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| 2MASS J19263017+3802518 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:59:05 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2012ApJS..199...24T |
15 | D | 1 | 5394 | 66 | Detection of potential transit signals in the first three quarters of Kepler mission data. | TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al. | ||
|
2012AJ....143..101M |
15 | D | 1 | 253 | 43 | The classification of Kepler B-star variables. | McNAMARA B.J., JACKIEWICZ J. and McKEEVER J. | ||
|
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. | ||
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
2015A&A...583A..65R |
16 | D | 1 | 20938 | 134 | Rotation, differential rotation, and gyrochronology of active Kepler stars. | REINHOLD T. and GIZON L. | ||
| 2018A&A...619A..98H | 16 | D | 4 | 70 | 27 | The Kepler view of magnetic chemically peculiar stars. | HUMMERICH S., MIKULASEK Z., PAUNZEN E., et al. | ||
|
2020A&A...640A..40H |
16 | D | 1 | 1016 | 21 | A plethora of new, magnetic chemically peculiar stars from LAMOST DR4. | HUMMERICH S., PAUNZEN E. and BERNHARD K. | ||
|
2022ApJS..259...63S |
17 | D | 2 | 10269 | 2 | Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. | SHANG L.-H., LUO A.-L., WANG L., et al. | ||
|
2023A&A...676A..55L |
17 | D | 1 | 790 | ~ | Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS. | LABADIE-BARTZ J., HUMMERICH S., BERNHARD K., et al. | ||
| 2025MNRAS.538.3247B | 485 | D | X F | 10 | 37 | ~ | GALEX UV survey of magnetic chemically peculiar stars in the Kepler prime field. | BERTONE E., HUMMERICH S., CHAVEZ M., et al. |