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K2-26 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.04.01CEST18:34:20 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015A&A...579A..19A ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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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