被识别为双线和三线的光谱信息及其视向速度
Shanshan Li ; Chunqian Li ; Yunfei Xu ; Linying Mi ; Chenzhou Cui ; Jianrong Shi ; Changhua Li ; Dongwei Fan
main表格：分类结果表包括视向速度值及其相关误差。列包括：A(J2000)；DEC(J2000)；来自Gaia DR3的Gaia源ID；G(mag)是Gaia的G星等；Multiplicity是分类结果；planID是来自LAMOST-MRS的计划名称；spID是来自LAMOST-MRS的光谱仪ID；fiberID是来自LAMOST-MRS的目标光纤ID；LMJM显示曝光开始时的本地修正儒略分；S/N代表所有像素的中位信噪比；RV1 (km/s)，RV2 (km/s)，和RV3 (km/s)，是使用CCF计算出的RV值，并按照它们的值排序。表格的完整版本包含30,288行。 common表格：与其他双星星表交叉后得到的SB2和SB3侯选体列表列表。
文件
main.txt
3.93 MB
common.txt
190.09 kB
论文信息
论文标题:
Mining double-line spectroscopic candidates in the LAMOST medium-resolution spectroscopic survey using human-AI hybrid method
发表期刊:
Astrophysical Journal Supplement Series
标识符
CSTR:
11379.11.101517
DOI:
10.12149/101517
VO Identifier:
ivo://China-VO/paperdata/101517
发布时间:
2024-11-22
使用统计
总下载量
253
引用
Shanshan Li et al. 2024. The information of the spectra identified as double- and triple-line, along with their RVs.. 版本 1.0. https://doi.org/10.12149/101517
@misc{10.12149/101517,
doi = {10.12149/101517},
url = {https://doi.org/10.12149/101517},
author = {Shanshan Li},
title = {The information of the spectra identified as double- and triple-line, along with their RVs.},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2024}
}
doi = {10.12149/101517},
url = {https://doi.org/10.12149/101517},
author = {Shanshan Li},
title = {The information of the spectra identified as double- and triple-line, along with their RVs.},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2024}
}
版本