The Many Possible Interpretations of Microlensing Event OGLE-2002-BLG-055
| dc.creator | Gaudi, B. Scott | |
| dc.creator | Han, Cheongho | |
| dc.date | 2004-02-17 | |
| dc.date | 2004-04-20 | |
| dc.date.accessioned | 2026-07-07T10:27:11Z | |
| dc.date.available | 2026-07-07T10:27:11Z | |
| dc.description | Microlensing event OGLE-2002-BLG-055 is characterized by a smooth, slightly asymmetric single-lens curve with an isolated, secure data point that is ~0.6 magnitudes brighter than neighboring points separated by a few days. It was previously suggested that the single deviant data point and global asymmetry were best explained by a planetary companion to the primary lens with mass ratio log(q)=-3 to -2, and parallax effects induced by the motion of the Earth. We revisit the interpretation of OGLE-2002-BLG-055, and show that the data can be explained by wide variety of models. We find that the deviant data point can be fit by a large number of qualitatively different binary-lens models whose mass ratios range, at the ~3-sigma level, from log(q) ~ -4 to -1. This range is consistent with a planet, brown dwarf, or M-dwarf companion for reasonable primary masses of M> 0.8 M_sun. A subset of these binary-lens fits consist of a family of continuously degenerate models whose mass ratios differ by an order-of-magnitude, but whose light curves differ by <2% for the majority of the perturbation. The deviant data point can also explained by a binary companion to the source with secondary/primary flux ratio of ~1%. This model has the added appeal that the global asymmetry is naturally explained by the acceleration of the primary induced by the secondary. The binary-source model yields a measurement of the Einstein ring radius projected on source plane of \hat r_E=1.87 +/- 0.40 AU. OGLE-2002-BLG-055 is an extreme example that illustrates the difficulties and degeneracies inherent in the interpretation of weakly perturbed and/or poorly sampled microlensing light curves. | |
| dc.description | 8 pages, 3 figures, 1 table. Minor changes. Accepted to ApJ, to appear in the August 10, 2004 issue (v611) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0402417 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0402417 | |
| dc.identifier | Astrophys.J.611:528-536,2004 | |
| dc.identifier | doi:10.1086/421971 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177078 | |
| dc.subject | Astrophysics | |
| dc.title | The Many Possible Interpretations of Microlensing Event OGLE-2002-BLG-055 | |
| dc.type | text |