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Deep-HiTS: Rotation Invariant Convolutional Neural Network for Transient Detection

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arxiv 1701.00458 v1 pith:KBJV65G3 submitted 2017-01-02 astro-ph.IM cs.CV

classification astro-ph.IMcs.CV
keywords transientdeep-hitsmodelapproachapproximatelycandidatescnnsconvolutional
verification ladder T0 review T1 audit T2 compute T3 formal
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We introduce Deep-HiTS, a rotation invariant convolutional neural network (CNN) model for classifying images of transients candidates into artifacts or real sources for the High cadence Transient Survey (HiTS). CNNs have the advantage of learning the features automatically from the data while achieving high performance. We compare our CNN model against a feature engineering approach using random forests (RF). We show that our CNN significantly outperforms the RF model reducing the error by almost half. Furthermore, for a fixed number of approximately 2,000 allowed false transient candidates per night we are able to reduce the miss-classified real transients by approximately 1/5. To the best of our knowledge, this is the first time CNNs have been used to detect astronomical transient events. Our approach will be very useful when processing images from next generation instruments such as the Large Synoptic Survey Telescope (LSST). We have made all our code and data available to the community for the sake of allowing further developments and comparisons at https://github.com/guille-c/Deep-HiTS.

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  1. The classification of real and bogus transients using active learning and semi-supervised learning

    astro-ph.IM 2024-12 conditional novelty 4.0 of 10

    RB-C1000, a pipeline combining active learning and semi-supervised pseudo-labeling, achieves roughly 98.8% real/bogus classification accuracy on new ZTF datasets using only 1,000 labels.

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