GaiaUnlimited: The old stellar disc of the Milky Way as traced by the red clump

Open Access

Fig. H.1

Relative residual (1-model/data) for ɡdr3wise[RC], corresponding to the four cases exploring warp parameters shown in Fig. 26. For each case, we show the residuals in successive R annuli (9.5 kpc<R< 14.5 kpc). The corner plots corresponding to each case are shown in Fig. 26.

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