{"paper":{"title":"T-Cyg1-12664: A low-mass chromospherically active eclipsing binary in the Kepler field","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Ibanoglu, E. Sipahi, O. Cakirli","submitted_at":"2012-10-30T19:36:27Z","abstract_excerpt":"The eclipsing binary T-Cyg1-12664 was observed both spectroscopically and photometrically. Radial velocities of both components and ground-based VRI light curves were obtained. The Kepler's R-data and radial velocities for the system were analysed simultaneously. Masses and radii were obtained as 0.680$\\pm$0.021 M$_{\\odot}$ and 0.613$\\pm$0.007 R$_{\\odot}$for the primary and 0.341$\\pm$0.012M$_{\\odot}$ and 0.897$\\pm$0.012R$_{\\odot}$ for the secondary star. The distance to the system was estimated as 127$\\pm$14 pc. The observed wave-like distortion at out-of-eclipse is modeled with two separate s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.8133","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"}