🤖 AI Summary
The proliferation of low-Earth-orbit satellites introduces low signal-to-noise ratio (SNR) streak artifacts in astronomical images, degrading photometric accuracy. To address this, we propose an end-to-end detection framework integrating U-Net with the Line Segment Detector (LSD). This is the first approach to jointly model semantic segmentation and geometric line detection: U-Net performs coarse localization of satellite trail regions, while LSD refines sub-pixel-accurate linear features, significantly enhancing robustness for weak-signal trails. Evaluated on simulated data from the Mini-SiTian Array, the method achieves >99% detection rate at SNR ≥ 3. On real observational data, it attains a recall of 79.57% and precision of 74.56%. The framework thus enables high-precision astronomical photometry and rigorous data quality control in satellite-contaminated imaging.
📝 Abstract
With the rapid increase in the number of artificial satellites, astronomical imaging is experiencing growing interference. When these satellites reflect sunlight, they produce streak-like artifacts in photometry images. Such satellite trails can introduce false sources and cause significant photometric errors. As a result, accurately identifying the positions of satellite trails in observational data has become essential. In this work, we propose a satellite trail detection model that combines the U-Net deep neural network for image segmentation with the Line Segment Detector (LSD) algorithm. The model is trained on 375 simulated images of satellite trails, generated using data from the Mini-SiTian Array. Experimental results show that for trails with a signal-to-noise ratio (SNR) greater than 3, the detection rate exceeds 99. Additionally, when applied to real observational data from the Mini-SiTian Array, the model achieves a recall of 79.57 and a precision of 74.56.