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

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Table 8:

Same as Table 6, but now with a cutoff value of 1.0 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	22	21	17	6	6	4	16	15	13	14	14	14
BE	296	268	195	157	135	77	483	461	371	275	242	127
CLCEP	0	0	0	0	0	0	0	0	0	0	0	0
CP	76	55	17	51	36	9	71	57	14	63	42	20
DMCEP	0	0	0	0	0	0	0	0	0	0	0	0
DSCUT	74	74	73	24	24	24	38	38	38	92	92	91
ECLF	107	107	107	93	93	93	74	74	74	117	117	117
ECLP	46	46	46	26	26	25	42	42	41	59	59	58
ELL	1	1	1	1	1	0	3	3	2	1	1	1
GDOR	19	19	12	5	4	2	15	13	6	21	16	10
LAPV	204	202	189	59	59	50	80	80	76	128	125	116
LBOO	1	1	1	1	1	1	0	0	0	1	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	1263	1220	1004	2102	2049	1773	639	613	461	2224	2148	1823
RRAB	0	0	0	1	1	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	0	0	0	0	0	0
SPB	51	51	51	11	11	11	20	20	20	64	64	64
SR	5	5	2	5	2	1	1	0	0	0	0	0

Source LaTeX | All tables | In the text

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