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  • SMA

    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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  • CompAS

    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

  • YTLA

    The Y.T. Lee Array (YTLA, formerly 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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  • CFHT

    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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  • TIARA

    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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  • ALMA

    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

  • CHARMS

    CHARMS is the acronym for "Coordinated Hydrodynamic and Astrophysical Research, Modeling, and Synthesis", an ASIAA/TIARA initiative that focuses on bridging the theory and numerical astrophysics with cutting­-edge observational astrophysics. > Learn more

  • Subaru

    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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  • GLT/VLBI

    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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  • TAOS

    Transneptunian Automated Occultation Survey, will measure the size distribution of small objects (~1 km diameter) in the Kuiper Belt and beyond.
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What's New rss feed

Upcoming Event
2017-11-28The 19th East Asia Sub-millimeter-wave Receiver Technology Workshop
2017-12-07Future Exploration of Star and Planet Formation with Subaru
2018-02-06ALMA NA-Taiwan Workshop - Magnetic Fields or Turbulence: Which is the critical factor for the formation of stars and planetary disks?
Special Seminarabstract and yearly list 14:20~15:20 [R1203]
Forming stellar siblings: a look at the chemistry and physics of multiple stars Nadia M. Murillo (Leiden Observatory)
Lunch Talkabstract and yearly list 12:00~13:00 [R1203]
Indications of IMF variations based on the occurrence rates of high-mass stars in Milky Way stellar clusters Sacha Hony (University of Heidelberg)
Special Seminarabstract and yearly list 14:20~15:20 [R1203]

Kyle Parfrey (Berkeley)
AS/NTU Joint Colloquiumabstract and yearly list 14:20~15:20 [Room 104, CCMS]
Sixty Years of Spiral Density Wave Theory Frank H. Shu (Academia Sinica (Academician), UC Berkeley, UC San Diego)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
Answering fundamental questions of exoplanet formation and habitability with new facilities Michael Ireland (ANU)
Lunch Talkabstract and yearly list 12:00~13:00 [R1203]

James Simpson (ASIAA)
Special Seminarabstract and yearly list 14:20~15:20 [R1203]
The Interstellar Medium and Gas Dynamics of High Redshift Dusty Star-Forming Galaxies and Quasars Daisy Leung (Cornell University)
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IAA Quarterly
IAA Quarterly
2017 Autumn Issue Online!

ASIAA Research Gallery
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