K2-30 , the SIMBAD biblio

K2-30 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:15:06


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Title First 3 Authors
2016AJ....151..171J 787           X C       19 12 16 Two hot jupiters from K2 campaign 4. JOHNSON M.C., GANDOLFI D., FRIDLUND M., et al.
2016ApJS..226....7C viz 173       D     X         5 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2016A&A...594A..50L viz 1000       D     X C       25 8 17 K2-30 b and K2-34 b: Two inflated hot Jupiters around solar-type stars. LILLO-BOX J., DEMANGEON O., SANTERNE A., et al.
2016A&A...594A.100B viz 16       D               2 532 86 New planetary and eclipsing binary candidates from campaigns 1-6 of the K2 mission. BARROS S.C.C., DEMANGEON O. and DELEUIL M.
2016PASP..128l4402B 882       D     X C       22 4 10 An independent discovery of two hot Jupiters from the (K2) mission. BRAHM R., JONES M., ESPINOZA N., et al.
2017A&A...603A..30S viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJ...853...37S 16       D               2 153 90 Evidence of an upper bound on the masses of planets and its implications for giant planet formation. SCHLAUFMAN K.C.
2018AJ....155..136M viz 16       D               1 521 127 275 candidates and 149 validated planets orbiting bright stars in K2 campaigns 0-10. MAYO A.W., VANDERBURG A., LATHAM D.W., et al.
2018ApJ...856..155G viz 96       D       C       7 149 5 Giant planets: good neighbors for habitable worlds? GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I.
2019AJ....157..124K viz 97       D       C       4 603 7 Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019ApJS..244...11K viz 16       D               1 2119 48 Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. KRUSE E., AGOL E., LUGER R., et al.
2019AJ....158..190H viz 16       D               1 343 61 Hot Jupiters are destroyed by tides while their host stars are on the main sequence. HAMER J.H. and SCHLAUFMAN K.C.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020AJ....159..194V viz 16       D               1 288 ~ A statistical search for star-planet interaction in the ultraviolet using GALEX. VISWANATH G., NARANG M., MANOJ P., et al.
2021A&A...645A...7K viz 17       D               1 1569 17 Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al.
2021ApJ...909..115C viz 17       D               1 2176 13 Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. CHEN D.-C., XIE J.-W., ZHOU J.-L., et al.
2021ApJ...914...56A 125           X         3 55 13 On a possible solution to the tidal realignment problem for hot Jupiters. ANDERSON K.R., WINN J.N. and PENEV K.
2021ApJ...919..138T viz 17       D               1 531 12 Further evidence for tidal spin-up of hot Jupiter host stars. TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R.
2021AJ....162..259Z viz 17       D               1 1094 12 Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022A&A...663A.161M viz 17       D               1 213 8 Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. MAGRINI L., DANIELSKI C., BOSSINI D., et al.
2023ApJ...946...61L viz 17       D               1 257 ~ A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2023AJ....165..262Z viz 17       D               1 314 ~ Scaling K2. VI. Reduced Small-planet Occurrence in High-galactic-amplitude Stars. ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al.
2023A&A...676A..90R viz 17       D               1 273 ~ The GAPS programme at TNG XLIV. Projected rotational velocities of 273 exoplanet-host stars observed with HARPS-N. RAINER M., DESIDERA S., BORSA F., et al.
2024A&A...688A.193D viz 18       D               1 182 ~ Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars. DA SILVA R., DANIELSKI C., DELGADO MENA E., et al.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2025RNAAS...9..275M 19       D               1 365 ~ An In-depth Study of Brown Dwarfs with TESS. MARCADON F. and PRSA A.
2025ApJS..281...61L 19       D               4 643 ~ Stellar Characterization, Magnesium Abundances, and Chromospheric Activity Analysis of Stars with Confirmed Exoplanets from the K2 Mission. LOAIZA-TACURI V., SOUTO D., QUISPE-HUAYNASI F., et al.
2026AJ....171..157S 20       D               2 480 ~ Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. SCHMIDT S.P. and SCHLAUFMAN K.C.

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