{"paper":{"title":"A Three-Year Multi-Wavelength Study of the Very High Energy Gamma-ray Blazar 1ES 0229+200","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bouvier, A. Falcone, A. Furniss, A. McCann, A. N. Otte, A. O'Faolain de Bhroithe, A. Popkow, A. S Madhavan, A. Varlotta, A. Weinstein, A. W. Smith, A. Zajczyk, B. Behera, B. Zitzer, C. A. Johnson, C. Duke, D. A. Williams, D. Hanna, D. Kieda, D. Nieto, D. Staszak, E. Aliu, E. Roache, F. Krennrich, G. Gyuk, G. H. Gillanders, G. H. Sembroski, G. Hughes, G. Maier, G. T. Richards, H. Fleischhack, H. Krawczynski, H. Prokoph, I. Telezhinsky, J. Dumm, J. Grube, J. H. Buckley, J. Holder, J. Millis, J. P. Finley, J. Quinn, J. S. Perkins, K. Berger, K. Byrum, K. Meagher, K. Ragan, L. Ciupik, L. C. Reyes, L. Fortson, M. Beilicke, M. Cerruti, M. Errando, M. J. Lang, M. Kertzman, M. P. Connolly, M. Pohl, M. Theiling, N. Galante, N. Park, P. Fortin, P. Kaaret, P. Majumdar, P. Moriarty, P. T. Reynolds, Q. Feng, R. A. Ong, R. Bird, R. Mukherjee, R. Welsing, S. Archambault, S. Federici, S. Griffin, S. McArthur, S. P. Wakely, S. T. Griffiths, S. Vincent, T. Arlen, T. Aune, T. B. Humensky, T. C. Weekes, V. Bugaev, V. V. Vassiliev, W. Benbow, W. Cui, X. Chen, Y. Khassen","submitted_at":"2013-12-23T16:31:57Z","abstract_excerpt":"The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blazar. Very-high-energy measurements of this active galactic nucleus have been used to place constraints on the intensity of the extragalactic background light and the intergalactic magnetic field. A multi-wavelength study of this object centered around very-high-energy observations by VERITAS is presented. This study obtained, over a period of three years, an 11.7 standard deviation detection and an average integral flu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.6592","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}