LAMOST_DIBs
Kefei Wu
This is a catalog of 11,003 sources with distinct DIB features. The catalog presents information of sources including the star designation, ra, dec, and the RVs, EWs, and FWHMs of the three DIB features, as well as their errors.The “flag” represents the DIB is measured through the spectrum of an early-type star or FGK-type star, 1= ”early-type”, while 0=”FGK-type”.
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Paper Information
Paper Title:
Diffuse interstellar bands λ6379, λ6614, and λ6660 in the LAMOST-MRS spectra
Publication:
Research in Astronomy and Astrophysics
Identifiers
CSTR:
11379.11.101123
DOI:
10.12149/101123
VO Identifier:
ivo://China-VO/paperdata/101123
Publication Date:
2022-06-13
Citation Guidelines
Kefei Wu et al. 2022. LAMOST_DIBs. Version 1.0. https://doi.org/10.12149/101123
@misc{10.12149/101123,
doi = {10.12149/101123},
url = {https://doi.org/10.12149/101123},
author = {Kefei Wu},
title = {LAMOST_DIBs},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
doi = {10.12149/101123},
url = {https://doi.org/10.12149/101123},
author = {Kefei Wu},
title = {LAMOST_DIBs},
version = {1.0},
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.
2022-06-13