Deep-HiTS: Rotation Invariant Convolutional Neural Network for Transient Detection
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Abstract (arXiv)
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.
Key facts. Cited by 12 papers in the map (data through 7 Oct 2026). First posted on arXiv 2 Jan 2017.
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Citing papers per year: 2021: 3; 2022: 3; 2023: 2; 2024: 0; 2025: 3; 2026: 1.
12 papers.
- 2022What's the Difference? The potential for Convolutional Neural Networks for transient detection without template subtractioncited by 4
- 2022Analysis of convolutional neural network image classifiers in a rotationally symmetric modelcited by 4
- 2021PNet -- A Deep Learning Based Photometry and Astrometry Bayesian Frameworkcited by 3
- 2023Domain Adaptation via Minimax Entropy for Real/Bogus Classification of Astronomical Alertscited by 3
- 2021MeerCRAB: MeerLICHT Classification of Real and Bogus Transients using Deep Learningcited by 1
- 2021The effect of phased recurrent units in the classification of multiple catalogs of astronomical lightcurvescited by 1
- 2025GMR-Conv: An Efficient Rotation and Reflection Equivariant Convolution Kernel Using Gaussian Mixture Ringscited by 1
- 2022Identifying Transients in the Dark Energy Survey using Convolutional Neural Networkscited by 0
- 2023Benefits of mirror weight symmetry for 3D mesh segmentation in biomedical applicationscited by 0
- 2025Equivariant Imaging Biomarkers for Robust Unsupervised Segmentation of Histopathologycited by 0
- 2025Pre-training vision models for the classification of alerts from wide-field time-domain surveyscited by 0
- 2026Identifying Gems from Roman RAPIDlycited by 0
- 2026Identifying Gems from Roman RAPIDly3 Jun 2026
- 2025Pre-training vision models for the classification of alerts from wide-field time-domain surveys12 Dec 2025
- 2025Equivariant Imaging Biomarkers for Robust Unsupervised Segmentation of Histopathology8 May 2025
- 2025GMR-Conv: An Efficient Rotation and Reflection Equivariant Convolution Kernel Using Gaussian Mixture Rings3 Apr 2025
- 2023Benefits of mirror weight symmetry for 3D mesh segmentation in biomedical applications29 Sep 2023
- 2023Domain Adaptation via Minimax Entropy for Real/Bogus Classification of Astronomical Alerts15 Aug 2023
- 2022Analysis of convolutional neural network image classifiers in a rotationally symmetric model11 May 2022
- 2022Identifying Transients in the Dark Energy Survey using Convolutional Neural Networks18 Mar 2022
- 2022What's the Difference? The potential for Convolutional Neural Networks for transient detection without template subtraction14 Mar 2022
- 2021PNet -- A Deep Learning Based Photometry and Astrometry Bayesian Framework28 Jun 2021
- 2021The effect of phased recurrent units in the classification of multiple catalogs of astronomical lightcurves7 Jun 2021
- 2021MeerCRAB: MeerLICHT Classification of Real and Bogus Transients using Deep Learning28 Apr 2021