Figure 12.
Observation uncertainty of StarGRUNet-LAMOST. The horizontal axis represents the signal-to-noise ratio of the spectra. Each subplot is labelled with the name of the corresponding stellar parameter or elemental abundance in the upper right-hand corner.

Observation uncertainty of StarGRUNet-LAMOST. The horizontal axis represents the signal-to-noise ratio of the spectra. Each subplot is labelled with the name of the corresponding stellar parameter or elemental abundance in the upper right-hand corner.

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