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相关论文: The hard X-ray continuum of Cen A observed with IN…

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The radio galaxy Cen A has been detected all the way up to the TeV energy range. This raises the question about the dominant emission mechanisms in the high-energy domain. Spectral analysis allows us to put constraints on the possible…

宇宙学与河外天体物理 · 物理学 2015-05-27 V. Beckmann , P. Jean , P. Lubinski , S. Soldi , R. Terrier

Aims. We present a 0.2--200 keV broad-band study of absorbed AGN observed with INTEGRAL, XMM-Newton, Chandra and ASCA to investigate the continuum shape and the absorbing/reflecting medium properties. Methods. The sources are selected in…

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

We observed a nearby radio galaxy, the Centaurus A (Cen A), three times with Suzaku in 2009, and measured the wide-band X-ray spectral variability more accurately than the previous measurements. The Cen A was in the active phase in 2009,…

高能天体物理现象 · 物理学 2015-05-30 Y. Fukazawa , K. Hiragi , S. Yamazaki , M. Mizuno , K. Hayashi , K. Hayashi , S. Nishino , H. Takahashi , M. Ohno

In this paper we discuss the broad-band X-ray characteristics of a complete sample of 36 type 1 AGN, detected by INTEGRAL in the 20-40 keV band above the 5.5sigma level. We present, for all the objects in the sample, the broad-band (1-110…

宇宙学与河外天体物理 · 物理学 2015-05-13 M. Molina , L. Bassani , A. Malizia , J. B. Stephen , A. J. Bird , A. J. Dean , F. Panessa , A. De Rosa , R. Landi

[Abridged]We report on the broadband X-ray properties of a complete sample of absorbed Seyfert galaxies hard X-ray selected with INTEGRAL. The sample is composed of 33 sources: 15 are newly discovered above 20 keV while 18 are already known…

宇宙学与河外天体物理 · 物理学 2015-06-03 A. De Rosa , F. Panessa , L. Bassani , A. Bazzano , A. Bird , R. Landi , A. Malizia , M. Molina , P. Ubertini

We present results on approximately one year of INTEGRAL observations of six AGN detected during the regular scans of the Galactic Plane. The sample is composed by five Seyfert 2 objects (MCG -05-23-16, NGC 4945, the Circinus galaxy, NGC…

Cen A hosts the closest active galactic nucleus to the Milky Way, which makes it an ideal target for investigating the dynamical processes in the vicinity of accreting supermassive black holes. In this paper, we present 14 Chandra HETGS…

In this paper, we present the hard X-ray spectral analysis of a complete sample of AGN de- tected by INTEGRAL/IBIS. In conjunction with IBIS spectra, we make use of Swift/BAT data, with the aim of cross-calibrating the two instruments,…

高能天体物理现象 · 物理学 2015-06-15 Manuela Molina , L. Bassani , A. Malizia , J. B. Stephen , A. J. Bird , A. Bazzano , P. Ubertini

We report on an analysis of \fermi data from four year of observations of the nearby radio galaxy Centaurus A (Cen A). The increased photon statistics results in a detection of high-energy ($>\:100$ MeV) $\gamma$-rays up to 50 GeV from the…

高能天体物理现象 · 物理学 2015-06-15 N. Sahakyan , R. Yang , F. A. Aharonian , F. M. Rieger

The Rossi X-ray Timing Explorer made a short (10 ks) observation of the radio galaxy Centaurus A on 14 August 1996. Analysis of the combined 2.5-240 keV spectrum has revealed a heavily absorbed(NH=9.42+/-0.24 e22 cm-2) primary power law…

In this letter we present the primary continuum parameters, the photon index Gamma and the high energy cut-off Ec, of 41 type-1 Seyfert galaxies extracted from the INTEGRAL complete sample of AGN. We performed a broad band (0.3-100 keV)…

高能天体物理现象 · 物理学 2015-06-18 A. Malizia , M. Molina , L. Bassani , J. B. Stephen , A. Bazzano , P. Ubertini , A. J. Bird

The question of the origin of the hard X-ray/soft gamma-ray emission in Centaurus A (Cen A) persists despite decades of observations. Results from X-ray instruments suggest a jet origin since the implied electron temperature (kT_e) would…

高能天体物理现象 · 物理学 2023-10-03 James Rodi , E. Jourdain , M. Molina , J. -P. Roques

In this paper we report on the broadband X-ray properties of a complete sample of 33 absorbed Seyfert galaxies hard X-ray selected with integral. The high quality broadband spectra obtained with both xmm, and integral-IBIS data are well…

宇宙学与河外天体物理 · 物理学 2011-12-21 A. De Rosa , F. Panessa , L. Bassani , A. Bazzano , A. J. Bird , R. Landi , A. Malizia , M. Molina , P. Ubertini

We present a detailed X-ray spectral analysis of the sources in the 1Ms catalog of the Chandra Deep Field South (CDFS) taking advantage of optical spectroscopy and photometric redshifts for 321 sources. As a default spectral model, we adopt…

We report on Cyg X-1 observations performed by the SPI telescope onboard the INTEGRAL mission and distributed over more than 6 years. We investigate the variability of the intensity and spectral shape of this peculiar source in the hard…

高能天体物理现象 · 物理学 2015-05-30 Elisabeth Jourdain , Jean-Pierre Roques , Julien Malzac

AGN exhibit complex hard X-ray spectra. Our current understanding is that the emission is dominated by inverse Compton processes which take place in the corona above the accretion disk, and that absorption and reflection in a distant…

高能天体物理现象 · 物理学 2009-06-25 V. Beckmann , T. J. -L. Courvoisier , N. Gehrels , P. Lubinski , J. Malzac , P. O. Petrucci , C. R. Shrader , S. Soldi

The anomalous X-ray pulsar 4U 0142+61 was studied by the INTEGRAL observations. The hard X-ray spectrum of 18 -- 500 keV for 4U 0142+61 was derived using near 9 years of INTEGRAL/IBIS data. We obtained the average hard X-ray spectrum of 4U…

高能天体物理现象 · 物理学 2015-05-27 Wei Wang , Hao Tong , Yan-Jun Guo

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 present four X-ray/gamma-ray spectra of Cyg X-1 observed in the hard ('low') state simultaneously by Ginga and GRO/OSSE on 1991 July 6. The 3-30 keV Ginga spectra are well represented by power laws with an energy spectral index of…

We present detailed spectral and temporal characteristics both in the hard X-ray (>10 keV) and soft X-ray (<10 keV) domains, obtained using data from INTEGRAL, XMM-Newton, ASCA and RXTE. The INTEGRAL time-averaged total spectrum shows a…

天体物理学 · 物理学 2009-11-13 P. R. den Hartog , L. Kuiper , W. Hermsen , V. M. Kaspi , R. Dib , J. Knoedlseder , F. P. Gavriil
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