Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets

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dc.citation.issue1
dc.citation.volume165
dc.contributor.authorShin IG
dc.contributor.authorYee JC
dc.contributor.authorGould A
dc.contributor.authorHwang K-H
dc.contributor.authorYang H
dc.contributor.authorBond IA
dc.contributor.authorAlbrow MD
dc.contributor.authorChung S-J
dc.contributor.authorHan C
dc.contributor.authorJung YK
dc.contributor.authorRyu Y-H
dc.contributor.authorShvartzvald Y
dc.contributor.authorZang W
dc.contributor.authorCha S-M
dc.contributor.authorKim D-J
dc.contributor.authorKim S-L
dc.contributor.authorLee C-U
dc.contributor.authorLee D-J
dc.contributor.authorLee Y
dc.contributor.authorPark B-G
dc.contributor.authorPogge RW
dc.contributor.authorAbe F
dc.contributor.authorBarry R
dc.contributor.authorBennett DP
dc.contributor.authorBhattacharya A
dc.contributor.authorFujii H
dc.contributor.authorFukui A
dc.contributor.authorHirao Y
dc.contributor.authorIshitani Silva S
dc.contributor.authorItow Y
dc.contributor.authorKirikawa R
dc.contributor.authorKondo I
dc.contributor.authorKoshimoto N
dc.contributor.authorMatsubara Y
dc.contributor.authorMatsumoto S
dc.contributor.authorMiyazaki S
dc.contributor.authorMuraki Y
dc.contributor.authorOkamura A
dc.contributor.authorOlmschenk G
dc.contributor.authorRanc C
dc.contributor.authorRattenbury NJ
dc.contributor.authorSatoh Y
dc.contributor.authorSumi T
dc.contributor.authorSuzuki D
dc.contributor.authorToda T
dc.contributor.authorTristram PJ
dc.contributor.authorVandorou A
dc.contributor.authorYama H
dc.date.accessioned2024-04-30T23:15:09Z
dc.date.accessioned2024-07-25T06:34:04Z
dc.date.available2022-09-08
dc.date.available2024-04-30T23:15:09Z
dc.date.available2024-07-25T06:34:04Z
dc.date.issued2022-12-07
dc.description.abstractWe present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6M Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2M Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25M Nep planet orbiting a very-low-mass M dwarf or a brown dwarf. These by-eye planet detections provide an important comparison sample to the sample selected with the AnomalyFinder algorithm, and in particular, KMT-2021-BLG-2294 is a case of a planet detected by eye but not by algorithm. KMT-2021-BLG-2294Lb is part of a population of microlensing planets around very-low-mass host stars that spans the full range of planet masses, in contrast to the planet population at ≲0.1 au, which shows a strong preference for small planets.
dc.description.confidentialfalse
dc.edition.editionJanuary 2023
dc.identifier.citationShin IG, Yee JC, Gould A, Hwang KH, Yang H, Bond IA, Albrow MD, Chung SJ, Han C, Jung YK, Ryu YH, Shvartzvald Y, Zang W, Cha SM, Kim DJ, Kim SL, Lee CU, Lee DJ, Lee Y, Park BG, Pogge RW, Abe F, Barry R, Bennett DP, Bhattacharya A, Fujii H, Fukui A, Hirao Y, Silva SI, Itow Y, Kirikawa R, Kondo I, Koshimoto N, Matsubara Y, Matsumoto S, Miyazaki S, Muraki Y, Okamura A, Olmschenk G, Ranc C, Rattenbury NJ, Satoh Y, Sumi T, Suzuki D, Toda T, Tristram PJ, Vandorou A, Yama H. (2023). Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets. Astronomical Journal. 165. 1.
dc.identifier.doi10.3847/1538-3881/ac9d93
dc.identifier.eissn1538-3881
dc.identifier.elements-typejournal-article
dc.identifier.issn0004-6256
dc.identifier.number8
dc.identifier.urihttps://mro.massey.ac.nz/handle/10179/70438
dc.languageEnglish
dc.publisherAmerican Astronomical Society
dc.publisher.urihttps://iopscience.iop.org/article/10.3847/1538-3881/ac9d93
dc.relation.isPartOfAstronomical Journal
dc.rights(c) The author/s
dc.rights.licenseCC BY 4.0
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleMass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
dc.typeJournal article
pubs.elements-id458874
pubs.organisational-groupOther
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