Group-scale halos produce a dual effect on infalling galaxies: pre-processing raises quiescent fraction early, while protection delays cluster-driven quenching to smaller d_R.
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IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
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The dual effect of group-scale environments on galaxy quenching during cluster infall: pre-processing and protection
Group-scale halos produce a dual effect on infalling galaxies: pre-processing raises quiescent fraction early, while protection delays cluster-driven quenching to smaller d_R.
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Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.