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The WXM localization is a long, narrow strip because the burst occurred at the edge of the WXM FOV in a region of the sky that would have been viewed by the YB-camera ...
... and the sky map can be found should read, http://astro.uchicago.edu/home/web/lamb/candidate_optical_afterglow.jpg and http://astro.uchicago.edu/home/web/lamb/wxm_loc_and ...
... Network reports: Total of five 24 x 16 arcmin fields covering most of the HETE WXM ... at August 24, 2003 20:40 UT, 4.0 hours after the inital burst under varying sky ...
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