  An exoplanet's optical phase curve constrains the thermal emission and albedo
of the planet's surface and/or atmosphere, as well as potentially constraining
the mass via gravitational influences on the host star. Recently, Jansen &
Kipping (2018) demonstrated that exoplanets with precisely constrained orbital
periods, as is typical of transiting planets, enable one to exploit a
Fourier-argument to non-parametrically separate optical phase curves from
long-term photometric time series in the presence of realistic noise
structures. This algorithm, dubbed phasma, was applied to 477 confirmed
exoplanets in the original paper. In this research note, we extend the sample
to all non-false positive Kepler Objects of Interest with periods less than ten
days. Our sample of 1998 detrended phase curves are made publicly available to
help the community search for various effects. A Python port of the phasma code
is also made available.
