{"paper":{"title":"The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.EP","authors_text":"A. Baruffolo, A. Bazzon, A. Boccaletti, A. Cheetham, A. Costille, A. Delboulb\\'e, A. J. Bohn, A.-L. Maire, A.-M. Lagrange, A. M\\\"uller, A. Orign\\'e, A. Pavlov, A. Roux, A. Sevin, A. Vigan, A. Zurlo, B. Biller, B. Salasnich, C. Dominik, C. Fontanive, C. Gry, C. Lazzoni, C. Mordasini, C. Moutou, C. Perrot, C. Petit, C. Soenke, D. Albert, D. Fantinel, D. Gisler, D. Le Mignant, D. Maurel, D. Mesa, D. Mouillet, D. Nardiello, D. Perret, E. Cascone, E. Giro, E. Hugot, E. Lagadec, E. Sissa, E. Stadler, F. Cantalloube, F. Kiefer, F. Madec, F. M\\'enard, F. Rigal, F. Wildi, G. Chauvin, G.-D. Marleau, G. Rousset, H. Le Coroller, H. M. Schmid, J. Antichi, J. Baudrand, J. Charton, J.-F. Sauvage, J. Hagelberg, J. H. Girard, J.-L. Beuzit, J. Pragt, J. Ramos, K. Dohlen, L. Abe, L. Gl\\\"uck, L. Weber, M. Bonavita, M. Bonnefoy, M. Carbillet, M. Carle, M. Feldt, M. Janson, M. Jaquet, M. Kasper, M. Langlois, M. Llored, M. Meyer, M. Samland, M. Su\\'arez, M. Turatto, N. Engler, N. Hubin, N. Meunier, O. M\\\"oller-Nilsson, P. Baudoz, P. Blanchard, P. Delorme, P. Feautrier, P. Gigan, P. Mart\\'inez, P. Puget, P. Rabou, R. Claudi, R. Galicher, R. Gratton, R. Ligi, R. Roelfsema, S. Bergeon, S. Desidera, S. Messina, S. Rochat, S. Udry, T. Fusco, Th. Henning, T. Moulin, T. Schmidt, V. De Caprio, V. D'Orazi, V. Squicciarini, W. Brandner, Y. Magnard, Z. Wahhaj","submitted_at":"2026-05-26T16:26:00Z","abstract_excerpt":"Unbiased surveys of large stellar samples are the prime means through which the prevalence of exoplanets can be derived, and crucial constraints to planet formation models can be set. Direct imaging (DI) is ideally positioned to probe the outer regions (5-300au) of planetary systems, providing complementary information to techniques such as transits and radial velocities. We present the full sample of the SpHere INfrared survey for Exoplanets (SHINE), the second largest DI campaign to date. SHINE observed 460 stars between 2015 and 2023 thanks to the Guaranteed Time Observations (GTO) allocate"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.27247","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/2605.27247/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"}