Table A.1
Parameters of the 4933 RRLs in the reference sample.
| source_id | RA | Dec. | pmra | pmdec | Lz | E | L⊥ | ecc | [Fe/H] | σ[Fe/H] | Substructure |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 5930541561668628736 | 249.1970 | −54.2037 | −17.171 | −14.857 | −745 | −177885 | 344 | 0.59 | −2.11 | 0.42 | Thamnos |
| 6471410229148825088 | 310.1242 | −53.2819 | −7.662 | −28.896 | −1789 | −133202 | 821 | 0.56 | −1.75 | 0.42 | Sequoia |
| 34113623857898880 | 44.5915 | 15.6717 | 1.760 | −37.565 | 98 | −135829 | 26 | 0.98 | −1.64 | 0.44 | GSE |
| 1193183528770580224 | 238.6171 | 15.3561 | −17.853 | 1.871 | −252 | −154345 | 210 | 0.91 | −1.49 | 0.44 | GSE |
| 1196737700107586176 | 238.3152 | 17.5699 | −11.729 | −4.870 | −533 | −179584 | 361 | 0.59 | −1.88 | 0.41 | Thamnos |
| 2098060604631085952 | 279.6238 | 39.5011 | −1.520 | −5.618 | 291 | −180257 | 503 | 0.84 | −1.65 | 0.35 | L-RL3 |
| 5768557209320424320 | 248.1040 | −83.9035 | −58.488 | −120.550 | −218 | −160786 | 789 | 0.91 | −1.97 | 0.50 | GSE |
| 702294777158642688 | 139.9645 | 33.8732 | −3.352 | −12.630 | 226 | −160275 | 272 | 0.87 | −1.50 | 0.41 | GSE |
| 2538463596221422976 | 18.4185 | 2.1610 | 7.466 | −11.608 | −262 | −167128 | 211 | 0.85 | −1.30 | 0.35 | GSE |
| 5783102618581820672 | 192.5538 | −81.9544 | 9.371 | 1.509 | −64 | −140426 | 722 | 0.95 | −1.63 | 0.40 | GSE |
Notes. Column (1) Gaia DR3 source_id; (2) and (3) Coordinates; (4) and (5) Proper motions; (6) Angular momentum along the Z-axis; (7) Total energy; (8) Component of angular momentum perpendicular to Lz; (9) Eccentricity; (10) and (11) Photometric metallicities and their corresponding uncertainties; (12) The sub-structure to which the star is assigned by the CLiMB algorithm. Columns (1)-(5) are taken from the Gaia DR3 gaia_source table (Gaia Collaboration 2023b). Columns (6)-(9) and (12) are calculated in this study. Columns (10) and (11) are from Muraveva et al. (2025). The full table is published at the CDS; a portion is shown here to illustrate its form and content.
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