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Fig. 6.


Distances to AMASCFI clusters along filaments of passive galaxies (red) and star-forming galaxies (blue) at low redshift 0.15 <  z ≤ 0.4 (left) and high redshift 0.4 <  z <  0.7 (right) for absolute magnitude-matched samples. The top distribution is the PDF of the distances to the skeleton. The filled areas around the curves represent the 68% confidence limits computed from 1000 bootstrap re-samplings of the distribution. The vertical lines and associated error bars are the median and error on the median of each distribution. The bottom panel shows the CDF.

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