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dc.contributor.authorXIE, Xiaojia
dc.contributor.authorDONG, Subo
dc.contributor.authorZHU, Wei
hal.structure.identifierThe Ohio State University [Columbus] [OSU]
dc.contributor.authorGOULD, A.
hal.structure.identifierAstronomical Observatory [Warsaw]
dc.contributor.authorUDALSKI, A.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBEAULIEU, J.-P.
dc.contributor.authorCLOSE, L.
dc.contributor.authorMALES, J.
hal.structure.identifierM2A 2019
dc.contributor.authorMARQUETTE, J.-B.
dc.contributor.authorMORZINSKI, K.
dc.contributor.authorPOGGE, R.
dc.contributor.authorYEE, J.
dc.date.issued2021-03-01
dc.identifier.issn0004-6256
dc.description.sponsorshipStatistiques des planètes proches de leur lieu de formation et leur distribution dans le disque et la barre de notre Galaxie
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.title.enMagAO Observations of the Binary Microlens OGLE-2014-BLG-1050 Prefer the Higher-mass Solution
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-3881/abd6c0
dc.subject.halPlanète et Univers [physics]
dc.identifier.arxiv2112.08029
bordeaux.journalThe Astronomical Journal
bordeaux.page113
bordeaux.volume161
bordeaux.issue3
bordeaux.peerReviewedoui
hal.identifierhal-03430357
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03430357v1
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