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| KOI-6142 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST19:13:54 |
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More on score
| 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...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. | ||
|
2015ApJS..217...31M
|
16 | D | 1 | 2033 | 213 | Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
|
2016A&A...594A..39F
|
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2017MNRAS.465.2634A
|
16 | D | 3 | 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. | ||
|
2019MNRAS.485.2380M
|
17 | D | 1 | 14330 | 108 | Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. | MURPHY S.J., HEY D., VAN REETH T., et al. | ||
|
2020ApJ...890...23L
|
17 | D | 3 | 4935 | 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. | ||
|
2020AJ....160..108B
|
17 | D | 1 | 6855 | 109 | The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
| 2021AJ....162..204H | 131 | X | 3 | 46 | 5 | A search for transits among the delta Scuti variables in Kepler. | HEY D.R., MONTET B.T., POPE B.J.S., et al. |
