collaborators

6 papers

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

Impact of lensing magnification on the power spectrum turnover

Yolanda Dube, Roy Maartens, Bikash R. Dinda +2

The turnover scale of the matter power spectrum -- and consequently of the standard galaxy power spectrum monopole -- encodes a fundamental signature of matter-radiation equa…

astro-ph.CO2026

Turnover detection using the power spectrum and bispectrum

Yolanda Dube, Bikash R. Dinda, Sheean Jolicoeur +1

The turnover at the peak of the Fourier matter power spectrum encodes a fundamental signature of matter-radiation equality in the early Universe. This delivers a potential standard…

astro-ph.CO2025

Multi-tracing the primordial Universe with future surveys

Mponeng Kopana, Sheean Jolicoeur, Roy Maartens

The fluctuations generated by Inflation are nearly Gaussian in the simplest models, but may be non-Gaussian in more complex models, potentially leading to signatures in the late Un…

astro-ph.CO2025

Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum

Sêcloka L. Guedezounme, Sheean Jolicoeur, Roy Maartens

Wide-angle and relativistic corrections to the Newtonian and flat-sky approximations are important for accurate modeling of the galaxy power spectrum of next-generation galaxy surv…

astro-ph.CO2025

Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys

Mponeng Kopana, Sheean Jolicoeur, Roy Maartens

The fluctuations produced during cosmic inflation may exhibit non-Gaussian characteristics that are imprinted in the large-scale structure of the Universe. This non-Gaussian imprin…