Table B.8.
Data for the RRLs in GGCs.
| source_id | Name | Var | In-situ/Acc. | Prog. | RA | Dec | Period | Amp(G) | [Fe/H] |
|---|---|---|---|---|---|---|---|---|---|
| [deg] | [deg] | [days] | [mag] | dex | |||||
| 2957940029686151168 | NGC1904 | V4 | 0 | H99 | 81.0741 | -24.5379 | 0.634 | 0.776 ± 0.059 | -1.60 |
| 2957940854319418752 | NGC1904 | V13 | 0 | H99 | 81.0442 | -24.5199 | 0.689 | 0.721 ± 0.069 | -1.60 |
| 3641359275974954496 | NGC5634 | V2 | 0 | H99 | 217.3986 | -5.9541 | 0.605 | 1.298 ± 0.197 | -1.88 |
| 3641359177190278528 | NGC5634 | V3 | 0 | H99 | 217.3929 | -5.9654 | 0.601 | 0.828 ± 0.106 | -1.88 |
| 4126218000877730048 | NGC6235 | V1 | 1 | G-E | 253.3511 | -22.1666 | 0.616 | 0.905 ± 0.031 | -1.28 |
Notes. source_id, Period and Amp(G) are from Gaia DR3 (Clementini et al. 2023); Name and Var are the names of the GGC hosting the RRLs and the RRL identification according to Clement et al. (2001); classification of the GGCs according to Belokurov & Kravtsov (2024): in situ = 1 accreted = 0; classification of GGCs according to Callingham et al. (2022), the meaning of the acronyms is explained in Table B.5; RA and Dec are given at J2016 from Gaia DR3; [Fe/H] is from Harris (1996). Only a portion of the table is listed here to guide the reader about its content. A machine-readable version of the full table is published at the CDS (Centre de Données astronomiques de Strasbourg, https://cds.u-strasbg.fr/
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