{"paper":{"title":"A transit survey to search for planets around hot subdwarfs: I. methods and performance tests on light curves from Kepler, K2, TESS, and CHEOPS","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Bekkelien, A. Brandeker, A. C. Cameron, A. Erikson, A. E. Simon, A. Fortier, A. Lecavelier des Etangs, A. M. S. Smith, A. Mustill, A. Thuillier, B. N. Barlow, B.-O. Demory, C. Broeg, C. Lovis, D. Barrado, D. Ehrenreich, D. Futyan, D. Gandolfi, D. Magrin, D. Pollacco, D. Queloz, D. S\\'egransan, E. Pall\\'e, F. J. Pozuelos, G. Anglada Escud\\'e, G. Bruno, G. M. Szab\\'o, G. Olofsson, G. Peter, G. Piotto, G. Scandariato, H. Rauer, I. Pagano, I. Ribas, J. Asquier, J. Cabrera, J. Laskar, J.-Y. Plesseria, K. G. Isaak, K. Heng, K. Westerdorff, L. Delrez, L. Fossati, L. Kiss, M. B. Davies, M. Beck, M. Deleuil, M. D\\'evora-Pajares, M. Fridlund, M. Gillon, M. Guedel, M. Lendl, M. Mecina, M. Steller, N. A. Walton, N. Billot, N. C. Santos, N. Rando, N. Thomas, O. D. S. Demangeon, P. F. L. Maxted, R. Alonso, R. H. {\\O}stensen, R. Ottensamer, R. Ragazzoni, R. Silvotti, S. C. C. Barros, S. Charnoz, S. Charpinet, S. G. Sousa, S. Hoyer, S. Udry, T. B\\'arczy, T. Beck, T. G. Wilson, V. Nascimbeni, V. Van Grootel, V. Viotto, W. Baumjohann, W. Benz, X. Bonfils, Y. Alibert","submitted_at":"2021-04-21T11:13:56Z","abstract_excerpt":"Context. Hot subdwarfs experienced strong mass loss on the Red Giant Branch (RGB) and are now hot and small He-burning objects. Aims. In this project we aim to perform a transit survey in all available light curves of hot subdwarfs from space-based telescopes (Kepler, K2, TESS, and CHEOPS), with our custom-made pipeline SHERLOCK, in order to determine the occurrence rate of planets around these stars, as a function of orbital period and planetary radius. Methods. In this first paper, we perform injection-and-recovery tests of synthetic transits for a selection of representative Kepler, K2 and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.10462","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2104.10462/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}