Figure 1.
![The dependencies of the error of the stellar atmospheric parameters (Teff, log g, and [Fe/H]) on SNRg. The spectral data are from the 115 942 common stars between LAMOST and APOGEE. The error refers to the MAE between the APOGEE_payne labels and the LASP estimations.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/514/3/10.1093_mnras_stac1625/1/stac1625fig1.jpeg?Expires=1749316868&Signature=Xkrf-AiSEU3-k9mtuYSWGURSx3KyfksSfyDBp8UpPVtaO8~JSIJNrLBhXOBY1gi0k9UvYaIpP--woPiU5P1JvXj1XQ5QmXwm7GalElKdTVEQ1iowomq-EMMgafDraKQzOD1R9fCcQsKXiRz1qaDXwfcWj58UTG8xRtpgZXbND2UTpcGA-WyGB9hyyqjthVkzrBC-X4o6o9qVo4lL6nKS5gKL4ol2AyBz2oSMcKlcqnF-jJdCL4pFrjf1KE7vdeMQjsZqM3X6gjCApnHNDRip5eu5KtNENs2Cz~A2ou4HK~yvB4UyW-htlAKyTzqQyxUxC8JMOlODgHUdlkZsKjwkgg__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
The dependencies of the error of the stellar atmospheric parameters (Teff, log g, and [Fe/H]) on SNRg. The spectral data are from the 115 942 common stars between LAMOST and APOGEE. The error refers to the MAE between the APOGEE_payne labels and the LASP estimations.
