# Searching for Moving Objects in HSC-SSP: Pipeline and Preliminary   Results

**Authors:** Ying-Tung Chen, Hsing-Wen Lin, Mike Alexandersen, Matthew J. Lehner,, Shiang-Yu Wang, Jen-Hung Wang, Fumi Yoshida, Yutaka Komiyama, Satoshi, Miyazaki

arXiv: 1705.01722 · 2018-02-14

## TL;DR

This paper presents a new pipeline for detecting trans-Neptunian objects in the HSC-SSP survey data, overcoming the survey's non-optimized cadence and dithering patterns, and reports preliminary detection results.

## Contribution

The authors develop a novel detection pipeline that re-arranges survey data, applies machine learning to filter false positives, and links orbits to identify TNOs in a non-dedicated survey.

## Key findings

- Successfully identified TNO candidates in early HSC-SSP data
- Demonstrated the pipeline's effectiveness despite survey limitations
- Provided initial catalog of detected TNOs

## Abstract

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is currently the deepest wide- field survey in progress. The 8.2 m aperture of Subaru telescope is very powerful in detect- ing faint/small moving objects, including near-Earth objects, asteroids, centaurs and Tran- Neptunian objects (TNOs). However, the cadence and dithering pattern of the HSC-SSP are not designed for detecting moving objects, making it difficult to do so systematically. In this paper, we introduce a new pipeline for detecting moving objects (specifically TNOs) in a non-dedicated survey. The HSC-SSP catalogs are re-arranged into the HEALPix architecture. Then, the stationary detections and false positive are removed with a machine learning al- gorithm to produce a list of moving object candidates. An orbit linking algorithm and visual inspections are executed to generate the final list of detected TNOs. The preliminary results of a search for TNOs using this new pipeline on data from the first HSC-SSP data release (Mar 2014 to Nov 2015) are also presented.

## Full text

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## Figures

12 figures with captions in the complete paper: https://tomesphere.com/paper/1705.01722/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1705.01722/full.md

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Source: https://tomesphere.com/paper/1705.01722