GCN Circular 5461
A.J. Levan (U. Hertfordshire), E. Rol, N.R. Tanvir (U. Leicester), A. Fruchter (STScI), J. Rhoads (ASU), C. Davis, A. Adamson (JAC) report for a larger collaboration: We obtained a second epoch of K-band observations of GRB 060814 at UKIRT beginining at August 16, 06:46 UT. The suggested IR afterglow (GCN Circ 5455) is still detected and has faded by 0.4 +/- 0.1 mags, confirming its association with GRB 060814. The afterglow decay is very slow, with alpha~0.25. This may well represent a signficant contribution from an underlying host galaxy (see GCN Circs 5456 & 5457).