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Fig. 10

Fig. 10 Refer to the following caption and surrounding text.

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Colour excesses from the Gaia GSP-Phot (Andrae et al. 2023) and ESP-HS (Creevey et al. 2023) pipelines (ordinate) versus the cluster E(GBPGRP) derived in this work (abscissa) for OCs. Only the ordinate changes between the two panels; the abscissa is always the Balmer-based E(GBPGRP) derived in Sect. 5. The black line shows the identity relation.

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