Radio and X-ray observations of an exceptional radio flare in the extreme z= 4.72 blazar GB B1428+4217 |
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| Authors: | M A Worsley A C Fabian G G Pooley C J Chandler |
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| Institution: | Institute of Astronomy, Madingley Road, Cambridge CB3 0HA;Mullard Radio Astronomy Observatory, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE;National Radio Astronomy Observatory, 1003 Lopezville Road, PO Box 0, Socorro, NM 87801, USA |
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| Abstract: | We report on the extreme behaviour of the high-redshift blazar GB B1428+4217 at z = 4.72 . A continued programme of radio measurements has revealed an exceptional flare in the light curve, with the 15.2-GHz flux density rising by a factor of ～3 from ～140 to ～430 mJy in a rest-frame time-scale of only ～4 months – much larger than any previous flares observed in this source. In addition to new measurements of the 1.4–43 GHz radio spectrum, we also present the analysis and results of a target-of-opportunity X-ray observation using XMM–Newton , made close to the peak in radio flux. Although the X-ray data do not show a flare in the high-energy light curve, we are able to confirm the X-ray spectral variability hinted at in previous observations. GB B1428+4217 is one of several high-redshift radio-loud quasars that display a low-energy break in the X-ray spectrum, probably due to the presence of excess absorption in the source. X-ray spectral analysis of the latest XMM–Newton data is shown to be consistent with the warm-absorption scenario which we have hypothesized previously. Warm absorption is also consistent with the observed X-ray spectral variability of the source, in which the spectral changes can be successfully accounted-for with a fixed column density of material in which the ionization state is correlated with hardness of the underlying power-law emission. |
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| Keywords: | galaxies: active galaxies: individual: GB B1428+4217 X-rays: galaxies |
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