activity
20052026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 9.7k across the 196 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.HEShow all

18 papers · 2 filters

astro-ph.HE2013★ 86 cited

A Three-Year Multi-Wavelength Study of the Very High Energy Gamma-ray Blazar 1ES 0229+200

E. Aliu, S. Archambault, T. Arlen +83

The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blaza…

astro-ph.HE2013★ 50 cited

Search for gamma-ray-emitting active galactic nuclei in the Fermi-LAT unassociated sample using machine learning

M. Doert, M. Errando

The second Fermi-LAT source catalog (2FGL) is the deepest all-sky survey available in the gamma-ray band. It contains 1873 sources, of which 576 remain unassociated. Machine-learni…

astro-ph.HE2013★ 50 cited

Long-term TeV and X-ray Observations of the Gamma-ray Binary HESS J0632+057

VERITAS Collaboration, E. Aliu, S. Archambault +297

HESS J0632+057 is the only gamma-ray binary known so far whose position in the sky allows observations with ground-based observatories both in the northern and southern hemispheres…

astro-ph.HE2013★ 21 cited

VERITAS Observations of the Microquasar Cygnus X-3

S. Archambault, M. Beilicke, W. Benbow +76

We report results from TeV gamma-ray observations of the microquasar Cygnus X-3. The observations were made with the Very Energetic Radiation Imaging Telescope Array System (VERITA…

astro-ph.HE2013★ 30 cited

Long term observations of B2 1215+30 with VERITAS

VERITAS collaboration, E. Aliu, S. Archambault +82

We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this period, the source was detected at very high energies (VHE; E > 100 GeV) by VER…

astro-ph.HE2013

Observations of low- and intermediate-frequency-peaked BL Lacs above 100 GeV with VERITAS

M. Errando

Most of the ~50 blazars detected to date at TeV energies (E>0.1 TeV) are high-frequency-peaked BL Lacs (HBLs). Only a handful episodic TeV detections of low- and intermediate-frequ…