  We report the discovery of two directly imaged, giant planet candidates
orbiting the metal-rich DAZ white dwarfs WD 1202-232 and WD 2105-82. JWST's
Mid-Infrared Instrument (MIRI) data on these two stars show a nearby resolved
source at a projected separation of 11.47 and 34.62 au, respectively. Assuming
the planets formed at the same time as their host stars, with total ages of 5.3
and 1.6Gyr, the MIRI photometry is consistent with giant planets with masses
about 1-7 Jupiter Masses. The probability of both candidates being false
positives due to red background sources is approximately 1 in 3000. If
confirmed, these would be the first directly imaged planets that are similar in
both age and separation to the giant planets in our own solar system, and they
would demonstrate that widely separated giant planets like Jupiter survive
stellar evolution. Giant planet perturbers are widely used to explain the tidal
disruption of asteroids around metal-polluted white dwarfs. Confirmation of
these two planet candidates with future MIRI imaging would provide evidence
that directly links giant planets to metal pollution in white dwarf stars.
