In November of last year, a collaborative effort involving representatives of the Academia Sinica Institute of Astronomy and Astrophysics, University of Wisconsin, NRAO, and the Green Bank Observatory gathered to review designs for a proposed
focal plane array for the GBT.
In addition to transitioning to a separate organization, we have two new high frequency instruments coming online this winter — MUSTANG2, a 70 - 105 GHz, 210 element bolometer array, and ARGUS, a 75 - 116 GHz, 16 element
focal plane array.
This new look at the galaxy was obtained with Argus, a 16 - pixel
focal plane array on the Green Bank Telescope.
Argus is a new 16 - element 75 - 116 GHz
focal plane array instrument installed on the GBT.
Not exact matches
The L - band cryogenic Phased
Array Feed (PAF) receiver, with nineteen dual - polarization crossed dipoles located in the
focal plane of a reflector antenna, was commissioned on the GBT in March 2017.