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相关论文: Detection of Hard X-Rays from the Compton-Thick Se…

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We obtained a wide-band spectrum of the Compton-thick Seyfert 2 galaxy Mrk 3 with Suzaku. The observed spectrum was clearly resolved into weak, soft power-law emission, a heavily absorbed power-law component, cold reflection, and many…

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.…

We report on the first detection above ~10 keV of the archetypal Compton-thick Seyfert 2 galaxy NGC 1068. This detection, obtained with the PDS instrument onboard BeppoSAX in the 20-100 keV range, confirms the hardness of the X--ray…

The Seyfert 2 galaxy NGC 7674 has been observed within the BeppoSAX Core Programme with the onboard narrow field instruments between 0.1 and 100 keV. The broad-band spectrum shows four most relevant spectral components: a) a soft excess…

天体物理学 · 物理学 2007-05-23 G. Malaguti , G. G. C. Palumbo , M. Cappi , A. Comastri , C. Otani , M. Matsuoka , M. Guainazzi , L. Bassani , F. Frontera

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…

高能天体物理现象 · 物理学 2015-05-19 A. Comastri , K. Iwasawa , R. Gilli , C. Vignali , P. Ranalli , G. Matt , F. Fiore

We present the 0.5 - 50 keV Suzaku broad-band X-ray spectral study of the Compton-thick AGN in NGC 5135. The Suzaku observation provides the first detection of NGC 5135 above 10 keV that allowed us, for the first time, to estimate the…

高能天体物理现象 · 物理学 2011-11-02 Veeresh Singh , Guido Risaliti , Valentina Braito , Prajval Shastri

We present results from a half-day observation by XMM-Newton of the nucleus of the nearby Seyfert 2 galaxy NGC 6300. The X-ray spectrum of the nucleus consists of a heavily absorbed hard component dominating the 3--10 keV band and a soft…

天体物理学 · 物理学 2009-11-10 Chiho Matsumoto , Aida Nava , Larry A. Maddox , Karen M. Leighly , Dirk Grupe , Hisamitsu Awaki , Shiro Ueno

In 2006 June, the obscured low luminosity active galactic nucleus in the nearby Seyfert 1.9 galaxy NGC 4258 was observed with Suzaku for ~ 100 ks. Utilizing the XIS and the HXD, the nucleus emission was detected over 2 to 40 keV range, with…

天体物理学 · 物理学 2015-05-13 Shin'ya Yamada , Takeshi Itoh , Kazuo Makishima , Kazuhiro Nakazawa

We present a Suzaku observation of the dwarf Seyfert galaxy NGC4395 with an estimated black hole mass of ~10^5 Msun. Rapid and strong X-ray variability with an rms amplitude of ~60 per cent is observed in the 0.4-10 keV band with the XIS…

宇宙学与河外天体物理 · 物理学 2016-03-02 K. Iwasawa , Y. Tanaka , L. C. Gallo

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…

天体物理学 · 物理学 2016-08-30 G. Matt , A. C. Fabian , M. Guainazzi , K. Iwasawa , L. Bassani , G. Malaguti

We present spectral analysis of two Suzaku observations of the Seyfert 2 galaxy, NGC 2110. This source has been known to show complex, variable absorption which we study in depth by analyzing these two observations set seven years apart and…

We present results of the ASCA observation of the Seyfert 2 galaxy NGC 4507. The 0.5-10 keV spectrum is rather complex and consists of several components: (1) a hard X-ray power law heavily absorbed by a column density of about 3 10^23…

天体物理学 · 物理学 2009-10-30 A. Comastri , C. Vignali , M. Cappi , G. Matt , R. Audano , H. Awaki , S. Ueno

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…

天体物理学 · 物理学 2009-11-07 C. Vignali , A. Comastri

The Seyfert 2 galaxy Mrk 1210 was found to exhibit a flat hard X-ray component by ASCA, although ASCA could not distinguish whether it is an absorbed direct component or a reflected one. We then observed Mrk 1210 with BeppoSAX, and found…

天体物理学 · 物理学 2015-06-24 Masanori Ohno , Yasushi Fukazawa , Naoko Iyomoto

We have analyzed a Suzaku long-look of the active galactic nucleus MCG-2-58-22, a type 1.5 Seyfert with very little X-ray absorption in the line of sight and prominent features arising from reflection off circumnuclear material: the Fe line…

宇宙学与河外天体物理 · 物理学 2015-05-28 Elizabeth Rivers , Alex Markowitz , Richard Rothschild

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…

We present the broad-band 0.6-150 keV Suzaku and Swift BAT spectra of the low luminosity Seyfert galaxy, NGC 7213. The time-averaged continuum emission is well fitted by a single powerlaw of photon index Gamma = 1.75 and from consideration…

高能天体物理现象 · 物理学 2015-05-19 A. P. Lobban , J. N. Reeves , D. Porquet , V. Braito , A. Markowitz , L. Miller , T. J. Turner

We report on the first observation of the Seyfert 1 galaxy NGC4593 in the 0.1-200 keV band, performed with the BeppoSAX observatory. Its spectral components are for the first time simultaneously measured: a power-law with photon spectral…

天体物理学 · 物理学 2007-05-23 M. Guainazzi , G. C. Perola , G. Matt , F. Nicastro , L. Bassani , F. Fiore , ; D. Dal Fiume , L. Piro

We report on our analysis of XMM-Newton observations of the Seyfert 2 galaxy ESO 138-G1 (z = 0.0091). These data reveal a complex spectrum in both its soft and hard portions. The 0.5-2 keV band is characterized by a strong 'soft-excess'…

宇宙学与河外天体物理 · 物理学 2015-05-30 E. Piconcelli , S. Bianchi , C. Vignali , E. Jimenez-Bailon , F. Fiore

We present analysis of NuSTAR X-ray observations in the 3-79 keV energy band of the Seyfert 2 galaxy NGC 4388, taken in 2013. The broadband sensitivity of NuSTAR, covering the Fe K$\alpha$ line and Compton reflection hump, enables tight…

高能天体物理现象 · 物理学 2017-07-19 N. Kamraj , E. Rivers , F. A. Harrison , M. Brightman , M. Balokovic
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