The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
We investigate the impact of the number of filaments connected to the nodes of the cosmic web on the physical properties of their galaxies using the Sloan Digital Sky Survey. We compare these measurements to the cosmological hydrodynamical simulations Horizon-(no)AGN and Simba. We find that more mas...
Prif Awduron: | Kraljic, K, Pichon, C, Codis, S, Laigle, C, Davé, R, Dubois, Y, Hwang, HS, Pogosyan, D, Arnouts, S, Devriendt, J, Musso, M, Peirani, S, Slyz, A, Treyer, M |
---|---|
Fformat: | Journal article |
Iaith: | English |
Cyhoeddwyd: |
Oxford University Press
2019
|
Eitemau Tebyg
-
Connecting the cosmic web to the spin of dark halos: implications for
galaxy formation
gan: Codis, S, et al.
Cyhoeddwyd: (2012) -
Galaxy evolution in the metric of the Cosmic Web
gan: Kraljic, K, et al.
Cyhoeddwyd: (2017) -
How the cosmic web induces intrinsic alignments of galaxies
gan: Codis, S, et al.
Cyhoeddwyd: (2016) -
Intrinsic alignment of simulated galaxies in the cosmic web: implications for weak lensing surveys
gan: Codis, S, et al.
Cyhoeddwyd: (2015) -
The Horizon-AGN simulation: evolution of galaxy properties over cosmic time
gan: Kaviraj, S, et al.
Cyhoeddwyd: (2017)