{
  "bibcode": "2006GCN..4653....1W",
  "body": "W.-H. Wang, Y. Kakazu (UH-IfA), B. P. Schmidt (ANU), \nL. L. Cowie (UH-IfA), S. B. Cenko, and D.-S. Moon (Caltech)\n\n\n   We have reobserved the field GRB060202 (Fox et al., GCN 4629) with \nthe Wide Field Camera on UKIRT in K-band filter at a mean epoch of \napproximately 5:45 UT on the February 4th.\nOur total integration time is 36 min.\n\nWe still see the faint source reported by Wang et al. (GCN 4638)\nat roughly the same magnitude (K=20.07 in 3\" aperture diameter).\n\n\n   We have imaged the same region also with the Low-Resolution \nImaging Spectrometer mounted on the 10-m Keck I telescope.\nObservations consisted of 4 x 150 s images taken in the I-band filter\nat a mean time about 5:50 UT on February 4th.\n\nThe faint source (S1) reported by Cenko et al. (GCN 4636) was detected \nat roughly the same magnitude (I = 22.9 +/- 0.3).\n\n\n  Our results suggest that the source S1 is not a GRB afterglow.",
  "circularId": 4653,
  "createdOn": 1139048835000,
  "email": "kakazu@ifa.hawaii.edu",
  "subject": "GRB 060202: UKIRT/WFCAM K-band and KeckI/LRIS I-band Observation",
  "submitter": "Yuko Kakazu at U of Hawaii/Inst. for Astro.  <kakazu@ifa.hawaii.edu>",
  "eventId": "GRB 060202"
}