  We propose accurate calculations of quasinormal modes of black holes in the
Einstein-aether theory, which were previously considered in the literature,
partially, with insufficient accuracy. We also show that the arbitrarily
long-lived modes, quasiresonances, are allowed in the Einstein-aether theory as
well and demonstrate that the asymptotic tails, unlike quasinormal frequencies,
are indistinguishable from those in the Einstein theory.
