Discovery of a new tev gamma-ray source: ver j0521+211
dc.contributor.author | Archambault, S. | |
dc.contributor.author | Arlen, T. | |
dc.contributor.author | Aune, T. | |
dc.contributor.author | Behera, B. | |
dc.contributor.author | Beilicke, M. | |
dc.contributor.author | Benbow, W. | |
dc.contributor.author | Bird, R. | |
dc.contributor.author | Bouvier, A. | |
dc.contributor.author | Buckley, J. H. | |
dc.contributor.author | Bugaev, V. | |
dc.contributor.author | Byrum, K. | |
dc.contributor.author | Cesarini, A. | |
dc.contributor.author | Ciupik, L. | |
dc.contributor.author | Connolly, M. P. | |
dc.contributor.author | Cui, W. | |
dc.contributor.author | Errando, M. | |
dc.contributor.author | Falcone, A. | |
dc.contributor.author | Federici, S. | |
dc.contributor.author | Feng, Q. | |
dc.contributor.author | Finley, J. P. | |
dc.contributor.author | Fortson, L. | |
dc.contributor.author | Furniss, A. | |
dc.contributor.author | Galante, N. | |
dc.contributor.author | Gall, D. | |
dc.contributor.author | Gillanders, G. H. | |
dc.contributor.author | Griffin, S. | |
dc.contributor.author | Grube, J. | |
dc.contributor.author | Gyuk, G. | |
dc.contributor.author | Hanna, D. | |
dc.contributor.author | Holder, J. | |
dc.contributor.author | Hughes, G. | |
dc.contributor.author | Humensky, T. B. | |
dc.contributor.author | Kaaret, P. | |
dc.contributor.author | Kertzman, M. | |
dc.contributor.author | Khassen, Y. | |
dc.contributor.author | Kieda, D. | |
dc.contributor.author | Krawczynski, H. | |
dc.contributor.author | Krennrich, F. | |
dc.contributor.author | Kumar, S. | |
dc.contributor.author | Lang, M. J. | |
dc.contributor.author | Madhavan, A. S | |
dc.contributor.author | Maier, G. | |
dc.contributor.author | Majumdar, P. | |
dc.contributor.author | McArthur, S. | |
dc.contributor.author | McCann, A. | |
dc.contributor.author | Millis, J. | |
dc.contributor.author | Moriarty, P. | |
dc.contributor.author | Mukherjee, R. | |
dc.contributor.author | O'Faoláin de Bhróithe, A. | |
dc.contributor.author | Ong, R. A. | |
dc.contributor.author | Otte, A. N. | |
dc.contributor.author | Park, N. | |
dc.contributor.author | Perkins, J. S. | |
dc.contributor.author | Pohl, M. | |
dc.contributor.author | Popkow, A. | |
dc.contributor.author | Prokoph, H. | |
dc.contributor.author | Quinn, J. | |
dc.contributor.author | Ragan, K. | |
dc.contributor.author | Reyes, L. C. | |
dc.contributor.author | Reynolds, P. T. | |
dc.contributor.author | Richards, G. T. | |
dc.contributor.author | Roache, E. | |
dc.contributor.author | Saxon, D. B. | |
dc.contributor.author | Sembroski, G. H. | |
dc.contributor.author | Smith, A. W. | |
dc.contributor.author | Staszak, D. | |
dc.contributor.author | Telezhinsky, I. | |
dc.contributor.author | Theiling, M. | |
dc.contributor.author | Varlotta, A. | |
dc.contributor.author | Vassiliev, V. V. | |
dc.contributor.author | Vincent, S. | |
dc.contributor.author | Wakely, S. P. | |
dc.contributor.author | Weekes, T. C. | |
dc.contributor.author | Weinstein, A. | |
dc.contributor.author | Welsing, R. | |
dc.contributor.author | Williams, D. A. | |
dc.contributor.author | Zitzer, B. | |
dc.contributor.author | Böttcher, M. | |
dc.contributor.author | Fegan, S. J. | |
dc.contributor.author | Fortin, P. | |
dc.contributor.author | Halpern, J. P. | |
dc.contributor.author | Kovalev, Y. Y. | |
dc.contributor.author | Lister, M. L. | |
dc.contributor.author | Liu, J. | |
dc.contributor.author | Pushkarev, A. B. | |
dc.contributor.author | Smith, P. S. | |
dc.contributor.author | , | |
dc.date.accessioned | 2018-09-20T16:00:03Z | |
dc.date.available | 2018-09-20T16:00:03Z | |
dc.date.issued | 2013-09-27 | |
dc.identifier.citation | Archambault, S. Arlen, T.; Aune, T.; Behera, B.; Beilicke, M.; Benbow, W.; Bird, R.; Bouvier, A.; Buckley, J. H.; Bugaev, V.; Byrum, K.; Cesarini, A.; Ciupik, L.; Connolly, M. P.; Cui, W.; Errando, M.; Falcone, A.; Federici, S.; Feng, Q.; Finley, J. P.; Fortson, L.; Furniss, A.; Galante, N.; Gall, D.; Gillanders, G. H.; Griffin, S.; Grube, J.; Gyuk, G.; Hanna, D.; Holder, J.; Hughes, G.; Humensky, T. B.; Kaaret, P.; Kertzman, M.; Khassen, Y.; Kieda, D.; Krawczynski, H.; Krennrich, F.; Kumar, S.; Lang, M. J.; Madhavan, A. S; Maier, G.; Majumdar, P.; McArthur, S.; McCann, A.; Millis, J.; Moriarty, P.; Mukherjee, R.; O'Faoláin de Bhróithe, A.; Ong, R. A.; Otte, A. N.; Park, N.; Perkins, J. S.; Pohl, M.; Popkow, A.; Prokoph, H.; Quinn, J.; Ragan, K.; Reyes, L. C.; Reynolds, P. T.; Richards, G. T.; Roache, E.; Saxon, D. B.; Sembroski, G. H.; Smith, A. W.; Staszak, D.; Telezhinsky, I.; Theiling, M.; Varlotta, A.; Vassiliev, V. V.; Vincent, S.; Wakely, S. P.; Weekes, T. C.; Weinstein, A.; Welsing, R.; Williams, D. A.; Zitzer, B.; Böttcher, M.; Fegan, S. J.; Fortin, P.; Halpern, J. P.; Kovalev, Y. Y.; Lister, M. L.; Liu, J.; Pushkarev, A. B.; Smith, P. S.; , (2013). Discovery of a new tev gamma-ray source: ver j0521+211. The Astrophysical Journal 776 (2), | |
dc.identifier.issn | 0004-637X,1538-4357 | |
dc.identifier.uri | http://hdl.handle.net/10379/10284 | |
dc.description.abstract | We report the detection of a new TeV gamma-ray source, VER J0521+211, based on observations made with the VERITAS imaging atmospheric Cherenkov Telescope Array. These observations were motivated by the discovery of a cluster of >30 GeV photons in the first year of Fermi Large Area Telescope observations. VER J0521+211 is relatively bright at TeV energies, with a mean photon flux of (1.93 +/- 0.13(stat) +/- 0.78(sys)) x 10(-11) cm(-2) s(-1) above 0.2 TeV during the period of the VERITAS observations. The source is strongly variable on a daily timescale across all wavebands, from optical to TeV, with a peak flux corresponding to similar to 0.3 times the steady Crab Nebula flux at TeV energies. Follow-up observations in the optical and X-ray bands classify the newly discovered TeV source as a BL Lac-type blazar with uncertain redshift, although recent measurements suggest z = 0.108. VER J0521+211 exhibits all the defining properties of blazars in radio, optical, X-ray, and gamma-ray wavelengths. | |
dc.publisher | IOP Publishing | |
dc.relation.ispartof | The Astrophysical Journal | |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Ireland | |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/3.0/ie/ | |
dc.subject | bl lacertae objects: individual (ver j0521+211) | |
dc.subject | gamma rays: galaxies | |
dc.subject | active galactic nuclei | |
dc.subject | large-area telescope | |
dc.subject | extragalactic background light | |
dc.subject | all-sky survey | |
dc.subject | high-energy emission | |
dc.subject | multiwavelength observations | |
dc.subject | source catalog | |
dc.subject | bl-lac | |
dc.subject | linear-polarization | |
dc.subject | detected blazars | |
dc.title | Discovery of a new tev gamma-ray source: ver j0521+211 | |
dc.type | Article | |
dc.identifier.doi | 10.1088/0004-637x/776/2/69 | |
dc.local.publishedsource | http://iopscience.iop.org/article/10.1088/0004-637X/776/2/69/pdf | |
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