{"paper":{"title":"Astrophysical false positives in direct imaging for exoplanets: a white dwarf close to a rejuvenated star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Vigan, A. Zurlo, C. Moutou, D. Mesa, D. Segransan, E. Covino, F. Wildi, G. Chauvin, J.C. Carson, J. Hagelberg, J.M. Almenara, K. Biazzo, M. Bonnefoy, M. Turatto, P. Delorme, R. Gratton, S. Desidera, S. Messina, S. Udry, V. D'Orazi","submitted_at":"2013-04-15T15:25:28Z","abstract_excerpt":"As is the case for all techniques involved in the research for exoplanets, direct imaging has to take into account the probability of so-called astrophysical false positives, which are phenomena that mimic the signature of objects we are seeking. In this work we aim to present a case of a false positive found during a direct imaging survey conducted with VLT/NACO. A promising exoplanet candidate was detected around the K2-type star HD\\,8049 in July 2010.Its contrast of $\\Delta H$=7.05 at 1.57 arcsec allowed us to guess the presence of a 35 \\MJup companion at 50 projected AU, for the nominal sy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.4130","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"}