CCAT will be a 25 m diameter submillimeter-wave telescope that will operate inside a dome located on Cerro Chajnantor in the Atacama Desert. The telescope must have high aperture efficiency at a wavelength of 350 microns and good performance out to a wavelength of 200 microns. A conceptual design for a carbon fiber reinforced plastic (CFRP) truss and primary reflector support truss has been developed. This design yields a telescope with a net �½ wave front error of <10 microns using a lookup table to adjust the segment actuators to compensate for gravitational deflections. Minor corrections may be required to compensate for the expected 20 C temperature excursions. These can be handled using a coarse lookup table
Abstract The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous inc...
Precision astronomic structures such as telescopes often require structural materials that possess u...
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into ...
CCAT will be a 25 m diameter submillimeter-wave telescope that will operate inside a dome located on...
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2-1.5 mm wavelength range...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The Cornell Caltech Atacama Telescope (CCAT) is a 25 m diameter telescope that will operate at wavel...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in ...
CCAT1 is a submillimeter telescope currently under development that will be located at an altitude o...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
A telescope mount with a single-point force support at the center of gravity of the primary mirror i...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
This paper describes the development of a Carbon Fiber-Reinforced Plastics (CFRP) structure for the ...
Abstract The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous inc...
Precision astronomic structures such as telescopes often require structural materials that possess u...
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into ...
CCAT will be a 25 m diameter submillimeter-wave telescope that will operate inside a dome located on...
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2-1.5 mm wavelength range...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The Cornell Caltech Atacama Telescope (CCAT) is a 25 m diameter telescope that will operate at wavel...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in ...
CCAT1 is a submillimeter telescope currently under development that will be located at an altitude o...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
A telescope mount with a single-point force support at the center of gravity of the primary mirror i...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
This paper describes the development of a Carbon Fiber-Reinforced Plastics (CFRP) structure for the ...
Abstract The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous inc...
Precision astronomic structures such as telescopes often require structural materials that possess u...
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into ...