Error Correction Factors of Observational Parameters(DR7_v2.0)
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 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.
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Error Correction Factors of Observational Parameters.csv
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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:
10.12149/101178
VO Identifier:
ivo://China-VO/paperdata/RAA/2022zhangshuhui/101178
Publication Date:
2022-12-13
Citation Guidelines
Zhengyi Shao et al. 2022. Error Correction Factors of Observational Parameters(DR7_v2.0). Version 2.0. https://doi.org/10.12149/101178
@misc{10.12149/101178,
doi = {10.12149/101178},
url = {https://doi.org/10.12149/101178},
author = {Zhengyi Shao},
title = {Error Correction Factors of Observational Parameters(DR7_v2.0)},
version = {2.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
doi = {10.12149/101178},
url = {https://doi.org/10.12149/101178},
author = {Zhengyi Shao},
title = {Error Correction Factors of Observational Parameters(DR7_v2.0)},
version = {2.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
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This DOI represents all versions, and will always resolve to the latest one.
2022-12-12