English
Related papers

Related papers: IGR J19140+098, a new INTEGRAL transient

200 papers

IGR J19140+098 was discovered during the early INTEGRAL observations of GRS1915+105 in March 2003. The following observations by INTEGRAL and RXTE show significant variability on various time scales from 100s to 1ks, but no pulsations. The…

Astrophysics · Physics 2007-05-23 C. Cabanac , J. Rodriguez , P. O Petrucci , G. Henri , D. Hannikainen , P. Durouchoux

IGR J19140+0951 (formerly known as IGR J19140+098) was discovered with the INTEGRAL satellite in March 2003. We report the details of the discovery, using an improved position for the analysis. We have performed a simultaneous study of the…

Astrophysics · Physics 2009-11-10 D. C. Hannikainen , J. Rodriguez , C. Cabanac , J. Schultz , N. Lund , O. Vilhu , P. O. Petrucci , G. Henri

The INTEGRAL observatory has been (re-)discovering new X-ray sources since the beginning of nominal operations in early 2003. These sources include X-ray binaries, Active Galactic Nuclei, cataclysmic variables, etc. Amongst the X-ray…

Astrophysics · Physics 2009-11-13 D. C. Hannikainen , M. G. Rawlings , P. Muhli , O. Vilhu , J. Schultz , J. Rodriguez

We present data from the first of six monitoring Open Time observations of GRS 1915+105 undertaken with the orbiting INTEGRAL satellite. The source was clearly detected with all three X-ray and gamma-ray instruments on board. GRS 1915+105…

We report the discovery of a high-energy transient with the IBIS/ISGRI detector on board the INTEGRAL observatory. The source, namely IGR J00291+5934, was first detected on 2nd December 2004 in the routine monitoring of the IBIS/ISGRI…

We present the transient nature of INTEGRAL source IGR J17285-2922, identified from a single period of activity during an IBIS/ISGRI Galactic Centre Deep Exposure in September 2003. The source has a maximum detection significance of 14…

INTEGRAL regularly scans the Galactic plane to search for new objects and in particular for absorbed sources with the bulk of their emission above 10-20 keV. The first new INTEGRAL source was discovered on 2003 January 29, 0.5 degree from…

One of the most recent discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. IGR J17544-2619, IGR J16465-4507 and XTE J1739-302 are among these sources.…

Astrophysics · Physics 2009-11-11 L. J. Pellizza , S. Chaty , I. Negueruela

The supergiant fast X-ray transient IGR J08408-4503 was discovered by INTEGRAL on May 15, 2006, during a bright flare. The source shows sporadic recurrent short bright flares, reaching a peak luminosity of 10^36 erg s^-1 within less than…

Astrophysics · Physics 2011-02-11 D. Gotz , M. Falanga , F. Senziani , A. De Luca , S. Schanne , A. von Kienlin

Details of the discovery of a new X-ray source, IGR J18462-0223, on October 12, 2007, during a short (several hours), intense (~ 35 mCrab at the peak) outburst of hard radiation by the IBIS/ISGRI gamma-ray telescope onboard the INTEGRAL…

High Energy Astrophysical Phenomena · Physics 2015-05-20 S. A. Grebenev , R. A. Sunyaev

We report the discovery with INTEGRAL on March 24, 2005, and follow-up observations of the distant Galactic X-ray nova IGR J17098-3628.

Astrophysics · Physics 2008-01-23 S. A. Grebenev , S. V. Molkov , M. G. Revnivtsev , R. A. Sunyaev

IGRJ19294+1816 was discovered by INTEGRAL in 2009 during a bright X-ray outburst and was classified as a possible Be X-ray binary or supergiant fast X-ray transient. On 2010 October 28, the source displayed a second X-ray outburst and a 2…

High Energy Astrophysical Phenomena · Physics 2015-05-28 E. Bozzo , C. Ferrigno , M. Falanga , R. Walter

The new transient IGR 16358-4726 was discovered on 2003 March 19 with INTEGRAL. We detected the source serendipitously during our 2003 March 24 observation of SGR 1627-41 with the Chandra X-ray Observatory at the 1.7 x 10^{-10} ergs s^{-1}…

The hard X-ray source IGRJ11215-5952 has been discovered with INTEGRAL during a short outburst in 2005 and proposed as a new member of the class of supergiant fast X-ray transients. We analysed INTEGRAL public observations of the source…

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

IGR J18179-1621 is a hard X-ray binary transient discovered recently by INTEGRAL. Here we report on detailed timing and spectral analysis on IGR J18179-1621 in X-rays based on available INTEGRAL and Swift data. From the INTEGRAL analysis,…

High Energy Astrophysical Phenomena · Physics 2017-04-26 J. Li , S. Zhang , D. F. Torres , A. Papitto , Y. P. Chen , J. M. Wang

IGR J18483-0311 is a high-mass X-ray binary recently discovered by INTEGRAL. Its periodic fast X-ray transient activity and its position in the Corbet diagram - although ambiguous - led to the conclusion that the source was a likely…

Astrophysics · Physics 2009-11-13 F. Rahoui , S. Chaty

Of the 21 new sources that INTEGRAL discovered up to Feb. 1, 2004, five were detected with the BeppoSAX Wide Field Cameras at earlier times. IGR J16320-4751 appears to be a persistently active X-ray source which hints at a supergiant…

Astrophysics · Physics 2007-05-23 Jean in 't Zand , John Heise , Pietro Ubertini , Angela Bazzano , Craig Markwardt

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…

IGR J17454-2919 is a hard X-ray transient discovered by INTEGRAL on 2014 September 27. We report on our 20ks Chandra observation of the source, performed about five weeks after the discovery, as well as on INTEGRAL and Swift monitoring…

High Energy Astrophysical Phenomena · Physics 2015-08-06 A. Paizis , M. A. Nowak , J. Rodriguez , A. Segreto , S. Chaty , A. Rau , J. Chenevez , M. Del Santo , J. Greiner , S. Schmidl

IGR J19140+0951 was discovered by INTEGRAL in 2003 in the 4-100 keV band. Observations with INTEGRAL and RXTE provide a tentative identification as a high-mass X-ray binary (HMXB) with a neutron star as accretor. However, an optical…

Astrophysics · Physics 2009-11-11 J. J. M. in 't Zand , P. G. Jonker , G. Nelemans , D. Steeghs , K. O'Brien
‹ Prev 1 2 3 10 Next ›