Table 1
RR Lyrae stars analyzed in this work.
| OBJ | Period d | ϖ mas | [Fe/H] dex | E(B − V) mag | E(B − V)G mag |
|---|---|---|---|---|---|
| U Lep | 0.5814789 | 0.989 ± 0.017 | −1.81 ± 0.17 | 0.029 | 0.05 |
| RX Eri | 0.5872453 | 1.723 ± 0.023 | −1.45 ± 0.15 | 0.053 | 0.08 |
| SV Eri | 0.713877 | 1.361 ±0.024 | −2.22 ± 0.02 | 0.078 | 0.09 |
| AE Boo | 0.3148921 | 1.143 ± 0.019 | −1.62 ± 0.08 | 0.023 | 0.00 |
| BB Eri | 0.5699097 | 0.722 ± 0.024 | −1.66 ± 0.04 | 0.043 | 0.05 |
| V467 Cen | 0.5514041 | 1.255 ± 0.023 | −0.57 ± 0.01 | 0.050 | − |
| V Ind | 0.4796017 | 1.506 ± 0.019 | −1.62 ± 0.01 | 0.040 | − |
| WZ Hya | 0.5377182 | 1.029 ± 0.016 | −1.48 ± 0.02 | 0.069 | 0.05 |
| SX For | 0.6053423 | 0.868 ± 0.015 | −2.20 ± 0.02 | 0.012 | − |
Notes. The table contains corresponding stellar pulsation periods, metallicities, Gaia parallaxes, and E(B − V) values applied in the dereddening process. Metallicities adopted from Crestani et al. (2021) work. The last column E(B − V)G contains reddening values from Green et al. (2019) used for the estimation of the reddening error.
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