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Related papers: Tracking the Complex Absorption in NGC 2110 with T…

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We present the results of the Suzaku observation of the Seyfert 2 galaxy NGC 4507. This source is one of the X-ray brightest Compton-thin Seyfert 2s and a candidate for a variable absorber. Suzaku caught NGC 4507 in a highly absorbed state…

High Energy Astrophysical Phenomena · Physics 2015-06-11 V. Braito , L. Ballo , J. N. Reeves , A. Ptak , G. Risaliti , T. J. Turner

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…

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 Chandra HETGS (250 ks over two epochs) and XMM-Newton EPIC and RGS (60 ks) observations of NGC 2110, which has been historically classified as a Narrow Emission Line Galaxy galaxy. Our results support the…

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

We have obtained a broad-band spectrum of the Compton-thick Seyfert 2 galaxy NGC 2273 with Suzaku. The spectrum reveals the first detection of hard X-rays above ~10 keV from NGC 2273. The broad-band spectrum is well represented by a…

Astrophysics · Physics 2008-10-28 H. Awaki , Y. Terashima , Y. Higaki , Y. Fukazawa

The Seyfert 2 galaxy NGC 2110 has been observed with BeppoSAX between 0.5 and 150 keV. The high energy instrument onboard, PDS, has succeeded in measuring for the first time the spectrum of this source in the 13-150 keV range. The PDS…

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

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

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

Here we present the results of a Suzaku observation of the Broad Line Radio Galaxy 3C 445. We confirm the results obtained with the previous X-ray observations which unveiled the presence of several soft X-ray emission lines and an overall…

High Energy Astrophysical Phenomena · Physics 2015-05-27 V. Braito , J. N. Reeves , R. M. Sambruna , J. Gofford

(Abridged) We present a two month Suzaku X-ray monitoring of the Seyfert 1 galaxy NGC 5548. The campaign consists of 7 observations. We analyze the response in the opacity of the gas that forms the ionized absorber to ionizing flux…

We disentangle X-ray disk reflection from complex line-of-sight absorption in the nearby Seyfert NGC 4151, using a suite of Suzaku, NuSTAR, and XMM-Newton observations. Extending upon earlier published work, we pursue a physically motivated…

High Energy Astrophysical Phenomena · Physics 2017-07-12 T. Beuchert , A. G. Markowitz , T. Dauser , J. A. García , M. L. Keck , J. Wilms , M. Kadler , L. W. Brenneman , A. A. Zdziarski

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

Between July 2012 and February 2013, NuSTAR and XMM-Newton performed four long-look joint obser- vations of the type 1.8 Seyfert, NGC 1365. We have analyzed the variable absorption seen in these observations in order to characterize the…

Suzaku observed a nearby Seyfert 2 galaxy NGC4945, which hosts one of the brightest active galactic nuclei above 20 keV. Combining data from the X-ray CCD camera (XIS) and the Hard X-ray Detector (HXD), the AGN intrinsic nuclear emission…

Low ionisation nuclear emission-line region (LINER) nuclei have been claimed to be different than other active galactic nuclei (AGN) due to the presence of complex absorbing structures along the line-of-sight and/or an inefficient mode of…

We report on the deepest X-ray observation of the narrow-line Seyfert 1 galaxy Mrk 335 in the low-flux state obtained with Suzaku. The data are compared to a 2006 high-flux Suzaku observation when the source was ~10-times brighter.…

High Energy Astrophysical Phenomena · Physics 2015-06-23 L. C. Gallo , D. R. Wilkins , K. Bonson , C-Y. Chiang , D. Grupe , M. L. Parker , A. Zoghbi , A. C. Fabian , S. Komossa , A. L. Longinotti

X-ray unabsorbed Seyfert 2 galaxies appear to have X-ray absorption column densities that are too low (NH < 10^22 cm-2) to explain the absence of broad emission lines in their optical spectra, challenging the standard AGN unification model.…

High Energy Astrophysical Phenomena · Physics 2011-05-25 Xing-Xing Huang , Jun-Xian Wang , Ying Tan , Huan Yang , Ya-Fang Huang

We present data from simultaneous Chandra, XMM-Newton and BeppoSAX observations of the Seyfert 1 galaxy NGC 3516, taken during 2001 April and Nov. We have investigated the nature of the very flat observed X-ray spectrum. Chandra grating…

Astrophysics · Physics 2014-10-13 T. J. Turner , S. B. Kraemer , I. M. George , J. N. Reeves , M. C. Bottorff
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