Unbiased long-term monitoring at TeV energies

Please always quote using this URN: urn:nbn:de:bvb:20-opus-197389
  • 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.

Download full text files

Export metadata

Additional Services

Share in Twitter Search Google Scholar Statistics
Author: María Magdalena González, Daniela Dorner, Thomas Bretz, José Andrés García-González
Document Type:Journal article
Faculties:Fakultät für Physik und Astronomie / Institut für Theoretische Physik und Astrophysik
Parent Title (English):Galaxies
Year of Completion:2019
Article Number:51
Source:Galaxies (2019) 7:2, 51. https://doi.org/10.3390/galaxies7020051
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Tag:TeV energies; monitoring; very high energies (VHE)
Release Date:2022/05/09
Date of first Publication:2019/04/28
Licence (German):License LogoCC BY: Creative-Commons-Lizenz: Namensnennung 4.0 International