TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1263 SUBJECT: IPN triangulation of GRB020305 (HETE 1939) DATE: 02/03/06 19:01:57 GMT FROM: Kevin Hurley at UCBerkeley/SSL K. Hurley and T. Cline, on behalf of the Ulysses and HETE GRB teams; G. Ricker, D. Lamb, and S. Woosley on behalf of the HETE Science Team; R. Vanderspek, G. Crew, J. Doty, G. Monnelly, J. Villasenor, N. Butler, T. Cline, J.G. Jernigan, A. Levine, F. Martel, E. Morgan, G. Prigozhin, J. Braga, R. Manchanda, and G. Pizzichini, on behalf of the HETE Operations and HETE Optical-SXC Teams; N. Kawai, M. Matsuoka, Y. Shirasaki, T. Tamagawa, K. Torii, T. Sakamoto, A. Yoshida, E. Fenimore, M. Galassi, T. Donaghy, C. Graziani, and T. Tavenner, on behalf of the HETE WXM Team; J-L Atteia, M. Boer, J-F Olive, P. Lestrade, and J-P Dezalay, on behalf of the HETE FREGATE Team; report: Ulysses observed GRB020305 (=H1939). As observed by both Ulysses and FREGATE, this event consists of two distinct episodes of emission separated by an ~ 200 s long quiescent period, raising the question of whether both episodes are from the same source. As the Ulysses and FREGATE time histories are identical to within statistics, we conclude that both episodes indeed had the same origin, and that the duration of this event is therefore ~280 s. As observed by Ulysses, the 25-100 keV fluence and peak flux over 0.5 s are ~7x10^-6 erg cm^-2 and 4.7 x 10^-7 erg cm^-2 s^-1. Triangulation using the FREGATE data gives an annulus centered at RA(2000)= 71.966 deg., Decl.(2000)= -81.411 deg., with radius 79.798 +/- 0.180 deg. (3 sigma). The center line of this annulus passes ~0.1 degrees from the center of the HETE WXM error circle, and the annulus intersects the error circle at: RA(2000) Dec(2000) 191.118 -14.317 190.483 -14.235 191.169 -14.687 190.332 -14.578 The combined annulus/error circle has an area approximately 2.4 times smaller than the error circle alone, or approximately 800 square arcminutes. A plot has been posted at ssl.berkeley.edu/ipn3/020305.