Fig. 5.
Top panel: median luminosity (in units of 1010 h−2 L⊙), in logarithmic scale, of the host filaments of E–E, E–S, and S–S pairs; aligned pairs (empty circles) and perpendicular pairs (filled triangles). Bottom panel: as in top panel but for the median of the number of galaxies. All the uncertainties were derived through a bootstrap resampling technique (Barrow et al. 1984).
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