Fig. 15
ASCA power spectrum of IGR J18410-0535 obtained by using events in the 1.9–4.9 keV energy range and a time resolution of 0.5 s. The arrow marks the apparent detection of pulsations at 0.211 Hz. As we discuss in the text, this excess in the power-spectrum is not statistically significant if the correct number of trials is taken into account (see Sect. 3.1).
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