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Fig. 2.

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Gallery of XP spectra for Gaia objects with SDSS-confirmed spectroscopic type (indicated in the top right corner of each panel). Three spectra of varying G magnitudes are displayed to illustrate the difference between brighter and fainter stars. Spectral lines typically used for classification are displayed for reference (see text). The Gaia DR3 source identification and the spectroscopic type probability predicted by our classifiers (Pclass) are also shown.

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