  Masses of galaxies are beginning to be measured systematically at redshifts z
> 0.3. Such data provide powerful and unique links and clues to theories,
simulations, and our understanding of early galaxy formation and evolution.
Discriminating masses of different kinds (e.g., dark matter, old stars, HI gas)
remains difficult, but a wide variety of techniques for measuring total
dynamical masses are being explored and found practical. I highlight three
recent optical studies of dynamical masses: 1) the emission line velocity
widths of blue galaxies and rotation curves of spirals that trace evolution in
the Tully-Fisher relation to z ~ 1; 2) the absorption line velocity dispersions
of early type galaxies in the field and clusters to track evolution in the
Fundamental Plane to z ~ 0.85; and 3) the kinematics of high redshift (z ~ 3)
Lyman-drop galaxies to constrain their nature, descendents, and progenitors.
The next decade shows promise of an explosive growth in this infant field of
measuring masses, especially in having much larger sample sizes, higher
precision and S/N, improved techniques and tools, and probes of more diverse
kinds of mass.
