activity
20082018
most citedA connection between star formation activity and cosmic rays in the starburst galaxy M 82

270 citations · 4.7k across the 67 of their papers we have counts for

collaborators
Showing 2011Show all

15 papers · 1 filter

astro-ph.CO2011★ 68 cited

VERITAS Observations of day-scale flaring of M87 in 2010 April

E. Aliu, T. Arlen, T. Aune +88

VERITAS has been monitoring the very-high-energy (VHE; >100GeV) gamma-ray activity of the radio galaxy M87 since 2007. During 2008, flaring activity on a timescale of a few days wa…

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

Very high energy follow-up observations of GRBs detected by Fermi and Swift

Taylor Aune

In many theoretical models of gamma-ray bursts (GRBs) and their afterglows, the emission of photons above 100 GeV is predicted. The Large Area Telescope (LAT) on-board the Fermi Ga…

astro-ph.CO2011★ 188 cited

The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87

The H. E. S. S. Collaboration, :, A. Abramowski +442

Abridged: The giant radio galaxy M 87 with its proximity, famous jet, and very massive black hole provides a unique opportunity to investigate the origin of very high energy (VHE;…

astro-ph.CO2011

VERITAS Observations of the BL Lac Object PG 1553+113 Between May 2010 and May 2011

Matthew Orr

VERITAS, an array of imaging atmospheric-Cherenkov telescopes, studies blazars in the energy range between ~100 GeV and ~30 TeV. With its excellent sensitivity at these energies, a…