The information of the spectra identified as double- and triple-line, along with their RVs.
李珊珊 ; 李春乾 ; 许允飞 ; 米琳莹 ; 崔辰州 ; 施建荣 ; 李长华 ; 樊东卫
main: The table presents the classification outcomes, including RV values and associated errors. The columns are: A(J2000); DEC(J2000); Gaia source ID from Gaia DR3; G(mag) is the G magnitude from Gaia; Multiplicity, which is the result of the classification; planID is the plan name from LAMOST-MRS; spID is the spectrograph ID from LAMOST-MRS; fiberID is the fiber ID of the target from LAMOST-MRS; LMJM,showing the local modified Julian Minute at the start of exposure; S/N representing the median S/N of all pixels; RV1 (km/s), RV2 (km/s), and RV3 (km/s), which are the RVs calculated from the first step using the conventional CCF technique and arranged in order of their values. The full version of this table with 30,288 rows. common: The list of common SB2 and SB3 candidates with other binary catalogs.
Files
.. main.txt
3.93 MB
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.. common.txt
190.09 kB
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Paper Information
Paper Title:
Mining double-line spectroscopic candidates in the LAMOST medium-resolution spectroscopic survey using human-AI hybrid method
Publication:
Astrophysical Journal Supplement Series
Identifiers
CSTR:
11379.11.101517
DOI:
10.12149/101517
VO Identifier:
ivo://China-VO/paperdata/101517
Publication Date:
2024-11-22
Citation Guidelines
李珊珊 et al. 2024. The information of the spectra identified as double- and triple-line, along with their RVs.. Version 1.0. https://doi.org/10.12149/101517
@misc{10.12149/101517,
doi = {10.12149/101517},
url = {https://doi.org/10.12149/101517},
author = {李珊珊},
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}
}
Versions
Version 1.0 (current)
2024-11-22
Main
This DOI represents all versions, and will always resolve to the latest one.
2024-11-22