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| TYC 3141-392-1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:14:17 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
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. | ||
|
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. | ||
|
2019ApJS..241...29Y
|
16 | D | 1 | 3420 | 70 | The flare catalog and the flare activity in the Kepler mission. | YANG H. and LIU J. | ||
|
2020ApJS..247....9Z
|
16 | D | 1 | 5575 | 26 | Magnetic activity of F-, G-, and K-type stars in the LAMOST-Kepler field. | ZHANG J., BI S., LI Y., et al. | ||
|
2021ApJ...906...40G
|
17 | D | 1 | 352 | ~ | Flare activity and magnetic feature analysis of the flare stars. II. Subgiant branch. | GOODARZI H., MEHRABI A., KHOSROSHAHI H.G., et al. | ||
|
2021AJ....161..189L
|
17 | D | 1 | 29956 | 19 | Gyro-kinematic ages for around 30,000 Kepler stars. | LU Y., ANGUS R., CURTIS J.L., et al. | ||
|
2023A&A...674A..34G
|
17 | D | 1 | 307215 | 85 | Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. | GAIA COLLABORATION, ARENOU F., BABUSIAUX C., et al. | ||
| 2025AJ....170..212S | 19 | D | 2 | 797 | ~ | A Homogeneous Catalog of Oscillating Solar-type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity. | SAYEED M., HUBER D., CHONTOS A., et al. |
