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Related papers: Rapid N_H changes in NGC 4151

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XMM-Newton observed the Seyfert 1.9 galaxy NGC 4258 in December 2000. At energies above 2 keV a hard nuclear point source is resolved that can be fitted by a highly absorbed power-law spectrum (NH = (8.0+-0.4)x10^22 cm^-2, photon index…

Astrophysics · Physics 2009-11-07 W. Pietsch , A. M. Read

BeppoSAX observed NGC4258 on December 1998, when its 2-10 keV luminosity was \~1E41 erg/s. 100% variability is observed in the 3-10 keV band on timescales of a half a day while 20% variability is observed on timescales of one hour. The…

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 spectroscopic analysis of XMM-Newton and NuSTAR observations of the 'complex' NLS1 PG 1535+547 at redshift $z=0.038$. These observations span three epochs: 2002 and 2006 with XMM-Newton alone, covering the $0.3-10$ keV energy…

We present XMM-Newton, NuSTAR, Swift and Hubble Space Telescope observations of the Narrow-line Seyfert 1 galaxy Mrk 335 in a protracted low state in 2018 and 2019. The X-ray flux is at the lowest level so far observed, and the extremely…

We present the results of a deep 300 ks Chandra HETG observation of the highly variable narrow-line Seyfert Type 1 galaxy NGC 4051. The HETG spectrum reveals 28 significant soft X-ray ionised lines in either emission or absorption;…

High Energy Astrophysical Phenomena · Physics 2015-05-27 A. P. Lobban , J. N. Reeves , L. Miller , T. J. Turner , V. Braito , S. B. Kraemer , D. M. Crenshaw

The Seyfert 2 Galaxy NGC 7172 was observed twice by BeppoSAX narrow field instruments approximately one year apart. As found in previous observations, the source is variable on short time scales (hours) by a factor of $\sim$30%, confirming…

We present NuSTAR observations of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever observed, and in 2013, when the source was at a more typical flux level. We include archival…

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 detailed broadband X-ray spectral variability of a Seyfert 1 galaxy 1H~0419--577 based on an archival \suzaku{} observation in July 2007, a new \suzaku{} observation performed in January 2010 and the two latest \xmm{}…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Main Pal , Gulab C. Dewangan

(Abridged) We present the results from {\it ASCA} observations of NGC 3227 along with those from a {\it ROSAT} observation. The 0.6--10 keV continuum is consistent with a powerlaw with $\Gamma \sim 1.6$, flatter than that typically observed…

Astrophysics · Physics 2016-08-30 I. M. George , R. F. Mushotzky , T. J. Turner , T. Yaqoob , A. Ptak , K. Nandra , H. Netzer

The bright type I Seyfert galaxy NGC 3516 was observed by {\it Suzaku} twice, in 2005 October 12--15 and 2009 October 28--November 2, for a gross time coverage of 242 and 544 ksec and a net exposure of 134 and 255 ksec, respectively. The…

High Energy Astrophysical Phenomena · Physics 2014-06-20 Hirofumi Noda , Kazuo Makishima , Kazuhiro Nakazawa , Shin'ya Yamada

A long ($>100,000$ seconds) observation of the bright BL Lac object PKS 2155-304 has been carried out with the Narrow Field Instruments of the BeppoSAX satellite as part of the Science Verification Phase. The source was detected between 0.1…

Astrophysics · Physics 2007-05-23 P. Giommi et al

We report on soft X-ray observations of the Seyfert 1 galaxy MCG-6-30-15 with the Low and Medium Energy Concentrator Spectrometers on board BeppoSAX. The time averaged 0.1-4 keV spectrum shows evidence for a complex warm absorber. K-edges…

Astrophysics · Physics 2008-02-03 Astrid Orr , S. Molendi , F. Fiore , P. Grandi , A. N. Parmar , Alan Owens

We present a detailed study of the X-ray and optical spectra of the luminous Seyfert galaxy Mrk 1393, which revealed variable partial obscuration of the active nucleus. The X-ray spectra obtained by XMM-Newton and Swift show moderate…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 T. G. Wang , H. Y. Zhou , D. Grupe , W. M. Yuan , X. B. Dong , H. L. Lu

We present the first X-ray monitoring observations of the X-ray bright FRI radio galaxy NGC6251 observed with RXTE for 1 year. The primary goal of this study is to shed light on the origin of the X-rays, by investigating the spectral…

Astrophysics · Physics 2009-11-13 M. Gliozzi , I. E. Papadakis , R. M. Sambruna

This paper presents the results of a dense and intensive X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051 carried out in 2000. Results of the optical analysis are consistent with previous measurements. The amplitude…

Astrophysics · Physics 2009-11-07 O. Shemmer , P. Uttley , H. Netzer , I. M. McHardy

Analysis of broad-band X/$\gamma$-ray spectra of NGC~4151 from contemporaneous observations by {\it GRO}/OSSE, {\it ROSAT}, {\it Ginga} and {\it ASCA}, shows that the data are well modelled with an intrinsic spectrum due to thermal…

Astrophysics · Physics 2007-05-23 P. Magdziarz , A. A. Zdziarski

We present and analyze a pointed ROSAT PSPC observation of the Seyfert galaxy NGC 4051. The X-ray spectrum consists of a powerlaw modified by absorption edges and an additional soft excess during the high-state in source flux. Modeling the…

Astrophysics · Physics 2007-05-23 Stefanie Komossa , Henner Fink

We present a detailed timing and spectral study of an extremely variable narrow-line Seyfert~1 galaxy NGC 4748 using observations in the year 2017 and 2014 performed with AstroSat and XMM-Newton, respectively. Both observations show…

High Energy Astrophysical Phenomena · Physics 2021-01-13 Main Pal , Neeraj Kumari , Pankaj Kushwaha , K. P. Singh , Alok C. Gupta , Sachindra Naik , G. C. Dewangan , P. Tripathi , Rathin Adhikari , O. Adegoke , H. Nandan
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