Unbiased Long-Term Monitoring at TeV Energies
AbstractFor 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
Share & Cite This Article
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.
González MM, Dorner D, Bretz T, García-González JA, FACT, HAWC and [email protected] Collaborations. Unbiased Long-Term Monitoring at TeV Energies. Galaxies. 2019; 7(2):51.Chicago/Turabian Style
González, María M.; Dorner, Daniela; Bretz, Thomas; García-González, José A.; FACT, HAWC and [email protected] Collaborations. 2019. "Unbiased Long-Term Monitoring at TeV Energies." Galaxies 7, no. 2: 51.
Note that from the first issue of 2016, MDPI journals use article numbers instead of page numbers. See further details here.