Fig. 5.
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M⋆–Z (top) and M⋆–SFR (bottom) relations, using the Pettini & Pagel (2004) and Hopkins et al. (2003) calibrations respectively. The galaxies in filaments (left), tendrils galaxies (centre), and voids (right) are marked as red points alongside their corresponding control samples in blue. All SF galaxies are represented in the background as a black density scatter plot. The dashed lines represent the linear regressions calculated by the Bayesian method for each galaxy type (in red) and its corresponding control sample (in blue). Error bars are the median errors of the axes calculated using Monte Carlo propagation.
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