Fig. 1
A solid line shows the spectral response ℰK of Kepler as a function of the wavelength λ (after Van Cleve et al. 2009), whereas dotted and dashed lines show the spectral responses of CoRoT seismo- and exofield (Auvergne et al. 2009). Grey profiles indicate the spectra (in arbitrary units) of black bodies with temperatures of 7000, 6000, and 5000 K, from top to bottom.
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