Refine
Has Fulltext
- no (11)
Language
- English (11)
Is part of the Bibliography
- yes (11) (remove)
Keywords
- radiation mechanisms: non-thermal (4)
- BL Lacertae objects: general (3)
- galaxies: active (3)
- BL Lacertae objects: individual: Mrk 421 (2)
- acceleration of particles (2)
- astroparticle physics (2)
- gamma rays: galaxies (2)
- gamma rays: general (2)
- Air showers (1)
- BL Lacertae objects: individual (Mrk 501) (1)
- BL Lacertae objects: individual: Markarian 501 (1)
- BL Lacertae objects: individual: Mrk 501 (1)
- BL Lacertae objects: individual: Mrk501 (1)
- Cherenkov Telescopes (1)
- Design concepts (1)
- Ground based gamma ray astronomy (1)
- ISM: individual objects (RX J1713.7-3946, G347.3-0.5) (1)
- Next generation Cherenkov telescopes (1)
- TeV gamma-ray astronomy (1)
- X-rays: galaxies (1)
- cosmic rays (1)
- galaxies: individual (M 87) (1)
- galaxies: individual (Markarian 501) (1)
- galaxies: jets (1)
- galaxies: nuclei (1)
- gamma rays: ISM (1)
- methods: data analysis (1)
Institute
Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in astrophysics, particle physics and cosmology. CTA 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 100 GeV and above 100 TeV. CTA will consist of two arrays (one in the north, one in the south) for full sky coverage and will be operated as open observatory. The design of CTA is based on currently available technology. This document reports on the status and presents the major design concepts of CTA.