{
  "bibcode": "2004GCN..2705....1O",
  "body": "K. Ogura(Kokugakuin Univ.), S. Nishiura (Tokyo Gakugei Univ.)\nM. Isogai(Tokyo Univ.) and  Y. Urata(RIKEN) report:\n\n\" We have imaged the entire HETE-2 error circle (Butler et al.,\nGCN 2701) using Kiso 1.05 m Schmidt telescope with 2kx2k CCD camera\nstarting at 2004 Sep 12.668 UTC. We obtained 3 x 300 sec R-band\nimages.  Each R-band image gives limiting magnitude of R~20 mag. using\nR magnitudes of near USNO_A2.0 stars as photometric references.  We\nfound a source around \"23:57:10 -00:56:42\" (R~19.4 mag.) which is not\nin DSS II images. But, comparing our second image with our third one,\nit seem to move about 4 arcsec in 5 minute. It may be minor\nplanet. Because of our network trouble we cannot access \"MINOR PLANET\nCHECKER\" page now.\"\n\nThis message may be cited.",
  "circularId": 2705,
  "createdOn": 1095061971000,
  "email": "urata@crab.riken.go.jp",
  "subject": "GRB040912 : Kiso Optical follow-up observation",
  "submitter": "Yuji Urata at RIKEN  <urata@crab.riken.go.jp>",
  "eventId": "GRB 040912"
}