K2-53 , the SIMBAD biblio

K2-53 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:48:20

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
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.
2016ApJS..225...32B viz 16       D               1 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 16       D               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.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.
2017ApJ...836..167D viz 16       D               1 144 30 Characterizing K2 candidate planetary systems orbiting low-mass stars. I. Classifying low-mass host stars observed during Campaigns 1-7. DRESSING C.D., NEWTON E.R., SCHLIEDER J.E., et al.
2019AJ....157..102L 219       D     X         6 17 4 Spitzer transit follow-up of planet candidates from the K2 mission. LIVINGSTON J.H., CROSSFIELD I.J.M., WERNER M.W., et al.
2019AJ....157..124K viz 16       D               1 603 7 Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019AJ....158...87D viz 16       D               3 179 ~ Characterizing K2 candidate planetary systems orbiting low-mass stars. IV. Updated properties for 86 cool dwarfs observed during Campaigns 1-17. DRESSING C.D., HARDEGREE-ULLMAN K., SCHLIEDER J.E., 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               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.
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.
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.
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.
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.
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.
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.
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.

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