collaborators

6 papers

astro-ph.CO2026

Cosmography of the Sloan Basin of Attraction and Neighborhood

Daniel Pomarede, R. Brent Tully, Aurelien Valade +2

The Sloan Great Wall is a dominant structure that is relatively nearby. As well as evident in redshift survey maps, its presence is manifested in distortions to cosmic expansion. H…

astro-ph.CO2026

An effective -Szekeres modelling of the local Universe with Cosmicflows-4

Marco Galoppo, Leonardo Giani, Morag Hills +1

We develop an effective description of the local cosmic environment, namely, for redshift , to quantify the bias induced by local structure on cosmological observab…

astro-ph.CO2026

Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4

Vincenzo Salzano, J. Beltrán Jiménez, Dario Bettoni +2

We investigate the angular anisotropy of the Hubble constant using the Cosmicflows-4 catalogue, with particular emphasis on three issues often treated only implicitly in the litera…

astro-ph.CO2026

Prior-free cosmological parameter estimation of Cosmicflows-4

C. Duangchan, A. Valade, N. I. Libeskind +1

As tracers of the underlying mass distributions, the peculiar velocities of galaxies are valuable probes of the Universe, allowing us to measure the Hubble constant or to map the l…

astro-ph.CO2026

Constraining cosmological simulations with peculiar velocities: a forward-modeling approach

Aurélien Valade, Noam Libeskind, Daniel Pomarède +4

Numerical simulations are a key tool to decipher the dynamics of gravitation. Yet, they fail to spatially reproduce the Universe we observe, limiting comparison between observation…

astro-ph.CO2025

Forecast for growth-rate measurement using peculiar velocities from LSST supernovae

Damiano Rosselli, Bastien Carreres, Corentin Ravoux +8

In this work, we investigate the feasibility of measuring the cosmic growth-rate parameter, , using peculiar velocities (PVs) derived from Type Ia supernovae (SNe Ia) in the…