Calibration of the Rossi X-ray Timing Explorer Proportional Counter Array
K. Jahoda, C. B. Markwardt, Y. Radeva, A. Rots, M. J. Stark, J. H. Swank, T. E. Strohmayer, W. Zhang
Abstract
We present the calibration and background model for the Proportional Counter Array (PCA) aboard the Rossi X-ray Timing Explorer (RXTE). The energy calibration is systematics limited below 10 keV with deviations from a power-law fit to the Crab nebula plus pulsar less than 1%. Unmodelled variations in the instrument background amount to less than 2% of the observed background below 10 keV and less than 1% between 10 and 20 keV. Individual photon arrival times are accurate to 4.4 micro-seconds at all times during the mission and to 2.5 micro-seconds after 29 April 1997. The peak pointing direction of the five collimators is known to a precision of a few arc-seconds
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