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Related papers: NGC454: unveiling a new "changing look" AGN

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We have conducted an extensive X-ray spectral variability study of a sample of 20 Compton-thin type II galaxies using broad band spectra from XMM-Newton, Chandra, and Suzaku. The aim is to study the variability of the neutral intrinsic…

Astrophysics of Galaxies · Physics 2020-07-15 Sibasish Laha , Alex G. Markowitz , Mirko Krumpe , Robert Nikutta , Richard Rothschild , Tathagata Saha

We report on a 100 ks Suzaku observation of the bright, nearby (z=0.008486) Seyfert 1.9 galaxy MCG -5-23-16. The broad-band (0.4-100 keV) X-ray spectrum allows us to determine the nature of the high energy emission with little ambiguity.…

In this paper we report the results of an X-ray monitoring campaign on the heavily obscured Seyfert galaxy Markarian 3 carried out between the fall of 2014 and the spring of 2015 with NuSTAR, Suzaku and XMM-Newton. The hard X-ray spectrum…

We present a systematic investigation of extremely X-ray variable active galactic nuclei (AGNs) in the $\approx 5.3~{\rm deg}^2$ XMM-SERVS XMM-LSS region. Eight variable AGNs are identified with rest-frame 2 keV flux density variability…

Astrophysics of Galaxies · Physics 2025-03-03 Zijian Zhang , Bin Luo , Linhua Jiang , W. N. Brandt , Jian Huang , Qingling Ni

We have analyzed the two longest (elapsed time > 3 days) BeppoSAX observations of the X-ray brightest Seyfert galaxy, NGC 4151, to search for spectral variability on time-scales from a few tens of ksec to years. We found in both cases…

Astrophysics · Physics 2008-11-26 S. Puccetti , F. Fiore , G. Risaliti , M. Capalbi , M. Elvis , F. Nicastro , .

We present a new X-ray analysis of the dwarf Seyfert galaxy NGC 4395, based on two archival XMM-Newton and Suzaku observations. This source is well known for a series of remarkable properties: one of the smallest estimated black hole masses…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Emanuele Nardini , Guido Risaliti

We present a spectral analysis of four coordinated NuSTAR+XMM-Newton observations of the Seyfert galaxy NGC 1365. These exhibit an extreme level of spectral variability, which is primarily due to variable line-of-sight absorption, revealing…

We analyze recent simultaneous Chandra/RXTE observations of the Seyfert 2 galaxy NGC 4945. The unprecedented spatial resolution of Chandra means we are able to separate the spectra of the nucleus, starburst and superwind regions, while the…

Astrophysics · Physics 2009-11-07 Chris Done , Greg M. Madejski , Piotr T. Zycki , Lincoln J. Greenhill

We present the analysis of Chandra and NuSTAR spectra of NGC 4968, a local (D$\sim$44 Mpc) 12$\mu$m-selected Seyfert 2 galaxy, enshrouded within Compton-thick layers of obscuring gas. We find no evidence of variability between the Chandra…

We present analysis of the long-term X-ray spectral variability of Seyfert galaxies as observed by Swift, which provides well-sampled observations over a much larger flux range and a much longer timescale than any other X-ray observatory.…

High Energy Astrophysical Phenomena · Physics 2015-02-27 S. D. Connolly , I. M. McHardy , T. Dwelly

NGC 3147 is so far the most convincing case of a "true" Seyfert 2 galaxy, i.e. a source genuinely lacking the Broad Line Regions. We obtained a Suzaku observation with the double aim to study in more detail the iron line complex, and to…

High Energy Astrophysical Phenomena · Physics 2015-06-04 G. Matt , S. Bianchi , M. Guainazzi , X. Barcons , F. Panessa

We present results of a long-term optical, UV and X-ray study of variability of the nearby changing-look (CL) Seyfert NGC 1566 which was observed with the Swift Observatory from 2007 to 2020. We summarize our previously published…

High Energy Astrophysical Phenomena · Physics 2022-02-15 Victor L. Oknyansky

The aim of this paper is to study the variability of the warm absorber "clouds of ionised gas within AGN", for the Seyfert 1 galaxies Arakelian 564. The X-ray spectra for four XMM-Newton observations of this object are analysed in EPIC and…

High Energy Astrophysical Phenomena · Physics 2019-09-04 B. Korany , M. I. Nouh

We present results on the Seyfert 2 galaxy NGC4388 in the Virgo cluster observed with ASCA during its PV phase. The 0.5-10 keV X-ray spectrum consists of multiple components; (1) a continuum component heavily absorbed by a column density NH…

Astrophysics · Physics 2015-06-24 K. Iwasawa , A. C. Fabian , S. Ueno , H. Awaki , Y. Fukazawa , K. Matsushita , K. Makishima

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 the results of a BeppoSAX observation of the nearby spiral galaxy NGC4945 in the 0.1-200 keV energy band. The nuclear X-ray emission emerges above ~7 keV, through an absorber with column density N_H ~ a few 10^24/cm/cm. Its…

Astrophysics · Physics 2009-09-25 M. Guainazzi , G. Matt , W. N. Brandt , L. A. Antonelli , P. Barr , L. Bassani

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 joint Chandra, XMM-Newton and NuSTAR analysis of two nearby Seyfert galaxies, NGC 3081 and ESO 565-G019. These are the only two having Chandra data in a larger sample of ten low redshift ($z \le 0.05$), candidates…

We present results from a 150 ksec Suzaku observation of the Seyfert 1.5 NGC 3516 in October 2005. The source was in a relatively highly absorbed state. Our best-fit model is consistent with the presence of a low-ionization absorber which…