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First superburst from a classical low-mass X-ray binary transient
L. Keek, J. J. M. in 't Zand, E. Kuulkers +3
We report the analysis of the first superburst from a transiently accreting neutron star system with the All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer. The superburst oc…
Discovery of the Spin Frequency of 4U 0614+09 with SWIFT/BAT
Tod Strohmayer, Craig Markwardt, Erik Kuulkers
We report the discovery of burst oscillations at 414.7 Hz during a thermonuclear X-ray burst from the low mass X-ray binary (LMXB) 4U 0614+091 with the Burst Alert Telescope (BAT)…
Intermediate long X-ray bursts from the ultra-compact binary source SLX 1737-282
M. Falanga, J. Chenevez, A. Cumming +3
Aims: The low persistent X-ray burster source SLX 1737-282 is classified as an ultra-compact binary candidate. We compare the data on SLX 1737-282 with the other similar objects an…
The Burst Spectra of EXO 0748-676 during a Long 2003 XMM-Newton Observation
J. Cottam, F. Paerels, M. Méndez +4
Gravitationally redshifted absorption lines from highly ionized iron have been previously identified in the burst spectra of the neutron star in EXO 0748-676. To repeat this detect…
The high energy emission of GRO J1655-40 as revealed with INTEGRAL spectroscopy of the 2005 outburst
M. D. Caballero-Garcia, J. M. Miller, E. Kuulkers +10
We present broadband (3-500 keV) INTEGRAL X-ray spectra and X-ray/optical light curves of the luminous black hole X-ray transient and relativistic jet source GRO J1655-40. Our anal…
IGR J17254-3257, a new bursting neutron star
J. Chenevez, M. Falanga, E. Kuulkers +6
The study of the observational properties of uncommonly long bursts from low luminosity sources with extended decay times up to several tens of minutes is important when investigat…
A description of sources detected by INTEGRAL during the first 4 years of observations
A. Bodaghee, T. J. -L. Courvoisier, J. Rodriguez +6
Parameters from the literature, such as positions, photoelectric absorption (nH), spin and orbital periods, and distances or redshifts, were collected for all ~500 sources detected…