A New Period Analysis of OGLE-III Data for SXP967

Details A New Period Analysis of OGLE-III Data for SXP967 A New Period Analysis of OGLE-III Data for SXP967

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1953....1s&link_type=abstract

The Astronomer's Telegram, #1953

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

We have analyzed 8 seasons of OGLE-III data for SXP967 (formerly SXP700; see discussion of the revised pulsar period by Haberl et al., 2008, A&A 489, 327). The I-band observations show long-term changes of 0.6 mag, which were removed via polynomial fitting to long segments of data (1-3 seasons in length). The remaining small-amplitude variations were analyzed using both periodogram and PDM techniques.

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