A clustering-based search for substructures in the Galactic plane and bulge using RR Lyrae stars as tracers

Open Access

Fig. C.1

Same as the lower-left and lower-middle panels of Fig. 2, but adopting the literature metallicity of the stars' host cluster (instead of their photometric metallicities) when using the PLZ relations from Prudil et al. (2024) to derive distances.

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