Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy

2011

175 citations recorded by the source corpus.

Citations in the corpus

Measurement of the extragalactic background light imprint on the spectra of the brightest blazars observed with H.E.S.S. (2012, unknown): “The trough between the COB and the CIB will be characterized by the Cherenkov Telescope Array (CTA, Actis et al. 2011) which will probe energies above 50 TeV.”
WIMP dark matter candidates and searches—current status and future prospects (2017, unknown): “one to XENON1T. Combined analysis leads to improved reconstruction of ˙vas indicated by the red region. Both gures are taken from [361]. putative signals from XENON1T and from two ID experiments: CTA [257] and FermiLAT [252] (for which we assume 15 years of exposure and 46 dSphs). We consider a benc”
Dark matter and fundamental physics with the Cherenkov Telescope Array (2012, unknown): “The Cherenkov Telescope Array (CTA) [1] will be an advanced facility for ground-based gamma-ray astronomy in the GeV–TeV regime.”
Cosmic-ray propagation with DRAGON2: I. numerical solver and astrophysical ingredients (2016, unknown): “HAWC [18] and CTA [19] should soon extend those measurements to higher energy.”
The extragalactic background light revisited and the cosmic photon–photon opacity (Corrigendum) (2017, unknown): “One such occasion will be offered by the Cherenkov Telescope Array (CTA) in a few years from now (Actis et al. 2011).”