Photometric identification of the periods of the first candidate extragalactic magnetic massive stars

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Fig. 6

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Photometric changes of 2dFS 936, once the 1370 d variation is removed. This plot uses the T₀ of Table 2 and a period of 0.402 d (i.e. a frequency of 2.48952 d^-1). The symbols for data are as in Fig. 1.

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