A Re-analysis of Timing Parameters of SGR 1833-0832

Details A Re-analysis of Timing Parameters of SGR 1833-0832 A Re-analysis of Timing Parameters of SGR 1833-0832

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2763....1b&link_type=abstract

The Astronomer's Telegram, #2763

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Pulsars, Soft Gamma-Ray Repeaters

Scientific paper

SGR 1833-0832 is discovered on 2010 March 19 (MJD 55274; GCN #10526) by Swift/BAT and monitored with XMM-Newton, Swift, and RossiXTE. About 90 days after the Swift/BAT event, Esposito et al., 2010, (ATEL #2691) reported the calculation of a second pulse frequency derivative component with respect to the phase-coherent timing solutions previously reported, which included only the period and its first time derivative (ATEL #2550, #2553; Gogus et al.

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