Error Correction Factors of Observational Parameters
Zhengyi Shao
Column 1 is the LAMOST IDs of the objects, columns 2-3 are the ID and duplicate observation numbers of stars in the duplicate SP-sample, columns 4-5 are the spectroscopy types classified by the LAMOST 1D pipeline and the LAMOST spectral S/N of g-band, columns 6-10 are the correction factors (k) of each parameter.
Files
table3-Error Correction Factors of Observational Parameters.csv
937.00 B
Paper Information
Paper Title:
Correction factors of the measurement errors of the LAMOST-LRS stellar parameters
Publication:
Research in Astronomy and Astrophysics
Identifiers
CSTR:
10.12149/101178
DOI:
10.12149/101177
VO Identifier:
ivo://China-VO/paperdata/RAA/2022zhangshuhui/101177
Publication Date:
2022-12-12
Citation Guidelines
Zhengyi Shao et al. 2022. Error Correction Factors of Observational Parameters. Version 1.0. https://doi.org/10.12149/101177
@misc{10.12149/101177,
doi = {10.12149/101177},
url = {https://doi.org/10.12149/101177},
author = {Zhengyi Shao},
title = {Error Correction Factors of Observational Parameters},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
doi = {10.12149/101177},
url = {https://doi.org/10.12149/101177},
author = {Zhengyi Shao},
title = {Error Correction Factors of Observational Parameters},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
Versions
Main
This DOI represents all versions, and will always resolve to the latest one.
2022-12-12