Fig. 3

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Relation between average indices – without the most active stars – for the three pairs of indices (from top to bottom) and the 3400–3900 K range. The values in ordinates have been shifted vertically to take the temperature effect into account (We selected points with Cam around 0.9 (for the two first plots) or Nam around 0.15 (for the last plot), fitted a linear function to the index versus Teff and applied the resulting correction to all points.). The red points and lines correspond to averages in bins in abscissa.
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