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A. Smette (NOAO/NASA-GSFC), T. R. Gull (NASA/GSFC), M. S. Sahu (NOAO/NASA-GSFC)
We present STIS--CCD spectra covering the range 2100-3100Å\ for both A&B images of the gravitational lens candidate UM~425. Although the spectrum of B has a low S/N ratio, we detect Broad Absorption Lines which confirms the lens nature of the system. We discuss the implications for the modelling of the lens.
The author(s) of this abstract have provided an email address for comments about the abstract: asmette@band3.gsfc.nasa.gov