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Penn Array Receiver


1. Scope

The Penn Array Receiver is a 64-pixel continuum imaging system for the 3mm band. The project is a collaboration of the University of Pennsylvania, NASA-Goddard Space Flight Center and the NRAO. The project is being funded through NRAO’s university-built instrumentation program. The project was formally initiated in the first quarter of 2002 with the signing of a memorandum of agreement between NRAO and Upenn. The NRAO is providing instrument machining services, control software and the interface to GBT systems, and data analysis software. The Penn Array Receiver will be designed as a facility instrument, accessible to all GBT Users. The Critical Design Review is expected to be held in Fall 2003, and scheduled delivery is in early 2005. More details on the PAR are available from Brian Mason’s GBT High Frequency Instrumentation Development web page. The PAR is being funded through NRAO’s university-built instrumentation program.

2. Strategic Value

The Penn Array receiver will be the first major new mm wave capability on the GBT, and will have significant scientific impacts on a wide range of fields such as the study of high redshift galaxies, the Sunyaev-Zel'dovich Effect, and star formation in our Galaxy.

3. Personnel

The following refers to GBT contact staff, not actual instrument builders.

6. Resource Requests for Cycle 1 2006

7. Project Artifacts

8. Random Notes, Links &c.

-- BrianMason - 26 Sep 2003

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