Notes. Columns: (1) galaxy names and the associated references for their GC system data, (2) integrated V-band absolute magnitudes (M_V), (3) total probability ratio in the depleted region ${\tilde{\text{P}}}_{\text{DEP}}$ total probability ratio in the outer region ${\tilde{\text{P}}}_{\text{OUT}}$ mean nearest neighbor distance ratio in the depleted region ${\text{N}}_{\tilde{\text{N}}}$ mean nearest neighbor distance ratio in the outer region ${\text{N}}_{\tilde{\text{N}}}$ p-value from the Kolmogorov-Smirnov (K-S) test for the inner regions (p_KS−DEP), (8) p-value from the K-S test for the outer regions (p_KS−OUT), (9) p-value from the chi-square test in the depleted region $\left(p_{{\chi }^2}\right)$ Poisson probability for the depleted region (p_Poisson), and (11) mean depopulation radius (R_DEP) with its standard deviation, obtained from 1000 CDF resampling.

References: ⁽¹⁾ Brüns & Kroupa (2012); ⁽²⁾ Ma et al. (2013); ⁽³⁾ Bland-Hawthorn & Gerhard (2016); ⁽⁴⁾ Kruijssen et al. (2019); ⁽⁵⁾ Baumgardt et al. (2019); ⁽⁶⁾ de Vaucouleurs et al. (1991); ⁽⁷⁾ Komiyama et al. (2018); ⁽⁸⁾ Galleti et al. (2004); ⁽⁹⁾ Harris (2023); ⁽¹⁰⁾ Crnojević et al. (2016); ⁽¹¹⁾ Beasley et al. (2008); ⁽¹²⁾ Woodley et al. (2007); ⁽¹³⁾ Alves-Brito et al. (2011); ⁽¹⁴⁾ Hartman et al. (2023). ^(a) For the Milky Way (MW) analysis, the semi-major axis measurements of GCs were employed instead of R_g.