The spin-down rate of Swift J1822.3-1606 finally measured: confirmation as magnetar

Details The spin-down rate of Swift J1822.3-1606 finally measured: confirmation as magnetar The spin-down rate of Swift J1822.3-1606 finally measured: confirmation as magnetar

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3665....1k&link_type=abstract

The Astronomer's Telegram, #3665

Statistics

X-Ray, Neutron Star, Soft Gamma-Ray Repeater, Transient, Pulsar

Scientific paper

Data from monitoring observations of magnetar-candidate Swift J1822.3-1606 with RXTE PCA covering a time span of about 10 weeks (MJD 55758-55826) since its discovery on July 14, 2011 (ATEL #3488; GCN #12159) have been used to construct an accurate phase-coherent timing solution. Barycentered pulse arrival times (ToA's; see ATEL #3493 for the adopted source location) have been obtained by a cross-correlation method with a high-statistics pulse-profile template.

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