Measuring the period of the delta Scuti variable U1425-01208594 in Cassiopeia

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The variability of U1425-01208594 was recently discovered by Schmidtobreick et al, who suggested that it is a member of the delta Scuti family of pulsating stars. Photometry conducted by the authors revealed a period of 0.06695(8) d and a peak-to-peak amplitude of 0.014 mag.
Accepted for publication in the Open European Journal on Variable Stars. 4 pages, 4 figures

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