collaborators

10 papers

gr-qc2026

Beyond ΛCDM with the SKA Observatory -- I: Probing Gravity on Cosmological Scales

S. Camera, C. Addis, S. L. Guedezounme +26

General relativity (GR) is currently the best description of the gravitational interaction at our disposal and is one of the foundations of the concordance cosmological model. For…

astro-ph.CO2026

Cosmology from HI galaxy surveys with the SKA

Ainulnabilah Nasirudin, Philip Bull, Ziad Sakr +8

The 21cm line from neutral hydrogen is expected to be a ubiquitous (albeit faint) tracer of galaxies in the late Universe. With SKAO-MID, large wide-field surveys of several millio…

astro-ph.CO2026

Predicted number counts and clustering of Hi galaxies from future radio surveys

Ainulnabilah Nasirudin, Philip Bull, Isabelle Ye

The 21cm emission line from neutral hydrogen (HI) contained within galaxies provides a way to make accurate spectroscopic redshift determinations at radio frequencies. Large arrays…

astro-ph.CO2026

Cosmology with Tully-Fisher HI Galaxy Surveys

Joël Mayor, Anthony Carr, Khaled Said +7

The SKA Observatory will enable measurements of the Tully-Fisher relation for statistical samples of HI selected galaxies out to unprecedented depths and redshifts thanks to its un…

astro-ph.CO2026

Observational Frontiers in the post-EoR 21-cm Intensity Mapping: Lessons from the SKA Pathfinders

Khandakar Md Asif Elahi, Somnath Bharadwaj, Philip Bull +21

The 21-cm line from neutral hydrogen has long been recognised as a promising tracer of the large-scale structure of the Universe. The line is weak however, making individual galaxy…

astro-ph.CO2026

Prospects for measuring the Doppler magnification dipole with LSST and DESI

Isabelle Ye, Philip Bull, Caroline Guandalin +2

We forecast the detectability of the Doppler magnification dipole with a joint analysis of galaxy spectroscopic redshifts and size measurements. The Doppler magnification arises fr…