Free Access
Volume 556, August 2013
Article Number A47
Number of page(s) 31
Section Extragalactic astronomy
Published online 23 July 2013

Online material

Table 2

Observational details.

Table 3

F-test and χ2/d.o.f. applied to the SMF0.

Table 4

F-test and χ2/d.o.f. applied to the SMF1.

Table 5

Final compilation of the best-fit models for the sample, including the individual best-fit model for each observation, and the simultaneous best-fit model with the varying parameters.

Table 6

Soft (0.5–2 keV) and hard (2–10 keV) intrinsic luminosities for individual (Cols. 3 and 5) and simultaneous (Cols. 4 and 6) fitting.

Table 7

Results for the best fit of the annular region (ring) in Chandra data, and the best fit obtained for the nucleus of XMM-Newton data when the contribution from the annular region was removed.

Table 8

Simultaneous fittings taking into account the contribution from the annular region given in Table 7.

Table 9

Statistics for the light curves. Name (Col. 1), obs ID (Col. 2), χ2/d.o.f. and the probability of being variable (Cols. 3 and 4) and normalized excess variance with errors (Cols. 5 and 6).

Table 10

UV luminosities derived from the OM observations. Name (Col. 1), obs ID (Col. 2), filter (Col. 3) and luminosity (Col. 4).

Table 11


© ESO, 2013

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