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| TYC 3557-534-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST16:31:15 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2014ApJS..211...24M 
|
16 | 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. | ||
|
2017ApJ...834..207M
|
16 | D | 1 | 4096 | 4 | Magnetic activity analysis for a sample of G-type main sequence Kepler targets. | MEHRABI A., HE H. and KHOSROSHAHI H. | ||
|
2017MNRAS.472.1618G
|
16 | D | 2 | 1784 | 106 | A Kepler study of starspot lifetimes with respect to light-curve amplitude and spectral type. | GILES H.A.C., COLLIER CAMERON A. and HAYWOOD R.D. | ||
|
2018MNRAS.481.3244G
|
16 | D | 1 | 3079 | 24 | Chemo-kinematics of the Milky Way from the SDSS-III MARVELS survey. | GRIEVES N., GE J., THOMAS N., et al. | ||
|
2019ApJ...879...69T
|
17 | D | 1 | 222609 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
|
2020ApJS..247....9Z
|
17 | 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. | ||
|
2020AJ....160..120J
|
17 | D | 1 | 365761 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2021AJ....161...68L
|
17 | D | 1 | 253 | 24 | Hot stars with Kepler planets have high obliquities. | LOUDEN E.M., WINN J.N., PETIGURA E.A., 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. |
