Download Very-high-energy Gamma-ray Observations of Pulsar Wind by Rubén López Coto PDF

By Rubén López Coto

This thesis is a accomplished paintings that addresses a number of the open questions presently being discusssed within the very-high-energy (VHE) gamma-ray neighborhood. It provides an in depth description of the MAGIC telescope including a glimpse of the long run Cherenkov Telescope Array (CTA). One part is dedicated to the layout, improvement and characterization of set off platforms for present and destiny imaging atmospheric Cherenkov telescopes. The ebook additionally contains a cutting-edge description of pulsar wind nebula (PWN) structures, the research of the multi-TeV spectrum of the Crab nebula, in addition to the invention of VHE gamma rays on the multiwavelength PWN 3C fifty eight, that have been sought at those wavelengths for greater than two decades. it is also the contextualization of this discovery among the present inhabitants of VHE gamma-ray PWNe. Cataclysmic variable stars characterize a brand new resource of gamma ray energies, and also are addressed the following. In remaining, the thesis reviews at the systematic look for VHE gamma-ray emissions of AE Aquarii in a multiwavelength context and the quest for VHE gamma-ray variability of novae in the course of outbursts at diverse wavelengths.

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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

This thesis is a accomplished paintings that addresses the various open questions at present being discusssed within the very-high-energy (VHE) gamma-ray neighborhood. It offers an in depth description of the MAGIC telescope including a glimpse of the longer term Cherenkov Telescope Array (CTA). One part is dedicated to the layout, improvement and characterization of set off platforms for present and destiny imaging atmospheric Cherenkov telescopes.

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

Example text

1 MAGIC integral ULs to steady flux of AE Aqr. . . . . . 2 MAGIC daily integral ULs to steady flux of AE Aqr . . . 3 MAGIC integral ULs to steady flux for different optical states of AE Aqr . . . . . . . . . . . . . . . . . 4 MAGIC integral ULs for pulsed emission of AE Aqr . . . 1 Differential ULs on the flux from YY Her measured by Fermi-LAT and MAGIC . . . . . . . . . . . . . 2 Differential ULs on the flux from ASASSN-13ax measured by Fermi-LAT and MAGIC .

Energy thresholds and rates for different DTs for single-telescope and stereo LSTs . . . . . . . . . . . L1 trigger rates for different NSB, DTs and for the two MAGIC telescopes. . . . . . . . . . . . . . . . . Summary of the results for the sensitivity ratio and c-ray rate ratio between the analysis applying the Topo-trigger macrocell cuts and without applying them for medium and low energies . . . . . . . . . . . . . . . .

PSR J0205+6449 phaseogram above 420 GeV . . . . . VHE c-ray luminosity, X-ray luminosity and ratio between luminosities of PWNe and PWN candidates as a function of the spin-down power of the central pulsar . . . . . . VHE c-ray luminosity histogram of PWNe and PWN candidates detected at VHE gamma rays . . . . . . . . VHE c-ray luminosity, X-ray luminosity and ratio between luminosities of PWNe and PWN candidates as a function of the characteristic age of the central pulsar .

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