From: Serena Nobili (serena@physto.se)
Date: Mon May 24 2004 - 09:18:11 PDT
Hi Peter,
thank you, that was in fact the problem.
Would it be possible to have the most recent version of the code?
Cheers
Serena
On Mon, 24 May 2004, Peter Nugent wrote:
>
>Hi Serena,
>
>Yes, I do not use that code anymore for modifying the templates. I think
>it won't work because the spectra are different sizes now (they run from
>0.1 - 2.5 instead of 0.25 - 1.0 microns with the same 10ang spacing). I
>adopted a more general technique along the lines of the splines that Rob
>talked about before, which also includes several arbitrary UV filters to
>keep that region in check.
>
>This simplest way you could use the previous version is to hack the new
>template to the same length as the one before.
>
>Cheers,
>
>Peter
>
>__
>Peter E. Nugent
>Staff Computational Scientist - Scientific Computing Group - NERSC
>Lawrence Berkeley National Laboratory
>M.S. 50F-1650 - 1 Cyclotron Road - Berkeley, CA, 94720-8139
>Phone:(510) 486-6942 - Fax:(510) 486-5812
>E-mail: penugent@LBL.gov - Web: http://supernova.LBL.gov/~nugent
>
>
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