Re: [Brahms-l] problem with pp reference spectra

For learning where the "newly produced bdst files" are, you can use the 
file catalog and it tells you directly.  I have written a simple program 
which I put into brat this morning.  Once it makes it into the afs (or 
if you checkout your own, it should be in there after installation), you 
can do
findfile run ltr
for example
findfile 15312 ltr
and that gives you a list of where all the ltr files for run 15312 are.  
For bdst, you would do
findfile 6723 dst

Hope it helps

Kris

yin.zhongbao@ift.uib.no wrote:

>Dear all,
>
>in order to answer JH's question he sent out a few days ago, I start 
>to wonder my reference spectrum got from PHENIX pion zero measurements.
>Since the pion zero measured starts at pt from 2 GeV/c, in principle it is 
>not safe to extend to low pt range by using their fitting function. 
>Recently STAR have published their pion spectra at midrapidity in p+p 
>collisions. I used them to produce the RAA for pi^- and the results
>are located at 
>www.ift.uib.no/~yin/RaaStar.gif
>
>So, it looks like that I should not use PHENIX pion zero measurement to 
>extract the reference spectrum. I may have been cheated by the contructed 
>reference spectrum since it describes our (pi^-+pi^+)/2 measurements well.
>Then I compared our measurements to STAR's, what I found that our pi^+ 
>measurements is almost consistent with STAR's data if not corrected for 
>the trigger inefficiency, but pi^- is much lower than STAR's measurement. 
>I think I have to look at our pp data once more to see if I can get them 
>right. Then I would like to ask where the newly produced bdst files are.
>
>Best regards,
>Zhongbao
>
>
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>
>  
>

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