{"paper":{"title":"Reanalyses of Anomalous Gravitational Microlensing Events in the OGLE-III Early Warning System Database with Combined Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Allan, A. Cassan, A. Cole, A. Fukui, A. Gould, A. Maury, A. Udalski, A. Williams, A. Yonehara, B.-G. Park, B. S. Gaudi, C. Coutures, C. Han, C. Pitrou, C. S. Botzler, C. Snodgrass, C.-U. Lee, C. Vinter, D. Dominis Prester, D. Fukunaga, D. J. Sullivan, D. Kubas, D. L. DePoy, D. Maoz, D. M. Bramich, D. Moorhouse, D. P. Bennett, D. Suzuki, E. O. Ofek, F. Abe, F. Mallia, G. Bolt, G. Pietrzy\\'nski, G. Thornley, G. W. Christie, H. Park, I. A. Bond, I.-G. Shin, I. Soszy\\'nski, I. Steele, J. A. R. Caldwell, J.-B. Marquette, J. C. Yee, J. Donatowicz, J. Drummond, J. Greenhill, J. Jeong, J. McCormick, J. Menzies, J.-P. Beaulieu, J. Wambsganss, J.-Y. Choi, K. C. Sahu, K.-H. Hwang, K. Horne, K. Masuda, K. Ohnishi, K. Pollard, K. Ulaczyk, K. Wada, L. A. G. Monard, \\L. Wyrzykowski, M. D. Albrow, M. Dominik, M. Freeman, M. Hoffman, M. Huber, M. Hundertmark, M. J. Burgdorf, M. K. Szyma\\'nski, N. J. Rattenbury, N. Kains, N. Koshimoto, N. Tsurumi, N. Yamai, P. C. M. Yock, P. Fouqu\\'e, P. J. Tristram, R. Martin, R. Poleski, R. Santallo, R. Street, R. W. Pogge, S. Dieters, S. Namba, S. R. Kane, T. Natusch, To. Saito, T. Sumi, U. G. J{\\o}rgensen, V. Batista, W. Allen, W. L. Sweatman, Y. Itow, Y. K. Jung, Y. Matsubara, Y. Muraki, Y. Tsapras","submitted_at":"2015-02-24T00:50:34Z","abstract_excerpt":"We reanalyze microlensing events in the published list of anomalous events that were observed from the OGLE lensing survey conducted during 2004-2008 period. In order to check the existence of possible degenerate solutions and extract extra information, we conduct analyses based on combined data from other survey and follow-up observation and consider higher-order effects. Among the analyzed events, we present analyses of 8 events for which either new solutions are identified or additional information is obtained. We find that the previous binary-source interpretations of 5 events are better i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.06663","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"}