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20112017
most citedDark Matter Constraints from a Joint Analysis of Dwarf Spheroidal Galaxy Observations with VERITAS

120 citations · 660 across the 18 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.HE2016★ 9 cited

A Search for Very High-Energy Gamma Rays from the Missing Link Binary Pulsar J1023+0038 with VERITAS

E. Aliu, S. Archambault, A. Archer +82

The binary millisecond radio pulsar PSR J1023+0038 exhibits many characteristics similar to the gamma-ray binary system PSR B1259--63/LS 2883, making it an ideal candidate for the…

astro-ph.HE2016★ 15 cited

Discovery of Very High Energy Gamma Rays from 1ES 1440+122

VERITAS Collaboration, S. Archambault, A. Archer +87

The BL Lacertae object 1ES 1440+122 was observed in the energy range from 85 GeV to 30 TeV by the VERITAS array of imaging atmospheric Cherenkov telescopes. The observations, taken…

astro-ph.HE2016★ 38 cited

Upper limits from five years of blazar observations with the VERITAS Cherenkov telescopes

S. Archambault, A. Archer, W. Benbow +78

Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenkov telescope array observed more than 130 blazars; of these, 26 were detected as…

astro-ph.HE2016★ 40 cited

TeV Gamma-ray Observations of The Galactic Center Ridge By VERITAS

A. Archer, W. Benbow, R. Bird +73

The Galactic Center Ridge has been observed extensively in the past by both GeV and TeV gamma-ray instruments revealing a wealth of structure, including a diffuse component as well…

astro-ph.IM2016★ 42 cited

A Search for Brief Optical Flashes Associated with the SETI Target KIC 8462852

A. U. Abeysekara, S. Archambault, A. Archer +78

The F-type star KIC 8462852 has recently been identified as an exceptional target for SETI (search for extraterrestrial intelligence) observations. We describe an analysis methodol…

astro-ph.HE2016★ 25 cited

Exceptionally bright TeV flares from the binary LS I +61 303

VERITAS Collaboration, S. Archambault, A. Archer +86

The TeV binary system LS I +61 303 is known for its regular, non-thermal emission pattern which traces the orbital period of the compact object in its 26.5 day orbit around…