Anatomy of the AGN in NGC 5548 - I. A global model for the broadband spectral energy distribution

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Table 3

Observed fluxes and intrinsic luminosities of NGC 5548 for 2000, 2001, and stacked 2013 data.


Observation	F _{0.3−2 keV}	L _{0.3−2 keV}	F _{2−10 keV}	L _{2−10 keV}	F _{0.001−10 keV}	L _{0.001−10 keV}	F _{1−1000 Ryd}	L _{1−1000 Ryd}

2000 (24 Dec.)	2.34	2.53	3.14	2.17	13.1	18.4	6.50	12.2
2001 (09 July)	2.72	2.47	3.87	2.67	13.6	15.8	8.04	10.9
2001 (12 July)	3.74	3.44	4.90	3.39	16.5	19.6	10.5	14.4
2013 (Summer)	0.30	2.21	2.80	2.35	10.5	17.9	4.09	11.7

Notes. The fluxes (F) are given in units of 10^-11 erg cm^-2 s^-1 and the intrinsic luminosities (L) are in 10⁴³ erg s^-1. The observed fluxes include all the absorptions described in Sects. 4.6–4.8. The host galaxy stellar emission (Sect. 4.2) is excluded from the reported flux and luminosities.

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