Multifrequency variability of the blazar AO 0235+164 the WEBT campaign in 2004-2005 and long-term SED analysis
Journal
Date Issued
2006
Author(s)
•
•
Kadler, M.
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Ibrahimov, M.A.
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Kurtanidze, O.M.
•
Larionov, V.M.
•
Tornikoski, M.
•
Boltwood, P.
•
Lee, C.-U.
•
Aller, M.F.
•
Romero, G.E.
•
Aller, H.D.
•
Araudo, A.T.
•
Arkharov, A.A.
•
Bach, U.
•
Barnaby, D.
•
Berdyugin, A.
•
•
Carini, M.T.
•
Carosati, D.
•
Cellone, S.A.
•
Cool, R.
•
•
Efimova, N.V.
•
Fuhrmann, L.
•
Hagen-Thorn, V.A.
•
Holcomb, M.
•
Ilyin, I.
•
Impellizzeri, V.
•
Ivanidze, R.Z.
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Kapanadze, B.Z.
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Kerp, J.
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Konstantinova, T.S.
•
Kovalev, Y.Y.
•
Kovalev, Yu.A.
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Kraus, A.
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Krichbaum, T.P.
•
Lähteenmäki, A.
•
•
•
Lindfors, E.
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Mattox, J.R.
•
•
Nikolashvili, M.G.
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Nilsson, K.
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Ohlert, J.
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Papadakis, I.E.
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Pasanen, M.
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Poteet, C.
•
Pursimo, T.
•
Ros, E.
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Sigua, L.A.
•
Smith, S.
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Takalo, L.O.
•
•
Tröller, M.
•
•
Ungerechts, H.
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Walters, R.
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Witzel, A.
•
Xilouris, E.
Abstract
A huge multiwavelength campaign targeting the blazar AO 0235+164 was
organized by the Whole Earth Blazar Telescope (WEBT) in 2003-2005 to study the
variability properties of the source. Monitoring observations were carried out
at cm and mm wavelengths, and in the near-IR and optical bands, while three
pointings by the XMM-Newton satellite provided information on the X-ray and UV
emission. We present the data acquired during the second observing season,
2004-2005, by 27 radio-to-optical telescopes. They reveal an increased near-IR
and optical activity with respect to the previous season. Increased variability
is also found at the higher radio frequencies, down to 15 GHz, but not at the
lower ones. The radio (and optical) outburst predicted to peak around
February-March 2004 on the basis of the previously observed 5-6 yr
quasi-periodicity did not occur. The analysis of the optical light curves
reveals now a longer characteristic time scale of 8 yr, which is also present
in the radio data. The spectral energy distributions corresponding to the
XMM-Newton observations performed during the WEBT campaign are compared with
those pertaining to previous pointings of X-ray satellites. Bright, soft X-ray
spectra can be described in terms of an extra component, which appears also
when the source is faint through a hard UV spectrum and a curvature of the
X-ray spectrum. Finally, there might be a correlation between the X-ray and
optical bright states with a long time delay of about 5 yr, which would require
a geometrical interpretation.
Volume
459
Issue
3
Start page
731
Issn Identifier
0004-6361
Ads BibCode
2006A&A...459..731R
Rights
open.access
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