  We construct Tully-Fisher relations (TFRs), from large samples of galaxies
with spatially-resolved H$\alpha$ emission maps from the K-band Multi-Object
Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at $z\approx1$.
We compare these to data from the Sydney-Australian-Astronomical-Observatory
Multi-object Integral-Field Spectrograph (SAMI) Galaxy Survey at $z\approx0$.
We stringently match the data quality of the latter to the former, and apply
identical analysis methods and sub-sample selection criteria to both to conduct
a direct comparison of the absolute $K$-band magnitude and stellar mass TFRs at
$z\approx1$ and $z\approx0$. We find that matching the quality of the SAMI data
to that of KROSS results in TFRs that differ significantly in slope, zero-point
and (sometimes) scatter in comparison to the corresponding original SAMI
relations. These differences are in every case as large or larger than the
differences between the KROSS $z\approx1$ and matched SAMI $z\approx0$
relations. Accounting for these differences, we compare the TFRs at $z\approx1$
and $z\approx0$. For disk-like, star-forming galaxies we find no significant
difference in the TFR zero-points between the two epochs. This suggests the
growth of stellar mass and dark matter in these types of galaxies is intimately
linked over this $\approx8$ Gyr period.
