Pulse Brain · Growing Health Evidence Index
Peer-reviewed

OGLE-2012-BLG-0455/MOA-2012-BLG-206: MICROLENSING EVENT WITH AMBIGUITY IN PLANETARY INTERPRETATIONS CAUSED BY INCOMPLETE COVERAGE OF PLANETARY SIGNAL

H. Park, Cheongho Han, Andrew Gould, A. Udalski, T. Sumi, P. Fouqué, J.-Y. Choi, Grant Christie, D. L. DePoy, Subo Dong, B. Scott Gaudi, Kyu‐Ha Hwang, Youn Kil Jung, A. Kavka, Chung‐Uk Lee, L. A. G. Monard, T. Natusch, H. Ngan, Richard W. Pogge, In-Gu Shin, Jennifer C. Yee, M. K. Szymański, M. Kubiak, I. Soszyński, G. Pietrzyński, R. Poleski, K. Ulaczyk, P. Pietrukowicz, S. Kozłowski, J. Skowron, Ł. Wyrzykowski, F. Abe, D. P. Bennett, I. A. Bond, C. S. Botzler, P. Chote, M. Freeman, Akihiko Fukui, D. Fukunaga, P. Harris, Y. Itow, Naoki Koshimoto, C. H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, S. Namba, Kei Ohnishi, Nicholas J. Rattenbury, To. Saito, D. J. Sullivan, W. L. Sweatman, Daisuke Suzuki, P. J. Tristram, K. Wada, N. Yamai, P. C. M. Yock, A. Yonehara

OakTrust (Texas A&M University Libraries) · 2019

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Summary

Characterizing a microlensing planet is done by modeling an observed lensing light curve. In this process, it is often confronted that solutions of different lensing parameters result in similar light curves, causing difficulties in uniquely interpreting the lens system, and thus understanding the causes of different types of degeneracy is important. In this work, we show that incomplete coverage of a planetary perturbation can result in degenerate solutions even for events where the planetary signal is detected with a high level of statistical significance. We demonstrate the degeneracy for an actually observed event OGLE-2012-BLG-0455/MOA-2012-BLG-206. The peak of this high-magnification event (Amax ∼ 400) exhibits very strong deviation from a point-lens model with Δχ2 ≳ 4000 for data se

Source type
Peer-reviewed study
Catalogue ID
BFmoakvi7g-tehhyg
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