{"paper":{"title":"Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) Keele University, (3) Queen's University, (4) University of Leicester, A. J. Norton (1), Belfast, D. R. Anderson (2), F. Faedi (3), Leicester, M. E. Lohr (1), Milton Keynes, R. G. West (4) ((1) The Open University, Staffordshire, U. C. Kolb (1), UK, UK)","submitted_at":"2012-05-08T12:50:32Z","abstract_excerpt":"SuperWASP light curves for 53 W UMa-type eclipsing binary (EB) candidates, identified in previous work as being close to the contact binary short-period limit, were studied for evidence of period change. The orbital periods of most of the stars were confirmed, and period decrease, significant at more than 5 sigma, was observed in three objects: 1SWASP J174310.98+432709.6 (-0.055 \\pm0.003 s/yr), 1SWASP J133105.91+121538.0 (-0.075 \\pm0.013 s/yr) and 1SWASP J234401.81-212229.1 (-0.313 \\pm0.019 s/yr). The magnitudes of the observed period changes cannot be explained by magnetic braking or gravitat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.1678","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"}