Abstract
We report on the discovery of high-energy (HE;E >0.1 GeV) and very-high-energy (VHE;E >100 GeV) γ-ray emission from the blazar RBS 0413 with Fermi and VERITAS. The spectral energy distribution (SED), including contemporaneous X-ray and optical observations, is presented. Synchrotron self-Compton, external-Compton and leptohadronic models are applied to the SED and the results are discussed.
| Original language | English |
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| Pages | 105-108 |
| Number of pages | 4 |
| DOIs | |
| Publication status | Published - 1 Jan 2011 |
| Event | 32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: 11 Aug 2011 → 18 Aug 2011 |
Conference
| Conference | 32nd International Cosmic Ray Conference, ICRC 2011 |
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| Country/Territory | China |
| City | Beijing |
| Period | 11/08/11 → 18/08/11 |
Keywords
- Active galactic nuclei
- Blazars
- Observations