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相关论文: The hidden X-ray Seyfert nucleus in 3C 273: BeppoS…

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We present preliminary results of BeppoSAX AO1 observations of 3C 273 performed in January 1997. We also present a close comparison with data obtained during the satellite SVP, in July 1996. On average, the AO1 flux is about a factor 2…

天体物理学 · 物理学 2019-08-14 Francesco Haardt

We report the results of a 3C273 observation performed during the Science Verification Phase (SVP) of the BeppoSax satellite. The broad-band spectrum is well represented by a power-law between 1 keV and 200 keV. The spectral slope is flat…

A BeppoSAX observation of the BLRG 3C390.3 is reported. For the first time, both the 6.4 keV iron line and a strong reflection hump, produced by the illumination of the primary X-ray emission on cold matter, are detected in this source. The…

天体物理学 · 物理学 2007-05-23 P. Grandi , M. Guainazzi , F. Haardt , L. Maraschi , E. Massaro , G. Matt , L. Piro , C. M. Urry

The apparency of low energy absorption features in Blazar LECS spectra has been reported during the early phase of the BeppoSAX mission (e.g. by Grandi et al. 1997 for 3C~273 SVP data; Giommi et al. 1997 for PKS 2155--304 SVP data), with…

天体物理学 · 物理学 2007-05-23 G. Fossati , F. Haardt

shortened) Results obtained from 9 X-ray observations of 3C 273 performed by ASCA are presented (for a total exposure time of about 160 000 s). The analysis and interpretation of the results is complicated by the fact that 4 of these…

天体物理学 · 物理学 2015-06-24 M. Cappi , M. Matsuoka , C. Otani , K. M. Leighly

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 present BeppoSAX observations of the Seyfert 1.8 galaxy NGC1365 in the 0.1--100 keV range. The source was 6 times brighter than during an ASCA observation 3 years earlier. The 4--10 keV flux is highly variable during the BeppoSAX…

天体物理学 · 物理学 2007-05-23 G. Risaliti , R. Maiolino , L. Bassani

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 present the results of the analysis of an archival 15 ks XMM-Newton observation of the nearby (z=0.057) radio-loud source 3C445, optically classified as a Broad-Line Radio Galaxy. While the RGS data are of insufficient quality to allow a…

天体物理学 · 物理学 2009-06-23 R. M. Sambruna , J. N. Reeves , V. Braito

We present the results of blazar 3C 273 obtained from simultaneous observations obtained using XMM-Newton and NuSTAR satellites during the period 2015-2019 in five epochs. When the spectra are modeled with a power-law, significant residuals…

高能天体物理现象 · 物理学 2025-02-19 Haritma Gaur , Main Pal , Muhammad S. Anjum , Kiran Wani , Pankaj Kushwaha , Ashwani Pandey , Liang Chen

We report the transition to an active state of the nucleus in the Seyfert 1.9 galaxy NGC 2992, discovered by means of new hard X-ray data. While the 2-10 keV flux declined by a factor of ~ 20 from 1978 to 1994, two recent BeppoSAX…

天体物理学 · 物理学 2007-05-23 R. Gilli , R. Maiolino , A. Marconi , G. Risaliti , M. Dadina , K. A. Weaver , E. J. M. Colbert

We report optical, radio and X-ray observations of the Narrow-Line Seyfert 1 galaxy RX J1702.5+3247. The soft (0.1-2 keV) X-ray flux, measured by BeppoSAX, is characterized by strong variability on short time scales (< 500 sec). The most…

天体物理学 · 物理学 2009-11-06 M. Gliozzi , W. Brinkmann , S. A. Laurent-Muehleisen , E. C. Moran , J. Whalen

We report on the 20 ksec observation of Vela X-1 performed by BeppoSAX on 1996 July 14 during its Science Verification Phase. We observed the source in two intensity states, characterized by a change in luminosity of a factor ~ 2, and a…

We have made BeppoSAX observations of the Seyfert 2/1.9 galaxy ESO103-G35, which contains a nuclear maser source and is known to be heavily absorbed in the X-rays. Analysis of the X-ray spectra observed by SAX in October 1996 and 1997…

天体物理学 · 物理学 2009-10-31 Belinda J. Wilkes , Smita Mathur , Fabrizio Fiore , Angelo Antonelli , Fabrizio Nicastro

We report broad-band X-ray measurements of the Be star Gamma Cassiopeiae by the BeppoSAX X-ray astronomy satellite. The observations took place on 1998 July, 18-23. The 0.1-200 keV X-ray spectrum is reasonably well fit by an optically thin…

天体物理学 · 物理学 2007-05-23 A. Owens , T. Oosterbroek , A. N. Parmar , R. Schulz , J. A. Stuwe , F. Haberl

We present a detailed X-ray study of the Broad Line Radio Galaxy 3C382, observed with the BeppoSAX satellite in a very bright state. The continuum emission is well modeled with a power law that steepens at high energies, with an e-folding…

天体物理学 · 物理学 2009-11-06 Paola Grandi , Laura Maraschi , C. Meg Urry , Giorgio Matt

We present the results of a long-look monitoring of 3C273 with RXTE between 1996 and 2000. A total of 230 observations amounts to a net exposure of 845ksec, with this spectral and variability analysis of 3C273 covering the longest…

We present new BeppoSAX LECS, MECS and PDS observations of five lobe-dominated, broad-line active galactic nuclei selected from the 2-Jy sample of southern radio sources. These include three radio quasars and two broad-line radio galaxies.…

天体物理学 · 物理学 2008-11-26 Paolo Padovani , Raffaella Morganti , Joachim Siebert , Fausto Vagnetti , Andrea Cimatti

We report results of a BeppoSAX observation of the low-mass X-ray binary (LMXB) dipping source XB 1916-053. The source joins the small group of LMXB detected at energies ~100 keV. The non-dip spectrum is well fitted by an absorbed blackbody…

天体物理学 · 物理学 2007-05-23 M. J. Church , A. N. Parmar , M. Balucinska-Church , T. Oosterbroek , D. Dal Fiume , M. Orlandini

We present new BeppoSAX LECS, MECS, and PDS observations of five lobe-dominated, broad-line active galactic nuclei selected from the 2 Jy sample of southern radio sources. These include three radio quasars and two broad-line radio galaxies.…

天体物理学 · 物理学 2009-10-30 R. Morganti , P. Padovani , J. Siebert , A. Cimatti , C. N. Tadhunter , F. Vagnetti
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