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

We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _Nep planet orbiting a very-lo...
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Autor*in:	In-Gu Shin [verfasserIn] Jennifer C. Yee [verfasserIn] Andrew Gould [verfasserIn] Kyu-Ha Hwang [verfasserIn] Hongjing Yang [verfasserIn] Ian A. Bond [verfasserIn] (Leading Authors) [verfasserIn] Michael D. Albrow [verfasserIn] Sun-Ju Chung [verfasserIn] Cheongho Han [verfasserIn] Youn Kil Jung [verfasserIn] Yoon-Hyun Ryu [verfasserIn] Yossi Shvartzvald [verfasserIn] Weicheng Zang [verfasserIn] Sang-Mok Cha [verfasserIn] Dong-Jin Kim [verfasserIn] Seung-Lee Kim [verfasserIn] Chung-Uk Lee [verfasserIn] Dong-Joo Lee [verfasserIn] Yongseok Lee [verfasserIn] Byeong-Gon Park [verfasserIn] Richard W. Pogge [verfasserIn] (The KMTNet Collaboration) [verfasserIn] Fumio Abe [verfasserIn] Richard Barry [verfasserIn] David P. Bennett [verfasserIn] Aparna Bhattacharya [verfasserIn] Hirosane Fujii [verfasserIn] Akihiko Fukui [verfasserIn] Yuki Hirao [verfasserIn] Stela Ishitani Silva [verfasserIn] Yoshitaka Itow [verfasserIn] Rintaro Kirikawa [verfasserIn] Iona Kondo [verfasserIn] Naoki Koshimoto [verfasserIn] Yutaka Matsubara [verfasserIn] Sho Matsumoto [verfasserIn] Shota Miyazaki [verfasserIn] Yasushi Muraki [verfasserIn] Arisa Okamura [verfasserIn] Greg Olmschenk [verfasserIn] Clément Ranc [verfasserIn] Nicholas J. Rattenbury [verfasserIn] Yuki Satoh [verfasserIn] Takahiro Sumi [verfasserIn] Daisuke Suzuki [verfasserIn] Taiga Toda [verfasserIn] Paul . J. Tristram [verfasserIn] Aikaterini Vandorou [verfasserIn] Hibiki Yama [verfasserIn] (The MOA Collaboration) [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Übergeordnetes Werk:	In: The Astronomical Journal - IOP Publishing, 2022, 165(2022), 1, p 8
Übergeordnetes Werk:	volume:165 ; year:2022 ; number:1, p 8

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-3881/ac9d93

Katalog-ID:	DOAJ089162285

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520			\|a We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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.
653		0	\|a Astronomy
700	0		\|a Jennifer C. Yee \|e verfasserin \|4 aut
700	0		\|a Andrew Gould \|e verfasserin \|4 aut
700	0		\|a Kyu-Ha Hwang \|e verfasserin \|4 aut
700	0		\|a Hongjing Yang \|e verfasserin \|4 aut
700	0		\|a Ian A. Bond \|e verfasserin \|4 aut
700	0		\|a (Leading Authors) \|e verfasserin \|4 aut
700	0		\|a Michael D. Albrow \|e verfasserin \|4 aut
700	0		\|a Sun-Ju Chung \|e verfasserin \|4 aut
700	0		\|a Cheongho Han \|e verfasserin \|4 aut
700	0		\|a Youn Kil Jung \|e verfasserin \|4 aut
700	0		\|a Yoon-Hyun Ryu \|e verfasserin \|4 aut
700	0		\|a Yossi Shvartzvald \|e verfasserin \|4 aut
700	0		\|a Weicheng Zang \|e verfasserin \|4 aut
700	0		\|a Sang-Mok Cha \|e verfasserin \|4 aut
700	0		\|a Dong-Jin Kim \|e verfasserin \|4 aut
700	0		\|a Seung-Lee Kim \|e verfasserin \|4 aut
700	0		\|a Chung-Uk Lee \|e verfasserin \|4 aut
700	0		\|a Dong-Joo Lee \|e verfasserin \|4 aut
700	0		\|a Yongseok Lee \|e verfasserin \|4 aut
700	0		\|a Byeong-Gon Park \|e verfasserin \|4 aut
700	0		\|a Richard W. Pogge \|e verfasserin \|4 aut
700	0		\|a (The KMTNet Collaboration) \|e verfasserin \|4 aut
700	0		\|a Fumio Abe \|e verfasserin \|4 aut
700	0		\|a Richard Barry \|e verfasserin \|4 aut
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700	0		\|a Aparna Bhattacharya \|e verfasserin \|4 aut
700	0		\|a Hirosane Fujii \|e verfasserin \|4 aut
700	0		\|a Akihiko Fukui \|e verfasserin \|4 aut
700	0		\|a Yuki Hirao \|e verfasserin \|4 aut
700	0		\|a Stela Ishitani Silva \|e verfasserin \|4 aut
700	0		\|a Yoshitaka Itow \|e verfasserin \|4 aut
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700	0		\|a Naoki Koshimoto \|e verfasserin \|4 aut
700	0		\|a Yutaka Matsubara \|e verfasserin \|4 aut
700	0		\|a Sho Matsumoto \|e verfasserin \|4 aut
700	0		\|a Shota Miyazaki \|e verfasserin \|4 aut
700	0		\|a Yasushi Muraki \|e verfasserin \|4 aut
700	0		\|a Arisa Okamura \|e verfasserin \|4 aut
700	0		\|a Greg Olmschenk \|e verfasserin \|4 aut
700	0		\|a Clément Ranc \|e verfasserin \|4 aut
700	0		\|a Nicholas J. Rattenbury \|e verfasserin \|4 aut
700	0		\|a Yuki Satoh \|e verfasserin \|4 aut
700	0		\|a Takahiro Sumi \|e verfasserin \|4 aut
700	0		\|a Daisuke Suzuki \|e verfasserin \|4 aut
700	0		\|a Taiga Toda \|e verfasserin \|4 aut
700	0		\|a Paul . J. Tristram \|e verfasserin \|4 aut
700	0		\|a Aikaterini Vandorou \|e verfasserin \|4 aut
700	0		\|a Hibiki Yama \|e verfasserin \|4 aut
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allfields	10.3847/1538-3881/ac9d93 doi (DE-627)DOAJ089162285 (DE-599)DOAJ91e6e3a12f91422c964acbfc3081faca DE-627 ger DE-627 rakwb eng QB1-991 In-Gu Shin verfasserin aut Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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. Astronomy Jennifer C. Yee verfasserin aut Andrew Gould verfasserin aut Kyu-Ha Hwang verfasserin aut Hongjing Yang verfasserin aut Ian A. Bond verfasserin aut (Leading Authors) verfasserin aut Michael D. Albrow verfasserin aut Sun-Ju Chung verfasserin aut Cheongho Han verfasserin aut Youn Kil Jung verfasserin aut Yoon-Hyun Ryu verfasserin aut Yossi Shvartzvald verfasserin aut Weicheng Zang verfasserin aut Sang-Mok Cha verfasserin aut Dong-Jin Kim verfasserin aut Seung-Lee Kim verfasserin aut Chung-Uk Lee verfasserin aut Dong-Joo Lee verfasserin aut Yongseok Lee verfasserin aut Byeong-Gon Park verfasserin aut Richard W. Pogge verfasserin aut (The KMTNet Collaboration) verfasserin aut Fumio Abe verfasserin aut Richard Barry verfasserin aut David P. Bennett verfasserin aut Aparna Bhattacharya verfasserin aut Hirosane Fujii verfasserin aut Akihiko Fukui verfasserin aut Yuki Hirao verfasserin aut Stela Ishitani Silva verfasserin aut Yoshitaka Itow verfasserin aut Rintaro Kirikawa verfasserin aut Iona Kondo verfasserin aut Naoki Koshimoto verfasserin aut Yutaka Matsubara verfasserin aut Sho Matsumoto verfasserin aut Shota Miyazaki verfasserin aut Yasushi Muraki verfasserin aut Arisa Okamura verfasserin aut Greg Olmschenk verfasserin aut Clément Ranc verfasserin aut Nicholas J. Rattenbury verfasserin aut Yuki Satoh verfasserin aut Takahiro Sumi verfasserin aut Daisuke Suzuki verfasserin aut Taiga Toda verfasserin aut Paul . J. Tristram verfasserin aut Aikaterini Vandorou verfasserin aut Hibiki Yama verfasserin aut (The MOA Collaboration) verfasserin aut In The Astronomical Journal IOP Publishing, 2022 165(2022), 1, p 8 (DE-627)312175647 (DE-600)2003104-X 15383881 nnns volume:165 year:2022 number:1, p 8 https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca kostenfrei https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/toc/1538-3881 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2110 GBV_ILN_2129 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 165 2022 1, p 8
spelling	10.3847/1538-3881/ac9d93 doi (DE-627)DOAJ089162285 (DE-599)DOAJ91e6e3a12f91422c964acbfc3081faca DE-627 ger DE-627 rakwb eng QB1-991 In-Gu Shin verfasserin aut Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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. Astronomy Jennifer C. Yee verfasserin aut Andrew Gould verfasserin aut Kyu-Ha Hwang verfasserin aut Hongjing Yang verfasserin aut Ian A. Bond verfasserin aut (Leading Authors) verfasserin aut Michael D. Albrow verfasserin aut Sun-Ju Chung verfasserin aut Cheongho Han verfasserin aut Youn Kil Jung verfasserin aut Yoon-Hyun Ryu verfasserin aut Yossi Shvartzvald verfasserin aut Weicheng Zang verfasserin aut Sang-Mok Cha verfasserin aut Dong-Jin Kim verfasserin aut Seung-Lee Kim verfasserin aut Chung-Uk Lee verfasserin aut Dong-Joo Lee verfasserin aut Yongseok Lee verfasserin aut Byeong-Gon Park verfasserin aut Richard W. Pogge verfasserin aut (The KMTNet Collaboration) verfasserin aut Fumio Abe verfasserin aut Richard Barry verfasserin aut David P. Bennett verfasserin aut Aparna Bhattacharya verfasserin aut Hirosane Fujii verfasserin aut Akihiko Fukui verfasserin aut Yuki Hirao verfasserin aut Stela Ishitani Silva verfasserin aut Yoshitaka Itow verfasserin aut Rintaro Kirikawa verfasserin aut Iona Kondo verfasserin aut Naoki Koshimoto verfasserin aut Yutaka Matsubara verfasserin aut Sho Matsumoto verfasserin aut Shota Miyazaki verfasserin aut Yasushi Muraki verfasserin aut Arisa Okamura verfasserin aut Greg Olmschenk verfasserin aut Clément Ranc verfasserin aut Nicholas J. Rattenbury verfasserin aut Yuki Satoh verfasserin aut Takahiro Sumi verfasserin aut Daisuke Suzuki verfasserin aut Taiga Toda verfasserin aut Paul . J. Tristram verfasserin aut Aikaterini Vandorou verfasserin aut Hibiki Yama verfasserin aut (The MOA Collaboration) verfasserin aut In The Astronomical Journal IOP Publishing, 2022 165(2022), 1, p 8 (DE-627)312175647 (DE-600)2003104-X 15383881 nnns volume:165 year:2022 number:1, p 8 https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca kostenfrei https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/toc/1538-3881 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2110 GBV_ILN_2129 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 165 2022 1, p 8
allfields_unstemmed	10.3847/1538-3881/ac9d93 doi (DE-627)DOAJ089162285 (DE-599)DOAJ91e6e3a12f91422c964acbfc3081faca DE-627 ger DE-627 rakwb eng QB1-991 In-Gu Shin verfasserin aut Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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. Astronomy Jennifer C. Yee verfasserin aut Andrew Gould verfasserin aut Kyu-Ha Hwang verfasserin aut Hongjing Yang verfasserin aut Ian A. Bond verfasserin aut (Leading Authors) verfasserin aut Michael D. Albrow verfasserin aut Sun-Ju Chung verfasserin aut Cheongho Han verfasserin aut Youn Kil Jung verfasserin aut Yoon-Hyun Ryu verfasserin aut Yossi Shvartzvald verfasserin aut Weicheng Zang verfasserin aut Sang-Mok Cha verfasserin aut Dong-Jin Kim verfasserin aut Seung-Lee Kim verfasserin aut Chung-Uk Lee verfasserin aut Dong-Joo Lee verfasserin aut Yongseok Lee verfasserin aut Byeong-Gon Park verfasserin aut Richard W. Pogge verfasserin aut (The KMTNet Collaboration) verfasserin aut Fumio Abe verfasserin aut Richard Barry verfasserin aut David P. Bennett verfasserin aut Aparna Bhattacharya verfasserin aut Hirosane Fujii verfasserin aut Akihiko Fukui verfasserin aut Yuki Hirao verfasserin aut Stela Ishitani Silva verfasserin aut Yoshitaka Itow verfasserin aut Rintaro Kirikawa verfasserin aut Iona Kondo verfasserin aut Naoki Koshimoto verfasserin aut Yutaka Matsubara verfasserin aut Sho Matsumoto verfasserin aut Shota Miyazaki verfasserin aut Yasushi Muraki verfasserin aut Arisa Okamura verfasserin aut Greg Olmschenk verfasserin aut Clément Ranc verfasserin aut Nicholas J. Rattenbury verfasserin aut Yuki Satoh verfasserin aut Takahiro Sumi verfasserin aut Daisuke Suzuki verfasserin aut Taiga Toda verfasserin aut Paul . J. Tristram verfasserin aut Aikaterini Vandorou verfasserin aut Hibiki Yama verfasserin aut (The MOA Collaboration) verfasserin aut In The Astronomical Journal IOP Publishing, 2022 165(2022), 1, p 8 (DE-627)312175647 (DE-600)2003104-X 15383881 nnns volume:165 year:2022 number:1, p 8 https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca kostenfrei https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/toc/1538-3881 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2110 GBV_ILN_2129 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 165 2022 1, p 8
allfieldsGer	10.3847/1538-3881/ac9d93 doi (DE-627)DOAJ089162285 (DE-599)DOAJ91e6e3a12f91422c964acbfc3081faca DE-627 ger DE-627 rakwb eng QB1-991 In-Gu Shin verfasserin aut Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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. Astronomy Jennifer C. Yee verfasserin aut Andrew Gould verfasserin aut Kyu-Ha Hwang verfasserin aut Hongjing Yang verfasserin aut Ian A. Bond verfasserin aut (Leading Authors) verfasserin aut Michael D. Albrow verfasserin aut Sun-Ju Chung verfasserin aut Cheongho Han verfasserin aut Youn Kil Jung verfasserin aut Yoon-Hyun Ryu verfasserin aut Yossi Shvartzvald verfasserin aut Weicheng Zang verfasserin aut Sang-Mok Cha verfasserin aut Dong-Jin Kim verfasserin aut Seung-Lee Kim verfasserin aut Chung-Uk Lee verfasserin aut Dong-Joo Lee verfasserin aut Yongseok Lee verfasserin aut Byeong-Gon Park verfasserin aut Richard W. Pogge verfasserin aut (The KMTNet Collaboration) verfasserin aut Fumio Abe verfasserin aut Richard Barry verfasserin aut David P. Bennett verfasserin aut Aparna Bhattacharya verfasserin aut Hirosane Fujii verfasserin aut Akihiko Fukui verfasserin aut Yuki Hirao verfasserin aut Stela Ishitani Silva verfasserin aut Yoshitaka Itow verfasserin aut Rintaro Kirikawa verfasserin aut Iona Kondo verfasserin aut Naoki Koshimoto verfasserin aut Yutaka Matsubara verfasserin aut Sho Matsumoto verfasserin aut Shota Miyazaki verfasserin aut Yasushi Muraki verfasserin aut Arisa Okamura verfasserin aut Greg Olmschenk verfasserin aut Clément Ranc verfasserin aut Nicholas J. Rattenbury verfasserin aut Yuki Satoh verfasserin aut Takahiro Sumi verfasserin aut Daisuke Suzuki verfasserin aut Taiga Toda verfasserin aut Paul . J. Tristram verfasserin aut Aikaterini Vandorou verfasserin aut Hibiki Yama verfasserin aut (The MOA Collaboration) verfasserin aut In The Astronomical Journal IOP Publishing, 2022 165(2022), 1, p 8 (DE-627)312175647 (DE-600)2003104-X 15383881 nnns volume:165 year:2022 number:1, p 8 https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca kostenfrei https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/toc/1538-3881 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2110 GBV_ILN_2129 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 165 2022 1, p 8
allfieldsSound	10.3847/1538-3881/ac9d93 doi (DE-627)DOAJ089162285 (DE-599)DOAJ91e6e3a12f91422c964acbfc3081faca DE-627 ger DE-627 rakwb eng QB1-991 In-Gu Shin verfasserin aut Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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. Astronomy Jennifer C. Yee verfasserin aut Andrew Gould verfasserin aut Kyu-Ha Hwang verfasserin aut Hongjing Yang verfasserin aut Ian A. Bond verfasserin aut (Leading Authors) verfasserin aut Michael D. Albrow verfasserin aut Sun-Ju Chung verfasserin aut Cheongho Han verfasserin aut Youn Kil Jung verfasserin aut Yoon-Hyun Ryu verfasserin aut Yossi Shvartzvald verfasserin aut Weicheng Zang verfasserin aut Sang-Mok Cha verfasserin aut Dong-Jin Kim verfasserin aut Seung-Lee Kim verfasserin aut Chung-Uk Lee verfasserin aut Dong-Joo Lee verfasserin aut Yongseok Lee verfasserin aut Byeong-Gon Park verfasserin aut Richard W. Pogge verfasserin aut (The KMTNet Collaboration) verfasserin aut Fumio Abe verfasserin aut Richard Barry verfasserin aut David P. Bennett verfasserin aut Aparna Bhattacharya verfasserin aut Hirosane Fujii verfasserin aut Akihiko Fukui verfasserin aut Yuki Hirao verfasserin aut Stela Ishitani Silva verfasserin aut Yoshitaka Itow verfasserin aut Rintaro Kirikawa verfasserin aut Iona Kondo verfasserin aut Naoki Koshimoto verfasserin aut Yutaka Matsubara verfasserin aut Sho Matsumoto verfasserin aut Shota Miyazaki verfasserin aut Yasushi Muraki verfasserin aut Arisa Okamura verfasserin aut Greg Olmschenk verfasserin aut Clément Ranc verfasserin aut Nicholas J. Rattenbury verfasserin aut Yuki Satoh verfasserin aut Takahiro Sumi verfasserin aut Daisuke Suzuki verfasserin aut Taiga Toda verfasserin aut Paul . J. Tristram verfasserin aut Aikaterini Vandorou verfasserin aut Hibiki Yama verfasserin aut (The MOA Collaboration) verfasserin aut In The Astronomical Journal IOP Publishing, 2022 165(2022), 1, p 8 (DE-627)312175647 (DE-600)2003104-X 15383881 nnns volume:165 year:2022 number:1, p 8 https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca kostenfrei https://doi.org/10.3847/1538-3881/ac9d93 kostenfrei https://doaj.org/toc/1538-3881 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2110 GBV_ILN_2129 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 165 2022 1, p 8
language	English
source	In The Astronomical Journal 165(2022), 1, p 8 volume:165 year:2022 number:1, p 8
sourceStr	In The Astronomical Journal 165(2022), 1, p 8 volume:165 year:2022 number:1, p 8
format_phy_str_mv	Article
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topic_facet	Astronomy
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container_title	The Astronomical Journal
authorswithroles_txt_mv	In-Gu Shin @@aut@@ Jennifer C. Yee @@aut@@ Andrew Gould @@aut@@ Kyu-Ha Hwang @@aut@@ Hongjing Yang @@aut@@ Ian A. Bond @@aut@@ (Leading Authors) @@aut@@ Michael D. Albrow @@aut@@ Sun-Ju Chung @@aut@@ Cheongho Han @@aut@@ Youn Kil Jung @@aut@@ Yoon-Hyun Ryu @@aut@@ Yossi Shvartzvald @@aut@@ Weicheng Zang @@aut@@ Sang-Mok Cha @@aut@@ Dong-Jin Kim @@aut@@ Seung-Lee Kim @@aut@@ Chung-Uk Lee @@aut@@ Dong-Joo Lee @@aut@@ Yongseok Lee @@aut@@ Byeong-Gon Park @@aut@@ Richard W. Pogge @@aut@@ (The KMTNet Collaboration) @@aut@@ Fumio Abe @@aut@@ Richard Barry @@aut@@ David P. Bennett @@aut@@ Aparna Bhattacharya @@aut@@ Hirosane Fujii @@aut@@ Akihiko Fukui @@aut@@ Yuki Hirao @@aut@@ Stela Ishitani Silva @@aut@@ Yoshitaka Itow @@aut@@ Rintaro Kirikawa @@aut@@ Iona Kondo @@aut@@ Naoki Koshimoto @@aut@@ Yutaka Matsubara @@aut@@ Sho Matsumoto @@aut@@ Shota Miyazaki @@aut@@ Yasushi Muraki @@aut@@ Arisa Okamura @@aut@@ Greg Olmschenk @@aut@@ Clément Ranc @@aut@@ Nicholas J. Rattenbury @@aut@@ Yuki Satoh @@aut@@ Takahiro Sumi @@aut@@ Daisuke Suzuki @@aut@@ Taiga Toda @@aut@@ Paul . J. Tristram @@aut@@ Aikaterini Vandorou @@aut@@ Hibiki Yama @@aut@@ (The MOA Collaboration) @@aut@@
publishDateDaySort_date	2022-01-01T00:00:00Z
hierarchy_top_id	312175647
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language_de	englisch
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III. Analysis of Three Giant Planets</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present the analysis of three more planets from the KMTNet 2021 microlensing season. 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callnumber-first	Q - Science
author	In-Gu Shin
spellingShingle	In-Gu Shin misc QB1-991 misc Astronomy Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
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topic_title	QB1-991 Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
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title	Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
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title_full	Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
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author_browse	In-Gu Shin Jennifer C. Yee Andrew Gould Kyu-Ha Hwang Hongjing Yang Ian A. Bond (Leading Authors) Michael D. Albrow Sun-Ju Chung Cheongho Han Youn Kil Jung Yoon-Hyun Ryu Yossi Shvartzvald Weicheng Zang Sang-Mok Cha Dong-Jin Kim Seung-Lee Kim Chung-Uk Lee Dong-Joo Lee Yongseok Lee Byeong-Gon Park Richard W. Pogge (The KMTNet Collaboration) Fumio Abe Richard Barry David P. Bennett Aparna Bhattacharya Hirosane Fujii Akihiko Fukui Yuki Hirao Stela Ishitani Silva Yoshitaka Itow Rintaro Kirikawa Iona Kondo Naoki Koshimoto Yutaka Matsubara Sho Matsumoto Shota Miyazaki Yasushi Muraki Arisa Okamura Greg Olmschenk Clément Ranc Nicholas J. Rattenbury Yuki Satoh Takahiro Sumi Daisuke Suzuki Taiga Toda Paul . J. Tristram Aikaterini Vandorou Hibiki Yama (The MOA Collaboration)
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author-letter	In-Gu Shin
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title_sort	mass production of 2021 kmtnet microlensing planets. iii. analysis of three giant planets
callnumber	QB1-991
title_auth	Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
abstract	We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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.
abstractGer	We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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.
abstract_unstemmed	We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ∼6 M _Jup planet orbiting an early M dwarf or a K dwarf, KMT-2021-BLG-0192Lb is a ∼2 M _Nep planet orbiting an M dwarf, and KMT-2021-BLG-2294Lb is a ∼1.25 M _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.
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container_issue	1, p 8
title_short	Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets
url	https://doi.org/10.3847/1538-3881/ac9d93 https://doaj.org/article/91e6e3a12f91422c964acbfc3081faca https://doaj.org/toc/1538-3881
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author2	Jennifer C. Yee Andrew Gould Kyu-Ha Hwang Hongjing Yang Ian A. Bond (Leading Authors) Michael D. Albrow Sun-Ju Chung Cheongho Han Youn Kil Jung Yoon-Hyun Ryu Yossi Shvartzvald Weicheng Zang Sang-Mok Cha Dong-Jin Kim Seung-Lee Kim Chung-Uk Lee Dong-Joo Lee Yongseok Lee Byeong-Gon Park Richard W. Pogge (The KMTNet Collaboration) Fumio Abe Richard Barry David P. Bennett Aparna Bhattacharya Hirosane Fujii Akihiko Fukui Yuki Hirao Stela Ishitani Silva Yoshitaka Itow Rintaro Kirikawa Iona Kondo Naoki Koshimoto Yutaka Matsubara Sho Matsumoto Shota Miyazaki Yasushi Muraki Arisa Okamura Greg Olmschenk Clément Ranc Nicholas J. Rattenbury Yuki Satoh Takahiro Sumi Daisuke Suzuki Taiga Toda Paul . J. Tristram Aikaterini Vandorou Hibiki Yama (The MOA Collaboration)
author2Str	Jennifer C. Yee Andrew Gould Kyu-Ha Hwang Hongjing Yang Ian A. Bond (Leading Authors) Michael D. Albrow Sun-Ju Chung Cheongho Han Youn Kil Jung Yoon-Hyun Ryu Yossi Shvartzvald Weicheng Zang Sang-Mok Cha Dong-Jin Kim Seung-Lee Kim Chung-Uk Lee Dong-Joo Lee Yongseok Lee Byeong-Gon Park Richard W. Pogge (The KMTNet Collaboration) Fumio Abe Richard Barry David P. Bennett Aparna Bhattacharya Hirosane Fujii Akihiko Fukui Yuki Hirao Stela Ishitani Silva Yoshitaka Itow Rintaro Kirikawa Iona Kondo Naoki Koshimoto Yutaka Matsubara Sho Matsumoto Shota Miyazaki Yasushi Muraki Arisa Okamura Greg Olmschenk Clément Ranc Nicholas J. Rattenbury Yuki Satoh Takahiro Sumi Daisuke Suzuki Taiga Toda Paul . J. Tristram Aikaterini Vandorou Hibiki Yama (The MOA Collaboration)
ppnlink	312175647
callnumber-subject	QB - Astronomy
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doi_str	10.3847/1538-3881/ac9d93
callnumber-a	QB1-991
up_date	2024-07-03T21:37:14.683Z
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