  High-energy neutrinos originating in astrophysical sources should be
accompanied by gamma-rays at production. Depending on the properties of the
emission environment and the distance of the source to the Earth, these
gamma-rays may be observed directly, or through the detection of lower energy
photons that result from interactions with the intervening radiation fields. In
this work, we present an automated tool that aims at using data from the
Fermi-Large Area Telescope to identify multiwavelength counterparts to
astrophysical neutrino events. The main goal of this tool is to enable prompt
follow-up observations with ground-based and space-based observatories in order
to help pinpoint the neutrino source.
