collaborators

5 papers

astro-ph.HE2026

A Turbulence-Driven Magnetic Reconnection Model for the High-Energy Neutrino Emission from NGC 1068

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Juan C. Rodríguez-Ramírez +1

We model the Seyfert II AGN NGC 1068 within a turbulence-induced magnetic reconnection framework to explain its high-energy emission. Observations reveal a neutrino flux excess hig…

astro-ph.HE2026

High-Energy Neutrino Emission in NGC1068 driven by Turbulent Magnetic Reconnection

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Juan C. Rodríguez-Ramírez +1

Astrophysical neutrinos from Active Galactic Nuclei (AGN) offer a unique window into high-energy particle acceleration in obscured environments. The nearby Type II Seyfert galaxy N…

astro-ph.HE2026

A Catalogue of Variable Active Galactic Nuclei Based on Multi-Timescale Variability Analysis from Fermi-LAT Data

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Tarek Hassan +2

Active Galactic Nuclei (AGN) sources feature supermassive black holes that launch relativistic plasma jets. They are key -ray sources providing a unique laboratory for studying…

astro-ph.HE2025

Cosmic Ray Acceleration by Turbulence-Driven Magnetic Reconnection and the Origin of the Neutrinos in NGC 1068

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Juan Carlos Rodríguez-Ramírez +1

The Seyfert Type II galaxy NGC 1068 has been identified as a potential neutrino source by IceCube, with a 4.2 significance detection of a 79 neutrino excess from…

astro-ph.HE2025

Detection Prospects for AGNs with the Cherenkov Telescope Array

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Tarek Hassan +9

The Cherenkov Telescope Array Observatory (CTAO) will enable detailed studies of Active Galactic Nuclei (AGN) in the very-high-energy (VHE) regime, as the next-generation ground-ba…