ID | Period (d) |
![]() |
[Fe/H] | [Fe/H]
![]() |
![]() |
1 | 0.552281 | 5.11936 | -1.38 | -1.65 | 0.19 |
5 | 0.615099 | 5.40388 | -1.42 | -1.69 | 0.28 |
7 | 0.588000 | 5.17437 | -1.51 | -1.79 | 0.23 |
12 | 0.587633 | 5.22300 | -1.46 | -1.73 | 0.22 |
14 | 0.608022 | 5.85473 | -0.91 | -1.16 | 0.20 |
21 | 0.612120 | 4.77138 | -2.06 | -2.36 | 0.28 |
23 | 0.523110 | 4.41584 | -1.95 | -2.25 | 0.17 |
24 | 0.596015 | 5.74087 | -0.96 | -1.21 | 0.38 |
25 | 0.800898 | 5.61235 | -2.19 | -2.50 | 0.17 |
27 | 0.596109 | 5.37598 | -1.34 | -1.61 | 0.14 |
34 | 0.562213 | 5.42900 | -1.11 | -1.36 | 0.15 |
37 | 0.598353 | 5.19618 | -1.54 | -1.82 | 0.15 |
44 | 0.528236 | 5.06653 | -1.30 | -1.57 | 0.25 |
45 | 0.561698 | 5.32247 | -1.21 | -1.48 | 0.15 |
49 | 0.547890 | 5.67561 | -0.77 | -1.02 | 0.19 |
59 | 0.522958 | 5.05802 | -1.28 | -1.55 | 0.25 |
71 | 0.460702 | 4.76450 | -1.26 | -1.52 | 0.16 |
76 | 0.577865 | 4.76634 | -1.88 | -2.18 | 0.17 |
79 | 0.572610 | 5.20478 | -1.40 | -1.67 | 0.26 |
97 | 0.547472 | 5.27824 | -1.18 | -1.45 | 0.25 |
103 | 0.483590 | 4.70712 | -1.44 | -1.71 | 0.16 |
104 | 0.602988 | 5.50416 | -1.25 | -1.51 | 0.15 |
109 | 0.730896 | 5.36499 | -2.08 | -2.38 | 0.15 |
115 | 0.554167 | 5.18484 | -1.32 | -1.59 | 0.16 |
120 | 0.612234 | 6.04222 | -0.73 | -0.98 | 0.21 |
121 | 0.426879 | 5.66504 | -0.14 | -0.35 | 0.30 |
124 | 0.561183 | 5.46345 | -1.06 | -1.32 | 0.45 |
128 | 0.621765 | 5.04672 | -1.82 | -2.11 | 0.16 |
134 | 0.643060 | 5.33914 | -1.63 | -1.91 | 0.14 |
137 | 0.609840 | 5.37539 | -1.42 | -1.69 | 0.17 |
144 | 0.580523 | 5.48349 | -1.15 | -1.41 | 0.21 |
Notes: The ID of RR Lyrae star as given in
Wu et al. (2005); [Fe/H]: iron abundance calculated from Fourier
parameters and in the scale of JK96; [Fe/H]
![]() ![]() |