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We present a detailed analysis of the intrinsic X-ray absorption in the Seyfert 1 galaxy NGC 4151 using Chandra/HETGS data obtained 2002 May, as part of a program which included simultaneous UV spectra using HST/STIS and FUSE. NGC 4151 was…

We present an investigation of the ultraviolet and X-ray spectra of the Seyfert 1.5 galaxy Markarian 817. The ultraviolet analysis includes two recent observations taken with the Cosmic Origins Spectrograph in August and December 2009, as…

We have obtained a far-ultraviolet spectrum (1150 - 1600 Ang.) of a hot subdwarf star behind the remnant of SN 1006 with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope. The high-quality spectrum is used to test previous…

We report the detection of ionized absorption in the ASCA spectrum of the narrow-line Seyfert 1 galaxy IRAS 17020+4544. Subsequent optical spectropolarimetry revealed high polarization increasing from 3% in the red to 5% in the blue,…

Astrophysics · Physics 2009-10-30 Karen M. Leighly , Laura E. Kay , Beverley J. Wills , D. Wills , Dirk Grupe

The Seyfert Galaxy Mrk 335 is known for its frequent changes of flux and spectral shape in the X-ray band occurred during recent years. These variations may be explained by the onset of a wind that previous, non-contemporaneous…

Most Ultraluminous X-ray sources (ULXs) are thought to be powered by super-Eddington accretion onto stellar-mass compact objects. Accretors in this extreme regime are naturally expected to ionise copious amounts of plasma in their vicinity…

High Energy Astrophysical Phenomena · Physics 2021-10-13 P. Kosec , C. Pinto , C. S. Reynolds , M. Guainazzi , E. Kara , D. J. Walton , A. C. Fabian , M. L. Parker , I. Valtchanov

The neutral intergalactic medium above redshift 6 is opaque to ionizing radiation, therefore one needs indirect measurements of the escape fraction of ionizing photons from galaxies of this epoch. Low-ionization state absorption lines are a…

Astrophysics of Galaxies · Physics 2021-02-10 V. Mauerhofer , A. Verhamme , J. Blaizot , T. Garel , T. Kimm , L. Michel-Dansac , J. Rosdahl

Blueshifted absorption lines in the X-ray spectra of AGN show that ultra-fast outflows with typical velocities $v \sim 0.1c$ are a common feature of these luminous objects. Such powerful AGN winds offer an explanation of the observed…

High Energy Astrophysical Phenomena · Physics 2018-09-12 Ken Pounds , Chris Nixon , Andrew Lobban , Andrew King

We present optical spectra and emission-line ratios of 12 Narrow-Line Seyfert 1 (NLS1) galaxies that we observed to study the ionizing EUV continuum. A common feature in the EUV continuum of active galactic nuclei is the big blue bump…

Astrophysics · Physics 2009-11-10 M. Dietrich , D. M. Crenshaw , S. B. Kraemer

We present the analysis of grating spectra of the Narrow Line Seyfert 1 Galaxy IRAS 17020+4544 observed by XMM-Newton in 2004 and 2014. In a previous work on these data, we reported the discovery of a multi-component ultra-fast outflow that…

Astrophysics of Galaxies · Physics 2018-12-05 Mario Sanfrutos , Anna Lia Longinotti , Yair Krongold , Matteo Guainazzi , Francesca Panessa

We report the serendipitous discovery of an absorption feature at 4.8 keV in the NuSTAR spectra of ESP 39607, a Seyfert 2 galaxy at $z = 0.201$, observed in May 2023 and August 2024. The feature is detected in both observations with…

High Energy Astrophysical Phenomena · Physics 2025-07-01 Alessandro Peca , Michael J. Koss , Roberto Serafinelli , Claudio Ricci , C. Megan Urry , Giulia Cerini , Peter G. Boorman

We present results from spectral analysis of ASCA data on the NLS1 Mrk 507. This galaxy was found to have an exceptionally flat ROSAT spectrum among the NLS1s. The ASCA spectrum however shows a clear absorption feature in the energy band…

Astrophysics · Physics 2009-10-30 K. Iwasawa , W. N. Brandt , A. C. Fabian

Transient X-ray obscuration in Seyfert 1 galaxies is thought to arise from clumpy accretion-disk winds near the broad-line region (BLR), but the wind structure and its short-timescale variability are difficult to measure because…

We present a detailed analysis of the intrinsic absorption in the Seyfert 1 galaxy NGC 4151 using UV spectra from the HST/STIS and FUSE, obtained 2002 May as part of a set of contemporaneous observations that included Chandra/HETGS spectra.…

We examine a 200 ks XMM-Newton observation of the narrow-line Seyfert 1 galaxy Mrk 493. The active galaxy was half as bright as in a previous 2003 snapshot observation and the current lower flux enables a study of the putative reflection…

High Energy Astrophysical Phenomena · Physics 2018-04-18 K. Bonson , L. C. Gallo , D. R. Wilkins , A. C. Fabian

X-ray observations of unabsorbed active galactic nuclei provide an opportunity to explore the innermost regions of supermassive black hole accretion discs. Our goal in this paper is to investigate the central environment of a Seyfert 1.5…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Jiri Svoboda , Matteo Guainazzi , Vladimir Karas

We present the spectral analysis of three Suzaku XIS observations of 3C 111 requested to monitor the predicted variability of its ultra-fast outflow on ~7 days time-scales. We detect an ionized iron emission line in the first observation…

High Energy Astrophysical Phenomena · Physics 2015-05-30 F. Tombesi , R. M. Sambruna , J. N. Reeves , C. S. Reynolds , V. Braito

We study the absorption and emission properties of the photoionised gas near one of the brightest and most variable AGN, the Seyfert galaxy NGC 4051, in order to constrain the geometry, dynamics and ionisation structure of the outflow. We…

Astrophysics · Physics 2007-05-23 M. Fenovcik , J. S. Kaastra , E. Costantini , K. C. Steenbrugge , F. Verbunt

PG 1448+273 is a luminous, nearby ($z=0.0645$), narrow line Seyfert 1 galaxy, which likely accretes close to the Eddington limit. Previous X-ray observations of PG 1448 with XMM-Newton in 2017 and NuSTAR in 2022 revealed the presence of an…

High Energy Astrophysical Phenomena · Physics 2024-08-28 J. N. Reeves , V. Braito , A. Luminari , D. Porquet , M. Laurenti , G. Matzeu , A. Lobban , S. Hagen

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
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