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相关论文: BeppoSAX observations of low-energy spectral featu…

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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 report the results of quasi-simultaneous observations of the bright quasar 3C 273 using the BeppoSAX Low-Energy Concentrator Spectrometer (LECS) and the ASCA Solid-State Imaging Spectrometer (SIS). These observations are part of an…

天体物理学 · 物理学 2007-05-23 Astrid Orr , T. Yaqoob , A. N. Parmar , L. Piro , N. E. White , P. Grandi

We present 3 methods for the subtraction of non-cosmic and unresolved cosmic backgrounds observed by the Low-Energy Concentrator Spectrometer (LECS) on-board BeppoSAX. Removal of these backgrounds allows a more accurate modeling of the…

天体物理学 · 物理学 2017-03-22 A. N. Parmar , T. Oosterbroek , A. Orr , M. Guainazzi , N. Shane , M. J. Freyberg , D. Ricci , A. Malizia

We present optical spectroscopic identification of sources identified in the BeppoSAX MECS fields of the High Energy LLarge Area Survey (HELLAS). In total 62 sources from a sample of 115 brighter than F_{5-10keV}>5x10^{-14} cgs have been…

天体物理学 · 物理学 2007-05-23 F. La Franca , F. Fiore , C. Vignali , A. Comastri , F. Pompilio , HELLAS consortium

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…

The spectrum of the 0.1-7.0 keV cosmic X-ray background (CXB) at galactic latitudes >|25| degrees has been measured using the BeppoSAX Low-Energy Spectrometer Concentrator (LECS). Above 1 keV the spectrum is consistent with a power-law of…

天体物理学 · 物理学 2007-05-23 A. N. Parmar , M. Guainazzi , T. Oosterbroek , A. Orr , F. Favata , D. Lumb , A. Malizia

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 present the first results of BeppoSAX observations of a small sample of low brightness FRI radio galaxies. The flux of all the targets is consistent with a thermal spectrum, as due to the presence of hot intracluster gas or galactic…

天体物理学 · 物理学 2015-06-24 E. Trussoni , F. Vagnetti , S. Massaglia , L. Feretti , P. Parma , R. Morganti , R. Fanti , P. Padovani , G. Bodo

We have surveyed about 50 deg-2 of sky in the largely unexplored 5-10 keV band using the BeppoSAX MECS instrument, finding 180 sources. After correction for the non uniform sky coverage we find about 18 sources deg-2 with F(5-10keV) >=…

We present a 0.2-10 keV spectrum of the low-mass X-ray binary Cygnus X-2 obtained using the Low Energy Concentrator Spectrometer on-board Bepposax. The spectrum can be described by a cut-off power-law model with absorption of (2.28 +/-…

天体物理学 · 物理学 2007-05-23 E. Kuulkers , A. N. Parmar , A. Owens , T. Oosterbroek , U. Lammers

We report on highlight results on celestial sources observed in the high energy band (>20 keV) with BeppoSAX. In particular we review the spectral properties of sources that belong to different classes of objects, i.e. stellar coronae…

天体物理学 · 物理学 2009-10-30 F. Frontera , D. Dal Fiume , G. Malaguti , L. Nicastro , M. Orlandini , E. Palazzi , E. Pian , F. Favata , A. Santangelo

The integrated emission of highly obscured AGN is expected to provide a major contribution to the X-ray energy density in the Universe: the X-ray background (XRB). The study of these objects is possible only at energies where the effects of…

天体物理学 · 物理学 2007-05-23 A. Comastri , F. Fiore , C. Vignali , F. La Franca , G. Matt

The BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed several tens of square degrees of the sky in the 5--10 keV band down to a flux of about 5 10^-14 erg cm-2 s-1. The extrapolation of the HELLAS logN--logS towards fainter…

天体物理学 · 物理学 2009-11-06 A. Comastri , F. Fiore , C. Vignali , G. Matt , G. C. Perola , F. La Franca

The high energy experiment PDS is one of the Narrow Field Instruments aboard the X-ray astronomy satellite BeppoSAX. It covers the energy band from 15 to 300 keV. Here we report results on its in-flight performance and observations of…

天体物理学 · 物理学 2009-10-30 F. Frontera , D. Dal Fiume , E. Costa , M. Feroci , M. Orlandini , L. Nicastro , E. Palazzi , G. Zavattini , P. Giommi

The PDS experiment onboard BeppoSAX is the most sensitive instrument ever above 10 keV. Preliminary results on the complete catalogue of AGN observed with it are presented in this paper.

天体物理学 · 物理学 2009-09-25 M. Guainazzi , T. Oosterbroek

The BeppoSAX 4.5-10 keV High Energy Large Area Survey has covered about 80 square degrees of sky down to a flux of F(5-10keV)~5E-14 cgs. Optical spectroscopic identification of about half of the sources in the sample (62) shows that many…

We report the BeppoSAX observations of 6 Flat Spectrum Radio Quasars. Three of them have a clear detection up to 100 keV with the PDS instrument. For 4 objects the X-ray spectrum is satisfactorily fitted by a power-law continuum with…

The LINER nucleus of the nearby spiral galaxy M81 was pointed by BeppoSAX, which caught it at the highest (2-10) keV flux level observed so far. The LECS, MECS and PDS data, extending over (0.1-100) keV, are used to investigate the physical…

天体物理学 · 物理学 2007-05-23 S. Pellegrini , M. Cappi , L. Bassani , G. Malaguti , G. G. C. Palumbo , M. Persic

First results on a medium-deep X-ray survey in the "new" 5-10 keV band carried out with the MECS detectors onboard BeppoSAX are presented. The High Energy Llarge Area Survey (HELLAS) is aimed to directly explore a band where the energy…

天体物理学 · 物理学 2009-10-31 A. Comastri , F. Fiore , P. Giommi , F. La Franca , M. Elvis , G. Matt , S. Molendi , G. C. Perola

We present the preliminary results of a survey that makes use of several deep exposures obtained with the X-Ray telescopes of the BeppoSAX satellite. The survey limiting sensitivity is 5 x 10^-14 cgs in the 2-10 keV band and 7 x 10^-14 cgs…

天体物理学 · 物理学 2011-02-11 P. Giommi , F. Fiore , D. Ricci , S. Molendi , M. C. Maccarone , A. Comastri
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