Gaia Data Release 1
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Fig. 10


Weighted linear least-squares fit performed over the MK magnitude of the five RR Lyrae stars in Benedict et al. (2011) using the MK values inferred from the HST parallaxes with (red solid line) and without (red dashed line) Lutz-Kelker correction and the MK values (blue filled circles) inferred from the TGAS parallaxes (black line). Green filled and open circles show the Type II Cepheid VY Pyx with the MK magnitude determined from the TGAS and HST parallax, respectively. The star was not used in the fit.

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