collaborators

5 papers

astro-ph.CO2026

One with HI: Modelling HI Intensity Mapping one-point statistics including systematics

Bernhard Vos-Gines, Cora Uhlemann

Neutral hydrogen (HI) traces the dark matter distribution of the Universe. Upcoming surveys such as the Square Kilometre Array Observatory (SKAO) will trace neutral hydrogen up to…

astro-ph.CO2026

Cosmology with HI Intensity Mapping

Laura Wolz, Gabriele Autieri, José Luis Bernal +18

The redshifted spectral emission from neutral hydrogen (HI) at rest wavelength 21 cm can be used as a tracer of large-scale structure and its evolution. Within the HI intensity map…

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

Recovery of 21 cm BAO: a configuration-space correlation function analysis

Zhongyue Zhang, Kwan Chuen Chan, Santiago Avila +1

Intensity mapping (IM) represents an innovative and potent probe to cosmology. One of its prime applications is to measure the Baryonic Acoustic Oscillations (BAO) in the late univ…

astro-ph.CO2025

Constraining GREA, an alternative theory accounting for the present cosmic acceleration

R. Calderon, J. Garcia-Bellido, B. Vos-Gines +34

The origin of the Universe's late-time accelerated expansion remains unknown. The General Relativistic Entropic Acceleration (GREA) theory offers a compelling alternative to CD…