List of exoplanets detected by microlensing

Source: Wikipedia, the free encyclopedia.

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 7 known multi-planetary systems detected by microlensing, all of which have two planets.[5]

List

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

Planet
 Mass (MJ)
AU
) 		Period (d) Eccentricity
Inclination
(°) 		Year of discovery
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]

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[179]
OGLE-2016-BLG-1540L ~35 M🜨 2017[180]
OGLE-2012-BLG-1323L ~2.3 M🜨 2018[181]
OGLE-2017-BLG-0560L ~1.9 MJ 2018[181]
OGLE-2019-BLG-0551L ~7.7 M🜨 2020[182]
KMT-2019-BLG-2073L ~59 M🜨 2020[183]
OGLE-2016-BLG-1928L ~0.3 M🜨 2020[184]
KMT-2017-BLG-2820L ~8.2 M🜨 2020[185]

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.[186]

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 M🜨 exomoon or a red dwarf with 18 M🜨 planet.

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    .
  47. S2CID 119105208
    .
  48. S2CID 119309343
    .
  49. S2CID 54034608
    .
  50. doi:10.1093/mnras/stw3185
    .
  51. S2CID 39292551
    .
  52. doi:10.3847/1538-3881/adcec2
    .
  53. S2CID 119077625
    .
  54. S2CID 56306676
    .
  55. S2CID 39514486
    .
  56. ^
    S2CID 119093055
    .
  57. S2CID 56010958
    .
  58. S2CID 119012722
    .
  59. S2CID 54706921
    .
  60. ISSN 0004-637X
    .
  61. ISSN 0035-8711
    .
  62. ISSN 0004-637X
    .
  63. ISSN 0004-6256
    .
  64. ISSN 0004-6256
    .
  65. doi:10.32023/0001-5237/68.1.1
    .
  66. ISSN 0004-6256
    .
  67. ISSN 0004-6256
    .
  68. ISSN 0001-5237
    .
  69. ISSN 0004-6256
    .
  70. ^
    ISSN 0004-6256
    .
  71. ISSN 0004-6256
    .
  72. ISSN 0004-6256
    .
  73. ISSN 0004-6256
    .
  74. ISSN 0004-6256
    .
  75. ISSN 0004-6256
    .
  76. ISSN 0004-6256
    .
  77. ISSN 0004-6256
    .
  78. ^
    ISSN 0004-6256
    .
  79. ISSN 0004-6256
    .
  80. ISSN 1225-4614
    .
  81. ^
    ISSN 0004-6256
    .
  82. ISSN 0004-6256
    .
  83. ISSN 0004-6256
    .
  84. ISSN 0004-6256
    .
  85. ISSN 0004-6256
    .
  86. ISSN 0004-6256
    .
  87. ISSN 0004-6256
    .
  88. S2CID 145052576
    .
  89. ISSN 0004-6256
    .
  90. ^
    ISSN 0004-6256
    .
  91. ISSN 0004-6256
    .
  92. ISSN 0004-6256
    .
  93. ISSN 0004-6256
    .
  94. ISSN 0004-6256
    .
  95. ISSN 0004-6256
    .
  96. ISSN 0004-6256
    .
  97. ^
    ISSN 0004-6361
    .
  98. ISSN 1225-4614
    .
  99. ISSN 0004-6256
    .
  100. ISSN 0004-6256
    .
  101. ISSN 0004-6256
    .
  102. ISSN 0004-6256
    .
  103. ISSN 0004-6256
    .
  104. ISSN 0004-6256
    .
  105. ISSN 0004-6256
    .
  106. ISSN 0004-6256
    .
  107. ISSN 0004-6256
    .
  108. ISSN 0004-6361
    .
  109. ISSN 1225-4614
    .
  110. ISSN 0004-6256
    .
  111. ISSN 0004-6256
    .
  112. ^
    ISSN 0004-6361
    .
  113. ISSN 0004-6256
    .
  114. ^
    ISSN 0004-6361
    .
  115. ISSN 0035-8711
    .
  116. ISSN 0004-6256
    .
  117. ^
    ISSN 0004-6256
    .
  118. ISSN 0004-6361
    .
  119. ISSN 0004-6256
    .
  120. S2CID 231728667
    .
  121. ISSN 0004-6361
    .
  122. ISSN 0004-6361
    .
  123. ISSN 0004-6256
    .
  124. ISSN 0035-8711
    .
  125. ^
    ISSN 0004-6256
    .
  126. ^
    ISSN 0004-6361
    .
  127. ISSN 1225-4614
    .
  128. ^
    ISSN 0004-6361
    .
  129. ^
    ISSN 0004-6256
    .
  130. ISSN 0035-8711
    .
  131. ^
    ISSN 0004-6361
    .
  132. ISSN 0035-8711
    .
  133. ISSN 0004-6256
    .
  134. ISSN 0004-6256
    .
  135. ISSN 0004-6256
    .
  136. ISSN 0004-6256
    .
  137. ^
    ISSN 0004-6256
    .
  138. ISSN 0004-6361
    .
  139. ^
    ISSN 0035-8711
    .
  140. ^
    ISSN 0004-6256
    .
  141. ^
    ISSN 0004-6361
    .
  142. ISSN 0004-6361
    .
  143. ISSN 0004-6361
    .
  144. ^
    ISSN 0035-8711
    .
  145. ISSN 0004-6361
    .
  146. ^
    ISSN 0004-6361
    .
  147. ISSN 0004-6256
    .
  148. ^
    ISSN 0004-6256
    .
  149. ^
    ISSN 0004-6256
    .
  150. ISSN 0004-6361
    .
  151. ISSN 0004-6256
    .
  152. ^
    ISSN 0004-6361
    .
  153. ISSN 0035-8711
    .
  154. ^
    ISSN 0004-6256
    .
  155. ISSN 0004-6361
    .
  156. ISSN 0004-6361
    .
  157. ISSN 0004-6361
    .
  158. ISSN 0004-6361
    .
  159. ^
    ISSN 0004-6361
    .
  160. ISSN 0035-8711
    .
  161. ^
    ISSN 0004-6256
    .
  162. ISSN 0004-6256
    .
  163. ^
    ISSN 0004-6256
    .
  164. ISSN 0004-6256
    .
  165. ISSN 0004-6361
    .
  166. ISSN 0004-6361
    .
  167. ISSN 0004-6361
    .
  168. ISSN 0004-6361
    .
  169. ^
    ISSN 0004-6361
    .
  170. ISSN 0004-6280
    .
  171. ^
    ISSN 0004-6361
    .
  172. ISSN 0004-6361
    .
  173. ISSN 0004-6361
    .
  174. ^
    ISSN 0004-6361
    .
  175. ISSN 0004-6256
    .
  176. ISSN 0004-6256
    .
  177. ^
    ISSN 0004-6256
    .
  178. ISSN 0004-6361
    .
  179. S2CID 118415208
    .
  180. S2CID 118894684
    .
  181. ^
    S2CID 119396791
    .
  182. S2CID 211817861
    .
  183. S2CID 235445277
    .
  184. S2CID 221971000
    .
  185. S2CID 222378863
    .
  186. S2CID 119282899
    .
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