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TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2229 SUBJECT: IPN triangulation of GRB030514 (annulus) DATE: 03/05/15 16:14:06 GMT FROM: Kevin Hurley at UCBerkeley/SSL <khurley@sunspot.ssl.berkeley.edu> K. Hurley, on behalf of the Ulysses GRB team, E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team, A. von Kienlin, G. Lichti, and A. Rau, on behalf of the INTEGRAL SPI-ACS GRB team, and T. Cline, on behalf of the Ulysses and Konus GRB teams, report: Ulysses, Konus-Wind, and INTEGRAL (SPI-ACS) observed this GRB at 66151 seconds. As observed by Ulysses, it had a duration of approximately 10 seconds, a 25-100 keV fluence of approximately 6.7E-06 erg/cm2, and a peak flux of approximately 5.1E-07 erg/cm2 s over 0.50 seconds. We have triangulated it to a preliminary annulus centered at RA, Decl(2000)= 151.734, 35.758 degrees, whose radius is 67.870 +/- 0.264 degrees (3 sigma). In addition, the Konus ecliptic latitude response limits the arrival directions to those portions of the annulus between RA, Decl = 94, -6.6 degrees and 172, -29.5 degrees. This annulus can be constrained and/or improved further, but as the event was not observed by Mars Odyssey, a small error box cannot be derived for it.
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