G78.2+2.1, using 21.4 hr of data taken by the VERITAS gamma-ray observatory in 2009. These data confirm the preliminary indications of gamma-ray emission previously seen in a two-year (2007-2009) blind survey of the Cygnus region by VERITAS. VER J2019+407, which is detected at a post-trials significance of 7.5 standard deviations in the 2009 data, is localized to the northwestern rim of the remnant in a region of enhanced radio and X-ray emission. It has an intrinsic extent of  and its spectrum is well-characterized by a differential power law (dN/dE = N 0 × (E/TeV)–Γ) with a photon index of Γ = 2.37 ± 0.14stat ± 0.20sys and a flux normalization of N 0 = 1.5 ± 0.2stat ± 0.4sys × 10–12 photon TeV–1 cm–2 s–1. This yields an integral flux of 5.2 ± 0.8stat ± 1.4sys × 10–12 photon cm–2 s–1above 320 GeV, corresponding to 3.7% of the Crab Nebula flux. We consider the relationship of the TeV gamma-ray emission with the GeV gamma-ray emission seen from SNR G78.2+2.1 as well as that seen from a nearby cocoon of freshly accelerated cosmic rays. Multiple scenarios are considered as possible origins for the TeV gamma-ray emission, including hadronic particle acceleration at the SNR shock.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Archambault, S. (author)
  • Arlen, T. (author)
  • Aune, T. (author)
  • Beilicke, M. (author)
  • Benbow, W. (author)
  • Bird, R. (author)
  • Bouvier, A. (author)
  • Bradbury, S. M. (author)
  • Buckley, J. H. (author)
  • Bugaev, V. (author)
  • Byrum, K. (author)
  • Cannon, A. (author)
  • Cesarini, A. (author)
  • Ciupik, L. (author)
  • Collins-Hughes, E. (author)
  • Connolly, M. P. (author)
  • Cui, W. (author)
  • Dickherber, R. (author)
  • Duke, C. (author)
  • Dumm, J. (author)
  • Dwarkadas, V. V. (author)
  • Errando, M. (author)
  • Falcone, A. (author)
  • Federici, S. (author)
  • Feng, Q. (author)
  • Finley, J. P. (author)
  • Finnegan, G. (author)
  • Fortson, L. (author)
  • Furniss, A. (author)
  • Galante, N. (author)
  • Gall, D. (author)
  • Gillanders, G. H. (author)
  • Godambe, S. (author)
  • Gotthelf, E. V. (author)
  • Griffin, S. (author)
  • Grube, J. (author)
  • Gyuk, G. (author)
  • Hanna, D. (author)
  • Holder, J. (author)
  • Huan, H. (author)
  • Hughes, G. (author)
  • Humensky, T. B. (author)
  • Kaaret, P. (author)
  • Karlsson, N. (author)
  • Kertzman, M. (author)
  • Khassen, Y. (author)
  • Kieda, D. (author)
  • Krawczynski, H. (author)
  • Krennrich, F. (author)
  • Lang, M. J. (author)
  • Lee, K. (author)
  • Madhavan, A. S. (author)
  • Maier, G. (author)
  • Majumdar, P. (author)
  • McArthur, S. (author)
  • McCann, A. (author)
  • Millis, J. (author)
  • Moriarty, P. (author)
  • Mukherjee, R. (author)
  • Nelson, T. (author)
  • O’Faoláin de Bhróithe, A. (author)
  • Ong, R. A. (author)
  • Orr, M. (author)
  • Otte, A. N. (author)
  • Pandel, D. (author)
  • Park, N. (author)
  • Perkins, J. S. (author)
  • Pohl, M. (author)
  • Popkow, A. (author)
  • Prokoph, HeikeDESY, Germany(Swepub:lnu)hepraa (author)
  • Quinn, J. (author)
  • Ragan, K. (author)
  • Reyes, L. C. (author)
  • Reynolds, P. T. (author)
  • Roache, E. (author)
  • Rose, H. J. (author)
  • Ruppel, J. (author)
  • Saxon, D. B. (author)
  • Schroedter, M. (author)
  • Sembroski, G. H. (author)
  • \c Sentürk, G. D. (author)
  • Skole, C. (author)
  • Telezhinsky, I. (author)
  • Tesić, G. (author)
  • Theiling, M. (author)
  • Thibadeau, S. (author)
  • Tsurusaki, K. (author)
  • Tyler, J. (author)
  • Varlotta, A. (author)
  • Vassiliev, V. V. (author)
  • Vincent, S. (author)
  • Wakely, S. P. (author)
  • Ward, J. E. (author)
  • Weekes, T. C. (author)
  • Weinstein, A. (author)
  • Weisgarber, T. (author)
  • Welsing, R. (author)
  • Williams, D. A. (author)
  • Zitzer, B. (author)
  • DESY, Germany (creator_code:org_t)

Related titles

  • In:Astrophysical Journal770:20004-637X1538-4357

Internet link

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Find more in SwePub

Search outside SwePub

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view