The supergiant fast X-ray transient IGRJ18483-0311 in quiescence: XMM-Newton, Swift and Chandra observations
Campana, S.; Israel, G.; Stella, L.; Bernardini, F.; Bozzo, E.; Bazzano, A.; Dean, A. J.; Mendez, M.; Falanga, M.; Giunta, A.
Italy, Switzerland, United Kingdom, Netherlands
Abstract
IGRJ18483-0311 was discovered with INTEGRAL in 2003 and later classified as a supergiant fast X-ray transient. It was observed in outburst many times, but its quiescent state is still poorly known. Here, we present the results of XMM-Newton, Swift and Chandra observations of IGRJ18483-0311. These data improved the X-ray position of the source, and provided new information on the timing and spectral properties of IGRJ18483-0311 in quiescence. We report the detection of pulsations in the quiescent X-ray emission of this source, and give for the first time a measurement of the spin-period derivative of this source. In IGRJ18483-0311, the measured spin-period derivative of -(1.3 +/- 0.3) × 10-9s s-1 likely results from light travel time effects in the binary. We compare the most recent observational results of IGRJ18483-0311 and SAXJ1818.6-1703, the two supergiant fast X-ray transients for which a similar orbital period has been measured.