Detectability of Solar Rotation Period across Various Wavelengths
The light curves of old G dwarfs obtained in the visible and near-infrared wavelength ranges are highly irregular. This significantly complicates the detectability of the rotation periods of stars similar to the Sun in large photometric surveys, such as Kepler and TESS. In this study, we show that l...
Furkejuvvon:
| Váldodahkkit: | , , , , , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
IOP Publishing
2025-01-01
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| Ráidu: | The Astrophysical Journal Letters |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.3847/2041-8213/adb0b3 |
| Fáddágilkorat: |
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