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| K2-186 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST11:08:32 |
| 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..136M |
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 |
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. | ||
|
2019ApJS..244...11K |
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 |
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. | ||
|
2022ApJS..261...26S |
17 | D | 8 | 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. | ||
|
2023ApJ...946...61L |
61 | D | X | 2 | 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. | |
|
2024A&A...691A..53S |
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...699A.100D |
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. |