On July 16, 2018, a workshop about TMT's Mid-Infrared Camera, High-disperser, and Integral field spectrograph (MICHI) was held at the National Astronomical Observatories, CAS (NAOC), Beijing.
The National Science Foundation’s (NSF) National Optical Astronomy Observatory (NOAO) and its collaborative partners, the Thirty Meter Telescope International Observatory (TIO) and the Giant Magellan Telescope Organization (GMTO) invite all interested U.S. scientists to participate in the development of exemplar Key Science Programs (KSPs) for the Giant Magellan Telescope (GMT) and Thirty Meter Telescope (TMT), preferably working in concert.
A new research frontier in astronomy and astrophysics will open in the mid-2020s with the advent of ground-based extremely large optical-infrared telescopes (ELTs) with primary mirrors in the 20-m – 40-m range. U.S. scientific leadership in astronomy and astrophysics will be significantly enhanced if the broad U.S. community can take advantage of the power of these new ELTs. In that context, the National Science Foundation’s (NSF) National...
Members of the TMT Science Advisory Committee (SAC) met in Pasadena on April 9&10, 2018 for their quarterly gathering. SAC representatives reported on their respective activities for the TMT project and discussed top-level requirements for TMT’s suite of science instruments.
Pasadena, March 16, 2018 - The conceptual design and scope of TMT’s Refrigerant Cooling System (REFR), which was executed and developed by a close Chinese-North American collaboration, successfully passed a recent conceptual design review. This system will be used to provide cooling to electronics enclosures mounted on the telescope structure. The system also maintains several TMT instrument enclosures at subzero temperatures to reduce thermal...
Pasadena, CA - March 8, 2018 - Future users of the Thirty Meter Telescope are now preparing studies of the science instruments that will be deployed after the telescope's first-light instrumentation suite.
The shipment of TMT’s first meniscus-shaped primary mirror segment to the Indian Institute of Astrophysics (IIA) in Bengaluru (Bangalore) has just been completed.
The Real-Time Controller of TMT’s Narrow Field InfraRed Adaptive Optics System (NFIRAOS) successfully passed its final design review and is ready to proceed to the fabrication phase, which is expected to last approximately four years.
Following a successful second IRIS Preliminary Design Phase Review (PDR-2) at the TMT Project Office in Pasadena, IRIS is proceeding into its Final Design phase. The focus of the second review, held in September, involved an assessment of the IRIS software (including its data reduction system) and electrical design (including its detectors) as well as programmatic aspects spanning project cost and overall schedule.
Representatives from the Thirty Meter Telescope’s (TMT’s) Wide-Field Optical Spectrograph (WFOS) team and TMT’s China partners gathered on October 16 in Beijing, China to discuss potential collaboration during the next stage of the conceptual design of WFOS.
