Environmental history of filament galaxies - Stellar mass assembly and star formation of filament galaxies

Open Access

Fig. 4.

Pie charts showing the fraction of galaxies inside filaments at z = 0 separated by their environmental history and mass for GAEA (top) and TNG100 (bottom). The fraction p and standard error ( $S E = \sqrt{\frac{p \cdot (1 - p)}{n}}$ $Mathematical equation: $ SE = \sqrt{\frac{p \cdot (1 - p)}{n}} $$ ) are indicated in each segment.

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