collaborators

5 papers

astro-ph.CO2026

Baryonification III: An accurate analytical model for the dispersion measure probability density function of fast radio bursts

MohammadReza Torkamani, Robert Reischke, Michael Kovač +6

We develop an analytical framework to predict the one-point probability distribution function (PDF) of dispersion measures (DMs) for fast radio bursts (FRBs) within the baryonifica…

astro-ph.CO2026

Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys

Joël Mayor, Marta Spinelli, Gabriella De Lucia +5

Upcoming galaxy surveys with the SKA Observatory will detect neutral hydrogen (HI) across unprecedented volumes, and their scientific return will crucially depend on predictive mod…

astro-ph.CO2025

The cosmological analysis of DES 32pt data from the Effective Field Theory of Large-Scale Structure

Guido D'Amico, Alexandre Refregier, Leonardo Senatore +1

We analyze the Dark Energy Survey (DES) Year 3 data using predictions from the Effective Field Theory of Large-Scale Structure (EFTofLSS). Specifically, we fit three two-point obse…

astro-ph.CO2025

Multiprobe constraints on early and late time dark energy

Alexander Reeves, Simone Ferraro, Andrina Nicola +1

We perform a multiprobe analysis combining cosmic microwave background (CMB) data from Planck and the Atacama Cosmology Telescope (ACT), ACT CMB lensing, and large-scale structure…

astro-ph.GA2025

ProMage: fast galaxy magnitudes emulation combining SED forward-modelling and machine learning

Luca Tortorelli, Silvan Fischbacher, Aaron S. G. Robotham +2

We present ProMage, a feed-forward neural network that emulates the computation of observer- and rest-frame magnitudes from the generative galaxy SED package ProSpect. The network…