collaborators

9 papers

astro-ph.CO2026

On the residual missing mass of the Bullet Cluster

Benoit Famaey

Modified Newtonian Dynamics (MOND) is a paradigm that can do away with dark matter at galaxy scales, but displays a residual missing mass discrepancy in galaxy clusters. Prompted b…

astro-ph.CO2025

Mass models of galaxy clusters from a non-parametric weak-lensing reconstruction

Tobias Mistele, Federico Lelli, Stacy McGaugh +2

We study the CLASH sample of galaxy clusters using a new deprojection method for weak gravitational lensing observations. This method is non-parametric, allowing us to infer mass p…

astro-ph.GA2025

A bar stability criterion distinguishing between modified gravity and dark matter in galaxies

Tahere Kashfi, Mahmood Roshan, Virginia Cuomo +3

This paper presents a study on the distinguishability of dark matter and Modified Newtonian Dynamics (MOND) at galactic scales based on the stability criterion proposed by Efstathi…

astro-ph.CO2025

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2025

A primordial origin to cosmic tensions: towards reconciling and with early dark energy and scale-dependent primordial non-Gaussianities

Clément Stahl, Vivian Poulin, Benoit Famaey +1

The Hubble () tension between direct measurements of the expansion rate and the prediction of the CDM cosmological model calibrated on the Cosmic Microwave Background (CMB…

astro-ph.GA2025

MUSE observations of dwarf galaxies and a stellar stream in the M83 group

Oliver Müller, Marina Rejkuba, Katja Fahrion +8

Spectroscopy for faint dwarf galaxies outside of our own Local Group is challenging. Here, we present MUSE spectroscopy to study the properties of four known dwarf satellites and o…