List of exoplanets detected by microlensing

Short description: None

| This astronomy needs to be updated. Please update this astronomy to reflect recent events or newly available information. (February 2026)

|

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 0.960 times the mass of earth, or OGLE-2016-BLG-0007Lb, which has a mass about 1.32 times the mass of earth.[1][2] The widest separation between a planet and a star is OGLE-2008-BLG-092Lb, which is 15 AU; the shortest separation is KMT-2020-BLG-0414Lc, which is 0.12 AU.[3][4] There are 9 known multi-planetary systems detected by microlensing, all of which have two planets.[5]

## Contents

* 1 List
* 1.1 Candidate rogue planets
* 1.2 Unconfirmed detections
* 2 See also
* 3 Notes
* 4 References
* 5 External links

## List

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

Planet  | Mass ([[Astronomy:Jupiter mass | J}}}}}}]])  | Projected separation (AU)  | Period (d)  | Eccentricity | Inclination (°)  | Year of discovery

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OGLE-2003-BLG-235Lb | 2.6 | 5.1 |  |  |  | 2004[6][7]
OGLE-2005-BLG-071Lb | 3.5 | 3.6 | ~ 3600 |  |  | 2005[8][9]
OGLE-2005-BLG-390Lb | 0.017 | 2.1 | 3500 |  |  | 2005[10]
OGLE-2005-BLG-169Lb | 0.04 | 2.8 | 3300 |  |  | 2006[11]
OGLE-2006-BLG-109Lb | 0.727 | 2.3 | 1790 |  | 64 | 2008[12]
OGLE-2006-BLG-109Lc | 0.271 | 4.5 | 4931 | 0.15 | 64 | 2008[12]
MOA-2007-BLG-192Lb | 0.01 | 0.66 |  |  |  | 2008[13]
MOA-2007-BLG-400Lb | 0.9 | 0.85 |  |  |  | 2008[14]
MOA-2008-BLG-310Lb | 0.23 | 1.25 |  |  |  | 2009[15]
OGLE-2007-BLG-368Lb | 0.0694 | 3.3 |  |  |  | 2009[16]
MOA-2009-BLG-319Lb | 0.157 | 2.0 |  |  |  | 2010[17]
MOA-2009-BLG-387Lb | 2.6 | 1.8 | 1970 |  |  | 2011[18]
MOA-2009-BLG-266Lb | 0.0327 | 3.2 | 2780 |  |  | 2011[19]
MOA-2011-BLG-293Lb | 2.4 | 1.0 |  |  |  | 2012[20]
MOA-bin-1Lb | 3.7 | 8.3 |  |  |  | 2012[21]
MOA-2010-BLG-477Lb | 1.5 | 2±1 |  |  |  | 2012[22]
OGLE-2012-BLG-0026Lb | 0.11 | 3.82 | ~3000 |  |  | 2012[23]
OGLE-2012-BLG-0026Lc | 0.68 | 4.63 | ~4000 |  |  | 2012[23]
MOA-2010-BLG-073Lb | 11 | 1.21 |  |  |  | 2012[24]
OGLE-2011-BLG-0251Lb | 0.53±0.21 | 2.72±0.75 or 1.5±0.5 |  |  |  | 2013[25]
OGLE-2012-BLG-0406Lb | 2.73±0.43 | 3.45±0.26 |  |  |  | 2013[26]
OGLE-2012-BLG-0358Lb | 1.9±0.2 | 0.87 |  |  |  | 2013[27]
MOA-2010-BLG-328Lb | 0.03 ± 0.0075 | 0.92 |  |  |  | 2013[28]
MOA-2011-BLG-322Lb | 11.6 | 4.3 |  |  |  | 2013[29]
MOA-2008-BLG-379Lb | 5±2.5 | 4±1.6 |  |  |  | 2013[30]
MOA-2011-BLG-262Lb[note 1] | ~0.053 or ~0.0015 | ~0.95 or ~0.13 |  |  |  | 2013[31]
MOA-2013-BLG-220Lb | 2.74 | 3.03 |  |  |  | 2014[32][33]
OGLE-2008-BLG-355Lb | 4.6 | 1.7 |  |  |  | 2014[34]
OGLE-2013-BLG-0341LBb | 0.00522 | 0.702 |  |  |  | 2014[35]
OGLE-2013-BLG-0102Lb | 13.6 | 0.8 |  |  |  | 2014[36]
OGLE-2008-BLG-092Lb | 0.137 | 15 |  |  |  | 2014[3]
OGLE-2014-BLG-0124Lb | 0.51±0.16 | 3.1±0.5 | ~2400 |  |  | 2014[37]
OGLE-2011-BLG-0265Lb | 1.0 ± 0.3 | 2 |  |  |  | 2014[38]
OGLE-2012-BLG-0563Lb | 0.39 | 0.74 |  |  |  | 2015[39]
OGLE-2015-BLG-0966Lb | 0.066 | 2.7 |  |  |  | 2015[40]
MOA-2010-BLG-353Lb | 0.27 | 1.72 |  |  |  | 2015[41]
MOA-2013-BLG-605Lb | 0.0102 | 0.93 |  |  |  | 2015[42]
MOA-2011-BLG-028Lb | 0.09 | 4.14 |  |  |  | 2015[43]
OGLE-2015-BLG-0954Lb | 3.4 | 1.6 |  |  |  | 2016[44]
OGLE-2014-BLG-1760Lb | 0.56 | 1.75 |  |  |  | 2016[45]
OGLE-2012-BLG-0724Lb | 0.47 | 1.6 |  |  |  | 2016[46]
OGLE-2015-BLG-0051Lb | 0.72 | 0.73 |  |  |  | 2016[47]
OGLE-2012-BLG-0950Lb | 0.079 | 2.2 |  |  |  | 2016[48]
OGLE-2007-BLG-349L(AB)b | 0.25 | 2.59 | 2557 |  |  | 2016[49]
OGLE-2014-BLG-0676Lb | 3.68 | 4.53 |  |  |  | 2016[50]
OGLE-2016-BLG-1195Lb | 0.0312 | 2.62 |  |  |  | 2017[51][52]
MOA-2012-BLG-505Lb | 0.0211 | 0.9 |  |  |  | 2017[53]
MOA-2012-BLG-006Lb | 8.4 | 10.2 |  |  |  | 2017[54]
MOA-2016-BLG-227Lb | 2.8 | 1.39 |  |  |  | 2017[55]
OGLE-2013-BLG-0132Lb | 0.29 | 3.6 |  |  |  | 2017[56]
OGLE-2013-BLG-1721Lb | 0.64 | 2.6 |  |  |  | 2017[56]
OGLE-2016-BLG-0263Lb | 4.1 | 5.4 |  |  |  | 2017[57]
OGLE-2016-BLG-0613L(AB)b | 4.18 | 6.4 |  |  |  | 2017[58]
OGLE-2016-BLG-1190Lb | 13.38 | 2.17 | 1220 | 0.42 | 41.2 | 2017[59]
UKIRT-2017-BLG-001Lb | 1.28 | 4.18 |  |  |  | 2018[60]
TCP J05074264+2447555b | 0.0629  | 0.940  |  |  |  | 2018[61][62][63]
OGLE-2017-BLG-1522Lb | 0.75  | 0.59  |  |  |  | 2018[64]
OGLE-2017-BLG-1434Lb  | 0.014±0.0016 | 1.18±0.1 |  |  |  | 2018[65]
OGLE-2017-BLG-1140Lb  | 1.59  | 1.02  |  |  |  | 2018[66]
OGLE-2017-BLG-0482Lb  | 0.028  | 1.8  |  |  |  | 2018[67]
OGLE-2017-BLG-0373Lb  | 0.401  | 2.424  |  |  |  | 2018[68]
OGLE-2017-BLG-0173Lb  | 0.01029  | 3.913  |  |  |  | 2018[69]
OGLE-2014-BLG-1722Lb  | 0.174  | 1.5  |  |  |  | 2018[70]
OGLE-2014-BLG-1722Lc  | 0.263  | 1.7  |  |  |  | 2018[70]
OGLE-2013-BLG-1761Lb  | 2.7  | 1.8  |  |  |  | 2018[71]
OGLE-2011-BLG-0173Lb  | 0.19  | 8  |  |  |  | 2018[72]
MOA-2016-BLG-319Lb  | 0.62  | 0.95  |  |  |  | 2018[73]
MOA-2015-BLG-337Lb  | 0.106  | 0.24  |  |  |  | 2018[74]
MOA-2011-BLG-291Lb  | 0.057  | 0.69  |  |  |  | 2018[75]
MOA-2010-BLG-117Lb  | 0.54  | 2.42  |  |  |  | 2018[76]
KMT-2017-BLG-0165Lb  | 0.11  | 3.45  |  |  |  | 2018[77]
KMT-2016-BLG-2142Lb  | 15.49  | 0.83  |  |  |  | 2018[78]
KMT-2016-BLG-1820Lb  | 4.57  | 1.08  |  |  |  | 2018[78]
KMT-2016-BLG-1397Lb  | 7.0  | 5.1  |  |  |  | 2018[79]
KMT-2016-BLG-0212Lb  | 18  | 2.2  |  |  |  | 2018[80]
OGLE-2018-BLG-1011Lb  | 1.8  | 1.8  |  |  |  | 2019[81]
OGLE-2018-BLG-1011Lc  | 2.8  | 0.8  |  |  |  | 2019[81]
OGLE-2018-BLG-0740Lb  | 4.8  | 5.0  | 5480  | 0  |  | 2019[82]
OGLE-2018-BLG-0596Lb  | 0.04383  | 0.97  |  |  |  | 2019[83]
OGLE-2016-BLG-1067Lb  | 0.43  | 1.70  |  |  |  | 2019[84]
OGLE-2015-BLG-1670Lb  | 0.0563  | 2.62  |  |  |  | 2019[85]
OGLE-2015-BLG-1649Lb  | 2.54  | 2.07  |  |  |  | 2019[86]
OGLE-2013-BLG-0911Lb  | 9.51  | 0.39  |  |  |  | 2019[87]
MOA-bin-29Lb | 0.6 | 0.48 |  |  |  | 2019[88]
KMT-2018-BLG-1990Lb  | 0.605  | 1.083  |  |  |  | 2019[89]
KMT-2017-BLG-1146Lb  | 0.71  | 1.6  |  |  |  | 2019[90]
KMT-2017-BLG-1038Lb  | 2.0  | 1.8  |  |  |  | 2019[90]
KMT-2016-BLG-1836Lb  | 2.2  | 3.5  |  |  |  | 2019[91]
KMT-2016-BLG-1107Lb  | 3.283  | 0.342  |  |  |  | 2019[92]
OGLE-2018-BLG-1700Lb  | 4.40  | 2.8  |  |  |  | 2020[93]
OGLE-2018-BLG-1269Lb  | 0.67  | 4.51  |  |  |  | 2020[94]
OGLE-2018-BLG-0677Lb  | 0.0125  | 0.63  |  |  |  | 2020[95]
OGLE-2018-BLG-0532Lb  | 0.01960  | 1.064  |  |  |  | 2020[96]
OGLE-2017-BLG-1375Lb  | 11.28  | 3.04  |  |  |  | 2020[97]
OGLE-2017-BLG-1049Lb  | 5.53  | 3.92  |  |  |  | 2020[98]
OGLE-2017-BLG-0604Lb  | 0.51  | 4.06  |  |  |  | 2020[97]
OGLE-2017-BLG-0406Lb  | 0.41  | 3.5  |  |  |  | 2020[99]
OGLE-2016-BLG-1227Lb  | 0.79  | 3.4  |  |  |  | 2020[100]
OGLE-2015-BLG-1771Lb  | 0.433  | 0.85  |  |  |  | 2020[101]
OGLE-2012-BLG-0838Lb  | 0.167  | 4.43  |  |  |  | 2020[102]
OGLE-2006-BLG-284LAb  | 0.453  | 2.17  |  |  |  | 2020[103]
KMT-2019-BLG-1953Lb  | 0.64  |  |  |  |  | 2020[104]
KMT-2019-BLG-1339Lb  | 1.25  | 2.15  |  |  |  | 2020[105]
KMT-2019-BLG-0842Lb  | 0.03234  | 3.31  |  |  |  | 2020[106]
KMT-2018-BLG-1292Lb  | 4.42  | 6.03  |  |  |  | 2020[107]
KMT-2018-BLG-0748Lb  | 0.19  | 0.62  |  |  |  | 2020[108]
KMT-2018-BLG-0029Lb  | 0.0239  | 4.27  |  |  |  | 2020[109]
KMT-2016-BLG-2397Lb  | 2.63  | 3.64  |  |  |  | 2020[97]
KMT-2016-BLG-2364Lb  | 3.93  | 2.63  |  |  |  | 2020[97]
OGLE-2019-BLG-1053Lb  | 0.00780  | 3.4  |  |  |  | 2021[110]
OGLE-2019-BLG-0960Lb  | 0.0079  | 1.90  |  |  |  | 2021[111]
OGLE-2019-BLG-0954Lb  | 14.2  | 2.65  |  |  |  | 2021[112]
OGLE-2019-BLG-0304Lb  | 0.510  | 1.23  |  |  |  | 2021[113]
OGLE-2019-BLG-0299Lb  | 6.220  | 2.80  |  |  |  | 2021[114]
OGLE-2017-BLG-1099Lb  | 3.02  | 2.73  |  |  |  | 2021[114]
OGLE-2018-BLG-1428Lb  | 0.77  | 3.30  |  |  |  | 2021[115]
OGLE-2018-BLG-1185Lb  | 0.0264  | 1.54  |  |  |  | 2021[116]
OGLE-2018-BLG-0962Lb  | 1.34  | 3.59  |  |  |  | 2021[117]
OGLE-2018-BLG-0567Lb  | 0.32  | 2.72  |  |  |  | 2021[117]
KMT-2017-BLG-2509Lb  | 2.09  | 2.14  |  |  |  | 2021[114]
KMT-2018-BLG-1976Lb  | 2.22  | 3.54  |  |  |  | 2021[112]
KMT-2018-BLG-1996Lb  | 1.09  | 4.27  |  |  |  | 2021[112]
KMT-2021-BLG-0322Lb  | 6.40  |  |  |  |  | 2021[118]
KMT-2020-BLG-0414Lb  | 0.00302  | 1.26  |  |  |  | 2021[4][1]
KMT-2020-BLG-0414Lc  | 27  | 0.12  |  |  |  | 2021[4][1]
KMT-2019-BLG-1715Lb  | 2.56  | 3.32  |  |  |  | 2021[119]
KMT-2019-BLG-0371Lb | 7.7 | 0.79 |  |  |  | 2021[120]
KMT-2018-BLG-1743Lb  | 0.245  | 1.449  |  |  |  | 2021[121]
KMT-2018-BLG-1025Lb  | 0.019064  | 1.305  |  |  |  | 2021[122]
KMT-2016-BLG-2605Lb  | 0.7710  | 0.681  |  |  |  | 2021[123]
OGLE-2019-BLG-1470L(AB)c  | 2.2  | 3.2  |  |  |  | 2022[124]
OGLE-2019-BLG-1492Lb  | 0.117  | 2.7  |  |  |  | 2022[125]
OGLE-2018-BLG-0977Lb  | 0.0201  | 2.0  |  |  |  | 2022[125]
OGLE-2018-BLG-0516Lb  | 0.0632  | 2.2  |  |  |  | 2022[125]
OGLE-2018-BLG-0506Lb  | 0.0513  | 3.0  |  |  |  | 2022[125]
OGLE-2019-BLG-0468Lb  | 3.43  | 3.29  |  |  |  | 2022[126]
OGLE-2019-BLG-0468Lc  | 10.22  | 2.77  |  |  |  | 2022[126]
OGLE-2019-BLG-0362Lb  | 3.26  | 2.18  |  |  |  | 2022[127]
OGLE-2018-BLG-1647Lb  | 0.970  | 1.36  |  |  |  | 2022[128]
OGLE-2018-BLG-1367Lb  | 0.950  | 1.21  |  |  |  | 2022[128]
OGLE-2018-BLG-1126Lb  | 0.056  | 3.23  |  |  |  | 2022[128]
OGLE-2018-BLG-1119Lb | 0.910  | 4.06  |  |  |  | 2022[129]
OGLE-2018-BLG-0298Lb  | 0.14  | 2.86  |  |  |  | 2022[129]
OGLE-2018-BLG-0383Lb  | 0.0201  | 1.8  |  |  |  | 2022[130]
OGLE-2017-BLG-1691Lb  | 0.046  | 2.41  |  |  |  | 2022[131]
OGLE-2018-BLG-0799Lb | 0.26  | 1.28  |  |  |  | 2022[132]
OGLE-2018-BLG-0932Lb  | 0.890  | 1.75  |  |  |  | 2022[128]
OGLE-2018-BLG-1212Lb  | 0.20  | 1.68  |  |  |  | 2022[128]
OGLE-2016-BLG-1093Lb  | 0.71  | 2.13  |  |  |  | 2022[133]
OGLE-2014-BLG-0319Lb  | 0.57  | 3.49  |  |  |  | 2022[134]
MOA-2020-BLG-135Lb  | 0.0356  | 1.11  |  |  |  | 2022[135]
MOA-2019-BLG-008Lb  | 18  |  |  |  |  | 2022[136]
KMT-2019-BLG-0253Lb  | 0.0488  | 1.1  |  |  |  | 2022[125]
KMT-2021-BLG-2294Lb  | 0.070  | 1.15  |  |  |  | 2022[137]
KMT-2021-BLG-1898Lb  | 0.730  | 1.9  |  |  |  | 2022[138]
KMT-2021-BLG-1689Lb  | 0.14  | 2.5  |  |  |  | 2022[139]
KMT-2021-BLG-0119Lb  | 5.52  | 2.92  |  |  |  | 2022[137]
KMT-2021-BLG-0192Lb  | 0.11  | 1.62  |  |  |  | 2022[137]
KMT-2021-BLG-0171Lb  | 0.0352  | 3.5  |  |  |  | 2022[139]
KMT-2021-BLG-1303Lb  | 0.38  | 2.89  |  |  |  | 2022[131]
KMT-2021-BLG-0320Lb  | 0.10  | 1.54  |  |  |  | 2022[131]
KMT-2021-BLG-1554Lb  | 0.12  | 0.72  |  |  |  | 2022[131]
KMT-2021-BLG-1391Lb  | 0.0143  | 2.29  |  |  |  | 2022[140]
KMT-2021-BLG-1372Lb  | 0.1928  | 2.37  |  |  |  | 2022[140]
KMT-2021-BLG-1253Lb  | 0.05994  | 1.52  |  |  |  | 2022[140]
KMT-2019-BLG-0953Lb  | 0.0289  | 3.1  |  |  |  | 2022[125]
KMT-2021-BLG-0748Lb  | 0.45  | 2.43  |  |  |  | 2022[140]
KMT-2021-BLG-1077Lb  | 0.22  | 1.26  |  |  |  | 2022[141]
KMT-2021-BLG-1077Lc  | 0.25  | 0.930  |  |  |  | 2022[141]
KMT-2021-BLG-0912Lb  | 0.00884  | 3.14  |  |  |  | 2022[142]
KMT-2021-BLG-0240Lb  | 0.21  | 2.8  |  |  |  | 2022[143]
KMT-2021-BLG-2974Lb  | 0.28  | 2.0  |  |  |  | 2022[144]
KMT-2019-BLG-1552Lb  | 4.05  | 2.6  |  |  |  | 2022[144]
KMT-2019-BLG-1042Lb  | 0.19  | 1.7  |  |  |  | 2022[144]
KMT-2018-BLG-1988Lb  | 0.0175  | 3.09  |  |  |  | 2022[145]
KMT-2019-BLG-0414Lb  | 4.57  | 1.16  |  |  |  | 2022[146]
KMT-2017-BLG-0673Lb  | 3.67  | 2.34  |  |  |  | 2022[146]
KMT-2018-BLG-0087Lb  | 0.23  | 0.870  |  |  |  | 2022[129]
KMT-2018-BLG-0030Lb  | 1.45  | 4.39  |  |  |  | 2022[129]
KMT-2018-BLG-0247Lb  | 2.11  | 2.46  |  |  |  | 2022[129]
KMT-2018-BLG-2602Lb  | 1.15  | 3.81  |  |  |  | 2022[129]
OGLE-2019-BLG-1180Lb  | 1.747  | 5.19  |  |  |  | 2023[147]
OGLE-2019-BLG-0679Lb  | 3.34  | 6.99  |  |  |  | 2023[148]
OGLE-2019-BLG-0249Lb  | 7.12  | 1.84  |  |  |  | 2023[148]
OGLE-2017-BLG-1806Lb  | 0.0166  | 1.75  |  |  |  | 2023[149]
MOA-2022-BLG-249Lb  | 0.0152  | 1.63  |  |  |  | 2023[150]
MOA-2020-BLG-208Lb  | 0.14  | 2.74  |  |  |  | 2023[151]
KMT-2022-BLG-1013Lb  | 0.31  | 1.38  |  |  |  | 2023[152]
KMT-2022-BLG-0440Lb  | 0.0485  | 1.9  |  |  |  | 2023[153]
KMT-2022-BLG-0371Lb  | 0.26  | 3.02  |  |  |  | 2023[152]
KMT-2021-BLG-2478Lb  | 0.900  | 1.85  |  |  |  | 2023[154]
KMT-2021-BLG-2010Lb  | 1.07  | 1.79  |  |  |  | 2023[155]
KMT-2021-BLG-1770Lb  | 21  | 0.900  |  |  |  | 2023[156]
KMT-2021-BLG-1547Lb  | 1.47  | 4.5  |  |  |  | 2023[157]
KMT-2021-BLG-1150Lb  | 0.880  | 4.5  |  |  |  | 2023[158]
KMT-2021-BLG-1105Lb  | 1.30  | 3.54  |  |  |  | 2023[154]
KMT-2021-BLG-0909Lb  | 1.26  | 1.75  |  |  |  | 2023[154]
KMT-2021-BLG-0712Lb  | 0.1202  | 2.22  |  |  |  | 2023[154]
KMT-2019-BLG-2783Lb  | 1.16  | 1.85  |  |  |  | 2023[148]
KMT-2019-BLG-1806Lb  | 0.0147  | 3.02  |  |  |  | 2023[149]
KMT-2019-BLG-1367Lb  | 0.0128  | 1.70  |  |  |  | 2023[149]
KMT-2019-BLG-1216Lb  | 0.0940  | 2.44  |  |  |  | 2023[148]
KMT-2019-BLG-0335Lb  | 21  | 1.64  |  |  |  | 2023[159]
KMT-2019-BLG-0298Lb  | 1.81  | 5.67  |  |  |  | 2023[148]
KMT-2019-BLG-0297Lb  | 19  | 0.960  |  |  |  | 2023[159]
KMT-2018-BLG-0885Lb  | 29  | 1.07  |  |  |  | 2023[159]
KMT-2017-BLG-1194Lb  | 0.0111  | 1.78  |  |  |  | 2023[149]
KMT-2017-BLG-1003Lb  | 0.01633  | 1.38  |  |  |  | 2023[149]
KMT-2017-BLG-0428Lb  | 0.0176  | 1.81  |  |  |  | 2023[149]
KMT-2016-BLG-1105Lb  | 0.00730  | 2.44  |  |  |  | 2023[149]
K2-2016-BLG-0005Lb | 1.10  | 4.16  | 4700  |  |  | 2023[160]
OGLE-2017-BLG-1275Lb  | 5.90  | 2.09  |  |  |  | 2024[161]
OGLE-2017-BLG-1237Lb  | 3.80  | 2.53  |  |  |  | 2024[161]
OGLE-2017-BLG-0640Lb  | 1.62  | 1.14  |  |  |  | 2024[161]
OGLE-2017-BLG-0448L b  | 0.0491+0.0434−0.0293 | 5.75+2.39−2.00 |  |  |  | 2024[162]
OGLE-2016-BLG-1800L b  | 2.59±1.46  | 1.88±0.51  |  |  |  | 2024[163]
OGLE-2016-BLG-1598L b  | 0.38±0.30  | 2.50±0.88  |  |  |  | 2024[163]
OGLE-2014-BLG-0221L b  | 4.35+1.65−1.91 | 3.76+0.96−1.07 |  |  |  | 2024[164]
MOA-2022-BLG-563L b  | 0.40+0.31−0.25 | 2.15+0.37−0.52 |  |  |  | 2024[165]
MOA-2016-BLG-526L b  | 0.047±0.021  | 2.07±0.35  |  |  |  | 2024[163]
KMT-2024-BLG-1044L b  | 0.02438+0.03785−0.01271 |  |  |  |  | 2024[166]
KMT-2023-BLG-1866L b  | 0.00827+0.00132−0.00214 | 2.63+0.37−0.34 |  |  |  | 2024[167]
KMT-2023-BLG-1743L b  | 20+30−10 | 1.16+0.17−0.21 |  |  |  | 2024[168]
KMT-2023-BLG-1642L b  | 1.08+1.53−0.58 | 1.41+0.22−0.27 |  |  |  | 2024[169]
KMT-2023-BLG-1454L b  | 0.630+0.710−0.340 | 1.18+0.17−0.18 |  |  |  | 2024[169]
KMT-2023-BLG-1431L b  | 0.0428+0.0261−0.0217 | 3.2+0.7−0.8 |  |  |  | 2024[170]
KMT-2023-BLG-0735L b  | 0.122±0.068  | 2.96+0.56−0.74 |  |  |  | 2024[171]
KMT-2023-BLG-0469L b  | 0.124+0.092−0.067 | 2.31+0.34−0.39 |  |  |  | 2024[171]
KMT-2023-BLG-0416L b  | 0.041+0.020−0.021 | 2.96+0.54−0.75 |  |  |  | 2024[172]
KMT-2022-BLG-2286L b  | 19+27−10 | 2.02+0.27−0.31 |  |  |  | 2024[173]
KMT-2022-BLG-0303L b  | 0.513+0.410−0.275 | 4.81+0.65−0.76 |  |  |  | 2024[174]
KMT-2021-BLG-2609L b  | 0.032+0.044−0.018 | 2.30+0.32−0.36 |  |  |  | 2024[174]
KMT-2016-BLG-2321L b  | 0.950±0.410  | 3.58±0.81  |  |  |  | 2024[175]
Gaia22dkvL b  | 0.591+0.152−0.052 | 1.40+0.77−0.34 |  |  |  | 2024[176]
OGLE-2016-BLG-0007L b  | 0.00415+0.00286−0.00211 | 10.1+3.8−3.4 | 14200+7700−3300 |  |  | 2025[2]
KMT-2021-BLG-0736L b  | 0.066+0.041−0.031 | 4.0+0.9−0.8 |  |  |  | 2025[177]
KMT-2019-BLG-0578L b  | 1.2+1.2−0.6 | 2.0±0.3  |  |  |  | 2025[177]
AT2021ueyL b  | 1.34+0.45−0.50 | 4.01+1.68−1.34 | 4168.69+2910.76−1713.98 |  |  | 2025[178]
KMT-2017-BLG-2197L b  | 8.840+8.290−4.910 | 15.91+2.08−2.68 |  |  |  | 2025[179]
KMT-2022-BLG-1790L b  | 1.73+0.95−0.89 | 5.25+0.75−1.04 |  |  |  | 2025[179]
KMT-2023-BLG-0119L b  | 0.26335+0.16820−0.14395 | 3.14+1.32−1.33 |  |  |  | 2025[180]
KMT-2022-BLG-2076L b  | 0.880+0.460−0.450 | 5.67+1.28−1.58 |  |  |  | 2025[179]
KMT-2023-BLG-0548L b  | 3.42+1.21−0.89 | 6.85+1.22−1.10 |  |  |  | 2025[181]
KMT-2023-BLG-0830L b  | 0.056+0.064−0.033 | 1.70+0.27−0.29 |  |  |  | 2025[181]
KMT-2023-BLG-0949L b  | 5.980+4.360−3.110 | 2.03+0.66−0.81 |  |  |  | 2025[181]
KMT-2023-BLG-1896L b  | 0.05144+0.03087−0.02656 | 2.86+1.12−1.02 |  |  |  | 2025[180]
KMT-2023-BLG-2209L b  | 0.800±0.380  | 3.51+0.095−1.12 |  |  |  | 2025[179]
KMT-2024-BLG-0404L b  | 27.24+39.81−13.62 | 0.85±0.11  |  |  |  | 2025[182]
KMT-2024-BLG-0404L c  | 0.0544+0.0802−0.0277 |  |  |  |  | 2025[182]
KMT-2024-BLG-1005L b  | 21+22−12 | 0.78+0.12−0.11 |  |  |  | 2025[183]
KMT-2024-BLG-1209L b  | 2.64+1.57−1.16 | 2.51+1.50−1.10 |  |  |  | 2025[184]
KMT-2024-BLG-1281L b  | 0.0600+0.0660−0.0360 | 1.96+0.30−0.38 |  |  |  | 2025[181]
KMT-2024-BLG-2059L b  | 0.022+0.012−0.013 | 2.55+0.56−0.89 |  |  |  | 2025[181]
KMT-2024-BLG-2242L b  | 0.044+0.076−0.024 | 0.890±0.120  |  |  |  | 2025[181]
MOA-2022-BLG-033L b  | 0.03823+0.02961−0.01966 | 2.15+1.17−0.75 |  |  |  | 2025[180]
MOA-2022-BLG-091L b  | 3.59+2.00−1.67 | 3.44+1.92−1.60 |  |  |  | 2025[184]
OGLE-2015-BLG-1609L b  | 0.240+0.900−0.170 |  |  |  |  | 2025[185]
OGLE-2016-BLG-0007L b  | 0.00415+0.00286−0.00211 | 10.1+3.8−3.4 | 14200+7700−3300 |  |  | 2025[186]
KMT-2022-BLG-1818L b  | 4.00+1.24−2.00 | 2.6±0.9  |  |  |  | 2026[187]
KMT-2022-BLG-1818L c  | 0.36+0.30−0.21 | 12.6+6.0−4.7 |  |  |  | 2026[187]

### Candidate rogue planets

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

Planet  | Mass | Year of discovery

|
|

MOA-2011-BLG-274L | 0.8000 0.8±0.3 MJ | 2014[188]
OGLE-2016-BLG-1540L | 0.1101 ~35 M🜨 | 2017[189]
OGLE-2012-BLG-1323L | 0.0072 ~2.3 M🜨 | 2018[190]
OGLE-2017-BLG-0560L | 1.9000 ~1.9 MJ | 2018[190]
OGLE-2019-BLG-0551L | 0.0242 ~7.7 M🜨 | 2020[191]
KMT-2019-BLG-2073L | 0.1857 ~59 M🜨 | 2020[192]
OGLE-2016-BLG-1928L | 0.0009 ~0.3 M🜨 | 2020[193]
KMT-2017-BLG-2820L | 0.0258 ~8.2 M🜨 | 2020[194]

### 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.[195]

## See also

* Lists of exoplanets
* Method of exoplanet detection using microlensing

## 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 M⊕ exomoon or a red dwarf with 18 M⊕ planet.

## References

1. ↑ 1.0 1.1 1.2 Zhang, Keming et al. (September 2024). "An Earth-Mass Planet and a Brown Dwarf in Orbit Around a White Dwarf". Accepted for Publication 8 (12): 1575–1582. doi:10.1038/s41550-024-02375-9. Bibcode: 2024NatAs...8.1575Z.
2. ↑ 2.0 2.1 Zang, Weicheng; Jung, Youn Kil; Yee, Jennifer C.; Hwang, Kyu-Ha; Yang, Hongjing; Udalski, Andrzej; Sumi, Takahiro; Gould, Andrew et al. (April 2025). "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits" (in en). Science 388 (6745): 400–404. doi:10.1126/science.adn6088. ISSN 0036-8075. PMID 40273242. Bibcode: 2025Sci...388..400Z. https://ui.adsabs.harvard.edu/abs/2025Sci...388..400Z/abstract.
3. ↑ 3.0 3.1 Poleski, Radosław et al. (13 October 2014). "Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet". The Astrophysical Journal 795 (1): 42. doi:10.1088/0004-637X/795/1/42. Bibcode: 2014ApJ...795...42P.
4. ↑ 4.0 4.1 4.2 Zang, Weicheng; Han, Cheongho; Kondo, Iona; Yee, Jennifer C.; Lee, Chung-Uk; Gould, Andrew; Mao, Shude; de Almeida, Leandro et al. (2021-11-01). "An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb". Research in Astronomy and Astrophysics 21 (9): 239. doi:10.1088/1674-4527/21/9/239. ISSN 1674-4527. Bibcode: 2021RAA....21..239Z. https://iopscience.iop.org/article/10.1088/1674-4527/21/9/239.
5. ↑ "Planetary Systems Composite Data". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PSCompPars. Retrieved 10 February 2026.
6. ↑ Bond, I. A. et al. (2004). "OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event". The Astrophysical Journal 606 (2): L155–L158. doi:10.1086/420928. Bibcode: 2004ApJ...606L.155B.
7. ↑ Bennett, David P. et al. (2006). "Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 Planetary Host Star". The Astrophysical Journal Letters 647 (2): L171–L174. doi:10.1086/507585. Bibcode: 2006ApJ...647L.171B.
8. ↑ Udalski, A. et al. (2005). "A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071". The Astrophysical Journal 628 (2): L109–L112. doi:10.1086/432795. Bibcode: 2005ApJ...628L.109U.
9. ↑ Dong, Subo et al. (2009). "OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion?". The Astrophysical Journal 695 (2): 970–987. doi:10.1088/0004-637X/695/2/970. Bibcode: 2009ApJ...695..970D.
10. ↑ Beaulieu, J.-P. et al. (January 2006). "Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing". Nature 439 (7075): 437–440. doi:10.1038/nature04441. PMID 16437108. Bibcode: 2006Natur.439..437B.
11. ↑ Gould, A. et al. (2006). "Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common". The Astrophysical Journal Letters 644 (1): L37–L40. doi:10.1086/505421. Bibcode: 2006ApJ...644L..37G.
12. ↑ 12.0 12.1 Gaudi, B.S. et al. (2008). "Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing". Science 319 (5865): 927–930. doi:10.1126/science.1151947. PMID 18276883. Bibcode: 2008Sci...319..927G.
13. ↑ Bennett, D. P. et al. (2008). "A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192". The Astrophysical Journal 684 (1): 663–683. doi:10.1086/589940. Bibcode: 2008ApJ...684..663B.
14. ↑ Dong, Subo et al. (2009). "Microlensing Event MOA-2007-BLG-400: Exhuming the Buried Signature of a Cool, Jovian-Mass Planet". The Astrophysical Journal 698 (2): 1826–1837. doi:10.1088/0004-637X/698/2/1826. Bibcode: 2009ApJ...698.1826D.
15. ↑ Janczak, Julia et al. (2010). "Sub-Saturn Planet MOA-2008-BLG-310Lb: Likely To Be In The Galactic Bulge". The Astrophysical Journal 711 (2): 731–743. doi:10.1088/0004-637X/711/2/731. Bibcode: 2010ApJ...711..731J.
16. ↑ Sumi, T. et al. (2010). "A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common". The Astrophysical Journal 710 (2): 1641–1653. doi:10.1088/0004-637X/710/2/1641. Bibcode: 2010ApJ...710.1641S.
17. ↑ Miyake, N. et al. (2011). "A Sub-Saturn Mass Planet, MOA-2009-BLG-319Lb". The Astrophysical Journal 728 (2): article number 120. doi:10.1088/0004-637X/728/2/120. Bibcode: 2011ApJ...728..120M. https://authors.library.caltech.edu/23045/1/Miyake2011p13143Astrophys_J.pdf.
18. ↑ Batista, Virginie et al. (2011). "MOA-2009-BLG-387Lb: A massive planet orbiting an M dwarf". Astronomy and Astrophysics 529: A102. doi:10.1051/0004-6361/201016111. Bibcode: 2011A&A...529A.102B. Data catalog: Bibcode: 2011yCat..35299102B
19. ↑ Muraki, Y. et al. (2011). "Discovery and Mass Measurements of a Cold, 10 Earth Mass Planet and Its Host Star". The Astrophysical Journal 741 (1): 22. doi:10.1088/0004-637X/741/1/22. Bibcode: 2011ApJ...741...22M.
20. ↑ Yee, J. C. et al. (2012). "MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS". The Astrophysical Journal 755 (2): 102. doi:10.1088/0004-637X/755/2/102. Bibcode: 2012ApJ...755..102Y.
21. ↑ Bennett, D. P.; Sumi, T.; Bond, I. A.; Kamiya, K.; Abe, F.; Botzler, C. S.; Fukui, A.; Furusawa, K. et al. (2012). "Planetary and Other Short Binary Microlensing Events from the Moa Short-Event Analysis". The Astrophysical Journal 757 (2): 119. doi:10.1088/0004-637X/757/2/119. Bibcode: 2012ApJ...757..119B.
22. ↑ Bachelet, E. et al. (2012). "MOA 2010-BLG-477Lb: CONSTRAINING THE MASS OF a MICROLENSING PLANET FROM MICROLENSING PARALLAX, ORBITAL MOTION, AND DETECTION OF BLENDED LIGHT". The Astrophysical Journal 754 (1): 73. doi:10.1088/0004-637X/754/1/73. Bibcode: 2012ApJ...754...73B.
23. ↑ 23.0 23.1 Han, C. et al. (2013). "THE SECOND MULTIPLE-PLANET SYSTEM DISCOVERED BY MICROLENSING: OGLE-2012-BLG-0026Lb, c—A PAIR OF JOVIAN PLANETS BEYOND THE SNOW LINE". The Astrophysical Journal 762 (2): L28. doi:10.1088/2041-8205/762/2/L28. Bibcode: 2013ApJ...762L..28H.
24. ↑ Street, R. A. et al. (2013). "Moa-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary". The Astrophysical Journal 763 (1): 67. doi:10.1088/0004-637X/763/1/67. Bibcode: 2013ApJ...763...67S.
25. ↑ Kains, N. et al. (2013). "A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251". Astronomy & Astrophysics 552: A70. doi:10.1051/0004-6361/201220626. Bibcode: 2013A&A...552A..70K.
26. ↑ Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon et al. (2014). "SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb". The Astrophysical Journal 782 (1): 47. doi:10.1088/0004-637X/782/1/47. Bibcode: 2014ApJ...782...47P.
27. ↑ Han, C. et al. (2013). "Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf". The Astrophysical Journal 778 (1): 38. doi:10.1088/0004-637X/778/1/38. Bibcode: 2013ApJ...778...38H.
28. ↑ Furusawa, K.; Udalski, A.; Sumi, T.; Bennett, D. P.; Bond, I. A.; Gould, A.; Jørgensen, U. G.; Snodgrass, C. et al. (23 April 2018). "MOA-2010-BLG-328Lb: A Sub-Neptune Orbiting very Late M Dwarf?". The Astrophysical Journal 779 (2): 91. doi:10.1088/0004-637X/779/2/91. Bibcode: 2013ApJ...779...91F.
29. ↑ Shvartzvald, Y. et al. (2014). "MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet". Monthly Notices of the Royal Astronomical Society 439: 604–610. doi:10.1093/mnras/stt2477.
30. ↑ Suzuki, D. et al. (2013). "MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM a HIGH MAGNIFICATION EVENT WITH a FAINT SOURCE". The Astrophysical Journal 780 (2): 123. doi:10.1088/0004-637X/780/2/123.
31. ↑ Bennett, D. P.; Batista, V.; Bond, I. A.; Bennett, C. S.; Suzuki, D.; Beaulieu, J.-P.; Udalski, A.; Donatowicz, J. et al. (7 April 2014). "A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge". The Astrophysical Journal 785 (2): 155. doi:10.1088/0004-637X/785/2/155. Bibcode: 2014ApJ...785..155B.
32. ↑ Yee, J. C.; Han, C.; Gould, A.; Skowron, J.; Bond, I. A.; Udalski, A.; Hundertmark, M.; Monard, L. A. G. et al. (2014). "MOA-2013-BLG-220Lb: Massive Planetary Companion to Galactic-Disk Host". The Astrophysical Journal 790 (1): 14. doi:10.1088/0004-637X/790/1/14. Bibcode: 2014ApJ...790...14Y.
33. ↑ Vandorou, Aikaterini; Bennett, David P.; Beaulieu, Jean-Philippe; Alard, Christophe; Blackman, Joshua W.; Cole, Andrew A.; Bhattacharya, Aparna; Bond, Ian A. et al. (2020). "Revisiting MOA 2013-BLG-220L: A Solar-type Star with a Cold Super-Jupiter Companion". The Astronomical Journal 160 (3): 121. doi:10.3847/1538-3881/aba2d3. Bibcode: 2020AJ....160..121V.
34. ↑ Koshimoto, N. et al. (20 June 2014). "OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND A LATE-TYPE STAR". The Astrophysical Journal 788 (2): 128. doi:10.1088/0004-637X/788/2/128. Bibcode: 2014ApJ...788..128K.
35. ↑ Gould, A. et al. (3 July 2014). "A terrestrial planet in a 1-AU orbit around one member of a 15-AU binary". Science 345 (6192): 46–49. doi:10.1126/science.1251527. PMID 24994642. Bibcode: 2014Sci...345...46G.
36. ↑ Jung, Y. K.; Udalski, A.; Sumi, T.; Han, C.; Gould, A.; Skowron, J.; Kozłowski, S.; Poleski, R. et al. (2014). "OGLE-2013-BLG-0102LA,B: Microlensing binary with components at star/brown-dwarf and brown-dwarf/planet boundaries". The Astrophysical Journal 798 (2): 123. doi:10.1088/0004-637X/798/2/123. Bibcode: 2015ApJ...798..123J.
37. ↑ Udalski, A.; Yee, J. C.; Gould, A.; Carey, S.; Zhu, W.; Skowron, J.; Kozłowski, S.; Poleski, R. et al. (2014). "Spitzer as Microlens Parallax Satellite: Mass Measurement for the OGLE-2014-BLG-0124L Planet and its Host Star". The Astrophysical Journal 799 (2): 237. doi:10.1088/0004-637X/799/2/237. Bibcode: 2015ApJ...799..237U.
38. ↑ Skowron, J.; Shin, I. -G.; Udalski, A.; Han, C.; Sumi, T.; Shvartzvald, Y.; Gould, A.; Dominis-Prester, D. et al. (2014). "OGLE-2011-BLG-0265Lb: A Jovian Microlensing Planet Orbiting an M Dwarf". The Astrophysical Journal 804 (1): 33. doi:10.1088/0004-637X/804/1/33. Bibcode: 2015ApJ...804...33S.
39. ↑ Fukui, A. et al. (2015). "OGLE-2012-BLG-0563Lb: A SATURN-MASS PLANET AROUND AN M DWARF WITH THE MASS CONSTRAINED BYSUBARUAO IMAGING". The Astrophysical Journal 809 (1): 74. doi:10.1088/0004-637X/809/1/74. Bibcode: 2015ApJ...809...74F.
40. ↑ Street, R. A. et al. (2016). "Spitzerparallax of Ogle-2015-BLG-0966: A Cold Neptune in the Galactic Disk". The Astrophysical Journal 819 (2): 93. doi:10.3847/0004-637X/819/2/93. Bibcode: 2016ApJ...819...93S.
41. ↑ Rattenbury, N. J. et al. (2015). "MOA-2010-BLG-353Lb: A possible Saturn revealed". Monthly Notices of the Royal Astronomical Society 454: 946–951. doi:10.1093/mnras/stv2045.
42. ↑ Sumi, T. et al. (2016). "The First Neptune Analog or Super-Earth with a Neptune-Like Orbit: Moa-2013-BLG-605Lb". The Astrophysical Journal 825 (2): 112. doi:10.3847/0004-637X/825/2/112. Bibcode: 2016ApJ...825..112S.
43. ↑ Skowron, J. et al. (2016). "MOA-2011-BLG-028Lb: A NEPTUNE-MASS MICROLENSING PLANET IN THE GALACTIC BULGE". The Astrophysical Journal 820 (1): 4. doi:10.3847/0004-637X/820/1/4. Bibcode: 2016ApJ...820....4S.
44. ↑ Shin, I. -G.; Ryu, Y. -H. et al. (June 2016). "A Super-Jupiter Microlens Planet Characterized by High-Cadence KMTNet Microlensing Survey Observations of OGLE-2015-BLG-0954". Journal of the Korean Astronomical Society 49 (3): 73–81. doi:10.5303/JKAS.2016.49.3.73. Bibcode: 2016JKAS...49...73S.
45. ↑ Bhattacharya, A. et al. (2016). "Discovery of a Gas Giant Planet in Microlensing Event Ogle-2014-BLG-1760". The Astronomical Journal 152 (5): 140. doi:10.3847/0004-6256/152/5/140. Bibcode: 2016AJ....152..140B.
46. ↑ Hirao, Y. et al. (2016). "Ogle-2012-BLG-0724Lb: A Saturn-Mass Planet Around an M Dwarf". The Astrophysical Journal 824 (2): 139. doi:10.3847/0004-637X/824/2/139. Bibcode: 2016ApJ...824..139H.
47. ↑ Han, C.; Udalski, A.; Gould, A.; Bozza, V.; Jung, Y. K.; Albrow, M. D.; Kim, S.-L.; Lee, C.-U. et al. (2016). "Ogle-2015-BLG-0051/KMT-2015-BLG-0048Lb: A Giant Planet Orbiting a Low-Mass Bulge Star Discovered by High-Cadence Microlensing Surveys". The Astronomical Journal 152 (4): 95. doi:10.3847/0004-6256/152/4/95. Bibcode: 2016AJ....152...95H.
48. ↑ Koshimoto, N. et al. (2016). "OGLE-2012-BLG-0950Lb: THE FIRST PLANET MASS MEASUREMENT FROM ONLY MICROLENS PARALLAX AND LENS FLUX". The Astronomical Journal 153: 1. doi:10.3847/1538-3881/153/1/1.
49. ↑ Bennett, D. P. et al. (2016). "THE FIRST CIRCUMBINARY PLANET FOUND BY MICROLENSING: OGLE-2007-BLG-349L(AB)c". The Astronomical Journal 152 (5): 125. doi:10.3847/0004-6256/152/5/125. Bibcode: 2016AJ....152..125B.
50. ↑ Rattenbury, N. J. et al. (2017). "Faint-source-star planetary microlensing: The discovery of the cold gas-giant planet OGLE-2014-BLG-0676Lb". Monthly Notices of the Royal Astronomical Society 466 (3): 2710–2717. doi:10.1093/mnras/stw3185.
51. ↑ Shvartzvald, Y.; Yee, J. C.; Novati, S. Calchi; Gould, A.; Lee, C.-U.; Beichman, C.; Bryden, G.; Carey, S. et al. (2017). "An Earth-mass Planet in a 1 au Orbit around an Ultracool Dwarf". The Astrophysical Journal 840 (1): L3. doi:10.3847/2041-8213/aa6d09. Bibcode: 2017ApJ...840L...3S.
52. ↑ Vandorou, Aikaterini; Dang, Lisa; Bennett, David P.; Koshimoto, Naoki; Terry, Sean K.; Beaulieu, Jean-Phillipe; Alard, Christophe; Bhattacharya, Aparna et al. (2025). "OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-dwarf Confirmed by Keck Adaptive Optics". The Astronomical Journal 169 (6): 319. doi:10.3847/1538-3881/adcec2. Bibcode: 2025AJ....169..319V.
53. ↑ Nagakane, M. et al. (2017). "MOA-2012-BLG-505Lb: A Super-Earth-mass Planet That Probably Resides in the Galactic Bulge". The Astronomical Journal 154 (1): 35. doi:10.3847/1538-3881/aa74b2. Bibcode: 2017AJ....154...35N.
54. ↑ Poleski, R. et al. (2017). "A companion on the planet/Brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing". Astronomy & Astrophysics 604: A103. doi:10.1051/0004-6361/201730928. Bibcode: 2017A&A...604A.103P.
55. ↑ Koshimoto, N. et al. (2017). "MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Light-curve Analysis and Keck AO Imaging". The Astronomical Journal 154 (1): 3. doi:10.3847/1538-3881/aa72e0. Bibcode: 2017AJ....154....3K.
56. ↑ 56.0 56.1 Mróz, Przemek et al. (2017). "OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs". The Astronomical Journal 154 (5): 205. doi:10.3847/1538-3881/aa8f98. Bibcode: 2017AJ....154..205M.
57. ↑ Han, C. et al. (2017). "OGLE-2016-BLG-0263Lb: Microlensing Detection of a Very Low-mass Binary Companion through a Repeating Event Channel". The Astronomical Journal 154 (4): 133. doi:10.3847/1538-3881/aa859a. Bibcode: 2017AJ....154..133H.
58. ↑ Han, C. et al. (2017). "OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System". The Astronomical Journal 154 (6): 223. doi:10.3847/1538-3881/aa9179. Bibcode: 2017AJ....154..223H.
59. ↑ Ryu, Y.-H. et al. (2017). "OGLE-2016-BLG-1190Lb: The FirstSpitzer Bulge Planet Lies Near the Planet/Brown-dwarf Boundary". The Astronomical Journal 155: 40. doi:10.3847/1538-3881/aa9be4.
60. ↑ Shvartzvald, Y.; Calchi Novati, S.; Gaudi, B. S.; Bryden, G.; Nataf, D. M.; Penny, M. T.; Beichman, C.; Henderson, C. B. et al. (2018-04-01). "UKIRT-2017-BLG-001Lb: A Giant Planet Detected through the Dust". The Astrophysical Journal 857 (1): L8. doi:10.3847/2041-8213/aab71b. ISSN 0004-637X. Bibcode: 2018ApJ...857L...8S.
61. ↑ Nucita, A. A.; Licchelli, D.; De Paolis, F.; Ingrosso, G.; Strafella, F.; Katysheva, N.; Shugarov, S. (2018-05-01). "Discovery of a bright microlensing event with planetary features towards the Taurus region: a super-Earth planet". Monthly Notices of the Royal Astronomical Society 476 (3): 2962–2967. doi:10.1093/mnras/sty448. ISSN 0035-8711. Bibcode: 2018MNRAS.476.2962N.
62. ↑ Zang, Weicheng; Dong, Subo; Gould, Andrew; Calchi Novati, Sebastiano; Chen, Ping; Yang, Hongjing; Li, Shun-Sheng; Mao, Shude et al. (2020-07-01). "Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event". The Astrophysical Journal 897 (2): 180. doi:10.3847/1538-4357/ab9749. ISSN 0004-637X. Bibcode: 2020ApJ...897..180Z.
63. ↑ Fukui, A.; Suzuki, D.; Koshimoto, N.; Bachelet, E.; Vanmunster, T.; Storey, D.; Maehara, H.; Yanagisawa, K. et al. (2019-11-01). "Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star". The Astronomical Journal 158 (5): 206. doi:10.3847/1538-3881/ab487f. ISSN 0004-6256. Bibcode: 2019AJ....158..206F.
64. ↑ Jung, Y. K.; Udalski, A.; Gould, A.; Ryu, Y. -H.; Yee, J. C.; and; Han, C.; Albrow, M. D. et al. (2018-05-01). "OGLE-2017-BLG-1522: A Giant Planet around a Brown Dwarf Located in the Galactic Bulge". The Astronomical Journal 155 (5): 219. doi:10.3847/1538-3881/aabb51. ISSN 0004-6256. Bibcode: 2018AJ....155..219J.
65. ↑ Udalski, A.; Ryu, Y.-H.; Sajadian, S.; Gould, A.; Mróz, P.; Poleski, R.; Szymański, M.K.; Skowron, J. et al. (March 2018). "OGLE-2017-BLG-1434Lb: Eighth q". Acta Astronomica 68 (1): 1–42. doi:10.32023/0001-5237/68.1.1. https://doi.org/10.32023/0001-5237/68.1.1.
66. ↑ Calchi Novati, S.; Skowron, J.; Jung, Y. K.; Beichman, C.; Bryden, G.; Carey, S.; Gaudi, B. S.; Henderson, C. B. et al. (2018-06-01). "Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-mass Microlensing Planet OGLE-2017-BLG-1140Lb". The Astronomical Journal 155 (6): 261. doi:10.3847/1538-3881/aac21c. ISSN 0004-6256. Bibcode: 2018AJ....155..261C.
67. ↑ Han, C.; Hirao, Y.; Udalski, A.; Lee, C. -U.; Bozza, V.; Gould, A.; and; Abe, F. et al. (2018-05-01). "OGLE-2017-BLG-0482Lb: A Microlensing Super-Earth Orbiting a Low-mass Host Star". The Astronomical Journal 155 (5): 211. doi:10.3847/1538-3881/aabad2. ISSN 0004-6256. Bibcode: 2018AJ....155..211H.
68. ↑ Skowron, J.; Ryu, Y. -H.; Hwang, K. -H.; Udalski, A.; Mróz, P.; Kozłowski, S.; Soszyński, I.; Pietrukowicz, P. et al. (2018-03-01). "OGLE-2017-BLG-0373Lb: A Jovian Mass-Ratio Planet Exposes A New Accidental Microlensing Degeneracy". Acta Astronomica 68 (1): 43–61. doi:10.32023/0001-5237/68.1.2. ISSN 0001-5237. Bibcode: 2018AcA....68...43S. https://ui.adsabs.harvard.edu/abs/2018AcA....68...43S.
69. ↑ Hwang, K. -H.; Udalski, A.; Shvartzvald, Y.; Ryu, Y. -H.; Albrow, M. D.; Chung, S. -J.; Gould, A.; Han, C. et al. (2018-01-01). "OGLE-2017-BLG-0173Lb: Low-mass-ratio Planet in a "Hollywood" Microlensing Event". The Astronomical Journal 155 (1): 20. doi:10.3847/1538-3881/aa992f. ISSN 0004-6256. Bibcode: 2018AJ....155...20H.
70. ↑ 70.0 70.1 Suzuki, D.; Bennett, D. P.; Udalski, A.; Bond, I. A.; Sumi, T.; Han, C.; Kim, Ho-il.; Abe, F. et al. (2018-06-01). "A Likely Detection of a Two-planet System in a Low-magnification Microlensing Event". The Astronomical Journal 155 (6): 263. doi:10.3847/1538-3881/aabd7a. ISSN 0004-6256. Bibcode: 2018AJ....155..263S.
71. ↑ Hirao, Y.; Udalski, A.; Sumi, T.; Bennett, D. P.; Koshimoto, N.; Bond, I. A.; Rattenbury, N. J.; Suzuki, D. et al. (2017-07-01). "OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf". The Astronomical Journal 154 (1): 1. doi:10.3847/1538-3881/aa73da. ISSN 0004-6256. Bibcode: 2017AJ....154....1H.
72. ↑ Poleski, Radosław; Gaudi, B. S.; Udalski, A.; Szymański, M. K.; Soszyński, I.; Pietrukowicz, P.; Kozłowski, S.; Skowron, J. et al. (2018-09-01). "An Ice Giant Exoplanet Interpretation of the Anomaly in Microlensing Event OGLE-2011-BLG-0173". The Astronomical Journal 156 (3): 104. doi:10.3847/1538-3881/aad45e. ISSN 0004-6256. Bibcode: 2018AJ....156..104P.
73. ↑ Han, Cheongho; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Jung, Youn Kil; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (2018-11-01). "MOA-2016-BLG-319Lb: Microlensing Planet Subject to Rare Minor-image Perturbation Degeneracy in Determining Planet Parameters". The Astronomical Journal 156 (5): 226. doi:10.3847/1538-3881/aae38e. ISSN 0004-6256. Bibcode: 2018AJ....156..226H.
74. ↑ Miyazaki, S.; Sumi, T.; Bennett, D. P.; Gould, A.; Udalski, A.; Bond, I. A.; Koshimoto, N.; Nagakane, M. et al. (2018-09-01). "MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary". The Astronomical Journal 156 (3): 136. doi:10.3847/1538-3881/aad5ee. ISSN 0004-6256. Bibcode: 2018AJ....156..136M.
75. ↑ Bennett, David P.; Udalski, Andrzej; Bond, Ian A.; Suzuki, Daisuke; Ryu, Yoon-Hyun; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna et al. (2018-09-01). "A Planetary Microlensing Event with an Unusually Red Source Star: MOA-2011-BLG-291". The Astronomical Journal 156 (3): 113. doi:10.3847/1538-3881/aad59c. ISSN 0004-6256. Bibcode: 2018AJ....156..113B.
76. ↑ Bennett, D. P.; Udalski, A.; Han, C.; Bond, I. A.; Beaulieu, J. -P.; Skowron, J.; Gaudi, B. S.; Koshimoto, N. et al. (2018-03-01). "The First Planetary Microlensing Event with Two Microlensed Source Stars". The Astronomical Journal 155 (3): 141. doi:10.3847/1538-3881/aaadfa. ISSN 0004-6256. Bibcode: 2018AJ....155..141B.
77. ↑ Jung, Youn Kil; Gould, Andrew; Zang, Weicheng; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D. et al. (2019-02-01). "KMT-2017-BLG-0165Lb: A Super-Neptune-mass Planet Orbiting a Sun-like Host Star". The Astronomical Journal 157 (2): 72. doi:10.3847/1538-3881/aaf87f. ISSN 0004-6256. Bibcode: 2019AJ....157...72J.
78. ↑ 78.0 78.1 Jung, Youn Kil; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Gould, Andrew; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju et al. (2018-11-01). "KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-low-mass Primaries". The Astronomical Journal 156 (5): 208. doi:10.3847/1538-3881/aae319. ISSN 0004-6256. Bibcode: 2018AJ....156..208J.
79. ↑ Zang, Weicheng; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Gould, Andrew; Wang, Tianshu; Zhu, Wei; Mao, Shude; Albrow, Michael D. et al. (2018-11-01). "KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet". The Astronomical Journal 156 (5): 236. doi:10.3847/1538-3881/aae537. ISSN 0004-6256. Bibcode: 2018AJ....156..236Z.
80. ↑ Hwang, K. -H.; Kim, H. -W.; Kim, D. -J.; Gould, A.; Albrow, M. D.; Chung, S. -J.; Han, C.; Jung, Y. K. et al. (2018-12-01). "KMT-2016-BLG-0212: First KMTNet-Only Discovery of a Substellar Companion". Journal of the Korean Astronomical Society 51 (6): 197–206. doi:10.5303/JKAS.2018.51.6.197. ISSN 1225-4614. Bibcode: 2018JKAS...51..197H. https://ui.adsabs.harvard.edu/abs/2018JKAS...51..197H.
81. ↑ 81.0 81.1 Han, Cheongho; Bennett, David P.; Udalski, Andrzej; Gould, Andrew; Bond, Ian A.; Shvartzvald, Yossi; Nikolaus, Kay-Sebastian; Hundertmark, Markus et al. (2019-09-01). "OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star". The Astronomical Journal 158 (3): 114. doi:10.3847/1538-3881/ab2f74. ISSN 0004-6256. Bibcode: 2019AJ....158..114H.
82. ↑ Han, Cheongho; Yee, Jennifer C.; Udalski, Andrzej; Bond, Ian A.; Bozza, Valerio; Cassan, Arnaud; Hirao, Yuki; Dong, Subo et al. (2019-09-01). "Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb". The Astronomical Journal 158 (3): 102. doi:10.3847/1538-3881/ab2df4. ISSN 0004-6256. Bibcode: 2019AJ....158..102H.
83. ↑ Jung, Youn Kil; Gould, Andrew; Udalski, Andrzej; Sumi, Takahiro; Yee, Jennifer C.; Shvartzvald, Yossi; Zang, Weicheng; and et al. (2019-07-01). "Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M Dwarf". The Astronomical Journal 158 (1): 28. doi:10.3847/1538-3881/ab237f. ISSN 0004-6256. Bibcode: 2019AJ....158...28J.
84. ↑ Calchi Novati, S.; Suzuki, D.; Udalski, A.; Gould, A.; Shvartzvald, Y.; Bozza, V.; Bennett, D. P.; Beichman, C. et al. (2019-03-01). "Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk". The Astronomical Journal 157 (3): 121. doi:10.3847/1538-3881/ab0106. ISSN 0004-6256. Bibcode: 2019AJ....157..121C.
85. ↑ Ranc, Clément; Bennett, David P.; Hirao, Yuki; Udalski, Andrzej; Han, Cheongho; Bond, Ian A.; Yee, Jennifer C.; and et al. (2019-06-01). "OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field". The Astronomical Journal 157 (6): 232. doi:10.3847/1538-3881/ab141b. ISSN 0004-6256. Bibcode: 2019AJ....157..232R.
86. ↑ Nagakane, M.; Lee, Chien-Hsiu; Koshimoto, N.; Suzuki, D.; Udalski, A.; Beaulieu, J. P.; Sumi, T.; Bennett, D. P. et al. (2019-11-01). "OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf". The Astronomical Journal 158 (5): 212. doi:10.3847/1538-3881/ab4881. ISSN 0004-6256. Bibcode: 2019AJ....158..212N.
87. ↑ Miyazaki, Shota; Sumi, Takahiro; Bennett, David P.; Udalski, Andrzej; Shvartzvald, Yossi; Street, Rachel; Bozza, Valerio; Yee, Jennifer C. et al. (2020-02-01). "OGLE-2013-BLG-0911Lb: A Secondary on the Brown-dwarf Planet Boundary around an M Dwarf". The Astronomical Journal 159 (2): 76. doi:10.3847/1538-3881/ab64de. ISSN 0004-6256. Bibcode: 2020AJ....159...76M.
88. ↑ Kondo, Iona et al. (2019). "MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star". The Astronomical Journal 158 (6): 224. doi:10.3847/1538-3881/ab4e9e. Bibcode: 2019AJ....158..224K.
89. ↑ Ryu, Yoon-Hyun; Hwang, Kyu-Ha; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Jung, Youn Kil; Shin, In-Gu et al. (2019-10-01). "KMT-2018-BLG-1990Lb: A Nearby Jovian Planet From A Low-cadence Microlensing Field". The Astronomical Journal 158 (4): 151. doi:10.3847/1538-3881/ab3a34. ISSN 0004-6256. Bibcode: 2019AJ....158..151R.
90. ↑ 90.0 90.1 Shin, I. -G.; Ryu, Y. -H.; Yee, J. C.; Gould, A.; Albrow, M. D.; Chung, S. -J.; Han, C.; Hwang, K. -H. et al. (2019-04-01). "Two Jupiter-mass Planets Discovered by the KMTNet Survey in 2017". The Astronomical Journal 157 (4): 146. doi:10.3847/1538-3881/ab07c2. ISSN 0004-6256. Bibcode: 2019AJ....157..146S.
91. ↑ Yang, Hongjing; Zhang, Xiangyu; Hwang, Kyu-Ha; Zang, Weicheng; Gould, Andrew; Wang, Tianshu; Mao, Shude; Albrow, Michael D. et al. (2020-03-01). "KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field". The Astronomical Journal 159 (3): 98. doi:10.3847/1538-3881/ab660e. ISSN 0004-6256. Bibcode: 2020AJ....159...98Y.
92. ↑ Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Kim, Hyoun-Woo; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Han, Cheongho; Jung, Youn Kil et al. (2019-01-01). "KMT-2016-BLG-1107: A New Hollywood-planet Close/Wide Degeneracy". The Astronomical Journal 157 (1): 23. doi:10.3847/1538-3881/aaf16e. ISSN 0004-6256. Bibcode: 2019AJ....157...23H.
93. ↑ Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Gould, Andrew; Bond, Ian A.; AUTHORS, LEADING; Albrow, Michael D.; Chung, Sun-Ju et al. (2020-02-01). "OGLE-2018-BLG-1700L: Microlensing Planet in Binary Stellar System". The Astronomical Journal 159 (2): 48. doi:10.3847/1538-3881/ab5db9. ISSN 0004-6256. Bibcode: 2020AJ....159...48H.
94. ↑ Jung, Youn Kil; Gould, Andrew; Udalski, Andrzej; Sumi, Takahiro; Yee, Jennifer C.; Han, Cheongho; Albrow, Michael D.; Chung, Sun-Ju et al. (2020-09-01). "OGLE-2018-BLG-1269Lb: A Jovian Planet with a Bright I = 16 Host". The Astronomical Journal 160 (3): 148. doi:10.3847/1538-3881/abacc8. ISSN 0004-6256. Bibcode: 2020AJ....160..148J.
95. ↑ Herrera-Martín, Antonio; Albrow, M. D.; Udalski, A.; Gould, A.; Ryu, Y. -H.; Yee, J. C.; Chung, S. -J.; Han, C. et al. (2020-06-01). "OGLE-2018-BLG-0677Lb: A Super-Earth Near the Galactic Bulge". The Astronomical Journal 159 (6): 256. doi:10.3847/1538-3881/ab893e. ISSN 0004-6256. Bibcode: 2020AJ....159..256H.
96. ↑ Ryu, Yoon-Hyun; Udalski, Andrzej; Yee, Jennifer C.; Penny, Matthew T.; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (2020-10-01). "OGLE-2018-BLG-0532Lb: Cold Neptune with Possible Jovian Sibling". The Astronomical Journal 160 (4): 183. doi:10.3847/1538-3881/abaa3f. ISSN 0004-6256. Bibcode: 2020AJ....160..183R.
97. ↑ 97.0 97.1 97.2 97.3 Han, Cheongho; Udalski, Andrzej; Kim, Doeon; Jung, Youn Kil; Ryu, Yoon-Hyun; KMTNet Collaboration; Albrow, Michael D.; Chung, Sun-Ju et al. (2020-10-01). "Four microlensing planets with faint-source stars identified in the 2016 and 2017 season data". Astronomy and Astrophysics 642: A110. doi:10.1051/0004-6361/202039066. ISSN 0004-6361. Bibcode: 2020A&A...642A.110H. https://ui.adsabs.harvard.edu/abs/2020A&A...642A.110H.
98. ↑ Kim, Yun Hak; Chung, Sun-Ju; Udalski, A.; Bond, Ian A.; Jung, Youn Kil; Gould, Andrew; Albrow, Michael D.; Han, Cheongho et al. (2020-12-01). "OGLE-2017-BLG-1049: Another Giant Planet Microlensing Event". Journal of the Korean Astronomical Society 53 (6): 161–168. doi:10.5303/JKAS.2020.53.6.161. ISSN 1225-4614. Bibcode: 2020JKAS...53..161K. https://ui.adsabs.harvard.edu/abs/2020JKAS...53..161K.
99. ↑ Hirao, Yuki; Bennett, David P.; Ryu, Yoon-Hyun; Koshimoto, Naoki; Udalski, Andrzej; Yee, Jennifer C.; Sumi, Takahiro; Bond, Ian A. et al. (2020-08-01). "OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk". The Astronomical Journal 160 (2): 74. doi:10.3847/1538-3881/ab9ac3. ISSN 0004-6256. Bibcode: 2020AJ....160...74H.
100. ↑ Han, Cheongho; Udalsk, Andrzej; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil; Lee, Chung-Uk et al. (2020-03-01). "OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event". The Astronomical Journal 159 (3): 91. doi:10.3847/1538-3881/ab6a9f. ISSN 0004-6256. Bibcode: 2020AJ....159...91H.
101. ↑ Zhang, Xiangyu; Zang, Weicheng; Udalski, Andrzej; Gould, Andrew; Ryu, Yoon-Hyun; Wang, Tianshu; Yang, Hongjing; Mao, Shude et al. (2020-03-01). "OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?". The Astronomical Journal 159 (3): 116. doi:10.3847/1538-3881/ab6f6d. ISSN 0004-6256. Bibcode: 2020AJ....159..116Z.
102. ↑ Poleski, R.; Suzuki, Daisuke; Udalski, A.; Xie, Xiaojia; Yee, J. C.; Koshimoto, Naoki; Gaudi, B. S.; Gould, A. et al. (2020-06-01). "A Wide-orbit Exoplanet OGLE-2012-BLG-0838Lb". The Astronomical Journal 159 (6): 261. doi:10.3847/1538-3881/ab8a49. ISSN 0004-6256. Bibcode: 2020AJ....159..261P.
103. ↑ Bennett, David P.; Udalski, Andrzej; Bond, Ian A.; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Donachie, Martin; Fujii, Hirosane et al. (2020-08-01). "A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System". The Astronomical Journal 160 (2): 72. doi:10.3847/1538-3881/ab9cb9. ISSN 0004-6256. Bibcode: 2020AJ....160...72B.
104. ↑ Han, Cheongho; Kim, Doeon; Jung, Youn Kil; Gould, Andrew; Bond, Ian A.; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (2020-07-01). "One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953". The Astronomical Journal 160 (1): 17. doi:10.3847/1538-3881/ab91ac. ISSN 0004-6256. Bibcode: 2020AJ....160...17H.
105. ↑ Han, Cheongho; Kim, Doeon; Udalski, Andrzej; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil et al. (2020-08-01). "KMT-2019-BLG-1339L: An M Dwarf with a Giant Planet or a Companion near the Planet/Brown Dwarf Boundary". The Astronomical Journal 160 (2): 64. doi:10.3847/1538-3881/ab9a3e. ISSN 0004-6256. Bibcode: 2020AJ....160...64H.
106. ↑ Jung, Youn Kil; Udalski, Andrzej; Zang, Weicheng; Bond, Ian A.; Yee, Jennifer C.; Han, Cheongho; Albrow, Michael D.; Chung, Sun-Ju et al. (2020-12-01). "KMT-2019-BLG-0842Lb: A Cold Planet below the Uranus/Sun Mass Ratio". The Astronomical Journal 160 (6): 255. doi:10.3847/1538-3881/abbe93. ISSN 0004-6256. Bibcode: 2020AJ....160..255J.
107. ↑ Ryu, Yoon-Hyun; Navarro, Maria Gabriela; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Jung, Youn Kil et al. (2020-02-01). "KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane". The Astronomical Journal 159 (2): 58. doi:10.3847/1538-3881/ab5e7e. ISSN 0004-6256. Bibcode: 2020AJ....159...58R.
108. ↑ Han, Cheongho; Shin, In-Gu; Jung, Youn Kil; Kim, Doeon; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (2020-09-01). "KMT-2018-BLG-0748Lb: sub-Saturn microlensing planet orbiting an ultracool host". Astronomy and Astrophysics 641: A105. doi:10.1051/0004-6361/202038173. ISSN 0004-6361. Bibcode: 2020A&A...641A.105H. https://ui.adsabs.harvard.edu/abs/2020A&A...641A.105H.
109. ↑ Gould, Andrew; Ryu, Yoon-Hyun; Calchi Novati, Sebastiano; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha et al. (2020-02-01). "KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet". Journal of the Korean Astronomical Society 53 (1): 9–26. doi:10.5303/JKAS.2020.53.1.9. ISSN 1225-4614. Bibcode: 2020JKAS...53....9G. https://ui.adsabs.harvard.edu/abs/2020JKAS...53....9G.
110. ↑ Zang, Weicheng; Hwang, Kyu-Ha; Udalski, Andrzej; Wang, Tianshu; Zhu, Wei; Sumi, Takahiro; Yee, Jennifer C.; Gould, Andrew et al. (2021-10-01). "Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet". The Astronomical Journal 162 (4): 163. doi:10.3847/1538-3881/ac12d4. ISSN 0004-6256. Bibcode: 2021AJ....162..163Z.
111. ↑ Yee, Jennifer C.; Zang, Weicheng; Udalski, Andrzej; Ryu, Yoon-Hyun; Green, Jonathan; Hennerley, Steve; Marmont, Andrew; Sumi, Takahiro et al. (2021-11-01). "OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet". The Astronomical Journal 162 (5): 180. doi:10.3847/1538-3881/ac1582. ISSN 0004-6256. Bibcode: 2021AJ....162..180Y.
112. ↑ 112.0 112.1 112.2 Han, Cheongho; Udalski, Andrzej; Kim, Doeon; Lee, Chung-Uk; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha et al. (2021-06-01). "Three microlensing planets with no caustic-crossing features". Astronomy and Astrophysics 650: A89. doi:10.1051/0004-6361/202140758. ISSN 0004-6361. Bibcode: 2021A&A...650A..89H. https://ui.adsabs.harvard.edu/abs/2021A&A...650A..89H.
113. ↑ Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Kim, Doeon; Ryu, Yoon-Hyun; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (2021-11-01). "OGLE-2019-BLG-0304: Competing Interpretations between a Planet-binary Model and a Binary-source + Binary-lens Model". The Astronomical Journal 162 (5): 203. doi:10.3847/1538-3881/ac1c09. ISSN 0004-6256. Bibcode: 2021AJ....162..203H.
114. ↑ 114.0 114.1 114.2 Han, Cheongho; Udalski, Andrzej; Kim, Doeon; Ryu, Yoon-Hyun; Bozza, Valerio; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (2021-11-01). "Three faint-source microlensing planets detected via the resonant-caustic channel". Astronomy and Astrophysics 655: A21. doi:10.1051/0004-6361/202141517. ISSN 0004-6361. Bibcode: 2021A&A...655A..21H. https://ui.adsabs.harvard.edu/abs/2021A&A...655A..21H.
115. ↑ Kim, Yun Hak; Chung, Sun-Ju; Udalski, Andrej; Gould, Andrew; Albrow, Michael D.; Jung, Youn Kil; Hwang, Kyu-Ha; Han, Cheongho et al. (2021-05-01). "OGLE-2018-BLG-1428Lb: a Jupiter-mass planet beyond the snow line of a dwarf star". Monthly Notices of the Royal Astronomical Society 503 (2): 2706–2712. doi:10.1093/mnras/stab534. ISSN 0035-8711. Bibcode: 2021MNRAS.503.2706K.
116. ↑ Kondo, Iona; Yee, Jennifer C.; Bennett, David P.; Sumi, Takahiro; Koshimoto, Naoki; Bond, Ian A.; Gould, Andrew; Udalski, Andrzej et al. (2021-08-01). "OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf". The Astronomical Journal 162 (2): 77. doi:10.3847/1538-3881/ac00ba. ISSN 0004-6256. Bibcode: 2021AJ....162...77K.
117. ↑ 117.0 117.1 Jung, Youn Kil; Han, Cheongho; Udalski, Andrzej; Gould, Andrew; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (2021-06-01). "OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel". The Astronomical Journal 161 (6): 293. doi:10.3847/1538-3881/abf8bd. ISSN 0004-6256. Bibcode: 2021AJ....161..293J.
118. ↑ Han, Cheongho; Gould, Andrew; Hirao, Yuki; Lee, Chung-Uk; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil et al. (2021-11-01). "KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations". Astronomy and Astrophysics 655: A24. doi:10.1051/0004-6361/202141939. ISSN 0004-6361. Bibcode: 2021A&A...655A..24H. https://ui.adsabs.harvard.edu/abs/2021A&A...655A..24H.
119. ↑ Han, Cheongho; Udalski, Andrzej; Kim, Doeon; Kil Jung, Youn; Lee, Chung-Uk; Bond, Ian A.; Albrow, Michael D.; Chung, Sun-Ju et al. (2021-06-01). "KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars". The Astronomical Journal 161 (6): 270. doi:10.3847/1538-3881/abf4d0. ISSN 0004-6256. Bibcode: 2021AJ....161..270H.
120. ↑ Kim, Yun Hak et al. (2021). "KMT-2019-BLG-0371 and the Limits of Bayesian Analysis". The Astronomical Journal 162 (1): 17. doi:10.3847/1538-3881/abf930. Bibcode: 2021AJ....162...17K.
121. ↑ Han, Cheongho; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil; Kim, Doeon; Kim, Hyoun-Woo et al. (2021-08-01). "KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars". Astronomy and Astrophysics 652: A145. doi:10.1051/0004-6361/202140923. ISSN 0004-6361. Bibcode: 2021A&A...652A.145H. https://ui.adsabs.harvard.edu/abs/2021A&A...652A.145H.
122. ↑ Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil et al. (2021-05-01). "KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star". Astronomy and Astrophysics 649: A90. doi:10.1051/0004-6361/202039817. ISSN 0004-6361. Bibcode: 2021A&A...649A..90H. https://ui.adsabs.harvard.edu/abs/2021A&A...649A..90H.
123. ↑ Ryu, Yoon-Hyun; Hwang, Kyu-Ha; Gould, Andrew; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Jung, Youn Kil et al. (2021-09-01). "Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605". The Astronomical Journal 162 (3): 96. doi:10.3847/1538-3881/ac062a. ISSN 0004-6256. Bibcode: 2021AJ....162...96R.
124. ↑ Kuang, Renkun; Zang, Weicheng; Jung, Youn Kil; Udalski, Andrzej; Yang, Hongjing; Mao, Shude; Albrow, Michael D.; Chung, Sun-Ju et al. (2022-10-01). "OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system?". Monthly Notices of the Royal Astronomical Society 516 (2): 1704–1720. doi:10.1093/mnras/stac2315. ISSN 0035-8711. Bibcode: 2022MNRAS.516.1704K.
125. ↑ 125.0 125.1 125.2 125.3 125.4 125.5 Hwang, Kyu-Ha; Zang, Weicheng; Gould, Andrew; Udalski, Andrzej; Bond, Ian A.; Yang, Hongjing; Mao, Shude; Mao, Shude et al. (2022-02-01). "Systematic KMTNet Planetary Anomaly Search. II. Six New q < 2 × 10-4 Mass-ratio Planets". The Astronomical Journal 163 (2): 43. doi:10.3847/1538-3881/ac38ad. ISSN 0004-6256. Bibcode: 2022AJ....163...43H.
126. ↑ 126.0 126.1 Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Kim, Doeon; Zhu, Wei; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (2022-02-01). "OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star". Astronomy and Astrophysics 658: A93. doi:10.1051/0004-6361/202142327. ISSN 0004-6361. Bibcode: 2022A&A...658A..93H. https://ui.adsabs.harvard.edu/abs/2022A&A...658A..93H.
127. ↑ Chung, Sun-Ju; Yee, Jennifer C.; Udalski, Andrej; Gould, Andrew; Albrow, Michael D.; Jung, Youn Kil; Hwang, Kyu-Ha; Han, Cheongho et al. (2022-08-01). "OGLE-2019-BLG-0362Lb: A Super-Jovian-Mass Planet around a Low-Mass Star". Journal of the Korean Astronomical Society 55 (4): 123–130. doi:10.5303/JKAS.2022.55.4.123. ISSN 1225-4614. Bibcode: 2022JKAS...55..123C. https://ui.adsabs.harvard.edu/abs/2022JKAS...55..123C.
128. ↑ 128.0 128.1 128.2 128.3 128.4 Gould, Andrew; Han, Cheongho; Zang, Weicheng; Yang, Hongjing; Hwang, Kyu-Ha; Udalski, Andrzej; Bond, Ian A.; Albrow, Michael D. et al. (2022-08-01). "Systematic KMTNet planetary anomaly search. V. Complete sample of 2018 prime-field". Astronomy and Astrophysics 664: A13. doi:10.1051/0004-6361/202243744. ISSN 0004-6361. Bibcode: 2022A&A...664A..13G. https://ui.adsabs.harvard.edu/abs/2022A&A...664A..13G.
129. ↑ 129.0 129.1 129.2 129.3 129.4 129.5 Jung, Youn Kil; Zang, Weicheng; Han, Cheongho; Gould, Andrew; Udalski, Andrzej; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (2022-12-01). "Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets". The Astronomical Journal 164 (6): 262. doi:10.3847/1538-3881/ac9c5c. ISSN 0004-6256. Bibcode: 2022AJ....164..262J.
130. ↑ Wang, Hanyue; Zang, Weicheng; Zhu, Wei; Hwang, Kyu-Ha; Udalski, Andrzej; Gould, Andrew; Han, Cheongho; Albrow, Michael D. et al. (2022-02-01). "Systematic Korea Microlensing Telescope Network planetary anomaly search - III. One wide-orbit planet and two stellar binaries". Monthly Notices of the Royal Astronomical Society 510 (2): 1778–1790. doi:10.1093/mnras/stab3581. ISSN 0035-8711. Bibcode: 2022MNRAS.510.1778W.
131. ↑ 131.0 131.1 131.2 131.3 Han, Cheongho; Kim, Doeon; Gould, Andrew; Udalski, Andrzej; Bond, Ian A.; Bozza, Valerio; Jung, Youn Kil; Albrow, Michael D. et al. (2022-08-01). "Four sub-Jovian-mass planets detected by high-cadence microlensing surveys". Astronomy and Astrophysics 664: A33. doi:10.1051/0004-6361/202243484. ISSN 0004-6361. Bibcode: 2022A&A...664A..33H. https://ui.adsabs.harvard.edu/abs/2022A&A...664A..33H.
132. ↑ Zang, Weicheng; Shvartzvald, Yossi; Udalski, Andrzej; Yee, Jennifer C.; Lee, Chung-Uk; Sumi, Takahiro; Zhang, Xiangyu; Yang, Hongjing et al. (2022-08-01). "OGLE-2018-BLG-0799Lb: a q 2.7 × 10-3 planet with Spitzer parallax". Monthly Notices of the Royal Astronomical Society 514 (4): 5952–5968. doi:10.1093/mnras/stac1631. ISSN 0035-8711. Bibcode: 2022MNRAS.514.5952Z.
133. ↑ Shin, In-Gu; Yee, Jennifer C.; Hwang, Kyu-Ha; Gould, Andrew; Udalski, Andrzej; Bond, Ian A.; Albrow, Michael D.; Chung, Sun-Ju et al. (2022-06-01). "OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge". The Astronomical Journal 163 (6): 254. doi:10.3847/1538-3881/ac6513. ISSN 0004-6256. Bibcode: 2022AJ....163..254S.
134. ↑ Miyazaki, Shota; Suzuki, Daisuke; Udalski, Andrzej; Koshimoto, Naoki; Bennett, David P.; Sumi, Takahiro; Rattenbury, Nicholas; Cheongho, Han et al. (2022-03-01). "OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions". The Astronomical Journal 163 (3): 123. doi:10.3847/1538-3881/ac4960. ISSN 0004-6256. Bibcode: 2022AJ....163..123M.
135. ↑ Ishitani Silva, Stela; Ranc, Clément; Bennett, David P.; Bond, Ian A.; Zang, Weicheng; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna et al. (2022-09-01). "MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis". The Astronomical Journal 164 (3): 118. doi:10.3847/1538-3881/ac82b8. ISSN 0004-6256. Bibcode: 2022AJ....164..118I.
136. ↑ Bachelet, E.; Tsapras, Y.; Gould, Andrew; Street, R. A.; Bennett, David P.; Hundertmark, M. P. G.; Bozza, V.; Bramich, D. M. et al. (2022-09-01). "MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary". The Astronomical Journal 164 (3): 75. doi:10.3847/1538-3881/ac78ed. ISSN 0004-6256. Bibcode: 2022AJ....164...75B.
137. ↑ 137.0 137.1 137.2 Shin, In-Gu; Yee, Jennifer C.; Gould, Andrew; Hwang, Kyu-Ha; Yang, Hongjing; Bond, Ian A.; Albrow, Michael D.; Chung, Sun-Ju et al. (2023-01-01). "Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets". The Astronomical Journal 165 (1): 8. doi:10.3847/1538-3881/ac9d93. ISSN 0004-6256. Bibcode: 2023AJ....165....8S.
138. ↑ Han, Cheongho; Gould, Andrew; Kim, Doeon; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (2022-07-01). "KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars". Astronomy and Astrophysics 663: A145. doi:10.1051/0004-6361/202243102. ISSN 0004-6361. Bibcode: 2022A&A...663A.145H. https://ui.adsabs.harvard.edu/abs/2022A&A...663A.145H.
139. ↑ 139.0 139.1 Yang, Hongjing; Zang, Weicheng; Gould, Andrew; Yee, Jennifer C.; Hwang, Kyu-Ha; Christie, Grant; Sumi, Takahiro; Zhang, Jiyuan et al. (2022-10-01). "KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations". Monthly Notices of the Royal Astronomical Society 516 (2): 1894–1909. doi:10.1093/mnras/stac2023. ISSN 0035-8711. Bibcode: 2022MNRAS.516.1894Y.
140. ↑ 140.0 140.1 140.2 140.3 Ryu, Yoon-Hyun; Kil Jung, Youn; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha et al. (2022-11-01). "Mass Production of 2021 KMTNet Microlensing Planets. I". The Astronomical Journal 164 (5): 180. doi:10.3847/1538-3881/ac8d6c. ISSN 0004-6256. Bibcode: 2022AJ....164..180R.
141. ↑ 141.0 141.1 Han, Cheongho; Gould, Andrew; Bond, Ian A.; Kil Jung, Youn; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Ryu, Yoon-Hyun et al. (2022-06-01). "KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing". Astronomy and Astrophysics 662: A70. doi:10.1051/0004-6361/202243550. ISSN 0004-6361. Bibcode: 2022A&A...662A..70H. https://ui.adsabs.harvard.edu/abs/2022A&A...662A..70H.
142. ↑ Han, Cheongho; Bond, Ian A.; Yee, Jennifer C.; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew P.; Hwang, Kyu-Ha et al. (2022-02-01). "KMT-2021-BLG-0912Lb: a microlensing super Earth around a K-type star". Astronomy and Astrophysics 658: A94. doi:10.1051/0004-6361/202142495. ISSN 0004-6361. Bibcode: 2022A&A...658A..94H. https://ui.adsabs.harvard.edu/abs/2022A&A...658A..94H.
143. ↑ Han, Cheongho; Kim, Doeon; Yang, Hongjing; Gould, Andrew; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (2022-08-01). "KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal". Astronomy and Astrophysics 664: A114. doi:10.1051/0004-6361/202243161. ISSN 0004-6361. Bibcode: 2022A&A...664A.114H. https://ui.adsabs.harvard.edu/abs/2022A&A...664A.114H.
144. ↑ 144.0 144.1 144.2 Zang, Weicheng; Yang, Hongjing; Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Gould, Andrew; Mao, Shude; Zhang, Xiangyu et al. (2022-09-01). "Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field". Monthly Notices of the Royal Astronomical Society 515 (1): 928–939. doi:10.1093/mnras/stac1883. ISSN 0035-8711. Bibcode: 2022MNRAS.515..928Z.
145. ↑ Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Kil Jung, Youn; Kim, Doeon; Lee, Chung-Uk et al. (2022-02-01). "KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf". Astronomy and Astrophysics 658: A62. doi:10.1051/0004-6361/202142077. ISSN 0004-6361. Bibcode: 2022A&A...658A..62H. https://ui.adsabs.harvard.edu/abs/2022A&A...658A..62H.
146. ↑ 146.0 146.1 Han, Cheongho; Lee, Chung-Uk; Gould, Andrew; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Kim, Doeon et al. (2022-10-01). "KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey". Astronomy and Astrophysics 666: A132. doi:10.1051/0004-6361/202244438. ISSN 0004-6361. Bibcode: 2022A&A...666A.132H. https://ui.adsabs.harvard.edu/abs/2022A&A...666A.132H.
147. ↑ Chung, Sun-Ju; Udalski, Andrzej; Yee, Jennifer C.; Gould, Andrew; Albrow, Michael D.; Jung, Youn Kil; Hwang, Kyu-Ha; Han, Cheongho et al. (2023-12-01). "OGLE-2019-BLG-1180Lb: Discovery of a Wide-orbit Jupiter-mass Planet around a Late-type Star". The Astronomical Journal 166 (6): 253. doi:10.3847/1538-3881/ad0723. ISSN 0004-6256. Bibcode: 2023AJ....166..253C.
148. ↑ 148.0 148.1 148.2 148.3 148.4 Jung, Youn Kil; Zang, Weicheng; Wang, Hanyue; Han, Cheongho; Gould, Andrew; Udalski, Andrzej; Albrow, Michael D.; Chung, Sun-Ju et al. (2023-06-01). "Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets". The Astronomical Journal 165 (6): 226. doi:10.3847/1538-3881/accb8f. ISSN 0004-6256. Bibcode: 2023AJ....165..226J.
149. ↑ 149.0 149.1 149.2 149.3 149.4 149.5 149.6 Zang, Weicheng; Jung, Youn Kil; Yang, Hongjing; Zhang, Xiangyu; Udalski, Andrzej; Yee, Jennifer C.; Gould, Andrew; Mao, Shude et al. (2023-03-01). "Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10-4 Planets from the First 4 yr Survey". The Astronomical Journal 165 (3): 103. doi:10.3847/1538-3881/acb34b. ISSN 0004-6256. Bibcode: 2023AJ....165..103Z.
150. ↑ Han, Cheongho; Gould, Andrew; Jung, Youn Kil; Bond, Ian A.; Zang, Weicheng; Chung, Sun-Ju; Albrow, Michael D.; Hwang, Kyu-Ha et al. (2023-06-01). "MOA-2022-BLG-249Lb: Nearby microlensing super-Earth planet detected from high-cadence surveys". Astronomy and Astrophysics 674: A89. doi:10.1051/0004-6361/202346166. ISSN 0004-6361. Bibcode: 2023A&A...674A..89H. https://ui.adsabs.harvard.edu/abs/2023A&A...674A..89H.
151. ↑ Olmschenk, Greg; Bennett, David P.; Bond, Ian A.; Zang, Weicheng; Jung, Youn Kil; Yee, Jennifer C.; Bachelet, Etienne; Abe, Fumio et al. (2023-04-01). "MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert". The Astronomical Journal 165 (4): 175. doi:10.3847/1538-3881/acbcc8. ISSN 0004-6256. Bibcode: 2023AJ....165..175O.
152. ↑ 152.0 152.1 Han, Cheongho; Lee, Chung-Uk; Zang, Weicheng; Jung, Youn Kil; Christie, Grant W.; Zhang, Jiyuan; Albrow, Michael D.; Chung, Sun-Ju et al. (2023-06-01). "KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals". Astronomy and Astrophysics 674: A90. doi:10.1051/0004-6361/202346298. ISSN 0004-6361. Bibcode: 2023A&A...674A..90H. https://ui.adsabs.harvard.edu/abs/2023A&A...674A..90H.
153. ↑ Zhang, Jiyuan; Zang, Weicheng; Jung, Youn Kil; Yang, Hongjing; Gould, Andrew; Sumi, Takahiro; Mao, Shude; Dong, Subo et al. (2023-07-01). "KMT-2022-BLG-0440Lb: A new q < 10-4 microlensing planet with the central-resonant caustic degeneracy broken". Monthly Notices of the Royal Astronomical Society 522 (4): 6055–6069. doi:10.1093/mnras/stad1398. ISSN 0035-8711. Bibcode: 2023MNRAS.522.6055Z.
154. ↑ 154.0 154.1 154.2 154.3 Ryu, Yoon-Hyun; Shin, In-Gu; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha et al. (2023-03-01). "Mass Production of 2021 KMTNet Microlensing Planets II". The Astronomical Journal 165 (3): 83. doi:10.3847/1538-3881/acab6b. ISSN 0004-6256. Bibcode: 2023AJ....165...83R.
155. ↑ Han, Cheongho; Lee, Chung-Uk; Zang, Weicheng; Jung, Youn Kil; Christie, Grant W.; Zhang, Jiyuan; Albrow, Michael D.; Chung, Sun-Ju et al. (2023-06-01). "KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals". Astronomy and Astrophysics 674: A90. doi:10.1051/0004-6361/202346298. ISSN 0004-6361. Bibcode: 2023A&A...674A..90H. https://ui.adsabs.harvard.edu/abs/2023A&A...674A..90H.
156. ↑ Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D.; Gould, Andrew; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (2023-10-01). "Brown dwarf companions in binaries detected in the 2021 season high-cadence microlensing surveys". Astronomy and Astrophysics 678: A190. doi:10.1051/0004-6361/202347014. ISSN 0004-6361. Bibcode: 2023A&A...678A.190H. https://ui.adsabs.harvard.edu/abs/2023A&A...678A.190H.
157. ↑ Han, Cheongho; Zang, Weicheng; Jung, Youn Kil; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D.; Gould, Andrew; Hwang, Kyu-Ha et al. (2023-10-01). "KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity". Astronomy and Astrophysics 678: A101. doi:10.1051/0004-6361/202347366. ISSN 0004-6361. Bibcode: 2023A&A...678A.101H. https://ui.adsabs.harvard.edu/abs/2023A&A...678A.101H.
158. ↑ Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Chung, Sun-Ju; Albrow, Michael D.; Hwang, Kyu-Ha; Ryu, Yoon-Hyun et al. (2023-07-01). "KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal". Astronomy and Astrophysics 675: A36. doi:10.1051/0004-6361/202346596. ISSN 0004-6361. Bibcode: 2023A&A...675A..36H. https://ui.adsabs.harvard.edu/abs/2023A&A...675A..36H.
159. ↑ 159.0 159.1 159.2 Han, Cheongho; Kil Jung, Youn; Kim, Doeon; Gould, Andrew; Bozza, Valerio; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D. et al. (2023-07-01). "Probable brown dwarf companions detected in binary microlensing events during the 2018-2020 seasons of the KMTNet survey". Astronomy and Astrophysics 675: A71. doi:10.1051/0004-6361/202245455. ISSN 0004-6361. Bibcode: 2023A&A...675A..71H. https://ui.adsabs.harvard.edu/abs/2023A&A...675A..71H.
160. ↑ Specht, D.; Poleski, R.; Penny, M. T.; Kerins, E.; McDonald, I.; Lee, Chung-Uk; Udalski, A.; Bond, I. A. et al. (2023-04-01). "Kepler K2 Campaign 9 - II. First space-based discovery of an exoplanet using microlensing". Monthly Notices of the Royal Astronomical Society 520 (4): 6350–6366. doi:10.1093/mnras/stad212. ISSN 0035-8711. Bibcode: 2023MNRAS.520.6350S.
161. ↑ 161.0 161.1 161.2 Ryu, Yoon-Hyun; Udalski, Andrzej; Yee, Jennifer C.; Zang, Weicheng; Shvartzvald, Yossi; Han, Cheongho; Gould, Andrew; Albrow, Michael D. et al. (2024-03-01). "Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets". The Astronomical Journal 167 (3): 88. doi:10.3847/1538-3881/ad1888. ISSN 0004-6256. Bibcode: 2024AJ....167...88R.
162. ↑ Zhai, Ruocheng; Poleski, Radosław; Zang, Weicheng; Jung, Youn Kil; Udalski, Andrzej; Kuang, Renkun; Albrow, Michael D.; Chung, Sun-Ju et al. (April 2024). "OGLE-2017-BLG-0448Lb: A Low Mass–Ratio Wide-orbit Microlensing Planet?" (in en). The Astronomical Journal 167 (4): 162. doi:10.3847/1538-3881/ad284f. ISSN 0004-6256. Bibcode: 2024AJ....167..162Z.
163. ↑ 163.0 163.1 163.2 Shin, In-Gu; Yee, Jennifer C.; Zang, Weicheng; Han, Cheongho; Yang, Hongjing; Gould, Andrew; Lee, Chung-Uk; Udalski, Andrzej et al. (June 2024). "Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field Planets" (in en). The Astronomical Journal 167 (6): 269. doi:10.3847/1538-3881/ad3ba3. ISSN 0004-6256. Bibcode: 2024AJ....167..269S.
164. ↑ Kirikawa, Rintaro; Sumi, Takahiro; Bennett, David P.; Suzuki, Daisuke; Koshimoto, Naoki; Miyazaki, Shota; Bond, Ian A.; Udalski, Andrzej et al. (April 2024). "OGLE-2014-BLG-0221Lb: A Jupiter Mass Ratio Companion Orbiting Either a Late-type Star or a Stellar Remnant" (in en). The Astronomical Journal 167 (4): 154. doi:10.3847/1538-3881/ad2703. ISSN 0004-6256. Bibcode: 2024AJ....167..154K.
165. ↑ Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (March 2024). "Three sub-Jovian-mass microlensing planets: MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb" (in en). Astronomy and Astrophysics 683: A115. doi:10.1051/0004-6361/202347951. ISSN 0004-6361. Bibcode: 2024A&A...683A.115H.
166. ↑ Han, Cheongho; Ryu, Yoon-Hyun; Lee, Chung-Uk; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil et al. (December 2024). "KMT-2024-BLG-1044L: A sub-Uranus microlensing planet around a host at the star–brown dwarf mass boundary" (in en). Astronomy and Astrophysics 692: A106. doi:10.1051/0004-6361/202451620. ISSN 0004-6361. Bibcode: 2024A&A...692A.106H. https://ui.adsabs.harvard.edu/abs/2024A&A...692A.106H/abstract.
167. ↑ Han, Cheongho; Bond, Ian A.; Udalski, Andrzej; Lee, Chung-Uk; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (July 2024). "KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host" (in en). Astronomy and Astrophysics 687: A241. doi:10.1051/0004-6361/202449618. ISSN 0004-6361. Bibcode: 2024A&A...687A.241H. https://ui.adsabs.harvard.edu/abs/2024A&A...687A.241H/abstract.
168. ↑ Han, Cheongho; Bond, Ian A.; Udalski, Andrzej; Lee, Chung-Uk; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (November 2024). "Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons" (in en). Astronomy and Astrophysics 691: A237. doi:10.1051/0004-6361/202451416. ISSN 0004-6361. Bibcode: 2024A&A...691A.237H. https://ui.adsabs.harvard.edu/abs/2024A&A...691A.237H/abstract.
169. ↑ 169.0 169.1 Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha et al. (March 2024). "KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals" (in en). Astronomy and Astrophysics 683: A187. doi:10.1051/0004-6361/202348245. ISSN 0004-6361. Bibcode: 2024A&A...683A.187H. https://ui.adsabs.harvard.edu/abs/2024A&A...683A.187H/abstract.
170. ↑ Bell, Aislyn; Zhang, Jiyuan; Zang, Weicheng; Jung, Youn Kil; Yee, Jennifer C.; Yang, Hongjing; Sumi, Takahiro; Udalski, Andrzej et al. (May 2024). "KMT-2023-BLG-1431Lb: A New q < 10‑4 Microlensing Planet from a Subtle Signature" (in en). Publications of the Astronomical Society of the Pacific 136 (5): 054402. doi:10.1088/1538-3873/ad48b8. ISSN 0004-6280. Bibcode: 2024PASP..136e4402B. https://ui.adsabs.harvard.edu/abs/2024PASP..136e4402B/abstract.
171. ↑ 171.0 171.1 Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (March 2024). "Three sub-Jovian-mass microlensing planets: MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb" (in en). Astronomy and Astrophysics 683: A115. doi:10.1051/0004-6361/202347951. ISSN 0004-6361. Bibcode: 2024A&A...683A.115H.
172. ↑ Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha et al. (March 2024). "KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals" (in en). Astronomy and Astrophysics 683: A187. doi:10.1051/0004-6361/202348245. ISSN 0004-6361. Bibcode: 2024A&A...683A.187H. https://ui.adsabs.harvard.edu/abs/2024A&A...683A.187H/abstract.
173. ↑ Han, Cheongho; Bond, Ian A.; Udalski, Andrzej; Lee, Chung-Uk; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha et al. (November 2024). "Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons" (in en). Astronomy and Astrophysics 691: A237. doi:10.1051/0004-6361/202451416. ISSN 0004-6361. Bibcode: 2024A&A...691A.237H. https://ui.adsabs.harvard.edu/abs/2024A&A...691A.237H/abstract.
174. ↑ 174.0 174.1 Han, Cheongho; Albrow, Michael D.; Lee, Chung-Uk; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil; Ryu, Yoon-Hyun et al. (September 2024). "KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations" (in en). Astronomy and Astrophysics 689: A209. doi:10.1051/0004-6361/202450873. ISSN 0004-6361. Bibcode: 2024A&A...689A.209H. https://ui.adsabs.harvard.edu/abs/2024A&A...689A.209H/abstract.
175. ↑ Shin, In-Gu; Yee, Jennifer C.; Zang, Weicheng; Han, Cheongho; Yang, Hongjing; Gould, Andrew; Lee, Chung-Uk; Udalski, Andrzej et al. (June 2024). "Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field Planets" (in en). The Astronomical Journal 167 (6): 269. doi:10.3847/1538-3881/ad3ba3. ISSN 0004-6256. Bibcode: 2024AJ....167..269S.
176. ↑ Wu, Zexuan; Dong, Subo; Yi, Tuan; Liu, Zhuokai; El-Badry, Kareem; Gould, Andrew; Wyrzykowski, L.; Rybicki, K. A. et al. (August 2024). "Gaia22dkvLb: A Microlensing Planet Potentially Accessible to Radial-velocity Characterization" (in en). The Astronomical Journal 168 (2): 62. doi:10.3847/1538-3881/ad5203. ISSN 0004-6256. Bibcode: 2024AJ....168...62W.
177. ↑ 177.0 177.1 Yang 杨, Hongjing 弘靖; Yee, Jennifer C.; Zhang 张, Jiyuan 纪元; Lee, Chung-Uk; Kim, Dong-Jin; Bond, Ian A.; Udalski, Andrzej; Hwang, Kyu-Ha et al. (2025-06-02). "Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events". The Astronomical Journal 169 (6): 295. doi:10.3847/1538-3881/adc73e. ISSN 0004-6256. Bibcode: 2025AJ....169..295Y.
178. ↑ Ban, M.; Voloshyn, P.; Adomavic̆ienė, R.; Bachelet, E.; Bozza, V.; Brincat, S. M.; Bruni, I.; Burgaz, U. et al. (2025-05-01). "AT2021uey: A planetary microlensing event outside the Galactic bulge" (in en). Astronomy & Astrophysics 697: A57. doi:10.1051/0004-6361/202554236. ISSN 0004-6361. Bibcode: 2025A&A...697A..57B. https://www.aanda.org/articles/aa/full_html/2025/05/aa54236-25/aa54236-25.html.
179. ↑ 179.0 179.1 179.2 179.3 Han, Cheongho; Albrow, Michael D.; Lee, Chung-Uk; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil; Ryu, Yoon-Hyun et al. (2025-05-02). "Four Planets Found through Microlensing Events Involving Faint Source Stars" (in en). The Astronomical Journal 169 (6): 288. doi:10.3847/1538-3881/adc5e7. ISSN 0004-6256. Bibcode: 2025AJ....169..288H.
180. ↑ 180.0 180.1 180.2 Han, Cheongho; Bond, Ian A.; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (February 2025). "MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals" (in en). Astronomy & Astrophysics 694: A90. doi:10.1051/0004-6361/202452027. ISSN 0004-6361. Bibcode: 2025A&A...694A..90H. https://ui.adsabs.harvard.edu/abs/2025A&A...694A..90H/abstract.
181. ↑ 181.0 181.1 181.2 181.3 181.4 181.5 Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Bond, Ian A.; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Jung, Youn Kil et al. (October 2025). "Six microlensing planets detected via sub-day signals during the 2023–2024 season". Astronomy & Astrophysics 702: A152. doi:10.1051/0004-6361/202554557. ISSN 0004-6361. Bibcode: 2025A&A...702A.152H. https://www.aanda.org/10.1051/0004-6361/202554557.
182. ↑ 182.0 182.1 Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Ryu, Yoon-Hyun; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha et al. (August 2025). "KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet". Astronomy & Astrophysics 700: A181. doi:10.1051/0004-6361/202452760. ISSN 0004-6361. Bibcode: 2025A&A...700A.181H. https://www.aanda.org/10.1051/0004-6361/202452760.
183. ↑ Han, Cheongho; Lee, Chung-Uk; Bond, Ian A.; Udalski, Andrzej; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Jung, Youn Kil et al. (December 2025). "Six binary brown dwarf candidates identified by microlensing". Astronomy & Astrophysics 704: A236. doi:10.1051/0004-6361/202555605. ISSN 0004-6361. Bibcode: 2025A&A...704A.236H. https://www.aanda.org/10.1051/0004-6361/202555605.
184. ↑ 184.0 184.1 Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Bond, Ian A.; Yang, Hongjing; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew et al. (July 2025). "MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals". Astronomy & Astrophysics 699: A91. doi:10.1051/0004-6361/202554182. ISSN 0004-6361. Bibcode: 2025A&A...699A..91H. https://www.aanda.org/10.1051/0004-6361/202554182.
185. ↑ Mróz, M. J.; Poleski, R.; Udalski, A.; Sumi, T.; Tsapras, Y.; Hundertmark, M.; Pietrukowicz, P.; Szymański, M. K. et al. (June 2025). "OGLE-2015-BLG-1609Lb: A sub-Jovian planet orbiting a low-mass stellar or brown dwarf host". Astronomy & Astrophysics 698: A126. doi:10.1051/0004-6361/202453454. ISSN 0004-6361. Bibcode: 2025A&A...698A.126M. https://www.aanda.org/10.1051/0004-6361/202453454.
186. ↑ Zang, Weicheng; Jung, Youn Kil; Yee, Jennifer C.; Hwang, Kyu-Ha; Yang, Hongjing; Udalski, Andrzej; Sumi, Takahiro; Gould, Andrew et al. (2025-04-25). "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits" (in en). Science 388 (6745): 400–404. doi:10.1126/science.adn6088. ISSN 0036-8075. PMID 40273242. Bibcode: 2025Sci...388..400Z. https://www.science.org/doi/10.1126/science.adn6088.
187. ↑ 187.0 187.1 Li, Hongyu; Zhang, Jiyuan; Han, Cheongho; Zang, Weicheng; Jung, Youn Kil; Udalski, Andrzej; Sumi, Takahiro; Yang, Hongjing et al. (2026-01-02). "KMT-2022-BLG-1818Lb,c: A Cold Super-Jupiter with a Saturn Sibling". The Astronomical Journal 171 (1): 41. doi:10.3847/1538-3881/ae1b8f. ISSN 0004-6256. Bibcode: 2026AJ....171...41L.
188. ↑ Freeman, M.; Philpott, L. C.; Abe, F.; Albrow, M. D.; Bennett, D. P.; Bond, I. A.; Botzler, C. S.; Bray, J. C. et al. (2014). "Can the masses of isolated planetary-mass gravitational lenses be measured by terrestrial parallax?". The Astrophysical Journal 799 (2): 181. doi:10.1088/0004-637X/799/2/181. Bibcode: 2015ApJ...799..181F.
189. ↑ Mróz, Przemek et al. (2018). "A Neptune-mass Free-floating Planet Candidate Discovered by Microlensing Surveys". The Astronomical Journal 155 (3): 121. doi:10.3847/1538-3881/aaaae9. Bibcode: 2018AJ....155..121M.
190. ↑ 190.0 190.1 Mróz, Przemek et al. (2019). "Two new free-floating or wide-orbit planets from microlensing". Astronomy & Astrophysics 622: A201. doi:10.1051/0004-6361/201834557. Bibcode: 2019A&A...622A.201M.
191. ↑ Mróz, Przemek et al. (2020). "A Free-floating or Wide-orbit Planet in the Microlensing Event OGLE-2019-BLG-0551". The Astronomical Journal 159 (6): 262. doi:10.3847/1538-3881/ab8aeb. Bibcode: 2020AJ....159..262M.
192. ↑ Kim, Hyoun-Woo; Hwang, Kyu-Ha; Gould, Andrew; Yee, Jennifer C.; Ryu, Yoon-Hyun; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho et al. (2021). "KMT-2019-BLG-2073: Fourth Free-floating Planet Candidate with θ e < 10 μas". The Astronomical Journal 162 (1): 15. doi:10.3847/1538-3881/abfc4a. Bibcode: 2021AJ....162...15K.
193. ↑ Mróz, Przemek et al. (2020). "A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event". The Astrophysical Journal Letters 903 (1): L11. doi:10.3847/2041-8213/abbfad. Bibcode: 2020ApJ...903L..11M.
194. ↑ Ryu, Yoon-Hyun et al. (2021). "KMT-2017-BLG-2820 and the Nature of the Free-floating Planet Population". The Astronomical Journal 161 (3): 126. doi:10.3847/1538-3881/abd55f. Bibcode: 2021AJ....161..126R.
195. ↑ Han, Cheongho; Bennett, David P.; Udalski, Andrzej; Jung, Youn Kil (2016). "A New Nonplanetary Interpretation of the Microlensing Event Ogle-2013-BLG-0723". The Astrophysical Journal 825 (1): 8. doi:10.3847/0004-637X/825/1/8. Bibcode: 2016ApJ...825....8H.

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