::: Sitemap Chinese Version中文 PrintPrint Friendly search help
Previous
  • Frank Shu
  • 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

  • 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

  • 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.
    > Learn more

  • 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.
    > Learn more

  • 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

What's New rss feed

Upcoming Event
2023-07-032023 ASIAA Summer Student Program
2023-11-06Scintillometry 2023
2023-11-202023 Advanced Telescope and Instrument Technology Conference
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
Quasar Variability and its Relation with Accretion Disc Properties Ji-Jia Tang (Australian National University/NTU)
Lunch Talkabstract and yearly list 12:00~12:40 [R1412]
Measuring the matter-radiation equality scale
Benedict Bahr Kalus (KASI)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
The Imaging X-ray Polarimetry Explorer (IXPE): A Paradigm-Breaking Scientific Mission Chien-Ting Chen (NASA MSFC/USRA)
Lunch Talkabstract and yearly list 12:00~12:40 [R1412]
How to grow a Supermassive Black Hole
Ken (ASIAA)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]

Hiro Nagataki (Riken)
IAA Quarterly
IAA Quarterly
2023 Spring Issue Online!
IAA Quarterly
Apply Time for NanoSIMS Facility

ASIAA Research Gallery
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.