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Related papers: Serpens X-1 observed by INTEGRAL

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We here report results of an INTEGRAL observation of the X-ray burst and atoll source Ser X-1 performed on May 2003. The object was observed for a total of 400 ks but nearly 8 degrees off-axis due to the amalgamation with an observation of…

Astrophysics · Physics 2007-05-23 N. Masetti , L. Foschini , E. Palazzi , L. Amati , E. Caroli , G. Di Cocco , F. Frontera , M. Orlandini

We present simultaneous X-ray polarimetric and spectral observations of the bright atoll source Ser~X-1 carried out with the Imaging X-ray Polarimetry Explorer (IXPE), NICER, and NuSTAR. We obtain an upper limit of 2% (99% confidence level)…

High Energy Astrophysical Phenomena · Physics 2024-08-30 F. Ursini , A. Gnarini , S. Bianchi , A. Bobrikova , F. Capitanio , M. Cocchi , S. Fabiani , R. Farinelli , P. Kaaret , G. Matt , M. Ng , J. Poutanen , S. Ravi , A. Tarana

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…

Astrophysics · Physics 2016-08-30 S. Molkov , A. Lutovinov , S. Grebenev

During a serendipitous observation of the BeppoSAX Wide Field Cameras, a very long Type I X-ray burst was observed from the low mass X-ray binary Serpens X-1. The burst lasted for approximately 4 hours and had an exponential decay time of…

Astrophysics · Physics 2009-11-07 R. Cornelisse , E. Kuulkers , J. J. M. in 't Zand , F. Verbunt , J. Heise

We present \nustar{} observation of the atoll type neutron star (NS) low-mass X-ray binary (LMXB) Serpens~X-1 (Ser~X-1) performed on 17 February 2018. We observed Ser~X-1 in a soft X-ray spectral state with 3-79 keV luminosity of…

High Energy Astrophysical Phenomena · Physics 2020-05-06 Aditya S. Mondal , Gulab C. Dewangan , B. Raychaudhuri

The Galactic bulge region is a rich host of variable high-energy point sources. Since 2005, February 17 we are monitoring the source activity in this region about every three days with INTEGRAL. Thanks to the large field of view, the…

We study three extraordinarily bright X-ray flares originating from Cyg X-1 seen on 2023 July 10 detected with INTEGRAL. The flares had a duration on the order of only ten minutes each, and within seconds reached a 1-100 keV peak luminosity…

We study the 4-200 keV spectral and temporal behaviour of the low mass X-ray binary 4U 1820-30 with INTEGRAL during 2003-2005. This source as been observed in both the soft (banana) and hard (island) spectral states. A high energy tail,…

Astrophysics · Physics 2008-11-26 Antonella Tarana , Angela Bazzano , Pietro Ubertini , Andrzej A. Zdziarski

In Spring 2005, the blazar 3C454.3 underwent a dramatic outburst at all wavelengths from mm to X-rays. This prompted INTEGRAL observations, accomplished in 15-18 May 2005. The source was detected by the INTEGRAL instruments from 3 to 200…

Astrophysics · Physics 2009-11-11 Elena Pian , Luigi Foschini , Volker Beckmann

Context: The transient hard X-ray source IGR J11321-5311 was discovered by INTEGRAL on June 2005, during observations of the Crux spiral arm. To date, this is the only detection of the source to be reported by any X/gamma-ray mission. Aims:…

Astrophysics · Physics 2009-11-13 V. Sguera , A. Bazzano , A. J. Bird , A. B. Hill , A. J. Dean , L. Bassani , A. Malizia , P. Ubertini

The INTEGRAL satellite extensively observed the black hole binary Cygnus X-1 from 2002 November to 2004 November during calibration, open time and core program (Galactic Plane Scan) observations. These data provide evidence for significant…

We report on Cyg X-1 observations performed by the SPI telescope onboard the INTEGRAL mission and distributed over more than 6 years. We investigate the variability of the intensity and spectral shape of this peculiar source in the hard…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Elisabeth Jourdain , Jean-Pierre Roques , Julien Malzac

We present the results of our study of the emission from the transient burster MX 0836-42 using its observations by the INTEGRAL and RXTE X-ray and gamma-ray observatories in the period 2003-2004. The source's broadband X-ray spectrum in…

Astrophysics · Physics 2009-11-13 I. V. Chelovekov , A. A. Lutovinov , S. A. Grebenev , R. A. Sunyaev

All of the observations performed with the IBIS telescope onboard the INTEGRAL observatory during the first one and a half years of its in-orbit operation (from February 10, 2003, through July 2, 2004) have been analyzed to find X-ray…

Astrophysics · Physics 2009-11-11 I. V. Chelovekov , S. A. Grebenev , R. A. Sunyaev

We present for the first time a study of the 3-200 keV broad band spectra of the bursting atoll source 4U 1728-34 (GX 354-0) along its hardness intensity diagram. The analysis was done using the INTEGRAL public and Galactic Center deep…

Astrophysics · Physics 2009-11-11 M. Falanga , D. Gotz , P. Goldoni , R. Farinelli , A. Goldwurm , S. Mereghetti , A. Bazzano , L. Stella

In 2005 March 22nd, the INTEGRAL satellite caught a type-I X-ray burst from the unidentified source XMMU J174716.1-281048, serendipitously discovered with XMM-Newton in 2003. Based on the type-I X-ray burst properties, we derived the…

Astrophysics · Physics 2009-06-23 M. Del Santo , L. Sidoli , P. Romano , A. Bazzano , A. Tarana , P. Ubertini , M. Federici , S. Mereghetti

We present results of a comprehensive analysis of the X-ray pulsar X Persei over the period 1996 to 2011, encompassing the quite low state and subsequent strong outburst activity. Using data from the RXTE and Swift observatories we detected…

High Energy Astrophysical Phenomena · Physics 2015-06-04 A. Lutovinov , S. Tsygankov , M. Chernyakova

We report results of the INTEGRAL Target of Opportunity observations of the transient X-ray burster XTE J1810-189. The observations were performed on April 3--6, 2008, soon after the discovery of the source and near the peak of its…

High Energy Astrophysical Phenomena · Physics 2010-04-26 I. Chelovekov , S. Grebenev

We present the results of an analysis of the quiescent X-ray emission from the Soft Gamma-Ray Repeater SGR1806-20, taken during an INTEGRAL ultra-deep survey of the Galactic Center region in autumn 2003. The total effective exposure time…

Astrophysics · Physics 2009-11-10 S. Molkov , K. Hurley , R. Sunyaev , P. Shtykovsky , M. Revnivtsev

We report on our discovery and follow-up observations of the X-ray source SAX J1747.0-2853 detected in outburst on 1998, March 10 with the BeppoSAX Wide Field Cameras in the energy range 2-28 keV. The source is located about half degree off…

Astrophysics · Physics 2009-10-31 L. Natalucci , A. Bazzano , M. Cocchi , P. Ubertini , J. Heise , E. Kuulkers , J. J. M. in 't Zand
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