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G.E. Allen (MIT CSR), A. Decourchelle (CEA Saclay)
We present an analysis of RXTE timing data of the Kepler supernova remnant. Power density spectral results will be presented for a broad energy range and separately for low, medium, and high-energy X-ray bands. The pulsed-flux limits will be presented. This work is supported in part by contract SAO SV1-61010.
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