GCN Circular 4653
W.-H. Wang, Y. Kakazu (UH-IfA), B. P. Schmidt (ANU), L. L. Cowie (UH-IfA), S. B. Cenko, and D.-S. Moon (Caltech) We have reobserved the field GRB060202 (Fox et al., GCN 4629) with the Wide Field Camera on UKIRT in K-band filter at a mean epoch of approximately 5:45 UT on the February 4th. Our total integration time is 36 min. We still see the faint source reported by Wang et al. (GCN 4638) at roughly the same magnitude (K=20.07 in 3" aperture diameter). We have imaged the same region also with the Low-Resolution Imaging Spectrometer mounted on the 10-m Keck I telescope. Observations consisted of 4 x 150 s images taken in the I-band filter at a mean time about 5:50 UT on February 4th. The faint source (S1) reported by Cenko et al. (GCN 4636) was detected at roughly the same magnitude (I = 22.9 +/- 0.3). Our results suggest that the source S1 is not a GRB afterglow.