//////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 616 SUBJECT: GRB000323 [IPN Position] DATE: 00/03/24 23:20:07 GMT FROM: Kevin Hurley at UCBerkeley/SSL K. Hurley, R. M. Kippen, S. Barthelmy, and T. Cline, on behalf of the Ulysses, BATSE, and NEAR GRB teams, report: Ulysses, BATSE, and NEAR observed GRB000323 (BATSE #8049). As observed by Ulysses, this burst had a T90 duration of about 90 s and a 25-100 keV fluence of about 4.3 x 10^-6 erg/cm^2. We have triangulated this burst to a preliminary ~750 sq. arcmin. error box whose coordinates are: RA(2000) DEC(2000) 12 h 51 m 59.81 s 48 o 49 ' 6.46 " (CENTER) 12 h 52 m 48.03 s 48 o 26 ' 56.20 " (CORNER) 12 h 50 m 24.05 s 48 o 46 ' 14.07 " (CORNER) 12 h 53 m 35.73 s 48 o 51 ' 54.67 " (CORNER) 12 h 51 m 10.65 s 49 o 11 ' 19.28 " (CORNER) Only minor refinements to this error box are expected. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 621 SUBJECT: GRB 000323, optical observations DATE: 00/03/28 20:39:47 GMT FROM: Arne A. Henden at USNO/USRA A. Henden (USRA/USNO) on behalf of the USNO GRB team, and A. J. Castro-Tirado, INTA-LAEFF (Madrid) and IAA-CSIC (Granada) and J. M. Castro Ceron, ROA (San Fernando) on behalf of the large Spanish-Czech BOOTES team, report: We have observed the entire error box of GRB 000323 (cf. Hurley et al., GCN#616), using the 0.3-m BOOTES-1 telescope and the USNOFS 1.0-m telescope. The BOOTES-1 data is unfiltered, and covers about 90 percent of the entire error box except for the extreme northern and southern corners. The USNO Cousins R-band data is a north/south mosaic that covers about 60 percent of the error box, missing the east and west corners. The UT exposure dates, length, and limiting magnitudes are: BOOTES-1 2000 March 25.00 1200seconds R=19.5 USNO 2000 March 25.42 600seconds R=21.5 USNO 2000 March 26.31 1200seconds R=22.2 The BOOTES-1 frame does not go as deep as the POSS-II red plate, but no new object is apparent from comparing the CCD data with POSS-II. The USNO datasets go somewhat deeper than POSS-II, but no variable object is detected brighter than R=21.5. A BVRI single-night calibration of the central part of the error box, taken on a photometric night in conjunction with a large number of Landolt standards, can be found at ftp://ftp.nofs.navy.mil/pub/outgoing/aah/grb/grb000323.dat