Fig. 4
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Location of emission-line cluster members in the Hertzsprung–Russell-like diagrams. Open symbols represent previously known emission stars; filled symbols indicate new emission candidates from Sect. 4. Left: observed CAMD (using the parallax of the cluster from Hunt & Reffert 2023). Centre: de-reddened CAMD using AG from BaSeL-3.1-based relations in Eq. (2). Right: GSP-Phot (Creevey et al. 2023; Andrae et al. 2023) parameters derived for the same sources.
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