Clover would have been an experiment to measure the polarization of the Cosmic Microwave Background. It was approved for funding in late 2004, with the aim of having the full telescope operational by 2009. The project was jointly run by Cardiff University, Oxford University, the Cavendish Astrophysics Group and the University of Manchester.
History
The Clover Project was meant to consist of two independent telescopes, one operating at 95 GHz with the other operating at both 150 and 225 GHz. Both telescopes were to be sited near the CBI site in the Atacama Desert, Chile. The two telescope receivers would have been large format focal plane arrays of either 100 or 200 bolometric detectors.
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