Veritas and multiwavelength observations of the bl lacertae object 1es 1741+196
dc.contributor.author | Abeysekara, A. U. | |
dc.contributor.author | Archambault, S. | |
dc.contributor.author | Archer, A. | |
dc.contributor.author | Benbow, W. | |
dc.contributor.author | Bird, R. | |
dc.contributor.author | Biteau, J. | |
dc.contributor.author | Buchovecky, M. | |
dc.contributor.author | Buckley, J. H. | |
dc.contributor.author | Bugaev, V. | |
dc.contributor.author | Byrum, K. | |
dc.contributor.author | Cardenzana, J. V | |
dc.contributor.author | Cerruti, M. | |
dc.contributor.author | Chen, X. | |
dc.contributor.author | Christiansen, J. L. | |
dc.contributor.author | Ciupik, L. | |
dc.contributor.author | Connolly, M. P. | |
dc.contributor.author | Cui, W. | |
dc.contributor.author | Dickinson, H. J. | |
dc.contributor.author | Dumm, J. | |
dc.contributor.author | Eisch, J. D. | |
dc.contributor.author | Errando, M. | |
dc.contributor.author | Falcone, A. | |
dc.contributor.author | Feng, Q. | |
dc.contributor.author | Finley, J. P. | |
dc.contributor.author | Fleischhack, H. | |
dc.contributor.author | Flinders, A. | |
dc.contributor.author | Fortin, P. | |
dc.contributor.author | Fortson, L. | |
dc.contributor.author | Furniss, A. | |
dc.contributor.author | Gillanders, G. H. | |
dc.contributor.author | Griffin, S. | |
dc.contributor.author | Grube, J. | |
dc.contributor.author | Gyuk, G. | |
dc.contributor.author | Huetten, M. | |
dc.contributor.author | Hanna, D. | |
dc.contributor.author | Holder, J. | |
dc.contributor.author | Humensky, T. B. | |
dc.contributor.author | Johnson, C. A. | |
dc.contributor.author | Kaaret, P. | |
dc.contributor.author | Kar, P. | |
dc.contributor.author | Kelley-Hoskins, N. | |
dc.contributor.author | Kertzman, M. | |
dc.contributor.author | Kieda, D. | |
dc.contributor.author | Krause, M. | |
dc.contributor.author | Krennrich, F. | |
dc.contributor.author | Lang, M. J. | |
dc.contributor.author | Maier, G. | |
dc.contributor.author | McArthur, S. | |
dc.contributor.author | McCann, A. | |
dc.contributor.author | Meagher, K. | |
dc.contributor.author | Moriarty, P. | |
dc.contributor.author | Mukherjee, R. | |
dc.contributor.author | Nieto, D. | |
dc.contributor.author | O'Brien, S. | |
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 | Pelassa, V. | |
dc.contributor.author | Petrashyk, A. | |
dc.contributor.author | Petry, D. | |
dc.contributor.author | Pohl, M. | |
dc.contributor.author | Popkow, A. | |
dc.contributor.author | Pueschel, E. | |
dc.contributor.author | Quinn, J. | |
dc.contributor.author | Ragan, K. | |
dc.contributor.author | Ratliff, G. | |
dc.contributor.author | Reyes, L. C. | |
dc.contributor.author | Reynolds, P. T. | |
dc.contributor.author | Reynolds, K. | |
dc.contributor.author | Richards, G. T. | |
dc.contributor.author | Roache, E. | |
dc.contributor.author | Rulten, C. | |
dc.contributor.author | Santander, M. | |
dc.contributor.author | Sembroski, G. H. | |
dc.contributor.author | Shahinyan, K. | |
dc.contributor.author | Smith, A. W. | |
dc.contributor.author | Staszak, D. | |
dc.contributor.author | Telezhinsky, I. | |
dc.contributor.author | Tucci, J. V. | |
dc.contributor.author | Tyler, J. | |
dc.contributor.author | Vincent, S. | |
dc.contributor.author | Wakely, S. P. | |
dc.contributor.author | Weiner, O. M. | |
dc.contributor.author | Weinstein, A. | |
dc.contributor.author | Wilhelm, A. | |
dc.contributor.author | Williams, D. A. | |
dc.contributor.author | Zitzer, B. | |
dc.date.accessioned | 2018-09-20T15:58:34Z | |
dc.date.available | 2018-09-20T15:58:34Z | |
dc.date.issued | 2016-04-01 | |
dc.identifier.citation | Abeysekara, A. U. Archambault, S.; Archer, A.; Benbow, W.; Bird, R.; Biteau, J.; Buchovecky, M.; Buckley, J. H.; Bugaev, V.; Byrum, K.; Cardenzana, J. V; Cerruti, M.; Chen, X.; Christiansen, J. L.; Ciupik, L.; Connolly, M. P.; Cui, W.; Dickinson, H. J.; Dumm, J.; Eisch, J. D.; Errando, M.; Falcone, A.; Feng, Q.; Finley, J. P.; Fleischhack, H.; Flinders, A.; Fortin, P.; Fortson, L.; Furniss, A.; Gillanders, G. H.; Griffin, S.; Grube, J.; Gyuk, G.; Huetten, M.; Hanna, D.; Holder, J.; Humensky, T. B.; Johnson, C. A.; Kaaret, P.; Kar, P.; Kelley-Hoskins, N.; Kertzman, M.; Kieda, D.; Krause, M.; Krennrich, F.; Lang, M. J.; Maier, G.; McArthur, S.; McCann, A.; Meagher, K.; Moriarty, P.; Mukherjee, R.; Nieto, D.; O'Brien, S.; O'Faoláin de Bhróithe, A.; Ong, R. A.; Otte, A. N.; Park, N.; Pelassa, V.; Petrashyk, A.; Petry, D.; Pohl, M.; Popkow, A.; Pueschel, E.; Quinn, J.; Ragan, K.; Ratliff, G.; Reyes, L. C.; Reynolds, P. T.; Reynolds, K.; Richards, G. T.; Roache, E.; Rulten, C.; Santander, M.; Sembroski, G. H.; Shahinyan, K.; Smith, A. W.; Staszak, D.; Telezhinsky, I.; Tucci, J. V.; Tyler, J.; Vincent, S.; Wakely, S. P.; Weiner, O. M.; Weinstein, A.; Wilhelm, A.; Williams, D. A.; Zitzer, B. (2016). Veritas and multiwavelength observations of the bl lacertae object 1es 1741+196. Monthly Notices of the Royal Astronomical Society 459 (3), 2550-2557 | |
dc.identifier.issn | 0035-8711,1365-2966 | |
dc.identifier.uri | http://hdl.handle.net/10379/10071 | |
dc.description.abstract | We present results from multiwavelength observations of the BL Lacertae object 1ES 1741 + 196, including results in the very high energy gamma-ray regime using the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The VERITAS time-averaged spectrum, measured above 180 GeV, is well modelled by a power law with a spectral index of 2.7 +/- 0.7(stat) +/- 0.2(syst). The integral flux above 180 GeV is (3.9 +/- 0.8(stat) +/- 1.0(syst)) x 10(-8) m(-2) s(-1), corresponding to 1.6 per cent of the Crab nebula flux on average. The multiwavelength spectral energy distribution of the source suggests that 1ES 1741+196 is an extreme-high-frequency-peaked BL Lacertae object. The observations analysed in this paper extend over a period of six years, during which time no strong flares were observed in any band. This analysis is therefore one of the few characterizations of a blazar in a non-flaring state. | |
dc.publisher | Oxford University Press (OUP) | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Ireland | |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/3.0/ie/ | |
dc.subject | astroparticle physics | |
dc.subject | relativistic processes | |
dc.subject | galaxies: individual: 1es 1741+196=ver j1744+195 | |
dc.subject | spectral energy-distributions | |
dc.subject | gamma-ray astronomy | |
dc.subject | x-ray | |
dc.subject | lac objects | |
dc.subject | source catalog | |
dc.subject | tev blazars | |
dc.subject | telescope | |
dc.subject | fermi | |
dc.subject | discovery | |
dc.subject | swift | |
dc.title | Veritas and multiwavelength observations of the bl lacertae object 1es 1741+196 | |
dc.type | Article | |
dc.identifier.doi | 10.1093/mnras/stw664 | |
dc.local.publishedsource | http://arxiv.org/pdf/1603.07286 | |
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