From: Andy Howell (DAHowell@lbl.gov)
Date: Wed Apr 30 2003 - 19:44:07 PDT
Greg,
This mainly a psychological effect of the rebinning -- I rebinned the
data to 20A.
I put up on the web page the same plot rebinned to 3A -- you can see it
looks like the
untouched data.
Also, the spectrum I show is cropped to only show where the template
spectrum and
the observation overlap. I put up another plot showing a different fit
with more of the data.
My program has the freedom to do other things to the data as well. In
my plots I have alread
subtracted host galaxy. Plus, my program either reddens or bluens the
spectrum to find the best fit.
So the spectrum I show may not correspond to reality -- I let it mangle
the observed
spectrum to find the best fit possible. Often it will find junk, but
the point is that
if there is a Ia signal there it should find it. Here I just chose one
example to show,
but I don't believe it -- I don't believe any of the fits.
-Andy
Greg Aldering wrote:
>Hi Andy,
>
>I am looking at the spectral fits to 98104 on your website. I don't see a
>relation between your spectrum and Isobel's. Am I even looking at the
>right thing? (Yours is labeled "Observed: 98104cc_comb.Ic.asc" and
>Isobel's is labeled "98104 (Keck) : 98104cc_comb.asc". Yours is a
>power law and Isobel's have plenty of wriggles.
>
>
>
>>Due to the E's 4000A break, you subtrack off more light blueward of 4000A
>>than redward, and this can mimic Ca from the SN.
>>
>>
>
>No. The effect of subtracting an elliptical is to decrease the strength
>of Ca - unless you let the elliptical go negative! But I do agree that
>9878 isn't convincing.
>
>- Greg
>
>
>
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