Reconstruction and analysis of highest energy γ-rays and its application to pulsar wind nebulae

Abstract: The High Altitude Water Cherenkov (HAWC) γ-ray observatory detects cosmic- and γ-rays in the TeV energy range. HAWC was recently upgraded with a sparse detector array (the outrigger array), which increases the instrumented area by a factor of 4-5 and will improve the sensitivity at energie...

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Bibliographic Details
Main Author: Joshi, Vikas (Author)
Format: Book/Monograph Thesis
Language:English
Published: Heidelberg 15 Feb. 2019
DOI:10.11588/heidok.00026062
Subjects:
Online Access:Resolving-System, kostenfrei, Volltext: http://dx.doi.org/10.11588/heidok.00026062
Resolving-System, kostenfrei, Volltext: http://nbn-resolving.de/urn:nbn:de:bsz:16-heidok-260626
Resolving-System, Volltext: https://nbn-resolving.org/urn:nbn:de:bsz:16-heidok-260626
Langzeitarchivierung Nationalbibliothek, Volltext: http://d-nb.info/1178427307/34
Verlag, kostenfrei, Volltext: http://www.ub.uni-heidelberg.de/archiv/26062
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Author Notes:put forward by Vikas Joshi M.Sc. (Physics) ; referees: Prof. Dr. Jim Hinton, Prof. Dr. Stefan Wagner
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Reconstruction and analysis of highest energy γ-rays and its application to pulsar wind nebulae by Joshi, Vikas (Author)

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Book/Monograph Thesis