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

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Table 7:

Same as Table 6, but now with a cutoff value of 2.0 for the Mahalanobis distance to the class centre.
	IRa01			LRc01			SRc01			LRa01
Class code	All	p>0.5	p>0.7	All	p>0.5	p>0.7	All	p>0.5	p>0.7	All	p>0.5	p>0.7
BCEP	49	47	35	11	10	30	36	32	26	38	37	30
BE	969	923	753	425	398	453	1448	1414	1189	709	668	453
CLCEP	0	0	0	0	0	1	0	0	0	1	1	1
CP	92	68	20	80	57	26	78	62	15	96	64	26
DMCEP	0	0	0	0	0	0	0	0	0	0	0	0
DSCUT	128	126	124	38	38	150	66	66	61	158	157	150
ECLF	112	112	112	95	95	118	82	82	82	118	118	118
ECLP	56	56	55	30	30	63	49	49	47	64	64	63
ELL	2	1	1	3	3	1	4	4	2	1	1	1
GDOR	44	35	18	7	6	14	30	24	11	31	24	14
LAPV	353	347	303	161	154	223	155	153	142	257	250	223
LBOO	6	6	4	1	1	1	2	2	1	2	1	1
MIRA	0	0	0	0	0	0	0	0	0	0	0	0
PTCEP	0	0	0	1	0	0	0	0	0	0	0	0
PVSG	3862	3794	3416	6762	6692	6210	3059	3020	2691	6820	6721	6210
RRAB	0	0	0	1	1	0	0	0	0	0	0	0
RRC	0	0	0	0	0	0	0	0	0	0	0	0
RRD	0	0	0	1	1	0	0	0	0	0	0	0
RVTAU	0	0	0	0	0	0	0	0	0	0	0	0
SPB	78	76	73	18	18	95	33	33	31	101	99	95
SR	5	5	2	5	2	0	1	0	0	0	0	0

Source LaTeX | All tables | In the text

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