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The only fact given is the antenna diameter which results in 40 meters, much less than Arecibo, and obviously this means a smaller resolving power. Other important parameters are the frequency searched, the bandwidth around it and the coordinates of the possible sources. These can be varied more easily from an array such as Allen or ALMA. All these parameters are described in an article on Serendip on the Arecibo Observatory home page and also given in the SETI home page. I would say that, all limitations withstanding, Arecibo is still a more powerful observing tool.
Tullio
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