K2-36 , the SIMBAD biblio

K2-36 , the SIMBAD biblio (42 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:46:39


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Title First 3 Authors
2004MNRAS.355..585G viz 1938 6 New Northern hemisphere common proper-motion pairs. GREAVES J.
2015A&A...579A..19A viz 16       D               1 8375 75 K2 Variable Catalogue: Variable stars and eclipsing binaries in K2 campaigns 1 and 0. ARMSTRONG D.J., KIRK J., LAM K.W.F., et al.
2016ApJS..222...14V viz 16       D               1 209 177 Planetary candidates from the first year of the K2 mission. VANDERBURG A., LATHAM D.W., BUCHHAVE L.A., et al.
2016ApJ...827...78S 606       D     X C       15 49 94 Eleven multiplanet systems from K2 campaigns 1 and 2 and the masses of two hot super-earths. SINUKOFF E., HOWARD A.W., PETIGURA E.A., et al.
2016ApJS..225...32B viz 16       D               2 1473 266 Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. BREWER J.M., FISCHER D.A., VALENTI J.A., et al.
2016ApJS..226....7C viz 291       D     X         8 400 165 197 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.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.
2017MNRAS.465.2634A viz 16       D               8 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2017A&A...603A..30S viz 16       D               4 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
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.
2019AJ....157..124K viz 16       D               2 603 7 Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019A&A...624A..38D viz 2502 T   A S   X C       59 21 2 So close, so different: characterization of the
K2-36 planetary system with HARPS-N.
DAMASSO M., ZENG L., MALAVOLTA L., 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.
2020ApJ...890...23L viz 16       D               2 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.
2020MNRAS.497.4091M 41           X         1 57 ~ Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution. MALDONADO R.F., VILLAVER E., MUSTILL A.J., et al.
2020A&A...642A.173N 83           X         2 35 53 The CARMENES search for exoplanets around M dwarfs. Two planets on opposite sides of the radius gap transiting the nearby M dwarf LTT 3780. NOWAK G., LUQUE R., PARVIAINEN H., et al.
2021ApJ...910L..19C 84               F     1 61 ~ When the peas jump around the pod: how stellar clustering affects the observed correlations between planet properties in multiplanet systems. CHEVANCE M., KRUIJSSEN J.M.D. and LONGMORE S.N.
2021AJ....162...62D 17       D               1 37 15 TKS X: confirmation of TOI-1444b and a comparative analysis of the ultra-short-period planets with hot Neptunes. DAI F., HOWARD A.W., BATALHA N.M., et al.
2021AJ....162..136D 142       D     X         4 10 ~ K2, Spitzer, and TESS transits of four sub-Neptune exoplanets. DUCK A., HARADA C.K., HARRELL J., et al.
2021ApJ...921...24S viz 17       D               4 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2022A&A...658A.107O 102       D         F     2 48 4 The similarity of multi-planet systems. OTEGI J.F., HELLED R. and BOUCHY F.
2022AJ....164...60S viz 17       D               2 854 2 Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? SWASTIK C., BANYAL R.K., NARANG M., et al.
2022ApJS..261...26S viz 17       D               2 1893 2 Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. SU T., ZHANG L.-Y., LONG L., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2023MNRAS.518.2068G viz 17       D               1 179 2 Chaos in multiplanetary extrasolar systems. GAJDOS P. and VANKO M.
2023ApJ...946...61L viz 148       D     X         4 257 ~ 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.
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...674A.137L 17       D               1 122 ~ Quantitative correlation of refractory elemental abundances between rocky exoplanets and their host stars. LIU Z. and NI D.
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.
2023A&A...676A.131H 87               F     2 48 ~ Forming rocky exoplanets around K-dwarf stars. HATALOVA P., BRASSER R., MAMONOVA E., et al.
2023A&A...677A..33B viz 148       D     X         4 120 ~ Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities No excess of cold Jupiters in small planet systems. BONOMO A.S., DUMUSQUE X., MASSA A., et al.
2023A&A...679A..33D 44           X         1 19 ~ A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO Radial velocities lead to the detection of transits with low signal-to-noise ratio. DAMASSO M., RODRIGUES J., CASTRO-GONZALEZ A., et al.
2024ApJ...968L..25B 18       D               1 225 ~ Friends Not Foes: Strong Correlation between Inner Super-Earths and Outer Gas Giants. BRYAN M.L. and LEE E.J.
2024ApJ...970...53L 18       D               3 242 ~ Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-hosting Stars. LOAIZA-TACURI V., CUNHA K., SMITH V.V., 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.
2024AJ....168..281B 18       D               1 40 ~ Revisiting the Relationship Between Rocky Exoplanet and Stellar Compositions: Reduced Evidence for a Super-Mercury Population. BRINKMAN C.L., POLANSKI A.S., HUBER D., et al.
2025A&A...697A.102T viz 19       D               1 176 ~ Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. TSANTAKI M., MAGRINI L., DANIELSKI C., et al.
2025ApJS..278...52H 578       D S   X C       11 136 ~ Planet Masses, Radii, and Orbits from NASA's K2 Mission. HOWARD A.W., SINUKOFF E., BLUNT S., 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.
2025ApJ...990..113M 19       D               1 274 ~ OWLS. I. The Olin Wilson Legacy Survey. MORRIS B.M., HEBB L., HAWLEY S.L., et al.
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.
2025A&A...704A.108C 19       D               1 111 ~ Refractory element abundances in rocky planets and their host stars: Revisiting the compositional link. CHEN X. and NI D.

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