Automated supervised classification of variable stars in the CoRoT programme - Method and application to the first four exoplanet fields

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Table 2:

Variability classes whose definition stars have been extended/replaced with CoRoT data, and the number of definition CoRoT light curves used.
Stellar variability class	$\char93$ CoRoT LCs
Variable Be-stars	5
$\beta$ -Cephei stars	6
$\delta$ -Scuti stars	23
Ellipsoidal variables	7
$\gamma$ -Doradus stars	2
Slowly Pulsating B-stars	21
Eclipsing binaries	31
RR-Lyrae, type ab	3
Double mode RR-Lyrae stars	1
Low-amplitude periodic variables	15

Source LaTeX | All tables | In the text

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