Table A.4
Table for 34 RRab type variables with the lowest Amplos located at the nonlinear part of the amplitude scaling relation. The first column contains the Gaia identifier. The following three columns contain the photometric and line-of-sight velocity amplitudes and the pulsation periods of a given variable. The last column contains the photometric metallicities listed in the Gaia RR Lyrae catalog (Clementini et al. 2023).
| source_id | AmpG [mag] | Amplos [km s−1] | P [day] | [Fe/H]phot [dex] |
|---|---|---|---|---|
| 3181149548774349824 | 0.395 ± 0.004 | 34.8 ± 5.0 | 0.64004 | −0.73 ± 0.23 |
| 3478166191064353920 | 0.312 ± 0.003 | 41.1 ± 5.6 | 0.64333 | −0.21 ± 0.24 |
| 4957668453282872448 | 0.179 ± 0.002 | 24.8 ± 3.3 | 0.71747 | 0.31 ± 0.27 |
| 4793950312913699328 | 0.376 ± 0.016 | 43.0 ± 10.0 | 0.61026 | −0.21 ± 0.28 |
| 5222811627876331648 | 0.316 ± 0.004 | 48.8 ± 8.9 | 0.61568 | −0.47 ± 0.28 |
| 1326205915830514176 | 0.137 ± 0.002 | 15.2 ± 5.5 | 0.61565 | − |
| 6164530246002222208 | 0.394 ± 0.008 | 44.5 ± 4.6 | 0.62509 | −0.77 ± 0.24 |
| 3959667827791428224 | 0.292 ± 0.003 | 42.0 ± 9.9 | 0.62838 | −0.30 ± 0.22 |
| 2198888054289887232 | 0.177 ± 0.002 | 20.5 ± 5.1 | 0.44949 | 0.07 ± 0.22 |
| 4387211137548084352 | 0.395 ± 0.008 | 43.2 ± 5.7 | 0.73768 | −0.38 ± 0.25 |
| 4137503800563739136 | 0.234 ± 0.006 | 31.4 ± 7.8 | 0.60553 | − |
| 1677592858356166528 | 0.262 ± 0.006 | 33.7 ± 3.5 | 0.80726 | − |
| 1954728333254872576 | 0.221 ± 0.002 | 27.1 ± 1.2 | 0.67400 | 0.33 ± 0.22 |
| 5810405553887250432 | 0.356 ± 0.005 | 37.0 ± 3.4 | 0.84691 | −0.07 ± 0.25 |
| 6409095201484462208 | 0.149 ± 0.002 | 23.5 ± 3.9 | 0.80212 | − |
| 4984655725669340544 | 0.361 ± 0.005 | 55.3 ± 6.9 | 0.61560 | −0.54 ± 0.23 |
| 1978708686175347968 | 0.214 ± 0.001 | 31.6 ± 2.2 | 0.64911 | −0.16 ± 0.22 |
| 4702297875480363648 | 0.331 ± 0.008 | 40.2 ± 1.6 | 0.72796 | −0.26 ± 0.30 |
| 3504228735513593600 | 0.203 ± 0.002 | 25.0 ± 8.0 | 0.65251 | −0.39 ± 0.28 |
| 5459760747346789888 | 0.168 ± 0.003 | 26.0 ± 4.0 | 0.69682 | 0.31 ± 0.32 |
| 5996105366938238336 | 0.321 ± 0.054 | 44.9 ± 11.1 | 0.58204 | − |
| 6151860053822639104 | 0.361 ± 0.007 | 39.7 ± 1.1 | 0.63780 | −0.78 ± 0.30 |
| 5993797084032636928 | 0.189 ± 0.008 | 17.7 ± 0.4 | 0.41930 | − |
| 4439524212872324736 | 0.183 ± 0.002 | 25.1 ± 3.5 | 0.64206 | −0.37 ± 0.26 |
| 4605376543969500160 | 0.333 ± 0.018 | 39.4 ± 8.8 | 0.58604 | −0.43 ± 0.35 |
| 6248312516647094528 | 0.179 ± 0.010 | 22.5 ± 2.4 | 0.58327 | − |
| 538832101445230720 | 0.194 ± 0.003 | 26.8 ± 1.0 | 0.64960 | −0.10 ± 0.26 |
| 2869411785820130304 | 0.316 ± 0.013 | 49.4 ± 8.1 | 0.69608 | 0.26 ± 0.30 |
| 6019142407624043136 | 0.356 ± 0.006 | 44.6 ± 10.3 | 0.47148 | 0.04 ± 0.22 |
| 6529376963198996352 | 0.326 ± 0.006 | 37.2 ± 7.7 | 0.89489 | 0.48 ± 0.45 |
| 1546016672688675200 | 0.365 ± 0.006 | 41.2 ± 0.6 | 0.59958 | −0.08 ± 0.22 |
| 1223679342759114752 | 0.365 ± 0.006 | 48.0 ± 3.8 | 0.76900 | −0.06 ± 0.29 |
| 5639451149541847552 | 0.360 ± 0.012 | 47.2 ± 8.9 | 0.73313 | − |
| 4136943255792306304 | 0.230 ± 0.004 | 29.8 ± 2.0 | 0.59972 | 0.09 ± 0.23 |
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