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相关论文: Compton reflection and iron fluorescence in BeppoS…

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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…

天体物理学 · 物理学 2009-11-07 G. Risaliti

We have studied the average 3-200 keV spectra of Seyfert galaxies of type 1 and 2, using data obtained with BeppoSAX. The average Seyfert 1 spectrum is well-fitted by a power law continuum with photon spectral index Gamma~1.9, a Compton…

天体物理学 · 物理学 2009-11-07 A. Malizia , L. Bassani , J. B. Stephen , G. Di Cocco , F. Fiore , A. J. Dean

We report on a joint ASCA and RXTE observation spanning an $\sim$ 400~ks time interval of the bright Seyfert~1 galaxy MCG--6-30-15. The data clearly confirm the presence of a broad skewed iron line ($W_{K\alpha} \sim$ 266 eV) and Compton…

天体物理学 · 物理学 2009-09-17 J. C. Lee , A. C. Fabian , W. N. Brandt , C. S. Reynolds , K. Iwasawa

The 0.5-150 keV broad-band spectra of a sample of nine bright type 1 Seyfert galaxies are analyzed here. These sources have been discovered/detected by INTEGRAL and subsequently observed with XMM--Newton for the first time with high…

天体物理学 · 物理学 2009-11-13 F. Panessa , L. Bassani , A. De Rosa , A. J. Bird , A. J. Dean , M. Fiocchi , A. Malizia , M. Molina , P. Ubertini , R. Walter

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…

天体物理学 · 物理学 2011-07-19 K. A. Pounds , J. N. Reeves , K. L. Page , R. Edelson , G. Matt , G. C. Perola

From the spectral analysis of a broadband (0.1-200 keV) BeppoSAX observation of the Seyfert 1 galaxy IC 4329A, the main results obtained are: a) the amount of reflection, together with the intensity of the iron K line, indicate a geometry…

天体物理学 · 物理学 2007-05-23 G. C. Perola

We study a broad-band X-ray observation by BeppoSAX of the broad-line radio galaxy 3C 120. The primary X-ray continuum is well described by a power law with the photon index of Gamma=1.85+-0.05 and a high-energy break or a cutoff. The…

天体物理学 · 物理学 2009-10-31 A. A. Zdziarski , P. Grandi

We report the first simultaneous measure of the X-ray broadband (0.1--200 keV) continuum and of the iron K-alpha fluorescent line profile in the Seyfert 1 galaxy MCG-6-30-15. Our data confirms the ASCA detection of a skewed and redshifted…

天体物理学 · 物理学 2007-05-23 M. Guainazzi , G. Matt , S. Molendi , A. Orr , F. Fiore , P. Grandi , A. Matteuzzi , T. Mineo , G. C. Perola , A. N. Parmar , L. Piro

IC 4329A is the brightest known Seyfert galaxy in hard (~2-30 keV) X-rays and is likely to be representative of Seyfert 1 galaxies as a class. A recent 100 ks BeppoSAX observation (Perola et al. 1999) clearly confirmed the presence of a…

天体物理学 · 物理学 2009-10-31 M. Cappi , G. Di Cocco , M. Dadina , G. Malaguti , M. Matsuoka , G. Matt , G. C. Perola , L. Piro

We report on the first spectrum up to 10 keV of the bright narrow-line Seyfert 1 galaxy Ton S 180, obtained with the imaging instruments onboard BeppoSAX. This is the first observed source in a sample of a dozen narrow-line Seyfert 1…

In this letter we present analysis of BeppoSAX data from a long look at the Seyfert 1 galaxy NGC 7469. The presence of a soft excess below 0.8 keV is confirmed by our analysis and no warm absorber component is required to fit the spectrum.…

天体物理学 · 物理学 2009-11-07 A. De Rosa , A. C. Fabian , L. Piro

The lack of variability of the broad iron line seen in the Seyfert 1 galaxy MCG-6-30-15 is studied using the EPIC pn data obtained from a 2001 observation of 325 ks, during which the count rate from the source varied by a factor of 5. The…

天体物理学 · 物理学 2009-11-07 A. C. Fabian , S. Vaughan

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

NuSTAR observed the bright Compton-thin, narrow line Seyfert 1 galaxy, NGC 5506, for about 56 ks. In agreement with past observations, the spectrum is well fit by a power law with Gamma~1.9, a distant reflection component and narrow ionized…

We present the broad band analysis of two BeppoSAX observations of the Sy 1 Mkn509. In 2000 the source was in a typical flux state, F{2-10keV}=2.7x10^{-11}erg cm^{-2} s^{-1}, while in 1998 it was found in a high flux state,…

天体物理学 · 物理学 2009-11-10 A. De Rosa , L. Piro , G. Matt , G. C. Perola

We report on a puzzling event occurred during a long BeppoSAX observation of the slow-rotating binary pulsar GX 1+4. During this event, lasting about 1 day, the source X-ray flux was over a factor 10 lower than normal. The low-energy…

The $BeppoSAX$ archive is currently the largest reservoir of high sensitivity simultaneous soft and hard-X ray data of Seyfert galaxies. From this database all the Seyfert galaxies (105 objects of which 43 are type I and 62 are type II)…

天体物理学 · 物理学 2009-11-13 Mauro Dadina

We selected a sample of eight bright unobscured (at least at the iron line energy) Seyfert Galaxies observed simultaneously by XMM-Newton and BeppoSAX, taking advantage of the complementary characteristics of the two missions. The main…

天体物理学 · 物理学 2009-11-10 S. Bianchi , G. Matt , I. Balestra , M. Guainazzi , G. C. Perola

We report on a 50 ks observation of the bright Seyfert 1 galaxy MCG--6-30-15 with the Rossi X-ray Timing Explorer. The data clearly show the broad fluorescent iron line (equivalent width ~ 250 eV), and the Compton reflection continuum at…

天体物理学 · 物理学 2009-10-30 J. C. Lee , A. C. Fabian , C. S. Reynolds , K. Iwasawa , W. N. Brandt

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
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