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Institute of Astronomy & Astrophysics, Academia Sinica

Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) has built up core groups in theoretical and experimental astrophysics and instrumentation, aspiring to be at the forefront of astronomical research. Research topics carried out at ASIAA range from solar system, star formation, to extra-galactic science and cosmology.

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Institute of Astronomy & Astrophysics, Academia Sinica | asiaa.sinica.edu.tw Reviews
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Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) has built up core groups in theoretical and experimental astrophysics and instrumentation, aspiring to be at the forefront of astronomical research. Research topics carried out at ASIAA range from solar system, star formation, to extra-galactic science and cosmology.
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1 Astronomy
2 Astrophysics
3 SAO/ASIAA Submillimeter Array (SMA)
4 Taiwanese-American Occultation Survey (TAOS)
5 Computational Astrophysics(CompAS)
6 Yuan Tseh Lee Array for Microwave Background Anisotropy (AMiBA)
7 Optical and Infrared Astronomy (OIR)
8 Theoretical Institute for Advanced Research in Astrophysics (TIARA)
9 Atacama Large Mil
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Institute of Astronomy & Astrophysics, Academia Sinica | asiaa.sinica.edu.tw Reviews

https://asiaa.sinica.edu.tw

Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) has built up core groups in theoretical and experimental astrophysics and instrumentation, aspiring to be at the forefront of astronomical research. Research topics carried out at ASIAA range from solar system, star formation, to extra-galactic science and cosmology.

SUBDOMAINS

events.asiaa.sinica.edu.tw events.asiaa.sinica.edu.tw

ASIAA Website

You will be redirected to ASIAA Academic Events.

sdl.asiaa.sinica.edu.tw sdl.asiaa.sinica.edu.tw

Superconducting Device Lab - Introduction_En

User(s) are online ( 1. User(s) are browsing Introduction. At 1994, ASIAA collaborated with Prof. C. C. Chi and prof. M.K. Wu,. To found a laboratory for superconducting device development. The short term goal of laboratory is to establish the capability of low temperature superconducting device fabrication in. The facilities for fabricating process of Nb-based SIS junction are established completely at 2000. More facilities are added to enhance our capability. New clean room is built in. We would like t...

outreach.asiaa.sinica.edu.tw outreach.asiaa.sinica.edu.tw

Education and Public Outreach, ASIAA

在教育與推廣活動方面,除了每年10月的中研院年度院區開放日活動,我們也參與每年在臺灣中部舉辦的 星光饗宴 觀星活動、南部舉辦的 南十字星星吶 活動,以及3月臺灣大學的 杜鵑花節 校區開放日活動。 網路天文新聞方面,2003年10月成立了 中研院天文網 中文網站,日前改址為 中研院天聞網. 更新日期: 2017-01-06 聯絡窗口: epo.

compas.asiaa.sinica.edu.tw compas.asiaa.sinica.edu.tw

Computational Astrophysics at ASIAA

Pattern speeds in galaxies. Daniel Pfenniger (University of Geneva). Winds from black hole accretion systems. Save the Planet, Feed the Star: How Planets can Survive Migration and Drive Accretion. Selected topics in theoretical astrophysics. Hydrodynamic processes in protoplanetary accretion disks. Self-consistent Neutrino-Driven Core-Collapse Supernova Simulations with Neutrino Transport. Kuo-Chuan Pan (University of Basel). Astrochemistry: gas-phase chemical network. Pak Shing Li (Berkeley). The CompAS...

sma.asiaa.sinica.edu.tw sma.asiaa.sinica.edu.tw

Sub-Millimeter Array, SMA

2016-08-02: 2016B Call for Proposals. The ASIAA SMA Time Allocation Committee, with the CfA SMA TAC, solicit SMA observing proposals for the 2016B semester:. Observing period : 2016 Nov 16 - 2017 May 15 (2016B semester). Proposal deadline: 2016 Aug. 12th (Fri.) 5:00AM in Taiwan. 2016-01-20: SMA-T TAC Chairs. Standard projects: Keiichi Asada. Filler projects (extragalactic): Kazushi Sakamoto. Filler projects (Galactic): Naomi Hirano. Since 1996, Acade mia Sinica Institute of Astronomy and Astrophysics.

asmab.asiaa.sinica.edu.tw asmab.asiaa.sinica.edu.tw

ASMAB

Gallery of weekly progress. Web Comments or Question?

vlbi.asiaa.sinica.edu.tw vlbi.asiaa.sinica.edu.tw

VLBI Group at ASIAA

Workshop: Black Hole Astrophysics with VLBI - Past, Present, and Future. EHT Collaboration Meeting 2016. M87 Workshop: Towards the 100th Anniversary of the Discovery of Cosmic Jets. ALMA Links with Other Observatories to Create Earth-size Telescope. GLT Team Meets with Kip Thorne. GLT Face to Face Meeting, Taipei. VLBI Experiment for APP commissioning with JCMT/SMA. East Asia VLBI Workshop 2015, Sapporo, Japan. GLT Project Risk Review, Taipei. EHT 13 mm VLBI Observation, Hawaii. GLT Face to Face Meeting.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

TAOS operates four small (50 cm) telescopes at Lulin observatory in central Taiwan. Each telescope is equipped with a 2kx2k CCD camera manufactured by Spectral Instruments. These cameras take 2.5 seconds to read out an entire image, which is much too slow to detect occultation events. We have thus developed a new readout technique which we call zipper mode. A detailed description of this readout method is given here. A CCD camera used by TAOS. The telescopes TAOS A and TAOS B at Lulin Observatory.

taos2.asiaa.sinica.edu.tw taos2.asiaa.sinica.edu.tw

TAOS II-Transneptunian Automated Occultation Survey

Welcome to TAOS II. TAOS II will build upon the successful operation of a precursor survey, TAOS I. The survey will operate three medium sized telescopes at the Observatorio Astronomico Nacional (OAN). To view the construction of the TAOS II system at San Pedro Mártir Observatory. Last Updated: 2014-10-17 Contact: wlyen. Privacy and Security Policy.

INTERNAL PAGES

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1

ASIAA - The Atacama Large Millimeter/Submillimeter Array (ALMA-T)

http://www.asiaa.sinica.edu.tw/project/alma.php

Information for Foreign Visitors. Interstellar and Circumstellar Medium. Atacama Large Millimeter/submillimeter Array (ALMA) - Taiwan. Click the image for more. The Innermost Mass Distribution of the Gravitational Lens SDP.81 from ALMA Observations. ALMA Revealing the Pseudo-disk, Keplerian Rotating disk, and Jet in the Very Young Protostellar System HH 212. ALMA Revealing the Pseudo-disk, Keplerian Rotating disk, and Jet in the Very Young Protostellar System HH 212. The ALMA alternative laser synthesizer.

2

ASIAA - Maps

http://www.asiaa.sinica.edu.tw/guide/map.php

Information for Foreign Visitors. Interstellar and Circumstellar Medium. Visitor Guide Astronomy-Mathematics Building Maps. Astronomy-Mathematics Building (ASMAB) Maps. In the winter of 2009,. Moved into the Astronomy-Mathematics Building (ASMAB), located on the campus of the National Taiwan University (. In Taipei. The Astronomy-Mathematics Building houses the. The AS Mathematics Institute and their. Provides a collection of photos during construction. Nearby hotels and directions from.

3

ASIAA - The Yuan Tseh Lee Array for Microwave Background Anisotropy (AMiBA)

http://www.asiaa.sinica.edu.tw/project/amiba.php

Information for Foreign Visitors. Interstellar and Circumstellar Medium. The Yuan Tseh Lee Array for Microwave Background Anisotropy (AMiBA). Click the image for more. Clock Distribution Drawer for YTLA. Clock Distribution Drawer for YTLA. Clock Distribution Drawer for YTLA. The first phase of AMiBA consisted of seven 0.6m antennas close-packed in the center of the 6m platfor. The first SZE signal with the 7-element AMiBA. The first SZE signal with the 7-element AMiBA. Structures tightly constrain the co...

4

ASIAA - Computation Fluid Dynamics-MagnetoHydroDynamics (CFD-MHD)

http://www.asiaa.sinica.edu.tw/project/compas.php

Information for Foreign Visitors. Interstellar and Circumstellar Medium. Computational Astrophysics (CompAS) Website. Click the image for more. Cotribution analysis of molecular line of a disk. Formation of Isothermal Circumplanetary Disks with Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets. Formation of Isothermal Circumplanetary Disks with Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets. HYDRODYNAMICAL SIMULATIONS OF THE BARRED SPIRAL GALAXY NGC 1097.

5

ARC-Taiwan ALMA Archive

http://www.asiaa.sinica.edu.tw/~kswang/ALMA/index.html

Contact person: Kuo-Song Wang (kswang AT asiaa.sinica.edu.tw). This ARC-Taiwan ALMA archival data preview database is built from the official ALMA archive. By Frank J. Lovas. Each dataset was processed for a preview. Purpose in the image domain. Users are recommended to re-process the datasets carefully for publications. The preview image cubes (CASA format) can be retrieved by an email to kswang AT asiaa.sinica.edu.tw for now. Darr; ↓ ↓ Pick up a category below ↓ ↓ ↓. Clustered Massive Galaxy Formation ...

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franz-in-schina.blogspot.com franz-in-schina.blogspot.com

Geschichtensammlung: Taiwan...

http://franz-in-schina.blogspot.com/2010/08/taiwan.html

Is ja nisch viel ßeit, wa! Mein Profil vollständig anzeigen. Dienstag, 10. August 2010. Nun ist also die erste Woche Taiwan schon wieder mehr als rum und dies weder viel zu schnell noch viel zu langsam sondern genau richtig! Taiwan ist für mich eine totale Überraschung. Ich bin zwar wie immer ohne jegliche Erwartungen hergekommen (zumindest hätte ich nicht sagen können, was ich denn für Erwartungen hätte), aber trotzdem ist es irgendwie anders als erwartet ;). Taiwan ist China ohne den nervigen Part!

oir.asiaa.sinica.edu.tw oir.asiaa.sinica.edu.tw

CFHT

http://oir.asiaa.sinica.edu.tw/cfht

Our activities in optical-IR astronomy have been rapidly growing in recent years. We have a dozen researchers (staff, postdocs and students) who are pursuing their own interests, ranging from asteroids to distant galaxies. Our institute has access to Canada-France-Hawaii Telescope (CFHT). Which has been recently developed by our institute. Last Updated: 2012-02-24 Contact: wlyen. Privacy and Security Policy. Photos by Canada-France-Hawaii Telescope / Coelum.

oir.asiaa.sinica.edu.tw oir.asiaa.sinica.edu.tw

SUBARU

http://oir.asiaa.sinica.edu.tw/subaru

In 2006, NAOJ proposed to construct the Hyper Suprime-Cam (HSC). Meanwhile, ASIAA is also working on the MOIRCS upgrade with Subaru telescope. MOIRCS is the major near-IR instrument of Subaru telescope. The upgrade of MOIRCS includes the installation of new Hawaii-2RG arrays with ASIC controller and Integral Field Unit (IFU) units. The upgrade work started in 2014 and is planned to be completed in 2015. Last Updated: 2014-09-17 Contact: wlyen. Privacy and Security Policy.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

http://taos.asiaa.sinica.edu.tw/tw/index.php

中美掩星計畫 ( Taiwan American Occultation Survey; 以下簡稱TAOS ) 的目的在於偵測包含古柏帶以及更遠處的直徑約1公里的小型天體。 幾十年以來,藉由大型望遠鏡,天文學家已經在海王星以外之處,發現超過1000顆直徑超過100公里的天體。 TAOS的主要目的就是估算直徑介於500公尺至30公里的古柏帶天體(Kuiper Belt Objects; KBOs)的數量。 掩星的發生機率極低,據估計,每顆星每年只會發生不到0.01次,因此我們必須長時間偵測數百顆星才有機會偵測到掩星事件。 TAOS利用位於中台灣的鹿林天文台的四部50公分小型望遠鏡來進行觀測,每部望遠鏡配置了由 Spectral Instruments. 這款相機需要2.5秒才能讀取一幅完整的影像,對於掩星來說,這樣的讀取速度實在太慢。 為此我們開發了一種新的,我們稱之為zipper mode的讀取技術,詳細的描述請參看 這裡. 位在鹿林天文台的TAOS A 和 TAOS B望遠鏡. Last Updated: 2014-09-11 Contact: wlyen.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

http://taos.asiaa.sinica.edu.tw/about.php

Taiwan, R.O.C. Room 217B, Baekyang Hall, Yonsei University. 50 Yonsei-ro, Seodaemun-gu, Seoul 120-749. No 300, Jhongda Rd, Jhongli City. Taiwan, R.O.C. Tel: 886-3-4227151 ext: 65950. Livermore, CA 94551-0808. Cambridge, MA 02138. Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan. Wei Ling Yen 嚴葦玲. Harvard-Smithsonian Center for Astrophysics, USA. Department of Astronomy, Yonsei University, South Korea. Stanford Linear Accelerator Center, Stanford, USA. Wen Ping Chen 陳文屏.

alma.asiaa.sinica.edu.tw alma.asiaa.sinica.edu.tw

Atacama Large Millimeter/submillimeter Array, ALMA - Taiwan

http://alma.asiaa.sinica.edu.tw/science_highlights.php

Science Goals for ALMA. The East-Asia Front End Integration Center. Alternative Laser Synthesizer (ALS). LO Reference Test Module (LORTM). Front End Service Vehicle (FESV). ALMA Community Day and CASA Workshop 2014. 9th ALMA TAIWAN User Workshop. 2nd tuCASA-ASIAA ALMA Imaging Workshop. Workshop for CY1 Phase II Procedure. ALMA TAIWAN Imaging Workshop. 4th ALMA TAIWAN User Workshop. Workshop for CY0 Phase II Procedure. 3nd ALMA TAIWAN User Workshop. 2nd ALMA TAIWAN User Workshop. The first ALMA-Taiwan res...

alma.asiaa.sinica.edu.tw alma.asiaa.sinica.edu.tw

Atacama Large Millimeter/submillimeter Array, ALMA - Taiwan

http://alma.asiaa.sinica.edu.tw/science_cycle1.php

Science Goals for ALMA. The East-Asia Front End Integration Center. Alternative Laser Synthesizer (ALS). LO Reference Test Module (LORTM). Front End Service Vehicle (FESV). ALMA Community Day and CASA Workshop 2014. 9th ALMA TAIWAN User Workshop. 2nd tuCASA-ASIAA ALMA Imaging Workshop. Workshop for CY1 Phase II Procedure. ALMA TAIWAN Imaging Workshop. 4th ALMA TAIWAN User Workshop. Workshop for CY0 Phase II Procedure. 3nd ALMA TAIWAN User Workshop. 2nd ALMA TAIWAN User Workshop. PI &#058 Lee Chin-Fei.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

http://taos.asiaa.sinica.edu.tw/links.php

Known Outer Solar System Objects (Wikipedia links). IAU/MPC (Minor Planet Center). Central Weather Bureau, Taiwan. The Kuiper Belt Electronic Newsletter. Last Updated: 2014-09-12 Contact: wlyen. Privacy and Security Policy.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

http://taos.asiaa.sinica.edu.tw/index.php

TAOS operates four small (50 cm) telescopes at Lulin observatory in central Taiwan. Each telescope is equipped with a 2kx2k CCD camera manufactured by Spectral Instruments. These cameras take 2.5 seconds to read out an entire image, which is much too slow to detect occultation events. We have thus developed a new readout technique which we call zipper mode. A detailed description of this readout method is given here. A CCD camera used by TAOS. The telescopes TAOS A and TAOS B at Lulin Observatory.

taos.asiaa.sinica.edu.tw taos.asiaa.sinica.edu.tw

TAOS

http://taos.asiaa.sinica.edu.tw/stellar_variability.php

The TAOS Project Stellar Variability. II Detection of 15 Variable Stars. I Detection of Low-Amplitude δ Scuti Stars. Data is not available. Last Updated: 2014-04-17 Contact: wlyen. Privacy and Security Policy.

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Institute of Astronomy & Astrophysics, Academia Sinica

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. 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. The Atacama Lar...

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Asiaa1408 (Joanna) - DeviantArt

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