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The JWST/NIRCam and NIRSpec instruments (and other on-going missions) are expected to yield repeatable and stable lightcurves, but no absolute calibration. To make the data usable for standard analysis techniques requires the use of an accurate absolute calibration of the infrared radiation. This involves a combination of the following steps: (1) Transfer the Spitzer absolute flux calibration to the closest star in the dynamic range of the JWST cameras, (2) Establish an absolute calibration from the Spitzer-calibrated star directly to the Sun, and (3) Optimize the infrared flux method for JWST.

Sensitivity and other attributes of the microwave system used for the selection of pulse compression technique in radar systems are discussed. The objectives of this project were (i) to develop the pulse compression technique and (ii) to evaluate the performance of the new developed technique in comparison with the existing technique. The new technique is a combination of second order difference-order (DO2) and second order different-integral (DOI2) technique. The pulse compression system developed in this work is based on the second order difference-order technique, which is a modification of the existing technique. The second order different-integral technique is used as the pre-processor to enhance the signal-to-noise ratio (SNR) of the input signal and to separate the real part from the imaginary part of the signal. The pulse compression system can be classified into the following two categories: (1) strong signal compression, which requires the use of real time signal processing system; (2) weak signal compression, which requires off-line signal processing.

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