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 H orizon-(no)AGN and Simba. We find that more massive galaxies are more connected, in...
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2020 (v1)Journal articleThe impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodesUploaded on: December 3, 2022
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2022 (v1)Journal article
The upcoming WEAVE-QSO survey will target a high density of quasars over a large area, enabling the reconstruction of the 3D density field through Lyman-α (Ly-α) tomography over unprecedented volumes smoothed on intermediate cosmological scales (≈ 16 Mpc h^−1). We produce mocks of the Ly-α forest using Ly-α Mass Association Scheme, and...
Uploaded on: February 22, 2023