Table 7: Mean intrinsic distance moduli (in magnitudes), as derived by the Wesenheit functions of BL Her and W Vir stars (the quantity Nis the number of averaged values).
Name $\mu_0$(BLH) N $\mu_0$(WV) N $\mu_0$(RR)
N2808 14.99 $\pm$ 0.06 1 - - 14.90
N5139 13.84 $\pm$ 0.08 4 13.78 $\pm$ 0.16 4 13.62
N6254 13.39 $\pm$ 0.20 4 13.56 $\pm$ 0.16 2 13.23
N6273 14.69 $\pm$ 0.06 1 14.77 $\pm$ 0.06 2 14.71
N6284 15.77 $\pm$ 0.06 2 - - 15.93
N6293 14.80 $\pm$ 0.06 1 - - 14.76
N6402 14.80 $\pm$ 0.08 8 14.93 $\pm$ 0.09 8 14.86
N6441 15.55 $\pm$ 0.07 2 15.53 $\pm$ 0.19 6 15.28
N6441mp 15.61 $\pm$ 0.07 2 15.58 $\pm$ 0.18 6 15.60
N6715 17.19 $\pm$ 0.10 2 - - 17.16
N6749 14.56 $\pm$ 0.08 1 - - 14.51
N6779 15.05 $\pm$ 0.06 4 15.31 $\pm$ 0.11 4 15.08

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