activity
20202026
most citedQuantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations

7 citations · 8 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2026

A high-dynamic-range view of the growth of structure and the warm/hot Universe

Luca Di Mascolo, Tony Mroczkowski, Joshiwa van Marrewijk +23

Baryons heat to temperatures above as they accrete onto massive overdensities -- galaxies, groups, clusters, and filaments -- where they ionize and become o…

astro-ph.IM2025★ 1 cited

The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope

The Simons Observatory Collaboration, M. Abitbol, I. Abril-Cabezas +419

We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large A…

astro-ph.CO2024

cosmocnc: A fast, flexible, and accurate galaxy cluster number count likelihood code for cosmology

Íñigo Zubeldia, Boris Bolliet

We introduce cosmocnc, a Python package for computing the number count likelihood of galaxy cluster catalogues in a fast, flexible and accurate way. cosmocnc offers three types of…

astro-ph.IM2023

class_sz I: Overview

B. Bolliet, A. Kusiak, F. McCarthy +16

class_sz is a versatile and robust code in C and Python that can compute theoretical predictions for a wide range of observables relevant to cross-survey science in the Stage IV er…

astro-ph.CO2020★ 7 cited

Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations

Íñigo Zubeldia, Anthony Challinor

CMB lensing is a promising, novel way to measure galaxy cluster masses that can be used, e.g., for mass calibration in galaxy cluster counts analyses. Understanding the statistics…