Abstract
Theoretical satellite profiles have been calculated by means of the modified quasi-static approximation. Comparison with the experimental results shows that the shape of the theoretical satellite band depends on precise knowledge of the interatomic potential curves. A simple quadratic approximation of the 0g-(2P32/+2P32/+2S12/) potential curve near the extremum was also tested in the case of the caesium 8565 AA satellite band.

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