Asteroid Discovery and Light Curve Extraction Using the Hough Transform -- A Rotation Period Study for Sub-Kilometer Main-Belt Asteroids
Kai-Jie Lo, Chan-Kao Chang, Hsing-Wen Lin, Meng-Feng Tsai, Wing-Huen, Ip, Wen-Ping Chen, Ting-Shuo Yeh, K. C. Chambers, E. A. Magnier, M. E. Huber,, R. J. Wainscoat

TL;DR
This study applies the Hough transform to high-cadence asteroid observations, successfully discovering thousands of faint sub-kilometer main-belt asteroids and determining their rotation periods, including super-fast rotators, revealing insights into their physical properties.
Contribution
It introduces a novel application of the Hough transform for asteroid detection and light curve extraction, enabling the discovery and rotation analysis of faint sub-kilometer main-belt asteroids.
Findings
Discovered 3574 new sub-kilometer main-belt asteroids.
Obtained 122 reliable rotation periods, including 13 super-fast rotators.
Super-fast rotators suggest low cohesion and a higher prevalence among small asteroids.
Abstract
The intra-night trajectories of asteroids can be approximated by straight lines, and so are their intra-night detections. Therefore, the Hough transform, a line detecting algorithm, can be used to connect the line-up detections to find asteroids. We applied this algorithm to a high-cadence Pan-STARRS 1 (PS1) observation, which was originally designed to collect asteroid light curves for rotation period measurements (Chang et al., 2019). The algorithm recovered most of the known asteroids in the observing fields and, moreover, discovered 3574 new asteroids with magnitude mainly of 21.5 < w_p1 < 22.5 mag. This magnitude range is equivalent to sub-kilometer main-belt asteroids (MBAs), which usually lack of rotation period measurements due to their faintness. Using the light curves of the 3574 new asteroids, we obtained 122 reliable rotation periods, of which 13 are super-fast rotators…
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