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| TYC 3142-1065-1 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:10:10 |
| 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..210....1C |
15 | D | 1 | 519 | 296 | Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler mission. | CHAPLIN W.J., BASU S., HUBER D., 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. | ||
|
2014ApJ...790L..23D |
15 | D | 1 | 79 | 34 | Rotation periods and ages of solar analogs and solar twins revealed by the Kepler mission. | DO NASCIMENTO J.-D.Jr, GARCIA R.A., MATHUR S., et al. | ||
|
2014A&A...572A..34G |
15 | D | 1 | 315 | 228 | Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations. | GARCIA R.A., CEILLIER T., SALABERT D., et al. | ||
|
2015ApJ...808..187B |
16 | D | 1 | 540 | 73 | The metallicities of stars with and without transiting planets. | BUCHHAVE L.A. and LATHAM D.W. | ||
|
2016AJ....152....6W |
16 | D | 1 | 3060 | 13 | Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. | WANG L., WANG W., WU Y., et al. | ||
| 2017RAA....17....5W | 16 | D | 1 | 180 | 4 | Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler. | WU Y.-Q., XIANG M.-S., ZHANG X.-F., et al. | ||
|
2018ApJ...858...28V |
16 | D | 1 | 459 | 13 | Investigating the metallicity-mixing-length relation. | VIANI L.S., BASU S., ONG J.M.J., et al. | ||
|
2018ApJ...861..149F |
16 | D | 1 | 2261 | 6 | The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. | FURLAN E., CIARDI D.R., COCHRAN W.D., et al. | ||
|
2020ApJS..251...15Z |
16 | D | 1 | 20886 | 38 | Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. | ZONG W., FU J.-N., DE CAT P., 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. | ||
|
2021ApJS..255...17S |
17 | D | 1 | 39591 | 57 | Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. | SANTOS A.R.G., BRETON S.N., MATHUR S., et al. | ||
|
2021AJ....162..184K |
17 | D | 1 | 8106 | 31 | Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data. | KOUNKEL M., COVEY K.R., STASSUN K.G., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022ApJ...930....7A |
17 | D | 1 | 4216 | 14 | Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity. | AVALLONE E.A., TAYAR J.N., VAN SADERS J.L., et al. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. | ||
|
2022A&A...664A..78F |
17 | D | 1 | 7452 | 7 | Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. | FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., 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. |