J. H. Buckley

TL;DR: The ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes as mentioned in this paper, which is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100GeV and above 100 TeV.

TL;DR: The Cherenkov Telescope Array (CTA) as discussed by the authors is a very high-energy (VHE) gamma ray observatory with an international collaboration with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America.

TL;DR: In this paper, the authors make a detailed phenomenological study of the possible detection rates given these three pieces of new information, and show that the proposed upgrade of the Whipple telescope will make it sensitive to a region of parameter space, with substantial improvements possible with the planned new generation of Air Cherenkov Telescope Arrays.

TL;DR: In this paper, the authors make a detailed phenomenological study of the possible detection rates given these three pieces of new information, and show that the proposed upgrade of the Whipple telescope will make it sensitive to a region of parameter space, with substantial improvements possible with the planned new generation of Air Cherenkov Telescope Arrays.

TL;DR: In this paper, the authors used a simple synchrotron self- Compton model to model the spectral energy distribution (SED) of a set of TeV blazars with good broadband data, to look for a connection of the jet properties to the properties of the central accreting black hole.