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Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-mass Microlensing Planet OGLE-2017-BLG-1140Lb
cris.lastimport.scopus | 2024-02-12T20:14:07Z |
dc.abstract.en | We analyze the combined Spitzer and ground-based data for OGLE-2017-BLG-1140 and show that the event was generated by a Jupiter-class ({m}<SUB>p</SUB>≃ 1.6 {M}<SUB>{{J</SUB>}{{u}}{{p}}}) planet orbiting a mid-late M dwarf (M≃ 0.2 {M}<SUB>⊙ </SUB>) that lies {D}<SUB>LS</SUB>}≃ 1.0 {kpc} in the foreground of the microlensed Galactic-bar source star. The planet-host projected separation is {a}<SUB>\perp </SUB>≃ 1.0 {au}, i.e., well beyond the snow line. By measuring the source proper motion {{\boldsymbol{μ }}}<SUB>s</SUB> from ongoing long-term OGLE imaging and combining this with the lens-source relative proper motion {{\boldsymbol{μ }}}<SUB>rel</SUB>} derived from the microlensing solution, we show that the lens proper motion {{\boldsymbol{μ }}}<SUB>l</SUB>={{\boldsymbol{μ }}}<SUB>rel</SUB>}+{{\boldsymbol{μ }}}<SUB>s</SUB> is consistent with the lens lying in the Galactic disk, although a bulge lens is not ruled out. We show that while the Spitzer and ground-based data are comparably well fitted by planetary (i.e., binary-lens (2L1S)) and binary-source (1L2S) models, the combination of Spitzer and ground-based data decisively favors the planetary model. This is a new channel to resolve the 2L1S/1L2S degeneracy, which can be difficult to break in some cases. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Novati, S. Calchi |
dc.contributor.author | Skowron, Jan |
dc.contributor.author | Jung, Y. K. |
dc.contributor.author | Beichman, C. |
dc.contributor.author | Bryden, G. |
dc.contributor.author | Carey, S. |
dc.contributor.author | Gaudi, B. S. |
dc.contributor.author | Henderson, C. B. |
dc.contributor.author | Shvartzvald, Y. |
dc.contributor.author | Yee, J. C. |
dc.contributor.author | Zhu, W. |
dc.contributor.author | Udalski, Andrzej |
dc.contributor.author | Szymański, Michał |
dc.contributor.author | Mróz, Przemysław |
dc.contributor.author | Poleski, Radosław |
dc.contributor.author | Soszyński, Igor |
dc.contributor.author | Kozłowski, Szymon |
dc.contributor.author | Pietrukowicz, Paweł |
dc.contributor.author | Ulaczyk, Krzysztof |
dc.contributor.author | Pawlak, Michał |
dc.contributor.author | Rybicki, Krzysztof |
dc.contributor.author | Iwanek, Patryk |
dc.contributor.author | Albrow, M. D. |
dc.contributor.author | Chung, S. -J. |
dc.contributor.author | Gould, A. |
dc.contributor.author | Han, C. |
dc.contributor.author | Hwang, K. -H. |
dc.contributor.author | Ryu, Y. -H. |
dc.contributor.author | Shin, I. -G. |
dc.contributor.author | Zang, W. |
dc.contributor.author | Cha, S. -M. |
dc.contributor.author | Kim, D. -J. |
dc.contributor.author | Kim, H. -W. |
dc.contributor.author | Kim, S. -L. |
dc.contributor.author | Lee, C. -U. |
dc.contributor.author | Lee, D. -J. |
dc.contributor.author | Lee, Y. |
dc.contributor.author | Park, B. -G. |
dc.contributor.author | Pogge, R. W. |
dc.date.accessioned | 2024-01-26T07:57:38Z |
dc.date.available | 2024-01-26T07:57:38Z |
dc.date.copyright | 2018-03-12 |
dc.date.issued | 2018 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Nie dotyczy |
dc.description.number | 6 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 155 |
dc.identifier.doi | 10.3847/1538-3881/AAC21C |
dc.identifier.issn | 0004-6256 |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/120402 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2018AJ....155..261C |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Astronomical Journal |
dc.relation.pages | 261 |
dc.rights | Other |
dc.sciencecloud | nosend |
dc.title | Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-mass Microlensing Planet OGLE-2017-BLG-1140Lb |
dc.type | JournalArticle |
dspace.entity.type | Publication |