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We correct a sign in the first variation of the on-shell action ofcosmological topologically massive gravity at the chiral point and present thethree equations affected by that sign. While this does not change any of themain conclusions of arXiv:0805.2610, it modifies the finite part of theBrown-York stress tensor. Our corrected Brown-York stress tensor is stillfinite, conserved and traceless, but no longer coincides with that of globalAdS_3. It agrees with results found in recent literature.

Erratum to `Instability in cosmological topologically massive gravity at the chiral point', arXiv:0805.2610