Filamentary regions of the cosmic web are the primary contributors to the residual large-scale conformity signal of low-mass central galaxies in both SAG and TNG300.
Star formation quenching in the infall region around galaxy clusters
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The role of filaments in the large-scale conformity signal
Filamentary regions of the cosmic web are the primary contributors to the residual large-scale conformity signal of low-mass central galaxies in both SAG and TNG300.