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相关论文: INTEGRAL and XMM-Newton observations towards the u…

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The COMPTEL unidentified source GRO J 1411-64 was observed by INTEGRAL and XMM-Newton in 2005. The Circinus Galaxy is the only source detected within the 4$\sigma$ location error of GRO J1411-64, but in here excluded as the possible…

IGR J16318-4848 is the prototype and one of the more extreme examples of the new class of highly obscured Galactic X-ray sources discovered by INTEGRAL. A monitoring campaign on this source has been carried out by XMM-Newton and INTEGRAL,…

天体物理学 · 物理学 2009-11-11 A. Ibarra , G. Matt , M. Guainazzi , E. Kuulkers , E. Jimenez-Bailon , J. Rodriguez , F. Nicastro , R. Walter

On 2003 September 17 INTEGRAL discovered a bright transient source 3 degrees from the Galactic Center, IGR J17544-2619. The field containing the transient was observed by XMM-Newton on 2003 March 17 and September 11 and 17. A bright source,…

天体物理学 · 物理学 2009-11-10 R. Gonzalez-Riestra , T. Oosterbroek , E. Kuulkers , A. Orr , A. N. Parmar

About 30% of the sources in the 4th INTEGRAL-IBIS catalogue are unidentified in that they lack an optical counterpart. To be able to classify them, X-ray observations are of crucial importance as they can place tighter constraints on the…

高能天体物理现象 · 物理学 2015-05-19 A. Malizia , L. Bassani , V. Sguera , J. B. Stephen , A. Bazzano , M. Fiocchi , A. J. Bird

We report on the results of a deep 1.6 Ms INTEGRAL observation of the Cassiopeia region performed from December 2003 to February 2004. Eleven sources were detected with the imager IBIS-ISGRI at energies above 20 keV, including three new…

天体物理学 · 物理学 2009-11-11 P. R. den Hartog , W. Hermsen , L. Kuiper , J. Vink , J. J. M. in 't Zand , W. Collmar

This letter presents the first results of an observational campaign to study the Galactic Centre with INTEGRAL. The mosaicked images obtained with the IBIS/ISGRI coded aperture instrument in the energy ranges 20-40 and 40-100 keV, give a…

A number of new X-ray sources (IGR J17091-3624, IGR/XTE J17391-3021, IGR J17464-3213 (= XTE J17464-3213 = H 1743-322), IGR J17597-2201, SAX/IGR J18027-2017) have been observed with the INTEGRAL observatory during ultra deep exposure of the…

天体物理学 · 物理学 2009-11-10 A. Lutovinov , M. Revnivtsev , S. Molkov , R. Sunyaev

The fourth transient accreting millisecond pulsar XTE J1807-294 was observed during its February/March 2003 outburst by INTEGRAL, partly simultaneously with the XMM-Newton and RXTE satellites. We present here the first study of the 0.5-200…

A recent analysis of COMPTEL data has revealed the existence of an unidentified and variable gamma-ray source, designated GRO J1411-64, at MeV energies in the galactic plane (Zhang et al. 2002). We discuss the possibility that such a source…

天体物理学 · 物理学 2007-05-23 Gustavo E. Romero , Mariana Orellana , Diego F. Torres

Hard X-ray imaging of the Galactic plane by the INTEGRAL satellite is uncovering large numbers of 20-100 keV "IGR" sources. We present results from Chandra, INTEGRAL, optical, and IR observations of 4 IGR sources: 3 sources in the Norma…

天体物理学 · 物理学 2011-02-11 John A. Tomsick , Sylvain Chaty , Jerome Rodriguez , Luigi Foschini , Roland Walter , Philip Kaaret

We present the results of Chandra and XMM-Newton observations for six hard X-ray sources (IGR J12134-6015, IGR J18293-1213, IGR J18219-1347, IGR J17350-2045, IGR J18048-1455, XTE J1901+014) from the INTEGRAL all-sky survey. Based on these…

高能天体物理现象 · 物理学 2015-06-11 D. I. Karasev , A. A. Lutovinov , M. G. Revnivtsev , R. A. Krivonos

We study the hard X-ray (20-100 keV) variability of the Galactic Center (GC) and of the nearby sources on the time scale of 1000 s. We find that 3 of the 6 hard X-ray sources detected by INTEGRAL within the central 1 degree of the Galaxy…

天体物理学 · 物理学 2007-05-23 A. Neronov , M. Chernyakova , T. J. -L. Courvoisier , R. Walter

The limited angular resolution of gamma-ray telescopes prevents a direct identification of the majority of sources detected so far. This is particularly true for the low latitude, probably galactic, ones only 10 % of which has been…

天体物理学 · 物理学 2009-11-11 N. La Palombara , R. P. Mignani , E. Hatziminaoglou , M. Schirmer , G. F. Bignami , P. Caraveo

The 0.5-150 keV broad-band spectra of a sample of nine bright type 1 Seyfert galaxies are analyzed here. These sources have been discovered/detected by INTEGRAL and subsequently observed with XMM--Newton for the first time with high…

天体物理学 · 物理学 2009-11-13 F. Panessa , L. Bassani , A. De Rosa , A. J. Bird , A. J. Dean , M. Fiocchi , A. Malizia , M. Molina , P. Ubertini , R. Walter

Early results from the INTEGRAL Core Program, for a sample of eight persistently bright neutron star low mass X-ray binaries in the energy range from 5 keV to 200 keV are presented. It is shown that INTEGRAL efficiently detects sources and…

The discovery of the X-ray source IGR J17252-3616 by INTEGRAL was reported on 9 February 2004. Regular monitoring by INTEGRAL shows that IGR J17252-3616 is a persistent hard X-ray source with an average count rate of 0.96 counts/s (~6.4…

(abridged) The first unidentified very high energy gamma ray source (TeV J2032+4130) in the Cygnus region has been the subject of intensive search for a counterpart source at other wavelengths. A deep ($\approx 50$ ksec) exposure of TeV…

天体物理学 · 物理学 2009-11-13 D. Horns , A. I. D. Hoffmann , A. Santangelo , F. A. Aharonian , G. P. Rowell

We report the detection of an unidentified gamma-ray source near the Galactic plane by the COMPTEL experiment aboard the Compton Gamma-Ray Observatory. The source is detected at a significance level of ~ 7.2 sigma in the energy range 1-3…

天体物理学 · 物理学 2009-11-07 S. Zhang , W. Collmar , V. Schonfelder

We present the results of the XMM-Newton observations of five hard X-ray emitters: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703, and IGR J17348-2045. The first source is a confirmed supergiant high mass X-ray binary,…

高能天体物理现象 · 物理学 2015-06-05 E. Bozzo , L. Pavan , C. Ferrigno , M. Falanga , S. Campana , S. Paltani , L. Stella , R. Walter

(abridged) We performed a homogeneous and systematic analysis of simultaneous X-ray and optical/UV properties of a group of 15 gamma-ray loud AGN, using observations performed with XMM-Newton. The sample is composed of 13 blazars (6 BL Lac…

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