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Table · dataset · 2022

Stellar parameters of LAMOST stars using SLAM

Listed in IVOA Registry (Virtual Observatory)

The LAMOST survey has provided 9 million spectra in its Data Release 5 (DR5) at R~1800.

Description

Extracting precise stellar labels is crucial for such a large sample. In this paper, we report the implementation of the Stellar LAbel Machine (SLAM), which is a data-driven method based on support vector regression (SVR), a robust nonlinear regression technique.

Thanks to the capability to model highly nonlinear problems with SVR, SLAM can generally derive stellar labels over a wide range of spectral types. This gives it a unique capability compared to other popular data-driven methods. To illustrate this capability, we test the performance of SLAM on stars ranging from Teff~4000 to ~8000K trained on LAMOST spectra and stellar labels.

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At g-band signal-to-noise ratio (S/Ng) higher than 100, the random uncertainties of Teff, logg, and [Fe/H] are 50K, 0.09dex, and 0.07dex, respectively. We then set up another SLAM model trained by APOGEE and LAMOST common stars to demonstrate its capability of dealing with high dimensional problems. The spectra are from LAMOST DR5 and the stellar labels of the training set are from APOGEE DR15, including Teff, logg, [M/H], [{alpha}/M], [C/M], and [N/M].

The cross-validated scatters at S/N_g_~100 are 49K, 0.10dex, 0.037dex, 0.026dex, 0.058dex, and 0.106dex for these parameters, respectively. This performance is at the same level as other up-to-date data-driven models.

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Catalogue records · 2

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