Photometric Data-driven Classification of Type Ia Supernovae in the Open Supernova Catalog
arXiv:2006.10489 · doi:10.1016/j.ascom.2021.100451
Abstract
We propose a novel approach for a machine-learning-based detection of the type Ia supernovae using photometric information. Unlike other approaches, only real observation data is used during training. Despite being trained on a relatively small sample, the method shows good results on real data from the Open Supernovae Catalog. We also investigate model transfer from the PLAsTiCC simulations train dataset to real data application, and the reverse, and find the performance significantly decreases in both cases, highlighting the existing differences between simulated and real data.
27 pages, 10 figures, accepted for publication in Astronomy and Computing
References in corpus (7)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- The NumPy array: a structure for efficient numerical computation
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics
- The Spectroscopic Diversity of Type Ia Supernovae
- SuperRAENN: A Semi-supervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium Deep Survey Supernovae
- Photometric classification of HSC transients using machine learning
Cited by in corpus (4)
- Pan-chromatic photometric classification of supernovae from multiple surveys and transfer learning for future surveys
- Understanding of the properties of neural network approaches for transient light curve approximations
- Supernova Light Curves Approximation based on Neural Network Models
- Optimizing Supernova Classification with Interpretable Machine Learning Models