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We present and discuss the high energy (E>4 keV) XMM-Newton spectrum of the Seyfert 2 galaxy, NGC 1068. Possible evidence for flux variability in both the neutral and ionized reflectors with respect to a BeppoSAX observation taken 3.5 years…

Astrophysics · Physics 2009-11-10 Giorgio Matt , Stefano Bianchi , Matteo Guainazzi , Silvano Molendi

We present an analysis of five Suzaku observations of the bright Seyfert1 galaxy IC 4329A. The broad energy band and high signal-to-noise ratio of the data give new constraints on the iron K alpha line profile and its relationship with the…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Giulia Mantovani , Kirpal Nandra , Gabriele Ponti

There is growing evidence for the presence of blueshifted Fe K absorption lines in a number of radio-quiet AGNs and QSOs. These may be fundamental to probe flow dynamics near supermassive black holes. Here we aim at verifying and better…

High Energy Astrophysical Phenomena · Physics 2015-05-13 M. Cappi , F. Tombesi , S. Bianchi , M. Dadina , M. Giustini , G. Malaguti , L. Maraschi , G. G. C. Palumbo , P. O. Petrucci , G. Ponti , C. Vignali , T. Yaqoob

We conduct X-ray reverberation mapping and spectral analysis of the radio galaxy Centaurus A to uncover its central structure. We compare the light curve of the hard X-ray continuum from Swift Burst Alert Telescope observations with that of…

High Energy Astrophysical Phenomena · Physics 2025-02-12 Toshiya Iwata , Atsushi Tanimoto , Hirokazu Odaka , Aya Bamba , Yoshiyuki Inoue , Kouichi Hagino

We present a broadband (~0.5-79 keV) spectral and temporal analysis of multiple NuSTAR observations combined with archival Suzaku and Chandra data of NGC4945, the brightest extragalactic source at 100 keV. We observe hard X-ray (> 10 keV)…

We report the spectral analysis of a long XMM-Newton observation of the well-studied, moderate luminosity Broad Line Seyfert 1 galaxy NGC 5548. The source was at an historically average brightness and we find the hard (3-10 keV) spectrum…

Astrophysics · Physics 2011-07-19 K. A. Pounds , J. N. Reeves , K. L. Page , R. Edelson , G. Matt , G. C. Perola

We present the analysis of 31 observations of 20 bright Compton thin Seyfert 2s, in the 0.1-200 keV band, performed with the BeppoSAX satellite. The sample consists of all Seyfert 2s in the BeppoSAX public archive, with a 2-10 keV flux…

Astrophysics · Physics 2009-11-07 G. Risaliti

A 2012 Suzaku observation of the Seyfert 1.5 galaxy Markarian 530 was analysed and found to exhibit two distinct modes of variability, which were found to be independent from one another. Firstly, the spectrum undergoes a smooth transition…

High Energy Astrophysical Phenomena · Physics 2018-06-06 H. J. S. Ehler , A. G. Gonzalez , L. C. Gallo

We present XMM-Newton observations of four low-redshift Seyfert galaxies selected to have low host luminosities (M_g>-20 mag) and small stellar velocity dispersions (sigma_star<45 km/s), which are among the smallest stellar velocity…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 C. E. Thornton , A. J. Barth , L. C. Ho , J. E. Greene

We report on four epochs of observations of the quasar PG 1211+143 using NuSTAR. The net exposure time is 300 ks. Prior work on this source found suggestive evidence of an 'ultra-fast outflow' (or, UFO) in the Fe K band, with a velocity of…

We report the results obtained by a broad-band (0.5-500 keV) data analysis of narrow-line Seyfert 1 galaxy NGC 4748 observed with an XMM-Newton/PN, INTEGRAL/ISGRI and SWIFT/BAT telescopes. This galaxy has a soft X-ray excess that is typical…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Anatoliy Vasylenko

We present the BeppoSAX broad-band X-ray spectrum of the Seyfert 2 galaxy NGC 3281. The source high-energy spectrum is characterized by the nuclear transmitted component, with an absorbing column density of about 2 10^24 cm^-2, while the…

Astrophysics · Physics 2009-11-07 C. Vignali , A. Comastri

We present a flux-resolved X-ray analysis of the dwarf Seyfert 1.8 galaxy NGC 4395, based on three archival $XMM-Newton$ and one archival $NuSTAR$ observations. The source is known to harbor a low mass black hole ($\sim 10^4- {\rm a~…

We present a long Suzaku observation of 3C 382. A Swift BAT spectrum from the 58-month survey is also analyzed, together with an archival XMM-Newton EPIC exposure. Our main result is the finding with Suzaku of a broad FeK line with a…

High Energy Astrophysical Phenomena · Physics 2015-05-27 R. M. Sambruna , F. Tombesi , J. N. Reeves , V. Braito , L. Ballo , M. Gliozzi , C. S. Reynolds

We present here the results of our analysis of X-ray properties of Seyfert 2 galaxy NGC 3281, based on the observational data obtained by XMM-Newton and INTEGRAL within the energy ranges 0.2-12 keV and 20-150 keV, respectively. The…

High Energy Astrophysical Phenomena · Physics 2014-01-20 A. A. Vasylenko , E. V. Fedorova , V. I. Zhdanov

We present a spectral analysis of NuSTAR and NICER observations of the luminous, persistently accreting neutron star (NS) low-mass X-ray binary Cygnus X-2. The data were divided into different branches that the source traces out on the…

High Energy Astrophysical Phenomena · Physics 2022-03-14 R. M. Ludlam , E. M. Cackett , J. A. García , J. M. Miller , A. L. Stevens , A. C. Fabian , J. Homan , M. NG , S. Guillot , D. J. K. Buisson , D. Chakrabarty

JHKL'M (1-5 micron) imaging of a sample of Seyfert (Sy) 2 galaxies is presented. We confirm that the 1-2.2 micron nuclear continuum of some Sy 2s is dominated by stellar emission, whereas the continuum emission at longer wavelengths (3-5…

Astrophysics · Physics 2009-10-31 A. Alonso-Herrero , A. C. Quillen , C. Simpson , A. Efstathiou , M. J. Ward

We analyzed the spectral shape of the Compton shoulder around the neutral Fe-K$_\alpha$ line of the Compton-thick type II Seyfert nucleus of the Circinus galaxy. The characteristics of this Compton shoulder with respect to the reflected…

High Energy Astrophysical Phenomena · Physics 2018-11-07 Masaya Hikitani , Masanori Ohno , Yasushi Fukazawa , Toshihiro Kawaguchi , Hirokazu Odaka

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…

The Seyfert 1 galaxy NGC4151 is characterized by complex X-ray absorption, well described by a dual absorber, composed of a uniform mildly ionized gas and a cold system that partially covers the central source. However, in one of the 5…

Astrophysics · Physics 2009-11-11 L. Piro , A. De Rosa , G. Matt , G. C. Perola
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