Characterizing Orbital Parameters of Hot Subdwarf Binaries with Multiple Spectroscopic Surveys
XInlin Zhao, Song Wang, Zhenxin Lei, Yangyang Dong, Buhui Lv, Chuanjie Zheng, Xiaohong Yang, Jifeng Liu
astro-ph.SR
Submitted: 2026-06-16
Comments: 26 pages, 15 figures, accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The MUCHFUSS project - Searching for the most massive companions to hot subdwarf stars in close binaries and finding the least massive ones
- Squeeze-and-Excitation Networks
- A brief introductory guide to TLUSTY and SYNSPEC
- Spectrophotometry and period analysis of the sdB eclipsing binary HW Virginis
- Deep learning-driven atmospheric parameter prediction for hot subdwarf stars with synthetic and observed spectra
- LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan
- Wide sdB binaries. I. Orbital and atmospheric parameters
- Synthetic spectra for O and B type subdwarf stars
- The peculiar sdB NGC6121-V46: A low-mass double degenerate ellipsoidal variable in a globular cluster
- Hot Subdwarfs in Binaries as the Source of the Far-UV Excess in Elliptical Galaxies
- Observing Orbital Decay in the Ultracompact Hot Subdwarf Binary System ZTFJ213056.71+442046.5
- CBAM: Convolutional Block Attention Module
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