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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

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  • © 2017

Overview

  • 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

Part of the book series: Springer Theses (Springer Theses)

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Table of contents (11 chapters)

  1. Contributions to the Lowering of the Threshold of Imaging Atmospheric Cherenkov Telescopes

  2. Pulsar Wind Nebulae

  3. Cataclysmic Variable Stars

Keywords

About this book

This thesis is a comprehensive work that addresses many of the open questions currently being discusssed in the very-high-energy (VHE) gamma-ray community. It presents a detailed description of the MAGIC telescope together with a glimpse of the future Cherenkov Telescope Array (CTA). One section is devoted to the design, development and characterization of trigger systems for current and future imaging atmospheric Cherenkov telescopes. The book also features a state-of-the-art description of pulsar wind nebula (PWN) systems, the study of the multi-TeV spectrum of the Crab nebula, as well as the discovery of VHE gamma rays at the multiwavelength PWN 3C 58, which were sought at these wavelengths for more than twenty years. It also includes the contextualization of this discovery amongst the current population of VHE gamma-ray PWNe. Cataclysmic variable stars represent a new source of gamma ray energies, and are also addressed here. In closing, the thesis reports on the systematic search for VHE gamma-ray emissions of AE Aquarii in a multiwavelength context and the search for VHE gamma-ray variability of novae during outbursts at different wavelengths.
 

Authors and Affiliations

  • Max Planck Institute for Nuclear Physics , Heidelberg, Germany

    Rubén López Coto

Bibliographic Information

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

  • Authors: Rubén López Coto

  • Series Title: Springer Theses

  • DOI: https://doi.org/10.1007/978-3-319-44751-3

  • Publisher: Springer Cham

  • eBook Packages: Physics and Astronomy, Physics and Astronomy (R0)

  • Copyright Information: Springer International Publishing AG, part of Springer Nature 2017

  • Hardcover ISBN: 978-3-319-44750-6Published: 07 October 2016

  • Softcover ISBN: 978-3-319-83128-2Published: 22 April 2018

  • eBook ISBN: 978-3-319-44751-3Published: 29 September 2016

  • Series ISSN: 2190-5053

  • Series E-ISSN: 2190-5061

  • Edition Number: 1

  • Number of Pages: XXXVIII, 217

  • Number of Illustrations: 26 b/w illustrations, 101 illustrations in colour

  • Topics: Astrophysics and Astroparticles, Astronomy, Observations and Techniques

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