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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

  • TAOS

    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.
    > Learn more

  • AMiBA

    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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  • 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

  • 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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  • 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

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Upcoming Event
2014-12-08Dawn of New Cosmology: Opportunities and Challenges in CMB Polarization and Large Scale Structure
2014-12-156th PFS Collaboration Meeting
2014-12-18Evolution of SMBHs with HSC: First results from initial dataset
2015-02-09East Asian Young Astronomers Meeting 2015
Tech Lunch Talkabstract and yearly list 12:00~13:00 [R1203]
Metrology Camera System of Prime Focus Spectrograph for Subaru Telescope
Chueh-Yi Chou (ASIAA)
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
Exploring Our Solar System with Mass Spectrometry
Wei-Ling Tseng (NTNU)
Astro-ph Coffee 15:30~16:00 [12F Interaction Area]
informal discussion of exciting new results on astro-ph
Lunch Talkabstract and yearly list 12:00~13:00 [R1203]
TBA
Shou-Hsien Weng (ASIAA)
Astro-ph Coffee 15:30~16:00 [12F Interaction Area]
informal discussion of exciting new results on astro-ph
Colloquiumabstract and yearly list 14:20~15:20 [R1203]
Dwarf Galaxies and Their Role as Building Blocks
Eva Grebel (Heidelberg University)
Open House
2014 AS Open House - IAA Achievement Exhibition on Nov. 1st
IAA Quarterly
IAA Quarterly
2014 Summer Issue Online!

ASIAA Research Gallery
TEL: 886-2-3365-2200 FAX: 886-2-2367-7849
General: asiaa_replaceTOat_sign_asiaa.sinica.edu.tw Media Request: epo_replaceTOat_sign_asiaa.sinica.edu.tw
11F of Astronomy-Mathematics Building, AS/NTU. No.1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.C.