A systematic Z1^2 and maximum-likelihood search of RXTE data finds dozens of intermittent pulse candidates in three accreting millisecond pulsars and derives an 8.76 h orbital period for SAX J1748.9-2021.
20 Search for pulsed γ-ray emission from radio pulsars in the COS-B data
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An Elaborate Search for Coherent Pulsations from Intermittent-AMXPs
A systematic Z1^2 and maximum-likelihood search of RXTE data finds dozens of intermittent pulse candidates in three accreting millisecond pulsars and derives an 8.76 h orbital period for SAX J1748.9-2021.