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| KOI-5809 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:50:08 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013ApJ...770...43M |
15 | D | 2 | 202 | 41 | Testing the metal of late-type Kepler planet hosts with iron-clad methods. | MANN A.W., GAIDOS E., KRAUS A., et al. | ||
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
2014ApJS..211...24M |
15 | D | 1 | 34022 | 573 | Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
|
2015ApJ...801....3M |
16 | D | 1 | 3357 | 109 | Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. | MAZEH T., PERETS H.B., McQUILLAN A., et al. | ||
|
2015ApJ...807..170H |
16 | D | 1 | 2117 | 10 | Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. | HOLCZER T., SHPORER A., MAZEH T., et al. | ||
|
2016ApJS..225....9H |
16 | D | 2 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
|
2017MNRAS.465.2634A |
16 | D | 1 | 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. | ||
|
2020MNRAS.499.3481A |
16 | D | 1 | 28505 | 24 | Evidence for metallicity-dependent spin evolution in the Kepler field. | AMARD L., ROQUETTE J. and MATT S.P. | ||
|
2020AJ....160..253L |
16 | D | 1 | 3432 | 12 | An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. | LU C.X., SCHLAUFMAN K.C. and CHENG S. | ||
|
2021AJ....161..189L |
17 | D | 1 | 29956 | 19 | Gyro-kinematic ages for around 30,000 Kepler stars. | LU Y., ANGUS R., CURTIS J.L., et al. |