RXTE timing observations of SGR 0418+5729

Astronomy and Astrophysics – Astronomy

Scientific paper

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X-Ray, Neutron Stars, Soft Gamma-Ray Repeaters, Transients

Scientific paper

Data from (publicly available) monitoring observations with RXTE of SGR 0418+5729 covering a time span of about 2 months since its discovery on June 5, 2009 (ATEL #2077,GCN #9499) have been used to construct an accurate phase-coherent timing solution. Such an analysis requires the pulse profile to be stable during the monitoring period in order to obtain reliable pulse time-of-arrivals, TOAs.

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