Comparison of our results, Δϖ_corr = (ϖ_GEDR3 − Z₅)−ϖ_PARAM, to a compilation of Gaia parallax offset residuals from the literature as a function of the magnitude in the G-band. Results displayed as open circles with vertical error bars are from the literature. Our findings for Kepler, K2, and TESS are shown as red, yellow, and blue shaded areas, respectively. Different literature sources used very astrophysically different objects and methods. Here we used the same methodology applied to a rather intrinsically homogeneous group of stars. The sign convention we use is such that positive values correspond to an overcorrection of parallaxes and negative values to an underestimation of parallaxes by L21.