Table A.1
Photometric and shock properties of the studied RR Lyrae stars.
ID | Ks | AmpKs | [Fe/H] | σ[Fe/H] | MV | ![]() |
MI | ![]() |
![]() |
![]() |
xHUMP | yHUMP | xBUMP | yBUMP | AmpHUMP | AmpBUMP | Oo | a2 | ![]() |
ClassHUMP | ClassBUMP |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[mag] | [mag] | [dex] | [dex] | [mag] | [mag] | [mag] | [mag] | [mag] | [mag] | ||||||||||||
01010 | 13.014 | 0.095 | −1.265 | 0.244 | 0.605 | 0.230 | 0.214 | 0.050 | −0.277 | 0.041 | −0.064 | −0.1067 | −0.3038 | 0.2360 | 0.0827 | 0.0510 | 1 | 2.463 × 10−10 | 7.945 × 10−12 | 2 | 2 |
01058 | 13.779 | 0.313 | −1.004 | 0.171 | 0.672 | 0.159 | 0.209 | 0.035 | −0.363 | 0.029 | −0.062 | −0.1299 | −0.2828 | 0.2614 | 0.0897 | 0.0710 | 1 | −2.943 × 10−10 | 1.897 × 10−11 | 2 | 3 |
01082 | 13.659 | 0.222 | −1.143 | 0.207 | 0.635 | 0.194 | 0.092 | 0.042 | −0.590 | 0.035 | −0.111 | −0.1757 | −0.3833 | 0.1762 | 0.1602 | 0.0521 | 1 | 3.074 × 10−12 | 9.346 × 10−12 | 3 | 2 |
01646 | 13.693 | 0.198 | −1.023 | 0.243 | 0.667 | 0.227 | 0.120 | 0.050 | −0.561 | 0.041 | −0.131 | −0.1644 | −0.4238 | 0.1852 | 0.0440 | 0.0287 | 1 | −1.309 × 10−11 | 4.212 × 10−11 | 1 | 1 |
01692 | 14.200 | 0.359 | −1.039 | 0.197 | 0.662 | 0.184 | 0.167 | 0.040 | −0.449 | 0.033 | −0.067 | −0.1016 | −0.3021 | 0.2687 | 0.0466 | 0.0671 | 2 | −1.586 × 10−10 | 9.942 × 10−12 | 1 | 4 |
01694 | 14.111 | 0.279 | −1.217 | 0.194 | 0.617 | 0.182 | 0.069 | 0.040 | −0.620 | 0.033 | −0.073 | −0.1019 | −0.3808 | 0.1946 | 0.0740 | 0.0484 | 2 | −4.227 × 10−10 | 6.114 × 10−11 | 2 | 3 |
01732 | 14.641 | 0.388 | −0.883 | 0.211 | 0.708 | 0.196 | 0.372 | 0.043 | −0.027 | 0.036 | −0.063 | −0.0279 | −0.2476 | 0.3355 | 0.0158 | 0.0416 | 1 | 8.722 × 10−11 | 3.240 × 10−12 | 1 | 3 |
01817 | 12.917 | 0.070 | −2.113 | 0.310 | 0.492 | 0.303 | 0.016 | 0.064 | −0.480 | 0.053 | −0.059 | −0.0256 | −0.2526 | 0.3286 | 0.0336 | 0.0427 | 1 | −1.138 × 10−10 | 3.731 × 10−11 | 1 | 3 |
01954 | 13.864 | 0.282 | −1.507 | 0.194 | 0.557 | 0.184 | −0.002 | 0.040 | −0.699 | 0.033 | −0.074 | −0.0589 | −0.3472 | 0.2485 | 0.0481 | 0.0547 | 2 | 2.991 × 10−10 | 9.175 × 10−11 | 1 | 3 |
01959 | 14.222 | 0.203 | −1.018 | 0.221 | 0.668 | 0.206 | 0.092 | 0.045 | −0.627 | 0.038 | −0.124 | −0.1782 | −0.3704 | 0.2177 | 0.1467 | 0.0423 | 2 | 6.636 × 10−11 | 2.444 × 10−11 | 3 | 1 |
02019 | 14.226 | 0.272 | −1.010 | 0.198 | 0.670 | 0.184 | 0.157 | 0.041 | −0.482 | 0.034 | −0.110 | −0.1805 | −0.3719 | 0.1989 | 0.1409 | 0.0698 | 1 | −2.651 × 10−11 | 2.995 × 10−11 | 3 | 2 |
02050 | 14.455 | 0.264 | −1.120 | 0.173 | 0.641 | 0.162 | 0.202 | 0.035 | −0.346 | 0.029 | −0.064 | −0.0948 | −0.2681 | 0.2848 | 0.0595 | 0.0674 | 1 | −6.851 × 10−11 | 1.861 × 10−11 | 2 | 3 |
02060 | 14.173 | 0.332 | −1.400 | 0.178 | 0.577 | 0.168 | 0.048 | 0.036 | −0.616 | 0.030 | −0.079 | −0.1299 | −0.2956 | 0.2422 | 0.1287 | 0.0856 | 2 | 2.627 × 10−12 | 2.042 × 10−11 | 2 | 3 |
02062 | 14.183 | 0.317 | −1.489 | 0.175 | 0.560 | 0.166 | 0.041 | 0.036 | −0.605 | 0.030 | −0.065 | −0.0970 | −0.2774 | 0.2851 | 0.0386 | 0.0737 | 2 | −3.015 × 10−10 | 7.012 × 10−11 | 2 | 4 |
02083 | 14.309 | 0.191 | −1.022 | 0.235 | 0.667 | 0.219 | 0.141 | 0.048 | −0.513 | 0.040 | −0.141 | −0.1276 | −0.3976 | 0.2195 | 0.0972 | 0.0286 | 1 | 2.851 × 10−11 | 4.972 × 10−11 | 1 | 1 |
02105 | 13.838 | 0.350 | −1.264 | 0.203 | 0.606 | 0.191 | 0.089 | 0.042 | −0.560 | 0.035 | −0.072 | −0.0718 | −0.3360 | 0.2523 | 0.0354 | 0.0553 | 2 | 1.438 × 10−10 | 3.503 × 10−11 | 1 | 4 |
02138 | 14.174 | 0.231 | −1.105 | 0.229 | 0.644 | 0.214 | 0.051 | 0.047 | −0.694 | 0.039 | −0.125 | −0.1782 | −0.3870 | 0.1968 | 0.1681 | 0.0388 | 2 | 9.229 × 10−11 | 2.954 × 10−11 | 4 | 1 |
02150 | 14.537 | 0.139 | −1.183 | 0.262 | 0.625 | 0.246 | 0.048 | 0.054 | −0.679 | 0.045 | −0.158 | −0.0809 | −0.4253 | 0.2269 | 0.0460 | 0.0134 | 1 | −4.280 × 10−10 | 3.396 × 10−10 | 1 | 1 |
02185 | 14.162 | 0.190 | −1.131 | 0.219 | 0.638 | 0.205 | 0.082 | 0.045 | −0.617 | 0.037 | −0.126 | −0.1740 | −0.3871 | 0.1824 | 0.1262 | 0.0407 | 1 | 1.214 × 10−10 | 2.147 × 10−10 | 3 | 1 |
02218 | 14.554 | 0.400 | −1.042 | 0.201 | 0.661 | 0.188 | 0.287 | 0.041 | −0.176 | 0.034 | −0.061 | −0.0300 | −0.2219 | 0.3634 | 0.0239 | 0.0509 | 1 | −1.232 × 10−10 | 1.114 × 10−11 | 1 | 3 |
02238 | 13.952 | 0.276 | −1.542 | 0.239 | 0.551 | 0.227 | −0.096 | 0.049 | −0.902 | 0.041 | −0.091 | −0.1551 | −0.3564 | 0.2361 | 0.1206 | 0.0322 | 2 | −1.937 × 10−11 | 7.667 × 10−11 | 2 | 1 |
02260 | 14.425 | 0.335 | −1.052 | 0.177 | 0.659 | 0.165 | 0.230 | 0.036 | −0.302 | 0.030 | −0.066 | −0.0387 | −0.2552 | 0.3064 | 0.0373 | 0.0621 | 1 | −1.422 × 10−10 | 2.779 × 10−11 | 1 | 3 |
02288 | 14.330 | 0.304 | −1.086 | 0.170 | 0.649 | 0.159 | 0.171 | 0.035 | −0.426 | 0.029 | −0.070 | −0.1274 | −0.2916 | 0.2523 | 0.1003 | 0.0719 | 1 | −1.222 × 10−10 | 2.383 × 10−11 | 2 | 3 |
02290 | 14.397 | 0.253 | −1.055 | 0.211 | 0.658 | 0.197 | 0.126 | 0.043 | −0.539 | 0.036 | −0.119 | −0.1581 | −0.3639 | 0.2092 | 0.1358 | 0.0518 | 1 | 7.020 × 10−11 | 1.902 × 10−11 | 3 | 2 |
02357 | 13.774 | 0.285 | −1.486 | 0.193 | 0.561 | 0.183 | −0.013 | 0.040 | −0.730 | 0.033 | −0.084 | −0.1392 | −0.3261 | 0.2433 | 0.1410 | 0.0644 | 2 | −6.056 × 10−10 | 1.342 × 10−10 | 2 | 3 |
02418 | 14.378 | 0.254 | −1.088 | 0.177 | 0.649 | 0.165 | 0.143 | 0.036 | −0.489 | 0.030 | −0.079 | −0.1621 | −0.3217 | 0.2221 | 0.1428 | 0.0627 | 1 | 3.791 × 10−12 | 1.494 × 10−11 | 2 | 3 |
02590 | 14.259 | 0.298 | −1.105 | 0.170 | 0.644 | 0.159 | 0.196 | 0.035 | −0.363 | 0.029 | −0.064 | −0.1247 | −0.2811 | 0.2661 | 0.0930 | 0.0719 | 1 | 2.301 × 10−9 | 3.606 × 10−10 | 2 | 4 |
02687 | 14.693 | 0.289 | −1.125 | 0.173 | 0.639 | 0.162 | 0.176 | 0.035 | −0.404 | 0.029 | −0.073 | −0.1481 | −0.2995 | 0.2384 | 0.1325 | 0.0832 | 1 | 2.037 × 10−10 | 1.022 × 10−11 | 2 | 3 |
02814 | 14.168 | 0.252 | −1.104 | 0.191 | 0.645 | 0.179 | 0.120 | 0.039 | −0.538 | 0.032 | −0.100 | −0.1645 | −0.3501 | 0.2269 | 0.1570 | 0.0644 | 1 | 5.179 × 10−11 | 2.704 × 10−11 | 3 | 2 |
… | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … | … |
Notes. The first column contains identification names for individual stars in the form of OGLE-BLG-RRLYR-ID. Columns 2 and 3 list the mean apparent magnitudes and amplitudes, respectively, in the Ks -band from the VVV photometric survey (Minniti et al. 2010). Columns 4 and 5 contain metallicity estimates and their errors calculated from the I band light curves. Columns 6–11 contain absolute magnitudes and their errors for the studied stars in the V, I, and Ks -bands, respectively. The approximate centers of the humps and bumps are listed in Cols. 12–17 contain the determined sizes of both shocks in the phased light curves. Column 18 lists the association with the Oosterhoff groups (1 – Oo I, 2 – Oo II). Columns 19 and 20 contain the parameter a2 and its error used to estimate the period change rate of the studied stars. The last two Cols. 21 and 22 list the categories 1–4 from the visual classification of the humps and bumps. The full table is available at the CDS.
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