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ヨネハラ アツノリ
YONEHARA ATSUNORI
米原 厚憲 所属 京都産業大学 理学部 宇宙物理・気象学科 職種 教授 |
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| 言語種別 | 英語 |
| 発行・発表の年月 | 2014/05 |
| 形態種別 | その他 |
| 標題 | OGLE-2012-BLG-0455/MOA-2012-BLG-206: MICROLENSING EVENT WITH AMBIGUITY IN PLANETARY INTERPRETATIONS CAUSED BY INCOMPLETE COVERAGE OF PLANETARY SIGNAL |
| 執筆形態 | その他 |
| 掲載誌名 | ASTROPHYSICAL JOURNAL |
| 出版社・発行元 | IOP PUBLISHING LTD |
| 巻・号・頁 | 787(1),pp.id. 71 (6 pp) |
| 著者・共著者 | H. Park,C. Han,A. Gould,A. Udalski,T. Sumi,P. Fouque,J. -Y. Choi,G. Christie,D. L. Depoy,Subo Dong,B. S. Gaudi,K. -H. Hwang,Y. K. Jung,A. Kavka,C. -U. Lee,L. A. G. Monard,T. Natusch,H. Ngan,R. W. Pogge,I. -G. Shin,J. C. Yee,M. K. Szymanski,M. Kubiak,I. Soszynski,G. Pietrzynski,R. Poleski,K. Ulaczyk,P. Pietrukowicz,S. Kozlowski,J. Skowron,L. Wyrzykowski,F. Abe,D. P. Bennett,I. A. Bond,C. S. Botzler,P. Chote,M. Freeman,A. Fukui,D. Fukunaga,P. Harris,Y. Itow,N. Koshimoto,C. H. Ling,K. Masuda,Y. Matsubara,Y. Muraki,S. Namba,K. Ohnishi,N. J. Rattenbury,To. Saito,D. J. Sullivan,W. L. Sweatman,D. Suzuki,P. J. Tristram,K. Wada,N. Yamai,P. C. M. Yock,A. Yonehara |
| 概要 | 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 (A(max) similar to 400) exhibits very strong deviation from a point-lens model with Delta chi(2) greater than or similar to 4000 for data sets with a total of 6963 measurements. From detailed modeling of the light curve, we find that the deviation can be explained by four distinct solutions, i.e., two very different sets of solutions, each with a twofold degeneracy. While the twofold (so-called close/wide) degeneracy is well understood, the degeneracy between the radically different solutions is not previously known. The model light curves of this degeneracy differ substantially in the parts that were not covered by observation, indicating that the degeneracy is caused by the incomplete coverage of the perturbation. It is expected that the frequency of the degeneracy introduced in this work will be greatly reduced with the improvement of the current lensing survey and follow-up experiments and the advent of new surveys. |
| DOI | 10.1088/0004-637X/787/1/71 |
| ISSN | 0004-637X/1538-4357 |