collaborators

5 papers

astro-ph.GA2026

Galaxy luminosity functions from far-UV to submillimetre at in the COLIBRE simulations

Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey +15

We present predictions from the recent COLIBRE cosmological hydrodynamical simulations of galaxy formation for the present-day galaxy luminosity functions (LFs) at wavelengths rang…

astro-ph.CO2026

Fast radio burst dispersion is an unbiased tracer of matter on large scales

Shion Andrew, Haochen Wang, Kiyoshi Masui +6

The dispersion of fast radio bursts (FRBs) measures the column density of free electrons, tracing the diffuse ionized gas that contains more than of all baryons. On linear s…

astro-ph.CO2026

Intrinsic alignments in the FLAMINGO simulations with two-point statistics

A. Herle, N. E. Chisari, H. Hoekstra +3

Intrinsic alignments are a major astrophysical contaminant for next generation large-sky surveys like Euclid and LSST. Large hydrodynamic simulations are crucial for informing the…

astro-ph.CO2025

Euclid: An emulator for baryonic effects on the matter bispectrum

P. A. Burger, G. Aricò, L. Linke +153

Understanding the impact of baryonic processes such as star formation and active galactic nuclei (AGN) feedback on matter clustering is crucial to ensure precise and unbiased cosmo…

astro-ph.CO2025

Unbiased estimates of the shapes of haloes using the positions of satellite galaxies

A. Herle, N. E. Chisari, H. Hoekstra +4

The shapes of dark matter haloes are sensitive to both cosmology and baryon physics, but are difficult to measure observationally. A promising way to constrain them is to use the p…