From: Gaston Folatelli (gaston@physto.se)
Date: Tue Nov 12 2002 - 06:09:59 PST
We have tried the infrared technique for sky subtraction on SuF02_081 but
our result is not any better than what we've got yesterday. We probably
ought to refine our implementation.
Looking at the spectrum we notice that, under the hypothesis that the
galaxy line is [OIII] 5007, the redshift would be 0.85 -which makes more
sense if we consider the discovery magnitude of this object- and the match
to a SN+galaxy wouldn't be worse than that at z=1.48. The prominent
feature we see at 7450 would land on 4000AA restframe, where a Ia at max
would peak. The other dips that are less noticiable are in agreement with
that redshift.
Gastón
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