Independent Analysis of the Distance to NGC1052-DF2
  The conclusion that the diffuse galaxy NGC1052-DF2 is deficient in dark
matter depends critically on the distance, as noted in the original publication
and subsequent works. The results of our preliminary assessment of the SBF
distance have already been referenced on the web. Here we present the details
of a more careful analysis, supply some context, and comment on the remaining
uncertainty.
