Time Delay Observations of the Gravitational Lens CLASS 1600+434 at 8 GHz

Mathematics – Logic

Scientific paper

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Scientific paper

Measurement of time delays in gravitational lens systems combined with an independent measure of the lens strength and a model of the lensing potential provide a method for determining the angular diameter distance to the lens. Measurements in many lensing systems will allow the extraction of cosmological parameters from the resulting angular diameter distance-redshift relation. We report on the results of a 45 epoch time delay observation of the gravitational lens CLASS 1600+434 performed using the VLA at 8 GHz over the period 10 Oct 1996 -- 23 May 1997.

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