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A well-instrumented Green Bank Telescope (GBT) operating at high frequencyrepresents a unique scientific resource for the US community. As afilled-aperture, 100m-diameter telescope, the GBT is ideally suited to fastmapping of extended, low surface brightness emission with excellentinstantaneous frequency coverage. This capability makes the GBT a key facilityfor a range of cutting edge science described in this document, only possibleat these frequencies. We note that the ability to perform the necessaryobservations is unique and highly complementary to the capabilities offered byinterferometers, and should be preserved. We argue that rather than divestingfrom this exceptional resource, it makes sense for the US community to investmoderately to maintain GBT operations and to instrument it in an optimalmanner, enabling it to become an extraordinary complement to existing andfuture radio interferometers. Adequately instrumented, the GBT would be apillar for 20-115 GHz science in the US and the world.

The Case for a Publicly Available, Well-Instrumented GBT Operating at 20-115 GHz