Volume 550, February 2013
|Number of page(s)||12|
|Published online||29 January 2013|
Variability and the X-ray/UV ratio of active galactic nuclei⋆
II. Analysis of a low-redshift Swift sample
1 Dipartimento di Fisica, Università di Roma “Tor Vergata”, via della Ricerca Scientifica 1, 00133 Roma, Italy
2 Dipartimento di Fisica, Università di Roma “La Sapienza”, Piazzale Aldo Moro 2, 00185 Roma, Italy
Received: 25 September 2012
Accepted: 14 December 2012
Context. Variability, both in X-ray and optical/UV, affects the well-known anti-correlation between the αox spectral index and the UV luminosity of active galactic nuclei, contributing part of the dispersion around the average correlation (intra-source dispersion) in addition to the differences among the time-average αox values from source to source (inter-source dispersion).
Aims. We aim to evaluate the intrinsic αox variations in individual objects and their effect on the dispersion of the αox − LUV anti-correlation.
Methods. We used simultaneous UV/X-ray data from Swift observations of a low-redshift sample to derive the epoch-dependent αox(t) indices. We corrected for the host galaxy contribution by a spectral fit of the optical/UV data. We computed ensemble structure functions to analyse the variability of multi-epoch data.
Results. We find a strong intrinsic αox variability, which significantly contributes (~40% of the total variance) to the dispersion of the αox − LUV anti-correlation (intra-source dispersion). The strong X-ray variability and weaker UV variability of this sample are comparable to other samples of low-z active galactic nuclei, and are neither caused by the high fraction of strongly variable narrow line Seyfert 1 galaxies, nor by dilution of the optical variability by the host galaxies. Dilution instead affects the slope of the anti-correlation, which steepens, once corrected, and becomes similar to higher luminosity sources. The structure function of αox increases with the time lag up to about one month. This indicates the important contribution of the intermediate-to-long timescale variations, which are possibly generated in the outer parts of the accretion disk.
Key words: surveys / galaxies: active / quasars: general / X-rays: galaxies
Table 1 is available in electronic form at http://www.aanda.org
© 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.