collaborators

30 papers

astro-ph.CO2026

Characterising the epoch of reionisation using the cross-correlation of the kSZ effect and CMB lensing

Niall MacCrann, Christopher Cain, Aleksandra Kusiak +5

We investigate the cross-correlation of the kinematic Sunyaev-Zeldovich (kSZ) effect with lensing of the cosmic microwave background (CMB) as a probe of the epoch of reionisation.…

astro-ph.CO2026

Evidence for a thermal pressure deficit in galaxy groups from the tSZ effect and weak lensing

Jared Siegel, Alexandra Amon, Jenny E. Greene +3

Measurements of the thermal Sunyaev-Zel'dovich (tSZ) effect have yet to form a consistent picture of the thermodynamic state of the gas in the intracluster medium: their interpreta…

astro-ph.CO2026

Baryons in the Darkest Sites of the Universe

Kritti Sharma, Vikram Ravi, Dhayaa Anbajagane +9

The pristine underdense patches of the Universe, cosmic voids, are powerful cosmological laboratories, uniquely sensitive to dark energy, modified gravity, and neutrino masses, yet…

astro-ph.CO2026

Self-consistent secondary cosmic microwave background anisotropies and extragalactic foregrounds in the FLAMINGO simulations

Tianyi Yang, Ian G. McCarthy, Fiona McCarthy +6

Secondary anisotropies in the cosmic microwave background (CMB) contain information that can be used to test both cosmological models and models of galaxy formation. Starting from…

astro-ph.CO2026

Field-Level Inference of Primordial Non-Gaussianity with the Quijote Simulation Suite

Adam Andrews, Jens Jasche, Guilhem Lavaux +10

Local primordial non-Gaussianity, parameterised as , will be stringently constrained using state-of-the-art methods applied to next-generation galaxy redshi…

astro-ph.CO2026

A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations

A. Baleato Lizancos, W. Coulton, A. Challinor +2

CMB lensing reconstructions are a sensitive probe of the growth of structure across cosmic time and a key tool to sharpen investigations of the very early Universe via delensing. A…