{"paper":{"title":"Discovery of a warm, dusty giant planet around HIP65426","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"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. Orign\\'e, A. Pavlov, A. Roux, A. Sevin, A. Vigan, A. Zurlo, B. Biller, B. Charnay, B. Salasnich, C. Dominik, C. Gry, C. Mordasini, C. Moutou, C. Perrot, C. Petit, C. Soenke, C. Thalmann, 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. Sissa, E. Stadler, F. Madec, F. Menard, F. Vakili, F. Wildi, G. Chauvin, G.D. Marleau, G. Rousset, H. Le Coroller, H.-M. Schmid, J. Antichi, J. Baudrand, J.-C. Augereau, J. Charton, J.-F. Sauvage, J. Girard, J. Hagelberg, J.-L. Baudino, J.-L. Beuzit, J. Milli, J. Olofsson, J. Pragt, J. Ramos, J. Schlieder, J. Szul\\'agyi, K. Dohlen, L. Abe, L. Gluck, L. Rodet, L. Weber, M. Bonavita, M. Bonnefoy, M. Carbillet, M. Carle, M. Cudel, M. Feldt, M. Janson, M. Jaquet, M. Kasper, M. Keppler, M. Langlois, M. Llored, M. Meyer, M. Samland, M. Suarez, M. Turatto, N. Engler, N. Hubin, O. Moller-Nilsson, P. Baudoz, P. Blanchard, P. Delorme, P. Feautrier, P. Gigan, P. Janin-Potiron, P. Martinez, P. Molliere, P. Puget, P. Rabou, Q. Kral, R. Claudi, R. Galicher, R. Gratton, R. Ligi, R. Rigal, R. Roelfsema, S. Antoniucci, S. Daemgen, S. Desidera, S. Messina, S. Peretti, S. Rochat, S. Udry, T. Buey, T. Fusco, T. Henning, T. Kopytova, T. Moulin, T.O.B. Schmidt, V. De Caprio, V. D'Orazi, W. Brandner, Y. Magnard, Z. Wahhaj","submitted_at":"2017-07-05T14:21:46Z","abstract_excerpt":"The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's unprecedented high-contrast and high-angular resolution imaging capabilities. It also intends at placing statistical constraints on the occurrence and orbital properties of the giant planet population at large orbits as a function of the stellar host mass and age to test planet formation theories. We use the IRDIS dual-band imager and the IFS integral field spectrograph of SPHERE to acquire high-constrast coronagrap"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.01413","kind":"arxiv","version":2},"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"}