{"paper":{"title":"KIC011764567: An evolved object showing substantial flare-activity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Akopian, G. Torres, M. Kitze, R. Neuh\\\"auser, V. Hambaryan","submitted_at":"2016-07-28T11:51:33Z","abstract_excerpt":"We intensively studied the flare activity on the stellar object KIC011764567. The star was thought to be solar type, with a temperature of $T_{eff} = (5640 \\pm 200)\\,$K, $\\log(g) = (4.3 \\pm 0.3)\\,$dex and a rotational period of Prot 22 d (Brown et al. 2011). High resolution spectra turn the target to an evolved object with Teff = (5300 \\pm 150) K, a metalicity of $[m/H] = (-0.5 \\pm 0.2)$, a surface gravity of $log(g) = (3.3 \\pm 0.4)\\,$dex, and a projected rotational velocity of $v sin i = (22 \\pm 1)\\,kms^{-1}$. Within an observing time span of 4 years we detected 150 flares in Kepler data in a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.08412","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"}