Probing variability patterns of the Fe K line complex in bright nearby AGNs

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Table 1:

Relevant features detected in the time-averaged spectra of the observations.
Source	Redshifted emission features	Broad Fe K $\alpha$	Highly Ionized Fe K $\alpha$ /Fe K $\beta$	Absorption features
IC 4329a	670^*		670^*	670^**
MCG -5-23-16	363^*, 1099^		1099^*
NGC 3783	193^, 371^, 372^*		193^, 371^, 372^*	193^,, 372^
NGC 3516	245^, 352^, 1250^**	1251^*		1250^, 1251^, 1252^, 1253^
MRK 509			250^, 1073^, 1074^*, 1168^	1073^*, 1168^,**
MCG -6-30-15	108A^, 302^, 303^*	108A^*, 301^, 303^*	303^**	108A^*
MCG +8-11-11			794^**
NGC 7314			256^*
ARK 120		679^*	679^*
MRK 279				1088^*,
NGC 3227	1279^*
IRAS 05078+1626			1410^**
MRK 590			837^*
MRK 766	265^*, 999^, 1000^, 1001^, 1002^, 1003^	1000^, 1001^, 1003^, 1004^*	82^, 265^, 999^*, 1000^, 1001^, 1002^
NGC 7469			912^**
MCG -2-58-22		180^**
NGC 526A			647^*	647^**
NGC 4051	263^, 541^		541^**	263^**
ESO 141-G055		1435A^, 1435B^, 1436^*	1436^*, 1445^	1445^*
ESO 198-G024		207^**		1128^**
AKN 564		930^*
NGC 7213			269^**
NGC 4593			465^*

^* Detection significance > $4\sigma$ ; ^** detection significance between $\sim$ $3\sigma$ -4 $\sigma$ .

Source LaTeX | All tables | In the text

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