The SPTpol camera is a dichroic polarimetric receiver at 90 and 150 GHz. Deployed in January 2012 on the South Pole Telescope (SPT), SPTpol is looking for faint polarization signals in the Cosmic Microwave Background (CMB). The camera consists of 180 individual Transition Edge Sensor (TES) polarimeters at 90 GHz and seven 84-polarimeter camera modules (a total of 588 polarimeters) at 150 GHz. We present the design, dark characterization, and in-lab optical properties of the 150 GHz camera modules. The modules consist of photolithographed arrays of TES polarimeters coupled to silicon platelet arrays of corrugated feedhorns, both of which are fabricated at NIST-Boulder. In addition to mounting hardware and RF shielding, each module also conta...
Next generation cosmic microwave background (CMB) polarization anisotropy measurements will feature ...
We describe 280 GHz bolometric detector arrays that instrument the balloon-borne polarimeter SPIDER....
Abstract Multi-chroic polarization sensitive detectors offer an avenue to increase both the spectral...
The SPTpol camera is a dichroic polarimetric receiver at 90 and 150 GHz. Deployed in January 2012 on...
The SPTpol camera is a dichroic polarimetric receiver at 90 and 150 GHz. Deployed in January 2012 on...
The SPTpol camera is a two-color, polarization-sensitive bolometer receiver, and was installed on th...
The SPTpol camera is a two-color, polarization-sensitive bolometer receiver, and was installed on th...
In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camer...
We present information about the design and fabrication of 90 GHz Transition Edge Sensor (TES) detec...
In 2012 the South Pole Telescope (SPT) will begin a 625 deg^2 survey to measure the polarization ani...
SPTpol is a dual-frequency polarization-sensitive camera that was deployed on the 10-meter South Pol...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
We have developed a 16-element, 97GHz, lownoise Transition Edge Sensor (TES) module that can be pack...
We have developed a 16-element, 97GHz, lownoise Transition Edge Sensor (TES) module that can be pack...
Next generation cosmic microwave background (CMB) polarization anisotropy measurements will feature ...
We describe 280 GHz bolometric detector arrays that instrument the balloon-borne polarimeter SPIDER....
Abstract Multi-chroic polarization sensitive detectors offer an avenue to increase both the spectral...
The SPTpol camera is a dichroic polarimetric receiver at 90 and 150 GHz. Deployed in January 2012 on...
The SPTpol camera is a dichroic polarimetric receiver at 90 and 150 GHz. Deployed in January 2012 on...
The SPTpol camera is a two-color, polarization-sensitive bolometer receiver, and was installed on th...
The SPTpol camera is a two-color, polarization-sensitive bolometer receiver, and was installed on th...
In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camer...
We present information about the design and fabrication of 90 GHz Transition Edge Sensor (TES) detec...
In 2012 the South Pole Telescope (SPT) will begin a 625 deg^2 survey to measure the polarization ani...
SPTpol is a dual-frequency polarization-sensitive camera that was deployed on the 10-meter South Pol...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
We have developed a 16-element, 97GHz, lownoise Transition Edge Sensor (TES) module that can be pack...
We have developed a 16-element, 97GHz, lownoise Transition Edge Sensor (TES) module that can be pack...
Next generation cosmic microwave background (CMB) polarization anisotropy measurements will feature ...
We describe 280 GHz bolometric detector arrays that instrument the balloon-borne polarimeter SPIDER....
Abstract Multi-chroic polarization sensitive detectors offer an avenue to increase both the spectral...