Add to ORKGCornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm telescope. The nominal location for this facility will be the high Atacama Desert of Northern Chile. The baseline design is a segmented mirror telescope optimized for operation at wavelengths longer than 200 microns to take advantage of a low precipitable water vapor at the site. We discuss science drivers and their implications for telescope design and technical requirements, and planned technical study areas
Institute of Astronomy, Graduate School of Science, the University of Tokyo is promoting the Univers...
The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background s...
The University of Tokyo Atacama Observatory Project is to construct and operate a 6.5m infrared tele...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
The Atacama Large Aperture Submillimeter Telescope (AtLAST) is a concept for a 50m class single-dish...
The Atacama Large Millimeter Array (ALMA) is a major ground-based telescope for millimeter and submi...
In the past decade a strong case has been made for the construction of a next generation, 25 to 40-m...
The Atacama Large Millimeter Array (ALMA) is a major ground based project for millimeter and submill...
We report on the plan to construct a 50 m class millimeter (mm) and sub-mm single dish telescope, th...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
The proposed next generation Event Horizon Telescope (ngEHT) concept envisions the imaging of variou...
The Atacama Cosmology Telescope (ACT) is a 6-meter diameter telescope designed to make detailed meas...
The coldest and densest structures of gas and dust in the Universe have unique spectral signatures a...
Institute of Astronomy, Graduate School of Science, the University of Tokyo is promoting the Univers...
The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background s...
The University of Tokyo Atacama Observatory Project is to construct and operate a 6.5m infrared tele...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
The Atacama Large Aperture Submillimeter Telescope (AtLAST) is a concept for a 50m class single-dish...
The Atacama Large Millimeter Array (ALMA) is a major ground-based telescope for millimeter and submi...
In the past decade a strong case has been made for the construction of a next generation, 25 to 40-m...
The Atacama Large Millimeter Array (ALMA) is a major ground based project for millimeter and submill...
We report on the plan to construct a 50 m class millimeter (mm) and sub-mm single dish telescope, th...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
The proposed next generation Event Horizon Telescope (ngEHT) concept envisions the imaging of variou...
The Atacama Cosmology Telescope (ACT) is a 6-meter diameter telescope designed to make detailed meas...
The coldest and densest structures of gas and dust in the Universe have unique spectral signatures a...
Institute of Astronomy, Graduate School of Science, the University of Tokyo is promoting the Univers...
The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background s...
The University of Tokyo Atacama Observatory Project is to construct and operate a 6.5m infrared tele...