You Only Stack Once (YOSO): A Motion-Filtered, Deep-Learning Framework for Detecting Faint Moving Sources
Nitya Pandey, César Fuentes, Pedro Bernardinelli, Valeria Frías, Colin Orion Chandler + 13 more
TLDR
YOSO is a motion-filtered deep-learning framework that detects faint, slow-moving Solar System objects in wide-field astronomical surveys.
Key contributions
- Introduces YOSO, an automated pipeline for detecting faint, slow-moving Solar System objects.
- Integrates a novel Gaussian Motion Filter (GMoF) to enhance signal-to-noise at the pixel level.
- GMoF amplifies object trails while suppressing random noise and static background features.
- Achieves a very low false positive rate by verifying detected sources exhibit trails and point-source consistency.
Why it matters
YOSO offers a versatile and scalable solution for detecting faint, slow-moving objects in astronomical surveys, crucial for the era of data-intensive astronomy. Its novel motion filter and low false positive rate make it a significant advancement over traditional methods.
Original Abstract
We present You Only Stack Once (YOSO), an automated pipeline designed to detect faint, slow-moving Solar System objects in wide-field astronomical surveys. The pipeline integrates a novel Gaussian Motion Filter (GMoF) that operates at the pixel level to enhance signal-to-noise for objects exhibiting a range of apparent rates of motion. Unlike conventional shift-and-stack methods, which rely on discrete velocity trials, GMoF amplifies trails while suppressing random noise and static background features. Applied to a subset of DEEP observations from the Dark Energy Camera, YOSO recovered 45 out of 73 previously detected objects, as well as 11 new TNOs. It also discovered 216 objects in the near Solar System. Although alternative shift-and-stack methods are sensitive to objects about 0.88 magnitudes fainter, YOSO's false positive rate is extremely low, since it detects only sources that exhibit a trail and are consistent with a point source when shifted at the right rate. We show how this method can be deployed on large surveys like LSST, and adapted for other domains that require motion-based signal enhancement, including exoplanet imaging through Angular Differential Imaging (ADI), and near-Earth object (NEO) detection for missions like NEO Surveyor. YOSO thus provides a versatile, scalable approach for extracting faint, motion-dependent signals in the era of data-intensive astronomy.
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