{"paper":{"title":"Oscillation frequencies for 35 \\Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Karoff, D. Huber, D. Stello, G. R. Davies, H. Kjeldsen, J. Christensen-Dalsgaard, M. N. Lund, M. S. Lundkvist, O. Benomar, R. Handberg, S. Basu, S. Hekker, T. L. Campante, T. R. Bedding, T. R. White, T. S. Metcalfe, V. Silva Aguirre, W. J. Chaplin, Y. Elsworth","submitted_at":"2015-11-06T15:01:06Z","abstract_excerpt":"\\Kepler has revolutionised our understanding of both exoplanets and their host stars. Asteroseismology is a valuable tool in the characterisation of stars and \\Kepler is an excellent observing facility to perform asteroseismology. Here we select a sample of 35 \\Kepler solar-type stars which host transiting exoplanets (or planet candidates) with detected solar-like oscillations. Using available \\Kepler short cadence data up to Quarter 16 we create power spectra optimised for asteroseismology of solar-type stars. We identify modes of oscillation and estimate mode frequencies by ``peak bagging'' "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.02105","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"}