Half a Million Binary Stars from the low resolution spectra of LAMOST
Yingjie Jing, Tian-Xiang Mao, Jie Wang, Chao Liu, and Xiaodian Chen

TL;DR
This paper introduces a CNN-based method to identify binary stars from low-resolution LAMOST spectra, resulting in a catalog of nearly half a million binaries that enhances understanding of stellar populations.
Contribution
The study presents a novel CNN approach trained on spectral data to detect binary stars, achieving high accuracy and producing a large, validated binary star catalog from LAMOST and Gaia data.
Findings
Achieved 0.949 AUC in binary star classification.
Detected 97% of known eclipsing binaries.
Catalog includes 468,634 binary stars, some beyond 10 kpc.
Abstract
Binary stars are prevalent yet challenging to detect. We present a novel approach using convolutional neural networks (CNNs) to identify binary stars from low-resolution spectra obtained by the LAMOST survey. The CNN is trained on a dataset that distinguishes binaries from single main sequence stars based on their positions on the Hertzsprung-Russell diagram. Specifically, the training data labels stars with mass ratios between approximately 0.71 and 0.93 as intermediate mass ratio binaries, while excluding those beyond this range. The network achieves high accuracy with an area under the receiver operating characteristic curve of 0.949 on the test set. Its performance is further validated against known eclipsing binaries (97% detection rate) and binary stars identified by radial velocity variations (92% detection rate). Applying the trained CNN to a sample of one million main sequence…
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.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies
