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Table 4.

Shifts of log P in the fundamentalization formula determined for RRc stars.

Band Δlog P Band Δlog P
(mag) (mag)
(Parallax): (Geometric distances):

g 0.296 ± 0.034 g 0.297 ± 0.036
r 0.247 ± 0.023 r 0.246 ± 0.025
i 0.223 ± 0.019 i 0.222 ± 0.020
W r ri $ W_{r}^{ri} $ 0.174 ± 0.013 W r ri $ W_{r}^{ri} $ 0.171 ± 0.014
W g gr $ W^{gr}_{g} $ 0.151 ± 0.015 W g gr $ W^{gr}_{g} $ 0.149 ± 0.015
W g gi $ W_{g}^{gi} $ 0.164 ± 0.012 W g gi $ W_{g}^{gi} $ 0.162 ± 0.013

(ABL method): (Photo-geometric distances):

g 0.298 ± 0.035 g 0.294 ± 0.035
r 0.249 ± 0.023 r 0.244 ± 0.024
i 0.226 ± 0.019 i 0.220 ± 0.020
W r ri $ W_{r}^{ri} $ 0.178 ± 0.012 W r ri $ W_{r}^{ri} $ 0.170 ± 0.014
W g gr $ W^{gr}_{g} $ 0.153 ± 0.014 W g gr $ W^{gr}_{g} $ 0.148 ± 0.016
W g gi $ W_{g}^{gi} $ 0.167 ± 0.012 W g gi $ W_{g}^{gi} $ 0.161 ± 0.013

Notes. Band: the Sloan–Pan-STARRS gP1rP1iP1 bands and Wesenheit indices; Δlog P: a new shift of log P for fundamentalization.

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