通过SPar方法获得的SMSS DR2中的恒星参数、消光和距离
Mingxu Sun
我们利用SPar算法为来自SkyMapper Southern Survey(SMSS)的1.41亿颗恒星提供了恒星参数,包括有效温度(Teff)、金属丰度(FeH)、绝对星等(M_{G})、距离(d)和消光值(E_{G_{BP},G_{RP}})。该算法采用拟合过程,通过匹配多波段的恒星测光数据,以个别恒星为基础推导出恒星参数(Teff、FeH、M_G、d和E_{G_{BP},G_{RP}})。通过将研究范围扩展到高和低银纬的恒星,本研究成功地纠正了位于低银纬的恒星的消光效应,从而精确确定了它们的恒星参数。
文件
论文信息
论文标题:
Stellar parameters, extinction, and distances for stars in SMSS DR2 by SPar method
发表期刊:
RAA
标识符
CSTR:
11379.11.101372
DOI:
10.12149/101372
VO Identifier:
ivo://China-VO/paperdata/101372
发布时间:
2025-05-13
使用统计
总下载量
196
引用
Mingxu Sun et al. 2025. Stellar parameters, extinction, and distances for stars in SMSS DR2 by SPar method. 版本 1.0. https://doi.org/10.12149/101372
@misc{10.12149/101372,
doi = {10.12149/101372},
url = {https://doi.org/10.12149/101372},
author = {Mingxu Sun},
title = {Stellar parameters, extinction, and distances for stars in SMSS DR2 by SPar method},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
doi = {10.12149/101372},
url = {https://doi.org/10.12149/101372},
author = {Mingxu Sun},
title = {Stellar parameters, extinction, and distances for stars in SMSS DR2 by SPar method},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
版本