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| KOI-5304 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST17:57:20 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 1987ApJS...65..161H | 1291 | 12 | Micrometer observations of double stars and new pairs. XIII. | HEINTZ W.D. | |||||
2013A&A...560A...4R 
|
16 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
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. | ||
|
2015ApJ...807..170H
|
16 | D | 1 | 2117 | 10 | Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. | HOLCZER T., SHPORER A., MAZEH T., et al. | ||
|
2016ApJS..225....9H
|
16 | D | 2 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., 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.465.2634A
|
16 | D | 1 | 5400 | 21 | Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. | ARMSTRONG D.J., POLLACCO D. and SANTERNE A. | ||
|
2020AJ....160...90A
|
17 | 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
|
17 | D | 1 | 28505 | 24 | Evidence for metallicity-dependent spin evolution in the Kepler field. | AMARD L., ROQUETTE J. and MATT S.P. |
