|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| KOI-6284 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:14:57 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2011AJ....141...83P |
15 | D | 1 | 1893 | 430 | Kepler eclipsing binary stars. I. Catalog and principal characterization of 1879 eclipsing binaries in the first data release. | PRSA A., BATALHA N., SLAWSON R.W., et al. | ||
|
2011AJ....142..160S |
15 | D | 1 | 2328 | 365 | Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. | SLAWSON R.W., PRSA A., WELSH W.F., 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. | ||
|
2015MNRAS.447.2714B |
16 | D | 1 | 209 | 133 | Flare stars across the H-R diagram. | BALONA L.A. | ||
|
2016AJ....151..101A |
16 | D | 1 | 447 | 17 | Kepler eclipsing binary stars. VIII. Identification of false positive eclipsing binaries and re-extraction of new light curves. | ABDUL-MASIH M., PRSA A., CONROY K., 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. | ||
|
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. | ||
|
2018ApJS..235....5Q |
16 | D | 2 | 2048 | 72 | Physical properties and evolutionary states of EA-type eclipsing binaries observed by LAMOST. | QIAN S.-B., ZHANG J., HE J.-J., et al. | ||
|
2019ApJ...879...69T |
16 | D | 1 | 222610 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
| 2019ApJ...884..126M | 16 | D | 1 | 113 | ~ | The SDSS-HET survey of Kepler eclipsing binaries. Description of the survey and first results. | MAHADEVAN S., BENDER C.F., HAMBLETON K., et al. | ||
|
2020AJ....160...90A |
16 | D | 1 | 13200 | 33 | Exploring the evolution of stellar rotation using galactic kinematics. | ANGUS R., BEANE A., PRICE-WHELAN A.M., et al. | ||
|
2020MNRAS.499.3481A |
16 | D | 1 | 28505 | 24 | Evidence for metallicity-dependent spin evolution in the Kepler field. | AMARD L., ROQUETTE J. and MATT S.P. | ||
|
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. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
|
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. | ||
|
2023A&A...670A..75C |
17 | D | 1 | 53 | 4 | New compact hierarchical triple system candidates identified using Gaia DR3. | CZAVALINGA D.R., MITNYAN T., RAPPAPORT S.A., 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. | ||
|
2024MNRAS.533.1290S |
18 | D | 1 | 7737 | ~ | The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. | SEE V., LU Y., AMARD L., et al. |