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   81210
   We propose to observe three SGRs (SGR0526-66, SGR1627-41, SGR1900+14),
   which are the strongest candidates of magnetars. We aim to detect
   pulsation from the former two targets to establish them as other
   samples of this category, and to derive luminosity - P-dot relation
   from the last one to clarify the mechanism of spin-down of magnetars.
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