In 1932 John S. Hall, a
graduate student at Yale, built a caesium-oxide photoelectric photometer giving
an effective wavelength of about 8000.With this he observed the Cepheid zeta Gem. Later Dr. A. L. Bennett used
the same equipment to observe many variables. His light curves for only AO Cas,
S Sge, and RT Aur were published. When Bennett was called for war work by the
Navy he left behind observations on 30 long period variables and a few others
of short period. As he did not return to astronomy after the war this wealth of
observations has never been published.