Add to ORKGCCAT will be a 25m diameter sub-millimeter telescope capable of operating in the 0.2 to 2.1mm wavelength range. It will be located at an altitude of 5600m on Cerro Chajnantor in northern Chile near the ALMA site. The anticipated first generation instruments include large format (60,000) kinetic inductance detector (KID) cameras, a large format heterodyne array and a direct detection multi-object spectrometer. The paper describes the architecture of the CCAT software and the development strategy
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2-1.5 mm wavelength range...
We present the detailed science case, and brief descriptions of the telescope design, site, and firs...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
CCAT will be a 25m diameter sub-millimeter telescope capable of operating in the 0.2 to 2.1mm wavele...
Abstract. CCAT will be a 25-meter telescope for submillimeter astronomy located at 5600 m altitude o...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama T...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
Five partners have currently joined a Consortium to develop the Cornell Caltech Atacama Telescope (C...
CCAT is a 25 meter submm telescope proposed to be built at 5600 meters elevation on Cerro Chajnantor...
We describe the Short Wavelength Camera (SWCam) for the CCAT observatory including the primary scien...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
Star formation, which drives the evolution of baryonic matter in the universe, occurs in the densest...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m, off-axis, low-emissivity, la...
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2-1.5 mm wavelength range...
We present the detailed science case, and brief descriptions of the telescope design, site, and firs...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...
CCAT will be a 25m diameter sub-millimeter telescope capable of operating in the 0.2 to 2.1mm wavele...
Abstract. CCAT will be a 25-meter telescope for submillimeter astronomy located at 5600 m altitude o...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama T...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
Five partners have currently joined a Consortium to develop the Cornell Caltech Atacama Telescope (C...
CCAT is a 25 meter submm telescope proposed to be built at 5600 meters elevation on Cerro Chajnantor...
We describe the Short Wavelength Camera (SWCam) for the CCAT observatory including the primary scien...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
Star formation, which drives the evolution of baryonic matter in the universe, occurs in the densest...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m, off-axis, low-emissivity, la...
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2-1.5 mm wavelength range...
We present the detailed science case, and brief descriptions of the telescope design, site, and firs...
Cornell and Caltech are undertaking a two year conceptual design study for a 25-m class sub-mm teles...