The CARMENES search for exoplanets around M dwarfs - Behaviour of the Paschen lines during flares and quiescence

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Fig. 2

pEW(Paβ) shown as a function of T_eff. Grey dots represent median(pEW(Paβ)) for each star, the coloured circles represent the mean of these median(pEW(Paβ)) measurements for each T_eff interval as introduced in the main text. The colours are chosen as in Figs. 3 and 5 to simplify comparison.

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