Probing galactic diffuse TeV gamma-ray emission with the HAWC observatory

  • HAWC Collaboration

Research output: Contribution to journalConference articlepeer-review

Abstract

Galactic diffuse TeV gamma-ray emission is produced by the interaction of high-energy cosmicray particles with matter and radiation in our Galaxy. The measurement of Galactic diffuse TeV gamma-ray emission would provide strong constraints on the acceleration and propagation of Galactic cosmic rays. The High Altitude Water Cherenkov (HAWC) Observatory, located in central Mexico at 4100 m above sea level, is sensitive to gamma rays between a few hundreds GeV and ∼ 100 TeV. Thanks to its large field of view of 2 steradians and excellent background estimation, HAWC has a unique capability to observe large extended sources such as Galactic diffuse emission. We present the analysis strategy to detect the Galactic diffuse emission with HAWC, including techniques to remove contaminations from localized sources.

Original languageEnglish
JournalProceedings of Science
StatePublished - 2017
Externally publishedYes
Event35th International Cosmic Ray Conference, ICRC 2017 - Bexco, Busan, Korea, Republic of
Duration: 10 Jul 201720 Jul 2017

Fingerprint

Dive into the research topics of 'Probing galactic diffuse TeV gamma-ray emission with the HAWC observatory'. Together they form a unique fingerprint.

Cite this