Cross-correlation imaging interferometers designed in the shape of a c
urve of constant width offer better sensitivity and imaging characteri
stics than other designs because they sample the Fourier space of the
image better than other shapes, for example, ''T's'' or ''Y's.'' In a
doss-correlation interferometer each pair of antennas measures one Fou
rier component with a spatial wavenumber proportional to the separatio
n of the pair. Placing the individual antennas of the interferometer a
long a curve of constant width, a curve that has the same diameter in
all directions, guarantees that the spatial resolution of the instrume
nt will be independent of direction because the measured Fourier compo
nents will have the same maximum spatial wavenumber in all directions.
The most uniform sampling within this circular region in Fourier spac
e will be created by the particular symmetric curve of constant width
that has the lowest degree of rotational symmetry or fewest number of
sides, which is the Reuleaux triangle. The constant width curve with t
he highest symmetry, the circle is the least satisfactory although sti
ll considerably better than T's or Y's. In all cases, the sampling can
be further improved by perturbing the antenna locations slightly off
a perfect curve to break down symmetries in the antenna pattern which
cause symmetries and hence nonuniformities in the sampling pattern in
Fourier space. Appropriate patterns of perturbations can be determined
numerically. As a numerical problem, optimizing the sampling in Fouri
er space can be thought of as a generalization of the traveling salesm
an problem to a continuous two-dimensional space. Self-organizing neur
al networks which are effective in solving the traveling salesman prob
lem are also effective in generating optimal interferometer shapes. Th
e Smithsonian Astrophysical Observatory's Submillimeter Array, a cross
-correlation imaging interferometer for astronomy, will be constructed
with a design based on the Reuleaux triangle.