A two arm, opto-mechanical positioner mechanism is presented in this proceedings as a candidate steering system for the millimeter-wave XSPEC spectrograph. The design is well matched to the expected target density on the sky, and meeting all requirements of the Cerro Chajnantor Atacama Telescope (CCAT), site environmental conditions (e.g., operating temperature and power dissipation), and the positioning requirements themselves for acquiring and tracking astronomical objects whose light is fed into the XSPEC spectrograph units. The prototype design has been fabricated and tested for basic operations
A common optical design for a coma-corrected, 6-meter aperture, crossed-Dragone telescope has been a...
How does one study the evolution of the Milky Way, or the expansion of the Universe, or explore the ...
SuperSpec is an integrated, on-chip spectrometer for millimeter and sub-millimeter astronomy. SuperS...
A two arm, opto-mechanical positioner mechanism is presented in this proceedings as a candidate stee...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
CCAT1 is a submillimeter telescope currently under development that will be located at an altitude o...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in ...
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into ...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama T...
The 25-m aperture Cornell Caltech Atacama Telescope (CCAT) will have a primary mirror that is divide...
Large multi-object spectroscopy telescopes measure the light from millions of stars and galaxies for...
We developed a scan mirror mechanism (SMM) that enable a slit-based spectrometer or spectropolarimet...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
A common optical design for a coma-corrected, 6-meter aperture, crossed-Dragone telescope has been a...
How does one study the evolution of the Milky Way, or the expansion of the Universe, or explore the ...
SuperSpec is an integrated, on-chip spectrometer for millimeter and sub-millimeter astronomy. SuperS...
A two arm, opto-mechanical positioner mechanism is presented in this proceedings as a candidate stee...
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be loc...
CCAT1 is a submillimeter telescope currently under development that will be located at an altitude o...
CCAT will be a 25 m diameter, submillimeter-wave telescope. It will be located on Cerro Chajnantor i...
The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in ...
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into ...
CCAT is a submillimeter telescope currently under development that will be located at an altitude of...
We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama T...
The 25-m aperture Cornell Caltech Atacama Telescope (CCAT) will have a primary mirror that is divide...
Large multi-object spectroscopy telescopes measure the light from millions of stars and galaxies for...
We developed a scan mirror mechanism (SMM) that enable a slit-based spectrometer or spectropolarimet...
Cornell, California Institute of Technology (Caltech), and Jet Propulsion Lab (JPL) have joined toge...
A common optical design for a coma-corrected, 6-meter aperture, crossed-Dragone telescope has been a...
How does one study the evolution of the Milky Way, or the expansion of the Universe, or explore the ...
SuperSpec is an integrated, on-chip spectrometer for millimeter and sub-millimeter astronomy. SuperS...