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相关论文: The X-ray absorber of PKS2126-158

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A BeppoSAX observation of the z=2.34 quasar PKS2149-306 produced a strong signal in the high energy PDS instrument up to a maximum observed energy of nearly 50 keV, 150 keV in the quasar frame. The Beppo-SAX spectrum spans almost 3 decades…

We present the 0.1-200 keV BeppoSAX spectrum of MR 2251-178 observed at two epochs in 1998 separated by 5 months. Both epochs show identical spectral shape and X-ray flux. Analysis of the combined spectra allow us to confirm the presence of…

天体物理学 · 物理学 2009-11-06 A. Orr , P. Barr , M. Guainazzi , A. N. Parmar , A. J. Young , ;

BeppoSAX observations of the high redshift (z=4.72) blazar GB 1428+4217 confirm the presence of a complex soft X-ray spectrum first seen with the ROSAT PSPC. Flattening below a rest frame energy of 5 keV can be accounted for by absorption…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , A. Celotti , K. Iwasawa , G. Ghisellini

A long ($>100,000$ seconds) observation of the bright BL Lac object PKS 2155-304 has been carried out with the Narrow Field Instruments of the BeppoSAX satellite as part of the Science Verification Phase. The source was detected between 0.1…

天体物理学 · 物理学 2007-05-23 P. Giommi et al

We report on the results of the spectral and timing analysis of a BeppoSAX observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with Fx(1-10 keV)= 4.7 x 10^{-12} erg cm^{-2} s^{-1}, which…

天体物理学 · 物理学 2009-11-07 P. Reig , M. Ribo , J. M. Paredes , J. Marti

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

We present the results of XMM-Newton observations of four high-z quasars, two radio-loud and two radio-quiet. One of the radio-loud objects, PKS 2126-158, clearly shows absorption in excess of the galactic value as claimed before from ASCA…

天体物理学 · 物理学 2011-05-23 E. Ferrero , W. Brinkmann

This paper presents a BeppoSAX observation of NGC 7582 made during 1998 November and an optical spectrum taken in 1998 October. The new X-ray data reveal a previously unknown hard X-ray component in NGC 7582, peaking close to 20 keV. Rapid…

天体物理学 · 物理学 2009-10-31 T. J. Turner , G. C. Perola , F. Fiore , G. Matt , I. M. George , L. Piro , L. Bassani

Results of a 2000 August 12-13 BeppoSAX observation of the 7.1 hr eclipsing, dipping, bursting, transient, low-mass X-ray binary (LMXRB) X1658-298 are presented. The spectrum outside of eclipses, dips and bursts can be modeled by the…

天体物理学 · 物理学 2009-11-06 T. Oosterbroek , A. N. Parmar , L. Sidoli , J. J. M. in 't Zand , J. Heise

We report on BeppoSAX observations of the X-ray transient XTE J0421+560 in quiescence 156, 541, and ~690 days after the maximum of the 1998 April outburst. In the first observation the source was soft with a power-law photon index of 4.0…

天体物理学 · 物理学 2007-05-23 A. N. Parmar , T. Belloni , M. Orlandini , D. Dal Fiume , A. Orr , N. Masetti

ASCA observations of 4 high redshift radio--loud quasars with 1.44$<$z$<$3.21 are presented. The spectral analysis for three of them (PKS 0332-403, PKS 0537-286, PKS 2149-306) reveals that their X-ray continuum emission is well represented…

天体物理学 · 物理学 2007-05-23 J. Siebert , M. Matsuoka , W. Brinkmann , M. Cappi , T. Mihara , T. Takahashi

We present results from BeppoSAX observations of 10 low redshift quasars. The quasars are part of the Laor et al. (1997) sample of 23 optically selected PG quasars with redshift <0.4 and low Galactic absorption along the line of sight.…

天体物理学 · 物理学 2007-05-23 T. Mineo , F. Fiore , A. Laor , E. Costantini , W. N. Brandt , A. Comastri , R. Della Ceca , M. Elvis , T. Maccacaro , S. Molendi

(Abridged) Spectral and time variability analysis of the region of the hard X-ray transient EXS 1737.9-2952 near the Galactic Centre (GC), using data from the Narrow Field Instruments of BeppoSAX is reported. The main results are the MECS…

天体物理学 · 物理学 2007-05-23 J. Huovelin , J. Schultz , O. Vilhu , D. Hannikainen , P. Muhli , Ph. Durouchoux

BeppoSAX observed 8 times the gamma-ray bright blazar PKS 0528+134 in Feb. and Mar. 1997, during a multiwavelength campaign involving EGRET, onboard CGRO, and ground based telescopes. The source was in its faintest X-ray state observed so…

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

During a BeppoSAX observation of the low-mass X-ray binary dip source XB 1323-619 a total of 10 type I X-ray bursts and parts of 12 intensity dips were observed. During non-bursting, non-dipping intervals, the 1-150 keV BeppoSAX spectrum…

天体物理学 · 物理学 2007-05-23 M. Balucinska-Church , M. J. Church , T. Oosterbroek , A. Segreto , R. Morley , A. N. Parmar

We present the results of a BeppoSAX observation of the fastest rotating pulsar known: PSR B1937+21. The ~200 ks observation (78.5 ks MECS/34 ks LECS on-source time) allowed us to investigate with high statistical significance both the…

天体物理学 · 物理学 2008-11-26 L. Nicastro , G. Cusumano , O. Loehmer , M. Kramer , L. Kuiper , W. Hermsen , T. Mineo , W. Becker

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

The BeppoSAX Narrow Field Instruments observed the galactic source GS1826-238 in October 1997, following a hard X-ray outburst with a peak flux of about 100 mCrab detected by BATSE. Two short X-ray bursts (about 150 s) were detected up to…

We report on the BeppoSAX observations of the gamma-ray blazar PKS 0528+134 performed in Feb and Mar 1997, during a multiwavelength campaign involving EGRET and ground based telescopes. The source was in a faint and hard state, with energy…

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