Fig. 3.
Same as in Fig. 2, but fitting an ABL in the general form of Eq. (5) (left panels) and Eq. (6) (right panels) for three different choices of the Gaia parallax zero-point offset. The fit is presented only for fundamental-mode pulsators as no sensible fit could be performed of the DCEP_1Os because our sample contains so few of them.
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