TMT

E297491

TMT is a planned next-generation ground-based optical and infrared observatory featuring a 30-meter primary mirror for extremely high-resolution astronomical observations.

All labels observed (1)

Label Occurrences
TMT canonical 2

How this entity was disambiguated

Statements (52)

Predicate Object
instanceOf astronomical observatory
ground-based optical telescope
infrared telescope
abbreviationFor Thirty Meter Telescope
alternativeProposedSite Roque de los Muchachos
surface form: Roque de los Muchachos Observatory, La Palma, Canary Islands, Spain
apertureClass extremely large telescope
comparedTo European Extremely Large Telescope
Giant Magellan Telescope
fullName Thirty Meter Telescope
governingOrganization TMT International Observatory LLC
hasInstrument Infrared Spectrograph
surface form: Infrared Imaging Spectrograph

Infrared Imaging Spectrograph (IRIS)
Infrared Multi-Slit Spectrometer
Infrared Multi-Slit Spectrometer
surface form: Infrared Multi-Slit Spectrometer (IRMS)

Mid-Infrared Camera and High-disperser Spectrograph
Mid-Infrared Camera and High-disperser Spectrograph
surface form: Mid-Infrared Camera and High-disperser Spectrograph (MICHI)

Planet Formation Instrument
Planet Formation Instrument
surface form: Planet Formation Instrument (PFI)

Wide Field Optical Spectrometer
Wide Field Optical Spectrometer (WFOS)
hasTechnology active optics
adaptive optics
laser guide star system
mirrorType segmented primary mirror
numberOfPrimaryMirrorSegments 492
partner California Institute of Technology
Canada
China
India
Japan
United States of America
surface form: United States

University of California system
surface form: University of California
plannedLocation Mauna Kea
surface form: Mauna Kea, Hawaii, United States
primaryMirrorDiameter 30 meters
scienceCaseIncludes direct imaging of exoplanets
precision cosmology measurements
probing conditions near supermassive black holes
spectroscopy of faint high-redshift galaxies
scienceGoals extremely high angular resolution imaging
high-resolution spectroscopy
study of black holes
study of dark matter and dark energy
study of exoplanets
study of galaxy formation and evolution
study of stellar populations
study of the early universe
status planned
telescopeDesign Ritchey–Chrétien reflector
surface form: Ritchey–Chrétien
telescopeType reflecting telescope
wavelengthRange mid-infrared
near-infrared
optical

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Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.