Asteroids are an indelible part of most astronomical surveys though only a few surveys are dedicated to their detection. Over the years, high cadence microlensing surveys have amassed several terabytes of data while scanning primarily the Galactic Bulge and Magellanic Clouds for microlensing events and thus provide a treasure trove of opportunities for scientific data mining. In particular, numerous asteroids have been observed by visual inspection of selected images. This paper presents novel deep learning-based solutions for the recovery and discovery of asteroids in the microlensing data gathered by the MOA project. Asteroid tracklets can be clearly seen by combining all the observations on a given night and these tracklets inform the structure of the dataset. Known asteroids were identified within these composite images and used for creating the labelled datasets required for supervised learning. Several custom CNN models were developed to identify images with asteroid tracklets. Model ensembling was then employed to reduce the variance in the predictions as well as to improve the generalisation error, achieving a recall of 97.67%. Furthermore, the YOLOv4 object detector was trained to localize asteroid tracklets, achieving a mean Average Precision (mAP) of 90.97%. These trained networks will be applied to 16 years of MOA archival data to find both known and unknown asteroids that have been observed by the survey over the years. The methodologies developed can be adapted for use by other surveys for asteroid recovery and discovery.
翻译:在大多数天文调查中,小行星是大多数天文调查的一个不可磨灭的部分,尽管只有为数不多的调查是专门用来探测小行星的。多年来,高浓度微通道调查收集了数兆字节的数据,同时主要为微传事件扫描银河大云和麦哲伦云,从而提供了科学数据挖掘机会的宝藏。特别是,通过对选定图像进行视觉检查,观察了许多小行星。本文介绍了在MOA项目收集的微粒数据中回收和发现小行星的新颖的深层次学习基础解决方案。通过将特定夜晚的所有观测结果结合起来,这些小行星轨迹可以清楚地看到几兆字节的数据。在这些综合图像中发现了已知的小行星和麦哲伦云云云云云云云,并用于创建监督性学习所需的标签数据集。一些自定义的CNN模型用来识别小行星追踪小行星的图像。随后采用了模型组合来减少预测中的差异,并改进了局部的误差,从而实现了97.67%的回收率。此外,经过培训的YOLOV-97号小行星探测器将被用于进行16年的数据收集。经过培训后,这些小行星探测器将被用于观测。