Extended Data Fig. 3: The posterior sampling results of the RVGSR distribution.
From: The tidal remnant of an unusually metal-poor globular cluster
The parameters p0, p1 and p2 are the best-fitting polynomial parameters for RVGSR(ϕ1) = p0 + p1ϕ1 + p2ϕ12; σrv is the intrinsic dispersion. Here the best-fitting parameters are calculated with ϕ1 in radians. This figure is made using the corner package55.
