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, SpainPresents a state-of-the-art overview of the imaging atmospheric Cherenkov technique and the MAGIC telescopesOffers a complete picture of the relation between pulsar properties and their very-high-energy gamma-ray emissionsFeatures cutting-edge results on the very-high-energy emissions of cataclysmic variable stars with contemporary observationsIncludes supplementary material: sn.pub/extras