collaborators

21 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 with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era

Suman Majumdar, Debanjan Sarkar, Leon Noble +38

The cosmological distribution of neutral hydrogen (HI) during the post-reionization era is highly non-Gaussian due to the underlying non-linear structure formation, complex galaxy…

astro-ph.CO2026

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum

Chris Addis, Sêcloka L. Guedezounme, Jessie Hammond +5

A major goal of ongoing and future cosmological surveys of the large-scale structure is to measure local type primordial non-Gaussianity in the galaxy power spectrum through the sc…

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…

astro-ph.CO2026

Cosmological peculiar velocities in general relativity

Chris Clarkson, Roy Maartens

We reconsider the late-time evolution of galaxy peculiar velocities in the 1+3 covariant approach to cosmological perturbation theory. It has recently been claimed that this approa…

astro-ph.CO2026

Calibration-independent consistency test of BAO and SNIa data: update

Bikash R. Dinda, Roy Maartens, Chris Clarkson

In a recent paper, arXiv:2509.19899, we presented a new method to test the consistency between uncalibrated BAO and SNIa data through a common parameter, the Alcock-Paczynski varia…