activity
20152018
most citedGamma rays from the quasar PKS 1441+25: story of an escape

99 citations · 474 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2018★ 19 cited

HESS J1943+213: An Extreme Blazar Shining Through The Galactic Plane

The VERITAS Collaboration, A. Archer, W. Benbow +60

HESS J1943+213 is a very-high-energy (VHE; 100 GeV) -ray source in the direction of the Galactic Plane. Studies exploring the classification of the source are converging towa…

astro-ph.HE2018★ 60 cited

A Very High Energy -Ray Survey towards the Cygnus Region of the Galaxy

The VERITAS Collaboration, A. U. Abeysekara, A. Archer +68

We present results from deep observations towards the Cygnus region using 300 hours of very-high-energy (VHE) -ray data taken with the VERITAS Cherenkov telescope array and over…

astro-ph.HE2018★ 9 cited

A strong limit on the very-high-energy emission from GRB 150323A

A. U. Abeysekara, A. Archer, W. Benbow +63

On 2015 March 23, VERITAS responded to a -BAT detection of a gamma-ray burst, with observations beginning 270 seconds after the onset of BAT emission, and only 135 seconds a…

astro-ph.HE2017★ 20 cited

Very-High-Energy -Ray Observations of the Blazar 1ES 2344+514 with VERITAS

C. Allen, S. Archambault, A. Archer +79

We present very-high-energy -ray observations of the BL Lac object 1ES 2344+514 taken by the Very Energetic Radiation Imaging Telescope Array System (VERITAS) between 2007 and 2…

astro-ph.HE2016★ 67 cited

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +290

We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1 which inc…

astro-ph.HE2016★ 39 cited

A search for spectral hysteresis and energy-dependent time lags from X-ray and TeV gamma-ray observations of Mrk 421

A. U. Abeysekara, S. Archambault, A. Archer +220

Blazars are variable emitters across all wavelengths over a wide range of timescales, from months down to minutes. It is therefore essential to observe blazars simultaneously at di…