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The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is thefirst interferometer dedicated to studying the cosmic microwave background(CMB) radiation at 3mm wavelength. The choice of 3mm was made to minimize thecontributions from foreground synchrotron radiation and Galactic dust emission.The initial configuration of seven 0.6m telescopes mounted on a 6-m hexapodplatform was dedicated in October 2006 on Mauna Loa, Hawaii. Scientificoperations began with the detection of a number of clusters of galaxies via thethermal Sunyaev-Zel'dovich effect. We compare our data with Subaru weak lensingdata in order to study the structure of dark matter. We also compare our datawith X-ray data in order to derive the Hubble constant.