CTA: the future of ground-based γ-ray astrophysics

@article{Persic2013CTATF,
  title={CTA: the future of ground-based $\gamma$-ray astrophysics},
  author={Massimo Persic},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2013},
  volume={239},
  pages={210-215}
}
  • M. Persic
  • Published 10 March 2013
  • Physics
  • arXiv: High Energy Astrophysical Phenomena
View PDF on arXiv
3 Citations

3 Citations

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References

SHOWING 1-10 OF 26 REFERENCES

Potential of EBL and cosmology studies with the Cherenkov Telescope Array

Dark matter and fundamental physics with the Cherenkov Telescope Array

Prospects for observations of pulsars and pulsar wind nebulae with CTA

Studies of active galactic nuclei with CTA

High energy γ-ray emission from compact galactic sources in the context of observations with the next generation Cherenkov Telescope Arrays

Multiwavelength Astronomy and CTA: X-rays

Active Galactic Nuclei under the scrutiny of CTA

Surveys with the Cherenkov Telescope Array

Observation of Pulsed γ-Rays Above 25 GeV from the Crab Pulsar with MAGIC

By developing a new electronic trigger, the threshold of the MAGIC telescope is lowered, revealing a relatively high cutoff energy in the phase-averaged spectrum, which indicates that the emission occurs far out in the magnetosphere, hence excluding the polar-cap scenario as a possible explanation of the measurement.

Binaries with the eyes of CTA