Esta é uma Lista de exoplanetas descobertos em 2018.[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)
↑ abcTakarada, Takuya; et al. (2018). «Planets around the evolved stars 24 Booties and γ Libra: A 30d-period planet and a double giant-planet system in possible 7:3 MMR». Publications of the Astronomical Society of Japan. 70 (4). arXiv:1804.04008. doi:10.1093/pasj/psy052
↑Ma, Bo; et al. (2018). «The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey». Monthly Notices of the Royal Astronomical Society. 480 (2). 2411 páginas. Bibcode:2018MNRAS.480.2411M. arXiv:1807.07098. doi:10.1093/mnras/sty1933
↑Rey, J.; Bouchy, F.; Stalport, M.; Deleuil, M.; Hébrard, G.; Almenara, J. M.; Alonso, R.; Barros, S. C. C.; Bonomo, A. S.; Cazalet, G.; Delisle, J. B.; Díaz, R. F.; Fridlund, M.; Guenther, E. W.; Guillot, T.; Montagnier, G.; Moutou, C.; Lovis, C.; Queloz, D.; Santerne, A.; Udry, S. (2018), «Brown dwarf companion with a period of 4.6 yr interacting with the hot Jupiter CoRoT-20 B», Astronomy & Astrophysics, 619: A115, arXiv:1807.01229, doi:10.1051/0004-6361/201833180
↑Han, Z.-T.; Qian, S.-B.; Zhu, L.-Y.; Zhi, Q.-J.; Dong, A.-J.; Soonthornthum, B.; Poshyachinda, S.; Sarotsakulchai, T.; Fang, X.-H.; Wang, Q.-S.; Voloshina, Irina (2018). «DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet». The Astrophysical Journal. 868: 53. doi:10.3847/1538-4357/aae64d
↑Pinamonti, M.; Damasso, M.; Marzari, F.; Sozzetti, A.; Desidera, S.; Maldonado, J.; Scandariato, G.; Affer, L.; Lanza, A. F.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Giacobbe, P.; González-Álvarez, E.; González Hernández, J. I.; Gratton, R.; Leto, G.; Malavolta, L.; Martinez Fiorenzano, A.; Micela, G.; Molinari, E.; Pagano, I.; Pedani, M.; Perger, M.; Piotto, G.; Rebolo, R.; Ribas, I.; et al. (2018). «The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction». Astronomy and Astrophysics. 617: A104. Bibcode:2018A&A...617A.104P. arXiv:1804.03476. doi:10.1051/0004-6361/201732535
↑ abLuque, R.; Nowak, G.; Pallé, E.; Kossakowski, D.; Trifonov, T.; Zechmeister, M.; Béjar, V. J. S.; Cardona Guillén, C.; Tal-Or, L.; Hidalgo, D.; Ribas, I.; Reiners, A.; Caballero, J. A.; Amado, P. J.; Quirrenbach, A.; Aceituno, J.; Cortés-Contreras, M.; Díez-Alonso, E.; Dreizler, S.; Guenther, E. W.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; Montes, D.; Morales, J. C.; Passegger, V. M.; Schmitt, J. H. M. M.; Schweitzer, A. (2018), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 620: A171, arXiv:1810.07572, doi:10.1051/0004-6361/201833423
↑ abcdBento, J.; Hartman, J. D.; Bakos, G. Á.; Bhatti, W.; Csubry, Z.; Penev, K.; Bayliss, D.; De Val-Borro, M.; Zhou, G.; Brahm, R.; Espinoza, N.; Rabus, M.; Jordán, A.; Suc, V.; Ciceri, S.; Sarkis, P.; Henning, T.; Mancini, L.; Tinney, C. G.; Wright, D. J.; Durkan, S.; Tan, T. G.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-39b, HATS-40b, HATS-41b, and HATS-42b: Three inflated hot Jupiters and a super-Jupiter transiting F stars», Monthly Notices of the Royal Astronomical Society, 477 (3): 3406–3423, arXiv:1804.01623, doi:10.1093/mnras/sty726
↑ abcdeEspinoza, N.; Hartman, J. D.; Bakos, G. Á.; Henning, T.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Suc, V.; Jordán, A.; Mancini, L.; Tan, T. G.; Penev, K.; Rabus, M.; Sarkis, P.; De Val-Borro, M.; Durkan, S.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-54b–HATS-58Ab: Five New Transiting Hot Jupiters Including One with a Possible Temperate Companion», The Astronomical Journal, 158 (2): 63, arXiv:1812.07668, doi:10.3847/1538-3881/ab26bb
↑Jackson, David G.; et al. (2022), «The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey», Monthly Notices of the Royal Astronomical Society, 518 (4): 4845–4860, arXiv:2211.01044, doi:10.1093/mnras/stac3192
↑ abSarkis, P.; Henning, Th.; Hartman, J. D.; Bakos, G. Á.; Brahm, R.; Jordán, A.; Bayliss, D.; Mancini, L.; Espinoza, N.; Rabus, M.; Csubry, Z.; Bhatti, W.; Penev, K.; Zhou, G.; Bento, J.; Tan, T. G.; Arriagada, P.; Butler, R. P.; Crane, J. D.; Shectman, S.; Tinney, C. G.; Wright, D. J.; Addison, B.; Durkan, S.; Suc, V.; Buchhave, L. A.; Val-Borro, M. de; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet around a Sun-like Star», The Astronomical Journal, 156 (5): 216, arXiv:1805.05925, doi:10.3847/1538-3881/aade54
↑ abcdefghijHartman, J. D.; Bakos, G. Á.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Henning, Th.; Jordán, A.; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V.; Val-Borro, M. de; Zhou, G.; Addison, B.; Arriagada, P.; Butler, R. P.; Crane, J.; Durkan, S.; Shectman, S.; Tan, T. G.; Thompson, I.; Tinney, C. G.; Wright, D. J.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-60b–HATS-69b: 10 Transiting Planets from HATSouth», The Astronomical Journal, 157 (2): 55, arXiv:1809.01048, doi:10.3847/1538-3881/aaf8b6
↑HATS-70b: A 13 Mjup brown dwarf transiting an A star, 2018, arXiv:1811.06925
↑A Jovian planet in an eccentric 11.5 day orbit around HD1397 discovered by TESS, 2018, arXiv:1811.01882
↑HD 1397b: a transiting warm giant planet orbiting a V = 7.8 mag sub-giant star discovered by TESS, 2018, arXiv:1811.02156
↑HD2685 b: A Hot-Jupiter orbiting an early F-type star detected by TESS, 2018, arXiv:1811.05518
↑ abcdefghijkLuhn, Jacob K.; Bastien, Fabienne A.; Wright, Jason T.; Johnson, John A.; Howard, Andrew W.; Isaacson, Howard (2018), «Retired a Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts», The Astronomical Journal, 157 (4): 149, arXiv:1811.03043, doi:10.3847/1538-3881/aaf5d0
↑ abcdefghMent, Kristo; Fischer, Debra A.; Bakos, Gaspar; Howard, Andrew W.; Isaacson, Howard (2018), «Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810», The Astronomical Journal, 156 (5): 213, arXiv:1809.01228, doi:10.3847/1538-3881/aae1f5
↑Yu, Liang; Rodriguez, Joseph E.; Eastman, Jason D.; Crossfield, Ian J. M.; Shporer, Avi; Gaudi, B. Scott; Burt, Jennifer; Fulton, Benjamin J.; Sinukoff, Evan; Howard, Andrew W.; Isaacson, Howard; Kosiarek, Molly R.; Ciardi, David R.; Schlieder, Joshua E.; Penev, Kaloyan; Vanderburg, Andrew; Stassun, Keivan G.; Bieryla, Allyson; Butler, R. Paul; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Latham, David W.; Murawski, Gabriel; Stevens, Daniel J.; Petigura, Erik A.; Kreidberg, Laura; Bristow, Makennah (2018), «Two Warm, Low-density Sub-Jovian Planets Orbiting Bright Stars in K2 Campaigns 13 and 14», The Astronomical Journal, 156 (3): 127, arXiv:1803.02858, doi:10.3847/1538-3881/aad6e7
↑Van Eylen, V.; et al. (2018), «HD 89345: A bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2», Monthly Notices of the Royal Astronomical Society, 478 (4): 4866–4880, arXiv:1805.01860, doi:10.1093/mnras/sty1390
↑Bang, Tae-Yang; Lee, Byeong-Cheol; Jeong, Gwang-Hui; Han, Inwoo; Park, Myeong-Gu (2018), «Search for Exoplanets Around Northern Circumpolar Stars III. Long-Period Radial Velocity Variations in Hd 18438 and Hd 158996», Journal of the Korean Astronomical Society, 51 (1), arXiv:1803.07213, doi:10.5303/JKAS.2018.51.1.17
↑The CARMENES search for exoplanets around M dwarfs A Neptune-mass planet traversing the habitable zone around HD 180617, 2018, arXiv:1808.01183
↑HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess, 2018, arXiv:1810.02341
↑ abDelisle, J.-B.; Ségransan, D.; Dumusque, X.; Diaz, R. F.; Bouchy, F.; Lovis, C.; Pepe, F.; Udry, S.; Alonso, R.; Benz, W.; 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. C.; Wyttenbach, A. (2018), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 614: A133, arXiv:1802.04631, doi:10.1051/0004-6361/201732529
↑Esposito, M.; Armstrong, D. J.; Gandolfi, D.; Adibekyan, V.; Fridlund, M.; Santos, N. C.; Livingston, J. H.; Mena, E. Delgado; Fossati, L.; Lillo-Box, J.; Barragán, O.; Barrado, D.; Cubillos, P. E.; Cooke, B.; Justesen, A. B. (1 de março de 2019). «HD 219666 b: a hot-Neptune from TESS Sector 1». Astronomy and Astrophysics. 623: A165. ISSN0004-6361. doi:10.1051/0004-6361/201834853
↑ abThe GAPS Programme with HARPS-N at TNG XVIII. Two new giant planets around the metal-poor stars HD 220197 and HD 233832, 2018, arXiv:1811.07776
↑ abAdamów, M.; Niedzielski, A.; Kowalik, K.; Villaver, E.; Wolszczan, A.; MacIejewski, G.; Gromadzki, M. (2018), «Tracking Advanced Planetary Systems (TAPAS) with HARPS-N», Astronomy & Astrophysics, 613: A47, arXiv:1801.04379, doi:10.1051/0004-6361/201732161
↑Leão, I. C.; Canto Martins, B. L.; Alves, S.; Pereira De Oliveira, G.; Cortés, C.; Brucalassi, A.; Melo, C. H. F.; De Freitas, D. B.; Pasquini, L.; De Medeiros, J. R. (2018), «Incidence of planet candidates in open clusters and a planet confirmation», Astronomy & Astrophysics, 620: A139, arXiv:1807.03196, doi:10.1051/0004-6361/201833123
↑Delgado Mena, E.; Lovis, C.; Santos, N. C.; Gomes Da Silva, J.; Mortier, A.; Tsantaki, M.; Sousa, S. G.; Figueira, P.; Cunha, M. S.; Campante, T. L.; Adibekyan, V.; Faria, J. P.; Montalto, M. (2018), «Planets around evolved intermediate-mass stars», Astronomy & Astrophysics, 619: A2, arXiv:1807.09608, doi:10.1051/0004-6361/201833152
↑ abcdeChristiansen, Jessie L.; Crossfield, Ian J. M.; Barentsen, Geert; Lintott, Chris J.; Barclay, Thomas; Simmons, Brooke D.; Petigura, Erik; Schlieder, Joshua E.; Dressing, Courtney D.; Vanderburg, Andrew; Ciardi, David R.; Allen, Campbell; McMaster, Adam; Miller, Grant; Veldthuis, Martin; Allen, Sarah; Wolfenbarger, Zach; Cox, Brian; Zemiro, Julia; Howard, Andrew W.; Livingston, John; Sinukoff, Evan; Catron, Timothy; Grey, Andrew; Kusch, Joshua J. E.; Terentev, Ivan; Vales, Martin; Kristiansen, Martti H. (11 de janeiro de 2018). «The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists». The Astronomical Journal (em inglês). 155 (2). 57 páginas. Bibcode:2018AJ....155...57C. ISSN1538-3881. arXiv:1801.03874. doi:10.3847/1538-3881/aa9be0
↑ abcDiez Alonso, E.; Suarez Gomez, S. L.; Gonzalez Hernandez, J. I.; Suarez Mascareno, A.; Gonzalez Gutierrez, C.; Velasco, S.; Toledo Padron, B.; de Cos Juez, F. J.; Rebolo, R. (2018), A system of three transiting super-Earths in a cool dwarf star, arXiv:1801.06249
↑ abcdefgAdams, Elisabeth R.; et al. (2020). «Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10». The Planetary Science Journal. 2 (4): 152. Bibcode:2021PSJ.....2..152A. arXiv:2011.11698. doi:10.3847/PSJ/ac0ea0
↑ abcAkana Murphy, Joseph M.; Kosiarek, Molly R.; Batalha, Natalie M.; Gonzales, Erica J.; Isaacson, Howard; Petigura, Erik A.; Weiss, Lauren M.; Grunblatt, Samuel K.; Ciardi, David R.; Fulton, Benjamin; Hirsch, Lea A.; Behmard, Aida; Rosenthal, Lee J. (2021), «Another Superdense Sub-Neptune in K2-182 b and Refined Mass Measurements for K2-199 b and C», The Astronomical Journal, 162 (6): 294, Bibcode:2021AJ....162..294A, arXiv:2110.05502, doi:10.3847/1538-3881/ac2830
↑Nava, Chantanelle; et al. (2021), «K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals», The Astronomical Journal, 163 (2): 41, Bibcode:2022AJ....163...41N, arXiv:2111.02608, doi:10.3847/1538-3881/ac3141
↑Curtis, Jason Lee; Vanderburg, Andrew; Torres, Guillermo; Kraus, Adam L.; Huber, Daniel; Mann, Andrew W.; Rizzuto, Aaron C.; Isaacson, Howard; Howard, Andrew W.; Henze, Christopher E.; Fulton, Benjamin J.; Wright, Jason T. (2018), «K2-231 b: A Sub-Neptune Exoplanet Transiting a Solar Twin in Ruprecht 147», The Astronomical Journal, 155 (4): 173, arXiv:1803.07430, doi:10.3847/1538-3881/aab49c
↑Wang, Songhu; Winn, Joshua N.; Addison, Brett C.; Dai, Fei; Rice, Malena; Holden, Bradford; Burt, Jennifer A.; Wang, Xian-Yu; Butler, R. Paul; Vogt, Steven S.; Laughlin, Gregory (2021), «The Aligned Orbit of the Eccentric Warm Jupiter K2-232b», The Astronomical Journal, 162 (2): 50, arXiv:2105.12902, doi:10.3847/1538-3881/ac0626
↑ abcDavid, Trevor J.; Crossfield, Ian J. M.; Benneke, Björn; Petigura, Erik A.; Gonzales, Erica J.; Schlieder, Joshua E.; Yu, Liang; Isaacson, Howard T.; Howard, Andrew W.; Ciardi, David R.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Cody, Ann Marie; Riedel, Adric; Schwengeler, Hans Martin; Tanner, Christopher; Ende, Martin (2018), «Three Small Planets Transiting the Bright Young Field Star K2-233», The Astronomical Journal, 155 (5): 222, arXiv:1803.05056, doi:10.3847/1538-3881/aabde8
↑Chakraborty, Abhijit; Roy, Arpita; Sharma, Rishikesh; Mahadevan, Suvrath; Chaturvedi, Priyanka; Prasad, Neelam J. S. S. V.; Anandarao, B. G. (2018), «Evidence of a Sub-Saturn around EPIC 211945201», The Astronomical Journal, 156: 3, arXiv:1805.03466, doi:10.3847/1538-3881/aac436
↑ abSoto, M. G.; Díaz, M. R.; Jenkins, J. S.; Rojas, F.; Espinoza, N.; Brahm, R.; Drass, H.; Jones, M. I.; Rabus, M.; Hartman, J.; Sarkis, P.; Jordán, A.; Lachaume, R.; Pantoja, B.; Vučković, M.; Ciardi, D. R.; Crossfield, I.; Dressing, C.; Gonzales, E.; Hirsch, L. (2018), «K2-237 b and K2-238 b: Discovery and characterization of two new transiting hot Jupiters from K2», Monthly Notices of the Royal Astronomical Society, 478 (4): 5356–5365, arXiv:1801.07959, doi:10.1093/mnras/sty1334
↑ abcdeAlonso, E Díez; Hernández, J I González; Suárez Gómez, S. L.; Aguado, D. S.; González Gutiérrez, C.; Suárez Mascareño, A.; Cabrera-Lavers, A.; González-Nuevo, J.; Toledo–Padrón, B.; Gracia, J.; De Cos Juez, F. J.; Rebolo, R. (2018), «Two planetary systems with transiting Earth-size and super-Earth planets orbiting late-type dwarf stars», Monthly Notices of the Royal Astronomical Society: Letters, arXiv:1806.01181, doi:10.1093/mnrasl/sly102
↑ abJohnson, M. C.; et al. (2018), «K2-260 b: A hot Jupiter transiting an F star, and K2-261 b: A warm Saturn around a bright G star», Monthly Notices of the Royal Astronomical Society, 481: 596–612, arXiv:1806.06099, doi:10.1093/mnras/sty2238
↑Mortier, A.; et al. (2018), «K2-263 b: A 50 d period sub-Neptune with a mass measurement using HARPS-N», Monthly Notices of the Royal Astronomical Society, 481 (2): 1839–1847, arXiv:1808.08187, doi:10.1093/mnras/sty2360
↑ abRizzuto, Aaron C.; Vanderburg, Andrew; Mann, Andrew W.; Kraus, Adam L.; Dressing, Courtney D.; Agüeros, Marcel A.; Douglas, Stephanie T.; Krolikowski, Daniel M. (2018), «Zodiacal Exoplanets in Time (ZEIT). VIII. A Two-planet System in Praesepe from K2 Campaign 16», The Astronomical Journal, 156 (5): 195, arXiv:1808.07068, doi:10.3847/1538-3881/aadf37
↑ abLivingston, John H.; et al. (2018), «K2-264: A transiting multiplanet system in the Praesepe open cluster», Monthly Notices of the Royal Astronomical Society, 484: 8–18, arXiv:1809.01968, doi:10.1093/mnras/sty3464
↑Gomes, G. O.; Bolmont, E.; Blanco-Cuaresma, S. (2021), «Influence of equilibrium tides on transit-timing variations of close-in super-Earths», Astronomy & Astrophysics, 651: A23, arXiv:2104.13808, doi:10.1051/0004-6361/202040202
↑ abcdRodriguez, Joseph E.; Becker, Juliette C.; Eastman, Jason D.; Hadden, Sam; Vanderburg, Andrew; Khain, Tali; Quinn, Samuel N.; Mayo, Andrew; Dressing, Courtney D.; Schlieder, Joshua E.; Ciardi, David R.; Latham, David W.; Rappaport, Saul; Adams, Fred C.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A.; Kristiansen, Martti H.; Omohundro, Mark; Schwengeler, Hans Martin; Stassun, Keivan G.; Terentev, Ivan (2018), «A Compact Multi-planet System with a Significantly Misaligned Ultra Short Period Planet», The Astronomical Journal, 156 (5): 245, arXiv:1806.08368, doi:10.3847/1538-3881/aae530
↑Yu, Liang; Zhou, George; Rodriguez, Joseph E.; Huang, Chelsea X.; Vanderburg, Andrew; Quinn, Samuel N.; Gaudi, B. Scott; Beichman, Charles A.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Ciardi, David R.; Crossfield, Ian J. M.; Eastman, Jason D.; Esquerdo, Gilbert A.; Latham, David W.; Stassun, Keivan G.; Villanueva, Steven (2018), «EPIC 246851721 b: A Tropical Jupiter Transiting a Rapidly Rotating Star in a Well-aligned Orbit», The Astronomical Journal, 156 (6): 250, arXiv:1807.10298, doi:10.3847/1538-3881/aae5d5
↑Nowak, Grzegorz; et al. (2020). «K2-280 b – a low density warm sub-Saturn around a mildly evolved star». Monthly Notices of the Royal Astronomical Society. 497 (4): 4423–4435. arXiv:2007.07939. doi:10.1093/mnras/staa2077
↑Petigura, Erik A.; et al. (2017). «Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy». The Astronomical Journal. 155: 21. arXiv:1711.06377. doi:10.3847/1538-3881/aa9b83
↑David, Trevor J.; Mamajek, Eric E.; Vanderburg, Andrew; Schlieder, Joshua E.; Bristow, Makennah; Petigura, Erik A.; Ciardi, David R.; Crossfield, Ian J. M.; Isaacson, Howard T.; Cody, Ann Marie; Stauffer, John R.; Hillenbrand, Lynne A.; Bieryla, Allyson; Latham, David W.; Fulton, Benjamin J.; Rebull, Luisa M.; Beichman, Chas; Gonzales, Erica J.; Hirsch, Lea A.; Howard, Andrew W.; Vasisht, Gautam; Ygouf, Marie (2018), «Discovery of a Transiting Adolescent Sub-Neptune Exoplanet with K2», The Astronomical Journal, 156 (6): 302, arXiv:1801.07320, doi:10.3847/1538-3881/aaeed7
↑ abcdPalle, E.; et al. (2018), «Detection and Doppler monitoring of K2-285 (EPIC 246471491), a system of four transiting planets smaller than Neptune», Astronomy & Astrophysics, 623: A41, arXiv:1808.00575, doi:10.1051/0004-6361/201834001
↑Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130, 2018, arXiv:1812.09242
↑Transiting planet candidate from K2 with the longest period, 2018, arXiv:1806.08757
↑Cañas, Caleb I.; Wang, Songhu; Mahadevan, Suvrath; Bender, Chad F.; De Lee, Nathan; Fleming, Scott W.; García-Hernández, D. A.; Hearty, Fred R.; Majewski, Steven R.; Roman-Lopes, Alexandre; Schneider, Donald P.; Stassun, Keivan G. (2018), «Kepler-730: A Hot Jupiter System with a Close-in, Transiting, Earth-sized Planet», The Astrophysical Journal, 870 (2): L17, arXiv:1812.08358, doi:10.3847/2041-8213/aafa1e
↑Beichman, C. A.; Giles, H. A. C.; Akeson, R.; Ciardi, D.; Christiansen, J.; Isaacson, H.; Marcy, G. M.; Sinukoff, E.; Greene, T.; Fortney, J. J.; Crossfield, I.; Hu, R.; Howard, A. W.; Petigura, E. A.; Knutson, H. A. (2018), «Validation and Initial Characterization of the Long-period Planet Kepler-1654 B», The Astronomical Journal, 155 (4): 158, arXiv:1802.08945, doi:10.3847/1538-3881/aaaeb6
↑Brady, Madison T.; Petigura, Erik A.; Knutson, Heather A.; Sinukoff, Evan; Isaacson, Howard; Hirsch, Lea A.; Fulton, Benjamin J.; Kosiarek, Molly R.; Howard, Andrew W. (2018), «Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity», The Astronomical Journal, 156 (4): 147, arXiv:1809.08436, doi:10.3847/1538-3881/aad773
↑Hébrard, G.; Bonomo, A. S.; Díaz, R. F.; Santerne, A.; Santos, N. C.; Almenara, J.-M.; Barros, S. C. C.; Boisse, I.; Bouchy, F.; Bruno, G.; Courcol, B.; Deleuil, M.; Demangeon, O.; Guillot, T.; Montagnier, G.; Moutou, C.; Rey, J.; Wilson, P. A. (2019), «SOPHIE velocimetry of Keplertransit candidates», Astronomy & Astrophysics, 623: A104, arXiv:1811.09580, doi:10.1051/0004-6361/201834333
↑Zang, Weicheng; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Gould, Andrew; Wang, Tianshu; Zhu, Wei; Mao, Shude; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Jung, Youn Kil; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2018), «KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet», The Astronomical Journal, 156 (5): 236, arXiv:1810.10792, doi:10.3847/1538-3881/aae537
↑ abJung, Youn Kil; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Gould, Andrew; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Shin, In-Gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2018), «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, arXiv:1805.09983, doi:10.3847/1538-3881/aae319
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↑Poleski, Radosław; Gaudi, B. S.; Udalski, A.; Szymański, M. K.; Soszyński, I.; Pietrukowicz, P.; Kozłowski, S.; Skowron, J.; Wyrzykowski, Ł.; Ulaczyk, K. (2018), «An Ice Giant Exoplanet Interpretation of the Anomaly in Microlensing Event OGLE-2011-BLG-0173», The Astronomical Journal, 156 (3): 104, arXiv:1805.00049, doi:10.3847/1538-3881/aad45e
↑ abSuzuki, D.; et al. (2018), «A Likely Detection of a Two-planet System in a Low-magnification Microlensing Event», The Astronomical Journal, 155 (6): 263, arXiv:1803.05238, doi:10.3847/1538-3881/aabd7a
↑OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field, 2018, arXiv:1810.00014
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↑Skowron, J.; et al. (2018), «OGLE-2017-BLG-0373Lb: A Jovian Mass-Ratio Planet Exposes a New Accidental Microlensing Degeneracy», Acta Astronomica, 68 (1), arXiv:1802.10067, doi:10.32023/0001-5237/68.1.2
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↑Blackman, J. W.; Beaulieu, J.-P.; Cole, A. A.; Koshimoto, N.; Vandorou, A.; Bhattacharya, A.; Marquette, J.-B.; Bennett, D. P. (2021). «OGLE-2017-BLG-1434Lb: Confirmation of a Cold Super-Earth Using Keck Adaptive Optics». The Astronomical Journal. 161 (6): 279. Bibcode:2021AJ....161..279B. arXiv:2107.06510. doi:10.3847/1538-3881/abfda3
↑Qatar Exoplanet Survey: Qatar-7b -- A Very Hot Jupiter Orbiting a Metal Rich F-Star, 2018, arXiv:1812.05601
↑Nucita, A. A.; Licchelli, D.; De Paolis, F.; Ingrosso, G.; Strafella, F.; Katysheva, N.; Shugarov, S. (2018), «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, arXiv:1802.06659, doi:10.1093/mnras/sty448
↑Fukui, A.; et al. (2019), «Kojima-1Lb is a Mildly Cold Neptune around the Brightest Microlensing Host Star», The Astronomical Journal, 158 (5): 206, arXiv:1909.11802, doi:10.3847/1538-3881/ab487f
↑Shvartzvald, Y.; Novati, S. Calchi; Gaudi, B. S.; Bryden, G.; Nataf, D. M.; Penny, M. T.; Beichman, C.; Henderson, C. B.; Jacklin, S.; Schlafly, E. F.; Huston, M. J. (2018), «UKIRT-2017-BLG-001Lb: A Giant Planet Detected through the Dust», The Astrophysical Journal, 857: L8, arXiv:1802.06795, doi:10.3847/2041-8213/aab71b
↑ abcdeAnderson, D. R.; et al. (2018). «The discovery of WASP-134b, WASP-134c, WASP-137b, WASP-143b and WASP-146b: three hot Jupiters and a pair of warm Jupiters orbiting Solar-type stars». arXiv:1812.09264 [astro-ph.EP]
↑ abcdefghHellier, Coel; et al. (2019). «New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South». Monthly Notices of the Royal Astronomical Society. 482: 1379–1391. arXiv:1803.02224. doi:10.1093/mnras/sty2741
↑ abcdLendl, M.; et al. (2019). «WASP-147b, 160Bb, 164b, and 165b: Two hot Saturns and two Jupiters, including two planets with metal-rich hosts». Monthly Notices of the Royal Astronomical Society. 482: 301–312. arXiv:1807.06973. doi:10.1093/mnras/sty2667
↑ abcBarkaoui, K.; et al. (2018), «Discovery of Three New Transiting Hot Jupiters: WASP-161 b, WASP-163 b, and WASP-170 B», The Astronomical Journal, 157 (2): 43, arXiv:1807.06548, doi:10.3847/1538-3881/aaf422
↑Wyttenbach, A.; West, R. G.; Udry, S.; Temple, L. Y.; Spake, J. J.; Smalley, B.; Ségransan, D.; Queloz, D.; Pollacco, D.; Pepe, F.; Maxted, P F L.; Nielsen, L. D.; Linder, E.; Lendl, M.; Jehin, E.; Gillon, M.; Ehrenreich, D.; Delrez, L.; Collier Cameron, A.; Burdanov, A.; Bouchy, F.; Triaud, A H M J.; Anderson, D. R.; Hellier, Coel (2018), «WASP-166b: A bloated super-Neptune transiting a V = 9 star», Monthly Notices of the Royal Astronomical Society, 488 (3): 3067–3075, arXiv:1811.05292, doi:10.1093/mnras/stz1903
↑Seidel, J. V.; Cegla, H. M.; Doyle, L.; Lafarga, M.; Brogi, M.; Gandhi, S.; Anderson, D. R.; Allart, R.; Buchschacher, N.; Lovis, C.; Sosnowska, D. (2022), «The hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium», Monthly Notices of the Royal Astronomical Society: Letters, 513: L15–L19, arXiv:2203.04494, doi:10.1093/mnrasl/slac027
↑Doyle, L.; Cegla, H. M.; Bryant, E.; Bayliss, D.; Lafarga, M.; Anderson, D. R.; Allart, R.; Bourrier, V.; Brogi, M.; Buchschacher, N.; Kunovac, V.; Lendl, M.; Lovis, C.; Moyano, M.; Roguet-Kern, N.; Seidel, J. V.; Sosnowska, D.; Wheatley, P. J.; Acton, J. S.; Burleigh, M. R.; Casewell, S. L.; Gill, S.; Goad, M. R.; Henderson, B. A.; Jenkins, J. S.; Tilbrook, R. H.; West, R. G. (2022), «The Hot Neptune WASP-166 b with ESPRESSO – I. Refining the planetary architecture and stellar variability», Monthly Notices of the Royal Astronomical Society, 516: 298–315, arXiv:2207.10127, doi:10.1093/mnras/stac2178
↑Labadie-Bartz, Jonathan; et al. (2018), «KELT-22Ab: A Massive, Short-Period Hot Jupiter Transiting a Near-solar Twin», The Astrophysical Journal Supplement Series, 240: 13, arXiv:1803.07559, doi:10.3847/1538-4365/aaee7e
↑Temple, L. Y.; Hellier, C.; Almleaky, Y.; Anderson, D. R.; Bouchy, F.; Brown, D J A.; Burdanov, A.; Cameron, Collier; Delrez, L.; Gillon, M.; Hall, R.; Jehin, E.; Lendl, M.; Maxted, P F L.; Nielsen, L. D.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Sohy, S.; Thompson, S.; Triaud, A H M J.; Turner, O. D.; Udry, S.; West, R. G. (2018), «Discovery of WASP-174b: Doppler tomography of a near-grazing transit», Monthly Notices of the Royal Astronomical Society, 480 (4): 5307–5313, arXiv:1802.00766, doi:10.1093/mnras/sty2197
↑WASP-190b: Tomographic discovery of a transiting hot Jupiter, 2018, arXiv:1811.05742