Fig. 2.
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Three-dimensional visualization of the five cosmic environments used in our analysis: galaxy clusters (red), cluster outskirts (blue), filaments (yellow), filaments outskirts (brown). Groups are shown as transparent magenta spheres, with radii equal to 3 times the R200 of each halo. Galaxies classified as filaments lie within 1 h−1 Mpc of the filament axis, while those in filament outskirts lie between 1 and 2 h−1 Mpc. This figure was generated using our SDSS DR18 dataset and environment classification scheme.
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