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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

  • 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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  • Theory

    We aim to perform advanced research leading the world in theoretical astrophysics and contribute to the development of related studies in ASIAA and Taiwan.
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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 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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Upcoming Event
2023-12-04Large-scale Parity Violation Workshop
2024-01-08Taipei Astronomy Workshop
Lunch Talkabstract and yearly list 12:00~12:40 [R1412]
Hurdling Exozodiacal Dust Challenges in Habitable Exoplanet Direct Imaging: Harder Than Anticipated? Yu-Chia Lin (U of Arizona)
Colloquiumabstract and yearly list 14:20~15:20 [1st Floor Auditorium]
Searching for dark-matter black holes from LVK gravitational-wave detectors Donghui Jeong (Penn State University / KIAS)
Lunch Talkabstract and yearly list 12:00~12:40 [R1412]
Circumnuclear structures and environments of nearby Seyfert galaxies with visualization of CARTA Ming-Yi Lin (ASIAA)
Seminarabstract and yearly list 14:20~15:20 [R1203]

Jong-Hak Woo (Seoul National University)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
The molecular ISM and astrochemistry in the starburst galaxy NGC 253: The ALCHEMI survey Nanase Harada (NAOJ)
IAA Quarterly
IAA Quarterly
2023 Autumn Issue Online!
IAA Quarterly
Apply Time for NanoSIMS Facility
TEL: 886-2-3365-2200 FAX: 886-2-2367-7849
General: asiaa_replace2@_asiaa.sinica.edu.tw Media Request: epo_replace2@_asiaa.sinica.edu.tw
11F of AS/NTU Astronomy-Mathematics Building, No.1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.C.