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OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event
dc.abstract.en | We present the analysis of the microlensing event OGLE-2016-BLG-1227. The light curve of this short-duration event appears to be a single-lens event affected by severe finite-source effects. Analysis of the light curve based on a single-lens single-source (1L1S) model yields very small values of the event timescale, ${t}_{{\rm{E}}}\sim 3.5$ days, and the angular Einstein radius, ${\theta }_{{\rm{E}}}\sim 0.009$ mas, making the lens a candidate of a free-floating planet. Close inspection reveals that the 1L1S solution leaves small residuals with an amplitude of ΔI ≲ 0.03 mag. We find that the residuals are explained by the existence of an additional widely separated heavier lens component, indicating that the lens is a wide-separation planetary system rather than a free-floating planet. From Bayesian analysis, it is estimated that the planet has a mass of ${M}_{{\rm{p}}}={0.79}_{-0.39}^{+1.30}\,{M}_{{\rm{J}}}$ and it is orbiting a low-mass host star with a mass of ${M}_{\mathrm{host}}={0.10}_{-0.05}^{+0.17}\,{M}_{\odot }$ located with a projected separation of ${a}_{\perp }={3.4}_{-1.0}^{+2.1}$ au. The planetary system is located in the Galactic bulge with a line-of-sight separation from the source star of ${D}_{\mathrm{LS}}={1.21}_{-0.63}^{+0.96}$ kpc. The event shows that there is a range of deviations in the signatures of host stars for apparently isolated planetary lensing events and that it is possible to identify a host even when a deviation is subtle. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Han, Cheongho |
dc.contributor.author | Udalski, Andrzej |
dc.contributor.author | Gould, Andrew |
dc.contributor.author | Albrow, Michael D. |
dc.contributor.author | Chung, Sun-Ju |
dc.contributor.author | Hwang, Kyu-Ha |
dc.contributor.author | Jung, Youn Kil |
dc.contributor.author | Lee, Chung-Uk |
dc.contributor.author | Ryu, Yoon-Hyun |
dc.contributor.author | Shin, In-Gu |
dc.contributor.author | Shvartzvald, Yossi |
dc.contributor.author | Yee, Jennifer C. |
dc.contributor.author | Zang, Weicheng |
dc.contributor.author | Cha, Sang-Mok |
dc.contributor.author | Kim, Dong-Jin |
dc.contributor.author | Kim, Hyoun-Woo |
dc.contributor.author | Kim, Seung-Lee |
dc.contributor.author | Lee, Dong-Joo |
dc.contributor.author | Lee, Yongseok |
dc.contributor.author | Park, Byeong-Gon |
dc.contributor.author | Pogge, Richard W. |
dc.contributor.author | Jee, M. James |
dc.contributor.author | Kim, Doeon |
dc.contributor.author | Kim, Chun-Hwey |
dc.contributor.author | Kim, Woong-Tae |
dc.contributor.author | Mróz, Przemysław |
dc.contributor.author | Szymański, Michał |
dc.contributor.author | Skowron, Jan |
dc.contributor.author | Poleski, Radosław |
dc.contributor.author | Soszyński, Igor |
dc.contributor.author | Pietrukowicz, Paweł |
dc.contributor.author | Kozłowski, Szymon |
dc.contributor.author | Ulaczyk, Krzysztof |
dc.date.accessioned | 2024-01-25T15:40:40Z |
dc.date.available | 2024-01-25T15:40:40Z |
dc.date.copyright | 2019-11-27 |
dc.date.issued | 2020 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Publikacja bezkosztowa |
dc.description.number | 3 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 159 |
dc.identifier.doi | 10.3847/1538-3881/AB6A9F |
dc.identifier.issn | 0004-6256 |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/114505 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2020AJ....159...91H |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Astronomical Journal |
dc.relation.pages | 91 |
dc.rights | Other |
dc.sciencecloud | nosend |
dc.title | OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event |
dc.type | JournalArticle |
dspace.entity.type | Publication |