{
  "bibcode": "2000GCN...862....1P",
  "body": "P.A. Price (Caltech), O. Pevunova, B. Madore (IPAC) and S.G. Djorgovski\n(Caltech) report on behalf of a larger collaboration:\n\n\"We have observed the afterglow candidate of GRB001007 (Price et al.,\nGCN #843, Frail & Berger, GCN #860) with the Palomar 60-inch telescope\nwith 4x900s exposures starting at Oct 25.34 UT.  We do not detect\nthe candidate to a limiting magnitude of R = 21.6 (based on the\nreference star from GCN #843, for 50% automated detection of artificial\nstars in the field).  The derived temporal decay slope between our two\nepochs (Oct 10.69 and Oct 25.34) is alpha > 1.9 .\"\n\nThis message may be cited.",
  "circularId": 862,
  "createdOn": 972509428000,
  "email": "pap@srl.caltech.edu",
  "subject": "GRB001007: Optical observations",
  "submitter": "Paul Price at RSAA, ANU at CIT  <pap@srl.caltech.edu>",
  "eventId": "GRB 001007"
}