Distance to MATLAS-2019. The left panel shows the different estimates where the R_e,GC is obtained assuming that the GC intrinsic profile follows a Gaussian model, while the right panel assumes a King model. Each of the points shows a different method or calibration used to estimate the distance to MATLAS-2019 as labelled. The grey box separates the distances obtained in Müller et al. (2021) and in Danieli et al. (2022). The (*) indicates the distance assumed in Danieli et al. (2022) based on the distance to the NGC5846 group. In the red box, we plot the weighted mean distance obtained using the different estimates for the GCLF and R_e,GC methods.