activity
20142024
most citedMultiple Galactic Sources with Emission Above 56 TeV Detected by HAWC

238 citations · 1.9k across the 55 of their papers we have counts for

collaborators

55 papers

astro-ph.HE2024★ 32 cited

The contribution of winds of star clusters to the Galactic cosmic-ray population

Giada Peron, Sabrina Casanova, Stefano Gabici +2

Cosmic rays are energetic nuclei that permeate the entire Galactic disk. Their existence requires the presence of powerful particle accelerators. While Galactic supernova explosion…

astro-ph.HE2023

Hadronic processes at work in 5BZB J0630-2406

Gaëtan Fichet de Clairfontaine, Sara Buson, Leonard Pfeiffer +6

Recent observations are shedding light on the important role that active galactic nuclei (AGN) play in the production of high-energy neutrinos. In this study, we focus on one objec…

astro-ph.HE2023★ 19 cited

Extragalactic neutrino factories

Sara Buson, Andrea Tramacere, Lenz Oswald +6

Identifying the astrophysical sources responsible for the high-energy cosmic neutrinos has been a longstanding challenge. In a previous work, we report evidence for a spatial corre…

astro-ph.HE2023★ 1 cited

An optimized search for dark matter in the galactic halo with HAWC

A. Albert, R. Alfaro, C. Alvarez +63

The Galactic Halo is a key target for indirect dark matter detection. The High Altitude Water Cherenkov (HAWC) observatory is a high-energy (~300 GeV to >100 TeV) gamma-ray detecto…

astro-ph.HE2023

A Contribution of the HAWC Observatory to the TeV era in the High Energy Gamma-Ray Astrophysics: The case of the TeV-Halos

Ramiro Torres-Escobedo, Hao Zhou, Eduardo de la Fuente +130

We present a short overview of the TeV-Halos objects as a discovery and a relevant contribution of the High Altitude Water Čerenkov (HAWC) observatory to TeV astrophysics. We discu…

astro-ph.HE2022★ 12 cited

Gamma-ray observations of MAXI J1820+070 during the 2018 outburst

H. Abe, S. Abe, V. A. Acciari +439

MAXI J1820+070 is a low-mass X-ray binary with a black hole as a compact object. This binary underwent an exceptionally bright X-ray outburst from March to October 2018, showing ev…