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| KOI-3722 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST22:53:39 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2011A&A...529A..89D 
|
15 | D | 1 | 3298 | 98 | Global stellar variability study in the field-of-view of the Kepler satellite. | DEBOSSCHER J., BLOMME J., AERTS C., et al. | ||
|
2014MNRAS.437.3473A
|
16 | D | 1 | 2614 | 45 | A catalogue of temperatures for Kepler eclipsing binary stars. | ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al. | ||
|
2014AJ....147..119C
|
16 | D | 2 | 8010 | 91 | Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. | COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al. | ||
|
2015ApJS..217...16R
|
16 | D | 1 | 8625 | 149 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
|
2016AJ....151...68K
|
16 | D | 2 | 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. | ||
|
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. | ||
|
2016ApJ...829...23D
|
16 | D | 1 | 4044 | 212 | The Kepler catalog of stellar flares. | DAVENPORT J.R.A. | ||
|
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. | ||
|
2017AJ....154..250L
|
16 | D | 1 | 2280 | 72 | Tidal synchronization and differential rotation of Kepler eclipsing binaries. | LURIE J.C., VYHMEISTER K., HAWLEY S.L., 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. |
