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Supplementary material to the paper "Radio Source Tracker: Autonomous Attitude Determination on a Radio Interferometric Swarm"

Monday 15 June 2026, by Corentin Louis

This document is a supplementary material to the main paper "Radio Source Tracker: Autonomous Attitude Determination on a Radio Interferometric Swarm". It presents the following additional details that are not included in the main paper due to space limitations:

  • Explanation on the chosen frequency ratio between ν1 and ν2
  • Accuracy results for other random interferometric configurations
  • Details on the bandwidth limits for full sky spectral coherence
  • Justification for the impact of the instrumental errors
  • Details on the Pipeline setup and internal methods
  • DOI: https://doi.org/10.25935/prex-kk46
  • Publisher: OSU Pythéas/AMU, Observatoire de Paris
  • Citation: Rouillé E., Cecconi B., Segret B., Girard J. N., and Loh A. (2026). Supplementary material to the paper "Radio Source Tracker: Autonomous Attitude Determination on a Radio Interferometric Swarm", in Planetary, Solar and Heliospheric Radio Emissions X. L., Lamy, C. K., Louis, G., Fischer, D. E., Morosan, P., Zarka eds. OSU Pythéas/AMU, Observatoire de Paris. Preprint. doi: 10.25935/prex-kk46
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