Re: high pt paper.

From: Ian Bearden (bearden@nbi.dk)
Date: Thu Jun 26 2003 - 07:27:28 EDT

  • Next message: Stephen Sanders: "Re: Progress report - KU"
    Hej Trine,
    Thanks for your comments!
    I agree that the Rcp is nice since we remove the p+pbar reference.
    About the 'selling point:'  I think that the only statement the data 
    allow us to make at this time is that the suppression is the same or 
    stronger at eta=2.2 than the suppression at eta=0.  As for the figures 
    you ask for, we are putting together a web page about the analysis 
    (similar to what Claus did for the d+Au analysis) and the plot will be 
    there.
    As to the centrality:  It is not possible now to go more peripheral, 
    but perhaps with a decent spectrometer trigger (in the upcoming Au+au 
    run) we can do this.
    Again, thanks for the input,
      Cheers,
    Ian
    On torsdag, jun 26, 2003, at 12:39 Europe/Copenhagen, Trine S. Tveter 
    wrote:
    
    > Dear all,
    >
    > On Wed, 25 Jun 2003, Jens Jørgen Gaardhøje wrote:
    >
    >> Enclosed please find an updated version of the high pt paper draft.
    >
    >> Claus has worked hard at a reanalysis and along the way we have 
    >> changed the
    >> figure strategy to focus more on the rapidity dependence, which is 
    >> the BRAHMS
    >> specialty. At the same time we focus more on the relative changes 
    >> between
    >> spectra and ratios. This should make us more independent of the p+p 
    >> 'reference'
    >> and of various systematic errors.
    >
    > I think the draft has really gained from the stronger focus on our 
    > unique
    > rapidity dependence and the emphasis on differential behaviour (R_CPs 
    > and
    > ratios of R_CP between different rapidities, which are independent of
    > our somewhat dubious "reference" spectrum.)
    >
    >> We have been debating whether to show all 4 centrality cuts or just 2 
    >> as in
    >> here. Opinions?
    >
    > It would have been interesting at least as a basis for discussion to 
    > see all 4
    > centrality cuts.  It would also strengthen the statistical material.  
    > The evidence
    > for stronger suppression at eta~2 is based on 3 points with large 
    > error bars
    > (Figure 3.)  I'm curious whether "R_CP"s utilizing more centrality 
    > bins would
    > confirm this trend - maybe one could use the central spectrum as 
    > reference since
    > it has smaller error bars, and compare also R(0-10/20-40) and 
    > R(0-10/10-20)
    > for the two rapidities?
    >
    > Is it possible at all to extract spectra for centralities in the region
    > 60 - 100%?
    >
    >> Claus hopes to be able to post a web page with details of the 
    >> analysis later.
    >
    >> We have had various input (ZBY, JN, MM, KH etc..). Not all has been 
    >> included
    >> yet into the manuscript. Not because of lack of good will but because 
    >> of lack of time.
    >
    >> Hope your comments will continue flowing. They are necessary if we 
    >> are to
    >> attempt  a submission not too far behind the other 3 experiments.
    >> All sorts of comments are greatly appreciated. Particularly those 
    >> that also
    >> concretely suggest a solution to a given problem.
    >
    > The effect of momentum resolution might be a little different in MRS 
    > and FS,
    > which would affect the R_AAs slightly.  (It would of course not affect 
    > the
    > R_CPs :-))  The spectra could easily be corrected for this effect, to 
    > the
    > extent we know the parameters of our Gaussian smearing.  I believe the
    > corrected spectra would be relatively softer at eta~2.
    >
    >> In particular we request your opinion about whether this approach 
    >> (text and
    >> figures) is suitable. If the general idea is acceptable by a 
    >> majority, the next
    >> job is to improve the quality of the draft, of figure appearance etc, 
    >>  while
    >> continuing analysis checks. Parallel processing is necessary.
    >
    > The general idea is fine in my opinion  :-)
    >
    >                                              Cheers,  Trine
    >
    >
    


    This archive was generated by hypermail 2.1.5 : Thu Jun 26 2003 - 07:31:14 EDT