Volume 556, August 2013
|Number of page(s)||31|
|Published online||23 July 2013|
F-test and χ2/d.o.f. applied to the SMF0.
F-test and χ2/d.o.f. applied to the SMF1.
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.
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.
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.
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).
UV luminosities derived from the OM observations. Name (Col. 1), obs ID (Col. 2), filter (Col. 3) and luminosity (Col. 4).
© ESO, 2013
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