Speaker
Jethro Stoffels
Description
The Radio Neutrino Observatory in Greenland (RNO-G) aims to detect UHE
neutrinos (E > 100 PeV). With an array of upward-facing near-surface antennas operating in the 80-700 MHz range, the RNO-G surface component is sensitive to broadband signals originating from many sources, such as background noise induced by the Milky Way. In this contribution, I use the measured Galactic noise to enhance/improve our understanding of the detector, particularly its application in calibrating the antenna orientation
| Collaboration(s) | RNO-G |
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