  We present a complete phenomenological prospectus for thermal relic
neutralinos. Including Sommerfeld enhancements to relic abundance and halo
annihilation calculations, we obtain direct, indirect, and collider discovery
prospects for all neutralinos with mass parameters $M_1,M_2,|\mu| < 4$ TeV,
that freeze out to the observed dark matter abundance, with scalar
superpartners decoupled. Much of the relic neutralino sector will be uncovered
by the direct detection experiments Xenon1T and LZ, as well as indirect
detection with CTA. We emphasize that thermal relic higgsinos will be found by
next-generation direct detection experiments, so long as $M_{1,2} < 4$ TeV.
Charged tracks at a 100 TeV hadron collider complement indirect searches for
relic winos. Thermal relic bino-winos still evade all planned experiments,
including disappearing charged-track searches. However, they can be discovered
by compressed electroweakino searches at a 100 TeV collider, completing the
full coverage of the relic neutralino surface.
