Scientists Industry

Sign In

About
The US-Extremely Large Telescope Program
Science with TMT
The Observatory
Education & Engagement
News & Multimedia
Documents
Blog

Home
About

Industry and Employment Opportunities

The US-Extremely Large Telescope Program

Science with TMT

Science Advisory Committee (SAC) webinars

TMT Science Forums

TMT's Technical and Scientific Heritage

Fundamental Physics and Cosmology

Early Universe, Galaxy Formation and the IGM

Supermassive Black Holes

Milky Way and Nearby Galaxies

Stars, Stellar Physics and the Interstellar Medium

Formation of Stars and Planets

Our Solar System

Time Domain Science

Science Instruments

Overview of Instrument Capabilities

Wide-Field Optical Spectrometer (WFOS)

Infrared Imaging Spectrograph (IRIS)

Multi-Objective Diffraction-limited High-Resolution Infrared Spectrograph (MODHIS)

Facility Adaptive Optics (NFIRAOS)

Second Generation Instruments

TMT International Science Development Teams

Information for TMT Observers

Science Capabilities

Science Operations

The Observatory

Summit Facilities and Enclosure

Telescope Systems

Adaptive Optics

Telescope Structure

Observatory Software

Education & Engagement

Education & Engagement

News & Multimedia

TMT E-news/Newsletter

Events
Documents
Blog

Scientists
Industry

Contact Us
Search

Sign In

FAQs
Partners
Governance
Industry and Employment Opportunities

Astro2020

Science Advisory Committee (SAC) webinars
TMT Science Forums
TMT's Technical and Scientific Heritage
Science Themes
Science Instruments
TMT International Science Development Teams
Information for TMT Observers

Summit Facilities and Enclosure
Telescope Systems

Conversations
Education & Engagement
Partnerships

Fundamental Physics and Cosmology
Early Universe, Galaxy Formation and the IGM
Supermassive Black Holes
Milky Way and Nearby Galaxies
Stars, Stellar Physics and the Interstellar Medium
Formation of Stars and Planets
Exoplanets
Our Solar System
Time Domain Science

Overview of Instrument Capabilities
Wide-Field Optical Spectrometer (WFOS)
Infrared Imaging Spectrograph (IRIS)
Multi-Objective Diffraction-limited High-Resolution Infrared Spectrograph (MODHIS)
Facility Adaptive Optics (NFIRAOS)
Second Generation Instruments

TMT Optics
Adaptive Optics
Controls
Telescope Structure
Observatory Software

News
For the Media
TMT E-news/Newsletter
Press Coverage
Events
Image Gallery
Multimedia

Board Members
SAC Members

Science Capabilities
Science Operations

Tmt comp background

Profile

Masayuki Akiyama (SAC Chair & Japan Co-Chair)

Professor

Tohoku University

The Thirty Meter Telescope (TMT) International Observatory (TIO) is an extraordinary international scientific endeavor that has the potential to revolutionize our understanding of the universe and our place within it. TIO’s preferred site is Maunakea, and TIO is working to be a model observatory that demonstrates deep respect for the significance of Maunakea to the community.

TIO’s members are the California Institute of Technology, University of California, the National Institutes of Natural Sciences of Japan, the Department of Science and Technology of India, and the National Research Council of Canada. The Association of Universities for Research in Astronomy is an associate member. Major funding has been provided by the Gordon and Betty Moore Foundation. The National Science Foundation has provided funding for recent design and development work.
inquiry@tmt.org

TMT Policies

Privacy Policy
Image Use Policy

Work with TMT

Employment Opportunities
Industry Opportunities

Quick Links

TMT La Palma

Sign up for TMT news and updates

Home About Contact

© 2022 - TMT International Observatory. All Rights Reserved.

Website designed by IPAC Communications & Education Team