We observed this target with EUVE for 580 ksec in June and July 1997. The target
was easily detected in the DSS. This immer portion of the
DSS image subtends 39 arcmin on the sky;
this represents only the first 195 ksec of the observation. The three-lobed
structure is an instrumental effect.
As expected, the dispersed spectrum is weak,
and we are still working on the optimal spectral extraction.
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