K2-281 , the SIMBAD biblio

K2-281 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST23:56:57

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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
2018AJ....155...21P viz 16       D               2 354 28 Planet candidates from K2 campaigns 5-8 and follow-up optical spectroscopy. PETIGURA E.A., CROSSFIELD I.J.M., ISAACSON H., et al.
2018AJ....156..277L viz 16       D               1 306 50 Sixty validated planets from K2 campaigns 5-8. LIVINGSTON J.H., CROSSFIELD I.J.M., PETIGURA E.A., 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               3 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.
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.
2024AJ....167...48M 332       D     X C       7 72 ~ Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars. MORGAN M., BOWLER B.P., TRAN Q.H., et al.
2024ApJ...970...53L 18       D               4 242 ~ 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.
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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