{"paper":{"title":"New and updated convex shape models of asteroids based on optical data from a large collaboration network","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Cikota, A. Collet, A. Debackere, A. Decock, A. Escalante del Valle, A. Hygate, A. Klotz, A. Leroy, A. Marciniak, A. Martin, A. Peyrot, A. Scholz, A. Spiridakis, A. Stiepen, A. Vagnozzi, B. Badue, B. Carry, B. Chinaglia, B.D. Warner, B. Lesquerbault, B. Mallecot, B. Modave, B. Morton, B. Skiff, B. Vanoutryve, C. Demeautis, C. Fournel, C. Gillier, C. Rinner, D.A. Oszkiewicz, D. Fradet, D. Higgins, D. Renauld, D. Ricci, D. Robilliard, D. Romeuf, D. Starkey, E. Barbotin, E. Conseil, E. Forn\\'e, E. Jehin, E. Kosturkiewicz, E. Morelle, E. Splanska, F. Carrier, F. Colas, F. Kugel, F. Manzini, F. Pilcher, F. Reignier, F. Richard, F. Sold\\'an, G. Canaud, G. Casalnuovo, G. Dubos, G. Hodosan, G. Rousseau, G. S\\'en\\'e, G. Tumolo, H. Hamanowa, H. Jacquinot, H. Pallares, I. Bozhinova, J. Brinsfield, J. Caron, J. Coloma, J-F. Coliac, J-F. Pirenne, J. Garlitz, J-G. Bosch, J. Hanu\\v{s}, J. Lecacheux, J. Manfroid, J. Montier, J.M. Vugnon, J. Nomen, J. Oey, J-P. Godard, J.P. Previt, J-P. Teng, J. Ruthroff, J. Strajnic, J. \\v{D}urech, K. Hay, K. Sobkowiak, L. Arnold, L. Berard, L. Bernasconi, L. Brunetto, L. Chalamet, L. Jerosimic, L. Salvador, M. Audejean, M. Bachschmidt, M. Cerda, M. Conjat, M. Cristofanelli, M. Delbo', M. Dr\\'o\\.zd\\.z, M. Dumont, M. Esteban, M. Fauerbach, M. Fauvaud, M. Gillon, M. Hren, M.J. Lopez-Gonzales, M. Lehk\\'y, M. Lutz, M. Paiella, M. Polinska, M. Polotto, M. Waucomont, M. Winiarski, M. Wolf, N. Berger, N. Esseiva, N. Innocent, O. Adam, O. Gerteis, O. Labrevoir, O. Wertz, P. Antonini, P.A. Salom, P. Aurard, P. Barroy, P. Baudouin, P. Korlevic, P. Krafft, P. Piron, P. Sogorb, Q. D\\'ehais, R. Anquetin, R. Behrend, R. Costa, R. Crippa, R. Durkee, R. Dymock, R. Esseiva, R. Giraud, R. Goncalves, R. Hirsch, R. Montaigut, R. Naves, R. Poncy, R. Roy, R. Stephens, R. Stoss, S. Bouley, S. Casulli, S. Charbonnel, S. Delmelle, S. Fauvaud, S. Hellmich, S. Heterier, S. Jawahar, S. Mottola, S. Sanchez, S. Sposetti, T. D\\'el\\'eage, T. Dulcamara, T. Fauchez, T. Santana-Ros, V. Afonina, V. Risoldi, W. Koff, W. Og{\\l}oza, Y. Damerdji, Y. Krugly","submitted_at":"2015-10-26T09:35:45Z","abstract_excerpt":"Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep insight into physical properties of main-belt asteroids or large collisional families. We aim to increase the number of asteroid shape models and rotation states. Such results are an important input for various further studies such as analysis of asteroid physical properties in different populations, including smaller collisional families, thermophysical modeling, and scaling shape models by disk-resolved images, or st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.07422","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"}