Figure 6.
![Performance evaluation of stellar atmospheric parameters (Teff, $\log \, g$, [Fe/H]) estimated by SPEMR on spectra with different S/N. The S/N intervals are $\rm 10 \le S/N \lt 20$, $\rm 20 \le S/N \lt 40$, $\rm 40 \le S/N \lt 60$, and $\rm 60 \le S/N \lt 100$, respectively. The vertical axis presents the distribution of differences between SPEMR predictions and ASPCAP results on the test set.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/523/4/10.1093_mnras_stad1778/1/stad1778fig6.jpeg?Expires=1749317282&Signature=HC3VCtfAf-I7dBGqGJXm71tYmWCijrt9c8K6VBg4pMcWO28Of9m9hfEzpKKkYXdtHiVguzHbB8Rb~0NLdj7Z5lafH9e2ifgyHbNJNRV~XWkg4JLvZiAyo-xnfs0PQ79-qtmM0jv8FW6xTrwLKS-Rn6yrDze2jbZp68rLxY8z5SPO1ZIudnHY4EBRiIoQ-g7MJ6PGdjKqSbZG8D72-d2lGDnKCHhHlrml2WXRobuY30exjfBPu6aJ0U8FhivORIPlWXqo5jMeN5jGRix-aT73l8vnZ~9byxqat5h2lacDf2cbLw1MbvIEB4cnqH2vnR2AWIYNHHSArR7etLS~K09cbw__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Performance evaluation of stellar atmospheric parameters (Teff, |$\log \, g$|, [Fe/H]) estimated by SPEMR on spectra with different S/N. The S/N intervals are |$\rm 10 \le S/N \lt 20$|, |$\rm 20 \le S/N \lt 40$|, |$\rm 40 \le S/N \lt 60$|, and |$\rm 60 \le S/N \lt 100$|, respectively. The vertical axis presents the distribution of differences between SPEMR predictions and ASPCAP results on the test set.
