Exploring the nature and synchronicity of early cluster formation in the
  Large Magellanic Cloud V: Multiple Populations in ancient Globular Clusters
  We examine four ancient Large Magellanic Cloud (LMC) globular clusters (GCs)
for evidence of multiple stellar populations using the Advanced Camera for
Surveys and Wide Field Camera 3 on the Hubble Space Telescope Programme
GO-14164. NGC 1466, NGC 1841, and NGC 2257 all show evidence for a redder,
secondary population along the main-sequence. Reticulum does not show evidence
for the presence of a redder population, but this GC has the least number of
stars and Monte Carlo simulations indicate that the sample of main sequence
stars is too small to robustly infer whether a redder population exists in this
cluster. The second, redder, population of the other three clusters constitutes
$\sim30-40\%$ of the total population along the main-sequence. This brings the
total number of ancient LMC GCs with known split or broadened main-sequences to
five. However, unlike for Hodge 11 and NGC 2210 (see arXiv:1904.01434), none of
the clusters show evidence for multiple populations in the horizontal branch.
We also do not find evidence of a second population along the Red Giant Branch
(RGB).
