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

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