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Optical and X‐ray observations are presented here of a newly reported X‐ray transient system in the Small Magellanic Cloud. The data reveal many previously unknown X‐ray detections of this system and clear evidence for a 45.99 d binary period. In addition, the optical photometry shows recurring outburst features at the binary period which may be well indicative of the neutron star interacting with a circumstellar disc around a Be star.

An optical and X‐ray study of the counterpart to the Small Magellanic Cloud X‐ray binary pulsar system SXP327