Table 1.
MW RR Lyr star sample and their main parameters.
Star | Period | ϖDR3 | RUWE | GOF | E(B − V) | ⟨g⟩ | ⟨r⟩ | ⟨i⟩ | [Fe/H] | Source |
---|---|---|---|---|---|---|---|---|---|---|
(days) | (mas) | (mag) | (mag) | (mag) | (mag) | (dex) | ||||
RRab | ||||||||||
AA Aql | 0.3617877 | 0.7615 ± 0.0179 | 1.14 | 3.96 | 0.0710 ± 0.0059 | 11.907 ± 0.004 | 11.786 ± 0.003 | 11.780 ± 0.003 | −0.42 ± 0.11 | 1 |
AV Peg | 0.3903814 | 1.5075 ± 0.0176 | 1.25 | 5.44 | 0.0520 ± 0.0007 | 10.606 ± 0.003 | 10.417 ± 0.002 | 10.395 ± 0.002 | −0.03 ± 0.07 | 1 |
BB Eri (a) | 0.5699097 | 0.7216 ± 0.0238 | 1.74 | 22.82 | 0.0430 ± 0.0015 | 11.628 ± 0.003 | 11.447 ± 0.003 | 11.392 ± 0.003 | −1.66 ± 0.07 | 1 |
BH Peg | 0.640993 | 1.1813 ± 0.0226 | 1.22 | 3.97 | 0.0700 ± 0.0008 | 10.629 ± 0.008 | 10.346 ± 0.005 | 10.247 ± 0.005 | – | – |
BK Tuc | 0.5500676 | 0.3630 ± 0.0172 | 1.34 | 8.98 | 0.0240 ± 0.0004 | 12.906 ± 0.007 | 12.741 ± 0.006 | 12.715 ± 0.006 | −1.86 ± 0.01 | 1 |
BR Aqr | 0.4818717 | 0.8075 ± 0.0217 | 0.90 | -2.09 | 0.0240 ± 0.0003 | 11.525 ± 0.002 | 11.367 ± 0.003 | 11.333 ± 0.005 | −0.94 ± 0.07 | 1 |
BT Aqr (a) | 0.4063595 | 0.5365 ± 0.0220 | 1.41 | 12.11 | 0.0400 ± 0.0002 | 12.502 ± 0.003 | 12.343 ± 0.002 | 12.322 ± 0.003 | −0.24 ± 0.04 | 1 |
CD Vel | 0.5735076 | 0.5874 ± 0.0137 | 1.26 | 7.44 | 0.1920 ± 0.0055 | 12.185 ± 0.006 | 11.953 ± 0.005 | 11.862 ± 0.004 | −1.84 ± 0.09 | 1 |
CP Aqr | 0.4634018 | 0.7754 ± 0.0236 | 1.04 | 0.78 | 0.0500 ± 0.0016 | 11.883 ± 0.007 | 11.755 ± 0.004 | 11.740 ± 0.003 | −0.62 ± 0.04 | 1 |
DH Hya (a) | 0.4890007 | 0.5033 ± 0.0266 | 1.55 | 16.42 | 0.0370 ± 0.0031 | 12.263 ± 0.003 | 12.147 ± 0.003 | 12.125 ± 0.003 | −1.78 ± 0.04 | 1 |
DN Aqr | 0.6337558 | 0.7785 ± 0.0195 | 0.95 | -0.97 | 0.0220 ± 0.0007 | 11.336 ± 0.006 | 11.170 ± 0.004 | 11.111 ± 0.006 | −1.74 ± 0.03 | 1 |
DX Del | 0.4726191 | 1.7584 ± 0.0150 | 0.99 | -0.43 | 0.0800 ± 0.0018 | 10.096 ± 0.002 | 9.859 ± 0.002 | 9.792 ± 0.003 | −0.43 ± 0.08 | 1 |
EW Cam | 0.628408 | 1.7499 ± 0.0136 | 1.04 | 1.30 | 0.0180 ± 0.0007 | 9.706 ± 0.003 | 9.492 ± 0.002 | 9.394 ± 0.002 | – | – |
HH Pup | 0.3907454 | 1.1377 ± 0.0151 | 1.07 | 1.82 | 0.1240 ± 0.0054 | 11.408 ± 0.005 | 11.195 ± 0.004 | 11.123 ± 0.003 | −0.73 ± 0.02 | 1 |
RR Cet | 0.55302836 | 1.6217 ± 0.0213 | 1.01 | 0.43 | 0.0200 ± 0.0003 | 9.835 ± 0.006 | 9.681 ± 0.007 | 9.640 ± 0.006 | −1.63 ± 0.10 | 1 |
RR Gru | 0.5524640 | 0.5105 ± 0.0142 | 1.05 | 1.45 | 0.0190 ± 0.0007 | 12.598 ± 0.003 | 12.399 ± 0.003 | 12.355 ± 0.003 | −0.47 ± 0.04 | 1 |
RR Leo | 0.4524021 | 1.0836 ± 0.0248 | 1.12 | 2.75 | 0.0340 ± 0.0035 | 10.816 ± 0.003 | 10.720 ± 0.002 | 10.721 ± 0.001 | −1.58 ± 0.08 | 1 |
RU Scl | 0.4933549 | 1.2800 ± 0.0317 | 1.24 | 5.20 | 0.0170 ± 0.0004 | 10.308 ± 0.008 | 10.207 ± 0.005 | 10.201 ± 0.004 | −1.45 ± 0.06 | 1 |
RV Cet | 0.62341 | 0.9762 ± 0.0177 | 1.14 | 3.21 | 0.0270 ± 0.0006 | 11.059 ± 0.005 | 10.844 ± 0.004 | 10.776 ± 0.004 | −1.50 ± 0.03 | 1 |
RV Phe (a) | 0.5964071 | 0.5606 ± 0.0197 | 1.44 | 14.27 | 0.0070 ± 0.0005 | 12.039 ± 0.003 | 11.856 ± 0.003 | 11.801 ± 0.004 | −1.54 ± 0.04 | 1 |
RX Cet | 0.57373 | 0.7647 ± 0.0303 | 1.33 | 6.21 | 0.0240 ± 0.0007 | 11.526 ± 0.006 | 11.346 ± 0.005 | 11.307 ± 0.004 | −1.53 ± 0.04 | 1 |
RX Eri | 0.5872453 | 1.7229 ± 0.0225 | 1.28 | 8.44 | 0.0530 ± 0.0018 | 9.810 ± 0.003 | 9.593 ± 0.003 | 9.548 ± 0.003 | −1.51 ± 0.08 | 1 |
S Ara | 0.451848 | 1.1271 ± 0.0169 | 1.04 | 0.94 | 0.0880 ± 0.0027 | 10.839 ± 0.015 | 10.707 ± 0.010 | 10.679 ± 0.009 | −1.40 ± 0.04 | 1 |
SS For | 0.49543 | 1.2868 ± 0.0205 | 1.27 | 8.44 | 0.0130 ± 0.0002 | 10.465 ± 0.024 | 10.297 ± 0.019 | 10.269 ± 0.010 | – | – |
ST Pic | 0.4857445 | 2.0822 ± 0.0123 | 1.00 | -0.03 | 0.0270 ± 0.0012 | 9.568 ± 0.002 | 9.459 ± 0.002 | 9.433 ± 0.002 | – | – |
SV Eri | 0.713877 | 1.3609 ± 0.0236 | 0.98 | -0.40 | 0.0780 ± 0.0023 | 10.122 ± 0.005 | 9.892 ± 0.004 | 9.798 ± 0.002 | −2.22 ± 0.03 | 1 |
SW And | 0.442262 | 1.9954 ± 0.0284 | 1.20 | 5.23 | 0.0330 ± 0.0011 | 9.812 ± 0.003 | 9.603 ± 0.004 | 9.567 ± 0.004 | −0.17 ± 0.05 | 2 |
SX For | 0.6053423 | 0.8680 ± 0.0146 | 0.97 | -0.99 | 0.0120 ± 0.0009 | 11.245 ± 0.003 | 11.051 ± 0.003 | 11.000 ± 0.003 | −1.81 ± 0.01 | 1 |
SZ Gem (a) | 0.5011303 | 0.7004 ± 0.0248 | 1.44 | 10.70 | 0.0380 ± 0.0004 | 11.822 ± 0.002 | 11.715 ± 0.002 | 11.697 ± 0.002 | −1.87 ± 0.10 | 2 |
TT Lyn | 0.597434355 | 1.4798 ± 0.0160 | 0.86 | -3.57 | 0.0150 ± 0.0005 | 10.019 ± 0.006 | 9.806 ± 0.005 | 9.746 ± 0.003 | −1.53 ± 0.01 | 2 |
U Lep | 0.5814789 | 0.9889 ± 0.0167 | 1.33 | 9.72 | 0.0290 ± 0.0015 | 10.671 ± 0.005 | 10.553 ± 0.003 | 10.534 ± 0.004 | −1.88 ± 0.28 | 1 |
U Pic | 0.4403750 | 0.8236 ± 0.0128 | 0.92 | -2.09 | 0.0090 ± 0.0002 | 11.465 ± 0.004 | 11.342 ± 0.004 | 11.345 ± 0.004 | −0.82 ± 0.03 | 1 |
UU Cet | 0.6060736 | 0.5334 ± 0.0191 | 1.20 | 4.83 | 0.0200 ± 0.0006 | 12.174 ± 0.004 | 11.972 ± 0.004 | 11.919 ± 0.004 | −1.66 ± 0.04 | 2 |
V341 Aql | 0.5780230 | 0.8822 ± 0.0230 | 1.21 | 5.61 | 0.0790 ± 0.0021 | 10.955 ± 0.003 | 10.827 ± 0.003 | 10.808 ± 0.003 | −1.47 ± 0.04 | 1 |
V4424 Sgr | 0.4245034 | 1.7868 ± 0.0145 | 1.05 | 1.22 | 0.0890 ± 0.0029 | 10.496 ± 0.006 | 10.179 ± 0.003 | 10.140 ± 0.003 | – | – |
V675 Sgr ( * ) | 0.6422935 | 1.1993 ± 0.0188 | 0.75 | -5.51 | 0.0910 ± 0.0055 | 10.536 ± 0.002 | 10.337 ± 0.002 | 10.279 ± 0.003 | −2.47 ± 0.02 | 2 |
V Ind | 0.4796017 | 1.5058 ± 0.0191 | 1.00 | 0.02 | 0.0400 ± 0.0009 | 10.076 ± 0.005 | 9.963 ± 0.002 | 9.985 ± 0.003 | −1.63 ± 0.03 | 1 |
VW Scl (a) | 0.5109117 | 0.9027 ± 0.0338 | 1.74 | 26.98 | 0.0140 ± 0.0011 | 11.106 ± 0.005 | 11.016 ± 0.004 | 11.043 ± 0.004 | −1.38 ± 0.23 | 1 |
W Tuc | 0.6422382 | 0.6276 ± 0.0133 | 0.98 | -0.58 | 0.0180 ± 0.0002 | 11.504 ± 0.003 | 11.393 ± 0.003 | 11.371 ± 0.003 | −1.90 ± 0.08 | 1 |
WY Ant | 0.5743427 | 0.9787 ± 0.0208 | 1.11 | 3.29 | 0.0550 ± 0.0009 | 10.995 ± 0.005 | 10.803 ± 0.004 | 10.744 ± 0.004 | −1.95 ± 0.06 | 1 |
X Ari | 0.6511796 | 1.8690 ± 0.0188 | 1.22 | 4.48 | 0.1670 ± 0.0053 | 9.798 ± 0.026 | 9.452 ± 0.006 | 9.323 ± 0.008 | −2.59 ± 0.05 | 1 |
X Ret | 0.49201 | 0.6590 ± 0.0144 | 1.38 | 9.78 | 0.0400 ± 0.0022 | 11.809 ± 0.009 | 11.663 ± 0.007 | 11.647 ± 0.006 | – | – |
XZ Gru | 0.8831035 | 0.8700 ± 0.0185 | 1.12 | 2.76 | 0.0040 ± 0.0006 | 10.864 ± 0.004 | 10.647 ± 0.004 | 10.575 ± 0.004 | – | – |
Z Mic | 0.5869258 | 0.8190 ± 0.0230 | 0.96 | -0.83 | 0.0820 ± 0.0028 | 11.792 ± 0.003 | 11.507 ± 0.003 | 11.397 ± 0.002 | −1.58 ± 0.05 | 1 |
RRc | ||||||||||
AE Boo | 0.3148921 | 1.1432 ± 0.0190 | 1.06 | 1.45 | 0.0230 ± 0.0012 | 10.722 ± 0.004 | 10.662 ± 0.003 | 10.681 ± 0.002 | −1.62 ± 0.09 | 1 |
CS Eri | 0.311331 | 2.1665 ± 0.0158 | 1.05 | 1.38 | 0.0170 ± 0.0004 | 9.056 ± 0.006 | 9.002 ± 0.006 | 9.050 ± 0.007 | −1.97 ± 0.09 | 1 |
EV Psc | 0.3062573 | 1.1328 ± 0.0300 | 1.12 | 3.21 | 0.0300 ± 0.0008 | 10.640 ± 0.003 | 10.555 ± 0.003 | 10.575 ± 0.003 | – | – |
IY Eri | 0.375026 | 0.7626 ± 0.0133 | 0.96 | −1.10 | 0.0230 ± 0.0011 | 11.133 ± 0.005 | 11.067 ± 0.004 | 11.109 ± 0.003 | – | – |
LS Her | 0.230808 | 1.0254 ± 0.0206 | 0.98 | −0.36 | 0.0360 ± 0.0009 | 10.977 ± 0.009 | 10.957 ± 0.007 | 11.006 ± 0.005 | – | – |
MT Tel (a) | 0.3169011 | 2.0704 ± 0.0301 | 1.65 | 11.93 | 0.0340 ± 0.0026 | 9.102 ± 0.006 | 9.085 ± 0.007 | 9.079 ± 0.004 | −2.60 ± 0.18 | 1 |
RU Psc (a) | 0.390385 | 1.2783 ± 0.0291 | 1.53 | 1.25 | 0.0390 ± 0.0002 | 10.333 ± 0.010 | 10.171 ± 0.006 | 10.157 ± 0.005 | – | – |
RU Sex | 0.350232 | 0.9155 ± 0.0206 | 1.33 | 8.54 | 0.0270 ± 0.0006 | 10.885 ± 0.003 | 10.806 ± 0.002 | 10.821 ± 0.002 | −1.97 ± 0.10 | 2 |
T Sex | 0.32469759 | 1.3400 ± 0.0225 | 1.16 | 3.16 | 0.0420 ± 0.0032 | 10.124 ± 0.004 | 10.075 ± 0.003 | 10.090 ± 0.003 | −1.49 ± 0.10 | 1 |
Notes. Star: name of a RR Lyr star; Period: period of a RR Lyr star adopted from AAVSO database; ϖDR3: parallax from Gaia DR3 catalog corrected with Lindegren et al. (2021) corrections; RUWE: renormalized unit weight error from the Gaia DR3 catalog; GOF: goodness-of-fit from the Gaia DR3 catalog; E(B − V): reddening value applied from Schlafly & Finkbeiner (2011) reddening map corrected for the MW model by Drimmel & Spergel (2001); ⟨g⟩, ⟨r⟩, ⟨i⟩: intensity-averaged mean magnitude from Fourier series fitting for the Pan-STARRS gP1rP1iP1 filters, respectively; [Fe/H]: the adopted iron abundance; Source: source of iron abundance (1 – Crestani et al. 2021a; 2 – Crestani et al. 2021b).
Stars rejected based on the RUWE and GOF parallax quality parameters given by the Gaia DR3 catalog.
( * )The SED showed that the Sloan gri mean magnitudes are systematically fainter than the photomertic compilation from Monson et al. (2017).
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