1A 1118-61: detection of the pulsation period in Swift-XRT data

Details 1A 1118-61: detection of the pulsation period in Swift-XRT data 1A 1118-61: detection of the pulsation period in Swift-XRT data

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1896....1m&link_type=abstract

The Astronomer's Telegram, #1896

Astronomy and Astrophysics

Astronomy

9

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

The Be/X-ray transient 1A 1118-61 triggered Swift on 2009 January 4 at 03:52:35.6 UT (Mangano et al., GCN Circ. #8777) and at 13:37:39.6 UT. The source was monitored by XRT for 4 days, and a total exposure of 26 ks of data were collected (17 ks in Windowed Timing mode and 9 ks in Photon Counting mode). The light curve is highly variable. We performed a temporal analysis with epoch folding search techniques around the expected pulsation period of 405 s.

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