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Related papers: Study of X-ray reflection features in a sample of …

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(Abridged) We present the results of fitting ASCA spectra of six narrow-line Seyfert 1 (NLS1) galaxies with the ionised reflection models of Ross & Fabian (1993). We find that five of the galaxies (TONS 180, PKS 0558-504, Ark 564, Mrk 335…

Astrophysics · Physics 2009-09-17 D. R. Ballantyne , K. Iwasawa , A. C. Fabian

We present and discuss BeppoSAX observations of Mrk841 and Mrk335, two Seyfert 1 galaxies in which previous observations have established the presence of soft excesses. We confirm the soft excess in both sources, even if for Mrk~841 a warm…

Astrophysics · Physics 2009-11-06 S. Bianchi , G. Matt , F. Haardt , L. Maraschi , F. Nicastro , G. C. Pero la , P. O. Petrucci , L. Piro

We present a detailed analysis of the XMM-Newton observations of five narrow-line Seyfert 1 galaxies (NLS1s). They all show very soft continuum emission in the X-ray band with a photon index of $\Gamma\gtrsim 2.5$. Therefore, they are…

High Energy Astrophysical Phenomena · Physics 2022-05-18 Jiachen Jiang , Luigi C. Gallo , Andrew C. Fabian , Michael L. Parker , Christopher S. Reynolds

We present a spectral variability study of the XMM-Newton and Suzaku observations of one of the most extreme Narrow Line Seyfert 1 galaxies, IRAS13224-3809. The X-ray spectrum is characterized by two main peculiar features, i) a strong soft…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 G. Ponti , L. C. Gallo , A. C. Fabian , G. Miniutti , A. Zoghbi , P. Uttley , R. R. Ross , R. V. Vasudevan , Y. Tanaka , W. N. Brandt

A model for the inner regions of accretion flows is presented where, due to disc instabilities, cold and dense material is clumped into deep sheets or rings. Surrounding these density enhancements is hot, tenuous gas where coronal…

Astrophysics · Physics 2009-11-07 A. C. Fabian , D. R. Ballantyne , A. Merloni , S. Vaughan , K. Iwasawa , Th. Boller

We present new results from BeppoSAX observations of reflection-dominated Seyfert galaxies, and namely: 1) the Compton-thick Seyfert 2s NGC1068 and Circinus Galaxy; 2) the Seyfert 1 NGC4051, whose nucleus was observed on May 1998 to have…

Astrophysics · Physics 2009-10-31 M. Guainazzi , G. Matt , F. Fiore

In active galactic nuclei, X-ray illumination of the accretion disk around a supermassive black hole (SMBH) results in the production of the K$\alpha$ fluorescent line of iron, which provides insights into accretion physics and SMBH spins.…

High Energy Astrophysical Phenomena · Physics 2025-03-13 A. Danehkar , W. N. Brandt

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric…

High Energy Astrophysical Phenomena · Physics 2017-03-08 Yanjun Xu , Mislav Balokovic , Dominic J. Walton , Fiona A. Harrison , Javier A. Garcia , Michael J. Koss

BeppoSAX observed the Seyfert 1 galaxy NGC 3783 for ~ 5 days from 1998 June 6 to 1998 June 10. The average flux during the observation was F(2-10 keV) ~ 6 X 10^{-11} erg cm^-2 s^-1. The long exposure provided a very high quality spectrum…

Astrophysics · Physics 2009-11-07 A. De Rosa , L. Piro , F. Fiore , P. Grandi , L. Maraschi , G. Matt , F. Nicastro , P. O. Petrucci

Over the last few years X-ray observations of broad-line radio galaxies (BLRGs) by ASCA, RXTE and BeppoSAX have shown that these objects seem to exhibit weaker X-ray reflection features (such as the iron K\alpha line) than radio-quiet…

Astrophysics · Physics 2009-11-07 D. R. Ballantyne , R. R. Ross , A. C. Fabian

We report on the first detection above ~10 keV of the archetypal Compton-thick Seyfert 2 galaxy NGC 1068. This detection, obtained with the PDS instrument onboard BeppoSAX in the 20-100 keV range, confirms the hardness of the X--ray…

We present the spectral analysis of an early XMM-Newton observation of the luminous Seyfert 1 galaxy Markarian 509. We find the hard (2-10 keV) continuum slope, including reflection, to be somewhat flatter ($\Gamma=1.75$) than for a typical…

Astrophysics · Physics 2009-11-06 Ken Pounds , James Reeves , Paul O'Brien , Kim Page , Martin Turner , Sergei Nayakshin

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being a sum of components reflected/scattered from cold (neutral)…

Astrophysics · Physics 2009-11-11 K. Pounds , S. Vaughan

We present results from fitting ionized accretion disc models to three long ASCA observations of the Seyfert 1 galaxy MCG--6-30-15. All three datasets can be fit by a model consisting of ionized reflection from the inner region of the…

Astrophysics · Physics 2009-11-06 D. R. Ballantyne , A. C. Fabian

We review recent progress on the modeling and use of reflection spectra from irradiated and ionized accretion discs. On the computational side, calculations of reflection spectra from discs with non-uniform density structure have shown that…

Astrophysics · Physics 2007-05-23 D. R. Ballantyne , R. R. Ross , A. C. Fabian

A long 280 ks observation of the Seyfert 1 galaxy NGC 3783 with XMM-Newton is reported. We focus on the oxygen line complex between 17 and 24 A as measured with the RGS spectrometers. Accurate absorption column densities and emission line…

Multi-epoch XMM-Newton spectra of the two Narrow Line Seyfert 1 (NLS1), Mrk 478 and EXO 1346.2+2645, are presented. The data were fitted with different models, including the relativistically-blurred reflection model reflionx, which was…

Astrophysics · Physics 2009-11-13 A. Zoghbi , A. C. Fabian , L. C. Gallo

We present an analysis of XMM-Newton observations of eleven Seyfert galaxies that appear to be missing a broad iron K alpha line. These objects represent a challenge to the established paradigm for active galactic nuclei, where a relatively…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Shyam Bhayani , Kirpal Nandra

Active galactic nuclei host an accretion disc with an X-ray producing corona around a supermassive black hole. In bright sources, such as the Seyfert 1 galaxy Mrk 335, reflection of the coronal emission off the accretion disc has been…

High Energy Astrophysical Phenomena · Physics 2015-12-15 L. Keek , D. R. Ballantyne

We report the results obtained by a broad-band (0.5-500 keV) data analysis of narrow-line Seyfert 1 galaxy NGC 4748 observed with an XMM-Newton/PN, INTEGRAL/ISGRI and SWIFT/BAT telescopes. This galaxy has a soft X-ray excess that is typical…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Anatoliy Vasylenko
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