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

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Table 6:

Same as Table 5, but now obtained with the GM classifier, with no restriction on 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	63	58	40	14	13	9	41	35	26	42	40	33
BE	1207	1157	941	520	490	349	1563	1528	1262	867	825	577
CLCEP	0	0	0	0	0	0	0	0	0	1	1	1
CP	93	69	21	93	69	27	82	66	17	97	65	27
DMCEP	0	0	0	0	0	0	0	0	0	0	0	0
DSCUT	151	146	141	45	45	43	69	69	64	197	195	179
ECLF	118	118	115	98	97	95	86	86	82	124	122	120
ECLP	57	57	55	34	31	29	56	52	47	67	64	63
ELL	3	2	1	3	3	1	6	6	4	1	1	1
GDOR	49	39	20	8	7	4	33	27	13	35	28	18
LAPV	420	413	355	196	187	143	167	165	150	305	297	254
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	2	2	1	0	0	0
PVSG	7605	7533	7055	10355	10284	9829	4780	4740	4309	9545	9444	8880
RRAB	0	0	0	2	2	1	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	1	0	0	0	0	0	0
RVTAU	0	0	0	0	0	0	5	5	4	0	0	0
SPB	92	89	83	32	32	27	37	36	33	125	122	114
SR	5	5	2	5	2	1	43	42	40	0	0	0

Source LaTeX | All tables | In the text

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