Unbiased Long-Term Monitoring at TeV Energies

For the understanding of the variable, transient and non-thermal universe, unbiased long-term monitoring is crucial. To constrain the emission mechanisms at the highest energies, it is important to characterize the very high energy emission and its correlation with observations at other wavelengths....

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Bibliographic Details
Published in:Galaxies 2019, Vol.7 (2), p.51
Main Authors: González, María, Dorner, Daniela, Bretz, Thomas, García-González, José
Format: Article
Language:English
Subjects:
Cosmic rays
Emission
Energy
Experiments
Gamma rays
Light
Measurement techniques
Monitoring
Radiation
Satellites
Sensors
Telescopes
TeV energies
very high energies (VHE)
Wavelengths
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Summary:For the understanding of the variable, transient and non-thermal universe, unbiased long-term monitoring is crucial. To constrain the emission mechanisms at the highest energies, it is important to characterize the very high energy emission and its correlation with observations at other wavelengths. At very high energies, only a limited number of instruments is available. This article reviews the current status of monitoring of the extra-galactic sky at TeV energies.
ISSN:2075-4434
2075-4434
DOI:10.3390/galaxies7020051