From: Greg Aldering (aldering@panisse.lbl.gov)
Date: Thu May 22 2003 - 08:27:55 PDT
Yes, the problem is that the stretch-luminosity relation has never
looked very good - we just have avoided ever showing it. I think the
plot has useful information - that our HST SNe all have local
counterparts even in the way they deviate from the stretch-luminosity
relation. Some would think that comparing the stretch distributions
should show the same thing, but then that is true only if SNe Ia are a
one-parameter family of stretch, which the reader can decide from the
figure.
One thing that would make this issue more robust is if we had done a
fit with alpha=0 and could say the cosmology wasn't much affected.
>On Wed, May 21, 2003 at 07:12:11PM -0700, Greg Aldering wrote:
>>
>> Hi Rob,
>>
>> Are the data in Figure 13 corrected for extinction? If so, then you
>> need to correct the label on the Y-axis. I would argue that we want to
>> show the extinction-correct points. Also, which subsample is plotted
>> here?
>
>They are extinction corrected; this is the primary subset, only HST and
>Low-z supernovae.
>
>I agree that it doesn't look that great, although if you look at it
>carefully I thikn the line that is fit makes sense, more sense than a
>horizontal line would. However, first impressions aren't good, and I'd
>not complain if we want to drop this figure from the paper.
This archive was generated by hypermail 2.1.4 : Thu May 22 2003 - 08:27:56 PDT