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We report on the results of a four-year long X-ray monitoring campaign of the central 1.2 square degrees of our Galaxy, performed with Chandra and XMM-Newton between 2005 and 2008. Our study focuses on the properties of transient X-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-04 N. Degenaar , R. Wijnands , E. M. Cackett , J. Homan , J. J. M. in 't Zand , E. Kuulkers , T. J. Maccarone , M. van der Klis

We present the first detection of pulsations from a neutron star in the submillimeter range. The source is the magnetar XTE J1810-197, observed with the James Clerk Maxwell Telescope (JCMT) on 2020 February 27, 2020 July 9 and 2021 May 15.…

We present the results of our search for optical counterparts to high-mass X-ray transient sources discovered by various X-ray missions. We obtained CCD images of the X-ray fields through BVR and Halpha filters in order to identify…

Astrophysics · Physics 2009-11-11 P. Reig , I. Negueruela , G. Papamastorakis , A. Manousakis , T. Kougentakis

Galactic transients, X-ray and gamma-ray binaries provide a proper environment for particle acceleration. This leads to the production of gamma rays with energies reaching the GeV-TeV regime. MAGIC has carried out deep observations of…

High Energy Astrophysical Phenomena · Physics 2019-08-14 A. Fernández-Barral , O. Blanch , E. de Oña Wilhelmi , D. F. Torres , C. Fruck , D. Hadasch , A. López-Oramas , P. Munar-Adrover , R. Zanin

The nature of very faint X-ray transients (VFXTs) - transient X-ray sources that peak at luminosities $L_X\lesssim10^{36} {\rm erg s^{-1}}$ - is poorly understood. The faint and often short-lived outbursts make characterising VFXTs and…

We report the discovery with BeppoSAX of a new 170.84 +/- 0.04 s X-ray pulsar, 1SAX J1324.4-6200, found serendipitously in the field of the X-ray binary X1323-619 in 1997 August. The source and periodicity are also detected in archival ASCA…

Astrophysics · Physics 2007-05-23 L. Angelini , M. J. Church , A. N. Parmar , M. Balucinska-Church , T. Mineo

The new transient X-ray pulsar XTE J0111.2-7317 was observed with Advanced Satellite for Cosmology and Astrophysics (ASCA) on 1998 November 18, a few days after its discovery with the Proportional Counter Array onboard the Rossi X-ray…

We have observed the radio-quiet X-ray pulsar 1E 1207.4-5209 with the high throughput EPIC cameras onboard XMM-Newton. The spectrum of this peculiar source is characterized by two broad absorption features which present significant…

Astrophysics · Physics 2007-05-23 A. De Luca , S. Mereghetti , P. A. Caraveo , R. P. Mignani , W. Becker , G. F. Bignami

We report on the discovery and analysis of the transient X-ray pulsar CXO/XMMU J073709.13+653544 detected in the 2004 August-October Chandra and XMM observations of the nearby spiral galaxy NGC2403. The source exhibits X-ray pulsations with…

Astrophysics · Physics 2008-11-26 Sergey Trudolyubov , William Priedhorsky , France Cordova

On 28 February 2007 a new outburst of the previously known transient source XTE J1856+053 was detected with RXTE/ASM. We present here the results of an XMM-Newton (0.5-10.0 keV) Target of Opportunity observation performed on 14 March 2007,…

Astrophysics · Physics 2011-08-31 G. Sala , J. Greiner , M. Ajello , N. Primak

One of the goals of the XMM-Newton survey of the Small Magellanic Cloud is the study of the Be/X-ray binary population. During one of our first survey observations a bright new transient - XMMUJ004814.0-732204 - was discovered. We present…

We present a study of the correlated spectral and timing behavior of the new X-ray transient SAX J1711.6-3808 during its 2001 outburst using data obtained with the RXTE. We also investigate the correlations between those source properties…

Astrophysics · Physics 2009-11-06 Rudy Wijnands , Jon M. Miller

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

We report the detection of a new radio transient source, GCRT J1746-2757, located only 1.1 degrees north of the Galactic center. Consistent with other radio transients toward the Galactic center, this source brightened and faded on a time…

Astrophysics · Physics 2009-11-07 Scott D. Hyman , T. Joseph W. Lazio , Namir E. Kassim

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at only 2.9" from SgrA*. We report the discovery of sharp and…

Astrophysics · Physics 2009-11-11 D. Porquet , N. Grosso , G. Belanger , A. Goldwurm , F. Yusef-Zadeh , R. S. Warwick , P. Predehl

In this paper we report on a long multi-wavelength observational campaign of the supergiant fast X-ray transient prototype IGR J17544-2619. A 150 ks-long observation was carried out simultaneously with XMM-Newton and NuSTAR, catching the…

High Energy Astrophysical Phenomena · Physics 2016-12-07 E. Bozzo , V. Bhalerao , P. Pradhan , J. Tomsick , P. Romano , C. Ferrigno , S. Chaty , L. Oskinova , A. Manousakis , R. Walter , M. Falanga , S. Campana , L. Stella , M. Ramolla , R. Chini

The neutron-star X-ray transient XTE J1701-462 was observed for $\sim$3 Ms with \xte during its 2006-2007 outburst. Here we report on the discovery of three type-I X-ray bursts from XTE J1701-462. They occurred as the source was in…

High Energy Astrophysical Phenomena · Physics 2009-06-25 Dacheng Lin , Diego Altamirano , Jeroen Homan , Ronald A. Remillard , Rudy Wijnands , Tomaso Belloni

We report here on the XMM-Newton observations of the three supergiant fast X-ray transients (SFXT) XTE J1739-302, IGRJ08408-4503, and IGRJ18410-0535. For the latter source we only discuss some preliminary results of our data analysis. Some…

High Energy Astrophysical Phenomena · Physics 2011-07-04 E. Bozzo , C. Ferrigno , J. C. Leyder , L. Stella , G. Israel , A. Giunta , M. Falanga , S. Campana

We report on BeppoSAX observations of the X-ray transient XTE J0421+560 in quiescence 156, 541, and ~690 days after the maximum of the 1998 April outburst. In the first observation the source was soft with a power-law photon index of 4.0…

Astrophysics · Physics 2007-05-23 A. N. Parmar , T. Belloni , M. Orlandini , D. Dal Fiume , A. Orr , N. Masetti

We present a timing and spectral analysis of the X-ray pulsar XTE J1946+274 observed with Suzaku during an outburst decline in 2010 October and compare with previous results. XTE J1946+274 is a transient X-ray binary consisting of a Be-type…