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We analyze the observations of the X-ray pulsar KS 1947+300 performed by theINTEGRAL and RXTE observatories over a wide (3-100 keV) X-ray energy range. Theshape of the pulse profile was found to depend on the luminosity of the source.Based on the model of a magnetized neutron star, we study the characteristicsof the pulsar using the change in its spin-up rate. We estimated the magneticfield strength of the pulsar and the distance to the binary.Comment: 21 pages, 9 figures, Astronomy Letters, 31, 88-97 (2005

Observations of the transient X-ray pulsar KS 1947+300 by the INTEGRAL and RXTE observatories