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Related papers: Ubiquitous column density variability in Seyfert 2…

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A sample of 102 local (0.02 < z < 0.1) Seyfert galaxies with black hole masses MBH > 10^7 M_sun was selected from the Sloan Digital Sky Survey (SDSS) and observed using the Keck 10-m telescope to study the scaling relations between MBH and…

In a continuing survey of active galactic nuclei observed by the Far Ultraviolet Spectroscopic Explorer, we provide a deeper analysis of intrinsic absorption features found in 35 objects. Our survey is for low-redshift and…

Astrophysics · Physics 2009-11-13 Jay P. Dunn , D. Michael Crenshaw , S. B. Kraemer , M. L. Trippe

A sample of X-ray and optically selected narrow emission-line galaxies (769 sources) from the 3XMM catalogue cross-correlated with SDSS (DR9) catalogue has been studied. Narrow-emission line active galactic nuclei (AGN; type-2) have been…

High Energy Astrophysical Phenomena · Physics 2016-10-19 Estelle Pons , Mike G. Watson

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 report on two Chandra observations, and a simultaneous Hubble Space Telescope ultraviolet observation, of the dwarf Seyfert 1 galaxy NGC 4395. Each Chandra observation had a duration of ~30 ks, with a separation of ~50 ks. The spectrum…

NGC 7582 is a well-studied X-ray bright Seyfert 2 with moderately heavy ($N_{\text{H}}\sim10^{23}-10^{24}$~cm$^{-2}$), highly variable absorption and strong reflection spectral features. The spectral shape changed around the year 2000,…

We present the second XMM-Newton observation (85 ks) of the narrow-line Seyfert 1 galaxy (NLS1) I Zw 1 and describe its mean spectral and timing characteristics. On average, I Zw 1 is ~35 per cent dimmer in 2005 than in the shorter (20 ks)…

Astrophysics · Physics 2008-11-26 L. C. Gallo , W. N. Brandt , E. Costantini , A. C. Fabian , K. Iwasawa , I. E. Papadakis

We present a composite 1-10 keV Seyfert 2 X-ray spectrum, derived from ASCA observations of a distance-limited sample of nearby galaxies. All 29 observed objects were detected. Above ~3 keV, the composite spectrum is inverted, confirming…

Astrophysics · Physics 2009-11-06 Edward C. Moran , Laura E. Kay , Marc Davis , Alexei V. Filippenko , Aaron J. Barth

We present a catalogue of ROSAT detected sources in the sample of spectroscopically selected Seyfert 1 and Seyfert 2 galaxies of Rafanelli et al. (1995). The catalogue contains 102 Seyfert 1 and 36 Seyfert 2 galaxies. The identification is…

Astrophysics · Physics 2009-11-06 F. Pfefferkorn , Th. Boller , P. Rafanelli

The Absorption Measure Distribution (AMD) in the X-ray outflows of Seyfert active galactic nuclei (AGN) describes the distribution of absorbing column density as a function of ionization parameter. Up to now, AMD has been measured only for…

Astrophysics of Galaxies · Physics 2019-08-21 T. P. Adhikari , A. Różańska , K. Hryniewicz , B. Czerny , E. Behar

X-ray reverberation, where light-travel time delays map out the compact geometry around the inner accretion flow in supermassive black holes, has been discovered in several of the brightest, most variable and well-known Seyfert galaxies. In…

High Energy Astrophysical Phenomena · Physics 2016-10-12 E. Kara , W. N. Alston , A. C. Fabian , E. M. Cackett , P. Uttley , C. S. Reynolds , A. Zoghbi

The optical classification of a Seyfert galaxy and whether it is considered X-ray absorbed are often used interchangeably. But there are many borderline cases and also numerous examples where the optical and X-ray classifications appear to…

We present long-term (months-years) X-ray spectral variability of the Seyfert 1.8 galaxy NGC 1365 as observed by Swift, which provides well sampled observations over a much longer timescale (6 years) and a much larger flux range than is…

High Energy Astrophysical Phenomena · Physics 2014-04-21 S. D. Connolly , I. M. McHardy , T. Dwelly

We present an X-ray spectral analysis of a sample of 8 bona-fide Seyfert 2 galaxies, selected on the basis of their high $[OIII]\lambda5007$ flux, from the Ho et al. (1997) spectroscopic sample of nearby galaxies. We find that, in general,…

Astrophysics · Physics 2008-11-26 A. Pappa , I. Georgantopoulos , G. C. Stewart , A. L. Zezas

The new $XMM-Newton$ data of seven Seyfert 2 galaxies with optical spectropolarimetric observations are presented. The analysis of 0.5 -- 10 keV spectra shows that all four Seyfert 2 galaxies with polarized broad lines (PBLs) are absorbed…

Astrophysics · Physics 2009-11-13 X. W. Shu , J. X. Wang , P. Jiang

We investigate the dependence of gas kinematics and column densities in the MgII-absorbing circumgalactic medium on galaxy color, azimuthal angle, and inclination to trace baryon cycle processes. Our sample of 30 foreground isolated…

Astrophysics of Galaxies · Physics 2015-10-14 Nikole M. Nielsen , Christopher W. Churchill , Glenn G. Kacprzak , Michael T. Murphy , Jessica L. Evans

We describe a complete volume limited sample of nearby active galaxies selected by their 14-195keV luminosity, and outline its rationale for studying the mechanisms regulating gas inflow and outflow. We describe also a complementary sample…

We compare X-ray and UV spectroscopic observations of NGC 5548. Both data sets show O VI absorption troughs associated with the AGN outflow from this galaxy. We find that the robust lower limit on the column density of the O VI X-ray trough…

We report evidence for persistent giant and rapid X-ray variability in the radio-quiet, ultrasoft, strong Fe II, narrow-line Seyfert 1 galaxy IRAS 13224-3809. Within a 30 day ROSAT High Resolution Imager (HRI) monitoring observation at…

Astrophysics · Physics 2015-06-24 Th. Boller , W. N. Brandt , A. C. Fabian , H. H. Fink

We present evidence of flux variability, on both short (hours) and long (months) time scales of the Seyfert 2 galaxy NGC 7172. These results are based on the ASCA observation of NGC 7172 performed on May 1996. The source was detected at a…

Astrophysics · Physics 2009-10-30 M. Guainazzi , G. Matt , L. A. Antonelli , F. Fiore , L. Piro , S. Ueno