  We report the discovery of the isolated neutron star (INS) candidates eRASSU
J065715.3+260428 and eRASSU J131716.9-402647 from the Spectrum Roentgen Gamma
(SRG) eROSITA All-Sky Survey. Selected for their soft X-ray emission and
absence of catalogued counterparts, both objects were recently targeted with
the Large Binocular Telescope and the Southern African Large Telescope. The
absence of counterparts down to deep optical limits (25 mag, 5$\sigma$) and, as
a result, large X-ray-to-optical flux ratios in both cases strongly suggest an
INS nature. The X-ray spectra of both sources are well described by a simple
absorbed blackbody, whereas other thermal and non-thermal models (e.g. a
hot-plasma emission spectrum or power law) are disfavoured by the spectral
analysis. Within the current observational limits, and as expected for cooling
INSs, no significant variation ($>2\sigma$) has been identified over the first
two-year time span of the survey. Upcoming dedicated follow-up observations
will help us to confirm the candidates' nature.
