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Stellar X-Ray Activity and Habitability Revealed by the ROSAT Sky Survey
DOI: 10.3847/1538-4365/ad4b17 Bibcode: 2024ApJS..273....8H

Liu, Jifeng; Wang, Song; Li, Xue +3 more

Using the homogeneous X-ray catalog from ROSAT observations, we conducted a comprehensive investigation into stellar X-ray activity–rotation relations for both single and binary stars. Generally, the relation for single stars consists of two distinct regions: a weak decay region, indicating a continued dependence of the magnetic dynamo on stellar …

2024 The Astrophysical Journal Supplement Series
Gaia 1
The Measurement of Masses of OB-type Stars from LAMOST DR5
DOI: 10.3847/1538-4365/ad0fe7 Bibcode: 2024ApJS..271...15H

Liu, Chao; Liu, Zhicun; Cui, Wenyuan +5 more

The measurements of masses and luminosities of massive stars play an important role in understanding the formation and evolution of their host galaxies. In this work, we present the measurement of masses and luminosities of 2946 OB-type stars, including 78 O-type stars and 2868 B-type stars, based on their stellar parameters (effective temperature…

2024 The Astrophysical Journal Supplement Series
Gaia 0
Se-ResNet+SVM Model: An Effective Method of Searching for Hot Subdwarfs from LAMOST
DOI: 10.3847/1538-4365/ad5b61 Bibcode: 2024ApJS..274....2C

Wu, Tianmin; Yi, Zhenping; Lei, Zhenxin +7 more

This paper presents a robust neural network approach for identifying hot subdwarfs. Our method leveraged the Squeeze-and-Excitation Residual Network to extract abstract features, which were combined with experience features to create hybrid features. These hybrid features were then classified using a support vector machine. To enhance accuracy, we…

2024 The Astrophysical Journal Supplement Series
Gaia 0
An Efficient Method for Batch Derivation of Detached Eclipsing Binary Parameters: Analysis of 34,907 OGLE Systems
DOI: 10.3847/1538-4365/ad833c Bibcode: 2024ApJS..275...12W

Liu, Wei; Ding, Xu; Ji, KaiFan +3 more

Detached eclipsing binary (EB) systems are crucial for measuring the physical properties of stars that evolve independently. Large-scale time-domain surveys have released a substantial number of light curves for detached EBs. Utilizing the Physics of Eclipsing Binaries package in conjunction with Markov Chain Monte Carlo (MCMC) methods for batch p…

2024 The Astrophysical Journal Supplement Series
Gaia 0
Estimating Stellar Atmospheric Parameters and [α/Fe] for LAMOST O-M-type Stars Using a Spectral Emulator
DOI: 10.3847/1538-4365/ad7505 Bibcode: 2024ApJS..275....8L

Luo, A. -Li; Li, Yin-Bi; Kong, Xiao +7 more

In this paper, we developed a spectral emulator based on the Mapping Nearby Galaxies at Apache Point Observatory Stellar Library (MaStar) and a grouping optimization strategy to estimate effective temperature (T eff), surface gravity (log g), metallicity ([Fe/H]), and the abundance of alpha elements with respect to iron ([α/Fe]) for O-M…

2024 The Astrophysical Journal Supplement Series
Gaia 0
X-Ray Emission of Nearby Low-mass and Sunlike Stars with Directly Imageable Habitable Zones
DOI: 10.3847/1538-4365/ad71d6 Bibcode: 2024ApJS..275....1B

Peacock, Sarah; Kane, Stephen R.; Schwieterman, Edward W. +5 more

Stellar X-ray and UV radiation can significantly affect the survival, composition, and long-term evolution of the atmospheres of planets in or near their host star's habitable zone (HZ). Especially interesting are planetary systems in the solar neighborhood that may host temperate and potentially habitable surface conditions, which may be analyzed…

2024 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 0
LEAVES: An Expandable Light-curve Data Set for Automatic Classification of Variable Stars
DOI: 10.3847/1538-4365/ad785b Bibcode: 2024ApJS..275...10F

Chen, Xiaodian; Fei, Ya; Yu, Ce +6 more

With the increasing amount of astronomical observation data, it is an inevitable trend to use artificial intelligence methods for automatic analysis and identification of light curves for full samples. However, data sets covering all known classes of variable stars that meet all research needs are not yet available. There is still a lack of standa…

2024 The Astrophysical Journal Supplement Series
Gaia 0
Physical Parameters and Magnetic Activity of M-type Stars Based on the LAMOST DR9, SDSS, and TESS Surveys
DOI: 10.3847/1538-4365/ad72f2 Bibcode: 2024ApJS..274...36L

Han, Xianming L.; Misra, Prabhakar; Zhang, Li-yun +3 more

We analyze a catalog comprising 781,232 spectra from 641,095 M dwarf stars from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) low-resolution spectroscopic data release 9. Based on the equivalent width of the Hα line, we ascertain the activity properties of the stars, identifying a total of 107,134 active stars, with 31,175…

2024 The Astrophysical Journal Supplement Series
Gaia 0
Atomic Transition Probabilities for Ultraviolet and Optical Lines of Tm II
DOI: 10.3847/1538-4365/ad614f Bibcode: 2024ApJS..274....9D

Roederer, I. U.; Den Hartog, E. A.; Voith, G. T.

We report new branching fraction measurements for 224 ultraviolet and optical transitions of Tm II. These transitions range in wavelength (wavenumber) from 2350 to 6417 Å (42,532–15,579 cm‑1) and originate in 13 odd-parity and 24 even-parity upper levels. Thirty-five of the 37 levels, accounting for 213 of the 224 transitions, are studi…

2024 The Astrophysical Journal Supplement Series
eHST 0
The Value-added Catalog of OB Stars in LAMOST DR7
DOI: 10.3847/1538-4365/ad833f Bibcode: 2024ApJS..275...24L

Shi, Jianrong; Liu, Zhicun; Cui, Wenyuan +4 more

In this work, we update the catalog of OB stars based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 7 and modify the OB stars' selection criteria in spectral line indices' space. The new catalog includes 37,778 spectra of 27,643 OB stars, of which 3827 OB stars are newly identified. The spectral subclasses of 27,643…

2024 The Astrophysical Journal Supplement Series
Gaia 0