Anatomy of the AGN in NGC 5548 - IV. The short-term variability of the outflows

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Volume 579 (July 2015)

A&A, 579 (2015) A42

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Table 1

List of XMM-Newton and Chandra data sets used for present analysis.

Obs.	Date	Satellites	F _{2030 Å} ^a	F _{0.3−2.0 keV} ^b	F _{2.0−10.0 keV} ^b
	yyyy-mm-dd		(10^-14 ergs^-1cm^-2A^-1)	(10^-12ergs^-1cm^-2)

XM1	2013-06-22	1 4	2.07	1.1	13.2
XM2	2013-06-30	1 4	2.28	3.5	29.9
XM3	2013-07-07	1 4	2.07	2.1	21.2
XM4	2013-07-11	1 4	2.32	3.6	32.1
XM5	2013-07-15	1 4	2.57	2.6	26.9
XM6	2013-07-19	1 4	2.74	2.3	27.4
XM7	2013-07-21	1 4	2.88	2.3	23.5
XM8	2013-07-23	1 4	3.09	2.2	25.1
XM9	2013-07-25	1 4	2.97	3.2	29.8
XM10	2013-07-27	1 4	3.29	3.0	29.4
XM11	2013-07-29	1 4	3.21	2.8	26.4
XM12	2013-07-31	1 4	3.21	2.2	23.6

CH1	2013-09-01	2 4	4.54	7.7	38.7
CH2	2013-09-02	2 4	4.48	4.4	29.7
CH3	2013-09-10	2 3 4	4.89	5.7	36.1

XM13	2013-12-20	1 4	3.27	2.1	21.8
XM14	2014-02-05	1 4	3.49	4.1	24.4

Notes. Instruments are labeled with numbers, as followed: 1: XMM-Newton, 2: Chandra, 3: NUSTAR, and 4: Swift.

^(a)

UV flux measured by Swift-UVOT, corrected for reddening.

^(b)

Observed flux in the quoted bands, as derived from our best-fit model.

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