activity
20242026
collaborators

5 papers

astro-ph.HE2026

Constraining cosmological parameters from very-high-energy -ray attenuation in blazar spectra: Bayesian inference and systematic uncertainties

Patryk Liniewicz, Emmanuel Moulin

Very-high-energy rays from active galactic nuclei are attenuated through pair production on the extragalactic background light (EBL), providing a probe of cosmic expansion. We…

astro-ph.HE2026

Assessing the sensitivity to Axion-Like-Particle Dark Matter with very-high-energy gamma-ray observations of selected AGN and galaxy cluster pairs

Cervane Grimaud, Denys Malyshev, Emmanuel Moulin

Axion-Like-Particles (ALPs) are pseudo-scalar particles actively searched as light dark matter candidates. ALPs can couple to photons which give rise to the possibility of oscillat…

hep-ph2026

Gamma-ray production in the cosmic-ray -- dark matter scattering as a probe of the axion-like particle -- proton interaction

Victor P. Goncalves, Emmanuel Moulin, Igor Reis +1

The production of very-high-energy (VHE, GeV) gamma rays resulting from the scattering of high-energy cosmic-ray protons off axion-like particles (ALPs) populati…

astro-ph.HE2025

Search for dark matter around intermediate mass black holes with the H.E.S.S. experiment

Jann Aschersleben, Dieter Horns, Emmanuel Moulin +1

Intermediate mass black holes (IMBHs), with masses ranging from a hundred and a million solar masses, are hypothesised to be surrounded by dense regions of dark matter known as dar…

astro-ph.HE2024

Nonparametric signal separation in very-high-energy gamma ray observations with probabilistic neural networks

Marion Ullmo, Emmanuel Moulin

An intriguing challenge in observational astronomy is the separation signals in areas where multiple signals intersect. A typical instance of this in very-high-energy (VHE, E$\gtrs…