{"paper":{"title":"Investigating Broadband Variability of the TeV Blazar 1ES 1959+650","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Barnacka, A. Bouvier, A. Falcone, A. Furniss, A. McCann, A. N. Otte, A. O'Faolain de Bhroithe, A. Popkow, A. Sadun, A. S Madhavan, A. Varlotta, A. Weinstein, A. Wilhelm, A. W. Smith, B. Zitzer (The VERITAS Collaboration), C. A. Johnson, D. A. Williams, D. Hanna, D. Kieda, D. Nieto, D. Staszak, E. Aliu, E. Collins-Hughes, E. Roache, F. Krennrich, F. Sheidaei, G. Gyuk, G. H. Gillanders, G. H. Sembroski, G. Hughes, G. T. Richards, H. Fleischhack, H. Krawczynski, H. Prokoph, I. Telezhinsky, J. D. Eisch, J. Dumm, J. Grube, J. H. Buckley, J. Holder, J. Millis, J. P. Finley, J. Quinn, J. Rajotte, J. S. Perkins, J. Tyler, K. Berger, K. Meagher, K. Ragan, K. Shahinyan, L. Ciupik, L. C. Reyes, L. Fortson, M. Beilicke, M. B\\\"ottcher, M. Cerruti, M. Fumagalli, M. J. Lang, M. Kertzman, M. P. Connolly, M. Pohl, M. Santander, M. Theiling, N. Galante, N. Hakansson, N. Park, P. Fortin, P. Kaaret, P. Kar, 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, T. Nelson, V. Bugaev, V. V. Vassiliev, W. Benbow, W. Cui, X. Chen, Y. Khassen","submitted_at":"2014-12-02T19:30:58Z","abstract_excerpt":"We summarize broadband observations of the TeV-emitting blazar 1ES 1959+650, including optical R-band observations by the robotic telescopes Super-LOTIS and iTelescope, UV observations by Swift UVOT, X-ray observations by the Swift X-ray Telescope (XRT), high-energy gamma-ray observations with the Fermi Large Area Telescope (LAT) and very-high-energy (VHE) gamma-ray observations by VERITAS above 315 GeV, all taken between 17 April 2012 and 1 June 2012 (MJD 56034 and 56079). The contemporaneous variability of the broadband spectral energy distribution is explored in the context of a simple sync"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.1031","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"}