  Numerous extended sources around Galactic pulsars have shown significant
$\gamma$-ray emission from GeV to TeV energies, revealing hundreds of TeV
energy electrons scattering off of the underlying photon fields through inverse
Compton scattering (ICS). HAWC TeV gamma-ray observations of few-degree
extended emission around the pulsars Geminga and Monogem, and LAT GeV emission
around Geminga, suggest that systems older than 100 kyr have multi-TeV $e^\pm$
propagating beyond the SNR-PWN system into the interstellar medium. Following
the discovery of few $\gamma$-ray sources by HAWC at energies E$>100$~TeV, we
investigate the presence of an extended $\gamma$-ray emission in Fermi-LAT data
around the three brightest sources detected by HAWC up to 100 TeV. We find an
extended emission of $\theta_{68} = 1.00^{+0.05}_{-0.07}$ deg around eHWC
J1825-134 and $\theta_{68} = 0.71\pm0.10$ deg eHWC J1907+063. The analysis with
ICS templates on Fermi-LAT data point to diffusion coefficient values which are
significantly lower than the average Galactic one. When studied along with HAWC
data, the $\gamma$-ray Fermi-LAT data provide invaluable insight into the very
high-energy electron and positron parent populations.
