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Fig. 12
Survey of the reduced χ2 obtained from Hα profile fitting for the observed solar flux spectra (top panel) and spectra of Procyon (bottom panel) with different αCMA and Teff. The preferred parameter area is located where χ2 is minimal. All χ2 are not normalized and indicate a good fit in each case.
This figure is made of several images, please see below:
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