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Astrometric Calibration and Source Characterisation of the Latest Generation Neuromorphic Event-based Cameras for Space Imaging

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arxiv 2211.09939 v1 pith:DQ4WZQWF submitted 2022-11-17 eess.SP astro-ph.IMeess.IV

classification eess.SPastro-ph.IMeess.IV
keywords event-basedspacecameraimagingsystemstechniquesawarenesscharacteristics
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As an emerging approach to space situational awareness and space imaging, the practical use of an event-based camera in space imaging for precise source analysis is still in its infancy. The nature of event-based space imaging and data collection needs to be further explored to develop more effective event-based space image systems and advance the capabilities of event-based tracking systems with improved target measurement models. Moreover, for event measurements to be meaningful, a framework must be investigated for event-based camera calibration to project events from pixel array coordinates in the image plane to coordinates in a target resident space object's reference frame. In this paper, the traditional techniques of conventional astronomy are reconsidered to properly utilise the event-based camera for space imaging and space situational awareness. This paper presents the techniques and systems used for calibrating an event-based camera for reliable and accurate measurement acquisition. These techniques are vital in building event-based space imaging systems capable of real-world space situational awareness tasks. By calibrating sources detected using the event-based camera, the spatio-temporal characteristics of detected sources or `event sources' can be related to the photometric characteristics of the underlying astrophysical objects. Finally, these characteristics are analysed to establish a foundation for principled processing and observing techniques which appropriately exploit the capabilities of the event-based camera.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Event-based Detectors for Laser Guide Star Tip-Tilt Sensing

    astro-ph.IM 2024-12 conditional novelty 5.0 of 10

    Event-based cameras can track a laser spot's tilt to about 1 pixel (15 arcsec) error in the lab, but the milliarcsecond accuracy required for laser guide star tip-tilt remains untested.

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