From: Peter Nugent (nugent@lbl.gov)
Date: Wed Mar 10 2004 - 05:46:21 PST
> When Peter did it, I believe he did it as a function of t rather than
> t/(1-s). Is this right Peter?
>
> My belief is that the differences will be smaller if you do
> K-corrections as t/(1-s) rather than as t. (I think Serena came to the
> same conclusion.)
I did it both ways, but t/(1+s) had smaller dispersion (I think we have
the plus sign there)
> As such, the 0.2 may be larger than even the "biggest reasonable case"
> systematic uncertainty.
This 0.2 was only for I-to-I corrections where the CaII IR triplet
dominates the entire bandpass. I have found 3 SNe (out of perhaps 20) that
have problems on this magnitude. In general it is much less (<< 0.05). It
is the fact that one feature dominates the bandpass that can cause havoc
and the fact that the number of observations out there is limited so I
don't know how to address the problem well.
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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