activity
20052026
most citedDesign Concepts for the Cherenkov Telescope Array

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

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Showing 2011 · astro-ph.HEShow all

13 papers · 2 filters

astro-ph.HE2011★ 21 cited

Gamma-Ray Emission from Two Blazars Behind the Galactic Plane: B2013+370 & B2023+336

E. Kara, M. Errando, W. Max-Moerbeck +7

B2013+370 and B2023+336 are two blazars at low-galactic latitude that were previously proposed to be the counterparts for the EGRET unidentified sources, 3EG J2016+3657 and 3EG J20…

astro-ph.HE2011

Radio-loud AGN contribution to the Extragalactic Gamma-Ray Background

Debbijoy Bhattacharya, M. Errando, R. Mukherjee +4

Origin of extragalactic gamma-ray background (EGRB) is still a matter of debate. EGRB can either have truly diffuse or unresolved discrete point sources origin. Majority of the Fer…

astro-ph.HE2011★ 5 cited

VERITAS Collaboration Contributions to the 32nd International Cosmic Ray Conference

The VERITAS Collaboration, E. Aliu, T. Arlen +96

Compilation of papers contributed by the VERITAS Collaboration to the 32nd International Cosmic Ray Conference, held 11-18 August 2011 in Beijing, China.

astro-ph.HE2011★ 40 cited

Multiwavelength Observations of the Previously Unidentified Blazar RX J0648.7+1516

E. Aliu, T. Aune, M. Beilicke +84

We report on the VERITAS discovery of very-high-energy (VHE) gamma- ray emission above 200 GeV from the high-frequency-peaked BL Lac object RXJ0648.7+1516 (GBJ0648+1516), associate…

astro-ph.HE2011★ 1 cited

Discovery and identification of two gamma-ray blazars at low galactic latitude with VERITAS

M. Errando

We report on the discovery of two gamma-ray sources at E > 200 GeV with VERITAS: RX J0648.7+1516 and VER J0521+211. Both sources are located at low galactic latitudes (|b| < 10 deg…

astro-ph.HE2011★ 1 cited

GeV-TeV Blazar Population Studies

G. D. Senturk, M. Errando, M. Boettcher +3

The synergy between the Fermi-LAT and ground-based Cherenkov telescope arrays gives us the opportunity for the first time to characterize the high energy emission (100 MeV - 10 TeV…