{"paper":{"title":"PSR J0007+7303 in the CTA1 SNR: New Gamma-ray Results from Two Years of Fermi-LAT Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, A. K. Harding, D. L. Wood, D. Parent, F. Gargano, F. Giordano, K. S. Wood, M. Coleman Miller, M. E. DeCesar, M. T. Wolff, P. S. Ray","submitted_at":"2011-07-21T03:44:55Z","abstract_excerpt":"One of the main results of the Fermi Gamma-Ray Space Telescope is the discovery of {\\gamma}-ray selected pulsars. The high magnetic field pulsar, PSR J0007+7303 in CTA1, was the first ever to be discovered through its {\\gamma}-ray pulsations. Based on analysis of 2 years of LAT survey data, we report on the discovery of {\\gamma}-ray emission in the off-pulse phase interval at the ~ 6{\\sigma} level. The flux from this emission in the energy range E \\geq 100 MeV is F_100 = (1.73\\pm0.40)\\times10^(-8) photons/cm^2/s and is best fitted by a power law with a photon index of {\\Gamma} = 2.54\\pm0.14. T"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.4151","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"}