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| KOI-7733 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST06:57:10 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2016ApJ...829...23D 
|
16 | D | 1 | 4045 | 212 | The Kepler catalog of stellar flares. | DAVENPORT J.R.A. | ||
|
2018A&A...614A..46B
|
16 | D | 1 | 1063 | 5 | The envelope of the power spectra of over a thousand δ Scuti stars. The Teff - νmax scaling relation. | BARCELO FORTEZA S., ROCA CORTES T. and GARCIA R.A. | ||
|
2018MNRAS.479..183B
|
16 | D | 1 | 2598 | 17 | Gaia luminosities of pulsating A-F stars in the Kepler field. | BALONA L.A. | ||
|
2019MNRAS.485.2380M
|
16 | 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
|
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. | ||
|
2020A&A...638A..59B
|
16 | D | 1 | 2220 | 17 | Unveiling the power spectra of δ Scuti stars with TESS. The temperature, gravity, and frequency scaling relation. | BARCELO FORTEZA S., MOYA A., BARRADO D., et al. | ||
|
2020AJ....160..108B
|
16 | 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. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
| 2021AJ....162..204H | 17 | D | 2 | 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. |
