activity
20012026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 2.3k across the 23 of their papers we have counts for

collaborators

24 papers

astro-ph.HE2026

Hard X-ray Sources in Fermi UFOs

Alessandro Paggi, Ioannis Liodakis, John Antoniadis +7

Identification and/or association of unidentified -ray sources with lower-energy counterparts represents a key challenge in modern astronomy, due to the relatively large positio…

astro-ph.HE2016★ 39 cited

A search for spectral hysteresis and energy-dependent time lags from X-ray and TeV gamma-ray observations of Mrk 421

A. U. Abeysekara, S. Archambault, A. Archer +220

Blazars are variable emitters across all wavelengths over a wide range of timescales, from months down to minutes. It is therefore essential to observe blazars simultaneously at di…

astro-ph.HE2013★ 67 cited

Observation of Markarian 421 in TeV gamma rays over a 14-year time span

V. A. Acciari, T. Arlen, T. Aune +73

The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been explored with the Whipple 10 m telescope. It is shown that the dynamic range of it…

astro-ph.CO2011★ 15 cited

On the driver of relativistic effects strength in Seyfert galaxies

M. Guainazzi, S. Bianchi, I. de la Calle Perez +2

Spectroscopy of X-ray emission lines emitted in accretion discs around supermassive black holes is one of the most powerful probes of the accretion flow physics and geometry, while…

astro-ph.HE2010★ 87 cited

Multi-wavelength Observations of the Flaring Gamma-ray Blazar 3C 66A in 2008 October

LAT collaboration, A. A. Abdo et al., the VERITAS collaboration +4

The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GA…

astro-ph.HE2010★ 129 cited

FERO: Finding Extreme Relativistic Objects. I. Statistics of Relativistic Fe Kalpha lines in Radio-Quiet Type 1 AGN

I. de la Calle Pérez, A. L. Longinotti, M. Guainazzi +10

Accretion models predict that fluorescence lines broadened by relativistic effects should arise from reflection of X-ray emission onto the inner region of the accretion disc surrou…