Esta é uma Lista de exoplanetas descobertos em 2019.[1][2]
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)
Uma super-Terra em trânsito com um período de 1 dia com uma composição semelhante à da Terra em torno de uma estrela brilhante (V=7.9) revelada por TESS[32]
[104] Até o momento, é o exoplaneta de menor massa confirmado, ou medido, usando a técnica da velocidade radial.[105] Estrela-mãe também conhecida como L 98-59.[106]
↑Luque, R.; Trifonov, T.; Reffert, S.; Quirrenbach, A.; Lee, M. H.; Albrecht, S.; Andersen, M. Fredslund; Antoci, V.; Grundahl, F.; Schwab, C.; Wolthoff, V. (13 de outubro de 2019). «Precise radial velocities of giant stars XIII. A second Jupiter orbiting in 4:3 resonance in the 7 CMa system». Astronomy & Astrophysics. A136. 631 páginas. Bibcode:2019A&A...631A.136L. arXiv:1910.05853. doi:10.1051/0004-6361/201936464
↑Benatti, S.; Nardiello, D.; Malavolta, L.; Desidera, S.; Borsato, L.; Nascimbeni, V.; Damasso, M.; D'Orazi, V.; Mesa, D.; Messina, S.; Esposito, M.; Bignamini, A.; Claudi, R.; Covino, E.; Lovis, C.; Sabotta, S. (outubro de 2019). «A possibly inflated planet around the bright young star DS Tucanae A». Astronomy & Astrophysics (em inglês). 630: A81. Bibcode:2019A&A...630A..81B. ISSN0004-6361. arXiv:1904.01591. doi:10.1051/0004-6361/201935598
↑Feng, Fabo; Anglada-Escudé, Guillem; Tuomi, Mikko; Jones, Hugh R. A.; Chanamé, Julio; Butler, Paul R.; Janson, Markus (14 de outubro de 2019), «Detection of the nearest Jupiter analog in radial velocity and astrometry data», Monthly Notices of the Royal Astronomical Society, 490 (4): 5002–5016, Bibcode:2019MNRAS.490.5002F, arXiv:1910.06804, doi:10.1093/mnras/stz2912
↑ abcJenkins, J. S.; Pozuelos, F. J.; Tuomi, M.; Berdiñas, Z. M.; Díaz, M. R.; Vines, J. I.; Suárez, Juan C.; Peña Rojas, P. A. (2019), «GJ 357: A low-mass planetary system uncovered by precision radial velocities and dynamical simulations», Monthly Notices of the Royal Astronomical Society, 490 (4): 5585–5595, arXiv:1909.00831, doi:10.1093/mnras/stz2937
↑Pinamonti, M.; Sozzetti, A.; Giacobbe, P.; Damasso, M.; Scandariato, G.; Perger, M.; González Hernández, J. I.; Lanza, A. F.; Maldonado, J.; Micela, G.; Suárez Mascareño, A.; Toledo-Padrón, B.; Affer, L.; Benatti, S.; Bignamini, A.; Bonomo, A. S.; Claudi, R.; Cosentino, R.; Desidera, S.; Maggio, A.; Martinez Fiorenzano, A.; Pagano, I.; Piotto, G.; Rainer, M.; Rebolo, R.; Ribas, I. (2019), «The HADES RV programme with HARPS-N at TNG», Astronomy & Astrophysics, 625: A126, arXiv:1903.11853, doi:10.1051/0004-6361/201834969
↑Affer, L.; Damasso, M.; Micela, G.; Poretti, E.; Scandariato, G.; Maldonado, J.; Lanza, A. F.; Covino, E.; Rubio, A. Garrido (31 de janeiro de 2019). «HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686». Astronomy & Astrophysics. 622: A193. Bibcode:2019A&A...622A.193A. ISSN0004-6361. arXiv:1901.05338. doi:10.1051/0004-6361/201834868
↑Nagel, E.; Czesla, S.; Schmitt, J. H. M. M.; Dreizler, S.; Anglada-Escudé, G.; Rodríguez, E.; Ribas, I.; Reiners, A.; Quirrenbach, A.; Amado, P. J.; Caballero, J. A.; Aceituno, J.; Béjar, V. J. S.; Cortés-Contreras, M.; González-Cuesta, L.; Guenther, E. W.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; López-González, M. J.; Montes, D.; Morales, J. C.; Passegger, V. M.; Rodríguez-López, C.; Schweitzer, A.; Zechmeister, M. (2019), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 622, pp. A153, arXiv:1901.02367, doi:10.1051/0004-6361/201834569
↑Bello-Arufe, Aaron; Cabot, Samuel H. C.; Mendonça, João M.; Buchhave, Lars A.; Rathcke, Alexander D. (2022), «Mining the Ultrahot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species», The Astronomical Journal, 163 (2): 96, Bibcode:2022AJ....163...96B, arXiv:2112.03292, doi:10.3847/1538-3881/ac402e
↑ abcdefghijklmnoFeng, Fabo; Crane, Jeffrey D.; Wang, Sharon Xuesong; Teske, Johanna K.; Shectman, Stephen A.; Díaz, Matías R.; Thompson, Ian B.; Jones, Hugh R. A.; Butler, R. Paul (2019), «Search for Nearby Earth Analogs. I. 15 Planet Candidates Found in PFS Data», The Astrophysical Journal Supplement Series, 242 (2), p. 25, Bibcode:2019ApJS..242...25F, arXiv:1904.08567, doi:10.3847/1538-4365/ab1b16
↑Dorval, P.; Talens, G. J. J.; Otten, G. P. P. L.; Brahm, R.; Jordán, A.; Torres, P.; Vanzi, L.; Zapata, A.; Henry, T.; Paredes, L.; Jao, W. C.; James, H.; Hinojosa, R.; Bakos, G. A.; Csubry, Z.; Bhatti, W.; Suc, V.; Osip, D.; Mamajek, E. E.; Mellon, S. N.; Wyttenbach, A.; Stuik, R.; Kenworthy, M.; Bailey, J.; Ireland, M.; Crawford, S.; Lomberg, B.; Kuhn, R.; Snellen, I. (2020), «MASCARA-4 b/B Ring-1 b: A retrograde hot Jupiter around a bright A-type star», Astronomy & Astrophysics, 635: A60, Bibcode:2020A&A...635A..60D, arXiv:1904.02733, doi:10.1051/0004-6361/201935611
↑Ahlers, John P.; Kruse, Ethan; Colón, Knicole D.; Dorval, Patrick; Talens, Geert Jan; Snellen, Ignas; Albrecht, Simon; Otten, Gilles; Ricker, George; Vanderspek, Roland; Latham, David; Seager, Sara; Winn, Joshua; Jenkins, Jon M.; Haworth, Kari; Cartwright, Scott; Morris, Robert; Rowden, Pam; Tenenbaum, Peter; Ting, Eric B. (2020), «Gravity-darkening Analysis of the Misaligned Hot Jupiter MASCARA-4 B», The Astrophysical Journal, 888 (2): 63, Bibcode:2020ApJ...888...63A, arXiv:1911.05025, doi:10.3847/1538-4357/ab59d0
↑Zhang, Yapeng; Snellen, Ignas A. G.; Wyttenbach, Aurèlien; Nielsen, Louise D.; Lendl, Monika; Casasayas-Barris, Núria; Chaverot, Guillaume; Kesseli, Aurora Y.; Lovis, Christophe; Pepe, Francesco A.; Psaridi, Angelica; Seidel, Julia V.; Udry, Stéphane; Ulmer-Moll, Solène (2022), «Transmission spectroscopy of the ultra-hot Jupiter MASCARA-4 B», Astronomy & Astrophysics, 666: A47, arXiv:2208.11427, doi:10.1051/0004-6361/202244203
↑Rickman, E. L.; et al. (maio de 2019). «The CORALIE survey for southern extrasolar planets. XVIII. Three new massive planets and two low-mass brown dwarfs at greater than 5 AU separation». Astronomy & Astrophysics. 625. 16 páginas. Bibcode:2019A&A...625A..71R. arXiv:1904.01573. doi:10.1051/0004-6361/201935356. A71
↑ abKane, Stephen R.; Dalba, Paul A.; Li, Zhexing; Horch, Elliott P.; Hirsch, Lea A.; Horner, Jonathan; Wittenmyer, Robert A.; Howell, Steve B.; Everett, Mark E.; Butler, R. Paul; Tinney, Christopher G.; Carter, Brad D.; Wright, Duncan J.; Jones, Hugh R. A.; Bailey, Jeremy; o'Toole, Simon J. (2019), «Detection of Planetary and Stellar Companions to Neighboring Stars via a Combination of Radial Velocity and Direct Imaging Techniques», The Astronomical Journal, 157 (6), p. 252, Bibcode:2019AJ....157..252K, arXiv:1904.12931, doi:10.3847/1538-3881/ab1ddf
↑Pinte, C.; Van Der Plas, G.; Ménard, F.; Price, D. J.; Christiaens, V.; Hill, T.; Mentiplay, D.; Ginski, C.; Choquet, E.; Boehler, Y.; Duchêne, G.; Perez, S.; Casassus, S. (2023), «Kinematic detection of a planet carving a gap in a protoplanetary disk», Nature Astronomy, 3 (12), pp. 1109–1114, arXiv:1907.02538, doi:10.1038/s41550-019-0852-6
↑ abTrifonov, Trifon; Stock, Stephan; Henning, Thomas; Reffert, Sabine; Kürster, Martin; Lee, Man Hoi; Bitsch, Bertram; Butler, R. Paul; Vogt, Steven S. (2019), «Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?», The Astronomical Journal, 157 (3): 93, Bibcode:2019AJ....157...93T, arXiv:1901.01935, doi:10.3847/1538-3881/aafa11
↑ abEspinoza, Néstor; et al. (2019), «HD 213885b: A transiting 1-d-period super-Earth with an Earth-like composition around a bright (V = 7.9) star unveiled by TESS», Monthly Notices of the Royal Astronomical Society, 491 (2), pp. 2982–2999, arXiv:1903.07694, doi:10.1093/mnras/stz3150
↑Janson, Markus; Asensio-Torres, Ruben; André, Damien; Bonnefoy, Mickaël; Delorme, Philippe; Reffert, Sabine; Desidera, Silvano; Langlois, Maud; Chauvin, Gaël; Gratton, Raffaele; Bohn, Alexander J.; Eriksson, Simon C.; Marleau, Gabriel-Dominique; Mamajek, Eric E.; Vigan, Arthur; Carson, Joseph C. (2019), «The B-Star Exoplanet Abundance Study: A co-moving 16–25 MJup companion to the young binary system HIP 79098», Astronomy & Astrophysics, 626, pp. A99, Bibcode:2019A&A...626A..99J, arXiv:1906.02787, doi:10.1051/0004-6361/201935687
↑Blunt, Sarah; Endl, Michael; Weiss, Lauren M.; Cochran, William D.; Howard, Andrew W.; MacQueen, Phillip J.; et al. (agosto 2019). «Radial Velocity Discovery of an Eccentric Jovian World Orbiting at 18 au». The Astronomical Journal. 158 (5): 181. Bibcode:2019AJ....158..181B. arXiv:1908.09925. doi:10.3847/1538-3881/ab3e63
↑ abcdHedges, Christina; Saunders, Nicholas; Barentsen, Geert; Coughlin, Jeffrey L.; De Miranda Cardoso, Josè Vinícius; Kostov, Veselin B.; Dotson, Jessie; Cody, Ann Marie (2019), «Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?», The Astrophysical Journal, 880 (1), pp. L5, Bibcode:2019ApJ...880L...5H, arXiv:1907.08244, doi:10.3847/2041-8213/ab2a74
↑Wells, R.; Poppenhaeger, K.; Watson, C. A. (2019), «Validation of a temperate fourth planet in the K2-133 multiplanet system», Monthly Notices of the Royal Astronomical Society, 487 (2): 1865–1873, arXiv:1905.05206, doi:10.1093/mnras/stz1334
↑Hamann, Aaron; Montet, Benjamin T.; Fabrycky, Daniel C.; Agol, Eric; Kruse, Ethan (2019), «K2-146: Discovery of Planet c, Precise Masses from Transit Timing, and Observed Precession», The Astronomical Journal, 158 (3), p. 133, Bibcode:2019AJ....158..133H, arXiv:1907.10620, doi:10.3847/1538-3881/ab32e3
↑ abcAdams, Elisabeth R.; Jackson, Brian; Johnson, Samantha; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Furlan, Elise; Howell, Steve B.; Jayanthi, Prasanna; MacQueen, Phillip J.; Matson, Rachel A.; Partyka-Worley, Ciera; Schlieder, Joshua; Scott, Nicholas J.; Stanton, Sevio M.; Ziegler, Carl (2020), Ultra Short Period Planets in K2 III: Neighbors Are Common With 12 New Multi-Planet Systems and 26 Newly Validated Planets in Campaigns 0-8, 10, arXiv:2011.11698
↑Alonso, E Díez; Hernández, J I González; Toledo–Padrón, B.; Gómez, S L Suárez; Mascareño, A Suárez; Aguado, D. S.; Gutiérrez, C González; Cabrera-Lavers, A.; Carballido–Landeira, J.; Bonavera, L.; Juez, F J de Cos; Rebolo, R. (2019), «A transiting super-Earth close to the inner edge of the habitable zone of an M0 dwarf star», Monthly Notices of the Royal Astronomical Society, arXiv:1901.04739, doi:10.1093/mnras/sty3467
↑ abHjorth, M.; Justesen, A. B.; Hirano, T.; Albrecht, S.; Gandolfi, D.; Dai, F.; Alonso, R.; Barragán, O.; Esposito, M.; Kuzuhara, M.; Lam, K. W. F.; Livingston, J. H.; Montanes-Rodriguez, P.; Narita, N.; Nowak, G.; Prieto-Arranz, J.; Redfield, S.; Rodler, F.; Van Eylen, V.; Winn, J. N.; Antoniciello, G.; Cabrera, J.; Cochran, W. D.; Csizmadia, Sz; De Leon, J.; Deeg, H.; Eigmüller, Ph; Endl, M.; Erikson, A.; et al. (2019), «K2-290: a warm Jupiter and a mini-Neptune in a triple-star system», Monthly Notices of the Royal Astronomical Society, 484 (3): 3522, Bibcode:2019MNRAS.484.3522H, arXiv:1901.03716, doi:10.1093/mnras/stz139
↑ abHjorth, Maria; Albrecht, Simon; Hirano, Teruyuki; Winn, Joshua N.; Dawson, Rebekah I.; Zanazzi, J. J.; Knudstrup, Emil; Sato, Bun'ei (2021), «A backward-spinning star with two coplanar planets», Proceedings of the National Academy of Sciences of the United States of America, 118 (8): e2017418118, Bibcode:2021PNAS..11817418H, PMC7923373, PMID33593909, arXiv:2102.07677, doi:10.1073/pnas.2017418118
↑ abDattilo, Anne; Vanderburg, Andrew; Shallue, Christopher J.; Mayo, Andrew W.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A.; Everett, Mark E.; Howell, Steve B.; Latham, David W.; Scott, Nicholas J.; Yu, Liang (2019), «Identifying Exoplanets with Deep Learning. II. Two New Super-Earths Uncovered by a Neural Network in K2 Data», The Astronomical Journal, 157 (5), p. 169, Bibcode:2019AJ....157..169D, arXiv:1903.10507, doi:10.3847/1538-3881/ab0e12
↑De Leon, J. P.; Livingston, J.; Endl, M.; Cochran, W. D.; Hirano, T.; García, R. A.; Mathur, S.; Lam, K W F.; Korth, J.; Trani, A. A.; Dai, F.; Díez Alonso, E.; Castro-González, A.; Fridlund, M.; Fukui, A.; Gandolfi, D.; Kabath, P.; Kuzuhara, M.; Luque, R.; Savel, A. B.; Gill, H.; Dressing, C.; Giacalone, S.; Narita, N.; Palle, E.; Van Eylen, V.; Tamura, M. (2021), «37 new validated planets in overlapping K2 campaigns», Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305
↑Rampalli, Rayna; Vanderburg, Andrew; Bieryla, Allyson; Latham, David W.; Quinn, Samuel N.; Baranec, Christoph; Berlind, Perry; Calkins, Michael L.; Cochran, William D.; Duev, Dmitry A.; Endl, Michael; Esquerdo, Gilbert A.; Jensen-Clem, Rebecca; Law, Nicholas M.; Mayo, Andrew W.; Riddle, Reed; Salama, Maïssa (2019), «A Hot Saturn Near (But Unassociated with) the Open Cluster NGC 1817», The Astronomical Journal, 158 (2), p. 62, Bibcode:2019AJ....158...62R, arXiv:1906.02395, doi:10.3847/1538-3881/ab27c2
↑Vines, Jose I.; et al. (2019), «NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf», Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv:1904.07997, doi:10.1093/mnras/stz2349
↑ abCostes, Jean C.; et al. (2019), «NGTS-8b and NGTS-9b: Two non-inflated hot-Jupiters», Monthly Notices of the Royal Astronomical Society, arXiv:1911.02814, doi:10.1093/mnras/stz3140
↑Zhu, Li-Ying; Qian, Sheng-Bang; Fernández Lajús, Eduardo; Wang, Zhi-Hua; Li, Lin-Jia; -J, Li L. (2019). «A close-in substellar object orbiting the sdOB-type eclipsing-binary system NSVS 14256825». Research in Astronomy and Astrophysics. 19 (9): 134. Bibcode:2019RAA....19..134Z. arXiv:1904.11664. doi:10.1088/1674-4527/19/9/134
↑Song, Shuo; Mai, Xinyu; Mutel, Robert L.; Pulley, David; Faillace, George; Watkins, Americo (2019). «An Updated Model for Circumbinary Planets Orbiting the SDB Binary NY Virginis». The Astronomical Journal. 157 (5): 184. Bibcode:2019AJ....157..184S. doi:10.3847/1538-3881/ab1139
↑ abcNielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020), «Mass determinations of the three mini-Neptunes transiting TOI-125», Monthly Notices of the Royal Astronomical Society, 492 (4): 5399, Bibcode:2020MNRAS.492.5399N, arXiv:2001.08834, doi:10.1093/mnras/staa197
↑ abKossakowski, Diana; et al. (2019), «TOI-150b and TOI-163b: Two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ», Monthly Notices of the Royal Astronomical Society, 490, pp. 1094–1110, arXiv:1906.09866, doi:10.1093/mnras/stz2433
↑Rodriguez, Joseph E.; et al. (2019), «An Eccentric Massive Jupiter Orbiting a Subgiant on a 9.5-day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images», The Astronomical Journal, 157 (5), p. 191, Bibcode:2019AJ....157..191R, arXiv:1901.09950, doi:10.3847/1538-3881/ab11d9
↑ abTeachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). «A resonant pair of warm giant planets revealed by TESS». Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv:1902.03900. doi:10.1093/mnras/stz1141
↑ abcVan Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), «Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley», Monthly Notices of the Royal Astronomical Society, arXiv:2101.01593, doi:10.1093/mnras/stab2143
↑Mikal-Evans, Thomas; Madhusudhan, Nikku; Dittmann, Jason; Guenther, Maximilian N.; Welbanks, Luis; Vincent Van Eylen; Crossfield, Ian J. M.; Daylan, Tansu; Kreidberg, Laura (2023), «Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor», The Astronomical Journal, 165 (3), p. 84, Bibcode:2023AJ....165...84M, arXiv:2211.15576, doi:10.3847/1538-3881/aca90b
↑David, Trevor J.; Cody, Ann Marie; Hedges, Christina L.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Ciardi, David R.; Beichman, Charles A.; Petigura, Erik A.; Fulton, Benjamin J.; Isaacson, Howard T.; Howard, Andrew W.; Gagné, Jonathan; Saunders, Nicholas K.; Rebull, Luisa M.; Stauffer, John R.; Vasisht, Gautam; Hinkley, Sasha (2019), «A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau», The Astronomical Journal, 158 (2): 79, Bibcode:2019AJ....158...79D, arXiv:1902.09670, doi:10.3847/1538-3881/ab290f
↑ abcDavid, Trevor J.; Petigura, Erik A.; Luger, Rodrigo; Foreman-Mackey, Daniel; Livingston, John H.; Mamajek, Eric E.; Hillenbrand, Lynne A. (2019), «Four newborn planets transiting the young solar analog V1298 Tau», The Astrophysical Journal, 885 (1): L12, Bibcode:2019ApJ...885L..12D, arXiv:1910.04563, doi:10.3847/2041-8213/ab4c99
↑Maciejewski, G. (2020), «Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. I. No Companions in Planetary Systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126», Acta Astronomica, 70 (3), p. 181, Bibcode:2020AcA....70..181M, arXiv:2010.11977, doi:10.32023/0001-5237/70.3.2
↑ abcdNielsen, L. D.; Bouchy, F.; Turner, O. D.; Anderson, D. R.; Barkaoui, K.; Benkhaldoun, Z.; Burdanov, A.; Cameron, A Collier; Delrez, L.; Gillon, M.; Ducrot, E.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P F L.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A H M J.; Udry, S.; West, R. G. (2019), «WASP-169, WASP-171, WASP-175, and WASP-182: Three hot Jupiters and one bloated sub-Saturn mass planet discovered by WASP-South», Monthly Notices of the Royal Astronomical Society, 489 (2), pp. 2478–2487, arXiv:1904.10388, doi:10.1093/mnras/stz2351
↑ abcTurner, Oliver D.; Anderson, D. R.; Barkaoui, K.; Bouchy, F.; Benkhaldoun, Z.; Brown, D J A.; Burdanov, A.; Collier Cameron, A.; Ducrot, E.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P F L.; Nielsen, L. D.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A H M J.; Udry, S.; West, R. G. (2019), «Three hot-Jupiters on the upper edge of the mass–radius distribution: WASP-177, WASP-181, and WASP-183», Monthly Notices of the Royal Astronomical Society, 485 (4), pp. 5790–5799, arXiv:1903.06622, doi:10.1093/mnras/stz742
↑ abcdHellier, Coel; Anderson, D. R.; Barkaoui, K.; Benkhaldoun, Z.; Bouchy, F.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Nielsen, L. D.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2019), «WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b», Monthly Notices of the Royal Astronomical Society, 490 (1): 1479, Bibcode:2019MNRAS.490.1479H, arXiv:1907.11667, doi:10.1093/mnras/stz2713
↑Temple, L. Y.; Hellier, C.; Anderson, D. R.; Barkaoui, K.; Bouchy, F.; Brown, D J A.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Ducrot, E.; Evans, D.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P F L.; McCormac, J.; Murray, C.; Nielsen, L. D.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Thompson, S.; Triaud, A H M J.; Turner, O. D.; Udry, S.; West, R. G.; Zouhair, B. (2019), «WASP-180Ab: Doppler tomography of a hot Jupiter orbiting the primary star in a visual binary», Monthly Notices of the Royal Astronomical Society, 490 (2), pp. 2467–2474, arXiv:1903.08002, doi:10.1093/mnras/stz2632
↑ abFeng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R. (2020), «Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs», The Astrophysical Journal Supplement Series, 250 (2): 29, Bibcode:2020ApJS..250...29F, arXiv:2008.07998, doi:10.3847/1538-4365/abb139
↑ abQuirrenbach, A.; Passegger, V. M.; Trifonov, T.; Amado, P. J.; Caballero, J. A.; Reiners, A.; Ribas, I.; Aceituno, J.; Béjar, V. J. S.; Chaturvedi, P.; González-Cuesta, L.; Henning, T.; Herrero, E.; Kaminski, A.; Kürster, M.; Lalitha, S.; Lodieu, N.; López-González, M. J.; Montes, D.; Pallé, E.; Perger, M.; Pollacco, D.; Reffert, S.; Rodríguez, E.; López, C. Rodríguez; Shan, Y.; Tal-Or, L.; Osorio, M. R. Zapatero; Zechmeister, M. (2022), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 663: A48, arXiv:2203.16504, doi:10.1051/0004-6361/202142915