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KOI-7607 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET16:02:03 |
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...822...86M | 16 | D | 1 | 6130 | 337 | False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. | MORTON T.D., BRYSON S.T., COUGHLIN J.L., 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. | ||
2018AJ....155..161Z | 16 | D | 1 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., et al. | ||
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. | ||
2018A&A...615A..49C | 16 | D | 1 | 224764 | 54 | Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. | CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al. | ||
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 | 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 | 1 | 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. | ||
2020A&A...638A..59B | 17 | 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. |