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. 11

Kiel diagrams of 644 287 Gaia-RVS stars in bins of S/N selected within the training sample limits. The stars are colour-coded by metallicity. In the background, we show 2D histograms (in grey) of 197 013 stars that fall outside of the training sample limits.

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