{
  "bibcode": "2003GCN..1968....1W",
  "body": "W. M. Wood-Vasey (LBNL/UCB), P. A. Price (RSAA/ANU), and D. Fox\n(Caltech), using images obtained by R. Bambery, S. Pravdo, M. Hicks,\nand K. Lawrence (Near-Earth Asteroid Tracking project, Jet Propulsion\nLaboratory), report that an image taken with the Palomar 1.2-m\ntelescope on 2003 Mar 24.27 UT shows the optical transient of Gilmore\net. al (GCN #1949) at a unfiltered magnitude of 18.83 +0.09-0.08.  Two\nprevious Mar 24 images taken under poor conditions do not show the OT:\n \nUT Date            Unfiltered Mag             \n---------------------------------------- \n2003 Mar 24.19   [ 16.59                 \n2003 Mar 24.23   [ 16.26                 \n2003 Mar 24.27     18.83  +0.09  -0.08   \n \nMagnitudes are calibration against >300 USNO-A V1.0 R-band stars in\nthe 0.25 sq. degree field of the images.  We clarify here that the\nlimiting magnitudes quoted in GCN #1957 were calculated in the same\nmanner.\n \nThis message may be cited.",
  "circularId": 1968,
  "createdOn": 1048790144000,
  "email": "wmwood-vasey@lbl.gov",
  "subject": "GRB030323: Detection on 2003/03/24",
  "submitter": "Michael Wood-Vasey at UC Berkeley/LBNL/SNfactory  <wmwood-vasey@lbl.gov>",
  "eventId": "GRB 030323"
}