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|a 9783642361340
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| 100 |
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|a Aharonian, Felix
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| 245 |
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|a Astrophysics at Very High Energies
|h Elektronische Ressource
|b Saas-Fee Advanced Course 40. Swiss Society for Astrophysics and Astronomy
|c by Felix Aharonian, Lars Bergström, Charles Dermer ; edited by Roland Walter, Marc Türler
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| 250 |
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|a 1st ed. 2013
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| 260 |
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|a Berlin, Heidelberg
|b Springer Berlin Heidelberg
|c 2013, 2013
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| 300 |
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|a XII, 361 p
|b online resource
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| 505 |
0 |
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|a Gamma Rays at Very High Energies -- Multi-messenger Astronomy and Dark Matter -- Sources of GeV Photons and the Fermi Results -- Index
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| 653 |
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|a Astronomy / Observations
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| 653 |
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|a Space Physics
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| 653 |
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|a Astronomy, Observations and Techniques
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| 653 |
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|a Astrophysics
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| 653 |
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|a Solar system
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| 700 |
1 |
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|a Bergström, Lars
|e [author]
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| 700 |
1 |
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|a Dermer, Charles
|e [author]
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| 700 |
1 |
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|a Walter, Roland
|e [editor]
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| 041 |
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7 |
|a eng
|2 ISO 639-2
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| 989 |
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|b Springer
|a Springer eBooks 2005-
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| 490 |
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|a Saas-Fee Advanced Course
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| 028 |
5 |
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|a 10.1007/978-3-642-36134-0
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| 856 |
4 |
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|u https://doi.org/10.1007/978-3-642-36134-0?nosfx=y
|x Verlag
|3 Volltext
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| 082 |
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|a 523.01
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| 520 |
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|a With the success of Cherenkov Astronomy and more recently with the launch of NASA’s Fermi mission, very-high-energy astrophysics has undergone a revolution in the last years. This book provides three comprehensive and up-to-date reviews of the recent advances in gamma-ray astrophysics and of multi-messenger astronomy. Felix Aharonian and Charles Dermer address our current knowledge on the sources of GeV and TeV photons, gleaned from the precise measurements made by the new instrumentation. Lars Bergström presents the challenges and prospects of astro-particle physics with a particular emphasis on the detection of dark matter candidates. The topics covered by the 40th Saas-Fee Course present the capabilities of current instrumentation and the physics at play in sources of very-high-energy radiation to students and researchers alike. This book will encourage and prepare readers for using space and ground-based gamma-ray observatories, as well as neutrino and other multi-messenger detectors
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