{"paper":{"title":"The SPHERE infrared survey for exoplanets (SHINE)- I Sample definition and target characterization","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. Deboulbe, A-L. Maire, A-M. Lagrange, A. Muller, A. Origne, A. Pavlov, A. Roux, A. Sevin, A. Vigan, A. Zurlo R. Asensio-Torres, B. Biller, B. Salasnich, C. Dominik, C. Fontaniv, C. Lazzoni, C. Petit, C. Soenke, D. Fantinel, D. Gisler, D. Le Mignant, D. Maurel, D. Mesa, D. Perret, E. Cascone, E. Covino, E. Giro, E. Hugot, E. Lagadec, E. Rickman, E. Rigliaco, E. Sissa, E. Stadler, F. Cantalloube, F.-J. Hambsch, F. Madec, F. Menard, F. Rigal, F. Wildi, G. Chauvin, G. Rousset, H. LeCoroller, H.M. Schmid, J. Alcala, J. Antichi, J. Baudrand, J. Carson, J. Charton, J.-F. Sauvage, J. Hagelberg, J.-L. Beuzit, J. Pragt, J. Ramon, J. Schlieder, K. Dohlen, L. Abe, L. Gluck, 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. Millward, M. Samland, M. Suarez, M. Turatto, N. Hubin, O. Moller-Nilsson, P. Baudoz, P. Blanchard, P. Delorme, P. Feautrier, P. Gigan, P. Martinez, P. Puget, P. Rabou, R. Claudi, R. Galicher, R. Gratton, R. Ligi, R. Roelfsema, S. Benatti, S. Desidera, S. Messina, S. Rochat, S. Udry, T. Buey, T. Fusco, T.G. Tan, Th. Henning, T. Kopytova, T. Moulin, T. Schmidt, V. De Caprio, V. D'Orazi, W. Brandner, Y. Magnard","submitted_at":"2021-03-07T14:32:43Z","abstract_excerpt":"Large surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from $\\sim$5 to 300 AU. A careful assessment of the stellar properties is crucial for a proper understanding of when, where, and how frequently planets form, and how they evolve. The sensitivity of detection limits to stellar age makes this a key parameter for direct imaging surveys. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the contex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.04366","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/2103.04366/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"}