Abstract
We test the parallaxes reported in the Gaia first data release using the
sample of eclipsing binaries with accurate, empirical distances from Stassun &
Torres (2016). We find a clear average offset of $-$0.25$\pm$0.05 mas in the
sense of the Gaia parallaxes being too small (i.e., the distances too long).
The documented Gaia systematic uncertainty is 0.3 mas, which the eclipsing
binary sample corroborates. The offset does not depend strongly on obvious
parameters such as color, brightness, or spatial position. However, with a
statistical significance of 99.7%, nearer stars possibly exhibit larger offsets
according to $\Delta-0.16 -0.02 \pi$ mas.
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