Table 2: Observed and predicted line fluxes of 2XMM J123204+215255.
Line Observed flux^a Predicted flux^b Corrected flux $A_\lambda^c$

[erg cm^-2 s^-1] [erg cm^-2 s^-1] [erg cm^-2 s^-1] [mag]

H $\alpha$ $(5\pm0.2)\times10^{-16}$ $1.7\times10^{-14}$ $4.6\times10^{-15}$ 2.4

H $\beta$ < $1\times10^{-16}$ $4.8\times10^{-15}$ - 5.3

[O III] < $3\times10^{-17}$ $2.9\times10^{-15}$ - -

^a Uncorrected for extinction, measured from the IR spectrum.
^b From the correlations of Panessa et al. (2006).
^c Extinction estimated from the model.

**Table 2:** Observed and predicted line fluxes of 2XMM J123204+215255.
Line	Observed flux^a	Predicted flux^b	Corrected flux	$A_\lambda^c$
	[erg cm^-2 s^-1]	[erg cm^-2 s^-1]	[erg cm^-2 s^-1]	[mag]
H $\alpha$	$(5\pm0.2)\times10^{-16}$	$1.7\times10^{-14}$	$4.6\times10^{-15}$	2.4
H $\beta$	< $1\times10^{-16}$	$4.8\times10^{-15}$	-	5.3
[O III]	< $3\times10^{-17}$	$2.9\times10^{-15}$	-	-

Source LaTeX | All tables | In the text