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Unbiased Long-Term Monitoring at TeV Energies

1
Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de México 04510, Mexico
2
Universität Würzburg, Institute for Theoretical Physics and Astrophysics, 97074 Würzburg, Germany
3
III. Physikalisches Institut A, RWTH Aachen University, 52074 Aachen, Germany
4
Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de México 04510, Mexico
*
Authors to whom correspondence should be addressed.
Galaxies 2019, 7(2), 51; https://doi.org/10.3390/galaxies7020051
Received: 28 February 2019 / Revised: 19 April 2019 / Accepted: 20 April 2019 / Published: 28 April 2019
(This article belongs to the Special Issue Monitoring the Non-Thermal Universe)
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PDF [712 KB, uploaded 28 April 2019]

Abstract

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. View Full-Text
Keywords: monitoring; very high energies (VHE); TeV energies monitoring; very high energies (VHE); TeV energies
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
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González, M.M.; Dorner, D.; Bretz, T.; García-González, J.A.; FACT, HAWC and [email protected] Collaborations. Unbiased Long-Term Monitoring at TeV Energies. Galaxies 2019, 7, 51.

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