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| 2MASS J19052704+4314462 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:33:13 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2011A&A...529A..89D |
15 | D | 1 | 3298 | 98 | Global stellar variability study in the field-of-view of the Kepler satellite. | DEBOSSCHER J., BLOMME J., AERTS C., 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...788..114R |
170 | D | X C | 4 | 184 | 17 | M-dwarf rapid rotators and the detection of relatively young multiple M-star systems. | RAPPAPORT S., SWIFT J., LEVINE A., et al. | |
| 2014MNRAS.441.2744V | 132 | D | X F | 3 | 16 | 21 | Looking for activity cycles in late-type Kepler stars using time-frequency analysis. | VIDA K., OLAH K. and SZABO R. | |
|
2016MNRAS.457.2877G |
16 | D | 1 | 4245 | 141 | They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. | GAIDOS E., MANN A.W., KRAUS A.L., et al. | ||
|
2017ApJ...849...36Y |
16 | D | 1 | 542 | 111 | The flaring activity of M dwarfs in the Kepler field. | YANG H., LIU J., GAO Q., et al. | ||
| 2019A&A...622A..40K | 16 | D | X | 1 | 46 | 5 | Cycle period, differential rotation, and meridional flow for early M dwarf stars. | KUKER M., RUDIGER G., OLAH K., 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. | ||
|
2019ApJS..244...37G |
16 | D | 1 | 1744 | ~ | Flare activity and magnetic feature analysis of the flare stars. | GOODARZI H., MEHRABI A., KHOSROSHAHI H.G., et al. | ||
|
2020AJ....160..253L |
16 | D | 1 | 3432 | 12 | An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. | LU C.X., SCHLAUFMAN K.C. and CHENG S. |