Oscillation and granulation power in 279 red giants both decrease from Kepler to TESS wavelengths as theory predicts, and the signal-to-noise ratio is roughly wavelength-independent.
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Testing the wavelength dependence of oscillations and granulation in red giants using Kepler and TESS
Oscillation and granulation power in 279 red giants both decrease from Kepler to TESS wavelengths as theory predicts, and the signal-to-noise ratio is roughly wavelength-independent.