collaborators

9 papers

astro-ph.HE2026

NMMA-Astro-COLIBRI: An Automated Light-Curve Supernovae Classification Service in the Multi-Survey Era

R. Weizmann Kiendrebeogo, Bernardo Cornejo Avila, Sofia Bisero +6

The surge in publicly available photometric alerts from wide-field surveys requires automated tools for real-time transient classification. We present NMMA--Astro-COLIBRI, an on-de…

astro-ph.HE2026

Gamma-Ray Constraints on Heavy Axion-Like-Particle Decays from Fermi-LAT and H.E.S.S. Blazar Spectra

A. Acharyya, F. Aharonian, M. Backes +117

The propagation of very-high-energy (VHE; GeV) gamma rays from extragalactic sources is affected by interactions with photons of the extragalactic background light…

astro-ph.HE2026

Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories

E. Loffredo, N. Hazra, U. Dupletsa +13

Next-generation gravitational wave (GW) observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, will observe binary neutron star (BNS) mergers across cosmic history…

astro-ph.IM2026

Enabling real-time multi-messenger follow-up of transient events with Astro-COLIBRI

Bernardo Cornejo Avila, Sofia Bisero, Mickäel Costa +4

Time-domain astrophysics is a rapidly growing field focused on the study of transient phenomena such as Gamma-Ray Bursts (GRBs), Fast Radio Bursts (FRBs), supernovae, novae, and AG…

astro-ph.IM2026

Astro-COLIBRI: An Innovative Platform for Real-Time Multi-Messenger Astrophysics

Bernardo Cornejo Avila, Sofia Bisero, Mickael Costa +4

The discovery of transient phenomena, such as supernovae, novae, Fast Radio Bursts (FRBs), Gamma-Ray Bursts (GRBs), and stellar flares, together with the emergence of new cosmic me…

astro-ph.IM2026

Multi-Messenger Studies with High-Energy Neutrinos and Gamma Rays: The WST Opportunity

Fabian Schüssler, Sofia Bisero, Bernardo Cornejo +5

The search for the sources of ultra-high-energy cosmic rays (UHECRs) using high-energy neutrinos represents a frontier in high-energy astrophysics. However, a critical bottleneck r…