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.
| Author: | María Magdalena González, Daniela Dorner, Thomas Bretz, José Andrés García-González |
|---|---|
| URN: | urn:nbn:de:bvb:20-opus-197389 |
| Document Type: | Journal article |
| Faculties: | Fakultät für Physik und Astronomie / Institut für Theoretische Physik und Astrophysik |
| Language: | English |
| Parent Title (English): | Galaxies |
| ISSN: | 2075-4434 |
| Year of Completion: | 2019 |
| Volume: | 7 |
| Issue: | 2 |
| Article Number: | 51 |
| Source: | Galaxies (2019) 7:2, 51. https://doi.org/10.3390/galaxies7020051 |
| DOI: | 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): |  CC BY: Creative-Commons-Lizenz: Namensnennung 4.0 International |