X-ray evidence for a mildly relativistic and variable outflow in the luminous Seyfert 1 galaxy Mrk 509

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Table 2:

3.5-10.5 keV continuum and Fe emission line parameters.
N $^{\circ}$	$\Gamma$	Energy¹	EW²	Flux³	$\chi^2/\nu$	$\Delta \chi ^2$
		(keV)	(eV)
1	$1.55\pm0.03$	$6.37\pm0.03$	$82\pm40$	3.0	924/850	61
2	$1.60\pm0.03$	$6.41\pm0.04$	$60\pm30$	3.8	992/991	42
4	$1.70\pm0.02$	$6.41\pm0.02$	$65\pm20$	3.5	1151/1194	130
5	$1.72\pm0.03$	$6.41\pm0.03$	$62\pm28$	3.6	990/1012	67
6	$1.69\pm0.02$	$6.43\pm0.03$	$58\pm20$	4.2	1175/1189	101

¹ Emission line rest-frame energy centroid, in units of keV; ² Emission line rest-frame equivalent width, in units of eV. The width of the line was fixed to $\sigma=0.1$ keV (see text for details); ³ 2-10 keV flux in units of 10^-11 erg s^-1 cm^-2.

Source LaTeX | All tables | In the text

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