The model fitting of Gaia DR3 classical Cepheid light and radial velocity curves

Open Access

Fig. 7.

Top panel: Comparison between the Gaia DR3 parallaxes, corrected according to the L21 recipe, and those obtained from our pulsation model fitting technique, shown together with 1:1 line (grey solid). Bottom panel: Residuals, $Δ = ϖ_{models} - ϖ_{DR 3}$ $\rm \Delta = \varpi_{models} - \varpi_{DR3}$ , around the 1:1 line plotted against the DR3+L21 parallaxes.

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