English

Highlights of the VERITAS Blazar Program

High Energy Astrophysical Phenomena 2019-08-13 v1

Abstract

The VERITAS array of 12-m atmospheric-Cherenkov telescopes in southern Arizona began full-scale operations in 2007, and is one of the world's most-sensitive detectors of astrophysical VHE (E>100 GeV) gamma rays. Approximately 50 blazars are known to emit VHE photons, and observations of blazars are a major focus of the VERITAS Collaboration. Nearly 2000 hours have been devoted to this program and ~130 blazars have already been observed with the array, in most cases with the deepest-ever VHE exposure. These observations have resulted in 21 detections, including 10 VHE discoveries. Recent highlights of the VERITAS blazar observation program, and the collaboration's long-term blazar observation strategy, are presented.

Keywords

Cite

@article{arxiv.1210.3567,
  title  = {Highlights of the VERITAS Blazar Program},
  author = {Wystan Benbow},
  journal= {arXiv preprint arXiv:1210.3567},
  year   = {2019}
}

Comments

4 pages, 2 figures, Submitted to the Proceedings of the 5th International Symposium on High-Energy Gamma-Ray Astronomy (Heidelberg)

R2 v1 2026-06-21T22:20:44.554Z