WebGitHub - fandongwei/pylamost: Python interface for LAMOST Data fandongwei / pylamost Public Notifications Fork Star master 1 branch 0 tags Code 15 commits Failed to load latest commit information. .gitignore LICENSE README.md acess_web.py notebook.tex pylamost-test.ipynb pylamost.py sample.txt README.md pylamost Python interface for … WebDec 28, 2024 · For main-sequence stars, the stellar parameters inferred from the official LAMOST Stellar Parameter Pipeline (LASP) are demonstrated to be accurate [typical uncertainties: σ T eff = 100 K, σ log g = 0.1 − 0.15 decimal exponent (dex, referring to a factor of ten), σ [Fe / H] = 0.1 dex] from comparisons with high-resolution spectroscopic …
LAMOST stellar parameter pipeline at Peking University …
WebIt is special reflecting Schmidt telescope with 4000 fibers in a field of view of 20 deg2 in the sky. Until July 2014, LAMOST has completed its pilot survey which was launched in … WebAug 14, 2012 · An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.pdf: 119. Asteroseismology of 1523 new red giants observed by Kepler Jie Yu, Daniel Huber, Timothy R. Bedding, et al. MNRAS 463 1297 2016 Yu Jie-MNRAS(2016).pdf: 120. LAMOST SPECTROGRAPH RESPONSE CURVES: STABILITY AND APPLICATION TO FLUX … c.s lewis style till we have faces
Ultracool dwarfs identified using spectra in LAMOST DR7
WebJul 1, 2015 · The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) project performed its five year formal survey since Sep. 2012, already fulfilled the pilot … WebLAMOST pipeline, not only the systematic overestimation for the RGB stars has been corrected, but also the artificial effect around the red clump stars disappears. Moreover, even the red bump stars, which extend to only about 0.1dex in logg, can be discriminated from the new estimated surface gravity. http://dr5.lamost.org/v3/doc/data-production-description c s lewis tao