From: Gaston Folatelli (gaston@physto.se)
Date: Fri Nov 08 2002 - 10:10:29 PST
We have reduced the four spectra taken at VLT last night. The
flux-calibrated spectra are retrievable in ASCII and FITS format from
http://www.physto.se/~snova/private/2002Arun/2002Arun.html
No definite conclusions can be drawn, it seems. We may want to burn more
on the candidates to be beyond z=1 in order to distinguish better the
wiggles.
Cheers,
The Swedes
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