KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three Microlensing Planets Detected via Partially Covered Signals

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aut.relation.endpageA90
aut.relation.journalAstronomy and Astrophysics: a European journal
aut.relation.startpageA90
aut.relation.volume674
dc.contributor.authorHan, Cheongho
dc.contributor.authorLee, Chung-Uk
dc.contributor.authorZang, Weicheng
dc.contributor.authorJung, Youn Kil
dc.contributor.authorChristie, Grant W
dc.contributor.authorZhang, Jiyuan
dc.contributor.authorAlbrow, Michael D
dc.contributor.authorChung, Sun-Ju
dc.contributor.authorGould, Andrew
dc.contributor.authorHwang, Kyu-Ha
dc.contributor.authorKim, Doeon
dc.contributor.authorRyu, Yoon-Hyun
dc.contributor.authorShin, In-Gu
dc.contributor.authorShvartzvald, Yossi
dc.contributor.authorYang, Hongjing
dc.contributor.authorYee, Jennifer C
dc.contributor.authorCha, Sang-Mok
dc.contributor.authorKim, Dong-Jin
dc.contributor.authorKim, Seung-Lee
dc.contributor.authorLee, Dong-Joo
dc.contributor.authorLee, Yongseok
dc.contributor.authorPark, Byeong-Gon
dc.contributor.authorPogge, Richard W
dc.contributor.authorNatusch, Tim
dc.contributor.authorMao, Shude
dc.contributor.authorMaoz, Dan
dc.contributor.authorPenny, Matthew T
dc.contributor.authorZhu, Wei
dc.date.accessioned2023-07-11T02:28:41Z
dc.date.available2023-07-11T02:28:41Z
dc.date.issued2023-06-07
dc.description.abstractAims. We inspect the four microlensing events KMT-2021-BLG-1968, KMT-2021-BLG-2010, KMT-2022-BLG-0371, and KMT-2022-BLG-1013, for which the light curves exhibit partially covered short-term central anomalies. We conduct detailed analyses of the events with the aim of revealing the nature of the anomalies. Methods. We tested various models that can explain the anomalies of the individual events, including the binary-lens (2L1S) and binary-source (1L2S) interpretations. Under the 2L1S interpretation, we thoroughly inspected the parameter space to determine the existence of degenerate solutions, and if they existed, we tested whether the degeneracy could be resolved. Results. We find that the anomalies in KMT-2021-BLG-2010 and KMT-2022-BLG-1013 are uniquely defined by planetary-lens interpretations with planet-to-host mass ratios of q ~ 2.8 × 10−3 and ~1.6 × 10−3, respectively. For KMT-2022-BLG-0371, a planetary solution with a mass ratio q ~ 4 × 10−4 is strongly favored over the other three degenerate 2L1S solutions with different mass ratios based on the χ2 and relative proper motion arguments, and a 1L2S solution is clearly ruled out. For KMT-2021-BLG-1968, on the other hand, we find that the anomaly can be explained either by a planetary or a binary-source interpretation, making it difficult to firmly identify the nature of the anomaly. From the Bayesian analyses of the identified planetary events, we estimate that the masses of the planet and host are (Mp/MJ, Mh/M⊙) = (1.07−0.68+1.15, 0.37−0.23+0.40), (0.26−0.11+0.13, 0.63−0.28+0.32), and (0.31−0.16+0.46, 0.18−0.10+0.28) for KMT-2021-BLG-2010L, KMT-2022-BLG-0371L, and KMT-2022-BLG-1013L, respectively.
dc.identifier.citationAstronomy and Astrophysics: a European journal, ISSN: 0004-6361 (Print); 1432-0746 (Online), EDP Sciences, 674, A90-A90. doi: 10.1051/0004-6361/202346298
dc.identifier.doi10.1051/0004-6361/202346298
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttp://hdl.handle.net/10292/16415
dc.publisherEDP Sciences
dc.relation.urihttps://www.aanda.org/articles/aa/full_html/2023/06/aa46298-23/aa46298-23.html
dc.rights.accessrightsOpenAccess
dc.rights.urihttps://creativecommons.org/licenses/by/4.0
dc.subject5109 Space Sciences
dc.subject51 Physical Sciences
dc.subject0201 Astronomical and Space Sciences
dc.subjectAstronomy & Astrophysics
dc.subject5101 Astronomical sciences
dc.subject5107 Particle and high energy physics
dc.subject5109 Space sciences
dc.titleKMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three Microlensing Planets Detected via Partially Covered Signals
dc.typeJournal Article
pubs.elements-id510831
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