Swift/XMM-Newton refined timing solution for SGR0501+4516

Details Swift/XMM-Newton refined timing solution for SGR0501+4516 Swift/XMM-Newton refined timing solution for SGR0501+4516

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1692....1i&link_type=abstract

The Astronomer's Telegram, #1692

Astronomy and Astrophysics

Astronomy

4

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

Scientific paper

The Swift satellite observed SGR 0501+4516 several times during the last two weeks (ATEL #1676, #1677, #1678, #1682, #1683), and XMM-Newton observed the source on August 23rd (ATEL #1688). By merging the two datasets we were able to obtain a phase-coherent timing solution. According to our analysis the preliminary period and period derivative of SGR 0501+4516 are: P = 5.7620699(4) s and Pdot = 5(1) x 10-12 s/s (1 sigma uncertainties).

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