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Stereoscopy of gamma-ray showers with the H.E.S.S. telescopes: First images of supernova remnants in the TeV range.

Lemoine-goumard, Marianne (2006) Stereoscopy of gamma-ray showers with the H.E.S.S. telescopes: First images of supernova remnants in the TeV range. PhD thesis LLR, EP - LLR, EP/X p.297.

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Alternative Locations: http://www.imprimerie.polytechnique.fr/Theses/Files/ Lemoine_Goumard.pdf

Abstract

The HESS (High Energy Stereoscopic
System) experiment in gamma-ray Astronomy consists of four imaging atmospheric Cherenkov telescopes devoted to the observation of the gamma-ray sky in the energy domain above 100 GeV and extending up to several tens of TeV. This thesis presents a new reconstruction method of gamma-ray induced air showers which takes full advantage of the stereoscopy and of the fine-grain imaging of the HESS cameras.
This new method provides an angular resolution better than 0 - 1
degree, an energy resolution of about 15% at zenith and a very efficient hadronic rejection based on a cut on the lateral spread of the electromagnetic shower. A new background subtraction method, well adapted to the study of extended sources, was also developed. No assumptions, either on the distribution of gamma-rays in the field of view, or on the distribution of hadrons are necessary. It provides two skymaps obtained from a maximum likelih!
ood fit: one for gamma-rays and the other for hadrons. These two analysis methods were applied to the study of the shell-type supernova remnants RX J1713.7-3946 and Vela Junior, allowing for the first time to resolve their morphology in the gamma-ray domain. A morphological and spectral study of these sources combined with a comparison of a simple model of emission processes provides some constraints on the parameters of the leptonic process. The different results obtained are discussed and compared with the supernova remnant SN 1006.

Item Type:PhD Thesis (PhD)
Thesis Supervisor:Bernard, Degrange
Date:May 2006
Board of examiners:Decourchelle, Anne and Katsanevas, Stavros and Parizot, Etienne and Rosier-lees, Sylvie and Smith, David
Ecole Doctorale:ED 447 ECOLE DOCTORALE DE L'ECOLE POLYTECHNIQUE
Discipline:LLR
Collection (Fonds):EP/X
Institution:EP/X
Department:EP - LLR
Subjects:3. Physics, Optics
Uncontrolled Keywords:Very high energy gamma-ray astronomy, imaging atmospheric Cherenkov, H.e.s.s., 3D Model, Supernova remnants, Rx j1713.7-3946, Rx j0852.0-4622, Vela Junior, Sn 1006, Astronomie gamma de très hautes énergies, imagerie Tcherenkov atmosphérique, H.e.s.s., Modèle 3D, Vestiges de supernovae, Rx j1713.7-3946, Rx j0852.0-4622, Vela Junior, Sn 1006

Table of content

Introduction
I. L'Astronomie gamma des hautes énergies
II. L'expérience H.E.S.S., un instrument de troisième génération
III. Analyse des données Tcherenkov
IV. Observations de vestiges de supernovae à coquilles
Conclusion

ID Code:1892
Deposited By:Laurence Vidament
Deposited On:15 September 2006

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