Swift phase-coherent P-Pdot solution for the 1E1547.0-5408 outburst

Details Swift phase-coherent P-Pdot solution for the 1E1547.0-5408 outburst Swift phase-coherent P-Pdot solution for the 1E1547.0-5408 outburst

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1770....1i&link_type=abstract

The Astronomer's Telegram, #1770

Astronomy and Astrophysics

Astronomy

4

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

Scientific paper

Swift XRT monitored 1E1547.0-5408 in the latest 5 days starting from about 90 seconds since the BAT trigger (Krimm et al. GCN 8311, 8312). During this period observations in the WT mode were carried out for a total exposure time of about 37ks. After having removed bursts and corrected the photon arrival times to the barycenter of the Solar System, the dataset was used to infer a phase-coherent timing solution including both a period and period derivative component.

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