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  • © 2019

Revealing the Most Energetic Light from Pulsars and Their Nebulae

  • Nominated as an outstanding Ph.D. thesis by the Complutense University of Madrid, Spain
  • Offers a comprehensive introduction to VHE emissions from pulsars, together with a detailed compilation of VHE observations of the Crab Pulsar and novel scientific results
  • Provides the most complete picture of VHE emissions from the Crab Pulsar to date

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

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Table of contents (9 chapters)

  1. Front Matter

    Pages i-xvii
  2. The Very-High-Energy Sky and the MAGIC Telescopes

    1. Front Matter

      Pages 1-1
    2. An Introduction to Very-High-Energy Astrophysics

      • David Carreto Fidalgo
      Pages 3-17
    3. Pulsars and Pulsar Wind Nebulae

      • David Carreto Fidalgo
      Pages 19-47
    4. Cherenkov Telescopes and MAGIC

      • David Carreto Fidalgo
      Pages 49-81
  3. Search for TeV Emission from the Crab and Other Pulsars

    1. Front Matter

      Pages 83-83
    2. MAGIC and the Crab Pulsar: History and Motivation

      • David Carreto Fidalgo
      Pages 85-97
    3. Analysis of MAGIC’s Data Set of the Crab Pulsar

      • David Carreto Fidalgo
      Pages 99-123
    4. Lorentz Invariance Violation: Limits from the Crab Pulsar

      • David Carreto Fidalgo
      Pages 125-140
    5. Search for the Next Very-High-Energy Pulsar

      • David Carreto Fidalgo
      Pages 141-155
  4. Looking for a Pulsar Wind Nebula in the Outer Part of Our Galaxy

    1. Front Matter

      Pages 157-157
    2. Does PSR J0631 Power a Pulsar Wind Nebula?

      • David Carreto Fidalgo
      Pages 159-166
    3. MAGIC Observations of PSR J0631: Analysis and Results

      • David Carreto Fidalgo
      Pages 167-177
  5. Back Matter

    Pages 179-208

About this book

This book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly large dataset from the MAGIC telescopes, and comprehensively discusses the implications of pulsed TeV gamma rays for state-of-the-art pulsar emission models. Using these results, the book subsequently explores new testing methodologies for Lorentz Invariance Violation, in terms of a wavelength-dependent speed of light. The book also covers an updated search for Very-High-Energy (VHE), >100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631. 


The observation of VHE gamma rays is essential to studying the non-thermal sources of radiation in our Universe. Rotating neutron stars, also known as pulsars, are an extreme source class known to emit VHE gamma rays. However, to date only two pulsars have been detected with emissions above 100 GeV, and our understanding of their emission mechanism is still lacking. 



Authors and Affiliations

  • Faculty of Physics, Complutense University of Madrid, Madrid, Spain

    David Carreto Fidalgo

Bibliographic Information

Buy it now

Buying options

eBook USD 84.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 109.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access