A photometric system
consisting of three near-infrared interference filters and designed for studies
of red variable stars is described.It represents a simplification of the writer's eight-color system of
classification photometry and is intended for use with small telescopes and
inexpensive instrumentation. The three filters measure an infrared magnitude, a
color index, and an index of TiO band strength, which indicates the spectral
type.Measurements on this system
should provide a valuable supplement to the visual light curves of red variable
stars.A set of standard stars is
given which will enable observers to reduce their measurements to a system of
absolute fluxes.A procedure is
described for deriving an index of TiO strength from the data and converting it
to spectral type.