Galaxy structure depends on environment at fixed stellar mass at >5σ, secondary to mass, with cluster-only effects at z<0.5 and multi-scale effects for massive systems at z≥0.5.
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3 Pith papers cite this work, alongside 106 external citations. Polarity classification is still indexing.
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Pith papers citing it
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representative citing papers
Galaxy properties in IllustrisTNG form a continuum across the multiscale caustic skeleton, with formation time of web components influencing colors and star formation activity.
Satellite abundance is higher in filaments than the field by factors of 1.9-3.5, but reduced up to 79% after halo mass matching and further suppressed by dark matter tracer choice in IllustrisTNG.
citing papers explorer
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Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
Galaxy structure depends on environment at fixed stellar mass at >5σ, secondary to mass, with cluster-only effects at z<0.5 and multi-scale effects for massive systems at z≥0.5.
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Galaxy Populations in the IllustrisTNG Caustic Skeleton
Galaxy properties in IllustrisTNG form a continuum across the multiscale caustic skeleton, with formation time of web components influencing colors and star formation activity.
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The impact of cosmic filaments on the abundance of satellite galaxies
Satellite abundance is higher in filaments than the field by factors of 1.9-3.5, but reduced up to 79% after halo mass matching and further suppressed by dark matter tracer choice in IllustrisTNG.