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The X-ray transient source EP240309a/EP\,J115415.8$-$501810 was first detected by the Wide-Field X-ray Telescope (WXT) on board Einstein Probe (EP) during the commissioning phase. Subsequent optical observations confirmed it as a…

We report on high energy observations of IGR J19140+0951 performed with RXTE on three occasions in 2002, 2003 and 2004, and INTEGRAL during a very well sampled and unprecedented high energy coverage of this source from early-March to…

Astrophysics · Physics 2009-11-10 J. Rodriguez , C. Cabanac , D. C. Hannikainen , V. Beckmann , S. E. Shaw , J. Schultz

We present the broadband phase averaged spectrum of one of the brightest intermediate polars V1223 Sgr, obtained with INTEGRAL and RXTE observatories (3-100 keV). Good statistical quality of the spectrum in a hard X-ray energy band…

Astrophysics · Physics 2009-11-10 M. Revnivtsev , A. Lutovinov , V. Suleimanov , R. Sunyaev , V. Zheleznyakov

Context: IGRJ11014-6103 is one of the still unidentified hard X-ray INTEGRAL sources, reported for the first time in the 4th IBIS/ISGRI catalog. Aims: We investigated the nature of IGR J11014-6103 by carrying out a multiwavelength analysis…

High Energy Astrophysical Phenomena · Physics 2013-03-20 L. Pavan , E. Bozzo , G. Pühlhofer , C. Ferrigno , M. Balbo , R. Walter

IGR J01583+6713 is a new transient source discovered by the INTEGRAL/IBIS hard X-ray surveys. Optical observations suggested that it should be a high mass X-ray binary, but its nature is still unclear. We used the INTEGRAL/IBIS data to…

High Energy Astrophysical Phenomena · Physics 2015-05-14 W. Wang

The European gamma-ray observatory INTEGRAL has found a group of hard X-ray sources which are highly absorbed, i.e., with column densities higher than about 10^{23}/cm^2. Here I give an overview of this class of INTEGRAL sources. The X-ray,…

Astrophysics · Physics 2009-11-11 Erik Kuulkers

Since its launch INTEGRAL has devoted a significant fraction of its observing time to the Galactic plane region. We present the results of INTEGRAL observations of the inner spiral arms of the Galaxy (Norma, Scutum and Sagittarius) with…

Astrophysics · Physics 2009-11-10 A. Lutovinov , M. Revnivtsev , M. Gilfanov , P. Shtykovskiy , S. Molkov , R. Sunyaev

We report on optical follow-up observations of an X-ray source initially detected by the Einstein Probe mission. Our investigations categorize the source as an intermediate polar, a class of magnetic cataclysmic variables, exhibiting an…

The NuSTAR Legacy program 'Unidentified INTEGRAL sources' targeted faint hard X-ray sources revealed by INTEGRAL in the Galactic plane in order to provide conclusive identification of their nature and insights on the population of faint…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Maïca Clavel , John A. Tomsick , Jeremy Hare , Roman Krivonos , Kaya Mori , Daniel Stern

IGR J18483-0311 is a supergiant fast X-ray transient whose compact object is located in a wide (18.5 d) and eccentric (e~0.4) orbit, which shows sporadic outbursts that reach X-ray luminosities of ~1e36 erg/s. We investigated the timing…

High Energy Astrophysical Phenomena · Physics 2015-06-17 L. Ducci , V. Doroshenko , M. Sasaki , A. Santangelo , P. Esposito , P. Romano , S. Vercellone

A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among these sources, two…

Astrophysics · Physics 2007-10-02 Sylvain Chaty

Analysis of INTEGRAL/IBIS survey observations has revealed that the rare intermediate polar and asynchronous polar cataclysmic variables are consistently found to emit in the 20-100 keV energy band, whereas synchronous polars and the common…

Astrophysics · Physics 2009-11-11 E. J. Barlow , C. Knigge , A. J. Bird , A. J. Dean , D. J. Clark , A. B. Hill , M. Molina , V. Sguera

We present detailed spectral and timing analysis of the hard x-ray transient IGR J16358-4726 using multi-satellite archival observations. A study of the source flux time history over 6 years, suggests that lower luminosity transient…

We present preliminary results of observations of X-ray pulsar SAX J2103.5+4545 with INTEGRAL observatory in Dec 2002. Maps of this sky region in energy bands 3-10, 15-40, 40-100 and 100-200 keV are presented. The source is significantly…

Astrophysics · Physics 2009-11-07 A. Lutovinov , S. Molkov , M. Revnivtsev

We have conducted low-frequency radio observations with the Giant Metrewave Radio Telescope (GMRT) of 40 new hard X-ray sources discovered by the INTEGRAL satellite. This survey was conducted in order, to study radio emissions from these…

Astrophysics · Physics 2009-11-11 M. Pandey , A. P. Rao , R. Manchanda , P. Durouchoux , C. H. Ishwara-Chandra

IGR J17503-2636 is a hard X-ray transient discovered by INTEGRAL on 2018 August 11. This was the first ever reported X-ray emission from this source. Following the discovery, follow-up observations were carried out with Swift, Chandra,…

High Energy Astrophysical Phenomena · Physics 2019-05-01 C. Ferrigno , E. Bozzo , A. Sanna , G. K. Jaisawal , J. M. Girard , T. Di Salvo , L. Burderi

Here we report the detection of a 626 s periodic modulation from the X-ray source 2XMM J174016.0-290337 located in the direction of the Galactic center. We present temporal and spectral analyses of archival XMM-Newton data and photometry of…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Sean A. Farrell , Andrew J. Gosling , Natalie A. Webb , Didier Barret , Simon R. Rosen , Masaaki Sakano , Benoit Pancrazi

Thanks to INTEGRAL's long exposures of the Galactic Plane, the two brightest Soft Gamma-Ray Repeaters, SGR 1806-20 and SGR 1900+14, have been monitored and studied in detail for the first time at hard-X/soft-gamma rays. SGR 1806-20, lying…

A new cataclysmic variable is identified as the optical counterpart of the faint and hard X-ray source RX J0757.0+6306 discovered during the ROSAT all-sky survey. Strong double-peaked emission lines bear evidence of an accretion disc via an…

We derive the spectra of the cosmic X-ray background (CXB) and of the Galactic ridge X-ray emission (GRXE) in the ~20-200 keV range from the data of the IBIS instrument aboard the INTEGRAL satellite obtained during the four dedicated…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 M. Turler , M. Chernyakova , T. J. -L. Courvoisier , P. Lubinski , A. Neronov , N. Produit , R. Walter