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相关论文: The BeppoSAX Deep Surveys

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We present a comprehensive study of the soft X-ray properties of the BeppoSAX High-Energy Large Area Survey (HELLAS) sources. A large fraction (about 2/3) of the hard X-ray selected sources is detected by ROSAT. The soft X-ray colors for…

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

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

The XMM-Newton Slew Survey (XSS) covers a significant fraction of the sky in a broad X-ray bandpass. Although shallow by contemporary standards, in the `classical' 2-10 keV band of X-ray astronomy, the XSS provides significantly better…

宇宙学与河外天体物理 · 物理学 2015-06-11 R. S. Warwick , R. D. Saxton , A. M. Read

(abridged) We present an analysis of the deepest hard X-ray survey to date of about 2500 deg^2 performed by the IBIS instrument on board INTEGRAL in the 20-60 keV band, with a total exposure time of 4 Ms. We find 34 candidate sources. The…

天体物理学 · 物理学 2009-11-13 S. Paltani , R. Walter , I. M. McHardy , T. Dwelly , C. Steiner , T. J. -L. Courvoisier

A complete sample of 60 serendipitous hard X-ray sources with flux in the range $\sim 1 \times 10^{-13}$ \ecs to $\sim 4 \times 10^{-12}$ \ecs (2 - 10 keV), detected in 87 ASCA GIS2 images, was recently presented in literature. Using this…

天体物理学 · 物理学 2009-10-31 R. Della Ceca , G. Castelli , V. Braito , I. Cagnoni , T. Maccacaro

The spectrum of the 1.0-8.0 keV cosmic X-ray background (CXB) at galactic latitudes > 25 degrees has been measured using the BeppoSAX LECS and MECS instruments. The spectrum is consistent with a power-law of photon index 1.40 +/- 0.04 and…

天体物理学 · 物理学 2007-05-23 A. Vecchi , S. Molendi , M. Guainazzi , F. Fiore , A. N. Parmar

We summarize here some of the main results we have reached so far in the ASCA Hard Serendipitous Survey, a survey program conducted in the 2-10 keV energy band. In particular we will discuss the number-flux relationship, the 2-10 keV…

天体物理学 · 物理学 2007-05-23 R. Della Ceca , V. Braito , I. Cagnoni , T. Maccacaro

We present the first results of the hard (5-10 keV) ASCA GIS survey SHEEP (Search for the High Energy Extragalactic Population). We have analysed 149 fields covering an area of 39 sq. deg detecting 69 sources. Several of these appear to be…

天体物理学 · 物理学 2007-05-23 I. Georgantopoulos , K. Nandra , A. Ptak

At a flux limit of ~10^(-11) erg/cm2/s in the 20-100 keV band, the PDS instrument on-board BeppoSAX offers the opportunity to study the extragalactic sky with an unprecedented sensitivity. In this work we report on the results of a search…

天体物理学 · 物理学 2009-11-11 R. Landi , A. Malizia , L. Bassani

We present ASCA GIS observations (total exposure 100-200 ksec) of three fields which form part of our deep ROSAT survey. We detect 26 sources down to a limiting flux (2-10 keV) of 5x10^{-14} erg cm-2 s-1. Sources down to this flux level…

We present X-ray spectra obtained with BeppoSAX (Satellite per Astronomia X) of 10 BL Lac objects, selected from the Einstein Medium Sensitivity and Slew Surveys. We find that in about half of the objects a fit in the 0.1-10 keV range with…

We present a study of the hard X-ray properties of a sample that includes all the Luminous Infrared Galaxies (LIGs, L_IR > 10^11 L_sun) observed in the 2-10 keV energy band (new and archival data). We find that a significant fraction of the…

天体物理学 · 物理学 2007-05-23 G. Risaliti , R. Gilli , R. Maiolino , M. Salvati

We report results of a serendipitous hard X-ray (3--20 keV), nearly all-sky (|b|>10deg) survey based on RXTE/PCA observations performed during satellite reorientations in 1996--2002. The survey is 80% (90%) complete to a 4$\sigma$ limiting…

天体物理学 · 物理学 2009-11-10 M. Revnivtsev , S. Sazonov , K. Jahoda , M. Gilfanov

The main results of broad-band (0.1-10 keV) BeppoSAX observations of a selected sample of NLS1s are presented and discussed. It is shown that all the available data are consistent with a scenario in which NLS1s are running at a high…

天体物理学 · 物理学 2009-10-31 Andrea Comastri

We present the X-ray source catalog in the Subaru/XMM-Newton deep survey. A continuous area of 1.14 deg^2 centered at R.A. = 02h18m and Dec. = -05d is mapped by seven pointings with XMM-Newton covering the 0.2-10 keV band. From the combined…

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 present the Extragalactic Serendipitous Swift Survey (ExSeSS), providing a new well-defined sample constructed from the observations performed using the Swift X-ray Telescope. The ExSeSS sample consists of 79,342 sources detected in the…

高能天体物理现象 · 物理学 2023-01-25 Jack N. Delaney , James Aird , Phil A. Evans , Cassandra Barlow-Hall , Julian P. Osborne , Michael G. Watson

(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

The nearby galaxy M33 was observed by the imaging X-ray instruments on-board BeppoSAX. Two observations at different phases of the 105.9 day intensity cycle of the luminous central source X-8 failed to reveal the expected modulation,…

The BeppoSAX satellite performed a survey of the Galactic Center Region in the 1-10 keV energy band with its Narrow Field Instruments. Several bright X-ray sources containing neutron stars and black holes have been observed and studied,…

天体物理学 · 物理学 2009-10-31 L. Sidoli , S. Mereghetti , A. Treves , L. Chiappetti , G. L. Israel , M. Orlandini , ;