From: Isobel Hook (imh@astro.ox.ac.uk)
Date: Mon Jan 12 2004 - 02:30:31 PST
Hi Gaston,
Thanks for addressing my comments.
I agree that the data tables would be fine on the web only. Some journals
will do this automatically - I once submitted a paper to A&A with some
large data tables, and they told me they would only publish those in the
electronic version of the paper. So I think it might be worth submitting
the tables with the paper, so that they get archived somewhere properly.
> - Yes, I have tried to plot the Delta_EW vs M_B for individual SNe. The
> very first versions of the paper, before Section 5 appeared, included this
> analysis. But again, the correlation was not as strong as the ones finally
> presented.
I just went back and looked at those. Actually I think they look pretty
good and although they're not as strong at the one you've found for
EW(2+3) they could be more useful because you only need one spectrum to
place an object on the plot (at least for CaII IR and FeII 4800). I would
encourage you to put those plots back in and give the equations of the
fits.
> - In my opinion, a plot of EW_(2+3) as a function of epoch wouldn't add
> really that much substance to the analysis.
I agree that it wont add to the analysis but since you go into quite a bit
of detail on the EW(2+3) feature, I think its important to show the data
that the analysis is based on.
Cheers,
Isobel.
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