Fig. B.2.
Posterior probability distribution for parameters of our model for a given RR Lyrae star in our sample (bestObjID = 1237649919501598744) with confidence intervals (CIs) color-coded. We see an offset between systemic velocities determined from Hβ, Hγ, and Hδ in comparison with a systemic velocity determined through the Hα line (see color histogram on the right-hand side of the figure).
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