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Related papers: IGR J17451-3022: a dipping and eclipsing low mass …

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We report on the broadband spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498$-$2921 during its April 2023 outburst using data from NICER (1$-$10 keV), NuSTAR (3$-$79 keV), Insight-HXMT (2$-$150 keV), and…

High Energy Astrophysical Phenomena · Physics 2024-11-06 Zhaosheng Li , L. Kuiper , Y. Y. Pan , M. Falanga , J. Poutanen , Y. P. Chen , R. X. Xu , M. Y. Ge , Y. Huang , L. M. Song , S. Zhang , F. J. Lu , S. N. Zhang

We present timing and spectral analysis of a sample of seven hard X-ray selected Cataclysmic Variable candidates based on simultaneous X-ray and optical observations collected with XMM-Newton , complemented with Swift/BAT and INTEGRAL/IBIS…

High Energy Astrophysical Phenomena · Physics 2017-08-02 F. Bernardini , D. de Martino , K. Mukai , D. M. Russell , M. Falanga , N. Masetti , C. Ferrigno , G. Israel

We report the results of extensive high-energy observations of the X-ray transient and black hole candidate XTE J1720-318 performed with INTEGRAL, XMM-Newton and RXTE. The source, which underwent an X-ray outburst in 2003 January, was…

Context. Supergiant fast X-ray transients are a subclass of high mass X-ray binaries that host a neutron star accreting mass from the wind of its OB supergiant companion. They are characterized by an extremely pronounced and rapid…

High Energy Astrophysical Phenomena · Physics 2015-05-18 E. Bozzo , L. Stella , C. Ferrigno , A. Giunta , M. Falanga , S. Campana , G. Israel , J. C. Leyder

We report here discovery of a 3.32 day orbital period in the Supergiant Fast X-ray Transient (SFXT) source IGR J16479-4514. Using the long term light curve of this source obtained with Swift-BAT in the energy range of 15-50 keV, we have…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Chetana Jain , Biswajit Paul , Anjan Dutta

We report on the identification of the new Galactic Center (GC) transient Swift J174540.7-290015 as a likely low mass X-ray binary (LMXB) located at only 16 arcsec from Sgr A*. This transient was detected on 2016 February 6th during the…

High Energy Astrophysical Phenomena · Physics 2016-06-15 G. Ponti , C. Jin , B. De Marco , N. Rea , A. Rau , F. Haberl , F. Coti Zelati , E. Bozzo , C. Ferrigno , G. C. Bower , P. Demorest

We have used the RXTE and INTEGRAL satellites simultaneously to observe the High Mass X-ray binary IGR J19140+0951. The spectra obtained in the 3-80 keV range have allowed us to perform a precise spectral analysis of the system along its…

Astrophysics · Physics 2009-06-23 Lionel Prat , Jerome Rodriguez , Diana C. Hannikainen

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…

High Energy Astrophysical Phenomena · Physics 2015-06-11 M. Fiocchi , A. Bazzano , A. J. Bird , S. P. Drave , L. Natalucci , P. Persi , L. Piro , P. Ubertini

The X-ray burster 4U1850-087, located in the Galactic globular cluster NGC6712, is an ultracompact binary (orbital period~21 min),likely harbouring a degenerate companion.The source has been observed at soft gamma-rays several times with…

Astrophysics · Physics 2009-11-11 L. Sidoli , A. Paizis , A. Bazzano , S. Mereghetti

We report on the X-ray properties of the new transient Swift J0840.7$-$3516, discovered with Swift/BAT in 2020 February, using extensive data of Swift, MAXI, NICER, and NuSTAR. The source flux increased for $\sim 10^3$ s after the…

We report on a spectroscopic analysis of the X-ray emission from IGR J17062-6143 in the aftermath of its June 2020 intermediate duration Type I X-ray burst. Using the Neutron Star Interior Composition Explorer, we started observing the…

We report on the detection and follow-up multi-wavelength observations of the new X-ray transient MAXI J1807+132 with the MAXI/GSC, Swift, and ground-based optical telescopes. The source was first recognized with the MAXI/GSC on 2017 March…

We report on the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsar IGR J17591-2342, detecting coherent X-ray pulsations…

IGRJ17361-4441 is a newly discovered INTEGRAL hard X-ray transient, located in the globular cluster NGC6388. We report here the results of the X-ray and radio observations performed with Swift, INTEGRAL, RXTE, and the Australia Telescope…

High Energy Astrophysical Phenomena · Physics 2015-05-30 E. Bozzo , C. Ferrigno , J. Stevens , T. M. Belloni , J. Rodriguez , P. R. den Hartog , A. Papitto , I. Kreykenbohm , F. Fontani , L. Gibaud

We have analysed in detail the discovery measurements of the X-ray burster SAX J1750.8-2900 by the Wide Field Cameras on board BeppoSAX in spring 1997, at a position ~1.2 degrees off the Galactic Centre. The source was in outburst on March…

We report on the discovery of a new X-ray pulsator, Swift J201424.9+152930 (Sw J2014). Owing to its X-ray modulation at 491 s, it was discovered in a systematic search for coherent signals in the archival data of the Swift X-ray Telescope.…

IGR J11305-6256 is one of the numerous sources discovered through the INTEGRAL scan of the Galactic Plane. Thanks to the Swift-BAT survey, that allows the frequent sampling of any sky region, we have discovered in the hard X-ray emission of…

High Energy Astrophysical Phenomena · Physics 2013-05-20 V. La Parola , A. D'Aì , G. Cusumano , A. Segreto , N. Masetti , A. Melandri

IGR J08408-4503 is a supergiant fast X-ray transient discovered in 2006 with a confirmed association with a O8.5Ib(f) supergiant star, HD 74194. We report on the analysis of two outbursts caught by Swift/BAT on 2006 October 4 and 2008 July…

IGR J17407-2808 is an enigmatic and poorly studied X-ray binary that was recently observed quasi-simultaneously with NuSTAR and XMM-Newton. In this paper we report the results of this observational campaign. During the first 60 ks of…

High Energy Astrophysical Phenomena · Physics 2023-06-14 L. Ducci , C. Malacaria , P. Romano , E. Bozzo , M. Berton , A. Santangelo , E. Congiu

The X-ray source RX J004717.4-251811 in the nearby starburst galaxy NGC 253 was found to undergo changes from a low to a high state twice, during an XMM-Newton EPIC observation in December 2000 and also during a Chandra observation one year…

Astrophysics · Physics 2009-11-07 W. Pietsch , F. Haberl , A. Vogler