The Submillimeter Array (SMA) allows us to observe submillimeter emission from warm, dense gas and dust at unprecedented high resolutions of up to 0.1 arcsecond.
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Taiwan-American Occultation Survey (TAOS) monitors some 1000 stars per night to search for the occultation of background stars by Solar system bodies located in the Kuiper Belt.
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The Y.T. Lee Array for Microwave Background Anisotropy (AMiBA) was dedicated on Mauna Loa in Hawaii during October 2006. It is the first instrument in Asia dedicated to the study of cosmology.
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The WIRCam on the Canada-France-Hawaii Telescope (CFHT) makes possible large-scale near-infrared imaging surveys to revolutionize the science of star formation, galactic structure and evolution, and the large scale structure in the Universe.
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The Theoretical Institute for Advanced Research in Astrophysics (TIARA) was established in 2004 to provide an integrated program of research and education in theoretical astrophysics.
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The Atacama Large Millimeter/submillimeter Array (ALMA) is the largest ground based astronomical telescope to be built, which will be the preeminent instrument for studies of the relic radiation from the early Universe and of the formation and evolution of stars, planetary systems, galaxies and even the origin of life itself. > Learn more

Since 2008 ASIAA has contributed to the wide field visible camera Hyper SuprimeCam (HSC) for Subaru telescope. The main scientific goal of the HSC will be the study of weak gravitational lensing over large areas of the sky so as to unveil the properties of dark matter and dark energy.
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By connecting SMA and ALMA with the Greenland Telescope forming a triangle, ASIAA VLBI project will render the imaging of the event horizon of a supermassive black hole.
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CompAS is a joint research project of ASIAA, the Institute of Mathematics (ASIM) of the Academia Sinica, and the Department of Mathematics of the National Taiwan University. Its main goal is to develop high-performance codes of computational fluid dynamics and magnetohydrodynamics (CFD-MHD) for astrophysical problems. > Learn more