Fig. 14
Each panel shows the comparison between the target stars and the templates used to obtain the continuum accretion luminosity (as listed in Table 3) in the region of the CaII H (λ393.37 nm) and CaII K (λ396.85 nm) lines. The CaII K line is blended with the Hϵ at λ 397.0 nm. These lines are tracers of the chromospheric activity of the young stars.
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