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The positions of the two error boxes for the soft gamma repeater (SGR) 1900]14 were determined by the "" network synthesis ÏÏ method, which employs observations by the Ulysses gamma-ray burst and CGRO BATSE instruments. The location of the Ðrst error box has been observed at optical, infrared, and X-ray wavelengths, resulting in the discovery of a ROSAT X-ray point source and a curious double infrared source. We have recently used the ROSAT HRI to observe the second error box to complete thedoi:10.1086/304910 fatcat:wwrj2et5rrbnfirrtvddzx5ufe