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Fig. C.1

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Examples of computed S/N using the inverse of 1.48 times a rolling MAD in YARARA river diagram maps (labeled as ’extracted’) and compared with the theoretical SNcont value if only photon-noise limited. In the case of a star photon-noise limited with S/Ncont ~ 200, both methods produce similar values (green and red curves). For a spectrum flat-field limited as for HD 128621 observations (blue and orange curves), the SNcont is saturated to the SNcont of the flat-field raw frames (black dashed line).

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