Fig. 18.

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Distribution of the Hα pseudo-equivalent width (pEW) obtained by ESP-ELS for 135 258 targets chosen in order to homogeneously cover the temperature domain as a function of the effective temperature derived by GSP-Phot and ESP-HS (Teff > 7500 K only for the latter). Left panel: we report the value obtained before the removal of the model estimate. Middle panel: we show the result saved in ew_espels_halpha (the model value is removed for sources with Teff ≤ 5000 K). Right panel: we show the result obtained when the model value (ew_espels_halpha_model) is also removed for stars hotter than 5000 K.
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