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. 16

Precision computed as the standard deviation of the CNN minus APOGEE (solid lines) and calibrated GSP-Spec minus APOGEE (dashed lines) as a function of S/N bins for 41 623 stars of the training sample (orange) and 76 996 stars of the observed sample (green, within the training sample limits).

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