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List of exoplanets detected by microlensing: Difference between revisions

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This is a '''list of ]s detected by ]'''. The phenomenon results in the background star's light being warped around a foreground object, causing a distorted image. If the foreground object is a star with an orbiting ], we would observe an abnormally ] image. By comparing the luminosity and light distortion of the background star to theoretical models, we can estimate the planet's mass and the distance from its star. This is a '''list of ]s detected by ]'''. The phenomenon results in the background star's light being warped around a foreground object, causing a distorted image. If the foreground object is a star with an orbiting ], we would observe an abnormally ] image. By comparing the luminosity and light distortion of the background star to theoretical models, we can estimate the planet's mass and the distance from its star.


The least massive planet detected by microlensing is KMT-2020-BLG-0414Lb, which has about the same mass as ]. The widest separation between a planet and a star is OGLE-2008-BLG-092Lb, which is ~15 ]; the shortest separation is MOA-2015-BLG-337Lb, which is 0.24 AU. There are 7 known ] detected by microlensing, all of which have two planets.<ref>{{cite web |title=Planetary Systems Composite Data |url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PSCompPars |website=] |accessdate=19 February 2023}}</ref> The least massive planet detected by microlensing is ]<nowiki/>b, which has a mass about 1.9 times the mass of ], or OGLE-2013-BLG-0341LBb, which has a mass about 2 times the mass of earth.<ref name="Zhang2024">{{cite journal |last1=Zhang |first1=Keming |last2=Zang |first2=Weicheng |last3=El-Badry |first3=Kareem |last4=Lu |first4=Jessica R. |display-authors=etal |date=September 2024 |title=An Earth-Mass Planet and a Brown Dwarf in Orbit Around a White Dwarf |journal=Accepted for publication |volume= |issue= |pages= |arxiv=2409.02157 |doi=}}</ref><ref name="Gould_2014" /> The widest separation between a planet and a star is OGLE-2008-BLG-092Lb, which is ~18 ]; the shortest separation is MOA-2015-BLG-337Lb, which is 0.24 AU. There are 7 known ] detected by microlensing, all of which have two planets.<ref>{{cite web |title=Planetary Systems Composite Data |url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PSCompPars |website=] |accessdate=19 February 2023}}</ref>


== List == == List ==
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| OGLE-2012-BLG-0950Lb || 0.079 || 2.2 || || || || 2016<ref name="Koshimoto2016"/> | OGLE-2012-BLG-0950Lb || 0.079 || 2.2 || || || || 2016<ref name="Koshimoto2016"/>
|- bgcolor="#7fffb0" |- bgcolor="#7fffb0"
| ] || 0.25 || 2.59 || 2557 || || || 2016<ref name="Bennett2016"/> | ] || 0.25 || 2.59 || 2557 || || || 2016<ref name="Bennett2016"/>
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| OGLE-2014-BLG-0676Lb || 3.68 || 4.53 || || || || 2016<ref name="Rattenbury2017"/> | OGLE-2014-BLG-0676Lb || 3.68 || 4.53 || || || || 2016<ref name="Rattenbury2017"/>
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|2018<ref>{{Cite journal |last1=Nucita |first1=A. A. |last2=Licchelli |first2=D. |last3=De Paolis |first3=F. |last4=Ingrosso |first4=G. |last5=Strafella |first5=F. |last6=Katysheva |first6=N. |last7=Shugarov |first7=S. |date=2018-05-01 |title=Discovery of a bright microlensing event with planetary features towards the Taurus region: a super-Earth planet |url=https://ui.adsabs.harvard.edu/abs/2018MNRAS.476.2962N |journal=Monthly Notices of the Royal Astronomical Society |volume=476 |issue=3 |pages=2962–2967 |doi=10.1093/mnras/sty448 |arxiv=1802.06659 |bibcode=2018MNRAS.476.2962N |issn=0035-8711}}</ref><ref>{{Cite journal |last1=Zang |first1=Weicheng |last2=Dong |first2=Subo |last3=Gould |first3=Andrew |last4=Calchi Novati |first4=Sebastiano |last5=Chen |first5=Ping |last6=Yang |first6=Hongjing |last7=Li |first7=Shun-Sheng |last8=Mao |first8=Shude |last9=Alton |first9=K. B. |last10=Brimacombe |first10=J. |last11=Carey |first11=Sean |last12=Christie |first12=G. W. |last13=Delplancke-Ströbele |first13=F. |last14=Feliz |first14=Dax L. |last15=Gaudi |first15=B. Scott |date=2020-07-01 |title=Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event |journal=The Astrophysical Journal |volume=897 |issue=2 |pages=180 |doi=10.3847/1538-4357/ab9749 |doi-access=free |arxiv=1912.00038 |bibcode=2020ApJ...897..180Z |issn=0004-637X}}</ref><ref>{{Cite journal |last1=Fukui |first1=A. |last2=Suzuki |first2=D. |last3=Koshimoto |first3=N. |last4=Bachelet |first4=E. |last5=Vanmunster |first5=T. |last6=Storey |first6=D. |last7=Maehara |first7=H. |last8=Yanagisawa |first8=K. |last9=Yamada |first9=T. |last10=Yonehara |first10=A. |last11=Hirano |first11=T. |last12=Bennett |first12=D. P. |last13=Bozza |first13=V. |last14=Mawet |first14=D. |last15=Penny |first15=M. T. |date=2019-11-01 |title=Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star |journal=The Astronomical Journal |volume=158 |issue=5 |pages=206 |doi=10.3847/1538-3881/ab487f |doi-access=free |arxiv=1909.11802 |bibcode=2019AJ....158..206F |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Nucita |first1=A. A. |last2=Licchelli |first2=D. |last3=De Paolis |first3=F. |last4=Ingrosso |first4=G. |last5=Strafella |first5=F. |last6=Katysheva |first6=N. |last7=Shugarov |first7=S. |date=2018-05-01 |title=Discovery of a bright microlensing event with planetary features towards the Taurus region: a super-Earth planet |journal=Monthly Notices of the Royal Astronomical Society |volume=476 |issue=3 |pages=2962–2967 |doi=10.1093/mnras/sty448 |doi-access=free |arxiv=1802.06659 |bibcode=2018MNRAS.476.2962N |issn=0035-8711}}</ref><ref>{{Cite journal |last1=Zang |first1=Weicheng |last2=Dong |first2=Subo |last3=Gould |first3=Andrew |last4=Calchi Novati |first4=Sebastiano |last5=Chen |first5=Ping |last6=Yang |first6=Hongjing |last7=Li |first7=Shun-Sheng |last8=Mao |first8=Shude |last9=Alton |first9=K. B. |last10=Brimacombe |first10=J. |last11=Carey |first11=Sean |last12=Christie |first12=G. W. |last13=Delplancke-Ströbele |first13=F. |last14=Feliz |first14=Dax L. |last15=Gaudi |first15=B. Scott |date=2020-07-01 |title=Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event |journal=The Astrophysical Journal |volume=897 |issue=2 |pages=180 |doi=10.3847/1538-4357/ab9749 |doi-access=free |arxiv=1912.00038 |bibcode=2020ApJ...897..180Z |issn=0004-637X}}</ref><ref>{{Cite journal |last1=Fukui |first1=A. |last2=Suzuki |first2=D. |last3=Koshimoto |first3=N. |last4=Bachelet |first4=E. |last5=Vanmunster |first5=T. |last6=Storey |first6=D. |last7=Maehara |first7=H. |last8=Yanagisawa |first8=K. |last9=Yamada |first9=T. |last10=Yonehara |first10=A. |last11=Hirano |first11=T. |last12=Bennett |first12=D. P. |last13=Bozza |first13=V. |last14=Mawet |first14=D. |last15=Penny |first15=M. T. |date=2019-11-01 |title=Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star |journal=The Astronomical Journal |volume=158 |issue=5 |pages=206 |doi=10.3847/1538-3881/ab487f |doi-access=free |arxiv=1909.11802 |bibcode=2019AJ....158..206F |issn=0004-6256}}</ref>
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|] |]
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|2018<ref>{{Cite journal |last=Hirao |first=Y. |last2=Udalski |first2=A. |last3=Sumi |first3=T. |last4=Bennett |first4=D. P. |last5=Koshimoto |first5=N. |last6=Bond |first6=I. A. |last7=Rattenbury |first7=N. J. |last8=Suzuki |first8=D. |last9=and |last10=Abe |first10=F. |last11=Asakura |first11=Y. |last12=Barry |first12=R. K. |last13=Bhattacharya |first13=A. |last14=Donachie |first14=M. |last15=Evans |first15=P. |date=2017-07-01 |title=OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf |url=https://ui.adsabs.harvard.edu/abs/2017AJ....154....1H |journal=The Astronomical Journal |volume=154 |pages=1 |doi=10.3847/1538-3881/aa73da |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Hirao |first1=Y. |last2=Udalski |first2=A. |last3=Sumi |first3=T. |last4=Bennett |first4=D. P. |last5=Koshimoto |first5=N. |last6=Bond |first6=I. A. |last7=Rattenbury |first7=N. J. |last8=Suzuki |first8=D. |last9=and |last10=Abe |first10=F. |last11=Asakura |first11=Y. |last12=Barry |first12=R. K. |last13=Bhattacharya |first13=A. |last14=Donachie |first14=M. |last15=Evans |first15=P. |date=2017-07-01 |title=OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf |journal=The Astronomical Journal |volume=154 |issue=1 |pages=1 |doi=10.3847/1538-3881/aa73da |doi-access=free |arxiv=1703.07623 |bibcode=2017AJ....154....1H |issn=0004-6256}}</ref>
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|OGLE-2011-BLG-0173Lb |OGLE-2011-BLG-0173Lb
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|2018<ref>{{Cite journal |last=Poleski |first=Radosław |last2=Gaudi |first2=B. S. |last3=Udalski |first3=A. |last4=Szymański |first4=M. K. |last5=Soszyński |first5=I. |last6=Pietrukowicz |first6=P. |last7=Kozłowski |first7=S. |last8=Skowron |first8=J. |last9=Wyrzykowski |first9=Ł. |last10=Ulaczyk |first10=K. |date=2018-09-01 |title=An Ice Giant Exoplanet Interpretation of the Anomaly in Microlensing Event OGLE-2011-BLG-0173 |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..104P |journal=The Astronomical Journal |volume=156 |pages=104 |doi=10.3847/1538-3881/aad45e |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Poleski |first1=Radosław |last2=Gaudi |first2=B. S. |last3=Udalski |first3=A. |last4=Szymański |first4=M. K. |last5=Soszyński |first5=I. |last6=Pietrukowicz |first6=P. |last7=Kozłowski |first7=S. |last8=Skowron |first8=J. |last9=Wyrzykowski |first9=Ł. |last10=Ulaczyk |first10=K. |date=2018-09-01 |title=An Ice Giant Exoplanet Interpretation of the Anomaly in Microlensing Event OGLE-2011-BLG-0173 |journal=The Astronomical Journal |volume=156 |issue=3 |pages=104 |doi=10.3847/1538-3881/aad45e |doi-access=free |arxiv=1805.00049 |bibcode=2018AJ....156..104P |issn=0004-6256}}</ref>
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|MOA-2016-BLG-319Lb |MOA-2016-BLG-319Lb
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|2018<ref>{{Cite journal |last=Han |first=Cheongho |last2=Bond |first2=Ian A. |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2018-11-01 |title=MOA-2016-BLG-319Lb: Microlensing Planet Subject to Rare Minor-image Perturbation Degeneracy in Determining Planet Parameters |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..226H |journal=The Astronomical Journal |volume=156 |pages=226 |doi=10.3847/1538-3881/aae38e |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Bond |first2=Ian A. |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2018-11-01 |title=MOA-2016-BLG-319Lb: Microlensing Planet Subject to Rare Minor-image Perturbation Degeneracy in Determining Planet Parameters |journal=The Astronomical Journal |volume=156 |issue=5 |pages=226 |doi=10.3847/1538-3881/aae38e |doi-access=free |arxiv=1809.07898 |bibcode=2018AJ....156..226H |issn=0004-6256}}</ref>
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|MOA-2015-BLG-337Lb |MOA-2015-BLG-337Lb
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|2018<ref>{{Cite journal |last=Miyazaki |first=S. |last2=Sumi |first2=T. |last3=Bennett |first3=D. P. |last4=Gould |first4=A. |last5=Udalski |first5=A. |last6=Bond |first6=I. A. |last7=Koshimoto |first7=N. |last8=Nagakane |first8=M. |last9=Rattenbury |first9=N. |last10=Abe |first10=F. |last11=Bhattacharya |first11=A. |last12=Barry |first12=R. |last13=Donachie |first13=M. |last14=Fukui |first14=A. |last15=Hirao |first15=Y. |date=2018-09-01 |title=MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..136M |journal=The Astronomical Journal |volume=156 |pages=136 |doi=10.3847/1538-3881/aad5ee |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Miyazaki |first1=S. |last2=Sumi |first2=T. |last3=Bennett |first3=D. P. |last4=Gould |first4=A. |last5=Udalski |first5=A. |last6=Bond |first6=I. A. |last7=Koshimoto |first7=N. |last8=Nagakane |first8=M. |last9=Rattenbury |first9=N. |last10=Abe |first10=F. |last11=Bhattacharya |first11=A. |last12=Barry |first12=R. |last13=Donachie |first13=M. |last14=Fukui |first14=A. |last15=Hirao |first15=Y. |date=2018-09-01 |title=MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary |journal=The Astronomical Journal |volume=156 |issue=3 |pages=136 |doi=10.3847/1538-3881/aad5ee |doi-access=free |arxiv=1804.00830 |bibcode=2018AJ....156..136M |issn=0004-6256}}</ref>
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|MOA-2011-BLG-291Lb |MOA-2011-BLG-291Lb
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|2018<ref>{{Cite journal |last=Bennett |first=David P. |last2=Udalski |first2=Andrzej |last3=Bond |first3=Ian A. |last4=Suzuki |first4=Daisuke |last5=Ryu |first5=Yoon-Hyun |last6=Abe |first6=Fumio |last7=Barry |first7=Richard K. |last8=Bhattacharya |first8=Aparna |last9=Donachie |first9=Martin |last10=Fukui |first10=Akihiko |last11=Hirao |first11=Yuki |last12=Kawasaki |first12=Kohei |last13=Kondo |first13=Iona |last14=Koshimoto |first14=Naoki |last15=Li |first15=Man Cheung Alex |date=2018-09-01 |title=A Planetary Microlensing Event with an Unusually Red Source Star: MOA-2011-BLG-291 |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..113B |journal=The Astronomical Journal |volume=156 |pages=113 |doi=10.3847/1538-3881/aad59c |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Bennett |first1=David P. |last2=Udalski |first2=Andrzej |last3=Bond |first3=Ian A. |last4=Suzuki |first4=Daisuke |last5=Ryu |first5=Yoon-Hyun |last6=Abe |first6=Fumio |last7=Barry |first7=Richard K. |last8=Bhattacharya |first8=Aparna |last9=Donachie |first9=Martin |last10=Fukui |first10=Akihiko |last11=Hirao |first11=Yuki |last12=Kawasaki |first12=Kohei |last13=Kondo |first13=Iona |last14=Koshimoto |first14=Naoki |last15=Li |first15=Man Cheung Alex |date=2018-09-01 |title=A Planetary Microlensing Event with an Unusually Red Source Star: MOA-2011-BLG-291 |journal=The Astronomical Journal |volume=156 |issue=3 |pages=113 |doi=10.3847/1538-3881/aad59c |doi-access=free |arxiv=1806.06106 |bibcode=2018AJ....156..113B |issn=0004-6256}}</ref>
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|MOA-2010-BLG-117Lb |MOA-2010-BLG-117Lb
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|2018<ref>{{Cite journal |last=Bennett |first=D. P. |last2=Udalski |first2=A. |last3=Han |first3=C. |last4=Bond |first4=I. A. |last5=Beaulieu |first5=J. -P. |last6=Skowron |first6=J. |last7=Gaudi |first7=B. S. |last8=Koshimoto |first8=N. |last9=Abe |first9=F. |last10=Asakura |first10=Y. |last11=Barry |first11=R. K. |last12=Bhattacharya |first12=A. |last13=Donachie |first13=M. |last14=Evans |first14=P. |last15=Fukui |first15=A. |date=2018-03-01 |title=The First Planetary Microlensing Event with Two Microlensed Source Stars |url=https://ui.adsabs.harvard.edu/abs/2018AJ....155..141B |journal=The Astronomical Journal |volume=155 |pages=141 |doi=10.3847/1538-3881/aaadfa |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Bennett |first1=D. P. |last2=Udalski |first2=A. |last3=Han |first3=C. |last4=Bond |first4=I. A. |last5=Beaulieu |first5=J. -P. |last6=Skowron |first6=J. |last7=Gaudi |first7=B. S. |last8=Koshimoto |first8=N. |last9=Abe |first9=F. |last10=Asakura |first10=Y. |last11=Barry |first11=R. K. |last12=Bhattacharya |first12=A. |last13=Donachie |first13=M. |last14=Evans |first14=P. |last15=Fukui |first15=A. |date=2018-03-01 |title=The First Planetary Microlensing Event with Two Microlensed Source Stars |journal=The Astronomical Journal |volume=155 |issue=3 |pages=141 |doi=10.3847/1538-3881/aaadfa |doi-access=free |arxiv=1707.09667 |bibcode=2018AJ....155..141B |issn=0004-6256}}</ref>
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|KMT-2017-BLG-0165Lb |KMT-2017-BLG-0165Lb
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|2018<ref>{{Cite journal |last=Jung |first=Youn Kil |last2=Gould |first2=Andrew |last3=Zang |first3=Weicheng |last4=Hwang |first4=Kyu-Ha |last5=Ryu |first5=Yoon-Hyun |last6=Han |first6=Cheongho |last7=Yee |first7=Jennifer C. |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zhu |first12=Wei |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2019-02-01 |title=KMT-2017-BLG-0165Lb: A Super-Neptune-mass Planet Orbiting a Sun-like Host Star |url=https://ui.adsabs.harvard.edu/abs/2019AJ....157...72J |journal=The Astronomical Journal |volume=157 |pages=72 |doi=10.3847/1538-3881/aaf87f |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Jung |first1=Youn Kil |last2=Gould |first2=Andrew |last3=Zang |first3=Weicheng |last4=Hwang |first4=Kyu-Ha |last5=Ryu |first5=Yoon-Hyun |last6=Han |first6=Cheongho |last7=Yee |first7=Jennifer C. |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zhu |first12=Wei |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2019-02-01 |title=KMT-2017-BLG-0165Lb: A Super-Neptune-mass Planet Orbiting a Sun-like Host Star |journal=The Astronomical Journal |volume=157 |issue=2 |pages=72 |doi=10.3847/1538-3881/aaf87f |doi-access=free |arxiv=1809.01288 |bibcode=2019AJ....157...72J |issn=0004-6256}}</ref>
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|KMT-2016-BLG-2142Lb |KMT-2016-BLG-2142Lb
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|2018<ref name=":1">{{Cite journal |last=Jung |first=Youn Kil |last2=Hwang |first2=Kyu-Ha |last3=Ryu |first3=Yoon-Hyun |last4=Gould |first4=Andrew |last5=Han |first5=Cheongho |last6=Yee |first6=Jennifer C. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Zang |first11=Weicheng |last12=Cha |first12=Sang-Mok |last13=Kim |first13=Dong-Jin |last14=Kim |first14=Hyoun-Woo |last15=Kim |first15=Seung-Lee |date=2018-11-01 |title=KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-low-mass Primaries |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..208J |journal=The Astronomical Journal |volume=156 |pages=208 |doi=10.3847/1538-3881/aae319 |issn=0004-6256}}</ref> |2018<ref name=":1">{{Cite journal |last1=Jung |first1=Youn Kil |last2=Hwang |first2=Kyu-Ha |last3=Ryu |first3=Yoon-Hyun |last4=Gould |first4=Andrew |last5=Han |first5=Cheongho |last6=Yee |first6=Jennifer C. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Zang |first11=Weicheng |last12=Cha |first12=Sang-Mok |last13=Kim |first13=Dong-Jin |last14=Kim |first14=Hyoun-Woo |last15=Kim |first15=Seung-Lee |date=2018-11-01 |title=KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-low-mass Primaries |journal=The Astronomical Journal |volume=156 |issue=5 |pages=208 |doi=10.3847/1538-3881/aae319 |doi-access=free |arxiv=1805.09983 |bibcode=2018AJ....156..208J |issn=0004-6256}}</ref>
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|KMT-2016-BLG-1820Lb |KMT-2016-BLG-1820Lb
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|2018<ref>{{Cite journal |last=Zang |first=Weicheng |last2=Hwang |first2=Kyu-Ha |last3=Kim |first3=Hyoun-Woo |last4=Gould |first4=Andrew |last5=Wang |first5=Tianshu |last6=Zhu |first6=Wei |last7=Mao |first7=Shude |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Han |first10=Cheongho |last11=Jung |first11=Youn Kil |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2018-11-01 |title=KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet |url=https://ui.adsabs.harvard.edu/abs/2018AJ....156..236Z |journal=The Astronomical Journal |volume=156 |pages=236 |doi=10.3847/1538-3881/aae537 |issn=0004-6256}}</ref> |2018<ref>{{Cite journal |last1=Zang |first1=Weicheng |last2=Hwang |first2=Kyu-Ha |last3=Kim |first3=Hyoun-Woo |last4=Gould |first4=Andrew |last5=Wang |first5=Tianshu |last6=Zhu |first6=Wei |last7=Mao |first7=Shude |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Han |first10=Cheongho |last11=Jung |first11=Youn Kil |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2018-11-01 |title=KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet |journal=The Astronomical Journal |volume=156 |issue=5 |pages=236 |doi=10.3847/1538-3881/aae537 |doi-access=free |arxiv=1810.10792 |bibcode=2018AJ....156..236Z |issn=0004-6256}}</ref>
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|KMT-2016-BLG-0212Lb |KMT-2016-BLG-0212Lb
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|2018<ref>{{Cite journal |last=Hwang |first=K. -H. |last2=Kim |first2=H. -W. |last3=Kim |first3=D. -J. |last4=Gould |first4=A. |last5=Albrow |first5=M. D. |last6=Chung |first6=S. -J. |last7=Han |first7=C. |last8=Jung |first8=Y. K. |last9=Ryu |first9=Y. -H. |last10=Shin |first10=I. -G. |last11=Shvartzvald |first11=Y. |last12=Yee |first12=J. C. |last13=Zang |first13=W. |last14=Zhu |first14=W. |last15=Cha |first15=S. -M. |date=2018-12-01 |title=KMT-2016-BLG-0212: First KMTNet-Only Discovery of a Substellar Companion |url=https://ui.adsabs.harvard.edu/abs/2018JKAS...51..197H |journal=Journal of Korean Astronomical Society |volume=51 |pages=197–206 |doi=10.5303/JKAS.2018.51.6.197 |issn=1225-4614}}</ref> |2018<ref>{{Cite journal |last1=Hwang |first1=K. -H. |last2=Kim |first2=H. -W. |last3=Kim |first3=D. -J. |last4=Gould |first4=A. |last5=Albrow |first5=M. D. |last6=Chung |first6=S. -J. |last7=Han |first7=C. |last8=Jung |first8=Y. K. |last9=Ryu |first9=Y. -H. |last10=Shin |first10=I. -G. |last11=Shvartzvald |first11=Y. |last12=Yee |first12=J. C. |last13=Zang |first13=W. |last14=Zhu |first14=W. |last15=Cha |first15=S. -M. |date=2018-12-01 |title=KMT-2016-BLG-0212: First KMTNet-Only Discovery of a Substellar Companion |url=https://ui.adsabs.harvard.edu/abs/2018JKAS...51..197H |journal=Journal of Korean Astronomical Society |volume=51 |issue=6 |pages=197–206 |doi=10.5303/JKAS.2018.51.6.197 |arxiv=1802.10246 |bibcode=2018JKAS...51..197H |issn=1225-4614}}</ref>
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|OGLE-2018-BLG-1011Lb |OGLE-2018-BLG-1011Lb
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|2019<ref name=":2">{{Cite journal |last=Han |first=Cheongho |last2=Bennett |first2=David P. |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=Shvartzvald |first6=Yossi |last7=Nikolaus |first7=Kay-Sebastian |last8=Hundertmark |first8=Markus |last9=Bozza |first9=Valerio |last10=Cassan |first10=Arnaud |last11=Hirao |first11=Yuki |last12=Bachelet |first12=Etienne |last13=Fouqué |first13=Pascal |last14=Authors |first14=Leading |last15=Albrow |first15=Michael D. |date=2019-09-01 |title=OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star |url=https://ui.adsabs.harvard.edu/abs/2019AJ....158..114H |journal=The Astronomical Journal |volume=158 |pages=114 |doi=10.3847/1538-3881/ab2f74 |issn=0004-6256}}</ref> |2019<ref name=":2">{{Cite journal |last1=Han |first1=Cheongho |last2=Bennett |first2=David P. |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=Shvartzvald |first6=Yossi |last7=Nikolaus |first7=Kay-Sebastian |last8=Hundertmark |first8=Markus |last9=Bozza |first9=Valerio |last10=Cassan |first10=Arnaud |last11=Hirao |first11=Yuki |last12=Bachelet |first12=Etienne |last13=Fouqué |first13=Pascal |last14=Authors |first14=Leading |last15=Albrow |first15=Michael D. |date=2019-09-01 |title=OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star |journal=The Astronomical Journal |volume=158 |issue=3 |pages=114 |doi=10.3847/1538-3881/ab2f74 |doi-access=free |arxiv=1907.01741 |bibcode=2019AJ....158..114H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-1011Lc |OGLE-2018-BLG-1011Lc
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|2019<ref>{{Cite journal |last=Han |first=Cheongho |last2=Yee |first2=Jennifer C. |last3=Udalski |first3=Andrzej |last4=Bond |first4=Ian A. |last5=Bozza |first5=Valerio |last6=Cassan |first6=Arnaud |last7=Hirao |first7=Yuki |last8=Dong |first8=Subo |last9=Kollmeier |first9=Juna A. |last10=Morrell |first10=Nidia |last11=Boutsia |first11=Konstantina |last12=authors |first12=Leading |last13=Albrow |first13=Michael D. |last14=Chung |first14=Sun-Ju |last15=Gould |first15=Andrew |date=2019-09-01 |title=Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb |url=https://ui.adsabs.harvard.edu/abs/2019AJ....158..102H |journal=The Astronomical Journal |volume=158 |pages=102 |doi=10.3847/1538-3881/ab2df4 |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Yee |first2=Jennifer C. |last3=Udalski |first3=Andrzej |last4=Bond |first4=Ian A. |last5=Bozza |first5=Valerio |last6=Cassan |first6=Arnaud |last7=Hirao |first7=Yuki |last8=Dong |first8=Subo |last9=Kollmeier |first9=Juna A. |last10=Morrell |first10=Nidia |last11=Boutsia |first11=Konstantina |last12=authors |first12=Leading |last13=Albrow |first13=Michael D. |last14=Chung |first14=Sun-Ju |last15=Gould |first15=Andrew |date=2019-09-01 |title=Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb |journal=The Astronomical Journal |volume=158 |issue=3 |pages=102 |doi=10.3847/1538-3881/ab2df4 |doi-access=free |arxiv=1905.00155 |bibcode=2019AJ....158..102H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0596Lb |OGLE-2018-BLG-0596Lb
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|2019<ref>{{Cite journal |last=Jung |first=Youn Kil |last2=Gould |first2=Andrew |last3=Udalski |first3=Andrzej |last4=Sumi |first4=Takahiro |last5=Yee |first5=Jennifer C. |last6=Shvartzvald |first6=Yossi |last7=Zang |first7=Weicheng |last8=and |last9=Han |first9=Cheongho |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Hwang |first12=Kyu-Ha |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Zhu |first15=Wei |date=2019-07-01 |title=Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M Dwarf |url=https://ui.adsabs.harvard.edu/abs/2019AJ....158...28J |journal=The Astronomical Journal |volume=158 |pages=28 |doi=10.3847/1538-3881/ab237f |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Jung |first1=Youn Kil |last2=Gould |first2=Andrew |last3=Udalski |first3=Andrzej |last4=Sumi |first4=Takahiro |last5=Yee |first5=Jennifer C. |last6=Shvartzvald |first6=Yossi |last7=Zang |first7=Weicheng |last8=and |last9=Han |first9=Cheongho |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Hwang |first12=Kyu-Ha |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Zhu |first15=Wei |date=2019-07-01 |title=Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M Dwarf |journal=The Astronomical Journal |volume=158 |issue=1 |pages=28 |doi=10.3847/1538-3881/ab237f |doi-access=free |arxiv=1905.05873 |bibcode=2019AJ....158...28J |issn=0004-6256}}</ref>
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|OGLE-2016-BLG-1067Lb |OGLE-2016-BLG-1067Lb
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|2019<ref>{{Cite journal |last=Calchi Novati |first=S. |last2=Suzuki |first2=D. |last3=Udalski |first3=A. |last4=Gould |first4=A. |last5=Shvartzvald |first5=Y. |last6=Bozza |first6=V. |last7=Bennett |first7=D. P. |last8=Beichman |first8=C. |last9=Bryden |first9=G. |last10=Carey |first10=S. |last11=Gaudi |first11=B. S. |last12=Henderson |first12=C. B. |last13=Yee |first13=J. C. |last14=Zhu |first14=W. |last15=Spitzer Team |date=2019-03-01 |title=Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk |url=https://ui.adsabs.harvard.edu/abs/2019AJ....157..121C |journal=The Astronomical Journal |volume=157 |pages=121 |doi=10.3847/1538-3881/ab0106 |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Calchi Novati |first1=S. |last2=Suzuki |first2=D. |last3=Udalski |first3=A. |last4=Gould |first4=A. |last5=Shvartzvald |first5=Y. |last6=Bozza |first6=V. |last7=Bennett |first7=D. P. |last8=Beichman |first8=C. |last9=Bryden |first9=G. |last10=Carey |first10=S. |last11=Gaudi |first11=B. S. |last12=Henderson |first12=C. B. |last13=Yee |first13=J. C. |last14=Zhu |first14=W. |last15=Spitzer Team |date=2019-03-01 |title=Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk |journal=The Astronomical Journal |volume=157 |issue=3 |pages=121 |doi=10.3847/1538-3881/ab0106 |doi-access=free |arxiv=1801.05806 |bibcode=2019AJ....157..121C |issn=0004-6256}}</ref>
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|OGLE-2015-BLG-1670Lb |OGLE-2015-BLG-1670Lb
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|2019<ref>{{Cite journal |last=Ranc |first=Clément |last2=Bennett |first2=David P. |last3=Hirao |first3=Yuki |last4=Udalski |first4=Andrzej |last5=Han |first5=Cheongho |last6=Bond |first6=Ian A. |last7=Yee |first7=Jennifer C. |last8=and |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Gould |first11=Andrew |last12=Hwang |first12=Kyu-Ha |last13=Jung |first13=Youn-Kil |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |date=2019-06-01 |title=OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field |url=https://ui.adsabs.harvard.edu/abs/2019AJ....157..232R |journal=The Astronomical Journal |volume=157 |pages=232 |doi=10.3847/1538-3881/ab141b |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Ranc |first1=Clément |last2=Bennett |first2=David P. |last3=Hirao |first3=Yuki |last4=Udalski |first4=Andrzej |last5=Han |first5=Cheongho |last6=Bond |first6=Ian A. |last7=Yee |first7=Jennifer C. |last8=and |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Gould |first11=Andrew |last12=Hwang |first12=Kyu-Ha |last13=Jung |first13=Youn-Kil |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |date=2019-06-01 |title=OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field |journal=The Astronomical Journal |volume=157 |issue=6 |pages=232 |doi=10.3847/1538-3881/ab141b |doi-access=free |arxiv=1810.00014 |bibcode=2019AJ....157..232R |issn=0004-6256}}</ref>
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|OGLE-2015-BLG-1649Lb |OGLE-2015-BLG-1649Lb
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|2019<ref>{{Cite journal |last=Nagakane |first=M. |last2=Lee |first2=Chien-Hsiu |last3=Koshimoto |first3=N. |last4=Suzuki |first4=D. |last5=Udalski |first5=A. |last6=Beaulieu |first6=J. P. |last7=Sumi |first7=T. |last8=Bennett |first8=D. P. |last9=Bond |first9=I. A. |last10=Rattenbury |first10=N. |last11=Bachelet |first11=E. |last12=Dominik |first12=M. |last13=Abe |first13=F. |last14=Barry |first14=R. K. |last15=Bhattacharya |first15=A. |date=2019-11-01 |title=OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf |url=https://ui.adsabs.harvard.edu/abs/2019AJ....158..212N |journal=The Astronomical Journal |volume=158 |pages=212 |doi=10.3847/1538-3881/ab4881 |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Nagakane |first1=M. |last2=Lee |first2=Chien-Hsiu |last3=Koshimoto |first3=N. |last4=Suzuki |first4=D. |last5=Udalski |first5=A. |last6=Beaulieu |first6=J. P. |last7=Sumi |first7=T. |last8=Bennett |first8=D. P. |last9=Bond |first9=I. A. |last10=Rattenbury |first10=N. |last11=Bachelet |first11=E. |last12=Dominik |first12=M. |last13=Abe |first13=F. |last14=Barry |first14=R. K. |last15=Bhattacharya |first15=A. |date=2019-11-01 |title=OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf |journal=The Astronomical Journal |volume=158 |issue=5 |pages=212 |doi=10.3847/1538-3881/ab4881 |doi-access=free |arxiv=1907.11536 |bibcode=2019AJ....158..212N |issn=0004-6256}}</ref>
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|OGLE-2013-BLG-0911Lb |OGLE-2013-BLG-0911Lb
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|2019<ref>{{Cite journal |last=Miyazaki |first=Shota |last2=Sumi |first2=Takahiro |last3=Bennett |first3=David P. |last4=Udalski |first4=Andrzej |last5=Shvartzvald |first5=Yossi |last6=Street |first6=Rachel |last7=Bozza |first7=Valerio |last8=Yee |first8=Jennifer C. |last9=Bond |first9=Ian A. |last10=Rattenbury |first10=Nicholas |last11=Koshimoto |first11=Naoki |last12=Suzuki |first12=Daisuke |last13=Fukui |first13=Akihiko |last14=Abe |first14=F. |last15=Bhattacharya |first15=A. |date=2020-02-01 |title=OGLE-2013-BLG-0911Lb: A Secondary on the Brown-dwarf Planet Boundary around an M Dwarf |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159...76M |journal=The Astronomical Journal |volume=159 |pages=76 |doi=10.3847/1538-3881/ab64de |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Miyazaki |first1=Shota |last2=Sumi |first2=Takahiro |last3=Bennett |first3=David P. |last4=Udalski |first4=Andrzej |last5=Shvartzvald |first5=Yossi |last6=Street |first6=Rachel |last7=Bozza |first7=Valerio |last8=Yee |first8=Jennifer C. |last9=Bond |first9=Ian A. |last10=Rattenbury |first10=Nicholas |last11=Koshimoto |first11=Naoki |last12=Suzuki |first12=Daisuke |last13=Fukui |first13=Akihiko |last14=Abe |first14=F. |last15=Bhattacharya |first15=A. |date=2020-02-01 |title=OGLE-2013-BLG-0911Lb: A Secondary on the Brown-dwarf Planet Boundary around an M Dwarf |journal=The Astronomical Journal |volume=159 |issue=2 |pages=76 |doi=10.3847/1538-3881/ab64de |doi-access=free |arxiv=1912.09613 |bibcode=2020AJ....159...76M |issn=0004-6256}}</ref>
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| MOA-bin-29Lb || 0.6 || 0.48 || || || || 2019<ref name="Kondo2019"/> | MOA-bin-29Lb || 0.6 || 0.48 || || || || 2019<ref name="Kondo2019"/>
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|2019<ref>{{Cite journal |last=Ryu |first=Yoon-Hyun |last2=Hwang |first2=Kyu-Ha |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Han |first6=Cheongho |last7=Jung |first7=Youn Kil |last8=Shin |first8=In-Gu |last9=Shvartzvald |first9=Yossi |last10=Yee |first10=Jennifer C. |last11=Zang |first11=Weicheng |last12=Cha |first12=Sang-Mok |last13=Kim |first13=Dong-Jin |last14=Kim |first14=Hyoun-Woo |last15=Kim |first15=Seung-Lee |date=2019-10-01 |title=KMT-2018-BLG-1990Lb: A Nearby Jovian Planet From A Low-cadence Microlensing Field |url=https://ui.adsabs.harvard.edu/abs/2019AJ....158..151R |journal=The Astronomical Journal |volume=158 |pages=151 |doi=10.3847/1538-3881/ab3a34 |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Hwang |first2=Kyu-Ha |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Han |first6=Cheongho |last7=Jung |first7=Youn Kil |last8=Shin |first8=In-Gu |last9=Shvartzvald |first9=Yossi |last10=Yee |first10=Jennifer C. |last11=Zang |first11=Weicheng |last12=Cha |first12=Sang-Mok |last13=Kim |first13=Dong-Jin |last14=Kim |first14=Hyoun-Woo |last15=Kim |first15=Seung-Lee |date=2019-10-01 |title=KMT-2018-BLG-1990Lb: A Nearby Jovian Planet From A Low-cadence Microlensing Field |journal=The Astronomical Journal |volume=158 |issue=4 |pages=151 |doi=10.3847/1538-3881/ab3a34 |doi-access=free |arxiv=1905.05509 |bibcode=2019AJ....158..151R |issn=0004-6256}}</ref>
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|KMT-2017-BLG-1146Lb |KMT-2017-BLG-1146Lb
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|2019<ref name=":3">{{Cite journal |last=Shin |first=I. -G. |last2=Ryu |first2=Y. -H. |last3=Yee |first3=J. C. |last4=Gould |first4=A. |last5=Albrow |first5=M. D. |last6=Chung |first6=S. -J. |last7=Han |first7=C. |last8=Hwang |first8=K. -H. |last9=Jung |first9=Y. K. |last10=Shvartzvald |first10=Y. |last11=Zang |first11=W. |last12=Lee |first12=C. -U. |last13=Cha |first13=S. -M. |last14=Kim |first14=D. -J. |last15=Kim |first15=H. -W. |date=2019-04-01 |title=Two Jupiter-mass Planets Discovered by the KMTNet Survey in 2017 |url=https://ui.adsabs.harvard.edu/abs/2019AJ....157..146S |journal=The Astronomical Journal |volume=157 |pages=146 |doi=10.3847/1538-3881/ab07c2 |issn=0004-6256}}</ref> |2019<ref name=":3">{{Cite journal |last1=Shin |first1=I. -G. |last2=Ryu |first2=Y. -H. |last3=Yee |first3=J. C. |last4=Gould |first4=A. |last5=Albrow |first5=M. D. |last6=Chung |first6=S. -J. |last7=Han |first7=C. |last8=Hwang |first8=K. -H. |last9=Jung |first9=Y. K. |last10=Shvartzvald |first10=Y. |last11=Zang |first11=W. |last12=Lee |first12=C. -U. |last13=Cha |first13=S. -M. |last14=Kim |first14=D. -J. |last15=Kim |first15=H. -W. |date=2019-04-01 |title=Two Jupiter-mass Planets Discovered by the KMTNet Survey in 2017 |journal=The Astronomical Journal |volume=157 |issue=4 |pages=146 |doi=10.3847/1538-3881/ab07c2 |doi-access=free |arxiv=1811.12505 |bibcode=2019AJ....157..146S |issn=0004-6256}}</ref>
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|KMT-2017-BLG-1038Lb |KMT-2017-BLG-1038Lb
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|2019<ref>{{Cite journal |last=Yang |first=Hongjing |last2=Zhang |first2=Xiangyu |last3=Hwang |first3=Kyu-Ha |last4=Zang |first4=Weicheng |last5=Gould |first5=Andrew |last6=Wang |first6=Tianshu |last7=Mao |first7=Shude |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Han |first10=Cheongho |last11=Jung |first11=Youn Kil |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2020-03-01 |title=KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159...98Y |journal=The Astronomical Journal |volume=159 |pages=98 |doi=10.3847/1538-3881/ab660e |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Yang |first1=Hongjing |last2=Zhang |first2=Xiangyu |last3=Hwang |first3=Kyu-Ha |last4=Zang |first4=Weicheng |last5=Gould |first5=Andrew |last6=Wang |first6=Tianshu |last7=Mao |first7=Shude |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Han |first10=Cheongho |last11=Jung |first11=Youn Kil |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2020-03-01 |title=KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field |journal=The Astronomical Journal |volume=159 |issue=3 |pages=98 |doi=10.3847/1538-3881/ab660e |doi-access=free |arxiv=1908.10011 |bibcode=2020AJ....159...98Y |issn=0004-6256}}</ref>
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|KMT-2016-BLG-1107Lb |KMT-2016-BLG-1107Lb
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|2019<ref>{{Cite journal |last=Hwang |first=Kyu-Ha |last2=Ryu |first2=Yoon-Hyun |last3=Kim |first3=Hyoun-Woo |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Gould |first6=Andrew |last7=Han |first7=Cheongho |last8=Jung |first8=Youn Kil |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2019-01-01 |title=KMT-2016-BLG-1107: A New Hollywood-planet Close/Wide Degeneracy |url=https://ui.adsabs.harvard.edu/abs/2019AJ....157...23H |journal=The Astronomical Journal |volume=157 |pages=23 |doi=10.3847/1538-3881/aaf16e |issn=0004-6256}}</ref> |2019<ref>{{Cite journal |last1=Hwang |first1=Kyu-Ha |last2=Ryu |first2=Yoon-Hyun |last3=Kim |first3=Hyoun-Woo |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Gould |first6=Andrew |last7=Han |first7=Cheongho |last8=Jung |first8=Youn Kil |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2019-01-01 |title=KMT-2016-BLG-1107: A New Hollywood-planet Close/Wide Degeneracy |journal=The Astronomical Journal |volume=157 |issue=1 |pages=23 |doi=10.3847/1538-3881/aaf16e |doi-access=free |arxiv=1805.08888 |bibcode=2019AJ....157...23H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-1700Lb |OGLE-2018-BLG-1700Lb
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|2020<ref>{{Cite journal |last=Han |first=Cheongho |last2=Lee |first2=Chung-Uk |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=AUTHORS |first6=LEADING |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2020-02-01 |title=OGLE-2018-BLG-1700L: Microlensing Planet in Binary Stellar System |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159...48H |journal=The Astronomical Journal |volume=159 |pages=48 |doi=10.3847/1538-3881/ab5db9 |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=AUTHORS |first6=LEADING |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2020-02-01 |title=OGLE-2018-BLG-1700L: Microlensing Planet in Binary Stellar System |journal=The Astronomical Journal |volume=159 |issue=2 |pages=48 |doi=10.3847/1538-3881/ab5db9 |doi-access=free |arxiv=1909.04854 |bibcode=2020AJ....159...48H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-1269Lb |OGLE-2018-BLG-1269Lb
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|2020<ref>{{Cite journal |last=Jung |first=Youn Kil |last2=Gould |first2=Andrew |last3=Udalski |first3=Andrzej |last4=Sumi |first4=Takahiro |last5=Yee |first5=Jennifer C. |last6=Han |first6=Cheongho |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Zhu |first13=Wei |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-09-01 |title=OGLE-2018-BLG-1269Lb: A Jovian Planet with a Bright I = 16 Host |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160..148J |journal=The Astronomical Journal |volume=160 |pages=148 |doi=10.3847/1538-3881/abacc8 |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Jung |first1=Youn Kil |last2=Gould |first2=Andrew |last3=Udalski |first3=Andrzej |last4=Sumi |first4=Takahiro |last5=Yee |first5=Jennifer C. |last6=Han |first6=Cheongho |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Zhu |first13=Wei |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-09-01 |title=OGLE-2018-BLG-1269Lb: A Jovian Planet with a Bright I = 16 Host |journal=The Astronomical Journal |volume=160 |issue=3 |pages=148 |doi=10.3847/1538-3881/abacc8 |doi-access=free |arxiv=2006.15774 |bibcode=2020AJ....160..148J |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0677Lb |OGLE-2018-BLG-0677Lb
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|2020<ref>{{Cite journal |last=Herrera-Martín |first=Antonio |last2=Albrow |first2=M. D. |last3=Udalski |first3=A. |last4=Gould |first4=A. |last5=Ryu |first5=Y. -H. |last6=Yee |first6=J. C. |last7=Chung |first7=S. -J. |last8=Han |first8=C. |last9=Hwang |first9=K. -H. |last10=Jung |first10=Y. K. |last11=Lee |first11=C. -U. |last12=Shin |first12=I. -G. |last13=Shvartzvald |first13=Y. |last14=Zang |first14=W. |last15=Cha |first15=S. -M. |date=2020-06-01 |title=OGLE-2018-BLG-0677Lb: A Super-Earth Near the Galactic Bulge |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159..256H |journal=The Astronomical Journal |volume=159 |pages=256 |doi=10.3847/1538-3881/ab893e |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Herrera-Martín |first1=Antonio |last2=Albrow |first2=M. D. |last3=Udalski |first3=A. |last4=Gould |first4=A. |last5=Ryu |first5=Y. -H. |last6=Yee |first6=J. C. |last7=Chung |first7=S. -J. |last8=Han |first8=C. |last9=Hwang |first9=K. -H. |last10=Jung |first10=Y. K. |last11=Lee |first11=C. -U. |last12=Shin |first12=I. -G. |last13=Shvartzvald |first13=Y. |last14=Zang |first14=W. |last15=Cha |first15=S. -M. |date=2020-06-01 |title=OGLE-2018-BLG-0677Lb: A Super-Earth Near the Galactic Bulge |journal=The Astronomical Journal |volume=159 |issue=6 |pages=256 |doi=10.3847/1538-3881/ab893e |doi-access=free |arxiv=2003.02983 |bibcode=2020AJ....159..256H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0532Lb |OGLE-2018-BLG-0532Lb
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|2020<ref>{{Cite journal |last=Ryu |first=Yoon-Hyun |last2=Udalski |first2=Andrzej |last3=Yee |first3=Jennifer C. |last4=Penny |first4=Matthew T. |last5=Zang |first5=Weicheng |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Han |first9=Cheongho |last10=Hwang |first10=Kyu-Ha |last11=Jung |first11=Youn Kil |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-10-01 |title=OGLE-2018-BLG-0532Lb: Cold Neptune with Possible Jovian Sibling |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160..183R |journal=The Astronomical Journal |volume=160 |pages=183 |doi=10.3847/1538-3881/abaa3f |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Udalski |first2=Andrzej |last3=Yee |first3=Jennifer C. |last4=Penny |first4=Matthew T. |last5=Zang |first5=Weicheng |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Han |first9=Cheongho |last10=Hwang |first10=Kyu-Ha |last11=Jung |first11=Youn Kil |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-10-01 |title=OGLE-2018-BLG-0532Lb: Cold Neptune with Possible Jovian Sibling |journal=The Astronomical Journal |volume=160 |issue=4 |pages=183 |doi=10.3847/1538-3881/abaa3f |doi-access=free |arxiv=1905.08148 |bibcode=2020AJ....160..183R |issn=0004-6256}}</ref>
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|OGLE-2017-BLG-1375Lb |OGLE-2017-BLG-1375Lb
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|2020<ref name=":7">{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Jung |first4=Youn Kil |last5=Ryu |first5=Yoon-Hyun |last6=KMTNet Collaboration |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Lee |first11=Chung-Uk |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2020-10-01 |title=Four microlensing planets with faint-source stars identified in the 2016 and 2017 season data |url=https://ui.adsabs.harvard.edu/abs/2020A&A...642A.110H |journal=Astronomy and Astrophysics |volume=642 |pages=A110 |doi=10.1051/0004-6361/202039066 |issn=0004-6361}}</ref> |2020<ref name=":7">{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Jung |first4=Youn Kil |last5=Ryu |first5=Yoon-Hyun |last6=KMTNet Collaboration |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Lee |first11=Chung-Uk |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2020-10-01 |title=Four microlensing planets with faint-source stars identified in the 2016 and 2017 season data |url=https://ui.adsabs.harvard.edu/abs/2020A&A...642A.110H |journal=Astronomy and Astrophysics |volume=642 |pages=A110 |doi=10.1051/0004-6361/202039066 |arxiv=2008.09258 |bibcode=2020A&A...642A.110H |issn=0004-6361}}</ref>
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|OGLE-2017-BLG-1049Lb |OGLE-2017-BLG-1049Lb
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|2020<ref>{{Cite journal |last=Kim |first=Yun Hak |last2=Chung |first2=Sun-Ju |last3=Udalski |first3=A. |last4=Bond |first4=Ian A. |last5=Jung |first5=Youn Kil |last6=Gould |first6=Andrew |last7=Albrow |first7=Michael D. |last8=Han |first8=Cheongho |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-12-01 |title=OGLE-2017-BLG-1049: Another Giant Planet Microlensing Event |url=https://ui.adsabs.harvard.edu/abs/2020JKAS...53..161K |journal=Journal of Korean Astronomical Society |volume=53 |pages=161–168 |doi=10.5303/JKAS.2020.53.6.161 |issn=1225-4614}}</ref> |2020<ref>{{Cite journal |last1=Kim |first1=Yun Hak |last2=Chung |first2=Sun-Ju |last3=Udalski |first3=A. |last4=Bond |first4=Ian A. |last5=Jung |first5=Youn Kil |last6=Gould |first6=Andrew |last7=Albrow |first7=Michael D. |last8=Han |first8=Cheongho |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-12-01 |title=OGLE-2017-BLG-1049: Another Giant Planet Microlensing Event |url=https://ui.adsabs.harvard.edu/abs/2020JKAS...53..161K |journal=Journal of Korean Astronomical Society |volume=53 |issue=6 |pages=161–168 |doi=10.5303/JKAS.2020.53.6.161 |arxiv=2012.11080 |bibcode=2020JKAS...53..161K |issn=1225-4614}}</ref>
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|OGLE-2017-BLG-0604Lb |OGLE-2017-BLG-0604Lb
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|2020<ref>{{Cite journal |last=Hirao |first=Yuki |last2=Bennett |first2=David P. |last3=Ryu |first3=Yoon-Hyun |last4=Koshimoto |first4=Naoki |last5=Udalski |first5=Andrzej |last6=Yee |first6=Jennifer C. |last7=Sumi |first7=Takahiro |last8=Bond |first8=Ian A. |last9=Shvartzvald |first9=Yossi |last10=Abe |first10=Fumio |last11=Barry |first11=Richard K. |last12=Bhattacharya |first12=Aparna |last13=Donachie |first13=Martin |last14=Fukui |first14=Akihiko |last15=Itow |first15=Yoshitaka |date=2020-08-01 |title=OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160...74H |journal=The Astronomical Journal |volume=160 |pages=74 |doi=10.3847/1538-3881/ab9ac3 |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Hirao |first1=Yuki |last2=Bennett |first2=David P. |last3=Ryu |first3=Yoon-Hyun |last4=Koshimoto |first4=Naoki |last5=Udalski |first5=Andrzej |last6=Yee |first6=Jennifer C. |last7=Sumi |first7=Takahiro |last8=Bond |first8=Ian A. |last9=Shvartzvald |first9=Yossi |last10=Abe |first10=Fumio |last11=Barry |first11=Richard K. |last12=Bhattacharya |first12=Aparna |last13=Donachie |first13=Martin |last14=Fukui |first14=Akihiko |last15=Itow |first15=Yoshitaka |date=2020-08-01 |title=OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk |journal=The Astronomical Journal |volume=160 |issue=2 |pages=74 |doi=10.3847/1538-3881/ab9ac3 |doi-access=free |arxiv=2004.09067 |bibcode=2020AJ....160...74H |issn=0004-6256}}</ref>
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|OGLE-2016-BLG-1227Lb |OGLE-2016-BLG-1227Lb
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|2020<ref>{{Cite journal |last=Han |first=Cheongho |last2=Udalsk |first2=Andrzej |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Hwang |first6=Kyu-Ha |last7=Jung |first7=Youn Kil |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-03-01 |title=OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159...91H |journal=The Astronomical Journal |volume=159 |pages=91 |doi=10.3847/1538-3881/ab6a9f |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Udalsk |first2=Andrzej |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Hwang |first6=Kyu-Ha |last7=Jung |first7=Youn Kil |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-03-01 |title=OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event |journal=The Astronomical Journal |volume=159 |issue=3 |pages=91 |doi=10.3847/1538-3881/ab6a9f |doi-access=free |arxiv=1911.11953 |bibcode=2020AJ....159...91H |issn=0004-6256}}</ref>
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|OGLE-2015-BLG-1771Lb |OGLE-2015-BLG-1771Lb
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|2020<ref>{{Cite journal |last=Zhang |first=Xiangyu |last2=Zang |first2=Weicheng |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Ryu |first5=Yoon-Hyun |last6=Wang |first6=Tianshu |last7=Yang |first7=Hongjing |last8=Mao |first8=Shude |last9=Mróz |first9=Przemek |last10=Skowron |first10=Jan |last11=Poleski |first11=Radoslaw |last12=Szymański |first12=Michał K. |last13=Soszyński |first13=Igor |last14=Pietrukowicz |first14=Paweł |last15=Kozłowski |first15=Szymon |date=2020-03-01 |title=OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf? |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159..116Z |journal=The Astronomical Journal |volume=159 |pages=116 |doi=10.3847/1538-3881/ab6f6d |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Zhang |first1=Xiangyu |last2=Zang |first2=Weicheng |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Ryu |first5=Yoon-Hyun |last6=Wang |first6=Tianshu |last7=Yang |first7=Hongjing |last8=Mao |first8=Shude |last9=Mróz |first9=Przemek |last10=Skowron |first10=Jan |last11=Poleski |first11=Radoslaw |last12=Szymański |first12=Michał K. |last13=Soszyński |first13=Igor |last14=Pietrukowicz |first14=Paweł |last15=Kozłowski |first15=Szymon |date=2020-03-01 |title=OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf? |journal=The Astronomical Journal |volume=159 |issue=3 |pages=116 |doi=10.3847/1538-3881/ab6f6d |doi-access=free |arxiv=1911.02439 |bibcode=2020AJ....159..116Z |issn=0004-6256}}</ref>
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|OGLE-2012-BLG-0838Lb |OGLE-2012-BLG-0838Lb
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|2020<ref>{{Cite journal |last=Poleski |first=R. |last2=Suzuki |first2=Daisuke |last3=Udalski |first3=A. |last4=Xie |first4=Xiaojia |last5=Yee |first5=J. C. |last6=Koshimoto |first6=Naoki |last7=Gaudi |first7=B. S. |last8=Gould |first8=A. |last9=Skowron |first9=J. |last10=Szymański |first10=M. K. |last11=Soszyński |first11=I. |last12=Pietrukowicz |first12=P. |last13=Kozłowski |first13=S. |last14=Wyrzykowski |first14=Ł. |last15=Ulaczyk |first15=K. |date=2020-06-01 |title=A Wide-orbit Exoplanet OGLE-2012-BLG-0838Lb |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159..261P |journal=The Astronomical Journal |volume=159 |pages=261 |doi=10.3847/1538-3881/ab8a49 |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Poleski |first1=R. |last2=Suzuki |first2=Daisuke |last3=Udalski |first3=A. |last4=Xie |first4=Xiaojia |last5=Yee |first5=J. C. |last6=Koshimoto |first6=Naoki |last7=Gaudi |first7=B. S. |last8=Gould |first8=A. |last9=Skowron |first9=J. |last10=Szymański |first10=M. K. |last11=Soszyński |first11=I. |last12=Pietrukowicz |first12=P. |last13=Kozłowski |first13=S. |last14=Wyrzykowski |first14=Ł. |last15=Ulaczyk |first15=K. |date=2020-06-01 |title=A Wide-orbit Exoplanet OGLE-2012-BLG-0838Lb |journal=The Astronomical Journal |volume=159 |issue=6 |pages=261 |doi=10.3847/1538-3881/ab8a49 |doi-access=free |arxiv=1901.05466 |bibcode=2020AJ....159..261P |issn=0004-6256}}</ref>
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|OGLE-2006-BLG-284LAb |OGLE-2006-BLG-284LAb
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| 2020<ref>{{Cite journal |last=Bennett |first=David P. |last2=Udalski |first2=Andrzej |last3=Bond |first3=Ian A. |last4=Abe |first4=Fumio |last5=Barry |first5=Richard K. |last6=Bhattacharya |first6=Aparna |last7=Donachie |first7=Martin |last8=Fujii |first8=Hirosane |last9=Fukui |first9=Akihiko |last10=Hirao |first10=Yuki |last11=Itow |first11=Yoshitaka |last12=Kawasaki |first12=Kohei |last13=Kirikawa |first13=Rintaro |last14=Kondo |first14=Iona |last15=Koshimoto |first15=Naoki |date=2020-08-01 |title=A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160...72B |journal=The Astronomical Journal |volume=160 |pages=72 |doi=10.3847/1538-3881/ab9cb9 |issn=0004-6256}}</ref> | 2020<ref>{{Cite journal |last1=Bennett |first1=David P. |last2=Udalski |first2=Andrzej |last3=Bond |first3=Ian A. |last4=Abe |first4=Fumio |last5=Barry |first5=Richard K. |last6=Bhattacharya |first6=Aparna |last7=Donachie |first7=Martin |last8=Fujii |first8=Hirosane |last9=Fukui |first9=Akihiko |last10=Hirao |first10=Yuki |last11=Itow |first11=Yoshitaka |last12=Kawasaki |first12=Kohei |last13=Kirikawa |first13=Rintaro |last14=Kondo |first14=Iona |last15=Koshimoto |first15=Naoki |date=2020-08-01 |title=A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System |journal=The Astronomical Journal |volume=160 |issue=2 |pages=72 |doi=10.3847/1538-3881/ab9cb9 |doi-access=free |arxiv=2005.07199 |bibcode=2020AJ....160...72B |issn=0004-6256}}</ref>
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|KMT-2019-BLG-1953Lb |KMT-2019-BLG-1953Lb
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|2020<ref>{{Cite journal |last=Han |first=Cheongho |last2=Kim |first2=Doeon |last3=Jung |first3=Youn Kil |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-07-01 |title=One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953 |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160...17H |journal=The Astronomical Journal |volume=160 |pages=17 |doi=10.3847/1538-3881/ab91ac |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Jung |first3=Youn Kil |last4=Gould |first4=Andrew |last5=Bond |first5=Ian A. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-07-01 |title=One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953 |journal=The Astronomical Journal |volume=160 |issue=1 |pages=17 |doi=10.3847/1538-3881/ab91ac |doi-access=free |arxiv=2002.05310 |bibcode=2020AJ....160...17H |issn=0004-6256}}</ref>
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|KMT-2019-BLG-1339Lb |KMT-2019-BLG-1339Lb
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|2020<ref>{{Cite journal |last=Han |first=Cheongho |last2=Kim |first2=Doeon |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-08-01 |title=KMT-2019-BLG-1339L: An M Dwarf with a Giant Planet or a Companion near the Planet/Brown Dwarf Boundary |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160...64H |journal=The Astronomical Journal |volume=160 |pages=64 |doi=10.3847/1538-3881/ab9a3e |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2020-08-01 |title=KMT-2019-BLG-1339L: An M Dwarf with a Giant Planet or a Companion near the Planet/Brown Dwarf Boundary |journal=The Astronomical Journal |volume=160 |issue=2 |pages=64 |doi=10.3847/1538-3881/ab9a3e |doi-access=free |arxiv=2003.02375 |bibcode=2020AJ....160...64H |issn=0004-6256}}</ref>
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|KMT-2019-BLG-0842Lb |KMT-2019-BLG-0842Lb
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|2020<ref>{{Cite journal |last=Jung |first=Youn Kil |last2=Udalski |first2=Andrzej |last3=Zang |first3=Weicheng |last4=Bond |first4=Ian A. |last5=Yee |first5=Jennifer C. |last6=Han |first6=Cheongho |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-12-01 |title=KMT-2019-BLG-0842Lb: A Cold Planet below the Uranus/Sun Mass Ratio |url=https://ui.adsabs.harvard.edu/abs/2020AJ....160..255J |journal=The Astronomical Journal |volume=160 |pages=255 |doi=10.3847/1538-3881/abbe93 |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Jung |first1=Youn Kil |last2=Udalski |first2=Andrzej |last3=Zang |first3=Weicheng |last4=Bond |first4=Ian A. |last5=Yee |first5=Jennifer C. |last6=Han |first6=Cheongho |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-12-01 |title=KMT-2019-BLG-0842Lb: A Cold Planet below the Uranus/Sun Mass Ratio |journal=The Astronomical Journal |volume=160 |issue=6 |pages=255 |doi=10.3847/1538-3881/abbe93 |doi-access=free |arxiv=1912.03822 |bibcode=2020AJ....160..255J |issn=0004-6256}}</ref>
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|KMT-2018-BLG-1292Lb |KMT-2018-BLG-1292Lb
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|2020<ref>{{Cite journal |last=Ryu |first=Yoon-Hyun |last2=Navarro |first2=Maria Gabriela |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Han |first6=Cheongho |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2020-02-01 |title=KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane |url=https://ui.adsabs.harvard.edu/abs/2020AJ....159...58R |journal=The Astronomical Journal |volume=159 |pages=58 |doi=10.3847/1538-3881/ab5e7e |issn=0004-6256}}</ref> |2020<ref>{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Navarro |first2=Maria Gabriela |last3=Gould |first3=Andrew |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Han |first6=Cheongho |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2020-02-01 |title=KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane |journal=The Astronomical Journal |volume=159 |issue=2 |pages=58 |doi=10.3847/1538-3881/ab5e7e |doi-access=free |arxiv=1905.04870 |bibcode=2020AJ....159...58R |issn=0004-6256}}</ref>
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|KMT-2018-BLG-0748Lb |KMT-2018-BLG-0748Lb
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|2020<ref>{{Cite journal |last=Han |first=Cheongho |last2=Shin |first2=In-Gu |last3=Jung |first3=Youn Kil |last4=Kim |first4=Doeon |last5=Yee |first5=Jennifer C. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Lee |first10=Chung-Uk |last11=Ryu |first11=Yoon-Hyun |last12=Shvartzvald |first12=Yossi |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-09-01 |title=KMT-2018-BLG-0748Lb: sub-Saturn microlensing planet orbiting an ultracool host |url=https://ui.adsabs.harvard.edu/abs/2020A&A...641A.105H |journal=Astronomy and Astrophysics |volume=641 |pages=A105 |doi=10.1051/0004-6361/202038173 |issn=0004-6361}}</ref> |2020<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Shin |first2=In-Gu |last3=Jung |first3=Youn Kil |last4=Kim |first4=Doeon |last5=Yee |first5=Jennifer C. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Lee |first10=Chung-Uk |last11=Ryu |first11=Yoon-Hyun |last12=Shvartzvald |first12=Yossi |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2020-09-01 |title=KMT-2018-BLG-0748Lb: sub-Saturn microlensing planet orbiting an ultracool host |url=https://ui.adsabs.harvard.edu/abs/2020A&A...641A.105H |journal=Astronomy and Astrophysics |volume=641 |pages=A105 |doi=10.1051/0004-6361/202038173 |arxiv=2007.05204 |bibcode=2020A&A...641A.105H |issn=0004-6361}}</ref>
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|KMT-2018-BLG-0029Lb |KMT-2018-BLG-0029Lb
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|2020<ref>{{Cite journal |last=Gould |first=Andrew |last2=Ryu |first2=Yoon-Hyun |last3=Calchi Novati |first3=Sebastiano |last4=Zang |first4=Weicheng |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |last9=Jung |first9=Youn Kil |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2020-02-01 |title=KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet |url=https://ui.adsabs.harvard.edu/abs/2020JKAS...53....9G |journal=Journal of Korean Astronomical Society |volume=53 |pages=9–26 |doi=10.5303/JKAS.2020.53.1.9 |issn=1225-4614}}</ref> |2020<ref>{{Cite journal |last1=Gould |first1=Andrew |last2=Ryu |first2=Yoon-Hyun |last3=Calchi Novati |first3=Sebastiano |last4=Zang |first4=Weicheng |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |last9=Jung |first9=Youn Kil |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Hyoun-Woo |date=2020-02-01 |title=KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet |url=https://ui.adsabs.harvard.edu/abs/2020JKAS...53....9G |journal=Journal of Korean Astronomical Society |volume=53 |issue=1 |pages=9–26 |doi=10.5303/JKAS.2020.53.1.9 |arxiv=1906.11183 |bibcode=2020JKAS...53....9G |issn=1225-4614}}</ref>
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|KMT-2016-BLG-2397Lb |KMT-2016-BLG-2397Lb
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|2021<ref>{{Cite journal |last=Zang |first=Weicheng |last2=Hwang |first2=Kyu-Ha |last3=Udalski |first3=Andrzej |last4=Wang |first4=Tianshu |last5=Zhu |first5=Wei |last6=Sumi |first6=Takahiro |last7=Yee |first7=Jennifer C. |last8=Gould |first8=Andrew |last9=Mao |first9=Shude |last10=Zhang |first10=Xiangyu |last11=Albrow |first11=Michael D. |last12=Chung |first12=Sun-Ju |last13=Han |first13=Cheongho |last14=Jung |first14=Youn Kil |last15=Ryu |first15=Yoon-Hyun |date=2021-10-01 |title=Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet |url=https://ui.adsabs.harvard.edu/abs/2021AJ....162..163Z |journal=The Astronomical Journal |volume=162 |pages=163 |doi=10.3847/1538-3881/ac12d4 |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Zang |first1=Weicheng |last2=Hwang |first2=Kyu-Ha |last3=Udalski |first3=Andrzej |last4=Wang |first4=Tianshu |last5=Zhu |first5=Wei |last6=Sumi |first6=Takahiro |last7=Yee |first7=Jennifer C. |last8=Gould |first8=Andrew |last9=Mao |first9=Shude |last10=Zhang |first10=Xiangyu |last11=Albrow |first11=Michael D. |last12=Chung |first12=Sun-Ju |last13=Han |first13=Cheongho |last14=Jung |first14=Youn Kil |last15=Ryu |first15=Yoon-Hyun |date=2021-10-01 |title=Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet |journal=The Astronomical Journal |volume=162 |issue=4 |pages=163 |doi=10.3847/1538-3881/ac12d4 |doi-access=free |arxiv=2103.11880 |bibcode=2021AJ....162..163Z |issn=0004-6256}}</ref>
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|OGLE-2019-BLG-0960Lb |OGLE-2019-BLG-0960Lb
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|2021<ref>{{Cite journal |last=Yee |first=Jennifer C. |last2=Zang |first2=Weicheng |last3=Udalski |first3=Andrzej |last4=Ryu |first4=Yoon-Hyun |last5=Green |first5=Jonathan |last6=Hennerley |first6=Steve |last7=Marmont |first7=Andrew |last8=Sumi |first8=Takahiro |last9=Mao |first9=Shude |last10=Gromadzki |first10=Mariusz |last11=Mróz |first11=Przemek |last12=Skowron |first12=Jan |last13=Poleski |first13=Radoslaw |last14=Szymański |first14=Michał K. |last15=Soszyński |first15=Igor |date=2021-11-01 |title=OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet |url=https://ui.adsabs.harvard.edu/abs/2021AJ....162..180Y |journal=The Astronomical Journal |volume=162 |pages=180 |doi=10.3847/1538-3881/ac1582 |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Yee |first1=Jennifer C. |last2=Zang |first2=Weicheng |last3=Udalski |first3=Andrzej |last4=Ryu |first4=Yoon-Hyun |last5=Green |first5=Jonathan |last6=Hennerley |first6=Steve |last7=Marmont |first7=Andrew |last8=Sumi |first8=Takahiro |last9=Mao |first9=Shude |last10=Gromadzki |first10=Mariusz |last11=Mróz |first11=Przemek |last12=Skowron |first12=Jan |last13=Poleski |first13=Radoslaw |last14=Szymański |first14=Michał K. |last15=Soszyński |first15=Igor |date=2021-11-01 |title=OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet |journal=The Astronomical Journal |volume=162 |issue=5 |pages=180 |doi=10.3847/1538-3881/ac1582 |doi-access=free |arxiv=2101.04696 |bibcode=2021AJ....162..180Y |issn=0004-6256}}</ref>
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|OGLE-2019-BLG-0954Lb |OGLE-2019-BLG-0954Lb
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|2021<ref name=":8">{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Lee |first4=Chung-Uk |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Gould |first7=Andrew |last8=Hwang |first8=Kyu-Ha |last9=Jung |first9=Youn Kil |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2021-06-01 |title=Three microlensing planets with no caustic-crossing features |url=https://ui.adsabs.harvard.edu/abs/2021A&A...650A..89H |journal=Astronomy and Astrophysics |volume=650 |pages=A89 |doi=10.1051/0004-6361/202140758 |issn=0004-6361}}</ref> |2021<ref name=":8">{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Lee |first4=Chung-Uk |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Gould |first7=Andrew |last8=Hwang |first8=Kyu-Ha |last9=Jung |first9=Youn Kil |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2021-06-01 |title=Three microlensing planets with no caustic-crossing features |url=https://ui.adsabs.harvard.edu/abs/2021A&A...650A..89H |journal=Astronomy and Astrophysics |volume=650 |pages=A89 |doi=10.1051/0004-6361/202140758 |arxiv=2104.06544 |bibcode=2021A&A...650A..89H |issn=0004-6361}}</ref>
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|OGLE-2019-BLG-0304Lb |OGLE-2019-BLG-0304Lb
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|2021<ref>{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Kim |first4=Doeon |last5=Ryu |first5=Yoon-Hyun |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Kil Jung |first10=Youn |last11=Kim |first11=Hyoun-Woo |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=OGLE-2019-BLG-0304: Competing Interpretations between a Planet-binary Model and a Binary-source + Binary-lens Model |url=https://ui.adsabs.harvard.edu/abs/2021AJ....162..203H |journal=The Astronomical Journal |volume=162 |pages=203 |doi=10.3847/1538-3881/ac1c09 |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Kim |first4=Doeon |last5=Ryu |first5=Yoon-Hyun |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Kil Jung |first10=Youn |last11=Kim |first11=Hyoun-Woo |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=OGLE-2019-BLG-0304: Competing Interpretations between a Planet-binary Model and a Binary-source + Binary-lens Model |journal=The Astronomical Journal |volume=162 |issue=5 |pages=203 |doi=10.3847/1538-3881/ac1c09 |doi-access=free |arxiv=2109.02209 |bibcode=2021AJ....162..203H |issn=0004-6256}}</ref>
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|OGLE-2019-BLG-0299Lb |OGLE-2019-BLG-0299Lb
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|2021<ref name=":9">{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Ryu |first4=Yoon-Hyun |last5=Bozza |first5=Valerio |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Lee |first11=Chung-Uk |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=Three faint-source microlensing planets detected via the resonant-caustic channel |url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..21H |journal=Astronomy and Astrophysics |volume=655 |pages=A21 |doi=10.1051/0004-6361/202141517 |issn=0004-6361}}</ref> |2021<ref name=":9">{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Ryu |first4=Yoon-Hyun |last5=Bozza |first5=Valerio |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Lee |first11=Chung-Uk |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=Three faint-source microlensing planets detected via the resonant-caustic channel |url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..21H |journal=Astronomy and Astrophysics |volume=655 |pages=A21 |doi=10.1051/0004-6361/202141517 |arxiv=2109.07068 |bibcode=2021A&A...655A..21H |issn=0004-6361}}</ref>
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|OGLE-2017-BLG-1099Lb |OGLE-2017-BLG-1099Lb
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|2021<ref>{{Cite journal |last=Kim |first=Yun Hak |last2=Chung |first2=Sun-Ju |last3=Udalski |first3=Andrej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Han |first8=Cheongho |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2021-05-01 |title=OGLE-2018-BLG-1428Lb: a Jupiter-mass planet beyond the snow line of a dwarf star |url=https://ui.adsabs.harvard.edu/abs/2021MNRAS.503.2706K |journal=Monthly Notices of the Royal Astronomical Society |volume=503 |pages=2706–2712 |doi=10.1093/mnras/stab534 |issn=0035-8711}}</ref> |2021<ref>{{Cite journal |last1=Kim |first1=Yun Hak |last2=Chung |first2=Sun-Ju |last3=Udalski |first3=Andrej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Han |first8=Cheongho |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2021-05-01 |title=OGLE-2018-BLG-1428Lb: a Jupiter-mass planet beyond the snow line of a dwarf star |journal=Monthly Notices of the Royal Astronomical Society |volume=503 |issue=2 |pages=2706–2712 |doi=10.1093/mnras/stab534 |doi-access=free |arxiv=2102.11463 |bibcode=2021MNRAS.503.2706K |issn=0035-8711}}</ref>
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|OGLE-2018-BLG-1185Lb |OGLE-2018-BLG-1185Lb
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|2021<ref>{{Cite journal |last=Kondo |first=Iona |last2=Yee |first2=Jennifer C. |last3=Bennett |first3=David P. |last4=Sumi |first4=Takahiro |last5=Koshimoto |first5=Naoki |last6=Bond |first6=Ian A. |last7=Gould |first7=Andrew |last8=Udalski |first8=Andrzej |last9=Shvartzvald |first9=Yossi |last10=Jung |first10=Youn Kil |last11=Zang |first11=Weicheng |last12=Bozza |first12=Valerio |last13=Bachelet |first13=Etienne |last14=Hundertmark |first14=Markus P. G. |last15=Rattenbury |first15=Nicholas J. |date=2021-08-01 |title=OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf |url=https://ui.adsabs.harvard.edu/abs/2021AJ....162...77K |journal=The Astronomical Journal |volume=162 |pages=77 |doi=10.3847/1538-3881/ac00ba |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Kondo |first1=Iona |last2=Yee |first2=Jennifer C. |last3=Bennett |first3=David P. |last4=Sumi |first4=Takahiro |last5=Koshimoto |first5=Naoki |last6=Bond |first6=Ian A. |last7=Gould |first7=Andrew |last8=Udalski |first8=Andrzej |last9=Shvartzvald |first9=Yossi |last10=Jung |first10=Youn Kil |last11=Zang |first11=Weicheng |last12=Bozza |first12=Valerio |last13=Bachelet |first13=Etienne |last14=Hundertmark |first14=Markus P. G. |last15=Rattenbury |first15=Nicholas J. |date=2021-08-01 |title=OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf |journal=The Astronomical Journal |volume=162 |issue=2 |pages=77 |doi=10.3847/1538-3881/ac00ba |doi-access=free |arxiv=2104.02157 |bibcode=2021AJ....162...77K |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0962Lb |OGLE-2018-BLG-0962Lb
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|2021<ref name=":10">{{Cite journal |last=Jung |first=Youn Kil |last2=Han |first2=Cheongho |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Yee |first5=Jennifer C. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zhu |first12=Wei |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2021-06-01 |title=OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel |url=https://ui.adsabs.harvard.edu/abs/2021AJ....161..293J |journal=The Astronomical Journal |volume=161 |pages=293 |doi=10.3847/1538-3881/abf8bd |issn=0004-6256}}</ref> |2021<ref name=":10">{{Cite journal |last1=Jung |first1=Youn Kil |last2=Han |first2=Cheongho |last3=Udalski |first3=Andrzej |last4=Gould |first4=Andrew |last5=Yee |first5=Jennifer C. |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zhu |first12=Wei |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2021-06-01 |title=OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel |journal=The Astronomical Journal |volume=161 |issue=6 |pages=293 |doi=10.3847/1538-3881/abf8bd |doi-access=free |arxiv=2102.07338 |bibcode=2021AJ....161..293J |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0567Lb |OGLE-2018-BLG-0567Lb
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|2021<ref>{{Cite journal |last=Han |first=Cheongho |last2=Gould |first2=Andrew |last3=Hirao |first3=Yuki |last4=Lee |first4=Chung-Uk |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Kim |first9=Doeon |last10=Mao |first10=Shude |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations |url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..24H |journal=Astronomy and Astrophysics |volume=655 |pages=A24 |doi=10.1051/0004-6361/202141939 |issn=0004-6361}}</ref> |2021<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Hirao |first3=Yuki |last4=Lee |first4=Chung-Uk |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Kim |first9=Doeon |last10=Mao |first10=Shude |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-11-01 |title=KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations |url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..24H |journal=Astronomy and Astrophysics |volume=655 |pages=A24 |doi=10.1051/0004-6361/202141939 |arxiv=2109.02210 |bibcode=2021A&A...655A..24H |issn=0004-6361}}</ref>
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|KMT-2020-BLG-0414Lb |]<nowiki/>b
|0.00381 |0.00588
|1.79 |2.07
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|2021<ref name=":4">{{Cite journal |last1=Zang |first1=Weicheng |last2=Han |first2=Cheongho |last3=Kondo |first3=Iona |last4=Yee |first4=Jennifer C. |last5=Lee |first5=Chung-Uk |last6=Gould |first6=Andrew |last7=Mao |first7=Shude |last8=de Almeida |first8=Leandro |last9=Shvartzvald |first9=Yossi |last10=Zhang |first10=Xiangyu |last11=Albrow |first11=Michael D. |last12=Chung |first12=Sun-Ju |last13=Hwang |first13=Kyu-Ha |last14=Jung |first14=Youn Kil |last15=Ryu |first15=Yoon-Hyun |date=2021-11-01 |title=An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb |url=https://iopscience.iop.org/article/10.1088/1674-4527/21/9/239 |journal=Research in Astronomy and Astrophysics |volume=21 |issue=9 |pages=239 |doi=10.1088/1674-4527/21/9/239 |issn=1674-4527}}</ref> |2021<ref name=":4">{{Cite journal |last1=Zang |first1=Weicheng |last2=Han |first2=Cheongho |last3=Kondo |first3=Iona |last4=Yee |first4=Jennifer C. |last5=Lee |first5=Chung-Uk |last6=Gould |first6=Andrew |last7=Mao |first7=Shude |last8=de Almeida |first8=Leandro |last9=Shvartzvald |first9=Yossi |last10=Zhang |first10=Xiangyu |last11=Albrow |first11=Michael D. |last12=Chung |first12=Sun-Ju |last13=Hwang |first13=Kyu-Ha |last14=Jung |first14=Youn Kil |last15=Ryu |first15=Yoon-Hyun |date=2021-11-01 |title=An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb |url=https://iopscience.iop.org/article/10.1088/1674-4527/21/9/239 |journal=Research in Astronomy and Astrophysics |volume=21 |issue=9 |pages=239 |doi=10.1088/1674-4527/21/9/239 |arxiv=2103.01896 |bibcode=2021RAA....21..239Z |issn=1674-4527}}</ref><ref name="Zhang2024" />
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|KMT-2020-BLG-0414Lc |]<nowiki/>c
|27
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|0.12 |22.3
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|2021<ref name=":4" /> |2021<ref name=":4" /><ref name="Zhang2024" />
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|KMT-2019-BLG-1715Lb |KMT-2019-BLG-1715Lb
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|2021<ref>{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Kil Jung |first4=Youn |last5=Lee |first5=Chung-Uk |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Kim |first11=Hyoun-Woo |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Zang |first15=Weicheng |date=2021-06-01 |title=KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars |url=https://ui.adsabs.harvard.edu/abs/2021AJ....161..270H |journal=The Astronomical Journal |volume=161 |pages=270 |doi=10.3847/1538-3881/abf4d0 |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Kim |first3=Doeon |last4=Kil Jung |first4=Youn |last5=Lee |first5=Chung-Uk |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Kim |first11=Hyoun-Woo |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Zang |first15=Weicheng |date=2021-06-01 |title=KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars |journal=The Astronomical Journal |volume=161 |issue=6 |pages=270 |doi=10.3847/1538-3881/abf4d0 |doi-access=free |arxiv=2104.00293 |bibcode=2021AJ....161..270H |issn=0004-6256}}</ref>
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| KMT-2019-BLG-0371Lb || 7.7 || 0.79 || || || || 2021<ref name="Kim2021"/> | KMT-2019-BLG-0371Lb || 7.7 || 0.79 || || || || 2021<ref name="Kim2021"/>
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|2021<ref>{{Cite journal |last=Han |first=Cheongho |last2=Albrow |first2=Michael D. |last3=Chung |first3=Sun-Ju |last4=Gould |first4=Andrew |last5=Hwang |first5=Kyu-Ha |last6=Jung |first6=Youn Kil |last7=Kim |first7=Doeon |last8=Kim |first8=Hyoun-Woo |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2021-08-01 |title=KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars |url=https://ui.adsabs.harvard.edu/abs/2021A&A...652A.145H |journal=Astronomy and Astrophysics |volume=652 |pages=A145 |doi=10.1051/0004-6361/202140923 |issn=0004-6361}}</ref> |2021<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Albrow |first2=Michael D. |last3=Chung |first3=Sun-Ju |last4=Gould |first4=Andrew |last5=Hwang |first5=Kyu-Ha |last6=Jung |first6=Youn Kil |last7=Kim |first7=Doeon |last8=Kim |first8=Hyoun-Woo |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2021-08-01 |title=KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars |url=https://ui.adsabs.harvard.edu/abs/2021A&A...652A.145H |journal=Astronomy and Astrophysics |volume=652 |pages=A145 |doi=10.1051/0004-6361/202140923 |arxiv=2107.00155 |bibcode=2021A&A...652A.145H |issn=0004-6361}}</ref>
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|KMT-2018-BLG-1025Lb |KMT-2018-BLG-1025Lb
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|2021<ref>{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Gould |first6=Andrew |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Kim |first9=Doeon |last10=Kim |first10=Hyoun-Woo |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-05-01 |title=KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star |url=https://ui.adsabs.harvard.edu/abs/2021A&A...649A..90H |journal=Astronomy and Astrophysics |volume=649 |pages=A90 |doi=10.1051/0004-6361/202039817 |issn=0004-6361}}</ref> |2021<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Gould |first6=Andrew |last7=Hwang |first7=Kyu-Ha |last8=Jung |first8=Youn Kil |last9=Kim |first9=Doeon |last10=Kim |first10=Hyoun-Woo |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2021-05-01 |title=KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star |url=https://ui.adsabs.harvard.edu/abs/2021A&A...649A..90H |journal=Astronomy and Astrophysics |volume=649 |pages=A90 |doi=10.1051/0004-6361/202039817 |arxiv=2102.01890 |bibcode=2021A&A...649A..90H |issn=0004-6361}}</ref>
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|KMT-2016-BLG-2605Lb |KMT-2016-BLG-2605Lb
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|2021<ref>{{Cite journal |last=Ryu |first=Yoon-Hyun |last2=Hwang |first2=Kyu-Ha |last3=Gould |first3=Andrew |last4=Yee |first4=Jennifer C. |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Jung |first8=Youn Kil |last9=Kim |first9=Hyoun-Woo |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2021-09-01 |title=Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605 |url=https://ui.adsabs.harvard.edu/abs/2021AJ....162...96R |journal=The Astronomical Journal |volume=162 |pages=96 |doi=10.3847/1538-3881/ac062a |issn=0004-6256}}</ref> |2021<ref>{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Hwang |first2=Kyu-Ha |last3=Gould |first3=Andrew |last4=Yee |first4=Jennifer C. |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Jung |first8=Youn Kil |last9=Kim |first9=Hyoun-Woo |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2021-09-01 |title=Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605 |journal=The Astronomical Journal |volume=162 |issue=3 |pages=96 |doi=10.3847/1538-3881/ac062a |doi-access=free |arxiv=2104.07906 |bibcode=2021AJ....162...96R |issn=0004-6256}}</ref>
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|OGLE-2019-BLG-1470L(AB)c |OGLE-2019-BLG-1470L(AB)c
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|2022<ref>{{Cite journal |last=Kuang |first=Renkun |last2=Zang |first2=Weicheng |last3=Jung |first3=Youn Kil |last4=Udalski |first4=Andrzej |last5=Yang |first5=Hongjing |last6=Mao |first6=Shude |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Han |first10=Cheongho |last11=Hwang |first11=Kyu-Ha |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2022-10-01 |title=OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system? |url=https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.1704K |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |pages=1704–1720 |doi=10.1093/mnras/stac2315 |issn=0035-8711}}</ref> |2022<ref>{{Cite journal |last1=Kuang |first1=Renkun |last2=Zang |first2=Weicheng |last3=Jung |first3=Youn Kil |last4=Udalski |first4=Andrzej |last5=Yang |first5=Hongjing |last6=Mao |first6=Shude |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Han |first10=Cheongho |last11=Hwang |first11=Kyu-Ha |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2022-10-01 |title=OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system? |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |issue=2 |pages=1704–1720 |doi=10.1093/mnras/stac2315 |doi-access=free |arxiv=2204.05606 |bibcode=2022MNRAS.516.1704K |issn=0035-8711}}</ref>
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|OGLE-2019-BLG-1492Lb |OGLE-2019-BLG-1492Lb
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|2022<ref name=":11">{{Cite journal |last=Hwang |first=Kyu-Ha |last2=Zang |first2=Weicheng |last3=Gould |first3=Andrew |last4=Udalski |first4=Andrzej |last5=Bond |first5=Ian A. |last6=Yang |first6=Hongjing |last7=Mao |first7=Shude |last8=Mao |first8=Shude |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Han |first11=Cheongho |last12=Kil Jung |first12=Youn |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Shvartzvald |first15=Yossi |date=2022-02-01 |title=Systematic KMTNet Planetary Anomaly Search. II. Six New q < 2 × 10-4 Mass-ratio Planets |url=https://ui.adsabs.harvard.edu/abs/2022AJ....163...43H |journal=The Astronomical Journal |volume=163 |pages=43 |doi=10.3847/1538-3881/ac38ad |issn=0004-6256}}</ref> |2022<ref name=":11">{{Cite journal |last1=Hwang |first1=Kyu-Ha |last2=Zang |first2=Weicheng |last3=Gould |first3=Andrew |last4=Udalski |first4=Andrzej |last5=Bond |first5=Ian A. |last6=Yang |first6=Hongjing |last7=Mao |first7=Shude |last8=Mao |first8=Shude |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Han |first11=Cheongho |last12=Kil Jung |first12=Youn |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Shvartzvald |first15=Yossi |date=2022-02-01 |title=Systematic KMTNet Planetary Anomaly Search. II. Six New q < 2 × 10-4 Mass-ratio Planets |journal=The Astronomical Journal |volume=163 |issue=2 |pages=43 |doi=10.3847/1538-3881/ac38ad |doi-access=free |arxiv=2106.06686 |bibcode=2022AJ....163...43H |issn=0004-6256}}</ref>
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|OGLE-2018-BLG-0977Lb |OGLE-2018-BLG-0977Lb
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|2022<ref name=":5">{{Cite journal |last=Han |first=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Kim |first4=Doeon |last5=Zhu |first5=Wei |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Kim |first11=Hyoun-Woo |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2022-02-01 |title=OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star |url=https://ui.adsabs.harvard.edu/abs/2022A&A...658A..93H |journal=Astronomy and Astrophysics |volume=658 |pages=A93 |doi=10.1051/0004-6361/202142327 |issn=0004-6361}}</ref> |2022<ref name=":5">{{Cite journal |last1=Han |first1=Cheongho |last2=Udalski |first2=Andrzej |last3=Lee |first3=Chung-Uk |last4=Kim |first4=Doeon |last5=Zhu |first5=Wei |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Gould |first8=Andrew |last9=Hwang |first9=Kyu-Ha |last10=Jung |first10=Youn Kil |last11=Kim |first11=Hyoun-Woo |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2022-02-01 |title=OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star |url=https://ui.adsabs.harvard.edu/abs/2022A&A...658A..93H |journal=Astronomy and Astrophysics |volume=658 |pages=A93 |doi=10.1051/0004-6361/202142327 |arxiv=2111.03755 |bibcode=2022A&A...658A..93H |issn=0004-6361}}</ref>
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|OGLE-2019-BLG-0468Lc |OGLE-2019-BLG-0468Lc
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|2022<ref name=":5" /> |2022<ref name=":5" />
|-
|OGLE-2019-BLG-0362Lb
|3.26
|2.18
|
|
|
|2022<ref>{{Cite journal |last1=Chung |first1=Sun-Ju |last2=Yee |first2=Jennifer C. |last3=Udalski |first3=Andrej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Han |first8=Cheongho |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2022-08-01 |title=OGLE-2019-BLG-0362Lb: A Super-Jovian-Mass Planet around a Low-Mass Star |url=https://ui.adsabs.harvard.edu/abs/2022JKAS...55..123C |journal=Journal of Korean Astronomical Society |volume=55 |issue=4 |pages=123–130 |doi=10.5303/JKAS.2022.55.4.123 |arxiv=2208.04230 |bibcode=2022JKAS...55..123C |issn=1225-4614}}</ref>
|-
|OGLE-2018-BLG-1647Lb
|0.970
|1.36
|
|
|
|2022<ref name=":12">{{Cite journal |last1=Gould |first1=Andrew |last2=Han |first2=Cheongho |last3=Zang |first3=Weicheng |last4=Yang |first4=Hongjing |last5=Hwang |first5=Kyu-Ha |last6=Udalski |first6=Andrzej |last7=Bond |first7=Ian A. |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Jung |first10=Youn Kil |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Cha |first15=Sang-Mok |date=2022-08-01 |title=Systematic KMTNet planetary anomaly search. V. Complete sample of 2018 prime-field |url=https://ui.adsabs.harvard.edu/abs/2022A&A...664A..13G |journal=Astronomy and Astrophysics |volume=664 |pages=A13 |doi=10.1051/0004-6361/202243744 |arxiv=2204.04354 |bibcode=2022A&A...664A..13G |issn=0004-6361}}</ref>
|-
|OGLE-2018-BLG-1367Lb
|0.950
|1.21
|
|
|
|2022<ref name=":12" />
|-
|OGLE-2018-BLG-1126Lb
|0.056
|3.23
|
|
|
|2022<ref name=":12" />
|-
|]
|0.910
|4.06
|
|
|
|2022<ref name=":13">{{Cite journal |last1=Jung |first1=Youn Kil |last2=Zang |first2=Weicheng |last3=Han |first3=Cheongho |last4=Gould |first4=Andrew |last5=Udalski |first5=Andrzej |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2022-12-01 |title=Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets |journal=The Astronomical Journal |volume=164 |issue=6 |pages=262 |doi=10.3847/1538-3881/ac9c5c |doi-access=free |arxiv=2206.11409 |bibcode=2022AJ....164..262J |issn=0004-6256}}</ref>
|-
|OGLE-2018-BLG-0298Lb
|0.14
|2.86
|
|
|
|2022<ref name=":13" />
|-
|OGLE-2018-BLG-0383Lb
|0.0201
|1.8
|
|
|
|2022<ref>{{Cite journal |last1=Wang |first1=Hanyue |last2=Zang |first2=Weicheng |last3=Zhu |first3=Wei |last4=Hwang |first4=Kyu-Ha |last5=Udalski |first5=Andrzej |last6=Gould |first6=Andrew |last7=Han |first7=Cheongho |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Jung |first10=Youn Kil |last11=Kim |first11=Doeon |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |date=2022-02-01 |title=Systematic Korea Microlensing Telescope Network planetary anomaly search - III. One wide-orbit planet and two stellar binaries |journal=Monthly Notices of the Royal Astronomical Society |volume=510 |issue=2 |pages=1778–1790 |doi=10.1093/mnras/stab3581 |doi-access=free |arxiv=2112.02414 |bibcode=2022MNRAS.510.1778W |issn=0035-8711}}</ref>
|-
|OGLE-2017-BLG-1691Lb
|0.046
|2.41
|
|
|
|2022<ref name=":14">{{Cite journal |last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Gould |first3=Andrew |last4=Udalski |first4=Andrzej |last5=Bond |first5=Ian A. |last6=Bozza |first6=Valerio |last7=Jung |first7=Youn Kil |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Hwang |first10=Kyu-Ha |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |date=2022-08-01 |title=Four sub-Jovian-mass planets detected by high-cadence microlensing surveys |url=https://ui.adsabs.harvard.edu/abs/2022A&A...664A..33H |journal=Astronomy and Astrophysics |volume=664 |pages=A33 |doi=10.1051/0004-6361/202243484 |arxiv=2205.10510 |bibcode=2022A&A...664A..33H |issn=0004-6361}}</ref>
|-
|]
|0.26
|1.28
|
|
|
|2022<ref>{{Cite journal |last1=Zang |first1=Weicheng |last2=Shvartzvald |first2=Yossi |last3=Udalski |first3=Andrzej |last4=Yee |first4=Jennifer C. |last5=Lee |first5=Chung-Uk |last6=Sumi |first6=Takahiro |last7=Zhang |first7=Xiangyu |last8=Yang |first8=Hongjing |last9=Mao |first9=Shude |last10=Novati |first10=Sebastiano Calchi |last11=Gould |first11=Andrew |last12=Zhu |first12=Wei |last13=Beichman |first13=Charles A. |last14=Bryden |first14=Geoffery |last15=Carey |first15=Sean |date=2022-08-01 |title=OGLE-2018-BLG-0799Lb: a q 2.7 × 10-3 planet with Spitzer parallax |journal=Monthly Notices of the Royal Astronomical Society |volume=514 |issue=4 |pages=5952–5968 |doi=10.1093/mnras/stac1631 |doi-access=free |arxiv=2010.08732 |bibcode=2022MNRAS.514.5952Z |issn=0035-8711}}</ref>
|-
|OGLE-2018-BLG-0932Lb
|0.890
|1.75
|
|
|
|2022<ref name=":12" />
|-
|OGLE-2018-BLG-1212Lb
|0.20
|1.68
|
|
|
|2022<ref name=":12" />
|-
|OGLE-2016-BLG-1093Lb
|0.71
|2.13
|
|
|
|2022<ref>{{Cite journal |last1=Shin |first1=In-Gu |last2=Yee |first2=Jennifer C. |last3=Hwang |first3=Kyu-Ha |last4=Gould |first4=Andrew |last5=Udalski |first5=Andrzej |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Han |first9=Cheongho |last10=Kil Jung |first10=Youn |last11=Woo Kim |first11=Hyoun |last12=Ryu |first12=Yoon-Hyun |last13=Shvartzvald |first13=Yossi |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2022-06-01 |title=OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge |journal=The Astronomical Journal |volume=163 |issue=6 |pages=254 |doi=10.3847/1538-3881/ac6513 |doi-access=free |arxiv=2201.04312 |bibcode=2022AJ....163..254S |issn=0004-6256}}</ref>
|-
|OGLE-2014-BLG-0319Lb
|0.57
|3.49
|
|
|
|2022<ref>{{Cite journal |last1=Miyazaki |first1=Shota |last2=Suzuki |first2=Daisuke |last3=Udalski |first3=Andrzej |last4=Koshimoto |first4=Naoki |last5=Bennett |first5=David P. |last6=Sumi |first6=Takahiro |last7=Rattenbury |first7=Nicholas |last8=Cheongho |first8=Han |last9=Abe |first9=Fumio |last10=Barry |first10=Richard K. |last11=Bhattacharya |first11=Aparna |last12=Bond |first12=Ian A. |last13=Fukui |first13=Akihiko |last14=Fujii |first14=Hirosane |last15=Hirao |first15=Yuki |date=2022-03-01 |title=OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions |journal=The Astronomical Journal |volume=163 |issue=3 |pages=123 |doi=10.3847/1538-3881/ac4960 |doi-access=free |arxiv=2112.14997 |bibcode=2022AJ....163..123M |issn=0004-6256}}</ref>
|-
|MOA-2020-BLG-135Lb
|0.0356
|1.11
|
|
|
|2022<ref>{{Cite journal |last1=Ishitani Silva |first1=Stela |last2=Ranc |first2=Clément |last3=Bennett |first3=David P. |last4=Bond |first4=Ian A. |last5=Zang |first5=Weicheng |last6=Abe |first6=Fumio |last7=Barry |first7=Richard K. |last8=Bhattacharya |first8=Aparna |last9=Fujii |first9=Hirosane |last10=Fukui |first10=Akihiko |last11=Hirao |first11=Yuki |last12=Itow |first12=Yoshitaka |last13=Kirikawa |first13=Rintaro |last14=Kondo |first14=Iona |last15=Koshimoto |first15=Naoki |date=2022-09-01 |title=MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis |journal=The Astronomical Journal |volume=164 |issue=3 |pages=118 |doi=10.3847/1538-3881/ac82b8 |doi-access=free |arxiv=2204.03672 |bibcode=2022AJ....164..118I |issn=0004-6256}}</ref>
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|MOA-2019-BLG-008Lb
|18
|
|
|
|
|2022<ref>{{Cite journal |last1=Bachelet |first1=E. |last2=Tsapras |first2=Y. |last3=Gould |first3=Andrew |last4=Street |first4=R. A. |last5=Bennett |first5=David P. |last6=Hundertmark |first6=M. P. G. |last7=Bozza |first7=V. |last8=Bramich |first8=D. M. |last9=Cassan |first9=A. |last10=Dominik |first10=M. |last11=Horne |first11=K. |last12=Mao |first12=S. |last13=Saha |first13=A. |last14=Wambsganss |first14=J. |last15=Zang |first15=Weicheng |date=2022-09-01 |title=MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary |journal=The Astronomical Journal |volume=164 |issue=3 |pages=75 |doi=10.3847/1538-3881/ac78ed |doi-access=free |arxiv=2205.07522 |bibcode=2022AJ....164...75B |issn=0004-6256}}</ref>
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|KMT-2019-BLG-0253Lb |KMT-2019-BLG-0253Lb
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|2022<ref name=":11" /> |2022<ref name=":11" />
|-
|KMT-2021-BLG-2294Lb
|0.070
|1.15
|
|
|
|2022<ref name=":15">{{Cite journal |last1=Shin |first1=In-Gu |last2=Yee |first2=Jennifer C. |last3=Gould |first3=Andrew |last4=Hwang |first4=Kyu-Ha |last5=Yang |first5=Hongjing |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Han |first9=Cheongho |last10=Jung |first10=Youn Kil |last11=Ryu |first11=Yoon-Hyun |last12=Shvartzvald |first12=Yossi |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2023-01-01 |title=Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets |journal=The Astronomical Journal |volume=165 |issue=1 |pages=8 |doi=10.3847/1538-3881/ac9d93 |doi-access=free |arxiv=2209.03886 |bibcode=2023AJ....165....8S |issn=0004-6256}}</ref>
|-
|KMT-2021-BLG-1898Lb
|0.730
|1.9
|
|
|
|2022<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Kim |first3=Doeon |last4=Jung |first4=Youn Kil |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2022-07-01 |title=KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars |url=https://ui.adsabs.harvard.edu/abs/2022A&A...663A.145H |journal=Astronomy and Astrophysics |volume=663 |pages=A145 |doi=10.1051/0004-6361/202243102 |arxiv=2204.11378 |bibcode=2022A&A...663A.145H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-1689Lb
|0.14
|2.5
|
|
|
|2022<ref name=":16">{{Cite journal |last1=Yang |first1=Hongjing |last2=Zang |first2=Weicheng |last3=Gould |first3=Andrew |last4=Yee |first4=Jennifer C. |last5=Hwang |first5=Kyu-Ha |last6=Christie |first6=Grant |last7=Sumi |first7=Takahiro |last8=Zhang |first8=Jiyuan |last9=Mao |first9=Shude |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Han |first12=Cheongho |last13=Jung |first13=Youn Kil |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |date=2022-10-01 |title=KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |issue=2 |pages=1894–1909 |doi=10.1093/mnras/stac2023 |doi-access=free |arxiv=2205.12584 |bibcode=2022MNRAS.516.1894Y |issn=0035-8711}}</ref>
|-
|KMT-2021-BLG-0119Lb
|5.52
|2.92
|
|
|
|2022<ref name=":15" />
|-
|KMT-2021-BLG-0192Lb
|0.11
|1.62
|
|
|
|2022<ref name=":15" />
|-
|KMT-2021-BLG-0171Lb
|0.0352
|3.5
|
|
|
|2022<ref name=":16" />
|-
|KMT-2021-BLG-1303Lb
|0.38
|2.89
|
|
|
|2022<ref name=":14" />
|-
|KMT-2021-BLG-0320Lb
|0.10
|1.54
|
|
|
|2022<ref name=":14" />
|-
|KMT-2021-BLG-1554Lb
|0.12
|0.72
|
|
|
|2022<ref name=":14" />
|-
|KMT-2021-BLG-1391Lb
|0.0143
|2.29
|
|
|
|2022<ref name=":17">{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Kil Jung |first2=Youn |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2022-11-01 |title=Mass Production of 2021 KMTNet Microlensing Planets. I |journal=The Astronomical Journal |volume=164 |issue=5 |pages=180 |doi=10.3847/1538-3881/ac8d6c |doi-access=free |arxiv=2202.03022 |bibcode=2022AJ....164..180R |issn=0004-6256}}</ref>
|-
|KMT-2021-BLG-1372Lb
|0.1928
|2.37
|
|
|
|2022<ref name=":17" />
|-
|KMT-2021-BLG-1253Lb
|0.05994
|1.52
|
|
|
|2022<ref name=":17" />
|- |-
|KMT-2019-BLG-0953Lb |KMT-2019-BLG-0953Lb
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|2022<ref name=":11" /> |2022<ref name=":11" />
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|KMT-2021-BLG-0748Lb
|0.45
|2.43
|
|
|
|2022<ref name=":17" />
|- bgcolor="#ffffb0" |- bgcolor="#ffffb0"
|KMT-2021-BLG-1077Lb |KMT-2021-BLG-1077Lb
Line 794: Line 1,018:
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| |
|2022<ref name=":6">{{Cite journal |last=Han |first=Cheongho |last2=Gould |first2=Andrew |last3=Bond |first3=Ian A. |last4=Kil Jung |first4=Youn |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Ryu |first8=Yoon-Hyun |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2022-06-01 |title=KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing |url=https://ui.adsabs.harvard.edu/abs/2022A&A...662A..70H |journal=Astronomy and Astrophysics |volume=662 |pages=A70 |doi=10.1051/0004-6361/202243550 |issn=0004-6361}}</ref> |2022<ref name=":6">{{Cite journal |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Bond |first3=Ian A. |last4=Kil Jung |first4=Youn |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Ryu |first8=Yoon-Hyun |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2022-06-01 |title=KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing |url=https://ui.adsabs.harvard.edu/abs/2022A&A...662A..70H |journal=Astronomy and Astrophysics |volume=662 |pages=A70 |doi=10.1051/0004-6361/202243550 |arxiv=2203.16734 |bibcode=2022A&A...662A..70H |issn=0004-6361}}</ref>
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|KMT-2021-BLG-1077Lc |KMT-2021-BLG-1077Lc
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|2022<ref name=":6" /> |2022<ref name=":6" />
|-
|KMT-2021-BLG-0912Lb
|0.00884
|3.14
|
|
|
|2022<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Bond |first2=Ian A. |last3=Yee |first3=Jennifer C. |last4=Zang |first4=Weicheng |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Gould |first7=Andrew P. |last8=Hwang |first8=Kyu-Ha |last9=Jung |first9=Youn Kil |last10=Kim |first10=Doeon |last11=Lee |first11=Chung-Uk |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Cha |first15=Sang-Mok |date=2022-02-01 |title=KMT-2021-BLG-0912Lb: a microlensing super Earth around a K-type star |url=https://ui.adsabs.harvard.edu/abs/2022A&A...658A..94H |journal=Astronomy and Astrophysics |volume=658 |pages=A94 |doi=10.1051/0004-6361/202142495 |arxiv=2111.04861 |bibcode=2022A&A...658A..94H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-0240Lb
|0.21
|2.8
|
|
|
|2022<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |last5=Jung |first5=Youn Kil |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2022-08-01 |title=KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal |url=https://ui.adsabs.harvard.edu/abs/2022A&A...664A.114H |journal=Astronomy and Astrophysics |volume=664 |pages=A114 |doi=10.1051/0004-6361/202243161 |arxiv=2204.11383 |bibcode=2022A&A...664A.114H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-2974Lb
|0.28
|2.0
|
|
|
|2022<ref name=":18">{{Cite journal |last1=Zang |first1=Weicheng |last2=Yang |first2=Hongjing |last3=Han |first3=Cheongho |last4=Lee |first4=Chung-Uk |last5=Udalski |first5=Andrzej |last6=Gould |first6=Andrew |last7=Mao |first7=Shude |last8=Zhang |first8=Xiangyu |last9=Zhu |first9=Wei |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Hwang |first12=Kyu-Ha |last13=Jung |first13=Youn Kil |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |date=2022-09-01 |title=Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field |journal=Monthly Notices of the Royal Astronomical Society |volume=515 |issue=1 |pages=928–939 |doi=10.1093/mnras/stac1883 |doi-access=free |arxiv=2204.02017 |bibcode=2022MNRAS.515..928Z |issn=0035-8711}}</ref>
|-
|KMT-2019-BLG-1552Lb
|4.05
|2.6
|
|
|
|2022<ref name=":18" />
|-
|KMT-2019-BLG-1042Lb
|0.19
|1.7
|
|
|
|2022<ref name=":18" />
|-
|KMT-2018-BLG-1988Lb
|0.0175
|3.09
|
|
|
|2022<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Albrow |first3=Michael D. |last4=Chung |first4=Sun-Ju |last5=Hwang |first5=Kyu-Ha |last6=Kil Jung |first6=Youn |last7=Kim |first7=Doeon |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2022-02-01 |title=KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf |url=https://ui.adsabs.harvard.edu/abs/2022A&A...658A..62H |journal=Astronomy and Astrophysics |volume=658 |pages=A62 |doi=10.1051/0004-6361/202142077 |arxiv=2111.08955 |bibcode=2022A&A...658A..62H |issn=0004-6361}}</ref>
|-
|KMT-2019-BLG-0414Lb
|4.57
|1.16
|
|
|
|2022<ref name=":19">{{Cite journal |last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Gould |first3=Andrew |last4=Jung |first4=Youn Kil |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Kim |first8=Doeon |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2022-10-01 |title=KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey |url=https://ui.adsabs.harvard.edu/abs/2022A&A...666A.132H |journal=Astronomy and Astrophysics |volume=666 |pages=A132 |doi=10.1051/0004-6361/202244438 |arxiv=2209.00112 |bibcode=2022A&A...666A.132H |issn=0004-6361}}</ref>
|-
|KMT-2017-BLG-0673Lb
|3.67
|2.34
|
|
|
|2022<ref name=":19" />
|-
|KMT-2018-BLG-0087Lb
|0.23
|0.870
|
|
|
|2022<ref name=":13" />
|-
|KMT-2018-BLG-0030Lb
|1.45
|4.39
|
|
|
|2022<ref name=":13" />
|-
|KMT-2018-BLG-0247Lb
|2.11
|2.46
|
|
|
|2022<ref name=":13" />
|-
|KMT-2018-BLG-2602Lb
|1.15
|3.81
|
|
|
|2022<ref name=":13" />
|-
|OGLE-2019-BLG-1180Lb
|1.747
|5.19
|
|
|
|2023<ref>{{Cite journal |last1=Chung |first1=Sun-Ju |last2=Udalski |first2=Andrzej |last3=Yee |first3=Jennifer C. |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Han |first8=Cheongho |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2023-12-01 |title=OGLE-2019-BLG-1180Lb: Discovery of a Wide-orbit Jupiter-mass Planet around a Late-type Star |journal=The Astronomical Journal |volume=166 |issue=6 |pages=253 |doi=10.3847/1538-3881/ad0723 |doi-access=free |arxiv=2312.01278 |bibcode=2023AJ....166..253C |issn=0004-6256}}</ref>
|-
|OGLE-2019-BLG-0679Lb
|3.34
|6.99
|
|
|
|2023<ref name=":20">{{Cite journal |last1=Jung |first1=Youn Kil |last2=Zang |first2=Weicheng |last3=Wang |first3=Hanyue |last4=Han |first4=Cheongho |last5=Gould |first5=Andrew |last6=Udalski |first6=Andrzej |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yang |first13=Hongjing |last14=Yee |first14=Jennifer C. |last15=Cha |first15=Sang-Mok |date=2023-06-01 |title=Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets |journal=The Astronomical Journal |volume=165 |issue=6 |pages=226 |doi=10.3847/1538-3881/accb8f |doi-access=free |arxiv=2302.13544 |bibcode=2023AJ....165..226J |issn=0004-6256}}</ref>
|-
|OGLE-2019-BLG-0249Lb
|7.12
|1.84
|
|
|
|2023<ref name=":20" />
|-
|OGLE-2017-BLG-1806Lb
|0.0166
|1.75
|
|
|
|2023<ref name=":21">{{Cite journal |last1=Zang |first1=Weicheng |last2=Jung |first2=Youn Kil |last3=Yang |first3=Hongjing |last4=Zhang |first4=Xiangyu |last5=Udalski |first5=Andrzej |last6=Yee |first6=Jennifer C. |last7=Gould |first7=Andrew |last8=Mao |first8=Shude |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Han |first11=Cheongho |last12=Hwang |first12=Kyu-Ha |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Shvartzvald |first15=Yossi |date=2023-03-01 |title=Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10-4 Planets from the First 4 yr Survey |journal=The Astronomical Journal |volume=165 |issue=3 |pages=103 |doi=10.3847/1538-3881/acb34b |doi-access=free |arxiv=2210.12344 |bibcode=2023AJ....165..103Z |issn=0004-6256}}</ref>
|-
|MOA-2022-BLG-249Lb
|0.0152
|1.63
|
|
|
|2023<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Jung |first3=Youn Kil |last4=Bond |first4=Ian A. |last5=Zang |first5=Weicheng |last6=Chung |first6=Sun-Ju |last7=Albrow |first7=Michael D. |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Doeon |date=2023-06-01 |title=MOA-2022-BLG-249Lb: Nearby microlensing super-Earth planet detected from high-cadence surveys |url=https://ui.adsabs.harvard.edu/abs/2023A&A...674A..89H |journal=Astronomy and Astrophysics |volume=674 |pages=A89 |doi=10.1051/0004-6361/202346166 |arxiv=2304.02815 |bibcode=2023A&A...674A..89H |issn=0004-6361}}</ref>
|-
|MOA-2020-BLG-208Lb
|0.14
|2.74
|
|
|
|2023<ref>{{Cite journal |last1=Olmschenk |first1=Greg |last2=Bennett |first2=David P. |last3=Bond |first3=Ian A. |last4=Zang |first4=Weicheng |last5=Jung |first5=Youn Kil |last6=Yee |first6=Jennifer C. |last7=Bachelet |first7=Etienne |last8=Abe |first8=Fumio |last9=Barry |first9=Richard K. |last10=Bhattacharya |first10=Aparna |last11=Fujii |first11=Hirosane |last12=Fukui |first12=Akihiko |last13=Hirao |first13=Yuki |last14=Silva |first14=Stela Ishitani |last15=Itow |first15=Yoshitaka |date=2023-04-01 |title=MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert |journal=The Astronomical Journal |volume=165 |issue=4 |pages=175 |doi=10.3847/1538-3881/acbcc8 |doi-access=free |arxiv=2210.02436 |bibcode=2023AJ....165..175O |issn=0004-6256}}</ref>
|-
|KMT-2022-BLG-1013Lb
|0.31
|1.38
|
|
|
|2023<ref name=":22">{{Cite journal |last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Zang |first3=Weicheng |last4=Jung |first4=Youn Kil |last5=Christie |first5=Grant W. |last6=Zhang |first6=Jiyuan |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Kim |first11=Doeon |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yang |first15=Hongjing |date=2023-06-01 |title=KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals |url=https://ui.adsabs.harvard.edu/abs/2023A&A...674A..90H |journal=Astronomy and Astrophysics |volume=674 |pages=A90 |doi=10.1051/0004-6361/202346298 |arxiv=2304.03871 |bibcode=2023A&A...674A..90H |issn=0004-6361}}</ref>
|-
|KMT-2022-BLG-0440Lb
|0.0485
|1.9
|
|
|
|2023<ref>{{Cite journal |last1=Zhang |first1=Jiyuan |last2=Zang |first2=Weicheng |last3=Jung |first3=Youn Kil |last4=Yang |first4=Hongjing |last5=Gould |first5=Andrew |last6=Sumi |first6=Takahiro |last7=Mao |first7=Shude |last8=Dong |first8=Subo |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Han |first11=Cheongho |last12=Hwang |first12=Kyu-Ha |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Shvartzvald |first15=Yossi |date=2023-07-01 |title=KMT-2022-BLG-0440Lb: A new q < 10-4 microlensing planet with the central-resonant caustic degeneracy broken |journal=Monthly Notices of the Royal Astronomical Society |volume=522 |issue=4 |pages=6055–6069 |doi=10.1093/mnras/stad1398 |doi-access=free |arxiv=2301.06779 |bibcode=2023MNRAS.522.6055Z |issn=0035-8711}}</ref>
|-
|KMT-2022-BLG-0371Lb
|0.26
|3.02
|
|
|
|2023<ref name=":22" />
|-
|KMT-2021-BLG-2478Lb
|0.900
|1.85
|
|
|
|2023<ref name=":23">{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Shin |first2=In-Gu |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |last9=Kil Jung |first9=Youn |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |date=2023-03-01 |title=Mass Production of 2021 KMTNet Microlensing Planets II |journal=The Astronomical Journal |volume=165 |issue=3 |pages=83 |doi=10.3847/1538-3881/acab6b |doi-access=free |arxiv=2207.07295 |bibcode=2023AJ....165...83R |issn=0004-6256}}</ref>
|-
|KMT-2021-BLG-2010Lb
|1.07
|1.79
|
|
|
|2023<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Zang |first3=Weicheng |last4=Jung |first4=Youn Kil |last5=Christie |first5=Grant W. |last6=Zhang |first6=Jiyuan |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Kim |first11=Doeon |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yang |first15=Hongjing |date=2023-06-01 |title=KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals |url=https://ui.adsabs.harvard.edu/abs/2023A&A...674A..90H |journal=Astronomy and Astrophysics |volume=674 |pages=A90 |doi=10.1051/0004-6361/202346298 |arxiv=2304.03871 |bibcode=2023A&A...674A..90H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-1770Lb
|21
|0.900
|
|
|
|2023<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Jung |first2=Youn Kil |last3=Bond |first3=Ian A. |last4=Chung |first4=Sun-Ju |last5=Albrow |first5=Michael D. |last6=Gould |first6=Andrew |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2023-10-01 |title=Brown dwarf companions in binaries detected in the 2021 season high-cadence microlensing surveys |url=https://ui.adsabs.harvard.edu/abs/2023A&A...678A.190H |journal=Astronomy and Astrophysics |volume=678 |pages=A190 |doi=10.1051/0004-6361/202347014 |arxiv=2307.04921 |bibcode=2023A&A...678A.190H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-1547Lb
|1.47
|4.5
|
|
|
|2023<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Zang |first2=Weicheng |last3=Jung |first3=Youn Kil |last4=Bond |first4=Ian A. |last5=Chung |first5=Sun-Ju |last6=Albrow |first6=Michael D. |last7=Gould |first7=Andrew |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Doeon |date=2023-10-01 |title=KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity |url=https://ui.adsabs.harvard.edu/abs/2023A&A...678A.101H |journal=Astronomy and Astrophysics |volume=678 |pages=A101 |doi=10.1051/0004-6361/202347366 |arxiv=2309.01280 |bibcode=2023A&A...678A.101H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-1150Lb
|0.880
|4.5
|
|
|
|2023<ref>{{Cite journal |last1=Han |first1=Cheongho |last2=Jung |first2=Youn Kil |last3=Bond |first3=Ian A. |last4=Gould |first4=Andrew |last5=Chung |first5=Sun-Ju |last6=Albrow |first6=Michael D. |last7=Hwang |first7=Kyu-Ha |last8=Ryu |first8=Yoon-Hyun |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yang |first11=Hongjing |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Doeon |date=2023-07-01 |title=KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal |url=https://ui.adsabs.harvard.edu/abs/2023A&A...675A..36H |journal=Astronomy and Astrophysics |volume=675 |pages=A36 |doi=10.1051/0004-6361/202346596 |arxiv=2305.15628 |bibcode=2023A&A...675A..36H |issn=0004-6361}}</ref>
|-
|KMT-2021-BLG-1105Lb
|1.30
|3.54
|
|
|
|2023<ref name=":23" />
|-
|KMT-2021-BLG-0909Lb
|1.26
|1.75
|
|
|
|2023<ref name=":23" />
|-
|KMT-2021-BLG-0712Lb
|0.1202
|2.22
|
|
|
|2023<ref name=":23" />
|-
|KMT-2019-BLG-2783Lb
|1.16
|1.85
|
|
|
|2023<ref name=":20" />
|-
|KMT-2019-BLG-1806Lb
|0.0147
|3.02
|
|
|
|2023<ref name=":21" />
|-
|KMT-2019-BLG-1367Lb
|0.0128
|1.70
|
|
|
|2023<ref name=":21" />
|-
|KMT-2019-BLG-1216Lb
|0.0940
|2.44
|
|
|
|2023<ref name=":20" />
|-
|KMT-2019-BLG-0335Lb
|21
|1.64
|
|
|
|2023<ref name=":24">{{Cite journal |last1=Han |first1=Cheongho |last2=Kil Jung |first2=Youn |last3=Kim |first3=Doeon |last4=Gould |first4=Andrew |last5=Bozza |first5=Valerio |last6=Bond |first6=Ian A. |last7=Chung |first7=Sun-Ju |last8=Albrow |first8=Michael D. |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yang |first13=Hongjing |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |date=2023-07-01 |title=Probable brown dwarf companions detected in binary microlensing events during the 2018-2020 seasons of the KMTNet survey |url=https://ui.adsabs.harvard.edu/abs/2023A&A...675A..71H |journal=Astronomy and Astrophysics |volume=675 |pages=A71 |doi=10.1051/0004-6361/202245455 |arxiv=2305.06605 |bibcode=2023A&A...675A..71H |issn=0004-6361}}</ref>
|-
|KMT-2019-BLG-0298Lb
|1.81
|5.67
|
|
|
|2023<ref name=":20" />
|-
|KMT-2019-BLG-0297Lb
|19
|0.960
|
|
|
|2023<ref name=":24" />
|-
|KMT-2018-BLG-0885Lb
|29
|1.07
|
|
|
|2023<ref name=":24" />
|-
|KMT-2017-BLG-1194Lb
|0.0111
|1.78
|
|
|
|2023<ref name=":21" />
|-
|KMT-2017-BLG-1003Lb
|0.01633
|1.38
|
|
|
|2023<ref name=":21" />
|-
|KMT-2017-BLG-0428Lb
|0.0176
|1.81
|
|
|
|2023<ref name=":21" />
|-
|KMT-2016-BLG-1105Lb
|0.00730
|2.44
|
|
|
|2023<ref name=":21" />
|-
|]
|1.10
|4.16
|4700
|
|
|2023<ref>{{Cite journal |last1=Specht |first1=D. |last2=Poleski |first2=R. |last3=Penny |first3=M. T. |last4=Kerins |first4=E. |last5=McDonald |first5=I. |last6=Lee |first6=Chung-Uk |last7=Udalski |first7=A. |last8=Bond |first8=I. A. |last9=Shvartzvald |first9=Y. |last10=Zang |first10=Weicheng |last11=Street |first11=R. A. |last12=Hogg |first12=D. W. |last13=Gaudi |first13=B. S. |last14=Barclay |first14=T. |last15=Barentsen |first15=G. |date=2023-04-01 |title=Kepler K2 Campaign 9 - II. First space-based discovery of an exoplanet using microlensing |journal=Monthly Notices of the Royal Astronomical Society |volume=520 |issue=4 |pages=6350–6366 |doi=10.1093/mnras/stad212 |doi-access=free |arxiv=2203.16959 |bibcode=2023MNRAS.520.6350S |issn=0035-8711}}</ref>
|-
|OGLE-2017-BLG-1275Lb
|5.90
|2.09
|
|
|
|2024<ref name=":25">{{Cite journal |last1=Ryu |first1=Yoon-Hyun |last2=Udalski |first2=Andrzej |last3=Yee |first3=Jennifer C. |last4=Zang |first4=Weicheng |last5=Shvartzvald |first5=Yossi |last6=Han |first6=Cheongho |last7=Gould |first7=Andrew |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Hwang |first10=Kyu-Ha |last11=Jung |first11=Youn Kil |last12=Shin |first12=In-Gu |last13=Yang |first13=Hongjing |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |date=2024-03-01 |title=Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets |journal=The Astronomical Journal |volume=167 |issue=3 |pages=88 |doi=10.3847/1538-3881/ad1888 |doi-access=free |arxiv=2307.13359 |bibcode=2024AJ....167...88R |issn=0004-6256}}</ref>
|-
|OGLE-2017-BLG-1237Lb
|3.80
|2.53
|
|
|
|2024<ref name=":25" />
|-
|OGLE-2017-BLG-0640Lb
|1.62
|1.14
|
|
|
|2024<ref name=":25" />
|} |}


Line 910: Line 1,494:
<ref name="Furusawa2013">{{cite journal|title=MOA-2010-BLG-328Lb: A Sub-Neptune Orbiting very Late M Dwarf?|first1=K.|last1=Furusawa|first2=A.|last2=Udalski|first3=T.|last3=Sumi|first4=D. P.|last4=Bennett|first5=I. A.|last5=Bond|first6=A.|last6=Gould|first7=U. G.|last7=Jørgensen|first8=C.|last8=Snodgrass|first9=D. Dominis|last9=Prester|first10=M. D.|last10=Albrow|first11=F.|last11=Abe|first12=C. S.|last12=Botzler|first13=P.|last13=Chote|first14=M.|last14=Freeman|first15=A.|last15=Fukui|first16=P.|last16=Harris|first17=Y.|last17=Itow|first18=C. H.|last18=Ling|first19=K.|last19=Masuda|first20=Y.|last20=Matsubara|first21=N.|last21=Miyake|first22=Y.|last22=Muraki|first23=K.|last23=Ohnishi|first24=N. J.|last24=Rattenbury|first25=To|last25=Saito|first26=D. J.|last26=Sullivan|first27=D.|last27=Suzuki|first28=W. L.|last28=Sweatman|first29=P. J.|last29=Tristram|first30=K.|last30=Wada|first31=P. C. M.|last31=Yock|first32=The MOA|last32=Collaboration|first33=M. K.|last33=Szymański|first34=I.|last34=Soszyński|first35=M.|last35=Kubiak|first36=R.|last36=Poleski|first37=K.|last37=Ulaczyk|first38=G.|last38=Pietrzyński|first39=Ł|last39=Wyrzykowski|first40=The OGLE|last40=Collaboration|first41=J.-Y.|last41=Choi|first42=G. W.|last42=Christie|first43=D. L.|last43=DePoy|first44=Subo|last44=Dong|first45=J.|last45=Drummond|first46=B. S.|last46=Gaudi|first47=C.|last47=Han|last48=L.-W. Hung|first49=K.-H.|last49=Hwang|first50=C.-U.|last50=Lee|first51=J.|last51=McCormick|first52=D.|last52=Moorhouse|first53=T.|last53=Natusch|first54=M.|last54=Nola|first55=E.|last55=Ofek|first56=R. W.|last56=Pogge|last57=I.-G. Shin|first58=J.|last58=Skowron|first59=G.|last59=Thornley|first60=J. C.|last60=Yee|first61=The μFUN|last61=Collaboration|first62=K. A.|last62=Alsubai|first63=V.|last63=Bozza|first64=P.|last64=Browne|first65=M. J.|last65=Burgdorf|first66=S. Calchi|last66=Novati|first67=P.|last67=Dodds|first68=M.|last68=Dominik|first69=F.|last69=Finet|first70=T.|last70=Gerner|first71=S.|last71=Hardis|first72=K.|last72=Harpsøe|first73=T. C.|last73=Hinse|last74=M. Hundertmark|first75=N.|last75=Kains|first76=E.|last76=Kerins|first77=C.|last77=Liebig|first78=L.|last78=Mancini|first79=M.|last79=Mathiasen|first80=M. T.|last80=Penny|first81=S.|last81=Proft|first82=S.|last82=Rahvar|last83=D. Ricci|first84=G.|last84=Scarpetta|first85=S.|last85=Schäfer|first86=F.|last86=Schönebeck|first87=J.|last87=Southworth|first88=J.|last88=Surdej|first89=J.|last89=Wambsganss|first90=The MiNDSTEp|last90=Consortium|first91=R. A.|last91=Street|first92=D. M.|last92=Bramich|first93=I. A.|last93=Steele|first94=Y.|last94=Tsapras|first95=The RoboNet|last95=Collaboration|first96=K.|last96=Horne|last97=J. Donatowicz|first98=K. C.|last98=Sahu|first99=E.|last99=Bachelet|first100=V.|last100=Batista|first101=T. G.|last101=Beatty|first102=J.-P.|last102=Beaulieu|first103=C. S.|last103=Bennett|first104=C.|last104=Black|last105=R. Bowens-Rubin|first106=S.|last106=Brillant|first107=J. A. R.|last107=Caldwell|first108=A.|last108=Cassan|first109=A. A.|last109=Cole|first110=E.|last110=Corrales|first111=C.|last111=Coutures|last112=S. Dieters|first113=P.|last113=Fouqué|first114=J.|last114=Greenhill|first115=C. B.|last115=Henderson|first116=D.|last116=Kubas|first117=J.-B.|last117=Marquette|first118=R.|last118=Martin|first119=J. W.|last119=Menzies|last120=B. Shappee|first121=A.|last121=Williams|first122=D.|last122=Wouters|first123=J. van|last123=Saders|first124=R.|last124=Zellem|first125=M.|last125=Zub|first126=The PLANET|last126=Collaboration|date=23 April 2018|journal=The Astrophysical Journal|volume=779|issue=2|pages=91|doi=10.1088/0004-637X/779/2/91|arxiv=1309.7714|bibcode=2013ApJ...779...91F|s2cid=59519570|display-authors=29}}</ref> <ref name="Furusawa2013">{{cite journal|title=MOA-2010-BLG-328Lb: A Sub-Neptune Orbiting very Late M Dwarf?|first1=K.|last1=Furusawa|first2=A.|last2=Udalski|first3=T.|last3=Sumi|first4=D. P.|last4=Bennett|first5=I. A.|last5=Bond|first6=A.|last6=Gould|first7=U. G.|last7=Jørgensen|first8=C.|last8=Snodgrass|first9=D. Dominis|last9=Prester|first10=M. D.|last10=Albrow|first11=F.|last11=Abe|first12=C. S.|last12=Botzler|first13=P.|last13=Chote|first14=M.|last14=Freeman|first15=A.|last15=Fukui|first16=P.|last16=Harris|first17=Y.|last17=Itow|first18=C. H.|last18=Ling|first19=K.|last19=Masuda|first20=Y.|last20=Matsubara|first21=N.|last21=Miyake|first22=Y.|last22=Muraki|first23=K.|last23=Ohnishi|first24=N. J.|last24=Rattenbury|first25=To|last25=Saito|first26=D. J.|last26=Sullivan|first27=D.|last27=Suzuki|first28=W. L.|last28=Sweatman|first29=P. J.|last29=Tristram|first30=K.|last30=Wada|first31=P. C. M.|last31=Yock|first32=The MOA|last32=Collaboration|first33=M. K.|last33=Szymański|first34=I.|last34=Soszyński|first35=M.|last35=Kubiak|first36=R.|last36=Poleski|first37=K.|last37=Ulaczyk|first38=G.|last38=Pietrzyński|first39=Ł|last39=Wyrzykowski|first40=The OGLE|last40=Collaboration|first41=J.-Y.|last41=Choi|first42=G. W.|last42=Christie|first43=D. L.|last43=DePoy|first44=Subo|last44=Dong|first45=J.|last45=Drummond|first46=B. S.|last46=Gaudi|first47=C.|last47=Han|last48=L.-W. Hung|first49=K.-H.|last49=Hwang|first50=C.-U.|last50=Lee|first51=J.|last51=McCormick|first52=D.|last52=Moorhouse|first53=T.|last53=Natusch|first54=M.|last54=Nola|first55=E.|last55=Ofek|first56=R. W.|last56=Pogge|last57=I.-G. Shin|first58=J.|last58=Skowron|first59=G.|last59=Thornley|first60=J. C.|last60=Yee|first61=The μFUN|last61=Collaboration|first62=K. A.|last62=Alsubai|first63=V.|last63=Bozza|first64=P.|last64=Browne|first65=M. J.|last65=Burgdorf|first66=S. Calchi|last66=Novati|first67=P.|last67=Dodds|first68=M.|last68=Dominik|first69=F.|last69=Finet|first70=T.|last70=Gerner|first71=S.|last71=Hardis|first72=K.|last72=Harpsøe|first73=T. C.|last73=Hinse|last74=M. Hundertmark|first75=N.|last75=Kains|first76=E.|last76=Kerins|first77=C.|last77=Liebig|first78=L.|last78=Mancini|first79=M.|last79=Mathiasen|first80=M. T.|last80=Penny|first81=S.|last81=Proft|first82=S.|last82=Rahvar|last83=D. Ricci|first84=G.|last84=Scarpetta|first85=S.|last85=Schäfer|first86=F.|last86=Schönebeck|first87=J.|last87=Southworth|first88=J.|last88=Surdej|first89=J.|last89=Wambsganss|first90=The MiNDSTEp|last90=Consortium|first91=R. A.|last91=Street|first92=D. M.|last92=Bramich|first93=I. A.|last93=Steele|first94=Y.|last94=Tsapras|first95=The RoboNet|last95=Collaboration|first96=K.|last96=Horne|last97=J. Donatowicz|first98=K. C.|last98=Sahu|first99=E.|last99=Bachelet|first100=V.|last100=Batista|first101=T. G.|last101=Beatty|first102=J.-P.|last102=Beaulieu|first103=C. S.|last103=Bennett|first104=C.|last104=Black|last105=R. Bowens-Rubin|first106=S.|last106=Brillant|first107=J. A. R.|last107=Caldwell|first108=A.|last108=Cassan|first109=A. A.|last109=Cole|first110=E.|last110=Corrales|first111=C.|last111=Coutures|last112=S. Dieters|first113=P.|last113=Fouqué|first114=J.|last114=Greenhill|first115=C. B.|last115=Henderson|first116=D.|last116=Kubas|first117=J.-B.|last117=Marquette|first118=R.|last118=Martin|first119=J. W.|last119=Menzies|last120=B. Shappee|first121=A.|last121=Williams|first122=D.|last122=Wouters|first123=J. van|last123=Saders|first124=R.|last124=Zellem|first125=M.|last125=Zub|first126=The PLANET|last126=Collaboration|date=23 April 2018|journal=The Astrophysical Journal|volume=779|issue=2|pages=91|doi=10.1088/0004-637X/779/2/91|arxiv=1309.7714|bibcode=2013ApJ...779...91F|s2cid=59519570|display-authors=29}}</ref>


<ref name="Shvartzvald2014">{{cite journal |arxiv=1310.0008|doi=10.1093/mnras/stt2477 |title=MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet |year=2014 |last1=Shvartzvald |first1=Y. |last2=Maoz |first2=D. |last3=Kaspi |first3=S. |last4=Sumi |first4=T. |last5=Udalski |first5=A. |last6=Gould |first6=A. |last7=Bennett |first7=D. P. |last8=Han |first8=C. |last9=Abe |first9=F. |last10=Bond |first10=I. A. |last11=Botzler |first11=C. S. |last12=Freeman |first12=M. |last13=Fukui |first13=A. |last14=Fukunaga |first14=D. |last15=Itow |first15=Y. |last16=Koshimoto |first16=N. |last17=Ling |first17=C. H. |last18=Masuda |first18=K. |last19=Matsubara |first19=Y. |last20=Muraki |first20=Y. |last21=Namba |first21=S. |last22=Ohnishi |first22=K. |last23=Rattenbury |first23=N. J. |last24=Saito |first24=To. |last25=Sullivan |first25=D. J. |last26=Sweatman |first26=W. L. |last27=Suzuki |first27=D. |last28=Tristram |first28=P. J. |last29=Wada |first29=K. |last30=Yock |first30=P. C. M. |journal=Monthly Notices of the Royal Astronomical Society |volume=439 |pages=604–610 |display-authors=1 }}</ref> <ref name="Shvartzvald2014">{{cite journal |arxiv=1310.0008|doi=10.1093/mnras/stt2477 |title=MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet |year=2014 |last1=Shvartzvald |first1=Y. |last2=Maoz |first2=D. |last3=Kaspi |first3=S. |last4=Sumi |first4=T. |last5=Udalski |first5=A. |last6=Gould |first6=A. |last7=Bennett |first7=D. P. |last8=Han |first8=C. |last9=Abe |first9=F. |last10=Bond |first10=I. A. |last11=Botzler |first11=C. S. |last12=Freeman |first12=M. |last13=Fukui |first13=A. |last14=Fukunaga |first14=D. |last15=Itow |first15=Y. |last16=Koshimoto |first16=N. |last17=Ling |first17=C. H. |last18=Masuda |first18=K. |last19=Matsubara |first19=Y. |last20=Muraki |first20=Y. |last21=Namba |first21=S. |last22=Ohnishi |first22=K. |last23=Rattenbury |first23=N. J. |last24=Saito |first24=To. |last25=Sullivan |first25=D. J. |last26=Sweatman |first26=W. L. |last27=Suzuki |first27=D. |last28=Tristram |first28=P. J. |last29=Wada |first29=K. |last30=Yock |first30=P. C. M. |journal=Monthly Notices of the Royal Astronomical Society |volume=439 |pages=604–610 |doi-access=free |display-authors=1 }}</ref>


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Latest revision as of 20:13, 9 December 2024

This article needs to be updated. Please help update this article to reflect recent events or newly available information. (August 2014)

This is a list of exoplanets detected by gravitational microlensing. The phenomenon results in the background star's light being warped around a foreground object, causing a distorted image. If the foreground object is a star with an orbiting planet, we would observe an abnormally bright image. By comparing the luminosity and light distortion of the background star to theoretical models, we can estimate the planet's mass and the distance from its star.

The least massive planet detected by microlensing is KMT-2020-BLG-0414Lb, which has a mass about 1.9 times the mass of earth, or OGLE-2013-BLG-0341LBb, which has a mass about 2 times the mass of earth. The widest separation between a planet and a star is OGLE-2008-BLG-092Lb, which is ~18 AU; the shortest separation is MOA-2015-BLG-337Lb, which is 0.24 AU. There are 7 known multi-planetary systems detected by microlensing, all of which have two planets.

List

Yellow rows denote the members of multi-planet systems. Green rows denote the members of multi-star systems.

Planet Mass (MJ) Projected separation (AU) Period (d) Eccentricity Inclination (°) Year of discovery
OGLE-2003-BLG-235Lb 2.6 5.1 2004
OGLE-2005-BLG-071Lb 3.5 3.6 ~ 3600 2005
OGLE-2005-BLG-390Lb 0.017 2.1 3500 2005
OGLE-2005-BLG-169Lb 0.04 2.8 3300 2006
OGLE-2006-BLG-109Lb 0.727 2.3 1790 64 2008
OGLE-2006-BLG-109Lc 0.271 4.5 4931 0.15 64 2008
MOA-2007-BLG-192Lb 0.01 0.66 2008
MOA-2007-BLG-400Lb 0.9 0.85 2008
MOA-2008-BLG-310Lb 0.23 1.25 2009
OGLE-2007-BLG-368Lb 0.0694 3.3 2009
MOA-2009-BLG-319Lb 0.157 2.0 2010
MOA-2009-BLG-387Lb 2.6 1.8 1970 2011
MOA-2009-BLG-266Lb 0.0327 3.2 2780 2011
MOA-2011-BLG-293Lb 2.4 1.0 2012
MOA-bin-1Lb 3.7 8.3 2012
MOA-2010-BLG-477Lb 1.5 2±1 2012
OGLE-2012-BLG-0026Lb 0.11 3.82 ~3000 2012
OGLE-2012-BLG-0026Lc 0.68 4.63 ~4000 2012
MOA-2010-BLG-073Lb 11 1.21 2012
OGLE-2011-BLG-0251Lb 0.53±0.21 2.72±0.75 or 1.5±0.5 2013
OGLE-2012-BLG-0406Lb 2.73±0.43 3.45±0.26 2013
OGLE-2012-BLG-0358Lb 1.9±0.2 0.87 2013
MOA-2010-BLG-328Lb 0.03 ± 0.0075 0.92 2013
MOA-2011-BLG-322Lb 11.6 4.3 2013
MOA-2008-BLG-379Lb 5±2.5 4±1.6 2013
MOA-2011-BLG-262Lb ~0.053 or ~0.0015 ~0.95 or ~0.13 2013
MOA-2013-BLG-220Lb 2.74 3.03 2014
OGLE-2008-BLG-355Lb 4.6 1.7 2014
OGLE-2013-BLG-0341LBb 0.00522 0.702 2014
OGLE-2013-BLG-0102Lb 13.6 0.8 2014
OGLE-2008-BLG-092Lb 0.137 ~18 2014
OGLE-2014-BLG-0124Lb 0.51±0.16 3.1±0.5 ~2400 2014
OGLE-2011-BLG-0265Lb 1.0 ± 0.3 2 2014
OGLE-2012-BLG-0563Lb 0.39 0.74 2015
OGLE-2015-BLG-0966Lb 0.066 2.7 2015
MOA-2010-BLG-353Lb 0.27 1.72 2015
MOA-2013-BLG-605Lb 0.0102 0.93 2015
MOA-2011-BLG-028Lb 0.09 4.14 2015
OGLE-2015-BLG-0954Lb 3.4 1.6 2016
OGLE-2014-BLG-1760Lb 0.56 1.75 2016
OGLE-2012-BLG-0724Lb 0.47 1.6 2016
OGLE-2015-BLG-0051Lb 0.72 0.73 2016
OGLE-2012-BLG-0950Lb 0.079 2.2 2016
OGLE-2007-BLG-349L(AB)b 0.25 2.59 2557 2016
OGLE-2014-BLG-0676Lb 3.68 4.53 2016
OGLE-2016-BLG-1195Lb 0.0312 2.62 2017
MOA-2012-BLG-505Lb 0.0211 0.9 2017
MOA-2012-BLG-006Lb 8.4 10.2 2017
MOA-2016-BLG-227Lb 2.8 1.39 2017
OGLE-2013-BLG-0132Lb 0.29 3.6 2017
OGLE-2013-BLG-1721Lb 0.64 2.6 2017
OGLE-2016-BLG-0263Lb 4.1 5.4 2017
OGLE-2016-BLG-0613L(AB)b 4.18 6.4 2017
OGLE-2016-BLG-1190Lb 13.38 2.17 1220 0.42 41.2 2017
UKIRT-2017-BLG-001Lb 1.28 4.18 2018
TCP J05074264+2447555b 0.0629 0.940 2018
OGLE-2017-BLG-1522Lb 0.75 0.59 2018
OGLE-2017-BLG-1434Lb 0.014±0.0016 1.18±0.1 2018
OGLE-2017-BLG-1140Lb 1.59 1.02 2018
OGLE-2017-BLG-0482Lb 0.028 1.8 2018
OGLE-2017-BLG-0373Lb 0.401 2.424 2018
OGLE-2017-BLG-0173Lb 0.01029 3.913 2018
OGLE-2014-BLG-1722Lb 0.174 1.5 2018
OGLE-2014-BLG-1722Lc 0.263 1.7 2018
OGLE-2013-BLG-1761Lb 2.7 1.8 2018
OGLE-2011-BLG-0173Lb 0.19 8 2018
MOA-2016-BLG-319Lb 0.62 0.95 2018
MOA-2015-BLG-337Lb 0.106 0.24 2018
MOA-2011-BLG-291Lb 0.057 0.69 2018
MOA-2010-BLG-117Lb 0.54 2.42 2018
KMT-2017-BLG-0165Lb 0.11 3.45 2018
KMT-2016-BLG-2142Lb 15.49 0.83 2018
KMT-2016-BLG-1820Lb 4.57 1.08 2018
KMT-2016-BLG-1397Lb 7.0 5.1 2018
KMT-2016-BLG-0212Lb 18 2.2 2018
OGLE-2018-BLG-1011Lb 1.8 1.8 2019
OGLE-2018-BLG-1011Lc 2.8 0.8 2019
OGLE-2018-BLG-0740Lb 4.8 5.0 5480 0 2019
OGLE-2018-BLG-0596Lb 0.04383 0.97 2019
OGLE-2016-BLG-1067Lb 0.43 1.70 2019
OGLE-2015-BLG-1670Lb 0.0563 2.62 2019
OGLE-2015-BLG-1649Lb 2.54 2.07 2019
OGLE-2013-BLG-0911Lb 9.51 0.39 2019
MOA-bin-29Lb 0.6 0.48 2019
KMT-2018-BLG-1990Lb 0.605 1.083 2019
KMT-2017-BLG-1146Lb 0.71 1.6 2019
KMT-2017-BLG-1038Lb 2.0 1.8 2019
KMT-2016-BLG-1836Lb 2.2 3.5 2019
KMT-2016-BLG-1107Lb 3.283 0.342 2019
OGLE-2018-BLG-1700Lb 4.40 2.8 2020
OGLE-2018-BLG-1269Lb 0.67 4.51 2020
OGLE-2018-BLG-0677Lb 0.0125 0.63 2020
OGLE-2018-BLG-0532Lb 0.01960 1.064 2020
OGLE-2017-BLG-1375Lb 11.28 3.04 2020
OGLE-2017-BLG-1049Lb 5.53 3.92 2020
OGLE-2017-BLG-0604Lb 0.51 4.06 2020
OGLE-2017-BLG-0406Lb 0.41 3.5 2020
OGLE-2016-BLG-1227Lb 0.79 3.4 2020
OGLE-2015-BLG-1771Lb 0.433 0.85 2020
OGLE-2012-BLG-0838Lb 0.167 4.43 2020
OGLE-2006-BLG-284LAb 0.453 2.17 2020
KMT-2019-BLG-1953Lb 0.64 2020
KMT-2019-BLG-1339Lb 1.25 2.15 2020
KMT-2019-BLG-0842Lb 0.03234 3.31 2020
KMT-2018-BLG-1292Lb 4.42 6.03 2020
KMT-2018-BLG-0748Lb 0.19 0.62 2020
KMT-2018-BLG-0029Lb 0.0239 4.27 2020
KMT-2016-BLG-2397Lb 2.63 3.64 2020
KMT-2016-BLG-2364Lb 3.93 2.63 2020
OGLE-2019-BLG-1053Lb 0.00780 3.4 2021
OGLE-2019-BLG-0960Lb 0.0079 1.90 2021
OGLE-2019-BLG-0954Lb 14.2 2.65 2021
OGLE-2019-BLG-0304Lb 0.510 1.23 2021
OGLE-2019-BLG-0299Lb 6.220 2.80 2021
OGLE-2017-BLG-1099Lb 3.02 2.73 2021
OGLE-2018-BLG-1428Lb 0.77 3.30 2021
OGLE-2018-BLG-1185Lb 0.0264 1.54 2021
OGLE-2018-BLG-0962Lb 1.34 3.59 2021
OGLE-2018-BLG-0567Lb 0.32 2.72 2021
KMT-2017-BLG-2509Lb 2.09 2.14 2021
KMT-2018-BLG-1976Lb 2.22 3.54 2021
KMT-2018-BLG-1996Lb 1.09 4.27 2021
KMT-2021-BLG-0322Lb 6.40 2021
KMT-2020-BLG-0414Lb 0.00588 2.07 2021
KMT-2020-BLG-0414Lc 27 22.3 2021
KMT-2019-BLG-1715Lb 2.56 3.32 2021
KMT-2019-BLG-0371Lb 7.7 0.79 2021
KMT-2018-BLG-1743Lb 0.245 1.449 2021
KMT-2018-BLG-1025Lb 0.019064 1.305 2021
KMT-2016-BLG-2605Lb 0.7710 0.681 2021
OGLE-2019-BLG-1470L(AB)c 2.2 3.2 2022
OGLE-2019-BLG-1492Lb 0.117 2.7 2022
OGLE-2018-BLG-0977Lb 0.0201 2.0 2022
OGLE-2018-BLG-0516Lb 0.0632 2.2 2022
OGLE-2018-BLG-0506Lb 0.0513 3.0 2022
OGLE-2019-BLG-0468Lb 3.43 3.29 2022
OGLE-2019-BLG-0468Lc 10.22 2.77 2022
OGLE-2019-BLG-0362Lb 3.26 2.18 2022
OGLE-2018-BLG-1647Lb 0.970 1.36 2022
OGLE-2018-BLG-1367Lb 0.950 1.21 2022
OGLE-2018-BLG-1126Lb 0.056 3.23 2022
OGLE-2018-BLG-1119Lb 0.910 4.06 2022
OGLE-2018-BLG-0298Lb 0.14 2.86 2022
OGLE-2018-BLG-0383Lb 0.0201 1.8 2022
OGLE-2017-BLG-1691Lb 0.046 2.41 2022
OGLE-2018-BLG-0799Lb 0.26 1.28 2022
OGLE-2018-BLG-0932Lb 0.890 1.75 2022
OGLE-2018-BLG-1212Lb 0.20 1.68 2022
OGLE-2016-BLG-1093Lb 0.71 2.13 2022
OGLE-2014-BLG-0319Lb 0.57 3.49 2022
MOA-2020-BLG-135Lb 0.0356 1.11 2022
MOA-2019-BLG-008Lb 18 2022
KMT-2019-BLG-0253Lb 0.0488 1.1 2022
KMT-2021-BLG-2294Lb 0.070 1.15 2022
KMT-2021-BLG-1898Lb 0.730 1.9 2022
KMT-2021-BLG-1689Lb 0.14 2.5 2022
KMT-2021-BLG-0119Lb 5.52 2.92 2022
KMT-2021-BLG-0192Lb 0.11 1.62 2022
KMT-2021-BLG-0171Lb 0.0352 3.5 2022
KMT-2021-BLG-1303Lb 0.38 2.89 2022
KMT-2021-BLG-0320Lb 0.10 1.54 2022
KMT-2021-BLG-1554Lb 0.12 0.72 2022
KMT-2021-BLG-1391Lb 0.0143 2.29 2022
KMT-2021-BLG-1372Lb 0.1928 2.37 2022
KMT-2021-BLG-1253Lb 0.05994 1.52 2022
KMT-2019-BLG-0953Lb 0.0289 3.1 2022
KMT-2021-BLG-0748Lb 0.45 2.43 2022
KMT-2021-BLG-1077Lb 0.22 1.26 2022
KMT-2021-BLG-1077Lc 0.25 0.930 2022
KMT-2021-BLG-0912Lb 0.00884 3.14 2022
KMT-2021-BLG-0240Lb 0.21 2.8 2022
KMT-2021-BLG-2974Lb 0.28 2.0 2022
KMT-2019-BLG-1552Lb 4.05 2.6 2022
KMT-2019-BLG-1042Lb 0.19 1.7 2022
KMT-2018-BLG-1988Lb 0.0175 3.09 2022
KMT-2019-BLG-0414Lb 4.57 1.16 2022
KMT-2017-BLG-0673Lb 3.67 2.34 2022
KMT-2018-BLG-0087Lb 0.23 0.870 2022
KMT-2018-BLG-0030Lb 1.45 4.39 2022
KMT-2018-BLG-0247Lb 2.11 2.46 2022
KMT-2018-BLG-2602Lb 1.15 3.81 2022
OGLE-2019-BLG-1180Lb 1.747 5.19 2023
OGLE-2019-BLG-0679Lb 3.34 6.99 2023
OGLE-2019-BLG-0249Lb 7.12 1.84 2023
OGLE-2017-BLG-1806Lb 0.0166 1.75 2023
MOA-2022-BLG-249Lb 0.0152 1.63 2023
MOA-2020-BLG-208Lb 0.14 2.74 2023
KMT-2022-BLG-1013Lb 0.31 1.38 2023
KMT-2022-BLG-0440Lb 0.0485 1.9 2023
KMT-2022-BLG-0371Lb 0.26 3.02 2023
KMT-2021-BLG-2478Lb 0.900 1.85 2023
KMT-2021-BLG-2010Lb 1.07 1.79 2023
KMT-2021-BLG-1770Lb 21 0.900 2023
KMT-2021-BLG-1547Lb 1.47 4.5 2023
KMT-2021-BLG-1150Lb 0.880 4.5 2023
KMT-2021-BLG-1105Lb 1.30 3.54 2023
KMT-2021-BLG-0909Lb 1.26 1.75 2023
KMT-2021-BLG-0712Lb 0.1202 2.22 2023
KMT-2019-BLG-2783Lb 1.16 1.85 2023
KMT-2019-BLG-1806Lb 0.0147 3.02 2023
KMT-2019-BLG-1367Lb 0.0128 1.70 2023
KMT-2019-BLG-1216Lb 0.0940 2.44 2023
KMT-2019-BLG-0335Lb 21 1.64 2023
KMT-2019-BLG-0298Lb 1.81 5.67 2023
KMT-2019-BLG-0297Lb 19 0.960 2023
KMT-2018-BLG-0885Lb 29 1.07 2023
KMT-2017-BLG-1194Lb 0.0111 1.78 2023
KMT-2017-BLG-1003Lb 0.01633 1.38 2023
KMT-2017-BLG-0428Lb 0.0176 1.81 2023
KMT-2016-BLG-1105Lb 0.00730 2.44 2023
K2-2016-BLG-0005Lb 1.10 4.16 4700 2023
OGLE-2017-BLG-1275Lb 5.90 2.09 2024
OGLE-2017-BLG-1237Lb 3.80 2.53 2024
OGLE-2017-BLG-0640Lb 1.62 1.14 2024

Candidate rogue planets

A number of candidate rogue planets have been detected by microlensing.

Planet Mass Year of discovery
MOA-2011-BLG-274L 0.8±0.3 MJ 2014
OGLE-2016-BLG-1540L ~35 M🜨 2017
OGLE-2012-BLG-1323L ~2.3 M🜨 2018
OGLE-2017-BLG-0560L ~1.9 MJ 2018
OGLE-2019-BLG-0551L ~7.7 M🜨 2020
KMT-2019-BLG-2073L ~59 M🜨 2020
OGLE-2016-BLG-1928L ~0.3 M🜨 2020
KMT-2017-BLG-2820L ~8.2 M🜨 2020

Unconfirmed detections

Some microlensing events, such as MACHO-98-BLG-35 and PA-99-N2, suggest the possible presence of a planetary companion to the lensing star, but this is unconfirmed. Since microlensing relies on a one-time chance alignment, it is likely not possible to confirm these detections.

In some cases, a planetary interpretation for a microlensing event was proposed, but has been disproven. MACHO-1997-BLG-41 was initially interpreted as a binary star system orbited by a circumbinary planet, but a different model with two stars and no planet was later found to be a better fit to the data. Similarly, OGLE-2013-BLG-0723L was initially interpreted as a binary system of a star and a brown dwarf, with a low-mass planet orbiting the brown dwarf, but a model where the system consists of two low-mass stars with no planet was found to be a better fit to the data.

See also

Notes

  1. The nature of the observed system is unclear. It is either a rogue planet with about 3.2 MJ masses and a 0.5 ME exomoon or a red dwarf with 18 ME planet.

References

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