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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.
    > Learn more

  • 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.
    > Learn more

  • 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.
    > Learn more

  • 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.
    > Learn more

  • TAOS

    Transneptunian Automated Occultation Survey, will measure the size distribution of small objects (~1 km diameter) in the Kuiper Belt and beyond.
    > Learn more

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Upcoming Event
2018-03-10ASIAA Outreach Activity @ NTU Azalea Festival 2018
2018-03-26ALMA Users Workshop 2018
Special Seminarabstract and yearly list 11:00~12:00 [R1203]
Observational study of evolution from formation of protostellar disks to formation of planets Hsi-Wei Yen (ESO)
Lunch Talkabstract and yearly list 12:15~13:15 [R1203]
Understanding the Evolution and Environments of Supernova Remnants Through the Lx-Size Diagram Po-Sheng Ou (NTU)
Special Seminarabstract and yearly list 11:00~12:00 [R1203]
From filaments to circumstellar disks: on the star and planet formation at parsec and 100s AU scales Ya-Wen Tang (ASIAA)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
Astrophysical neutrinos and new physics
Guey-Lin Lin (NCTU)
Special Seminarabstract and yearly list 14:20~15:20 [R1203]
Triple-ridge structure of relativistic jets driven by black holes
Taiki Ogihara (Tohoku University)
ASIAA Outreach Activity @ NTU Azalea Festival
ASIAA Outreach Activity
@ NTU Azalea Festival
IAA Quarterly
IAA Quarterly
2017 Winter Issue Online!

ASIAA Research Gallery
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