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Dataset of artefacts for machine learning applications in astronomy

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arxiv 2504.08053 v1 pith:PUV5Y46T submitted 2025-04-10 astro-ph.IM

classification astro-ph.IM
keywords artefactsdatadatasetanomalyapplicationsavailabledatasetsdetection
verification ladder T0 review T1 audit T2 compute T3 formal
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Accurate photometry in astronomical surveys is challenged by image artefacts, which affect measurements and degrade data quality. Due to the large amount of available data, this task is increasingly handled using machine learning algorithms, which often require a labelled training set to learn data patterns. We present an expert-labelled dataset of 1127 artefacts with 1213 labels from 26 fields in ZTF DR3, along with a complementary set of nominal objects. The artefact dataset was compiled using the active anomaly detection algorithm PineForest, developed by the SNAD team. These datasets can serve as valuable resources for real-bogus classification, catalogue cleaning, anomaly detection, and educational purposes. Both artefacts and nominal images are provided in FITS format in two sizes (28 x 28 and 63 x 63 pixels). The datasets are publicly available for further scientific applications.

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  1. What ZTF Saw Where Rubin Looked: Anomaly Hunting in DR23

    astro-ph.IM 2025-07 conditional novelty 5.0 of 10

    Applying the SNAD PineForest anomaly detector to ZTF DR23 light curves in LSSTComCam fields uncovered six uncatalogued variable stars and improved parameters for six known variables.

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