The outflow in Mrk 509 - A method to calibrate XMM-Newton EPIC-pn and RGS

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Table 4:

Emission line parameters for all observations, fluxes are corrected for Galactic absorption.
Line	Observation	Wavelength	Flux	FWHM
		( $\AA$ )	(ph m^-2 s^-1)	( $\AA$ )
O VII r	1	21.602 (f)	3.0 $\pm$ 0.4	0.8 (f)
O VII r	2	21.602 (f)	2.3 $\pm$ 0.6	0.8 (f)
O VII r	3	21.602 (f)	2.3 $\pm$ 0.5	0.8 (f)
O VII r	all	21.602 (f)	2.4 $\pm$ 0.3	0.8 (f)
N VII Ly $\alpha$	1	24.78 (f)	1.0 $\pm$ 0.3	0.8 (f)
N VII Ly $\alpha$	2	24.78 (f)	0.8 $\pm$ 0.4	0.8 (f)
N VII Ly $\alpha$	3	24.78 (f)	1.0 $\pm$ 0.4	0.8 (f)
N VII Ly $\alpha$	all	24.78 (f)	1.1 $\pm$ 0.2	0.8 (f)
O VII f	1	22.07 $\pm$ 0.01	0.6 $\pm$ 0.2	-
O VII f	2	22.07 $\pm$ 0.03	0.2 $\pm$ 0.2	-
O VII f	3	21.99 $\pm$ 0.02	1.0 $\pm$ 0.5	-
O VII f	all	21.99 $\pm$ 0.02	0.30 $\pm$ 0.11	-

Notes. ⁽¹⁾ The (f) indicates that the parameter was kept fixed.

Source LaTeX | All tables | In the text

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