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| K2-5 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:46:47 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2015ApJ...806..215F | 16 | D | 2 | 67 | 104 | A systematic search for transiting planets in the K2 data. | FOREMAN-MACKEY D., MONTET B.T., HOGG D.W., et al. | ||
|
2015A&A...579A..19A |
16 | D | 1 | 8375 | 75 | 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. | ||
|
2015ApJ...809...25M |
17 | D | 1 | 35 | 123 | Stellar and planetary properties of K2 campaign 1 candidates and validation of 17 planets, including a planet receiving earth-like insolation. | MONTET B.T., MORTON T.D., FOREMAN-MACKEY D., et al. | ||
|
2016ApJS..222...14V |
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. | ||
| 2016AJ....151..159S | 16 | D | 2 | 76 | 11 | Planet Hunters. X searching for nearby neighbors of 75 planet and eclipsing binary candidates from the K2 Kepler extended mission. | SCHMITT J.R., TOKOVININ A., WANG J., et al. | ||
| 2016ApJ...827...78S | 960 | D | X C | 24 | 49 | 94 | Eleven multiplanet systems from K2 campaigns 1 and 2 and the masses of two hot super-earths. | SINUKOFF E., HOWARD A.W., PETIGURA E.A., et al. | |
|
2016ApJS..226....7C |
16 | D | 5 | 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. | ||
|
2017MNRAS.465.2634A |
16 | D | 8 | 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. | ||
|
2017A&A...603A..30S |
16 | D | 4 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
| 2018AJ....155..127H | 17 | D | 1 | 53 | 70 | Exoplanets around low-mass stars unveiled by K2. | HIRANO T., DAI F., GANDOLFI D., et al. | ||
|
2019AJ....157..124K |
16 | D | 2 | 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 | 2 | 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. | ||
|
2021AJ....162..259Z |
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. | ||
| 2023MNRAS.520.5283G | 87 | X | 2 | 91 | 6 | The TIME Table: rotation and ages of cool exoplanet host stars. | GAIDOS E., CLAYTOR Z., DUNGEE R., et al. | ||
|
2023AJ....165..168O |
17 | D | 1 | 281 | 1 | The Demographics of Terrestrial Planets in the Venus Zone. | OSTBERG C., KANE S.R., LI Z., et al. | ||
|
2023AJ....165..262Z |
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. | ||
|
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. | ||
|
2025ApJ...993..233W |
19 | D | 2 | 391 | ~ | An Analysis of the Radius Gap in a Sample of Kepler, K2, and TESS Exoplanets Orbiting M-dwarf Stars. | WANDERLEY F., CUNHA K., SMITH V.V., 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. |