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Related papers: The Phoenix galaxy: UGC4203 re-birth from its ashe…

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We discuss the properties of a small sample of Seyfert 2 galaxies whose X-ray spectrum changed appearance on time scales of years, becoming reflection-dominated from Compton-thin, or viceversa. A reflection--dominated spectrum is usually…

Astrophysics · Physics 2009-11-07 G. Matt , M. Guainazzi , R. Maiolino

In recent years, several Seyfert 2 galaxies have been discovered that change state when observed in X-rays a few years apart, switching from Compton-thin to reflection-dominated or viceversa. We observed a member of this class of…

High Energy Astrophysical Phenomena · Physics 2009-11-13 G. Matt , S. Bianchi , H. Awaki , A. Comastri , M. Guainazzi , K. Iwasawa , E. Jimenez-Bailon , F. Nicastro

In this paper, a BeppoSAX observation of the bright Seyfert 2 galaxy NGC6300 is presented. The rapidly variable emission from the active nucleus is seen through a Compton-thin (NH ~ 3x10^23 atomoms/cm/cm) absorber. A Compton-reflection…

Astrophysics · Physics 2009-11-07 M. Guainazzi

Aims. We study the long-term variability of the well-known Seyfert 2 galaxy Mrk 1210 (a.k.a. UGC 4203, or the Phoenix galaxy). Methods. The source was observed by many X-ray facilities in the last 20 years. Here we present a NuSTAR…

We present a Chandra monitoring campaign of the highly variable Seyfert galaxy UGC 4203 (the "Phoenix Galaxy") which revealed variations in the X-ray absorbing column density on time scales of two weeks. This is the third, clear case, after…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 G. Risaliti , M. Elvis , S. Bianchi , G. Matt

Results from BeppoSAX observations of Compton--thick Seyfert 2 galaxies are summarized and reviewed, and their general properties derived and discussed. In five out of the seven observed sources, the nucleus is directly visible at high…

Astrophysics · Physics 2016-08-30 G. Matt , A. C. Fabian , M. Guainazzi , K. Iwasawa , L. Bassani , G. Malaguti

We present Chandra and XMM-Newton observations of a small sample (11 objects) of optically-selected Seyfert~2 galaxies, for which ASCA and BeppoSAX had suggested Compton-thick obscuration of the Active Nucleus (AGN). The main goal of this…

Astrophysics · Physics 2009-09-17 M. Guainazzi , A. C. Fabian , K. Iwasawa , G. Matt , F. Fiore

We present multiple Chandra and XMM-Newton observations of the type 1.8 Seyfert Galaxy NGC 1365, which shows the most dramatic X-ray spectral changes observed so far in an AGN: the source switched from reflection dominated to transmission…

Astrophysics · Physics 2017-10-18 G. Risaliti , M. Elvis , G. Fabbiano , A. Baldi , A. Zezas

We present the results of a Suzaku monitoring campaign of the Seyfert 2 galaxy, NGC7582. The source is characterized by very rapid (on timescales even lower than a day) changes of the column density of an inner absorber, together with the…

Astrophysics of Galaxies · Physics 2011-02-11 Stefano Bianchi , Enrico Piconcelli , Marco Chiaberge , Elena Jimenez Bailon , Giorgio Matt , Fabrizio Fiore

A modification of the popular unification model for Seyfert galaxies is proposed, which takes into account recent observational findings on the statistical properties of both type 1 and type 2 Seyferts. In the proposed scenario,…

Astrophysics · Physics 2007-05-23 Giorgio Matt

In this paper we present the current status of a XMM-Newton program to observe an optically-defined, complete and unbiased sample of Compton-thick Seyfert 2 galaxies. The main goal of this project is the measurement of the occurrence rate…

Astrophysics · Physics 2017-08-23 M. Guainazzi , P. Rodriguez-Pascual , A. C. Fabian , K. Iwasawa , G. Matt , F. Fiore

We present the multi-epoch monitoring with NuSTAR and XMM-Newton of NGC 1358, a nearby Seyfert 2 galaxy whose properties made it a promising candidate X-ray changing look AGN, i.e., a source whose column density could transition from its…

We present the results of the latest NuSTAR monitoring campaign of the Compton-thick Seyfert 2 galaxy NGC 1068, composed of four $\sim$50 ks observations performed between July 2017 and February 2018 to search for flux and spectral…

Astrophysics of Galaxies · Physics 2020-01-17 A. Zaino , S. Bianchi , A. Marinucci , G. Matt , F. E. Bauer , W. N. Brandt , P. Gandhi , M. Guainazzi , K. Iwasawa , S. Puccetti , C. Ricci , D. J. Walton

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 results from an XMM-Newton observation of the nearby Seyfert 2 galaxy NGC5643. The nucleus exhibits a very flat X-ray continuum above 2 keV, together with a prominent K-alpha fluorescent iron line. This indicates heavy…

Astrophysics · Physics 2009-11-10 M. Guainazzi , P. Rodriguez-Pascual , A. C. Fabian , K. Iwasawa , G. Matt

We present results from a ~55 ks long XMM-Newton observation of the obscured AGN, NGC 5643, performed in July 2009. A previous, shorter (about 10 ks) XMM-Newton observation in February 2003 had left two major issues open, the nature of the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 G. Matt , S. Bianchi , A. Marinucci , M. Guainazzi , K. Iwawasa , E. Jimenez Bailon

Scanning and pointed RXTE observations of the nearby Seyfert 2 galaxy NGC 6300 reveal that it is a source of hard X-ray continuum and large equivalent width Fe K$\alpha$ emission. These properties are characteristic of Compton-reflection…

Astrophysics · Physics 2009-10-31 K. M. Leighly , J. P. Halpern , H. Awaki , M. Cappi , S. Ueno , J. Siebert

We present a detailed analysis of the X-ray spectrum of the Seyfert 2 galaxy NGC454E, belonging to the interacting system NGC454. Observations performed with Suzaku, XMM-Newton and Swift allowed us to detect a dramatic change in the…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-26 Elena Marchese , Valentina Braito , Roberto Della Ceca , Alessandro Caccianiga , Paola Severgnini

We present X-ray spectral analyses for three Seyfert 2 active galactic nuclei, NGC 424, NGC 1320, and IC 2560, observed by NuSTAR in the 3-79 keV band. The high quality hard X-ray spectra allow detailed modeling of the Compton reflection…

We present Suzaku observations of five hard X-ray selected nearby Seyfert 2 galaxies. All the sources were clearly detected with the pin Hard X-ray Detector up to several tens of keV, allowing for a fairly good characterization of the…

High Energy Astrophysical Phenomena · Physics 2015-05-19 A. Comastri , K. Iwasawa , R. Gilli , C. Vignali , P. Ranalli , G. Matt , F. Fiore
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