X-ray spectral variability of seven LINER nuclei with XMM-Newton and Chandra data

Free Access

Issue		A&A Volume 556, August 2013


Article Number		A47
Number of page(s)		31
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201321563
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

Summary.

© ESO, 2013

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.