activity
20242026
collaborators

5 papers

astro-ph.CO2026

meer21cm: an Analysis Pipeline and Comprehensive Toolkit for HI Intensity Mapping

Zhaoting Chen, Steven Cunnington, Daniel Tassie +23

We present meer21cm, a comprehensive python package for cosmological data analysis of single-dish HI intensity mapping surveys. This package is simple to use, with a modularised co…

astro-ph.CO2026

Angular correlation functions of bright Lyman-break galaxies at

Isabelle Ye, Philip Bull, Rebecca A. A. Bowler +3

We investigate the clustering of Lyman-break galaxies at redshifts of 3 5 within the COSMOS field by measuring the angular two-point correlation function. Our…

astro-ph.CO2025

Bayesian evidence for flux scale errors in Galactic synchrotron maps

Michael J. Wilensky, Melis O. Irfan, Philip Bull

The 408 MHz Haslam map is widely used as a low-frequency anchor for the intensity and morphology of Galactic synchrotron emission. Multi-frequency, multi-experiment fits show evide…

astro-ph.CO2025

MeerKLASS L-band deep-field intensity maps: entering the HI dominated regime

MeerKLASS Collaboration, Matilde Barberi-Squarotti, José L. Bernal +18

We present results from MeerKAT single-dish HI intensity maps, the final observations to be performed in L-band in the MeerKAT Large Area Synoptic Survey (MeerKLASS) campaign. The…

astro-ph.CO2024

Constraining Post-Newtonian Parameters with the Cosmic Microwave Background

Daniel B. Thomas, Theodore Anton, Timothy Clifton +1

The Parameterised Post-Newtonian (PPN) approach is the default framework for performing precision tests of gravity in nearby astrophysical systems. In recent works we have extended…