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相关论文: High-Energy sources before INTEGRAL -- INTEGRAL re…

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We present results of observations of the Aql X-1 field performed in March-April 2003 with the INTEGRAL observatory. This TOO (Target Of Opportunity) INTEGRAL observations was initiated upon receiving an indication from the ASM/RXTE that…

天体物理学 · 物理学 2016-08-30 S. Molkov , A. Lutovinov , S. Grebenev

The second IBIS/ISGRI survey has produced a catalogue containing 209 hard X-ray sources visible down to a flux limit of around 1 milliCrab. The point source location accuracy of typically 1-3 arcminutes has allowed the counterparts for most…

天体物理学 · 物理学 2009-11-11 J. B. Stephen , L. Bassani , A. Malizia , A. Bazzano , P. Ubertini , A. J. Bird , A. J. Dean , F. Lebrun , R. Walter

The latest INTEGRAL/IBIS all-sky survey lists 219 hard X-ray sources whose nature is still unknown. We report on our ongoing campaign aimed at identifying these high-energy emitters by exploiting the focusing capabilities of the X-ray…

高能天体物理现象 · 物理学 2017-07-05 R. Landi , L. Bassani , A. Bazzano , A. J. Bird , M. Fiocchi , A. Malizia , F. Panessa , V. Sguera , P. Ubertini

We present a catalog of 5184 candidate infrared counterparts to X-ray sources detected towards the Galactic center. The X-ray sample contains 9017 point sources detected in this region by the Chandra X-ray Observatory, including data from a…

星系天体物理 · 物理学 2009-09-28 Jon C. Mauerhan , Michael P. Muno , Mark R. Morris , Franz E. Bauer , Shogo Nishiyama , Tetsuya Nagata

We have carried out an extensive search for gamma-ray lines in the first year of public data from the Spectrometer (SPI) on the INTEGRAL mission. INTEGRAL has spent a large fraction of its observing time in the Galactic Plane with…

天体物理学 · 物理学 2008-11-26 B. J. Teegarden , K. Watanabe

The hard X-ray source IGR J16318-4848 was recently discovered by the INTEGRAL observatory (Courvoisier et al.) and subsequently uncovered in archival data of ASCA observations in 1994 (Murakami et al.). We present results of a detailed…

天体物理学 · 物理学 2009-11-07 M. Revnivtsev , S. Sazonov , M. Gilfanov , R. Sunyaev

We present the first unbiased source catalog of the Monitor of All-sky X-ray Image (MAXI) mission at high Galactic latitudes ($|b| > 10^{\circ}$), produced from the first 7-month data (2009 September 1 to 2010 March 31) of the Gas Slit…

INTEGRAL made 3 observations in 2003 April of the black hole candidate H 1743-322 during the rising part, and close to the maximum, of an outburst. H 1743-322 was previously observed in outburst in 1977-1978. The source is located in a…

天体物理学 · 物理学 2009-11-10 A. N. Parmar , E. Kuulkers , T. Oosterbroek , P. Barr , R. Much , A. Orr O. R. Williams , C. Winkler

We present results from a sample of 106 high-luminosity IRAS sources observed with the Very Large Array in the B and C configurations. 96 sources were observed in the X-band and 52 in the K-band, with 42 of them observed at both…

星系天体物理 · 物理学 2023-06-16 D. Quiroga-Gonzalez , M. A. Trinidad , E. de la Fuente , J. M. Masque , T. Rodriguez-Esnard

With the unequalled INTEGRAL observatory, ESA has provided a unique tool to the astronomical community that has made Europe the world leader in the field of gamma-ray astronomy. INTEGRAL provides an unprecedented survey of the soft…

天体物理学 · 物理学 2008-11-26 Jürgen Knödlseder

Deep observations of the Small Magellanic Cloud (SMC) and region were carried out in the hard X-ray band by the INTEGRAL observatory in 2008-2009. The field of view of the instrument permitted simultaneous coverage of the entire SMC and the…

The COMPTEL unidentified source GRO J1411-64 was observed by INTEGRAL, and its central part, also by XMM-Newton. The data analysis shows no hint for new detections at hard X-rays. The upper limits in flux herein presented constrain the…

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL. The high energy spectrum exhibits such a high column density that the source is undetectable in X-rays below 2 keV. We used the NTT telescope of ESO to obtain…

天体物理学 · 物理学 2009-11-10 P. Filliatre , S. Chaty

We present a new edition of the catalogue of high-mass X-ray binaries in the Galaxy. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other…

天体物理学 · 物理学 2008-11-26 Q. Z. Liu , J. van Paradijs , E. P. J. van den Heuvel

Results of simultaneous INTEGRAL and optical observations of galactic microquasar SS433 in May 2003 and INTEGRAL/RXTE observations in March 2004 are presented. Persistent precessional variability with a maximum to minimum uneclipsed hard…

AX J1910.7+0917 is a still unidentified source discovered with ASCA and observed more recently with IBIS/ISGRI, mainly noticeable for its rather hard spectrum. We analyzed all the public available data on this source, and we took advantage…

高能天体物理现象 · 物理学 2011-04-28 L. Pavan , E. Bozzo , C. Ferrigno , C. Ricci , A. Manousakis , R. Walter , L. Stella

The X-ray spectra of X-ray binaries are dominated by emission of either soft or hard X-rays which defines their soft and hard spectral states. Cygnus X-3 is amongst the list of X-ray binaries that show quite complex behavior, with various…

高能天体物理现象 · 物理学 2021-01-20 F. Cangemi , J. Rodriguez , V. Grinberg , R. Belmont , P. Laurent , J. Wilms

IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23--28 April 2003. Aims: To detect new outbursts from IGR J18483-0311 using INTEGRAL…

天体物理学 · 物理学 2009-11-13 V. Sguera , A. B. Hill , A. J. Bird , A. J. Dean , A. Bazzano , P. Ubertini , N. Masetti , R. Landi , A. Malizia , D. J. Clark , M. Molina

We report on temporal and spectral analysis of the INTEGRAL fast transient candidate IGR J16328-4726 observed with Beppo SAX in 1998 and more recently with INTEGRAL. The MECS X-ray data show a frequent micro activity typical of the…

高能天体物理现象 · 物理学 2015-06-11 M. Fiocchi , A. Bazzano , A. J. Bird , S. P. Drave , L. Natalucci , P. Persi , L. Piro , P. Ubertini

In June 2015, the source V404 Cygni (= GS2023+38) underwent an extraordinary outburst. We present the results obtained during the first revolution dedicated to this target by the INTEGRAL mission, and focus on the spectral behavior in the…