English

Latest news from the HAWC outrigger array

Instrumentation and Methods for Astrophysics 2019-08-22 v1 High Energy Astrophysical Phenomena

Abstract

The High Altitude Water Cherenkov (HAWC) observatory is a very high energy gamma-ray detector located in Mexico. In late 2018, the HAWC collaboration completed a major upgrade consisting of the addition of a sparse outrigger array of 345 small water Cherenkov detectors (WCDs) surrounding the 300 WCDs of the main array and extending the instrumented area by a factor of 4. It provides an improved reconstruction of the showers whose core and footprint are not well contained in the array and increases the effective area in the range of a few TeV to beyond 100 TeV. This improvement in sensitivity will help to have a better understanding of the Galactic sources that accelerate particles up to the knee of the cosmic ray spectrum. In this contribution, we will show the current status, the performance, and the first results from the HAWC outrigger array.

Keywords

Cite

@article{arxiv.1908.07634,
  title  = {Latest news from the HAWC outrigger array},
  author = {Vincent Marandon and Armelle Jardin-Blicq and Harm Schoorlemmer},
  journal= {arXiv preprint arXiv:1908.07634},
  year   = {2019}
}

Comments

Proceedings of the 36th International Cosmic Ray Conference, 2019, Madison, WI, USA

R2 v1 2026-06-23T10:52:44.761Z