K2-26 , the SIMBAD biblio

K2-26 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.04.01CEST18:34:20


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Title First 3 Authors
2015A&A...579A..19A viz 16       D               1 8374 42 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 81 Planetary candidates from the first year of the K2 mission. VANDERBURG A., LATHAM D.W., BUCHHAVE L.A., et al.
2016ApJ...818...87S 4103   K A D     X C       101 15 21 Two small temperate planets transiting nearby M dwarfs in K2 campaigns 0 and 1. SCHLIEDER J.E., CROSSFIELD I.J.M., PETIGURA E.A., et al.
2016ApJ...822...39B 326     A D     X C       8 9 15 Spitzer observations of exoplanets discovered with the Kepler K2 mission. BEICHMAN C., LIVINGSTON J., WERNER M., et al.
2016ApJS..226....7C viz 260       D     X         7 400 70 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017A&A...603A..30S viz 16       D               2 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018AJ....155..127H 17       D               1 53 17 Exoplanets around low-mass stars unveiled by K2. HIRANO T., DAI F., GANDOLFI D., et al.
2019AJ....158...87D viz 17       D               9 179 ~ 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 17       D               1 2118 ~ Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. KRUSE E., AGOL E., LUGER R., et al.
2019ApJ...887..261M viz 17       D               3 329 ~ Exomoons in the habitable zones of M dwarfs. MARTINEZ-RODRIGUEZ H., CABALLERO J.A., CIFUENTES C., et al.
2020ApJ...890...23L viz 17       D               1 4935 ~ 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 18       D               1 2175 ~ 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.

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2023.04.01-18:34:20

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