Fig. 4.

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Cumulative distribution of the ex situ IGL fraction in our group sample at z = 0, measured across all three orthogonal projections. IGL particles along the LOS passing through galaxies are excluded, resulting in a slight underestimation of the IGL fraction and mass; this introduces a mild variation in the assessment of this component from different viewing angles. See Table 1 for the location and scale parameters of the corresponding PDFs.
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