HAWC detects M87 at 5.21 sigma over 7.5 years and finds a low-state power-law spectrum extending to 26.5 TeV, with only marginal detection of 3C 264.
VERITAS: Status and Highlights
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emission above 100 GeV from 40 astrophysical sources. These include blazars, pulsar wind nebulae, supernova remnants, gamma-ray binary systems, a starburst galaxy, a radio galaxy, the Crab pulsar, and gamma-ray sources whose origin remains unidentified. In 2009, the array was reconfigured, greatly improving the sensitivity. We summarize the current status of the observatory, describe some of the scientific highlights since 2009, and outline plans for the future.
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Longtime Monitoring of TeV Radio Galaxies with HAWC
HAWC detects M87 at 5.21 sigma over 7.5 years and finds a low-state power-law spectrum extending to 26.5 TeV, with only marginal detection of 3C 264.