Figure 9.
![Distribution of dwarfs (log g > 4) in [X/Fe]–[Fe/H] space. The two left-hand columns are the estimation results of the GALAH catalogue, and the two right-hand columns are the estimation results of the StarGRUNet-LAMOST catalogue. The colour intensity characterizes the density of the sample distribution.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/521/4/10.1093_mnras_stad831/1/stad831fig9.jpeg?Expires=1749317435&Signature=tONM52xFj0xkUcYiBiTUIcek5bZMDNMEH1kYrdU6I3KTYSn2cNy8ZbKorXK4SzbA9yeyG1JL4fxITs5ZVxJhXQ3n2rkabGcj~wE2j7Rgy4RRBsHXVCLkVPl6I~zuD2-noyLcEbkZI-f1UKfji1I-EwrVPtjgHxhP1i90Hk~Fbp5rkNA6Ej~~vCskvd60gkwROdm-1BOJn0xOFV~PtqisRlZk~pZFis3raCz2BbbYN~77-l7Cz7knAewJgRbwK7W7vgYJX5ZcOzfNttH3rpV5EarMUKxnSPBa3SJ-fsI2nHuYRrb1OiRZ~duIVMYa-FPUzQWJ-IJOMNxtOHlc9iooaw__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Distribution of dwarfs (log g > 4) in [X/Fe]–[Fe/H] space. The two left-hand columns are the estimation results of the GALAH catalogue, and the two right-hand columns are the estimation results of the StarGRUNet-LAMOST catalogue. The colour intensity characterizes the density of the sample distribution.
