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Table 3

Number of good candidate variability class members obtained without and with the use of additional spectral classification attributes.

Variability class # (LC attributes only) # (Teff and log   (g) added) # (additional inspection)

γ Dor 159 330
δ Sct 285 343
SPB 207 8
β Cep 86 6
RR Lyrae (RRab) 4
RR Lyrae (RRd) 1
Binaries (eclipsing/ellipsoidal) 259
Rotational modulation 203
Be 9
Hybrid γ Dor/δ Sct 28

Notes.The last column lists variables discovered by additional inspection of the Giraffe spectra and the CoRoT light curves.

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