Fig. B.2
Example of optical spectra obtained with AAT/AAOmega for for stars in the AAOmega field not selected as photometric candidates. Spectra are normalised at 7500 Å and offset for clarity. Left: a sample of field M dwarfs with spectral types ranging from M1 to M6. Right: a sample of late-K/early-M dwarfs, giants, white dwarfs, and young active M dwarfs.
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