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dc.contributor.authorPOLESKI, R.
hal.structure.identifierDepartment of Astronomy [Ohio State University]
dc.contributor.authorGAUDI, B. S.
dc.contributor.authorXIE, Xiaojia
dc.contributor.authorUDALSKI, A.
dc.contributor.authorYEE, J. C.
dc.contributor.authorSKOWRON, J.
dc.contributor.authorSZYMAŃSKI, M. K.
dc.contributor.authorSOSZYŃSKI, I.
dc.contributor.authorPIETRUKOWICZ, P.
dc.contributor.authorKOZŁOWSKI, S.
dc.contributor.authorWYRZYKOWSKI, Ł.
dc.contributor.authorULACZYK, K.
dc.contributor.authorHAN, C.
dc.contributor.authorDONG, Subo
dc.contributor.authorMORZINSKI, K. M.
dc.contributor.authorMALES, J. R.
dc.contributor.authorCLOSE, L. M.
hal.structure.identifierDepartment of Astronomy [Ohio State University]
dc.contributor.authorGOULD, A.
hal.structure.identifierDepartment of Astronomy [Ohio State University]
dc.contributor.authorPOGGE, R. W.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBEAULIEU, J.-P.
hal.structure.identifierM2A 2019
dc.contributor.authorMARQUETTE, J.-B.
dc.date.issued2019-05-14
dc.identifier.issn0004-6256
dc.description.abstractEnWe present the discovery of a planet on a very wide orbit in the microlensing event OGLE-2012-BLG-0838. The signal of the planet is well separated from the main peak of the event and the planet-star projected separation is found to be twice larger than the Einstein ring radius, which roughly corresponds to a projected separation of ~4 AU. Similar planets around low-mass stars are very hard to find using any technique other than microlensing. We discuss microlensing model fitting in detail and discuss the prospects for measuring the mass and distance of lens system directly.
dc.description.sponsorshipStatistiques des planètes proches de leur lieu de formation et leur distribution dans le disque et la barre de notre Galaxie - ANR-18-CE31-0002
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.title.enA Wide Orbit Exoplanet OGLE-2012-BLG-0838Lb
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-3881/ab8a49
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1901.05466
bordeaux.journalThe Astronomical Journal
bordeaux.peerReviewedoui
hal.identifierhal-01993586
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01993586v1
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