comments for Rob

From: Pilar Ruiz-Lapuente (pilar@MPA-Garching.MPG.DE)
Date: Tue Feb 25 2003 - 19:20:12 PST

  • Next message: Gerson Goldhaber: "sn92ag"

     Hi Rob,
     I just summarize here my impressions (other things have already been
     mentioned by people on the web page). Congratulations for your work!

     Pilar
     ___________

     I would say that this paper is (and should be) the paper
     where everybody will see the most up to date results on
     Omega(M), Omega (Lambda) and w by the SCP (sort of what the P99 paper
     has been up to now using the previous 42 high-z SN Ia).

     I just would like to mention a few general things along that line.
     
     1/One of them is the abstract. I would go more directly to the results
     and mention as well Omega (Lambda) with errorbars in a similar way as in
     P99 (for flat case). People want to go quickly to the numbers from
     SNe Ia, and get them from the abstract (if possible).
     I think the second sentence "When ...dark energy" on the abstract
     should be removed.
     

     2/Along the same lines I would add in Table 8 Omega (Lambda) (for the
     reason that SNeIa are relevant probes for Lambda). I'm thinking in
     something closer to Table 3 in P99, best fit column.

     3/ You end the paper with a quotation to Bahcall et al.
     (2003) paper and its determination of Omega(M) from the SDSS
     cluster result. This is made in the context of using their value
     for Omega(M) to get limits on the index of the equation of state.
     It seems to give a lot of weigth to such particular method (the last
     sentence of any paper is a very noticeable one). Would not just
     be better to quote the limits for the flat Universe? (or flat
     Universe plus an upper limit on Omega(M)?).
     Everybody is confident on the flatness results from the various
     CMB experiments, but the SDSS results are less well established.
     Equal weight seems to be given in the paper to the CMB results as to
     the cluster ones (abstract, introduction, conclusions). I would say
     that the CMB results are sound since they come from many independent
     measurements. Nothing gives the same soundness to the cluster
     method, as far as I know. There are discrepancies using this method.

    4/ More references to the previous SCP articles (the last ones) updating
    the questions that have been addressed. Perhaps adding a small
    section on recent tests on the SNIa method (?).

    5/ Should one mention as well WMAP? (Introduction)

    6/ If tables with the data are included, I would place them in
      an appendix. And just a figure with all lightcurves (in the
      appendix as well) to avoid disrupting the logical flow of the
      article.

    I stop here these short comments. I like very much the paper and
     you have done a lot of work (and perhaps still do some, best luck!).
     Cheers!



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