BB Main Page - CRAL-wiki

Main Page

From CRAL-wiki

(Difference between revisions)
Jump to: navigation, search
(Cahill Radio Astronomy Lab Wiki)
(Cahill Radio Astronomy Lab Wiki)
Line 6: Line 6:
|-valign="top"
|-valign="top"
|width="300pt"|'''RADIO PROJECTS'''
|width="300pt"|'''RADIO PROJECTS'''
-
*[http://www.stanford.edu/group/church_group/cgi-bin/ATI_wiki/index.php/Argus ARGUS] A 16-element dual-pol W-band spectroscopic receiver array for GBT ([[ARGUS_local local]]).
+
*[http://www.stanford.edu/group/church_group/cgi-bin/ATI_wiki/index.php/Argus ARGUS] A 16-element dual-pol W-band spectroscopic receiver array for GBT (local ARGUS pages).
*[http://astrowiki.physics.ox.ac.uk/CBass/WebHome CBASS] A 5 GHz all-sky survey.
*[http://astrowiki.physics.ox.ac.uk/CBass/WebHome CBASS] A 5 GHz all-sky survey.
*[[KISS]] Improving HEMT amplifiers for radio astronomy.
*[[KISS]] Improving HEMT amplifiers for radio astronomy.

Revision as of 23:36, 25 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 (local ARGUS pages).
  • 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
Personal tools