{"paper":{"title":"OGLE-2008-BLG-513Lb: The Orbital Solution for a Microlensing Planet","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Gould, A. Udalski, A. Williams, C. Han, et al, I.A. Bond, J. An, J.C. Yee, J. Greenhill, J. McCormick, L.A.G. Monard, M.D. Albrow, M. Dominik, N. Kains, P. Fouque, S. Kozlowski, Subo Dong, Y. Tsapras","submitted_at":"2011-06-20T20:00:06Z","abstract_excerpt":"A static binary star solution for OGLE-2008-BLG-513 has been\nfound. The mass ratio and separation for this solution are q~0.28,\ns~0.86. This model has a chi^2 comparable to the chi^2 of the model\nwith a planetary mass ratio and orbital motion that was presented in\nthis paper. Because the model with a static, binary star lens is\nsimpler than the model originally presented in this paper, Occam's\nRazor says it is likely to be the correct solution. Consequently, this\npaper has been withdrawn from ApJ."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.4013","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"}