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KOI-8007 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST17:01:19 |
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 |
---|---|---|---|---|---|---|---|---|---|
2014ApJ...788..114R | 252 | D | X C | 6 | 184 | 17 | M-dwarf rapid rotators and the detection of relatively young multiple M-star systems. | RAPPAPORT S., SWIFT J., LEVINE A., et al. | |
2015ApJ...815..127W | 16 | D | 2 | 59 | 64 | Planet hunters. VIII. Characterization of 41 long-period exoplanet candidates from Kepler archival data. | WANG J., FISCHER D.A., BARCLAY T., et al. | ||
2016AJ....151...68K | 16 | D | 1 | 2914 | 316 | Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. | KIRK B., CONROY K., PRSA A., et al. | ||
2016MNRAS.457.2877G | 16 | D | 1 | 4245 | 141 | They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. | GAIDOS E., MANN A.W., KRAUS A.L., et al. | ||
2017AJ....153..193A | 1503 | S X C | 35 | 36 | 22 | Toward detection of exoplanetary rings via transit photometry: methodology and a possible candidate. | AIZAWA M., UEHARA S., MASUDA K., et al. | ||
2018AJ....156...50G | 16 | D | 1 | 54 | ~ | The best planets to harbor detectable exomoons. | GUIMARAES A. and VALIO A. | ||
2018ApJ...866...99B | 16 | D | 1 | 7129 | 233 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
2019MNRAS.485.2681R | 42 | X | 1 | 23 | 5 | Deep long asymmetric occultation in EPIC 204376071. | RAPPAPORT S., ZHOU G., VANDERBURG A., et al. | ||
2019ApJS..241...29Y | 17 | D | 1 | 3421 | 70 | The flare catalog and the flare activity in the Kepler mission. | YANG H. and LIU J. | ||
2019AJ....157..218K | 17 | D | 2 | 142 | 26 | Transiting planets near the snow line from Kepler. I. Catalog. | KAWAHARA H. and MASUDA K. | ||
2019MNRAS.490.1111R | 84 | X | 2 | 3 | ~ | Fast and precise light-curve model for transiting exoplanets with rings. | REIN E. and OFIR A. | ||
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. | ||
2020MNRAS.497.1870S | 43 | X | 1 | 8 | ~ | The structure and stability of extended, inclined circumplanetary disc or ring systems. | SPEEDIE J. and ZANAZZI J.J. | ||
2022AJ....164..215B | 45 | X | 1 | 63 | 11 | Kepler and the Behemoth: Three Mini-Neptunes in a 40 Million Year Old Association. | BOUMA L.G., KERR R., CURTIS J.L., et al. |