3 papers
astro-ph.SR2026
Introducing PxP: A Population Synthesis Framework for Predicting YSO Properties
J. Peltonen, E. Rosolowsky, A Ginsburg +3
The most direct method of measuring the star formation rate is with young stellar objects (YSOs), but this requires high-resolution observations and high-quality models. Using the…
astro-ph.CO2025
Euclid: Systematic uncertainties from the halo mass conversion on galaxy cluster number count data analyses
T. Gayoux, P. -S. Corasaniti, T. R. G. Richardson +153
The large catalogues of galaxy clusters expected from the Euclid survey will enable cosmological analyses of cluster number counts that require accurate cosmological model predicti…
astro-ph.CO2025
The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
P. S. Corasaniti, T. R. G. Richardson, S. Ettori +7
Measurements of the sparsity of galaxy clusters can be used to probe the cosmological information encoded in the host dark matter halo profile, and infer constraints on the cosmolo…