English

Very-high-energy blazars: updates from VERITAS observations and multi-wavelength campaigns

High Energy Astrophysical Phenomena 2019-08-13 v1

Abstract

VERITAS is an array of four 12-m atmospheric Cherenkov telescopes, designed to observe the very-high-energy (VHE; E \geq100 GeV) sky. Since 2007, it has detected more than 20 extra-galactic sources, the majority of which are active-galactic-nuclei of the blazar class. In this paper we present a selection of the most recent results from the VERITAS blazar observing program, in particular in the context of broad-band multi-wavelength campaigns. Four results are highlighted: the detection of the flat-spectrum-radio-quasar PKS 1222+216 (4C +21.35) during March 2014; the γ\gamma-ray flare from the BL Lac object 1ES 1727+502, observed under bright-moonlight conditions during May 2013; the bright γ\gamma-ray flare from the BL Lac object 1ES 1011+496 during February 2014; and the long-term campaign on the BL Lac object PKS 1424+240, currently the farthest (z > 0.60), persistent VHE emitter

Keywords

Cite

@article{arxiv.1501.03554,
  title  = {Very-high-energy blazars: updates from VERITAS observations and multi-wavelength campaigns},
  author = {Matteo Cerruti},
  journal= {arXiv preprint arXiv:1501.03554},
  year   = {2019}
}

Comments

8 pages, 3 figures; to appear in the Proceedings of the 10th INTEGRAL Workshop "A Synergistic View of the High Energy Sky" - Integral 2014, 15-19 September 2014, Annapolis, MD, USA