Year: 2025
Type: conference-paper
Abstract: The Radio Neutrino Observatory in Greenland (RNO-G) aims to detect ultra high energy 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, we use the measured Galactic noise to enhance/improve our understanding of the detector, particularly its application in calibrating the antenna orientation.
DOI: 10.22323/1.501.1189
Author: Jethro Stoffels
Institution: Vrije Universiteit Brussel
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: Infrastructure to enhance IceCube, G1876581842, Collaborative Research: WoU-MMA: New Advancements to Enable Multi-Messenger Neutrino Astrophysics with the Radio Neutrino Observatory in Greenland, RII Track-2 FEC: The IceCube EPSCoR Initiative (IEI) - IceCube and the Data Revolution, G434337789, G6461067166, Reconstruction of the properties of ultra-high energy neutrinos from radio detector data using deep learning, Collaborative Research: WoU-MMA: Ultrahigh Energy Neutrinos with the Radio Neutrino Observatory in Greenland, Collaborative Research: WoU-MMA: New Advances to Enable Multi-Messenger Neutrino Astrophysics with the Radio Neutrino Observatory in Greenland, Collaborative Research: WoU-MMA: Ultrahigh Energy Neutrinos with the Radio Neutrino Observatory in Greenland, Collaborative Research: WoU-MMA: New Advancements to Enable Multi-Messenger Neutrino Astrophysics with the Radio Neutrino Observatory in Greenland, Discovering neutrinos of extreme energies with the Radio Neutrino Observatory Greenland, WoU-MMA: Cosmic Ray and Background Identification with RNO-G
OpenAlex ID: W4414492048
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