We study several quintessence models which are exotic at Q = 0, anduse a simple constraint Q ≥ H/2π to check when they enter the tracking regime,disregarding the details of inflation. We find that it can also give strong constraintsfor V = V0Q-α, which has to enter the tracking regime after lnz ～ 10, while forthe supergravity model V = V0Q-αexp(kQ2/2), the constraint is much weaker. Forthe exponential form of inverse power-law potential V = Voexp(λ/Q), it exhibits noconstraints.
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