A Robust Hot Subdwarfs Identification Method Based on Deep Learning
Lei Tan, Ying Mei, Zhicun Liu, Yangping Luo, Hui Deng, Feng Wang,, Linhua Deng, Chao Liu

TL;DR
This paper presents a deep learning-based method using CNNs for accurate and automated identification of hot subdwarf stars from spectral data, significantly improving detection efficiency and accuracy.
Contribution
It introduces a hybrid CNN model for hot subdwarf identification, achieving over 96% accuracy and enabling large-scale spectral classification.
Findings
Achieved 96.17% accuracy on test set
Validated 96.05% accuracy on independent sample
Discovered 25 new hot subdwarfs through manual validation
Abstract
Hot subdwarf star is a particular type of star that is crucial for studying binary evolution and atmospheric diffusion processes. In recent years, identifying Hot subdwarfs by machine learning methods has become a hot topic, but there are still limitations in automation and accuracy. In this paper, we proposed a robust identification method based on the convolutional neural network (CNN). We first constructed the dataset using the spectral data of LAMOS DR7-V1. We then constructed a hybrid recognition model including an 8-class classification model and a binary classification model. The model achieved an accuracy of 96.17% on the testing set. To further validate the accuracy of the model, we selected 835 Hot subdwarfs that were not involved in the training process from the identified LAMOST catalog (2428, including repeated observations) as the validation set. An accuracy of 96.05% was…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Code & Models
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomical Observations and Instrumentation · Stellar, planetary, and galactic studies
