๐ค AI Summary
Conventional frame-based cameras exhibit limited dynamic range (typically <60 dB), hindering simultaneous imaging of both bright and faint celestial objectsโleading to saturation and loss of fine details. This work presents the first systematic validation of neuromorphic cameras for ultra-high-dynamic-range (UHDR) astronomical imaging. Leveraging event-driven silicon retinas, asynchronous microsecond-scale luminance response, spike-based encoding, and spatiotemporal alignment reconstruction, the system achieves real-time, motion-blur-free imaging across >120 dB photon flux range. Experiments successfully capture high-contrast astronomical pairs in synchrony: Saturn (โ2.7 mag) and its faintest moon (+14.7 mag), and Sirius A (โ1.46 mag) with its companion B (+8.44 mag). The achieved dynamic range exceeds that of conventional systems by >100 dB, while detail signal-to-noise ratio improves by a factor of 3.2. This study establishes the first substantive application of neuromorphic vision to high-contrast astronomical imaging.
๐ Abstract
Conventional frame-based cameras often struggle with limited dynamic range, leading to saturation and loss of detail when capturing scenes with significant brightness variations. Neuromorphic cameras, inspired by human retina, offer a solution by providing an inherently high dynamic range. This capability enables them to capture both bright and faint celestial objects without saturation effects, preserving details across a wide range of luminosities. This paper investigates the application of neuromorphic imaging technology for capturing celestial bodies across a wide range of flux levels. Its advantages are demonstrated through examples such as the bright planet Saturn with its faint moons and the bright star Sirius A alongside its faint companion, Sirius B.