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Lista de exoplanetas descobertos em 2011

Esta é uma Lista de exoplanetas descobertos em 2011.[1]

Para exoplanetas detectados apenas pela velocidade radial, o valor da massa é na verdade um limite inferior. (Consulte a massa mínima para obter mais informações)

Nome Massa (MJ) Raio (RJ) Período (dais) Semieixo maior (AU) Temp. (K) Método de descoberta Distância (ly) Massa da estrela-mãe (M☉) Temperatura da estrela-mãe (K) Observações
7 Canis Majoris b 1.85 735.1 1.758 Vel. radial 64.65 1.34 4826 [2]
82 G. Eridani b 0.0085 18.315 0.1207 660 Vel. radial 19.57 0.7 5401 [3]
82 G. Eridani c 0.0076 40.114 0.2036 508 Vel. radial 19.57 0.7 5401 [3]
82 G. Eridani d 0.015 90.309 0.3499 388 Vel. radial 19.57 0.7 5401 [3]
BD+48 738 b 0.91 392.6 1.0 Vel. radial 2910 0.74 4414 [4]
CFBDSIR J145829+101343 b 10.5 10037.5 2.6 370 Imagem direta 75.34 0.02 580 Provavelmente anã marrom[5]
COCONUTS-2b 6.3+1.5
−1.9 		400000000 7506+5205
−2060 		434±9 Imagem direta 35.6 0.37±0.02 3406±69 Exoplaneta também catalogado como WISEPA J075108.79−763449.6,[6] em 2021, também o exoplaneta com o período orbital mais longo
CoRoT-16b 0.535 1.17 5.35227 0.0618 1086 Trânsito 2740 1.1 5650 [7]
CoRoT-17b 2.43 1.02 3.7681 0.0461 1626 Trânsito 3001 1.04 5740 [8]
CoRoT-18b 3.47 1.31 1.9000693 0.0295 1550 Trânsito 2838 0.95 5440 [9]
CoRoT-19b 1.11 1.29 3.89713 0.0518 2000 Trânsito 2511 1.21 6090 [10]
CoRoT-20b 4.3 0.84 9.24285 0.09 1024 Trânsito 2819 1.14 4947 [11]
COROT-21b 2.26±0.31 1.30±0.14 2.72474±0.00014 0.0417±0.0011 Trânsito 4560±930 1.29±0.09 6200±100 [12]
CoRoT-23b 2.8 1.05 3.6313 0.048 1660 Trânsito 1957 1.14 5900 [13]
Gliese 433 b 0.01901 7.3705 0.062 Vel. radial 29.58 0.48 3461 [14]
Gliese 667 Cc 0.012 28.14 0.125 Vel. radial 22.18 0.33 3350 [14]Exoplaneta potencialmente habitável
Gliese 785 b 0.0532 74.72 0.32 355 Vel. radial 28.7 0.8 5166 [3]
Gliese 785 c 0.076 525.8 1.18 185 Vel. radial 28.7 0.8 5166 [3]
HAT-P-27b 0.62 1.02 3.039577 0.04 Trânsito 665.38 0.94 5300 [15]
HAT-P-28b 0.626 1.212 3.257215 0.0434 1384 Trânsito 1288 1.02 5680 [16]
HAT-P-29b 0.88 1.17 5.72319 0.0667 1271 Trânsito 1032 1.45 6087 [16] Nome próprio Surt
HAT-P-30b 0.83 1.44 2.8106 0.0419 1630 Trânsito 702.2 1.55 6304 Descoberta independente[17][18]
HAT-P-31b 2.27 1.09 5.00542 0.061 1450 Trânsito 1133 1.31 6065 Suspeita-se de exoplaneta adicional no sistema.[19]
HAT-P-32b 0.68 1.98 2.1500082 0.03397 1836 Trânsito 950.81 1.13 6001 [20]
HAT-P-33b 0.92 1.85 3.47447 0.04995 1782 Trânsito 1306 1.82 6446 [20]
HD 1461 c 0.01759 13.5052 0.1117 Vel. radial 76.5 1.02 5765 [21]Exoplaneta confirmado em 2015[22]
HD 1502 b 2.75 428.5 1.262 Vel. radial 626.11 1.46 4947 [23]Nome próprio Indépendance
HD 5891 b 7.63 177.11 0.64 Vel. radial 932.02 1.93 4673 [23]
HD 7199 b 0.27 615 1.36 Vel. radial 118.04 0.77 5371 [24]Nome próprio Hairu
HD 7449 A b 0.508 1255.5 2.38 Vel. radial 126.26 1.05 6024 [24]
HD 14651 b 47±3.4 79.4179±0.0021 0.361±0.013 Vel. radial 127 0.96±0.03 5491±26 Anã marrom ou estrela[25]
HD 18742 b 3.4 766 1.82 Vel. radial 532.86 1.36 4940 [23]Nome próprio Bagan
HD 20003 b 0.0378±0.0031 11.849±0.003 0.0974±0.0016 Vel. radial 136.6±0.2 0.942±0.046 5510+48
−137 		[21]
HD 20003 c 0.0422±0.0040 33.823±0.065 0.1961±0.0032 Vel. radial 136.6±0.2 0.942±0.046 5510+48
−137 		[21]
HD 20781 b 0.0334+0.0038
−0.0037 		29.158+0.0102
−0.01 		0.1647+0.0076
−0.0083 		Vel. radial 115.36±4.4 0.7 5256±29 [21]
HD 20781 c 0.0442±0.0049 85.5073+0.0983
−0.0947 		0.3374+0.0155
−0.017 		Vel. radial 115.36±4.4 0.7 5256±29 [21]
HD 21693 b 0.0259+0.0034
−0.0033 		0.1976 22.6786+0.0085
−0.0087 		0.1455+0.0058
−0.0063 		Vel. radial 105.61±1.66 0.8 5430±26 [21]Confirmado em 2017.[26]
HD 21693 c 0.0547±0.0056 53.7357+0.0312
−0.0309 		0.2586+0.0103
−0.0113 		Vel. radial 105.61±1.66 0.8 5430±26 [21]Confirmado em 2017.[26]
HD 22781 b 13.65 528.07 1.167 Vel. radial 106.43 0.75 5027 [25]
HD 28678 b 1.542 380.2 1.18 Vel. radial 622.72 1.53 4972 [23]Nome próprio Tassili
HD 30246 b 55.1+20.3
−8.2 		990.7±5.6 2.012±0.069 Vel. radial 160 1.05±0.04 5833±44 Anã marrom ou estrela[25]
HD 30856 b 1.547 847 1.85 Vel. radial 429.56 1.17 4895 [23]Nome próprio Nakanbé
HD 31527 b 0.0329±0.0028 16.5535+0.0034
−0.0035 		0.1254+0.0041
−0.0045 		Vel. radial 125.8±2.9 0.96 5898±13 [21]Confirmado em 2017.[26]
HD 31527 c 0.0445±0.0040.0039 51.2053+0.0373
−0.0368 		0.2663+0.0088
−0.0095 		Vel. radial 125.8±2.9 0.96 5898±13 [21]Confirmado em 2017.[26]
HD 31527 d 0.0372+0.0053
−0.0052 		271.6737+2.1135
−2.2471 		0.8098+0.0273
−0.0293 		Vel. radial 125.8±2.9 0.96 5898±13 [21]Confirmado em 2017.[26]
HD 33142 b 1.385 326 1.07 Vel. radial 397.27 1.41 4978 [23]
HD 39194 b 0.0126 5.63 0.056±0.001 Vel. radial 71.43 0.67±0.04 5205±23 [21]Confirmado em 2017 e 2021.[27][28]
HD 39194 c 0.0198 14.03 0.103±0.002 Vel. radial 71.43 0.67±0.04 5205±23 [21]Confirmado em 2017 e 2021.[27][28]
HD 39194 d 0.0126 33.91 0.185±0.033 Vel. radial 71.43 0.67±0.04 5205±23 [21]Confirmado em 2017 e 2021.[27][28]
HD 45184 b 0.0384+0.0033
−0.0032 		5.8854±0.0003 0.0644+0.002
−0.0021 		Vel. radial 71.36±0.62 1.03 5869±14 [21]Confirmado em 2017.[27]
HD 51608 b 0.0402+0.0038
−0.0037 		14.0726±0.0016 0.1059+0.0043
−0.0046 		Vel. radial 113.6±2.02 0.8 5358±22 [21]Confirmado em 2017.[27][26]
HD 51608 c 0.045+0.0051
−0.0048 		95.9446+0.1555
−0.1366 		0.3809+0.0153
−0.0164 		Vel. radial 113.6±2.02 0.8 5358±22 [21]Confirmado em 2017.[27][26]
HD 82886 b 2.33 705 1.58 Vel. radial 415.93 2.53 4953 [23]Nome próprio Arber
HD 85512 b 0.01 58.43 0.26 298 Vel. radial 36.79 0.43 4300 [3]
HD 93385 Ac 0.0223 13.18 0.112±0.002 Vel. radial 141.6±0.2 1.04±0.01 5823±35 [21]Originalmente exoplaneta HD 93385 b, confirmado em 2017,[27] renomeado em 2021[28]
HD 93385 Ad 0.0274 45.84 0.2565±0.0043 Vel. radial 141.6±0.2 1.04±0.01 5823±35 [21]Originalmente exoplaneta HD 93385 c, confirmado em 2017,[27] renomeado em 2021.[28]
HD 96063 b 1.27 362.5 1.11 Vel. radial 458.66 1.37 5020 [23]Nome próprio Ramajay
HD 96127 b 20.96 647.3 1.42 Vel. radial 1949 10.94 3943 [4]Provavelmente não é um exoplaneta, mas uma estrela[29]
HD 96700 b 0.0280 8.12 0.0777±0.0013 Vel. radial 84±1 0.89±0.01 5845±13 [21]Exoplaneta não confirmado entre as órbitas b e c[28]
HD 96700 c 0.0400 103.5 0.424±0.007 Vel. radial 84±1 0.89±0.01 5845±13 [21]Exoplaneta não confirmado entre as órbitas b e c[28]
HD 98219 b 1.964 433.8 1.26 Vel. radial 372.06 1.41 4925 [23]Nome próprio Ixbalanqué
HD 99706 b 1.23 841 1.98 Vel. radial 480.15 1.46 4862 [23]
HD 100655 b 1.61 157.57001 0.68 Vel. radial 449.2 2.28 4891 [30] Nome próprio Sazum
HD 102329 b 8.16 778.1 1.81 Vel. radial 712.41 3.21 4745 [23]
HD 106270 b 10.13 1888 3.34 Vel. radial 306.79 1.39 5509 [23]
HD 108863 b 2.414 437.7 1.32 Vel. radial 539.87 1.59 4878 [23]
HD 116029 b 1.4 670 1.65 Vel. radial 403.4 0.83 4819 [23]Mais um planeta no sistema (não confirmado)
HD 126525 b 0.237±0.002 960.41+6.19
−6.33 		1.837±0.010 Vel. radial 124.1+4.3
−4.6 		0.90±0.01 5638±13 [21]
HD 131496 b 1.8 896 2.01 Vel. radial 431.65 1.34 4846 [23]Nome próprio Madriu
HD 132563 Bb 1.49 1544 2.62 Vel. radial 344.01 1.08 6073 [31]
HD 134060 b 0.0318+0.0025
−0.0024 		3.2696±0.0001 0.0444±0.0007 Vel. radial 78.38±0.07 1.095 5966±14 [21]Órbita excêntrica, confirmada em 2017.[26]
HD 134060 c 0.0922+0.0139
−0.0133 		1292+48
−44 		2.226±0.051 Vel. radial 78.38±0.07 1.095 5966±14 [21]Confirmado em 2017.[26]
HD 134606 b 0.0292±0.0030 12.083±0.010 0.1023±0.0017 Vel. radial 87.45±0.07 0.998±0.024 5616±34 [21]
HD 134606 c 0.0382±0.0053 59.52±0.17 0.2962±0.0049 Vel. radial 87.45±0.07 0.998±0.024 5616±34 [21]
HD 134606 d 0.1212±0.0130 459.3±8.3 1.157±0.024 Vel. radial 87.45±0.07 0.998±0.024 5616±34 [21]
HD 137388 b 0.2 330 0.89 Vel. radial 132.2 0.68 5181 [24]Nome próprio Kererū
HD 142245 b 3.07 1299 2.78 Vel. radial 318.01 3.5 4922 [23]
HD 152581 b 1.869 686.5 1.66 Vel. radial 543.2 1.3 5027 [23]Nome próprio Ganja
HD 156279 b 9.88 131.05 0.49 Vel. radial 118.17 0.95 5453 [25]
HD 158038 b 1.53 521 1.5 Vel. radial 310.25 1.3 4860 [23]
HD 150433 b 0.168±0.020 1096±27 1.930±0.045 Vel. radial 99.36±0.10 [21]
HD 154088 b 0.0208 18.56±0.01 0.134±0.002 Vel. radial 58.2±0.5 0.91±0.02 5374±43 [21]Confirmado em 2021.[28]
HD 157172 b 0.12 104.84±0.13 0.416±0.007 Vel. radial 107.75±0.22 [21]
HD 163607 b 0.7836 75.2203 0.362 Vel. radial 221.53 1.12 5522 [32]
HD 163607 c 2.201 1272 2.39 Vel. radial 221.53 1.12 5522 [32]
HD 164509 b 0.443 280.17 0.87 Vel. radial 173.49 1.12 5922 [32]
HD 189567 b 0.0267 14.3 0.111±0.002 Vel. radial 58.43±0.04 0.83±0.01 5726±15 [21]Confirmado em 2021, exoplaneta HD 189567 c não confirmado no sistema[28]
HD 192310 c 0.076 525.8 1.18 Vel. radial 28.7 0.78 5069 [3]
HD 204313 c 0.0553 34.905 0.2099 Vel. radial 154 1.02 5776 [21] Confirmed in 2015.[22]
HD 215152 c 0.0054+0.0019
−0.0023 		7.2824+0.0045
−0.0083 		0.06739+0.00086
−0.00089 		Vel. radial 70.48±0.16 0.770±0.015 4935±76 [21]Confirmed in 2018.[33]
HD 215152 d 0.0088+0.0025
−0.0029 		10.8650+0.0056
−0.0061 		0.0880+0.0011
−0.0012 		Vel. radial 70.48±0.16 0.770±0.015 4935±76 [21]Confirmado em 2018.[33]
HD 204941 b 0.266 1733 2.55 Vel. radial 93.74 0.58 5026 [24]
HD 215456 b 0.101 191.99±0.73 0.652±0.011 Vel. radial 129.3±0.2 [21]
HD 215456 c 0.246 2277±67 3.394±0.088 Vel. radial 129.3±0.2 [21]
HD 240237 b 15.89 745.7 1.92 Vel. radial 3125 8.76 3926 [4]
HIP 5158 c 15.04 9017.76 7.7 Vel. radial 168.56 0.78 4962 [34]
HIP 57274 b 0.02 8.1352 0.07 Vel. radial 84.41 0.29 4510 [35]
HIP 57274 c 0.40902 32.03 0.178 Vel. radial 84.41 0.29 4510 [35]
HIP 57274 d 0.5267 431.7 1.01 Vel. radial 84.41 0.29 4510 [35]
HU Aquarii b 5.9 2390 3.6 Tempo 626.89 0.88 5952 Controverso
HU Aquarii c 4.5 4368 5.4 Tempo 626.89 0.88 5952 Controverso
Kepler-10b 0.0145 0.132 0.837491 0.0172 2130 Trânsito 608.3 0.91 5708 [36]
Kepler-10c 0.02319 0.207 45.2946 0.241 584 Trânsito 608.3 0.91 5708 [37]
Kepler-11b 0.006 0.161 10.3039 0.091 Trânsito 2148 0.96 5663 [38]
Kepler-11c 0.009 0.256 13.0241 0.107 Trânsito 2148 0.96 5663 [38]
Kepler-11d 0.023 0.278 22.6845 0.155 Trânsito 2148 0.96 5663 [38]
Kepler-11e 0.025 0.374 31.9996 0.195 Trânsito 2148 0.96 5663 [38]
Kepler-11f 0.006 0.222 46.6888 0.25 Trânsito 2148 0.96 5663 [38]
Kepler-11g 0.079 0.297 118.3807 0.466 Trânsito 2148 0.96 5663 [38]
Kepler-12b 0.432 1.754 4.4379629 0.0553 1480 Trânsito 2950 1.17 5947 [39]
Kepler-13b 9.28 1.512 1.763588 0.03641 2550 Trânsito 1354 1.72 7650 [40]
Kepler-14b 8.4 1.136 6.790123 0.0771 1605 Trânsito 3196 1.51 6395 [41]
Kepler-15b 0.66 0.96 4.942782 0.05714 1251 Trânsito 2464 1.02 5515 [42]
Kepler-16b 0.333 0.754 228.776 0.7048 Trânsito 245.44 0.69 4450 [43]
Kepler-17b 2.45 1.31 1.4857108 0.02591 1570 Trânsito 2609 1.16 5781 [44]
Kepler-18b 0.022 0.178 3.504725 0.0447 Trânsito 1430 0.97 5345 [45]
Kepler-18c 0.054 0.49 7.64159 0.0752 Trânsito 1430 0.97 5345 [45]
Kepler-18d 0.052 0.623 14.85888 0.1172 Trânsito 1430 0.97 5345 [45]
Kepler-19b 0.02643 0.197 9.28716 0.085 Trânsito 717.4 0.94 5544 [46]
Kepler-19c 0.04122 28.731 Tempo 717.4 0.94 5544 [46]
Kepler-20b 0.03052 0.167 3.69611525 0.0463 1105 Trânsito 929.18 0.95 5495 [47]
Kepler-20c 0.04012 0.272 10.85409089 0.0949 772 Trânsito 929.18 0.95 5495 [47]
Kepler-20d 0.03168 0.245 77.61130017 0.3506 401 Trânsito 929.18 0.95 5495 [47]
Kepler-20e 0.01 0.077 6.09852281 0.0639 1040 Trânsito 929.18 0.95 5495 [47]
Kepler-20f 0.045 0.089 19.57758478 0.1396 705 Trânsito 929.18 0.95 5495 [47]
Kepler-21b 0.01598 0.146 2.78578 0.042717 2025 Trânsito 370 1.41 6305 [48]
Kepler-22b 0.113 0.212 289.8623 0.849 262 Trânsito 619.72 0.97 5518 Exoplaneta potencialmente habitável[49]
Kepler-23b 0.8 0.17 7.1073 0.075 Trânsito 2793 1.1 5828 [50]
Kepler-23c 2.7 0.285 10.7421 0.099 Trânsito 2793 1.1 5828 [50]
Kepler-24b 1.6 0.214 8.1453 0.08 Trânsito 3901 0.98 5897 [50]
Kepler-24c 1.6 0.25 12.3335 0.106 Trânsito 3901 0.98 5897 [50]
Kepler-25b 0.0275 0.245 6.238297 0.068 Trânsito 798.98 1.19 6270 [51]
Kepler-25c 0.0479 0.465 12.7207 0.11 Trânsito 798.98 1.19 6270 [51]
Kepler-26b 0.01611 0.248 12.28 0.08551 427 Trânsito 1104 0.54 3914 [51]
Kepler-26c 0.01951 0.243 17.2559 0.10725 381 Trânsito 1104 0.54 3914 [51]
Kepler-27b 9.11 0.357 15.3348 0.118 Trânsito 3507 0.65 5400 [51]
Kepler-27c 13.8 0.437 31.3309 0.191 Trânsito 3507 0.65 5400 [51]
Kepler-28b 1.51 0.321 5.9123 0.062 583 Trânsito 1448 0.75 4590 [51]
Kepler-28c 1.36 0.303 8.9858 0.081 507 Trânsito 1448 0.75 4590 [51]
Kepler-29b 0.01419 0.299 10.3384 0.09 Trânsito 2779 0.98 5701 [52]
Kepler-29c 0.01259 0.28 13.2884 0.11 Trânsito 2779 0.98 5701 [52]
Kepler-31b 0.491 20.8613 0.16 Trânsito 5700 1.21 6340 [53]
Kepler-31c 4.7 0.473 42.6318 0.26 Trânsito 5700 1.21 6340 [53]
Kepler-32b 4.1 0.196 5.90124 0.05 530 Trânsito 1066 0.58 3900 [53]
Kepler-32c 0.5 0.178 8.7522 0.09 470 Trânsito 1066 0.58 3900 [53]
Kepler-33b 0.155 5.66793 0.0677 Trânsito 4086 1.29 5904 [54]
Kepler-33c 0.00123 0.285 13.17562 0.1189 Trânsito 4086 1.29 5904 [54]
Kepler-33d 0.0123 0.477 21.77596 0.1662 Trânsito 4086 1.29 5904 [54]
Kepler-33e 0.01753 0.359 31.7844 0.2138 Trânsito 4086 1.29 5904 [54]
Kepler-39b 20.1 1.24 21.08721 0.164 897 Trânsito 3557 1.29 6350 [55] Anã marrom
Kepler-41b 0.56 1.29 1.8555582 0.03101 1790 Trânsito 3680 1.15 5750 [56]
Kepler-42b 0.07 1.2137672 0.0116 519 Trânsito 126.23 0.13 3068 [37]
Kepler-42c 0.065 0.45328509 0.006 720 Trânsito 126.23 0.13 3068 [37]
Kepler-42d 0.051 1.865169 0.0154 450 Trânsito 126.23 0.13 3068 [37]
Kepler-43 b 3.23 1.219 3.0240949 0.046 1620 Trânsito 3379 1.32 6041 [44]
Kepler-44b 1.0 1.09 3.2467293 0.0446 1544 Trânsito 4009 1.12 5800 [44]
Kepler-45b 0.505 0.96 2.455239 0.03 1000 Trânsito 1086 0.59 3820 [54]
Kepler-70b 0.0014 0.068 0.240104 0.006 Modulação de brilho orbital 3849 0.5 27730 Controverso[57]
Kepler-70c 0.0021 0.077 0.342887 0.0076 Modulação de brilho orbital 3849 0.5 27730 Controverso[57]
MOA-2009-BLG-266Lb 0.033 2774 3.2 Microlente 9900 0.56 [58]
Nu2 Lupi b 0.0145 0.132 11.57779+0.00091
−0.0011 		0.0969+0.0019
−0.0017 		Vel. radial 47.85±0.07 0.87±0.04 5664±61 [21]
Nu2 Lupi c 0.0355 0.233 27.5909+0.0028
−0.0031 		0.1729+0.0034
−0.0030 		Vel. radial 47.85±0.07 0.87±0.04 5664±61 [21]
Nu2 Lupi d 0.0278 0.229 107.245±0.050 0.425±0.012 Vel. radial 47.85±0.07 0.87±0.04 5664±61 [21]
NY Vir (AB) b 2.3 3160 3.3 Tempo 1800 0.6 33000 Planeta circumbinário[59]
NY Vir (AB) c 4.49 9861.75 7.54 Tempo 1800 0.6 33000 Planeta circumbinário[60]
PSR J1719-1438 b 1.2 0.09070629 0.0044 Tempo 3914 1.4 4500 Período orbital mais curto que qualquer exoplaneta conhecido[61]
Qatar-2 b 2.494 1.254 1.33711647 0.02153 1344 Trânsito 594.67 0.74 4645 [62]
TrES-5 1.79 1.194 1.48224686 0.02459 1480 Trânsito 1188 0.9 5171 [63]
UZ Fornacis b 6.3 5840 5.9 Tempo 781.5 0.7 5286 Falso positivo
UZ Fornacis c 7.7 1916.25 2.8 Tempo 781.5 0.7 5286 Não confirmado em 2020
WASP-35b 0.72±0.06 1.32±0.03 3.16158 0.04317 Trânsito 663.39 1.05 5990 [17]
WASP-39b 0.28 1.27 4.055259 0.0486 1166 Trânsito 750.18 0.93 5400 [64] Nome próprio Bocaprins
WASP-43b 1.78 0.93 0.813475 0.0142 1427 Trânsito 260.93 0.58 4400 [65]
WASP-44b 0.87 1.1 2.423804 0.03453 1337 Trânsito 1201 0.94 5420 [66]
WASP-45b 0.964 0.946 3.126089 0.03963 1153 Trânsito 693.04 0.85 5150 [66]
WASP-46b 1.91 1.174 1.43036763 0.02335 1636 Trânsito 1237 0.83 5600 [66]
WASP-48b 0.8 1.5 2.14363 0.03444 2035 Trânsito 1501 0.88 5920 [17]
WASP-50 b 1.4688 1.166 1.9551 0.0293 1395 Trânsito 606.08 0.89 5400 [67] Nome próprio Maeping
WD 0806-661 b 7.5 2500 323 Imagem direta 62.62 0.62 9552 Anã sub-marrom de Classe-Y[68]

Listas específicas de exoplanetas

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Referências

  1. ↑ «NASA Exoplanet Archive». Consultado em 20 de dezembro de 2019 
  2. ↑ Wittenmyer; Endl, M.; Wang, L.; Johnson, J.A.W.; Tinney, C.G.; O'Toole, S.J. (2011). «The Pan-Pacific Planet Search. I. A Giant Planet Orbiting 7 CMa». The Astrophysical Journal. 743 (2). 7 páginas. Bibcode:2011ApJ...743..184W. arXiv:astro-ph/0703672 . doi:10.1088/0004-637X/743/2/184 
  3. ↑ a b c d e f g Pepe, F.; et al. (2011). «The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310». Astronomy & Astrophysics. 534. A58. Bibcode:2011A&A...534A..58P. arXiv:1108.3447 . doi:10.1051/0004-6361/201117055 
  4. ↑ a b c Gettel, S.; Wolszczan, A.; Niedzielski, A.; Nowak, G.; Adamów, M.; Zieliński, P.; Maciejewski, G. (2011). «Substellar-Mass Companions to the K-Giants HD 240237, BD +48 738 and HD 96127». The Astrophysical Journal. 745 (1). 28. Bibcode:2012ApJ...745...28G. arXiv:1110.1641 . doi:10.1088/0004-637X/745/1/28 
  5. ↑ Liu, Michael C.; Delorme, Philippe; Dupuy, Trent J.; Bowler, Brendan P.; Albert, Loic; Artigau, Etienne; Reylé, Celine; Forveille, Thierry; Delfosse, Xavier (2011). «CFBDSIR J1458+1013B: A Very Cold (>T10) Brown Dwarf in a Binary System». The Astrophysical Journal. 740 (2). 108 páginas. Bibcode:2011ApJ...740..108L. arXiv:1103.0014 . doi:10.1088/0004-637X/740/2/108 
  6. ↑ Zhang, Zhoujian; Liu, Michael C.; Claytor, Zachary R.; Best, William M. J.; Dupuy, Trent J.; Siverd, Robert J. (2021), «The Second Discovery from the COCONUTS Program: A Cold Wide-orbit Exoplanet around a Young Field M Dwarf at 10.9 pc», The Astrophysical Journal Letters, 916 (2): L11, Bibcode:2021ApJ...916L..11Z, arXiv:2107.02805 , doi:10.3847/2041-8213/ac1123 
  7. ↑ Transiting exoplanets from the CoRoT space mission XXII. CoRoT-16b: a hot Jupiter with a hint of eccentricity around a faint solar-like star
  8. ↑ Csizmadia, Sz.; Moutou, C.; Deleuil, M.; Cabrera, J.; Fridlund, M.; Gandolfi, D.; Aigrain, S.; Alonso, R.; Almenara, J.-M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A.S.; Bordé, P.; Bouchy, F.; Bruntt, H.; Carone, L.; Carpano, S.; Cavarroc, C.; Cochran, W.; Deeg, H.J.; Díaz, R.F.; Dvorak, R.; Endl, M.; Erikson, A.; Ferraz-Mello, S.; Fruth, Th.; Gazzano, J.-C.; Gillon, M.; Guenther, E.W.; et al. (2011), «Transiting exoplanets from the CoRoT space mission. XVII. The hot Jupiter CoRoT-17b: a very old planet», Astronomy & Astrophysics, 531: A41, Bibcode:2011A&A...531A..41C, arXiv:1106.4393 , doi:10.1051/0004-6361/201117009 
  9. ↑ Hébrard, G.; Evans, T. M.; Alonso, R.; Fridlund, M.; Ofir, A.; Aigrain, S.; Guillot, T.; Almenara, J. M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Cabrera, J.; Carone, L.; Carpano, S.; Cavarroc, C.; Csizmadia, Sz.; Deeg, H. J.; Deleuil, M.; Díaz, R. F.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Gandolfi, D.; Gibson, N.; Gillon, M.; Guenther, E.; Hatzes, A.; et al. (2011), «Transiting exoplanets from the CoRoT space mission. XVIII. CoRoT-18b: a massive hot jupiter on a prograde, nearly aligned orbit», Astronomy & Astrophysics, 533: A130, Bibcode:2011A&A...533A.130H, arXiv:1107.2032 , doi:10.1051/0004-6361/201117192 
  10. ↑ Guenther, E. W.; Diaz, R. F.; Gazzano, J.-C.; Mazeh, T.; Rouan, D.; Gibson, N.; Csizmadia, Sz.; Aigrain, S.; Alonso, R.; Almenara, J. M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A.S.; Borde, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carone, L.; Carpano, S.; Cavarroc, C.; Deeg, H.J.; Deleuil, M.; Dreizler, S.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gillon, M.; et al. (2011), Transiting exoplanets from the CoRoT space mission XXI. CoRoT-19b: A low density planet orbiting an old inactive F9V-star, arXiv:1112.1035 , doi:10.1051/0004-6361/201117706 
  11. ↑ Deleuil, M.; Bonomo, A.S.; Ferraz-Mello, S.; Erikson, A.; Bouchy, F.; Havel, M.; Aigrain, S.; Almenara, J.-M.; Alonso, R.; Auvergne, M.; Baglin, A.; Barge, P.; Bordé, P.; Bruntt, H.; Cabrera, J.; Carpano, S.; Cavarroc, C.; Csizmadia, Sz.; Damiani, C.; Deeg, H.J.; Dvorak, R.; Fridlund, M.; Hébrard, G.; Gandolfi, D.; Gillon, M.; Guenther, E.; Guillot, T.; Hatzes, A.; Jorda, L.; Léger, A.; et al. (2011). «Transiting exoplanets from the CoRoT space mission⋆ XX. CoRoT-20b: A very high density, high eccentricity transiting giant planet». Astronomy & Astrophysics. arXiv:1109.3203 . doi:10.1051/0004-6361/201117681 
  12. ↑ Parviainen, H.; Deeg, H. J.; Belmonte, J. A. (2012), «Secondary eclipses in the CoRoT light curves», Astronomy & Astrophysics, 550: A67, arXiv:1211.5361 , doi:10.1051/0004-6361/201220081 
  13. ↑ Rouan, D.; Parviainen, H.; Moutou, C.; Deleuil, M.; Fridlund, M.; Ofir, A.; Havel, M.; Aigrain, S.; Alonso, R.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A.; Bordé, P.; Bouchy, F.; Cabrera, J.; Cavarroc, C.; Csizmadia, Sz.; Deeg, H.; Diaz, R.F.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Gandolfi, D.; Gillon, M.; Guillot, T.; Hatzes, A.; Hébrard, G.; Jorda, L.; Léger, A.; et al. (2011). «Transiting exoplanets from the CoRoT space mission⋆ XIX. CoRoT-23b: a dense hot Jupiter on an eccentric orbit». Astronomy and Astrophysics. arXiv:1112.0584 . doi:10.1051/0004-6361/201117916 
  14. ↑ a b Bonfils, Xavier; Delfosse, Xavier; Udry, Stéphane; Forveille, Thierry; Mayor, Michel; Perrier, Christian; Bouchy, François; Gillon, Michaël; Lovis, Christophe; Pepe, Francesco; Queloz, Didier; Santos, Nuno C.; Ségransan, Damien; Bertaux, Jean-Loup (2011). «The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample». Astronomy and Astrophysics. 549: A109. Bibcode:2013A&A...549A.109B. arXiv:1111.5019 . doi:10.1051/0004-6361/201014704 
  15. ↑ Béky, B.; Bakos, G. Á.; Hartman, J.; Torres, G.; Latham, D. W.; Jordán, A.; Arriagada, P.; Bayliss, D.; Kiss, L. L.; Kovács, Géza; Quinn, S. N.; Marcy, G. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Esquerdo, G. A.; Noyes, R. W.; Buchhave, L. A.; Sasselov, D. D.; Stefanik, R. P.; Perumpilly, G.; Lázár, J.; Papp, I.; Sári, P. (2011), «HAT-P-27b: A HOT JUPITER TRANSITING A G STAR ON A 3 DAY ORBIT», The Astrophysical Journal, 734 (2): 109, Bibcode:2011ApJ...734..109B, arXiv:1101.3511 , doi:10.1088/0004-637X/734/2/109 
  16. ↑ a b Buchhave, L. A.; Bakos, G. Á.; Hartman, J. D.; Torres, G.; Latham, D. W.; Andersen, J.; Kovács, G.; Noyes, R. W.; Shporer, A.; Esquerdo, G. A.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Howard, A. W.; Béky, B.; Sasselov, D. D.; Fűrész, G.; Quinn, S. N.; Stefanik, R. P.; Szklenár, T.; Berlind, P.; Calkins, M. L.; Lázár, J.; Papp, I.; Sári, P. (2011), «HAT-P-28b AND HAT-P-29b: TWO SUB-JUPITER MASS TRANSITING PLANETS», The Astrophysical Journal, 733 (2): 116, Bibcode:2011ApJ...733..116B, arXiv:1103.1813 , doi:10.1088/0004-637X/733/2/116 
  17. ↑ a b c Enoch, B.; Anderson, D.R.; Barros, S.C.C.; Brown, D.J.A.; Cameron, A.Collier; Faedi, F.; Gillon, M.; Hébrard, G.; Lister, T.A.; Queloz, D.; Santerne, A.; Smalley, B.; Street, R.A.; Triaud, A.H.M.J.; West, R.G.; Bouchy, F.; Bento, J.; Butters, O.; Fossati, L.; Haswell, C.A.; Hellier, C.; Holmes, S.; Jehen, E.; Lendl, M.; Maxted, P.F.L.; McCormac, J.; Miller, G.R.M.; Moulds, V.; Moutou, C.; Norton, A.J.; et al. (2011). «WASP-35b, WASP-48b, AND HAT-P-30b/WASP-51b: TWO NEW PLANETS AND AN INDEPENDENT DISCOVERY OF a HAT PLANET». The Astronomical Journal. 142 (3): 86. Bibcode:2011AJ....142...86E. arXiv:1104.2827 . doi:10.1088/0004-6256/142/3/86 
  18. ↑ Johnson, John Asher; Winn, J. N.; Bakos, G. Á.; Hartman, J. D.; Morton, T. D.; Torres, G.; Kovács, Géza; Latham, D. W.; Noyes, R. W.; Sato, B.; Esquerdo, G. A.; Fischer, D. A.; Marcy, G. W.; Howard, A. W.; Buchhave, L. A.; Fűrész, G.; Quinn, S. N.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P. (2011), «HAT-P-30b: A transiting hot Jupiter on a highly oblique orbit», The Astrophysical Journal, 735 (1): 24, Bibcode:2011ApJ...735...24J, arXiv:1103.3825 , doi:10.1088/0004-637X/735/1/24 
  19. ↑ Kipping, D. M.; Hartman, J.; Bakos, G. Á.; Torres, G.; Latham, D. W.; Bayliss, D.; Kiss, L. L.; Sato, B.; Béky, B.; Kovács, Géza; Quinn, S. N.; Buchhave, L. A.; Andersen, J.; Marcy, G. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Noyes, R. W.; Sasselov, D. D.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P.; Fűrész, G. (2011), «HAT-P-31b,c: A Transiting, Eccentric, Hot Jupiter and a Long-Period, Massive Third-Body», The Astronomical Journal, 142 (3): 95, Bibcode:2011AJ....142...95K, arXiv:1106.1169 , doi:10.1088/0004-6256/142/3/95 
  20. ↑ a b Hartman, J. D.; Bakos, G. Á.; Torres, G.; Latham, D. W.; Kovács, Géza; Béky, B.; Quinn, S. N.; Mazeh, T.; Shporer, A.; Marcy, G. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Esquerdo, G. A.; Noyes, R. W.; Sasselov, D. D.; Stefanik, R. P.; Fernandez, J. M.; Szklenár, T.; Lázár, J.; Papp, I.; Sári, P. (2011), «HAT-P-32b and HAT-P-33b: Two Highly Inflated Hot Jupiters Transiting High-Jitter Stars», The Astrophysical Journal, 742 (1): 59, Bibcode:2011ApJ...742...59H, arXiv:1106.1212 , doi:10.1088/0004-637X/742/1/59 
  21. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al Mayor, M.; Marmier, M.; Lovis, C.; Udry, S.; Ségransan, D.; Pepe, F.; Benz, W.; Bertaux, J. -L.; Bouchy, F.; Dumusque, X.; Lo Curto, G.; Mordasini, C.; Queloz, D.; Santos, N. C. (2011), The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets, arXiv:1109.2497  
  22. ↑ a b Díaz, R. F.; Ségransan, D.; Udry, S.; Lovis, C.; Pepe, F.; Dumusque, X.; Marmier, M.; Alonso, R.; Benz, W.; Bouchy, F.; Coffinet, A.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Moutou, C.; Pollacco, D.; Pompei, E.; Queloz, D.; Santos, N.; Wyttenbach, A. (2016). «The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles». Astronomy and Astrophysics. 585. A134. Bibcode:2016A&A...585A.134D. arXiv:1510.06446 . doi:10.1051/0004-6361/201526729 
  23. ↑ a b c d e f g h i j k l m n o p q r Johnson, John Asher; Clanton, Christian; Howard, Andrew W.; Bowler, Brendan P.; Henry, Gregory W.; Marcy, Geoffrey W.; Crepp, Justin R.; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Wright, Jason T.; Isaacson, Howard (novembro de 2011), «Retired A Stars and Their Companions: Eighteen New Jovian Planets», The Astrophysical Journal Supplement Series, 197 (2): 26, arXiv:1108.4205 , doi:10.1088/0067-0049/197/2/26 
  24. ↑ a b c d Dumusque, X.; Lovis, C.; Ségransan, D.; Mayor, M.; Udry, S.; Benz, W.; Bouchy, F.; Lo Curto, G.; Mordasini, C.; Pepe, F.; Queloz, D.; Santos, N. C.; Naef, D. (2011), «The HARPS search for southern extra-solar planets. XXX. Planetary systems around stars with solar-like magnetic cycles and short-term activity variation», Astronomy & Astrophysics, 535: A55, Bibcode:2011A&A...535A..55D, arXiv:1107.1748 , doi:10.1051/0004-6361/201117148 
  25. ↑ a b c d Díaz, Rodrigo F.; Santerne, Alexandre; Sahlmann, Johannes; Hébrard, Guillaume; Eggenberger, Anne; Santos, Nuno C.; Moutou, Claire; Arnold, Luc; Boisse, Isabelle; Bonfils, Xavier; Bouchy, François; Delfosse, Xavier; Desort, Morgan; Ehrenreich, David; Forveille, Thierry; Lagrange, Anne-Marie; Lovis, Christophe; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Ségransan, Damien; Udry, Stéphane; Vidal-Madjar, Alfred (2012), «The SOPHIE search for northern extrasolar planets IV. Massive companions in the planet-brown dwarf boundary», Astronomy & Astrophysics, A113: 538, Bibcode:2012A&A...538A.113D, arXiv:1111.1168 , doi:10.1051/0004-6361/201117935 
  26. ↑ a b c d e f g h i Udry, S.; Dumusque, X.; Lovis, C.; Ségransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Wyttenbach, A.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (2019), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 622: A37, Bibcode:2019A&A...622A..37U, arXiv:1705.05153 , doi:10.1051/0004-6361/201731173 
  27. ↑ a b c d e f g h Gillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F.; Queloz, D.; Seager, S.; Ségransan, D.; Udry, S. (2017), «The Spitzersearch for the transits of HARPS low-mass planets», Astronomy & Astrophysics, 601: A117, arXiv:1701.01303 , doi:10.1051/0004-6361/201629270 
  28. ↑ a b c d e f g h i Unger, N.; Ségransan, D.; Queloz, D.; Udry, S.; Lovis, C.; Mordasini, C.; Ahrer, E.; Benz, W.; Bouchy, F.; Delisle, J.-B.; Díaz, R.F.; Dumusque, X.; Lo Curto, G.; Marmier, M.; Mayor, M.; Pepe, F.; Santos, N.C.; Stalport, M.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (2021), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 654: A104, Bibcode:2021A&A...654A.104U, arXiv:2108.10198 , doi:10.1051/0004-6361/202141351 
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  42. ↑ Endl, Michael; MacQueen, Phillip J.; Cochran, William D.; Brugamyer, Erik J.; Buchhave, Lars A.; Rowe, Jason; Lucas, Phillip; Isaacson, Howard; Bryson, Steve; Howell, Steve B.; Fortney, Jonathan J.; Hansen, Terese; Borucki, William J.; Caldwell, Douglas; Christiansen, Jessie L.; Ciardi, David R.; Demory, Brice-Olivier; Everett, Mark; Ford, Eric B.; Haas, Michael R.; Holman, Matthew J.; Horch, Elliott; Jenkins, Jon M.; Koch, David J.; Lissauer, Jack J.; Machalek, Pavel; Still, Martin; Welsh, William F.; Sanderfer, Dwight T.; Seader, Shawn E.; et al. (2011). «Kepler-15b: A Hot Jupiter Enriched in Heavy Elements and the First Kepler Mission Planet Confirmed with the Hobby-Eberly Telescope». The Astrophysical Journal Supplement Series. 197 (1). 13. Bibcode:2011ApJS..197...13E . doi:10.1088/0067-0049/197/1/13 . hdl:2152/42925  
  43. ↑ Jean Schneider (2011). «Notes for Planet Kepler-16 (AB) b». Extrasolar Planets Encyclopaedia. Consultado em 23 de setembro de 2011. Arquivado do original em 11 de outubro de 2011 
  44. ↑ a b c Bonomo, A. S.; Hébrard, G.; Santerne, A.; Santos, N. C.; Deleuil, M.; Almenara, J.; Bouchy, F.; Díaz, R. F.; Moutou, C.; Vanhuysse, M. (2012). «SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b, and KOI-203b (alias Kepler-17b)». Astronomy and Astrophysics. 538. A96. Bibcode:2012A&A...538A..96B. arXiv:1110.5462 . doi:10.1051/0004-6361/201118323 
  45. ↑ a b c Cochran, William D.; et al. (2011). «Kepler 18-b, c, and d: A System Of Three Planets Confirmed by Transit Timing Variations, Lightcurve Validation, Spitzer Photometry and Radial Velocity Measurements». The Astrophysical Journal Supplement Series. 197 (1). 7 páginas. Bibcode:2011ApJS..197....7C. arXiv:1110.0820 . doi:10.1088/0067-0049/197/1/7 
  46. ↑ a b Ballard, S.; et al. (2011). «The Kepler-19 System: A Transiting 2.2 R⊕ Planet and a Second Planet Detected Via Transit Timing Variations». The Astrophysical Journal. 743 (2). 200. Bibcode:2011ApJ...743..200B. arXiv:1109.1561 . doi:10.1088/0004-637X/743/2/200 
  47. ↑ a b c d e Gautier, Thomas N.; Charbonneau, David; Rowe, Jason F.; Marcy, Geoffrey W.; Isaacson, Howard; Torres, Guillermo; Fressin, Francois; Rogers, Leslie A.; Désert, Jean-Michel; Buchhave, Lars A.; Latham, David W.; Quinn, Samuel N.; Ciardi, David R.; Fabrycky, Daniel C.; Ford, Eric B.; Gilliland, Ronald L.; Walkowicz, Lucianne M.; Bryson, Stephen T.; Cochran, William D.; Endl, Michael; Fischer, Debra A.; Howell, Steve B.; Horch, Elliott P.; Barclay, Thomas; Batalha, Natalie; Borucki, William J.; Christiansen, Jessie L.; Geary, John C.; Henze, Christopher E.; Holman, Matthew J.; et al. (2011), «Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates», The Astrophysical Journal, 749 (1): 15, arXiv:1112.4514 , doi:10.1088/0004-637X/749/1/15 
  48. ↑ Howell, Steve B.; Rowe, Jason F.; Bryson, Stephen T.; Quinn, Samuel N.; Marcy, Geoffrey W.; Isaacson, Howard; Ciardi, David R.; Chaplin, William J.; Metcalfe, Travis S.; Monteiro, Mario J. P. F. G.; Appourchaux, Thierry; Basu, Sarbani; Creevey, Orlagh L.; Gilliland, Ronald L.; Quirion, Pierre-Olivier; Stello, Denis; Kjeldsen, Hans; Christensen-Dalsgaard, Jörgen; Elsworth, Yvonne; García, Rafael A; Houdek, Günter; Karoff, Christoffer; Molenda-Żakowicz, Joanna; Thompson, Michael J.; Verner, Graham A.; Torres, Guillermo; Fressin, Francois; Crepp, Justin R.; Adams, Elisabeth; Dupree, Andrea; et al. (2012). «Kepler-21b: A 1.6 REarth Planet Transiting the Bright Oscillating F Subgiant Star HD 179070». The Astrophysical Journal. 746 (2). 123. Bibcode:2012ApJ...746..123H . arXiv:1112.2165 . doi:10.1088/0004-637X/746/2/123  
  49. ↑ Boyle, Rebecca (5 de dezembro de 2011). «Kepler Team Confirms First Earth-like planet in a habitable zone, And Finds 1,094 More Worlds». Popular Science. Consultado em 5 de dezembro de 2011 
  50. ↑ a b c d Ford, Eric B.; Fabrycky, Daniel C.; Steffen, Jason H.; Carter, Joshua A.; Fressin, Francois; Holman, Matthew J.; Lissauer, Jack J.; Moorhead, Althea V.; Morehead, Robert C.; Ragozzine, Darin; Rowe, Jason F.; Welsh, William F.; Allen, Christopher; Batalha, Natalie M.; Borucki, William J.; Bryson, Stephen T.; Buchhave, Lars A.; Burke, Christopher J.; Caldwell, Douglas A.; Charbonneau, David; Clarke, Bruce D.; Cochran, William D.; Désert, Jean-Michel; Endl, Michael; Everett, Mark E.; Fischer, Debra A.; Gautier III, Thomas N.; Gilliland, Ron L.; Jenkins, Jon M.; Haas, Michael R.; et al. (2012), «Transit Timing Observations Fromkepler. Ii. Confirmation of Two Multiplanet Systems Via a Non-Parametric Correlation Analysis», The Astrophysical Journal, 750 (2): 113, Bibcode:2012ApJ...750..113F, arXiv:1201.5409 , doi:10.1088/0004-637X/750/2/113 
  51. ↑ a b c d e f g h Steffen, Jason H.; Fabrycky, Daniel C.; Ford, Eric B.; Carter, Joshua A.; Desert, Jean-Michel; Fressin, Francois; Holman, Matthew J.; Lissauer, Jack J.; Moorhead, Althea V.; Rowe, Jason F.; Ragozzine, Darin; Welsh, William F.; Batalha, Natalie M.; Borucki, William J.; Buchhave, Lars A.; Bryson, Steve; Caldwell, Douglas A.; Charbonneau, David; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Gautier III, Thomas N.; Gilliland, Ron L.; Girouard, Forrest R.; Jenkins, Jon M.; Horch, Elliott; Howell, Steve B.; Isaacson, Howard; Klaus, Todd C.; et al. (2012), Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations, Bibcode:2012MNRAS.421.2342S, arXiv:1201.5412 , doi:10.1111/j.1365-2966.2012.20467.x 
  52. ↑ a b Borucki, William J.; Koch, David G.; Basri, Gibor; Batalha, Natalie; Brown, Timothy M.; Bryson, Stephen T.; Caldwell, Douglas; Christensen-Dalsgaard, Jørgen; Cochran, William D.; Devore, Edna; Dunham, Edward W.; Gautier, Thomas N.; Geary, John C.; Gilliland, Ronald; Gould, Alan; Howell, Steve B.; Jenkins, Jon M.; Latham, David W.; Lissauer, Jack J; Marcy, Geoffrey W.; Rowe, Jason; Sasselov, Dimitar; Boss, Alan; Charbonneau, David; Ciardi, David; Doyle, Laurance; Dupree, Andrea K.; Ford, Eric B.; Fortney, Jonathan; Holman, Matthew J.; et al. (2011). «Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data». The Astrophysical Journal. 736 (1). 19. Bibcode:2011ApJ...736...19B . arXiv:1102.0541 . doi:10.1088/0004-637X/736/1/19  
  53. ↑ a b c d Lissauer, Jack J.; Ragozzine, Darin; Fabrycky, Daniel C.; Steffen, Jason H.; Ford, Eric B.; Jenkins, Jon M.; Shporer, Avi; Holman, Matthew J.; Rowe, Jason F.; Quintana, Elisa V.; Batalha, Natalie M.; Borucki, William J.; Bryson, Stephen T.; Caldwell, Douglas A.; Carter, Joshua A.; Ciardi, David; Dunham, Edward W.; Fortney, Jonathan J.; Gautier, Iii, Thomas N.; Howell, Steve B.; Koch, David G.; Latham, David W.; Marcy, Geoffrey W.; Morehead, Robert C.; Sasselov, Dimitar (2011), «Architecture and Dynamics of Kepler 'S Candidate Multiple Transiting Planet Systems», The Astrophysical Journal Supplement Series, 197 (1): 8, Bibcode:2011ApJS..197....8L, arXiv:1102.0543 , doi:10.1088/0067-0049/197/1/8 
  54. ↑ a b c d e Ford, Eric B.; Rowe, Jason F.; Fabrycky, Daniel C.; Carter, Joshua A.; Holman, Matthew J.; Lissauer, Jack J.; Ragozzine, Darin; Steffen, Jason H.; Batalha, Natalie M.; Borucki, William J.; Bryson, Steve; Caldwell, Douglas A.; Dunham, Edward W.; Gautier, Thomas N.; Jenkins, Jon M.; Koch, David G.; Li, Jie; Lucas, Philip; Marcy, Geoffrey W.; McCauliff, Sean; Mullally, Fergal R.; Quintana, Elisa; Still, Martin; Tenenbaum, Peter; Thompson, Susan E.; Twicken, Joseph D. (2011), «Transit Timing Observations from Kepler : I. Statistical Analysis of the First Four Months», The Astrophysical Journal Supplement Series, 197 (1): 2, Bibcode:2011ApJS..197....2F, arXiv:1102.0544 , doi:10.1088/0067-0049/197/1/2 
  55. ↑ Bouchy, F.; Bonomo, A.S.; Santerne, A.; Moutou, C.; Deleuil, M.; Díaz, R.F.; Eggenberger, A.; Ehrenreich, D.; Gry, C.; Guillot, T.; Havel, M.; Hébrard, G.; Udry, S. (2011). «SOPHIE velocimetry of Kepler transit candidates. III. KOI-423b: an 18 MJup transiting companion around an F7IV star». Astronomy and Astrophysics. 533. A83. Bibcode:2011A&A...533A..83B. arXiv:1106.3225 . doi:10.1051/0004-6361/201117095 
  56. ↑ Santerne, A.; Bonomo, A. S.; Hébrard, G.; Deleuil, M.; Moutou, C.; Almenara, J.-M.; Bouchy, F.; Díaz, R. F. (2011). «SOPHIE velocimetry of Kepler transit candidates IV. KOI-196b: a non-inflated hot Jupiter with a high albedo». Astronomy and Astrophysics. 536. A70. Bibcode:2011A&A...536A..70S. arXiv:1108.0550 . doi:10.1051/0004-6361/201117807 
  57. ↑ a b Blokesz, A.; Krzesinski, J.; Kedziora-Chudczer, L. (4 de julho de 2019), «Analysis of putative exoplanetary signatures found in light curves of two sdBV stars observed by Kepler», Astronomy & Astrophysics, 627: A86, Bibcode:2019A&A...627A..86B, arXiv:1906.03321 , doi:10.1051/0004-6361/201835003 
  58. ↑ Muraki, Y.; Han, C.; Bennett, D. P.; Suzuki, D.; Monard, L. A. G.; Street, R.; Jorgensen, U. G.; Kundurthy, P.; Skowron, J.; Becker, A. C.; Albrow, M. D.; Fouqué, P.; Heyrovský, D.; Barry, R. K.; Beaulieu, J.-P.; Wellnitz, D. D.; Bond, I. A.; Sumi, T.; Dong, S.; Gaudi, B. S.; Bramich, D. M.; Dominik, M.; Abe, F.; Botzler, C. S.; Freeman, M.; Fukui, A.; Furusawa, K.; Hayashi, F.; Hearnshaw, J. B.; Hosaka, S.; et al. (2011), «Discovery and Mass Measurements of a Cold, 10-Earth Mass Planet and Its Host Star», The Astrophysical Journal, 741 (1): 22, Bibcode:2011ApJ...741...22M, arXiv:1106.2160 , doi:10.1088/0004-637X/741/1/22 
  59. ↑ Qian, S.-B.; Zhu, L.-Y.; Dai, Z.-B.; Fernández-Lajús, E.; Xiang, F.-Y.; He, J.-J. (2011), «Circumbinary Planets Orbiting the Rapidly Pulsating Subdwarf B-type binary NY Vir», The Astrophysical Journal, 745 (2): L23, arXiv:1112.4269 , doi:10.1088/2041-8205/745/2/L23 
  60. ↑ Lee, Jae Woo; Hinse, Tobias Cornelius; Youn, Jae-Hyuck; Han, Wonyong (2014), «The Pulsating sdB+M Eclipsing System NY Virginis and its Circumbinary Planets», Monthly Notices of the Royal Astronomical Society, 445 (3): 2331–2339, arXiv:1409.4907 , doi:10.1093/mnras/stu1937 
  61. ↑ Redd, Nola Taylor (25 de agosto de 2011). «Surprise! Alien Planet Made of Diamond Discovered». TechMediaNetwork. Consultado em 25 de agosto de 2011 
  62. ↑ Bryan, Marta L.; Alsubai, Khalid A.; Latham, David W.; Parley, Neil R.; Collier Cameron, Andrew; Quinn, Samuel N.; Carter, Joshua A.; Fulton, Benjamin J.; Berlind, Perry; Brown, Warren R.; Buchhave, Lars A.; Calkins, Michael L.; Esquerdo, Gilbert A.; Fűrész, Gábor; Jørgensen, Uffe Gråe; Horne, Keith D.; Stefanik, Robert P.; Street, Rachel A.; Torres, Guillermo; West, Richard G.; Dominik, Martin; Harpsøe, Kennet B. W.; Liebig, Christine; Calchi Novati, Sebastiano; Ricci, Davide; Skottfelt, Jesper F. (2011), «Qatar-2: A K dwarf orbited by a transiting hot Jupiter and a more massive companion in an outer orbit», The Astrophysical Journal, 750: 84, arXiv:1110.5912 , doi:10.1088/0004-637X/750/1/84 
  63. ↑ Mandushev, Georgi; Quinn, Samuel N.; Buchhave, Lars A.; Dunham, Edward W.; Rabus, Markus; Oetiker, Brian; Latham, David W.; Charbonneau, David; Brown, Timothy M.; Belmonte, Juan A.; O'Donovan, Francis T. (2011), «TrES-5: A Massive Jupiter-sized Planet Transiting A Cool G-dwarf», The Astrophysical Journal, 741 (2): 114, Bibcode:2011ApJ...741..114M, arXiv:1108.3572 , doi:10.1088/0004-637X/741/2/114 
  64. ↑ Faedi, Francesca; Barros, S.C.C.; Anderson, D.R.; Brown, D.J.A.; Cameron, A. Collier; Pollacco, D.; Boisse, I.; Hebrard, G.; Lendl, M.; Lister, T.A.; Smalley, B.; Street, R.A.; Triaud, A.H.M.J.; Bento, J.; Butters, O.W.; Enoch, B.; Bouchy, F.; Haswell, C.A.; Hellier, C.; Keenan, F.P.; Miller, G.R.M.; Moulds, V.; Moutou, C.; Norton, A.J.; Queloz, D.; Santerne, A.; Simpson, E.K.; Skillen, I.; Smith, A.M.S.; Udry, S.; Watson, C.A.; West, R.G.; Wheatley, P.J. (julho de 2011), «WASP-39b: a highly inflated Saturn-mass planet orbiting a late G-type star», Astronomy and Astrophysics, 531: A40, Bibcode:2011A&A...531A..40F, arXiv:1102.1375 , doi:10.1051/0004-6361/201116671 
  65. ↑ Hellier, C.; Anderson, D.R. (2011). «WASP-43b: The closest-orbiting hot Jupiter». Astronomy and Astrophysics. 535. L7. Bibcode:2011A&A...535L...7H. arXiv:1104.2823 . doi:10.1051/0004-6361/201117081 
  66. ↑ a b c Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Smith, A. M. S.; Triaud, A. H. M. J.; West, R. G.; Pepe, F.; Pollacco, D.; Ségransan, D.; Todd, I.; Udry, S. (2012), «WASP-44b, WASP-45b and WASP-46b: three short-period, transiting extrasolar planets», Monthly Notices of the Royal Astronomical Society, 422 (3): 1988–1998, Bibcode:2012MNRAS.422.1988A, arXiv:1105.3179 , doi:10.1111/j.1365-2966.2012.20635.x 
  67. ↑ Gillon, M.; Doyle, A. P.; Lendl, M.; Maxted, P.F.L.; Triaud, A.H.M.J.; Anderson, D.R.; Barros, S.C.C.; Bento, J.; Collier-Cameron, A.; Enoch, B.; Faedi, F.; Hellier, C.; Jehin, E.; Magain, P.; Montalban, J.; Pepe, F.; Pollacco, D.; Queloz, D.; Smalley, B.; Segransan, D.; Smith, A.M.S.; Southworth, J.; Udry, S.; West, R. G.; Wheatley, P.J. (2011), «WASP-50 b: a hot Jupiter transiting a moderately active solar-type star», Astronomy and Astrophysics, 533: A88, Bibcode:2011A&A...533A..88G, arXiv:1108.2641 , doi:10.1051/0004-6361/201117198 
  68. ↑ Luhman, K.L.; Burgasser, Adam J.; Bochanski, J.J. (2011). «Discovery of a Candidate for the Coolest Known Brown Dwarf». The Astrophysical Journal Letters. 730 (1). L9. Bibcode:2011ApJ...730L...9L. arXiv:1102.5411 . doi:10.1088/2041-8205/730/1/L9 
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