Table 1.
Distance moduli for tested stellar systems using derived PMZ relations.
| Band | μNGC 6121 | μNGC 5139 | μLMC | μSMC |
|---|---|---|---|---|
| [mag] | [mag] | [mag] | [mag] | |
| GBP | 11.00 ± 0.13 | 13.61 ± 0.13 | 18.45 ± 0.16 | 18.97 ± 0.20 |
| V | 11.25 ± 0.16 | 13.54 ± 0.10 | 18.43 ± 0.14 | 19.02 ± 0.18 |
| G | 11.12 ± 0.11 | 13.57 ± 0.09 | 18.49 ± 0.13 | 19.02 ± 0.17 |
| GRP | 11.17 ± 0.08 | 13.61 ± 0.14 | 18.48 ± 0.13 | 18.90 ± 0.17 |
| I | 11.26 ± 0.11 | 13.55 ± 0.08 | 18.45 ± 0.12 | 18.91 ± 0.16 |
| J | 11.24 ± 0.06 | 13.63 ± 0.05 | 18.44 ± 0.17 | – |
| H | 11.16 ± 0.07 | 13.58 ± 0.05 | – | – |
| Ks | 11.27 ± 0.04 | 13.65 ± 0.04 | 18.50 ± 0.13 | 19.08 ± 0.19 |
| Lit. | 11.28 ± 0.04 | 13.58 ± 0.10 | 18.48 ± 0.02 | 18.98 ± 0.03 |
Notes. The first column contains the source for calculated distance moduli (passbands and literature value). The second and third columns represent the distance moduli of two globular clusters, NGC 6121 and NGC 5139. The last two columns list distance moduli for Magellanic Clouds.
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