activity
20052020
most citedMeasurement of the Crab Nebula Spectrum Past 100 TeV with HAWC

147 citations · 234 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2020★ 6 cited

HAWC and Fermi-LAT Detection of Extended Emission from the Unidentified Source 2HWC J2006+341

A. Albert, R. Alfaro, C. Alvarez +71

The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best d…

astro-ph.HE2019★ 147 cited

Measurement of the Crab Nebula Spectrum Past 100 TeV with HAWC

HAWC Collaboration, A. U. Abeysekara, A. Albert +102

We present TeV gamma-ray observations of the Crab Nebula, the standard reference source in ground-based gamma-ray astronomy, using data from the High Altitude Water Cherenkov (HAWC…

astro-ph.IM2019★ 52 cited

The Astrophysical Multimessenger Observatory Network (AMON): Performance and Science Program

Hugo A. Ayala Solares, Stephane Coutu, D. F. Cowen +9

The Astrophysical Multimessenger Observatory Network (AMON) has been built with the purpose of enabling near real-time coincidence searches using data from leading multimessenger o…

astro-ph.IM2014★ 16 cited

VAMOS: a Pathfinder for the HAWC Gamma-Ray Observatory

A. U. Abeysekara, R. Alfaro, C. Alvarez +133

VAMOS was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and…

astro-ph.IM2014★ 10 cited

Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America

Pierre Auger Collaboration, Gabriele Curci

The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the mon…

astro-ph2005★ 3 cited

The Central Laser Facility at the Pierre Auger Observatory

F. Arqueros, J. Bellido, C. Covault +18

The Central Laser Facility is located near the middle of the Pierre Auger Observatory in Argentina. It features a UV laser and optics that direct a beam of calibrated pulsed light…