  A handedness in the arrival directions of high-energy photons from outside
our Galaxy can be related to the helicity of an intergalactic magnetic field.
Previous estimates by arXiv:1310.4826 and arXiv:1412.3171 showed a hint of a
signal present in the photons observed by the Fermi Large Area Telescope (LAT).
An update on the measurement of handedness in Fermi-LAT data is presented using
more than 10 years of observations. Simulations are performed to study the
uncertainty of the measurements, taking into account the structure of the
exposure caused by the energy-dependent instrument response and its observing
profile, as well as the background from the interstellar medium. The
simulations are required to accurately estimate the uncertainty and to show
that previously the uncertainty was significantly underestimated. The apparent
signal in the earlier analysis of {\em Fermi}-LAT data is rendered
non-significant.
