Late-Time Observations of Type Ia Supernova SN 2014J with the Hubble
  Space Telescope Wide Field Camera 3
  Recent works have studied the late-time light curves of Type Ia supernovae
(SNe Ia) when these were older than 500 days past B-band maximum light. Of
these, SN 2014J, which exploded in the nearby galaxy M82, was studied with the
Advanced Camera for Surveys onboard the Hubble Space Telescope (HST) by Yang et
al. Here, I report complementary photometry of SN 2014J taken with the HST Wide
Field Camera 3 when it was ~360-1300 days old. My F555W measurements are
consistent with the F606W measurements of Yang et al., but the F438W
measurements are ~1 mag fainter than their F475W measurements. I corroborate
their finding that even though SN 2014J has spatially resolved light echoes,
its photometry is not contaminated by an unresolved echo. Finally, I compare
the F438W and F555W light curves of SN 2014J to those of the other late-time
SNe Ia observed to date and show that more intrinsically luminous SNe have
slower light-curve decline rates. This is consistent with the correlation
claimed by Graur et al., which was based on a comparison of pseudo-bolometric
light curves. By conducting a direct comparison of the late-time light curves
in the same filters, I remove any systematic uncertainties introduced by the
assumptions that go into constructing the pseudo-bolometric light curves, thus
strengthening the Graur et al. claim.
