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(Cahill Radio Astronomy Lab Wiki)
(Cahill Radio Astronomy Lab Wiki)
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*[[KISS]] Improving HEMT amplifiers for radio astronomy.
*[[KISS]] Improving HEMT amplifiers for radio astronomy.
*[[KuPOL]] A new Ku-band correlation receiver for the OVRO 40m.
*[[KuPOL]] A new Ku-band correlation receiver for the OVRO 40m.
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*[http://www.stanford.edu/group/church_group/cgi-bin/ATI_wiki/index.php/Main_Page MASII]  
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*[http://www.stanford.edu/group/church_group/cgi-bin/ATI_wiki/index.php/Main_Page MASII] Prototype 'arrayable' W-band spectroscopic front ends.
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*[https://cmb.uchicago.edu/project/index.php/Module_Development_Program QUIET MDP]  
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*[https://cmb.uchicago.edu/project/index.php/Module_Development_Program QUIET MDP] Next generation polarimeter modules for B-mode polarization.
|width="300pt"|'''DIGITAL PROJECTS'''
|width="300pt"|'''DIGITAL PROJECTS'''
* [[CARMA correlator upgrade]]
* [[CARMA correlator upgrade]]

Revision as of 19:53, 4 June 2012

InP WaferOVRO 40mQUIET LNA sectionDigital receiverCryoprobe chuck

Cahill Radio Astronomy Lab Wiki

RADIO PROJECTS
  • ARGUS A 16-element dual-pol W-band spectroscopic receiver array for GBT.
  • CBASS A 5 GHz all-sky survey.
  • KISS Improving HEMT amplifiers for radio astronomy.
  • KuPOL A new Ku-band correlation receiver for the OVRO 40m.
  • MASII Prototype 'arrayable' W-band spectroscopic front ends.
  • QUIET MDP Next generation polarimeter modules for B-mode polarization.
DIGITAL PROJECTS MEETINGS
OVRO-CAMPUS TECHNICAL DEVELOPMENT LAB USING THE WIKI
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