Fig. 2
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Example spectra of a WDMS binary (top, Gaia ID 1057463111970047488. Note: in this work, we use the DR3 IDs), a cataclysmic variable (middle top: Gaia ID 3703726255561754880), a hot WD (middle bottom: Gaia ID1060659289192635904) and a low-mass low-metallicity subdwarf as revealed by the broad absorption feature at ~7000 Å (bottom: Gaia ID 1048217078174314496) arising from the visual inspection of the Gaia spectra.
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