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| 2MASS J19512969+4514433 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:14:16 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013A&A...557L..10N |
15 | D | 1 | 12151 | 189 | Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. | NIELSEN M.B., GIZON L., SCHUNKER H., et al. | ||
|
2014ApJS..211...24M |
15 | D | 1 | 34022 | 573 | Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
| 2014AJ....148..125P | 15 | D | 1 | 75 | 3 | The EB Factory project. II. Validation with the Kepler field in preparation for K2 and TESS. | PARVIZI M., PAEGERT M. and STASSUN K.G. | ||
|
2016AJ....151...68K |
16 | D | 1 | 2915 | 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. | ||
|
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. | ||
|
2016AJ....152..158T |
16 | D | 1 | 4388 | 37 | Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). | TWICKEN J.D., JENKINS J.M., SEADER S.E., et al. | ||
|
2017AJ....154..250L |
16 | D | 1 | 2281 | 72 | Tidal synchronization and differential rotation of Kepler eclipsing binaries. | LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al. | ||
|
2019ApJS..244...43Z |
16 | D | 1 | 1328 | 22 | Unbiased distribution of binary parameters from LAMOST and Kepler observations. | ZHANG J., QIAN S.-B., WU Y., et al. | ||
|
2024A&A...685A..62I |
18 | D | 1 | 2906 | ~ | Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. | IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al. |