{
  "bibcode": "2003GCN..1835....1B",
  "body": "F. Bertoldi (MPIfR Bonn), D.A. Frail (NRAO), E. Berger (Caltech),\nK.M. Menten (MPIfR Bonn), S. Kulkarni (Caltech) report:\n\nThe infrared afterglow candidate to GRB 030115 (GCN 1816, 1818) was observed\nat 250 GHz (1.2 mm) with the 117-channel Max-Planck Millimeter\nBolometer (MAMBO) array at the IRAM 30 m telescope on Pico Veleta\n(Spain).\n\nTwo observations of 20 minutes each were made starting 2003 January 16,\n1:50 UT (22.5 hours after the burst), and January 18, 7:30 UT,\nunder good and moderate conditions, respectively. The integrated flux\ndensities derived from these observations are \n\n  2003 Jan 16.08 UT    0.4 +- 0.9 mJy\n  2003 Jan 18.31 UT    2.9 +- 1.6 mJy\n\nA 3-sigma 250 GHz upper flux limit of ~ 3 mJy and 5 mJy is thus\nestablished for the respective epochs.",
  "circularId": 1835,
  "createdOn": 1043892323000,
  "email": "bertoldi@mpifr-bonn.mpg.de",
  "subject": "GRB030115: 1.2 mm upper limits with MAMBO @ IRAM 30m",
  "submitter": "Frank Bertoldi at MPIFR/Bonn  <bertoldi@mpifr-bonn.mpg.de>",
  "eventId": "GRB 030115"
}