activity
20032022
most citedA Very High Energy Gamma-Ray Spectrum of 1ES 2344+514

36 citations · 88 across the 6 of their papers we have counts for

collaborators

7 papers

physics.plasm-ph2022

Optimizing laser coupling, matter heating, and particle acceleration from solids using multiplexed ultraintense lasers

Weipeng Yao, Motoaki Nakatsutsumi, Sébastien Buffechoux +20

Realizing the full potential of ultrahigh-intensity lasers for particle and radiation generation will require multi-beam arrangements due to technology limitations. Here, we invest…

physics.plasm-ph2011★ 28 cited

Hollow microspheres as targets for staged laser-driven proton acceleration

M. Burza, A. Gonoskov, G. Genoud +6

A coated hollow core microsphere is introduced as a novel target in ultra-intense laser-matter interaction experiments. In particular, it facilitates staged laser-driven proton acc…

astro-ph.HE2010

Veritas: Status c. 2009

T. C. Weekes, the VERITAS Collaboration

VERITAS is a ground-based gamma-ray observatory that uses the imaging atmospheric Cherenkov technique and operates in the very high-energy (VHE) region of the gamma- ray spectrum f…

astro-ph2007★ 24 cited

Very High Energy Observations of Gamma-Ray Burst Locations with the Whipple Telescope

D. Horan, R. W. Atkins, H. M. Badran +56

Gamma-ray burst (GRB) observations at very high energies (VHE, E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE compon…

astro-ph2005★ 36 cited

A Very High Energy Gamma-Ray Spectrum of 1ES 2344+514

M. Schroedter, H. M. Badran, J. H. Buckley +26

The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a source of very high energy (VHE) gamma rays by the Whipple Collaboration in 199…

astro-ph2003

Search for TeV Emission at the Location of Milagro Sky Survey Hot Spot Using the Whipple Gamma-Ray Telescope

A. Falcone

A recent report from the Milagro collaboration included an all-sky map created using one year of data from Milagro (peak sensitivity at 3-4 TeV for Crab-like spectra). This map inc…