{"paper":{"title":"Transit Timing Analysis in the HAT-P-32 system","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"A. Pannicke, C. Ga{\\l}an, D. Cohen, D. Dimitrov, D. Kjurkchieva, D. Puchalski, E. Derman, E. G\\\"o\\u{g}\\\"u\\c{s}, E. Jensen, G. Maciejewski, G. Saral, I. Bernt, J. G. Schmidt, J. M. Ohlert, L. Marschall, M. Fernandez, M. Kitze, M. Mallonn, M. M. Hohle, M. Seeliger, R. Errmann, R. Neuh\\\"auser, S. Bilir, T. Ak, T. G\\\"uver, T. O. B. Schmidt, V. Casanova","submitted_at":"2014-04-25T08:51:18Z","abstract_excerpt":"We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YETI network. In 25 cases, complete transit light curves with a timing precision better than $1.4\\:$min have been obtained. These light curves have been used to refine the system properties, namely inclination $i$, planet-to-star radius ratio $R_\\textrm{p}/R_\\textrm{s}$, and the ratio between the semimajor axis and the stellar radius $a/R_\\textrm{s}$. First analyses by Hartman et al. (2011) suggest the existence of a s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.6354","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"}