From: Chris Lidman (clidman@eso.org)
Date: Thu Apr 01 2004 - 15:44:43 PST
Hi Lifan,
From the label on the x-ordinate, it would appear that this is for the
R filter. Can you do the same for I? Also, is this plot applicable to a
single redshift?
Cheers, Chris.
On Thu, 2004-04-01 at 19:29, Lifan Wang wrote:
> Hi,
>
>
> Here is the histogram of K-corrections for all of the spectra that I
> have. The template spectrum Serena sent to me is marked by the red "temp".
>
> I might have found the reason for the difference between my K-corr and
> the Serena's. In my fit, I only normalize the spectra to the observed
> magnitudes close to the region of interest, and use a smooth function for
> the normalization. When I try to include all the colors, I do end up
> something closer to what I can get from Serena's template, but I think
> this is unphysical.
>
> In the attached figure, the spectrum from Serena's template is treated
> just as the observed spectra. They are normalized to to VRI magnitudes,
> normalizing only to RI magnitudes makes no difference in my results.
>
> Note that contrary to what's in Rob's email, that in my approach, I did
> not "applying the function that pushes it a little up here, a little down
> there, in comparison to what Serena did".
>
> The normalization function I use has NO wiggles, and as it seems, we all
> agree that this is important.
>
> Because my normalization applies only for VRI, the spectra in U and B
> are arbitrary. I hope this also addresses Rob's previous email requesting
> my spectra at 3000A.
>
> Cheers,
>
> Lifan
>
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