LAMOST Spectra used in this paper and supplementary materials
Guang-Wei Li
This dataset contains the raw spectra during flare and quienscence used in this paper, as well as the flare-only spectra obtained by Equation 4 and the Ha emission lines obtained by Equation 5. The arc lamp of the Th I 6459 emission line which was used as the LAMOST instrumental profile is also provided. Lightcurve data from TESS Sector 15, 16 and 22 are given in Sector15.pdf, Sector16.pdf and Sector22.pdf, respectively. The best fitted vsini by templates of Teff = 3500, 3600, 3700, 3800,and 3900 K and logg = 4.5 and 5.0 dex are given in vsini.pdf. 62 emission lines identified in the first flare-only spectrum is given in emissions.csv.
Files
vsini.pdf
58.10 kB
Sector22.pdf
96.88 kB
Sector16.pdf
598.42 kB
Sector15.pdf
646.42 kB
ThI6459.fits
8.44 kB
quiescence_spectrum.fits
272.81 kB
flare_spectra.fits
1.58 MB
flare_only.fits
1.13 MB
emission_Ha.fits
315.00 kB
emissions.csv
1.42 kB
readme.txt
732.00 B
Paper Information
Paper Title:
Locate a stellar flare from the M dwarf LAMOST J1332+5057
Publication:
The Astrophysical Journal, 1006:170 (12pp), 2026 August 1
Bibcode:
2026ApJ..1006..170L
Identifiers
CSTR:
11379.11.101659
DOI:
10.12149/101659
VO Identifier:
ivo://China-VO/paperdata/101659
Publication Date:
2026-07-28
Usage Statistics
Total Downloads
260
Citations
Guang-Wei Li et al. 2026. LAMOST Spectra used in this paper and supplementary materials. Version 1.0. https://doi.org/10.12149/101659
@misc{10.12149/101659,
doi = {10.12149/101659},
url = {https://doi.org/10.12149/101659},
author = {Guang-Wei Li},
title = {LAMOST Spectra used in this paper and supplementary materials},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2026}
}
doi = {10.12149/101659},
url = {https://doi.org/10.12149/101659},
author = {Guang-Wei Li},
title = {LAMOST Spectra used in this paper and supplementary materials},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2026}
}
Versions
Main
This DOI represents all versions, and will always resolve to the latest one.
2026-07-28