Table E.1.
Uncertainties included in TRGB calibration and LMC or SMC distances.
| Uncertainties related to | Considered elements | σ [mag] |
|---|---|---|
| Milky Way GC TRGB calibration; see Table 1 | ![]() |
|
| GC distances | †Covariant GC distance uncertainties from Lengen et al. (2026), which include: | ![]() |
| a) GC parallax uncertainties (Cruz Reyes et al. 2024) with | ||
| Individual parallax uncertainties (Lindegren et al. 2021b) | ||
| Parallax zero-point corrections (Lindegren et al. 2021a) | ||
| Angular covariance of GDR3 parallaxes (Maíz Apellániz et al. 2021) | ||
| Corrected GDR3 parallax uncertainties (Maíz Apellániz et al. 2021) | ||
| b) Photometric uncertainties (Clementini et al. 2023; Ripepi et al. 2023) | ||
| c) Intrinsic scatter of the period–luminosity relation | ||
| d) Metallicity dependence of PL relations | ||
| e) Model-fitting uncertainties | ||
| Photometry | photometric quality cuts applied; see Sect. 2 | |
| †bootstrap resampling in absolute magnitude space; see Appendix E |
![]() |
|
| Extinction | Uncertainties of E(B − V) and consistency in the recent literature | |
| RV differences for GCs not found to be significant in literature | ||
| Range of AI/E(B − V) yields only minor differences due to low average E(B − V) | ||
| mTRGB from Table 3 in KA24 | ||
| smoothing bias, Sobel filter response, extinction, metallicity, among others | ||
| LMC uncertainty on GRP, 0 for SARGs | 0.009 | |
| SMC uncertainty on GRP, 0 for SARGs | 0.035 | |
| TRGB-based distance modulus | MW GC TRGB calibration in RP band (joint stat. & syst.) | |
| mTRGB (joint stat. & syst.) | ||
| homogeneous space-based GDR3 RP-band observations in GCs and LMC/SMC | ||
| identical TRGB measurement process (unweighted Sobel, smoothing insensitivity) | ||
| colour-based metallicity corrections: remains within 1σ | ||
Notes. Statistical and systematic uncertainties are considered jointly in this analysis. The table provides an overview of the most significant elements with references for more information. † indicates items treated simultaneously to determine the uncertainties reported above (see Appendix E). Numbers reported in column σ must be considered for information only and were derived by running the analysis separately considering only the distance covariance matrix or bootstrap resampling. NB: the final calibration is based on a single joint inference that simultaneously incorporates both approaches. Its asymmetric uncertainties can thus not be exactly reproduced by a summing the values reported here in quadrature.
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