{
  "body": "F. Mannucci (CAISMI, CNR, Firenze), V. Calamai (INAF, Oss. Astrofisico di\nArcetri), E. Palazzi, N.  Masetti (ITeSRE, CNR, Bologna), E. Pian (INAF,\nAstr. Obs. Trieste), P. Saracco (INAF, Astr. Obs.  Brera), A. Antonelli\n(INAF, Astr. Obs. Rome), on behalf of a larger collaboration,\n\nreport:\n\nWe imaged the field of XRF011030 (GCN 1118) with TIRGO equipped with the\nnear-IR camera ARNICA and the J and K filters on Oct 30, 18:15 - 21:22 UT.\nThe PSF FWHM was about 2.0\".  A standard star for flux calibration is\navailable in the K band only; the J band image was calibrated instead by\nusing an average zero point. No source is detected at the position of the\nradio transient reported by Taylor et al. (GCN 1136), nor in the Chandra\nerror box of the X-ray source detected by Harrison et al. (GCN 1143) to\n5-sigma limiting magnitudes of J=19.8 and K=18.0.\n\nThis message may be cited.",
  "eventId": "XRF 011030",
  "version": 2,
  "createdOn": 1006352754000,
  "subject": "XRF011030: J and K band observations",
  "email": "pian@tesre.bo.cnr.it",
  "bibcode": "2001GCN..1145....1M",
  "circularId": 1145,
  "editedOn": 1777052377511,
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov>",
  "submitter": "Elena Pian at ITESRE-CNR,Bologna  <pian@tesre.bo.cnr.it>"
}