{"paper":{"title":"Discovery of a Glitch in the Accretion Powered Pulsar SXP 1062","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Baykal (1) ((1) Physics Department, Baskent University), D. Cerri-Serim (1), Electronics Engineering, Middle East Technical University (2) Department of Electrical, M. M. Serim (1), S. C. Inam (2), S. Sahiner (1)","submitted_at":"2017-06-02T15:41:14Z","abstract_excerpt":"We present timing analysis of the accretion powered pulsar SXP 1062, based on the observations of \\textit{Swift}, \\textit{XMM-Newton} and \\textit{Chandra} satellites covering a time span of about 2 years. We obtain a phase coherent timing solution which shows that SXP 1062 has been steadily spinning down with a rate $-\\,4.29(7) \\times 10^{-14}$ Hz s$^{-1}$ leading to a surface magnetic field estimate of about $1.5 \\times 10^{14}$ G. We also resolve the binary orbital motion of the system from X-ray data which confirms an orbital period of 656(2) days. On MJD 56834.5, a sudden change in pulse f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.00727","kind":"arxiv","version":2},"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"}