Suzaku observations of moderately obscured (Compton-thin) Active Galactic Nuclei selected by Swift/BAT Hard X-ray Survey
T Kawamuro, Y Ueda, F Tazaki, C Ricci… - The Astrophysical …, 2016 - iopscience.iop.org
We report the results obtained by a systematic, broadband (0.5–150 keV) X-ray spectral
analysis of moderately obscured (Compton-thin, $22\leqslant\mathrm {log}{N} _ {{\rm {H}}}\lt …
analysis of moderately obscured (Compton-thin, $22\leqslant\mathrm {log}{N} _ {{\rm {H}}}\lt …
Highly ionized disc and transient outflows in the Seyfert galaxy IRAS 18325–5926
We report on strong X-ray variability and the Fe K-band spectrum of the Seyfert galaxy IRAS
18325–5926 obtained from the 2001 XMM-Newton EPIC pn observation with a duration of …
18325–5926 obtained from the 2001 XMM-Newton EPIC pn observation with a duration of …
X-ray time delays from the Seyfert 2 galaxy IRAS 18325− 5926
AP Lobban, WN Alston… - Monthly Notices of the …, 2014 - academic.oup.com
Using new XMM–Newton observations we detect hard X-ray time lags in the rapid variability
of the Compton-thin Seyfert 2 galaxy IRAS 18325− 5926. The higher-energy X-ray variations …
of the Compton-thin Seyfert 2 galaxy IRAS 18325− 5926. The higher-energy X-ray variations …
The iron K line profile of IRAS 18325–5926
AP Lobban, S Vaughan - Monthly Notices of the Royal …, 2014 - academic.oup.com
Abstract IRAS 18325− 5926 is an X-ray bright, Compton-thin, type 2 Seyfert galaxy and it
was the first Seyfert 2 in which the presence of a broad Fe Kα emission line was claimed …
was the first Seyfert 2 in which the presence of a broad Fe Kα emission line was claimed …
X-ray time delays from the Seyfert 2 galaxy IRAS 18325− 5926
SA Vaughan, AP Lobban - 2014 - figshare.le.ac.uk
Using new XMM–Newton observations we detect hard X-ray time lags in the rapid variability
of the Compton-thin Seyfert 2 galaxy IRAS 18325− 5926. The higher-energy X-ray variations …
of the Compton-thin Seyfert 2 galaxy IRAS 18325− 5926. The higher-energy X-ray variations …
The iron K line profile of IRAS 18325–5926
SA Vaughan, AP Lobban - 2014 - figshare.le.ac.uk
IRAS 18325− 5926 is an X-ray bright, Compton-thin, type 2 Seyfert galaxy and it was the first
Seyfert 2 in which the presence of a broad Fe Kα emission line was claimed. However …
Seyfert 2 in which the presence of a broad Fe Kα emission line was claimed. However …