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Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with MAGIC and Development of Trigger Systems for IACTs

Rubén López Coto

978-3-319-44751-3

2017
Edition 1
- Nominated as an outstanding PhD thesis by the Universitat Autònoma de Barcelona, Spain
- Presents a state-of-the-art overview of the imaging atmospheric Cherenkov technique and the MAGIC telescopes
- Offers a complete picture of the relation between pulsar properties and their very-high-energy gamma-ray emissions
- Features cutting-edge results on the very-high-energy emissions of cataclysmic variable stars with contemporary observations
- Includes supplementary material: sn.pub/extras
€180

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