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We present the first results of the Hubble Space Telescope/Faint Object Camera long-slit spectroscopy of the inner 8" of the Narrow Line Region of NGC 4151 at a spatial resolution of 0".029. The emission gas is characterized by an…

Astrophysics · Physics 2015-06-24 Claudia Winge , D. J. Axon , F. D. Macchetto , A. Capetti

We present the analysis of X-ray spectral varability made on a sample of 7 Seyfert 1 bright galaxies, using XMM-Newton data. From the "XMM-Newton Science Archive" we selected those bright Seyfert 1 showing one or more prominent flares in…

Astrophysics · Physics 2008-11-26 B. De Marco , M. Cappi , M. Dadina , G. G. C. Palumbo

We present an XMM-Newton observation of the bright, narrow-line, ultrasoft Seyfert 1 galaxy Ton S180. The 0.3-10 keV X-ray spectrum is steep and curved, showing a steep slope above 2.5 keV (Gamma ~ 2.3) and a smooth, featureless excess of…

Astrophysics · Physics 2008-11-26 S. Vaughan , Th. Boller , A. C. Fabian , D. R. Ballantyne , W. N. Brandt , J. Trumper

We present an analysis of the first two XRISM/Resolve spectra of the well-known Seyfert-1.5 active galactic nucleus in NGC 4151, obtained in December 2023. Our work focuses on the nature of the narrow Fe K$_{\alpha}$ emission line at 6.4…

High Energy Astrophysical Phenomena · Physics 2024-08-27 XRISM Collaboration

The notion of source states characterizing the X-ray emission from black hole binaries has revealed to be a very useful tool to disentangle the complex spectral and aperiodic phenomenology displayed by those classes of accreting objects. We…

High Energy Astrophysical Phenomena · Physics 2015-06-16 M. D. Caballero-Garcia , T. Belloni , A. Wolter

We present a detailed analysis of the complex soft X-ray spectrum of NGC 4151 measured by the RGS instruments aboard XMM-Newton. The XMM-Newton RGS spectra demonstrate that the soft X-ray emission is extremely rich in X-ray emission lines…

Astrophysics · Physics 2009-11-10 N. J. Schurch , R. S. Warwick , R. E. Griffiths , S. M. Kahn

We present a detailed, time-resolved analysis of the Fe K band of the Seyfert 1.5 galaxy NGC 3516 observed with XRISM. The 249 ks observation spanning $\sim$310 ks in elapsed time reveals an exceptionally rich and time-variable absorption…

We test the two-corona accretion scenario for active galactic nuclei in the case of the `bare' Seyfert 1 galaxy HE 1143-1810. We perform a detailed study of the broad-band UV--X-ray spectral properties and of the short-term variability. We…

High Energy Astrophysical Phenomena · Physics 2020-02-12 F. Ursini , P. -O. Petrucci , S. Bianchi , G. Matt , R. Middei , G. Marcel , J. Ferreira , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , A. Marinucci , G. Ponti , A. Tortosa

We present the first results from a detailed analysis of a new, long ($\sim100$ ks) XMM-Newton observation of the narrow-line Seyfert 1 galaxy PG 1404$+$226 which showed a large-amplitude, rapid X-ray variability by a factor of $\sim7$ in…

High Energy Astrophysical Phenomena · Physics 2018-08-29 Labani Mallick , Gulab C. Dewangan

We investigate the relationship between the long term X-ray spectral variability in the Seyfert 1.5 galaxy NGC 4151 and its intrinsic absorption, by comparing the 2014 simultaneous ultraviolet/X-Ray observations taken with Hubble STIS…

Astrophysics of Galaxies · Physics 2016-12-21 J. D. Couto , S. B. Kraemer , T. J. Turner , D. M. Crenshaw

We report on the first XMM-Newton observation of the highly X-ray variable, radio-quiet, Narrow-Line Seyfert 1 galaxy IRAS 13224-3809 obtained during the guaranteed time programme with a 64 ks exposure. The most remarkable spectral feature…

Astrophysics · Physics 2009-11-07 Th. Boller , Y. Tanaka , A. Fabian , W. N. Brandt , L. Gallo , N. Anabuki , Y. Haba , S. Vaughan

We present the analysis of multi-wavelength XMM-Newton data from the Seyfert galaxy NGC 3783, including UV imaging, X-ray and UV lightcurves, the 0.2-10 keV X-ray continuum, the iron K-alpha emission line, and high-resolution spectroscopy…

We present the first high-resolution X-ray spectrum of the Seyfert 1.5 galaxy NGC 4151. Observations with the Chandra High Energy Transmission Grating Spectrometer reveal a spectrum dominated by narrow emission lines from a spatially…

Astrophysics · Physics 2009-10-31 P. M. Ogle , H. L. Marshall , J. C. Lee , C. R. Canizares

We report on the XMM-Newton timing properties of the most X-ray variable, radio-quiet, NLS1 IRAS 13224-3809. IRAS 13224-3809 continues to display the extremely variable behavior that was previously observed with ROSAT and ASCA; however, no…

Astrophysics · Physics 2009-09-17 L. C. Gallo , Th. Boller , Y. Tanaka , A. C. Fabian , W. N. Brandt , W. F. Welsh , N. Anabuki , Y. Haba

We investigate the origin of the soft X-ray excess component in Seyfert galaxies observed when their luminosity exceeds 0.1% of the Eddington luminosity ($L_{\mathrm{Edd}}$). The evolution of a dense blob in radiatively inefficient…

High Energy Astrophysical Phenomena · Physics 2020-10-28 Taichi Igarashi , Yoshiaki Kato , Hiroyuki R. Takahashi , Ken Ohsuga , Yosuke Matsumoto , Ryoji Matsumoto

We report on one of the brightest flux levels of the Seyfert 2 galaxy NGC 2992 ever observed in X-rays, on May 2019. The source has been monitored every few days from March 26, 2019 to December 14, 2019 by Swift-XRT, and simultaneous…

High Energy Astrophysical Phenomena · Physics 2020-06-24 A. Marinucci , S. Bianchi , V. Braito , B. De Marco , G. Matt , R. Middei , E. Nardini , J. N. Reeves

We present the X-ray spectral results from the longest X-ray multi-mirror mission-Newton observation, 133 ks, of the low luminosity active galactic nucleus NGC 7213. The hardness ratio analysis of the X-ray light curves discloses a rather…

High Energy Astrophysical Phenomena · Physics 2015-06-12 D. Emmanoulopoulos , I. E. Papadakis , F. Nicastro , I. M. McHardy

MCG-6-30-15, at a distance of 37 Mpc (z=0.008), is the archetypical Seyfert 1 galaxy showing very broad Fe K$\alpha$ emission. We present results from a joint NuSTAR and XMM-Newton observational campaign that, for the first time, allows a…

The narrow-line quasar PHL 1092 was observed by XMM-Newton at two epochs separated by nearly thirty months. Timing analyses confirm the extreme variability observed during previous X-ray missions. A measurement of the radiative efficiency…

Astrophysics · Physics 2009-09-17 L. C. Gallo , Th. Boller , W. N. Brandt , A. C. Fabian , D. Grupe

Variations in the X-ray emission from the narrow line Seyfert 1 galaxy, Markarian 335 (Mrk 335), are studied on both long and short timescales through observations made between 2006 and 2013 with XMM-Newton, Suzaku and NuSTAR. Changes in…

High Energy Astrophysical Phenomena · Physics 2015-06-23 D. R. Wilkins , L. C. Gallo