activity
20162024
most citedMonte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

72 citations · 97 across the 11 of their papers we have counts for

collaborators
Showing 2023Show all

7 papers · 1 filter

astro-ph.IM20231 cited

Polarization analysis of the VLTI and GRAVITY

GRAVITY Collaboration, F. Widmann, X. Haubois N. Schuhler +59

The goal of this work is to characterize the polarization effects of the VLTI and GRAVITY. This is needed to calibrate polarimetric observations with GRAVITY for instrumental effec…

astro-ph.HE20231 cited

Long-term monitoring of the radio-galaxy M87 in gamma-rays: joint analysis of MAGIC, VERITAS and Fermi-LAT data

M. Molero, P. Batista, L. Fortson +4

M87 was discovered in the very-high-energy band (VHE, E > 100 GeV) with HEGRA in 2003, long before its emission was detected in the high-energy band (HE, E > 100 MeV) with Fermi-LA…

astro-ph.HE2023

TeV Detection of the Extreme HSP Blazar RBS 1366 by VERITAS

Deivid Ribeiro

Extreme high-synchrotron-peak blazars (EHSPs) are postulated as the most efficient and extreme particle accelerators in the universe but remain enigmatic as a possible new class of…

astro-ph.HE2023

Optimizing the Wasserstein GAN for TeV Gamma Ray Detection with VERITAS

Deivid Ribeiro, Yuping Zheng, Ramana Sankar +1

The observation of very-high-energy (VHE, E>100 GeV) gamma rays is mediated by the imaging atmospheric Cherenkov technique (IACTs). At these energies, gamma rays interact with the…

astro-ph.IM2023

Exploring the Potential of the Pulsed Laser onboard the CALIPSO Satellite to Improve Calibration with VERITAS

Gregory Foote

Imaging Atmospheric Cherenkov Telescopes (IACTs) are used to detect bright nanosecond-duration flashes of optical light originating from interactions of cosmic/gamma-rays in the at…

astro-ph.HE20237 cited

VERITAS and Fermi-LAT constraints on the Gamma-ray Emission from Superluminous Supernovae SN2015bn and SN2017egm

A. Acharyya, C. B. Adams, P. Bangale +56

Superluminous supernovae (SLSNe) are a rare class of stellar explosions with luminosities ~10-100 times greater than ordinary core-collapse supernovae. One popular model to explain…