本文中使用的LAMOST光谱及补充材料
Guang-Wei Li
本数据集包含宁静和耀发期的原始光谱，和利用方程4和5计算得到的flare-only光谱和Ha发射线光谱。在计算自转速度时，用于表示LAMOST中分辨率仪器轮廓的Th I 6459 也一并给出。从TESS Sector 15，16 和 22的光变曲线得到信息分别在Sector15.pdf，Sector16.pdf 和 Sector22.pdf中给出。vsini.pdf展示了从 Teff = 3500，3600，3700，3800和 3900 K， logg = 4.5 和 5.0 dex模版中获得的最好的自转速度。emissions.csv 给出了从第一条 flare-only光谱中得到的62条发射线。
文件
vsini.pdf
58.10 kB
Sector22.pdf
96.88 kB
Sector16.pdf
598.42 kB
Sector15.pdf
646.42 kB
ThI6459.fits
8.44 kB
quiescence_spectrum.fits
272.81 kB
flare_spectra.fits
1.58 MB
flare_only.fits
1.13 MB
emission_Ha.fits
315.00 kB
emissions.csv
1.42 kB
readme.txt
732.00 B
论文信息
论文标题:
Locate a stellar flare from the M dwarf LAMOST J1332+5057
发表期刊:
The Astrophysical Journal, 1006:170 (12pp), 2026 August 1
Bibcode:
2026ApJ..1006..170L
标识符
CSTR:
11379.11.101659
DOI:
10.12149/101659
VO Identifier:
ivo://China-VO/paperdata/101659
发布时间:
2026-07-28
使用统计
总下载量
188
引用
Guang-Wei Li et al. 2026. LAMOST Spectra used in this paper and supplementary materials. 版本 1.0. https://doi.org/10.12149/101659
@misc{10.12149/101659,
doi = {10.12149/101659},
url = {https://doi.org/10.12149/101659},
author = {Guang-Wei Li},
title = {LAMOST Spectra used in this paper and supplementary materials},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2026}
}
doi = {10.12149/101659},
url = {https://doi.org/10.12149/101659},
author = {Guang-Wei Li},
title = {LAMOST Spectra used in this paper and supplementary materials},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2026}
}
版本