Search Publications

On why the iron K-shell absorption in AGN is not a signature of the local warm/hot intergalactic medium
DOI: 10.1111/j.1745-3933.2008.00443.x Bibcode: 2008MNRAS.385L.108R

Done, Chris; Terashima, Yuichi; Hayashida, Kiyoshi +5 more

We present a comparison between the 2001 XMM-Newton and 2005 Suzaku observations of the quasar, PG1211+143, at z = 0.0809. Variability is observed in the 7 keV iron K-shell absorption line (at 7.6 keV in the quasar frame), which is significantly weaker in 2005 than during the 2001 XMM-Newton observation. From a recombination time-scale of <4 yr…

2008 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 149
Suzaku observations of Markarian 335: evidence for a distributed reflector
DOI: 10.1111/j.1365-2966.2008.12844.x Bibcode: 2008MNRAS.384.1316L

Larsson, J.; Ponti, G.; Fabian, A. C. +3 more

We report on a 151-ks net exposure Suzaku observation of the narrow-line Seyfert 1 galaxy Mrk 335. The 0.5-40 keV spectrum contains a broad Fe line, a strong soft excess below about 2 keV and a Compton hump around 20-30 keV. We find that a model consisting of a power law and two reflectors provides the best fit to the time-averaged spectrum. In th…

2008 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 38
Exploring the disc/jet interaction in the radio-loud quasar 4C+74.26 with Suzaku
DOI: 10.1111/j.1365-2966.2008.13497.x Bibcode: 2008MNRAS.388.1037L

Larsson, J.; Fabian, A. C.; Miniutti, G. +1 more

We report on a 90 ks Suzaku observation of the radio-loud quasar 4C+74.26. The source was observed in its highest flux state to date, and we find that it brightened by about 20 per cent during the observation. We see evidence of spectral hardening as the count rate increases and also find that the rms variability increases with energy up to about …

2008 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku XMM-Newton 24
Swift captures the spectrally evolving prompt emission of GRB070616
DOI: 10.1111/j.1365-2966.2007.12763.x Bibcode: 2008MNRAS.384..504S

Page, M. J.; Norris, J. P.; O'Brien, P. T. +14 more

The origins of gamma-ray burst (GRB) prompt emission are currently not well understood and in this context long, well-observed events are particularly important to study. We present the case of GRB070616, analysing the exceptionally long-duration multipeaked prompt emission, and later afterglow, captured by all the instruments on-board Swift and b…

2008 Monthly Notices of the Royal Astronomical Society
Suzaku 21