Late-type galaxies dominate shape-shape alignments in the filaments of the Perseus-Pisces supercluster while early-types cluster near dense centers, indicating distinct tidal mechanisms out to 1 Mpc/h.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
-
Dissecting the Perseus-Pisces supercluster observed with CFHT-MegaCam: Exploring late-type galaxy shape alignments within the local cosmic web
Late-type galaxies dominate shape-shape alignments in the filaments of the Perseus-Pisces supercluster while early-types cluster near dense centers, indicating distinct tidal mechanisms out to 1 Mpc/h.
-
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.