Introduction
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Introduction
A key science goal of the ARISE Space VLBI mission is the imaging of cores of gamma-ray blazars on scales of light months or less. This requires observations of moderate-to-high sensitivity at 43 and 86 GHz. In particular, it is desirable to be able to choose from a set of at least 100 detectable sources at 86 GHz. This memo addresses the resulting requirements on the mission sensitivity and the capability for detecting the desired number of sources.
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