GCN Circular 4897
N.R. Tanvir (U. Hertfordshire), E. Rol (U. Leicester), K. Wiersema, R. Starling (U. Amsterdam) and N. O'Mahoney (ING) report on behalf of a larger collaboration: We observed the field of GRB 060319 with WHT/LIRIS. A 10 min K-band exposure was made beginning at Mar 19 06.38 UT (ie. approximately 5.4 hours post-burst). A faint source is visible within the XRT error circle reported by Beardmore et al. (GCN 4895). The coordinates of the source are (relative to DSS system) approximately: 11 45 33.5 +60 00 39.0 (J2000) The magnitude relative to two nearby 2MASS stars is K=19.0+-0.3. It is not possible to tell whether the source is constant or variable.