List of exoplanets discovered in 2010

Last updated

This is a List of exoplanets discovered in 2010. [1]

Contents

For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
2MASS J04414489+2301513 b 7.515.0imaging456.630.02
24 Sextantis b 1.99452.81.333radial vel.235.531.545098
24 Sextantis c 0.868832.08radial vel.235.531.545098
Alpha Arietis b 1.8380.81.2radial vel.65.921.54553Host star also known as Hamal
CoRoT-8b 0.220.576.212290.063870transit12390.885080
CoRoT-10b 2.750.9713.24060.1055600transit11250.895075
CoRoT-11b 2.331.432.994330.04361657transit18271.276440
CoRoT-12b 0.9171.442.8280420.040161442transit37511.085675
CoRoT-13b 1.3080.8854.035190.0511700transit34571.095945
CoRoT-14b 7.61.091.512140.0271952transit43711.136035
Gliese 676 Ab 6.71056.81.82radial vel.52.280.733734
Gliese 876 e 0.046124.260.3343radial vel.15.260.323129
Gliese 1148 b 0.3042541.380.166radial vel.35.940.353264
Gliese 3634 b 0.0262.645610.0287radial vel.64.580.453685
GSC 06214-00210 b 16.01.83202300imaging472.940.94200
HAT-P-14b 3.441.424.627670.05961624transit730.942.656600Proper name Sissi
HAT-P-15b 1.941.0610.86350.0965904transit631.331.05568 [2] Proper name Tryzub
HAT-P-16b 4.1931.2892.775960.04131626transit766.491.226158 [3]
HAT-P-17b 0.581.0510.338520.0882792transit302.130.995246
HAT-P-17c 3.455845.6radial vel.302.130.995246
HAT-P-18b 0.1970.9955.5080230.0559852transit541.440.774803 [4]
HAT-P-19b 0.2921.1324.0087780.04661010transit701.260.844990 [4]
HAT-P-20b 7.2460.8672.8753170.0361970transit228.320.764595 [5]
HAT-P-21b 4.871.114.124480.04941283transit911.571.245588 [5] Proper name Bambaruush
HAT-P-22b 2.471.153.212220.04141463transit267.331.135302 [5]
HAT-P-23b 1.341.091.212880.02321951transit12020.585905 [5] Proper name Jebus
HAT-P-24b 0.751.33.355240.046511637transit13711.376373
HAT-P-25b 0.5691.1353.652815140.04661182transit988.121.015519 [6]
HAT-P-26b 0.070.634.234520.04791001transit464.491.125079 [7]
HD 1461 b 0.020265.771520.0634radial vel.76.551.025765
BD-11 4672 b 0.61634±142.36±0.04radial vel.88.60.5714475±100 [8]
HD 1690 b 8.795331.36radial vel.25091.864374 [8]
HD 4313 b 8.795331.36radial vel.438±21.864374 [9]
HD 25171 b 0.95±0.11845±153.02±0.16radial vel.179.3±4.91.09±0.36160±65 [8]
HD 217786 A b 13.013192.38radial vel.178.741.025966Orbiting a primary star in binary system, planet is likely a low-mass brown dwarf [8]
HD 8535 b 0.6813132.45radial vel.171.241.136136
HD 10180 c 0.04165.759690.06412radial vel.127.211.065911
HD 10180 d 0.037816.3570.12859radial vel.127.211.065911
HD 10180 e 0.080549.7480.2699radial vel.127.211.065911
HD 10180 f 0.0722122.7440.4929radial vel.127.211.065911
HD 10180 g 0.0732604.671.427radial vel.127.211.065911
HD 10180 h 0.206622053.381radial vel.127.211.065911
HD 25171 b 0.9151802.292.971radial vel.181.681.086125 [8]
HD 28254 b 1.1611162.15radial vel.178.411.065664
HD 31253 b 0.624661.26radial vel.189.961.76130 [10]
HD 38283 b 0.4363.21.02radial vel.124.271.375981Proper name Yanyan
HD 43197 b 0.6327.80.92radial vel.183.630.965508Proper name Equiano
HD 44219 b 0.58472.31.19radial vel.164.391.05752
HD 86226 b 0.9216952.84radial vel.149.191.065903 [11]
HD 95089 b 1.26464.41.36radial vel.448.351.544918 [9]
HD 97658 b 0.030.219.49090.0796757radial vel.70.390.895175
HD 102365 b 0.05122.10.46radial vel.30.30.855630
HD 102956 b 0.966.49470.0807radial vel.398.971.664985Proper name Isagel
HD 109246 b 0.8668.270.33radial vel.221.71.25844 [12] Proper name Fold
HD 113538 b 0.36663.21.24radial vel.51.860.584462 [8]
HD 113538 c 0.9318182.44radial vel.51.860.584462 [8]
HD 114783 c 0.611+0.056
−0.053		4319+151
−130		radial vel.66.5±1.30.85±0.035135±44 [13]
HD 129445 b 1.618402.9radial vel.220.390.995605 [11]
HD 136418 b 2.14464.31.29radial vel.344.071.484989 [9] Proper name Awasis
HD 145457 b 2.23176.30.76radial vel.443.01.234769Proper name Chura
HD 152079 b 2.6612918.924.187radial vel.287.391.155907 [11]
HD 156668 b 0.0134.64550.05radial vel.79.420.774850
HD 164604 b 1.99792641.4721.331radial vel.128.540.774684 [11] Proper name Caleuche
HD 175167 b 8.9712902.4radial vel.232.331.375635 [11]
HD 176051 b 1.510161.76astrometry491.07/0.716000/?First planet discovered by astrometry, it is not known which star it orbits
HD 177830 c 0.15110.90.5137radial vel.205.091.74901 [10]
HD 180314 b 20.13396.031.46radial vel.400.52.24924
HD 180902 b 1.685510.91.4radial vel.342.121.414961 [9]
HD 181342 b 2.54564.11.592radial vel.394.041.694945 [9] Proper name Dopere
HD 200964 b 1.599606.31.565radial vel.237.251.394982
HD 200964 c 1.214852.51.96radial vel.237.251.394982
HD 204313 b 3.461920.13.07radial vel.156.11.035783
HD 206610 b 2.036673.21.74radial vel.482.011.554842 [9] Proper name Naron
HD 212771 b 2.39380.71.19radial vel.363.711.565003 [9] Proper name Victoriapeak
HD 218566 b 0.2225.70.69radial vel.94.10.764730 [10] Proper name Ugarit
HIP 12961 b 0.3657.4350.25radial vel.76.290.693901Proper name Aumatex
HIP 78530 b 23.07402700imaging511.12.510500
HR 8799 e 10.01.1720815.616.41150imaging128.511.517400
Kepler-8b 0.591.4163.52249910.04741680transit34341.216213
Kepler-9b 0.136550.7419.238910.143transit20031.025774
Kepler-9c 0.094080.72138.98530.227transit20031.025774
Kepler-9d 0.1461.5928510.02732026transit20031.025774
Kepler-40b 2.21.176.873490.081620transit88071.486510
Kepler-71b 1.113.905120.0477transit26090.955545
MOA-2009-BLG-319Lb 0.162.4microlensing199000.38
MOA-2009-BLG-387Lb 2.5619821.82microlensing186000.19
NN Serpentis c 7.335573.555.35timing16310.5457000
NN Serpentis d 2.32883.53.43timing16310.5457000
Qatar 1 b 1.2941.1431.42002420.023321532±219transit608.660.845013 [14] [15]
Ross 458 c 6.285361.221168imaging37.540.493621Has the largest orbit for a circumbinary planet
SR 12 AB c 13.01100imaging366±183828Circumbinary, already at the deuterium-burning mass limit and still accreting. [16] [17]
WASP-8b 2.541.138.158720.0801950transit294.171.345600
WASP-21b 0.31.074.3224820.0521340transit849.110.895800Proper name Bendida
WASP-22b 0.671.233.532690.0471502transit10451.466000Proper name Koyopa'
WASP-23b  [ ru ]0.8840.9622.94442560.0376transit680.840.785150 [18]
WASP-24b 1.241.382.341210.036511772transit10601.436075
WASP-25b 0.441.073.764830.04731210transit693.760.675750 [19] [20] [21]
WASP-26b 0.851.212.75660.039851650transit830.130.866034 [22]
WASP-28b 0.9071.2133.408830.044691468transit13001.026150, [23] also rediscovered in 2014 [24]
WASP-29b 0.230.773.922730.0457970transit286.440.774800 [25] [26] [27] [28] [29]
WASP-31b 0.4781.5493.40590960.046591575transit11741.166302
WASP-32b 2.630.962.718660.0394transit907.30.726140 [30] [31] [32] [33] Proper name Viculus
WASP-33b 2.0931.5931.219870.02392782transit399.11.57430
WASP-34b 0.561.04.317680.05241250transit432.460.965700 [34] Proper name Haik
WASP-36b 2.3611.3271.537365960.026771733transit12741.085959 [35] [36] [37] [38] [39] [40]
WASP-37b 1.81.163.5774690.04461323+23
−15		transit11190.925±0.125800±150Metal-poor host star [41]
WASP-38b 3.441.236.871880.075221250transit446.11.766180 [42] [32] [43] Proper name Iztok [44]
WASP-41b 0.941.183.0524040.041244transit5900.935545 [45]
HD 192310 b 0.05374.720.32radial vel.28.70.785069 [46]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

Related Research Articles

<span class="mw-page-title-main">Wide Angle Search for Planets</span> Exoplanet search project

WASP or Wide Angle Search for Planets is an international consortium of several academic organisations performing an ultra-wide angle search for exoplanets using transit photometry. The array of robotic telescopes aims to survey the entire sky, simultaneously monitoring many thousands of stars at an apparent visual magnitude from about 7 to 13.

WASP-5 is a magnitude 12 G-type main-sequence star located about 1,020 light-years away in the Phoenix constellation. The star is likely older than the Sun, slightly enriched in heavy elements and is rotating rapidly, being spun up by the tides raised by the giant planet on a close orbit.

WASP-16 is a magnitude 11 yellow dwarf main sequence star, with characteristics similar to the Sun, located in the Virgo constellation.

WASP-79b, also known as Pollera, is an extrasolar planet orbiting the star CD-30 1812. This planet is in the constellation Eridanus, and is about 810 light-years from Earth.

WASP-32 is a yellow main-sequence star in the constellation of Pisces. The star was given the formal name Parumleo in January 2020, Latin for small lion and referencing the national animal of Singapore.

WASP-26 is a yellow main sequence star in the constellation of Cetus.

WASP-25 is a yellow main sequence star in the constellation of Hydra.

WASP-50 is a G-type main-sequence star about 610 light-years away. The star is older than the Sun and slightly depleted in heavy elements compared to the Sun, and has a close to average starspot activity. Despite its advanced age, the star is rotating rapidly, being spun up by the tides raised by giant planet on close orbit.

WASP-189 b is an extrasolar planet that has an orbital period around its host star, WASP-189, of less than three earth days, and is about 322 light-years away in the Libra constellation. It was first discovered in 2018, and was observed in 2020 by CHEOPS.

WASP-78, is a single F-type main-sequence star about 2500 light-years away. It is likely to be younger than the Sun at 3.4+1.5
−0.8 billion years. WASP-78 is depleted in heavy elements, having a 45% concentration of iron compared to the Sun.

BD+00 316 is an ordinary star with a close-orbiting planetary companion in the equatorial constellation of Cetus. It is also known as WASP-71 since 2019; BD+00 316 is the stellar identifier from the Bonner Durchmusterung catalogue. With an apparent visual magnitude of 10.56, it is too faint to be visible to the naked eye. This star is located at a distance of 1,160 light-years based on parallax measurements, and is drifting further away with a heliocentric radial velocity of 7.7 km/s.

WASP-62, formally named Naledi, is a single star about 573 light-years away. It is an F class main-sequence star, orbited by a planet, WASP-62b. The age of WASP-62 is much younger than the Sun at 0.8±0.6 billion years, and it has a metal abundance similar to the Sun.

WASP-61 is a single F-type main-sequence star about 1560 light-years away. The star age is much likely younger than the Sun's at approximately 3.8+1.8
−0.9 billion years. WASP-61 is depleted in heavy elements, having just 40% of the solar abundance of iron.

WASP-88 is a F-type main-sequence star. Its surface temperature is 6450±61 K. WASP-88 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.03±0.04, and is younger at an age of 3.0±1.3 billion years.

WASP-84, also known as BD+02 2056, is a G-type main-sequence star 327 light-years away in the constellation Hydra. Its surface temperature is 5350±31 K and is slightly enriched in heavy elements compared to the Sun, with a metallicity Fe/H index of 0.05±0.02. It is rich in carbon and depleted of oxygen. WASP-84's age is probably older than the Sun at 8.5+4.1
−5.5 billion years. The star appears to have an anomalously small radius, which can be explained by the unusually high helium fraction or by it being very young.

WASP-80 is a K-type main-sequence star about 162 light-years away. The star's age is much younger than the Sun's at 1.352±0.222 billion years. WASP-80 is similar to the Sun in concentration of heavy elements, although this measurement is highly uncertain.

References

  1. ↑ "NASA Exoplanet Archive" . Retrieved 20 December 2019.
  2. ↑ Kovács, G.; Bakos, G. Á.; Hartman, J. D.; Torres, G.; Noyes, R. W.; Latham, D. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Isaacson, H.; Sasselov, D. D.; Stefanik, R. P.; Esquerdo, G. A.; Fernandez, J. M.; Lázár, B. Béky J.; Papp, I.; Sári, P.; Sári, P. (2010), "HAT-P-15b: A 10.9-day Extrasolar Planet Transiting a Solar-type Star", The Astrophysical Journal, 724 (2): 866–877, arXiv: 1005.5300 , Bibcode:2010ApJ...724..866K, doi:10.1088/0004-637X/724/2/866, S2CID   119207125
  3. ↑ Buchhave, L. A.; Bakos, G. Á.; Hartman, J. D.; Torres, G.; Kovács, G.; Latham, D. W.; Noyes, R. W.; Esquerdo, G. A.; Everett, M.; Howard, A. W.; Marcy, G. W.; Fischer, D. A.; Johnson, J. A.; Andersen, J.; Fűrész, G.; Perumpilly, G.; Sasselov, D. D.; Stefanik, R. P.; Béky, B.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-16b: A 4 MJ PLANET TRANSITING A BRIGHT STAR ON AN ECCENTRIC ORBIT", The Astrophysical Journal, 720 (2): 1118–1125, arXiv: 1005.2009 , Bibcode:2010ApJ...720.1118B, doi:10.1088/0004-637X/720/2/1118, S2CID   34104016
  4. 1 2 Hartman, J. D.; Bakos, G. Á.; Sato, B.; Torres, G.; Noyes, R. W.; Latham, D. W.; Kovács, G.; Fischer, D. A.; Howard, A. W.; Johnson, J. A.; Marcy, G. W.; Buchhave, L. A.; Füresz, G.; Perumpilly, G.; Béky, B.; Stefanik, R. P.; Sasselov, D. D.; Esquerdo, G. A.; Everett, M.; Csubry, Z.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-18b and HAT-P-19b: Two Low-Density Saturn-Mass Planets Transiting Metal-Rich K Stars", The Astrophysical Journal, 726: 52, arXiv: 1007.4850 , doi:10.1088/0004-637X/726/1/52, S2CID   10896305
  5. 1 2 3 4 Bakos, G. Á.; Hartman, J.; Torres, G.; Latham, D. W.; Kovács, Géza; Noyes, R. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Howard, A. W.; Kipping, D.; Esquerdo, G. A.; Shporer, A.; Béky, B.; Buchhave, L. A.; Perumpilly, G.; Everett, M.; Sasselov, D. D.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-20b--HAT-P-23b: Four Massive Transiting Extrasolar Planets", The Astrophysical Journal, 742 (2): 116, arXiv: 1008.3388 , doi:10.1088/0004-637X/742/2/116, S2CID   119182075
  6. ↑ Quinn, S. N.; Bakos, G. Á.; Hartman, J.; Torres, G.; Kovács, G.; Latham, D. W.; Noyes, R. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Howard, A. W.; Szentgyorgyi, A.; Fűrész, G.; Buchhave, L. A.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Perumpilly, G.; Everett, M.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-25b: a Hot-Jupiter Transiting a Moderately Faint G Star", The Astrophysical Journal, 745: 80, arXiv: 1008.3565 , doi:10.1088/0004-637X/745/1/80, S2CID   119291022
  7. ↑ Hartman, J. D.; Bakos, G. Á.; Kipping, D. M.; Torres, G.; Kovács, G.; Noyes, R. W.; Latham, D. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Isaacson, H.; Quinn, S. N.; Buchhave, L. A.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Esquerdo, G. A.; Everett, M.; Perumpilly, G.; Lázár, J.; Papp, I.; Sári, P. (2011), "HAT-P-26b: A Low-Density Neptune-Mass Planet Transiting a K Star", The Astrophysical Journal, 728 (2): 138, arXiv: 1010.1008 , Bibcode:2011ApJ...728..138H, doi:10.1088/0004-637X/728/2/138, S2CID   119228956
  8. 1 2 3 4 5 6 7 Moutou, Claire; Mayor, Michel; Lo Curto, Gaspare; Ségransan, Damien; Udry, Stéphane; Bouchy, François; Benz, Willy; Lovis, Christophe; Naef, Dominique; Pepe, Francesco; Queloz, Didier; Santos, Nuno C.; Sousa, Sérgio Gonçalves (2010), The HARPS search for southern extra-solar planets: XXVI: Seven new planetary systems, arXiv: 1012.3830 , doi:10.1051/0004-6361/201015371, S2CID   118696125
  9. 1 2 3 4 5 6 7 Johnson, John Asher; Howard, Andrew W.; Bowler, Brendan P.; Henry, Gregory W.; Marcy, Geoffrey W.; Wright, Jason T.; Fischer, Debra A.; Isaacson, Howard (2010), "Retired a Stars and Their Companions. IV. Seven Jovian Exoplanets from Keck Observatory1", Publications of the Astronomical Society of the Pacific, 122 (892): 701–711, arXiv: 1003.3445 , Bibcode:2010PASP..122..701J, doi:10.1086/653809, S2CID   188131
  10. 1 2 3 Meschiari, Stefano; et al. (2011). "The Lick-Carnegie Survey: Four New Exoplanet Candidates". The Astrophysical Journal. 727 (2). 117. arXiv: 1011.4068 . Bibcode:2011ApJ...727..117M. doi:10.1088/0004-637X/727/2/117. S2CID   59065004.
  11. 1 2 3 4 5 Arriagada, Pamela; Butler, R. Paul; Minniti, Dante; López-Morales, Mercedes; Shectman, Stephen A.; Adams, Fred C.; Boss, Alan P.; Chambers, John E. (2010), "Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program", The Astrophysical Journal, 711 (2): 1229–1235, arXiv: 1001.4093 , Bibcode:2010ApJ...711.1229A, doi:10.1088/0004-637X/711/2/1229, S2CID   118682009
  12. ↑ Boisse, Isabelle; Eggenberger, Anne; Santos, Nuno C.; Lovis, Christophe; Bouchy, François; Hébrard, Guillaume; Arnold, Luc; Bonfils, Xavier; Delfosse, Xavier; Desort, Morgan; Díaz, Rodrigo F.; Ehrenreich, David; Forveille, Thierry; Gallenne, Alexandre; Lagrange, Anne-Marie; Moutou, Claire; Udry, Stéphane; Pepe, Francesco; Perrier, Christian; Perruchot, Sandrine; Pont, Frédéric; Queloz, Didier; Santerne, Alexandre; Ségransan, Damien; Vidal-Madjar, Alfred (2010). "The SOPHIE search for northern extrasolar planets". Astronomy & Astrophysics. 523: A88. arXiv: 1006.4984 . doi:10.1051/0004-6361/201014909. S2CID   59134481.
  13. ↑ Giant Planet Occurrence in the Stellar Mass-Metallicity Plane
  14. ↑ Alsubai, K. A.; Parley, N. R.; Bramich, D. M.; West, R. G.; Sorensen, P. M.; Collier Cameron, A.; Latham, D. W.; Horne, K.; Anderson, D. R.; Bakos, G. Á.; Brown, D. J. A.; Buchhave, L. A.; Esquerdo, G. A.; Everett, M. E.; Fűrész, G.; Hartman, J. D.; Hellier, C.; Miller, G. M.; Pollacco, D.; Quinn, S. N.; Smith, J. C.; Stefanik, R. P.; Szentgyorgyi, A. (2011). "Qatar-1b: A hot Jupiter orbiting a metal-rich K dwarf star". Monthly Notices of the Royal Astronomical Society. 417 (1): 709–716. arXiv: 1012.3027 . Bibcode:2011MNRAS.417..709A. doi:10.1111/j.1365-2966.2011.19316.x. S2CID   55675165.
  15. ↑ Garhart, Emily; Deming, Drake; Mandell, Avi; Knutson, Heather A.; Wallack, Nicole; Burrows, Adam; Fortney, Jonathan J.; Hood, Callie; Seay, Christopher; Sing, David K.; Benneke, Björn; Fraine, Jonathan D.; Kataria, Tiffany; Lewis, Nikole; Madhusudhan, Nikku; McCullough, Peter; Stevenson, Kevin B.; Wakeford, Hannah (2020). "Statistical Characterization of Hot Jupiter Atmospheres Using Spitzer's Secondary Eclipses". The Astronomical Journal. 159 (4): 137. arXiv: 1901.07040 . Bibcode:2020AJ....159..137G. doi: 10.3847/1538-3881/ab6cff . S2CID   119209434.
  16. ↑ A new take on the low-mass brown dwarf companions on wide orbits in Upper-Scorpius.
  17. ↑ M. Kuzuhara, M. Tamura, M. Ishii, T. Kudo, S. Nishiyama, and R. Kandori, "THE WIDEST-SEPARATION SUBSTELLAR COMPANION CANDIDATE TO A BINARY T TAURI STAR", 2011
  18. ↑ Triaud, A. H. M. J.; Queloz, D.; Hellier, C.; Gillon, M.; Smalley, B.; Hebb, L.; Collier Cameron, A.; Anderson, D.; Boisse, I.; Hébrard, G.; Jehin, E.; Lister, T.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Ségransan, D.; Simpson, E.; Udry, S.; West, R. (2011). "WASP-23b: A transiting hot Jupiter around a K dwarf and its Rossiter-Mc Laughlin effect". Astronomy & Astrophysics. 531: A24. arXiv: 1103.2603 . Bibcode:2011A&A...531A..24T. doi:10.1051/0004-6361/201016367. S2CID   7786007.
  19. ↑ Enoch, B.; Cameron, A. Collier; Anderson, D. R.; Lister, T. A.; Hellier, C.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Brown, D. J. A.; Gillon, M.; Hebb, L.; Lendl, M.; Parley, N.; Pepe, F.; Pollacco, D.; Segransan, D.; Simpson, E.; Street, R. A.; Udry, S. (2010). "WASP-25b: A 0.6 MJ planet in the Southern hemisphere". Monthly Notices of the Royal Astronomical Society: no. arXiv: 1009.5917 . doi:10.1111/j.1365-2966.2010.17550.x. S2CID   6314762.
  20. ↑ Brown, D. J. A.; Cameron, A. Collier; Anderson, D. R.; Enoch, B.; Hellier, C.; Maxted, P. F. L.; Miller, G. R. M.; Pollacco, D.; Queloz, D.; Simpson, E.; Smalley, B.; Triaud, A. H. M. J.; Boisse, I.; Bouchy, F.; Gillon, M.; Hébrard, G. (2012). "Rossiter-Mc Laughlin effect measurements for WASP-16, WASP-25 and WASP-31★". Monthly Notices of the Royal Astronomical Society. 423 (2): 1503–1520. arXiv: 1203.4971 . Bibcode:2012MNRAS.423.1503B. doi:10.1111/j.1365-2966.2012.20973.x. S2CID   53445367.
  21. ↑ Southworth, John; Hinse, T. C.; Burgdorf, M.; Calchi Novati, S.; Dominik, M.; Galianni, P.; Gerner, T.; Giannini, E.; Gu, S.-H.; Hundertmark, M.; Jørgensen, U. G.; Juncher, D.; Kerins, E.; Mancini, L.; Rabus, M.; Ricci, D.; Schäfer, S.; Skottfelt, J.; Tregloan-Reed, J.; Wang, X.-B.; Wertz, O.; Alsubai, K. A.; Andersen, J. M.; Bozza, V.; Bramich, D. M.; Browne, P.; Ciceri, S.; d'Ago, G.; Damerdji, Y.; et al. (2014). "High-precision photometry by telescope defocussing – VI. WASP-24, WASP-25 and WASP-26★". Monthly Notices of the Royal Astronomical Society. 444 (1): 776–789. arXiv: 1407.6253 . Bibcode:2014MNRAS.444..776S. doi:10.1093/mnras/stu1492. S2CID   53641330.
  22. ↑ Smalley, B.; Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Hellier, C.; Lister, T. A.; Maxted, P. F. L.; Queloz, D.; Triaud, A. H. M. J.; West, R. G.; Bentley, S. J.; Enoch, B.; Pepe, F.; Pollacco, D. L.; Segransan, D.; Smith, A. M. S.; Southworth, J.; Udry, S.; Wheatley, P. J.; Wood, P. L.; Bento, J. (2010). "WASP-26b: A 1-Jupiter-mass planet around an early-G-type star". Astronomy and Astrophysics. 520: A56. arXiv: 1004.1542 . Bibcode:2010A&A...520A..56S. doi:10.1051/0004-6361/201014705. S2CID   55114421.
  23. ↑ internet archive - WASP-28b: a hot Jupiter transiting a low-metallicity star
  24. ↑ Anderson, D. R.; Collier Cameron, A.; Hellier, C.; Lendl, M.; Lister, T. A.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Smith, A. M. S.; Triaud, A. H. M. J.; Brown, D. J. A.; Gillon, M.; Neveu-Vanmalle, M.; Pepe, F.; Pollacco, D.; Ségransan, D.; Udry, S.; West, R. G.; Wheatley, P. J. (2014), "WASP-20b and WASP-28b: A hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars", Astronomy & Astrophysics, 575: A61, arXiv: 1402.1482 , doi:10.1051/0004-6361/201423591, S2CID   119211951
  25. ↑ Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Brown, D. J. A.; Enoch, B.; Lister, T. A.; Pepe, F.; Pollacco, D.; Ségransan, D.; Udry, S. (2010). "WASP-29b: A SATURN-SIZED TRANSITING EXOPLANET". The Astrophysical Journal. 723 (1): L60–L63. arXiv: 1009.5318 . Bibcode:2010ApJ...723L..60H. doi:10.1088/2041-8205/723/1/L60. S2CID   64119308.
  26. ↑ A Gemini ground-based transmission spectrum of WASP-29b: a featureless spectrum from 515 to 720 nm
  27. ↑ TERMS PHOTOMETRY OF KNOWN TRANSITING EXOPLANETS
  28. ↑ WASP-29b: Another Cool Exoplanet With Abundant CO?
  29. ↑ Ian Wong, "Optical to near-infrared transmission spectra of three cool gas giants"
  30. ↑ Lei-Lei Sun, Sheng-Hong Gu, Xiao-Bin Wang at al., "Long-term transit timing monitoring and homogenous study of WASP-32", 2015
  31. ↑ Brothwell, R. D.; Watson, C. A.; Hébrard, G.; Triaud, A. H. M. J.; Cegla, H. M.; Santerne, A.; Hébrard, E.; Anderson, D. R.; Pollacco, D.; Simpson, E. K.; Bouchy, F.; Brown, D. J. A.; Chew, Y. Gómez Maqueo; Cameron, A. Collier; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Busuttil, R.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Haswell, C. A.; Hellier, C.; Jehin, E.; Kolb, U.; et al. (2014). "A window on exoplanet dynamical histories: Rossiter–Mc Laughlin observations of WASP-13b and WASP-32b". Monthly Notices of the Royal Astronomical Society. 440 (4): 3392–3401. arXiv: 1403.4095 . Bibcode:2014MNRAS.440.3392B. doi:10.1093/mnras/stu520. S2CID   118435056.
  32. 1 2 Brown, D. J. A.; Collier Cameron, A.; Díaz, R. F.; Doyle, A. P.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; Anderson, D. R.; Enoch, B.; Hellier, C.; Maxted, P. F. L.; Miller, G. R. M.; Pollacco, D.; Queloz, D.; Boisse, I.; Hébrard, G. (2012). "Analysis of Spin-Orbit Alignment in the Wasp-32, Wasp-38, and Hat-P-27/Wasp-40 Systems". The Astrophysical Journal. 760 (2): 139. arXiv: 1303.5649 . Bibcode:2012ApJ...760..139B. doi:10.1088/0004-637X/760/2/139. S2CID   54033638.
  33. ↑ P. F. L. Maxted, D. R. Anderson, A. Collier Cameron, M. Gillon, C. Hellier, D. Queloz, B. Smalley, A. H. M. J. Triaud, R. G. West, R. Enoch, "WASP-32b: A Transiting Hot Jupiter Planet Orbiting a Lithium-Poor, Solar-Type Star", 2010
  34. ↑ WASP-34b: a near-grazing transiting sub-Jupiter-mass exoplanet in a hierarchical triple system
  35. ↑ Smith, A. M. S.; Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Hellier, C.; Lendl, M.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Barros, S. C. C.; Jehin, E.; Pepe, F.; Pollacco, D.; Segransan, D.; Southworth, J.; Street, R. A.; Udry, S. (2012). "WASP-36b: A NEW TRANSITING PLANET AROUND a METAL-POOR G-DWARF, AND AN INVESTIGATION INTO ANALYSES BASED ON a SINGLE TRANSIT LIGHT CURVE". The Astronomical Journal. 143 (4): 81. arXiv: 1110.5313 . Bibcode:2012AJ....143...81S. doi:10.1088/0004-6256/143/4/81. S2CID   67754202.
  36. ↑ WASP-36 b Solar analogue 1.5 day orbital period 2.4 Jupiter masses 1.4 Jupiter radii
  37. ↑ Zhou, G.; Bayliss, D. D. R.; Kedziora-Chudczer, L.; Tinney, C. G.; Bailey, J.; Salter, G.; Rodriguez, J. (2015). "Secondary eclipse observations for seven hot-Jupiters from the Anglo-Australian Telescope". Monthly Notices of the Royal Astronomical Society. 454 (3): 3002–3019. arXiv: 1509.04147 . Bibcode:2015MNRAS.454.3002Z. doi:10.1093/mnras/stv2138. S2CID   84835437.
  38. ↑ Mancini, L.; Kemmer, J.; Southworth, J.; Bott, K.; Mollière, P.; Ciceri, S.; Chen, G.; Henning, Th. (2016). "An optical transmission spectrum of the giant planet WASP-36 b". Monthly Notices of the Royal Astronomical Society. 459 (2): 1393–1402. arXiv: 1603.08031 . Bibcode:2016MNRAS.459.1393M. doi:10.1093/mnras/stw659. S2CID   53411511.
  39. ↑ Maciejewski, G.; Dimitrov, D.; Mancini, L.; Southworth, J.; Ciceri, S.; D'Ago, G.; Bruni, I.; Raetz, St.; Nowak, G.; Ohlert, J.; Puchalski, D.; Saral, G.; Derman, E.; Petrucci, R.; Jofre, E.; Seeliger, M.; Henning, T. (2016). "New transit observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b, and WASP-39 B". Acta Astronomica. 66 (1): 55. arXiv: 1603.03268 . Bibcode:2016AcA....66...55M.
  40. ↑ Secondary eclipse observations for seven hot-Jupiters from the Anglo-Australian Telescope, 2015
  41. ↑ Simpson, E. K.; Faedi, F.; Barros, S. C. C.; Brown, D. J. A.; Cameron, A. Collier; Hebb, L.; Pollacco, D.; Smalley, B.; Todd, I.; Butters, O. W.; Hébrard, G.; McCormac, J.; Miller, G. R. M.; Santerne, A.; Street, R. A.; Skillen, I.; Triaud, A. H. M. J.; Anderson, D. R.; Bento, J.; Boisse, I.; Bouchy, F.; Enoch, B.; Haswell, C. A.; Hellier, C.; Holmes, S.; Horne, K.; Keenan, F. P.; Lister, T. A.; Maxted, P. F. L.; et al. (2011). "WASP-37b: A 1.8MJEXOPLANET TRANSITING a METAL-POOR STAR". The Astronomical Journal. 141 (1): 8. arXiv: 1008.3096 . Bibcode:2011AJ....141....8S. doi:10.1088/0004-6256/141/1/8. S2CID   20036137.
  42. ↑ Simpson, E. K.; Pollacco, D.; Cameron, A. Collier; Hébrard, G.; Anderson, D. R.; Barros, S. C. C.; Boisse, I.; Bouchy, F.; Faedi, F.; Gillon, M.; Hebb, L.; Keenan, F. P.; Miller, G. R. M.; Moutou, C.; Queloz, D.; Skillen, I.; Sorensen, P.; Stempels, H. C.; Triaud, A.; Watson, C. A.; Wilson, P. A. (2011). "The spin-orbit angles of the transiting exoplanets WASP-1b, WASP-24b, WASP-38b and HAT-P-8b from Rossiter-Mc Laughlin observations★". Monthly Notices of the Royal Astronomical Society. 414 (4): 3023–3035. arXiv: 1011.5664 . Bibcode:2011MNRAS.414.3023S. doi:10.1111/j.1365-2966.2011.18603.x. S2CID   46522188.
  43. ↑ Barros, S. C. C.; Faedi, F.; Collier Cameron, A.; Lister, T. A.; McCormac, J.; Pollacco, D.; Simpson, E. K.; Smalley, B.; Street, R. A.; Todd, I.; Triaud, A. H. M. J.; Boisse, I.; Bouchy, F.; Hébrard, G.; Moutou, C.; Pepe, F.; Queloz, D.; Santerne, A.; Segransan, D.; Udry, S.; Bento, J.; Butters, O. W.; Enoch, B.; Haswell, C. A.; Hellier, C.; Keenan, F. P.; Miller, G. R. M.; Moulds, V.; Norton, A. J.; et al. (2011). "WASP-38b: A transiting exoplanet in an eccentric, 6.87d period orbit". Astronomy & Astrophysics. 525: A54. arXiv: 1010.0849 . Bibcode:2011A&A...525A..54B. doi:10.1051/0004-6361/201015800. S2CID   5723076.
  44. ↑ The IAU announces names for WASP exoplanets
  45. ↑ Maxted, P. F. L.; Anderson, D. R.; Collier Cameron, A.; Hellier, C.; Queloz, D.; Smalley, B.; Street, R. A.; Triaud, A. H. M. J.; West, R. G.; Gillon, M.; Lister, T. A.; Pepe, F.; Pollacco, D.; Ségransan, D.; Smith, A. M. S.; Udry, S. (2010), "WASP-41b: A Transiting Hot Jupiter Planet Orbiting a Magnetically Active G8V Star", Publications of the Astronomical Society of the Pacific, 123 (903): 547–554, arXiv: 1012.2977 , doi:10.1086/660007, S2CID   40017204
  46. ↑ Pepe, Francesco; 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. arXiv: 1108.3447 . Bibcode:2011A&A...534A..58P. doi:10.1051/0004-6361/201117055. S2CID   15088852.
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