A correlation between the spectral and timing properties of AGN

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Volume 494 / No 3 (February II 2009)

A&A, 494 3 (2009) 905-913

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Table 1:

Black hole mass and timing properties of the AGN in the sample.
Name	$M_{\rm BH}/10^6$ $M_{\odot}$	Ref.	$\nu_{\rm br}/10^{-7}$ Hz	Ref.
Fairall 9	$255\pm 56$	P04	$\rm 4.0^{+2.3}_{-0}$	MA03
PG 0804+761	$693\pm 83$	P04	9.6	PA03
NGC 3227	$42\pm 21$	P04	$\rm 200^{+250}_{-140}$	UM05
NGC 3516	$43\pm 15$	P04	$\rm 20^{+30}_{-10}$	MA03
NGC 3783	$30\pm 5$	P04	$\rm 40^{+37}_{-20}$	MA03
NGC 4051	1.9 $\pm 0.8$	P04	$\rm 5050^{+1100}_{-3000}$	M04
NGC 4151	$13\pm 5$	P04	$\rm 13^{+19}_{-4}$	MA03
Mrk 766	3.5	W02	$\rm 6100^{+3500}_{-2500}$	V03
NGC 4258	$39\pm 1$	H99	$\rm0.2^{+23}_{-0}$	MA05
NGC 4395	$0.05\pm 0.05$	V05	$\rm 19\,300^{+9600}_{-15000}$	V05
MCG -6-30-15	$4.5\pm 1.5$	M05	$\rm 770^{+1200}_{-310}$	M05
NGC 5506	88	PA04	$\rm 130^{+830}_{-72}$	UM05
NGC 5548	$67\pm 3$	P04	$\rm 6.3^{+19}_{-0}$	MA03
Ark 564	$2.6\pm 0.3$	B04	$\rm 23\,000^{+5800}_{-6600}$	PA02

Reference used for $M_{\rm BH}$ : B04: Botte et al. (2004); H99 - Hernstein et al. (1999); M05 - M $^{\rm c}$ Hardy et al. (2005); PA04 - Papadakis (2004); P04 - Peterson et al. (2004); V05: Vaughan et al. (2005); W02 - Woo & Urry (2002). Reference used for $\nu_{\rm br}$ : MA03 - Markowitz et al. (2003); M04 - M $^{\rm c}$ Hardy et al. (2004); PA02 - Papadakis et al. (2002); PA03 - Papadakis et al. 2003; V03 - Vaughan & Fabian (2003).

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