Add to ORKGIn order to fully characterize the astronomical potential of remote sites on the antarctic plateau, we have developed a suite of instruments covering UV to sub-millimeter wavelengths. In addition, we have successfully demonstrated the use of an acoustic radar at the South Pole to measure the height of the turbulent atmospheric boundary layer. Each instrument is designed to operate independently and autonomously, producing reliable, fully calibrated data without human intervention. Although designed primarily for use in Antarctica, these instrument use novel technology that is applicable to other astronomical applications as well
Hereafter we give a brief history of our contribution to astronomical site testing in Antarctica, at...
The primary limitation to ground based astronomy is the Earth’s atmosphere. The atmosphere above the...
The Antarctic plateau has superb astronomical seeing above a turbulent boundary layer. This layer ha...
In order to fully characterize the astronomical potential of remote sites on the antarctic plateau, ...
Over the past decade we have developed a series of increasingly sophisticated robotic instruments fo...
We have assembled a team with expertise in astronomical site testing in the Antarctic and expertise ...
At altitudes of up to 4100m, the Domes of the Antarctic plateau provide unique opportunities for gro...
Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, ...
Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, ...
Abstract: We have developed a 350 µm radiometer to perform automated site testing in remote regions ...
The perfect site for astronomical interferometry would be one where the wind speeds throughout the a...
We have developed a 350 mum radiometer to perform automated site testing in remote regions of Antarc...
The height of the atmospheric boundary layer on the Antarctic plateau is of particular interest to m...
The unique advantages for astronomy on the Antarctic plateau are now well established. In particular...
We discuss the site conditions for astronomy at the South Pole and over the Antarctic plateau. We fi...
Hereafter we give a brief history of our contribution to astronomical site testing in Antarctica, at...
The primary limitation to ground based astronomy is the Earth’s atmosphere. The atmosphere above the...
The Antarctic plateau has superb astronomical seeing above a turbulent boundary layer. This layer ha...
In order to fully characterize the astronomical potential of remote sites on the antarctic plateau, ...
Over the past decade we have developed a series of increasingly sophisticated robotic instruments fo...
We have assembled a team with expertise in astronomical site testing in the Antarctic and expertise ...
At altitudes of up to 4100m, the Domes of the Antarctic plateau provide unique opportunities for gro...
Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, ...
Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, ...
Abstract: We have developed a 350 µm radiometer to perform automated site testing in remote regions ...
The perfect site for astronomical interferometry would be one where the wind speeds throughout the a...
We have developed a 350 mum radiometer to perform automated site testing in remote regions of Antarc...
The height of the atmospheric boundary layer on the Antarctic plateau is of particular interest to m...
The unique advantages for astronomy on the Antarctic plateau are now well established. In particular...
We discuss the site conditions for astronomy at the South Pole and over the Antarctic plateau. We fi...
Hereafter we give a brief history of our contribution to astronomical site testing in Antarctica, at...
The primary limitation to ground based astronomy is the Earth’s atmosphere. The atmosphere above the...
The Antarctic plateau has superb astronomical seeing above a turbulent boundary layer. This layer ha...