Spectroscopic follow-up of variability-selected active galactic nuclei in the Chandra Deep Field South

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Table 3:

Summary of variability and X-ray results in the area with X-ray information.
	Galaxies	NELG	BLAGN	NLAGN^a	Total
Variable sources detected in hard X-rays	1	3	42	0	46
Variable sources not detected in hard X-rays	4	6	5	0	15
Total number of variable sources	5	9	47	0	61
Non variable sources detected in hard X-rays	10	36	13	15	74
Non variable sources not detected in hard X-rays	11	18	5	3	37
Total number of non variable sources	21	54	18	18	111
Total	26	63	65	18	172

^a NLAGN = Narrow Line AGN, reported by Szokoly et al. (2004) as high excitation line
sources (HEX) and by Treister et al. (2008) as obscured AGN (OAGN).

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