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Related papers: The first X-ray eclipse of IGRJ16479-4514?

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The starburst galaxy M82 contains two ultraluminous X-ray sources (ULXs), CXOM82 J095550.2+694047 (=X41.4+60) and CXOM82 J095551.1+694045 (=X42.3+59), which are unresolved by XMM-Newton. We revisited the two XMM-Newton observations of M82…

Astrophysics · Physics 2010-05-25 Hua Feng , Philip Kaaret

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO La Silla) in the course of a Target of…

Astrophysics · Physics 2007-05-23 Sylvain Chaty , Philippe Filliatre

This paper reports the discovery of a bright X-ray transient source, Suzaku J1305-4913, in the south-west arm of the nearby Seyfert II galaxy NGC 4945. It was detected at a 0.5 -- 10 keV flux of $2.2 \times 10^{-12}$ erg cm$^{-2}$ s$^{-1}$…

We report the result of an XMM-Newton observation of the black-hole X-ray transient XTE J1650-500 in quiescence. The source was not detected and we set upper limits on the 0.5-10 keV luminosity of 0.9e31-1.0e31 erg/s (for a newly derived…

After almost 2.5 years of actively accreting, the neutron star X-ray transient and eclipsing binary MXB 1659-29 returned to quiescence in 2001 September. We report on a Chandra observation of this source taken a little over a month after…

We present the results from analyses of Suzaku observations of the supergiant X-ray binaries IGR J16207-5129 and IGR J17391-3021. For IGR J16207-5129, we provide the first broadband (0.5--60 keV) spectrum from which we confirm a large…

High Energy Astrophysical Phenomena · Physics 2010-12-16 A. Bodaghee , J. A. Tomsick , J. Rodriguez , S. Chaty , K. Pottschmidt , R. Walter , P. Romano

We present the results of our optical identification of the X-ray source IGR J16547-1916 detected by the INTEGRAL observatory during a deep all-sky survey. Analysis of the spectroscopic data from the SWIFT and INTEGRAL observatories in the…

High Energy Astrophysical Phenomena · Physics 2015-05-20 A. Lutovinov , R. Burenin , M. Revnivtsev , V. Suleimanov , A. Tkachenko

We report on X-ray and optical observations of the X-ray burster EXO 1747-214. This source is an X-ray transient, and its only known outburst was observed in 1984-1985 by the EXOSAT satellite. We re-analyzed the EXOSAT data to derive the…

Astrophysics · Physics 2009-11-13 John A. Tomsick , Dawn M. Gelino , Philip Kaaret

We present the results obtained from a comprehensive timing and spectral study of two high-mass X-ray binary sources using NuSTAR observations. These two sources, IGR J16320-4751 and IGR J16479-4514, were discovered by INTEGRAL and have…

High Energy Astrophysical Phenomena · Physics 2023-06-05 Varun , Gayathri Raman

IGR J17361-4441 was discovered by INTEGRAL undergoing its first detectable X-ray outburst in 2011 and initially classified as an accreting X-ray binary in the globular cluster NGC 6388. A reanalysis of the outburst data collected with…

High Energy Astrophysical Phenomena · Physics 2014-10-15 E. Bozzo , A. Papitto , C. Ferrigno , T. M. Belloni

We present the results of our study of the luminous (L_{X} ~ 10^{39} erg/s) X-ray binary CXOU J121538.2+361921 in NGC 4214, the high mass X-ray binary with the shortest known orbital period. Using Chandra data, we confirm the ~13,000 s (3.6…

High Energy Astrophysical Phenomena · Physics 2023-07-17 Zikun Lin , Roberto Soria , Douglas A. Swartz

During the analysis of the INTEGRAL observatory archival data we found a powerful X-ray burst, registered by JEM-X and IBIS/ISGRI telescopes on April 16, 2005 from a weak and poorly known source AX J1754.2-2754. Analysis of the burst…

Astrophysics · Physics 2008-11-26 I. V. Chelovekov , S. A. Grebenev

XMMSL1 J171900.4-353217 is a very-faint X-ray transient that was discovered in 2010 March when it exhibited an outburst. We report on 7 observations, obtained with the X-Ray Telescope (XRT) aboard the Neil Gehrels {\it{Swift}} Observatory…

High Energy Astrophysical Phenomena · Physics 2024-10-01 O. Ahmed , N. Degenaar , R. Wijnands , M. Armas Padilla

We report on a multi-wavelength study of the recently discovered X-ray transient XMMU J004243.6+412519 in M31, based on data collected with Swift and the 1.8-m Copernico Telescope at Cima Ekar in Asiago (Italy) between 2012 February and…

High Energy Astrophysical Phenomena · Physics 2013-01-17 P. Esposito , S. E. Motta , F. Pintore , L. Zampieri , L. Tomasella

We present observations of the X-ray transient XTEJ1755-324 performed during summer 1997 with the XTE satellite and with the SIGMA hard X-ray telescope onboard the GRANAT observatory. The source was first detected in soft X-rays with XTE on…

The orbital profile of the High Mass X-ray binary IGR J16393-4643 shows a dip in its X-ray intensity, which was previously interpreted as an eclipse. Unlike most eclipsing HMXBs, where the X-ray eclipses are about two orders of magnitude…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Sanhita Kabiraj , Nazma Islam , Biswajit Paul

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

We report here on the longest deep X-ray observation of a SFXT outside outburst, with an average luminosity level of 1E33 erg/s (assuming 3 kpc distance). This observation was performed with Suzaku in December 2009 and was targeted on…

High Energy Astrophysical Phenomena · Physics 2015-05-19 L. Sidoli , P. Esposito , L. Ducci

We present results from a ~55 ks long XMM-Newton observation of the obscured AGN, NGC 5643, performed in July 2009. A previous, shorter (about 10 ks) XMM-Newton observation in February 2003 had left two major issues open, the nature of the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 G. Matt , S. Bianchi , A. Marinucci , M. Guainazzi , K. Iwawasa , E. Jimenez Bailon

We report the discovery of a transient jet in the supersoft X-ray source RX J0925-4758 . The jet was observed in the Halpha line during a single night in June 1997 and had disappeared one day later. RX J0925-4758 is the third supersoft…

Astrophysics · Physics 2016-08-30 C. Motch