K2-49 , the SIMBAD biblio

K2-49 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:26:46


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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..226....7C viz 16       D               2 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017ApJ...837...72M 56 18 Stellar and planetary parameters for K2's late-type dwarf systems from C1 to C5. MARTINEZ A.O., CROSSFIELD I.J.M., SCHLIEDER J.E., et al.
2017MNRAS.465.2634A viz 16       D               4 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
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               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 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.
2022ApJS..261...26S viz 17       D               4 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.
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.

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