activity
20152025
most citedAutoSourceID-Light. Fast Optical Source Localization via U-Net and Laplacian of Gaussian

11 citations · 20 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2025

BGRem: A background noise remover for astronomical images based on a diffusion model

Rodney Nicolaas, Sascha Caron, Fiorenzo Stoppa +4

Context: Astronomical imaging aims to maximize signal capture while minimizing noise. Enhancing the signal-to-noise ratio directly on detectors is difficult and expensive, leading…

astro-ph.IM2025

Towards a foundation model for astrophysical source detection: An End-to-End Gamma-Ray Data Analysis Pipeline Using Deep Learning

Judit Pérez-Romero, Saptashwa Bhattacharyya, Sascha Caron +9

The increasing volume of gamma-ray data demands new analysis approaches that can handle large-scale datasets while providing robustness for source detection. We present a Deep Lear…

astro-ph.HE2023

Chasing Gravitational Waves with the Cherenkov Telescope Array

Jarred Gershon Green, Alessandro Carosi, Lara Nava +563

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts…

astro-ph.IM2023★ 1 cited

Interpolation of Instrument Response Functions for the Cherenkov Telescope Array in the Context of pyirf

Rune Michael Dominik, Maximilian Linhoff, Julian Sitarek

The Cherenkov Telescope Array (CTA) will be the next generation ground-based very-high-energy gamma-ray observatory, constituted by tens of Imaging Atmospheric Cherenkov Telescopes…

astro-ph.HE2023

Variability studies of active galactic nuclei from the long-term monitoring program with the Cherenkov Telescope Array

Guillaume Grolleron, Josefa Becerra González, Jonathan Biteau +13

Blazars are active galactic nuclei (AGN) with a relativistic jet oriented toward the observer. This jet is composed of accelerated particles which can display emission over the ent…

astro-ph.IM2023

Performance update of an event-type based analysis for the Cherenkov Telescope Array

Juan Bernete, Orel Gueta, Tarek Hassan +3

The Cherenkov Telescope Array (CTA) will be the next-generation observatory in the field of very-high-energy (20 GeV to 300 TeV) gamma-ray astroparticle physics. The traditional ap…

astro-ph.HE2023

Dark matter searches in dwarf spheroidal galaxies with the Cherenkov Telescope Array

Francesco Gabriele Saturni, Michele Doro, Aldo Morselli +1

Dark matter (DM) is one of the major components in the Universe. However, at present its existence is still only inferred through indirect astronomical observations. DM particles c…

astro-ph.IM2022★ 11 cited

AutoSourceID-Light. Fast Optical Source Localization via U-Net and Laplacian of Gaussian

Fiorenzo Stoppa, Paul Vreeswijk, Steven Bloemen +9

. With the ever-increasing survey speed of optical wide-field telescopes and the importance of discovering transients when they are still young, rapid and reliable s…

astro-ph.HE2017★ 1 cited

An Interpretation of the Cosmic Ray Spectrum from 10 GeV to 3 TeV Measured by CALET on the ISS

S. Bhattacharyya, H. Motz, Y. Asaoka +1

A combined interpretation of the CALET spectrum up to 3 TeV and the AMS-02 positron spectrum up to 500 GeV was performed and the results are discussed. To parametri…

astro-ph.HE2015★ 7 cited

CALET's Sensitivity to Dark Matter Annihilation in the Galactic Halo

Holger Motz, Yoichi Asaoka, Shoji Torii +1

CALET (Calorimetric Electron Telescope), installed on the ISS in August 2015, directly measures the electron+positron cosmic rays flux up to 20 TeV. With its proton rejection capab…