{"paper":{"title":"The SPHERE infrared survey for exoplanets (SHINE) -- II. Observations, Data reduction and analysis Detection performances and early-results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A.Baruffolo, A. Bazzon, A. Boccaletti, A. Cheetham, A. Costille, A. Delboulbe, A.-L. Maire, A.-M. Lagrange, A. Muller, A. Origne, A. Pavlov, A. Perreti, A. Roux, A. Sevin, A. Vigan, A. Zurlo, B. Biller, B. Salasnich, C. Dominik, C. Fontanive, C. Gry, C. Lazzoni, C. Perrot, C. Petit, C. Romero, C. Soenke, D. Fantinel, D. Gisler, D. Le Mignant, D. Maurel, D. Mesa, D. Mouillet, D. Perret, D. Rouan, E. Cascone, E. Giro, E. Hugot, E. Lagadec, E. Rickman, E. Sissa, E. Stadler, E. Thiebaut, F. Allard, F. Cantalloube, F. Madec, F. Menard, F. Rigal, F. Wildi, G. Chauvin, G. Rousset, G. Salter, H. Le Coroller, H.M. Schmid, J. Antichi, J. Baudrand, J. Charton, J. F. Sauvage, J. Girard, J. Hagelberg, J. Lannier, J.-L. Beuzit, J. Milli, J. Pragt, J. Ramos, K. Dohlen, L. Abe, L. Denis, L. Gluck, L. Mugnier, L. Rodet, L. Weber, M. Bonavita, M. Bonnefoy, M. Carbillet, M. Carle, M. Feldt, M. Janson, M. Jaquet, M. Kasper, M. Keppler, M. Langlois, M. Llored, M. Meyer, M. Samland, M. Suarez, M. Turatto, N. Hubin, N. Meunier, O. Flasseur, O. Moller-Nilsson, P. Baudoz, P. Blanchard, P. Delorme, P. Feautrier, P. Gigan, P. Janin-Potiron, P. Martinez, P. Puget, P. Rabou, P. Rubini, R. Claudi, R. Galicher, R. Gratton, R. Ligi, R. Roelfsema, S. Daemgen, S. Desidera, S. Messina, S. Rochat, S. Udry, T. Bhowmik, T. Fusco, Th. Henning, T. Kopytova, T. Moulin, T. Schmidt, V. De Caprio, V. D'Orazi, W. Brandner, Y. Magnard, Z. Wahhaj","submitted_at":"2021-03-05T23:09:36Z","abstract_excerpt":"Over the past decades, direct imaging has confirmed the existence of substellar companions (exoplanets or brown dwarfs) on wide orbits (>10 au) from their host stars. To understand their formation and evolution mechanisms, we have initiated in 2015 the SPHERE infrared survey for exoplanets (SHINE), a systematic direct imaging survey of young, nearby stars to explore their demographics.} {We aim to detect and characterize the population of giant planets and brown dwarfs beyond the snow line around young, nearby stars. Combined with the survey completeness, our observations offer the opportunity"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.03976","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/2103.03976/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"}