Beyond Gaia DR3: Tracing the [α/M] – [M/H] bimodality from the inner to the outer Milky Way disc with Gaia-RVS and convolutional neural networks

Open Access

Fig. 23

Comparison of CNN [Fe/H] with respect to GALAH DR3 for 10 open clusters. The clusters are listed in the top-left corner. We also computed a mean [Fe/H] and the associated error bar (computed as standard deviation). The mean bias is written next to the cluster name.

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