Swift observation of the AXP 1E 1048.1-5937 following a glitch

Details Swift observation of the AXP 1E 1048.1-5937 following a glitch Swift observation of the AXP 1E 1048.1-5937 following a glitch

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1043....1c&link_type=abstract

The Astronomer's Telegram, #1043

Astronomy and Astrophysics

Astronomy

9

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

Scientific paper

Following the discovery of a sudden spin-up and pulsed flux increase in the 6.5-s anomalous X-ray pulsar (AXP) 1E 1048.1-5937 (Dib et al. 2007, ATel #1041), Swift observed the source on April 3 2007, UT16:01:21. The first set of data in Photon Counting mode amounts to 2409 s. The source is well detected at a count rate of 0.88+/-0.02 c/s. This is mildly piled-up so that in the following analysis we excluded the central part of the point spread function (2 pixels).

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