Minutes of Brahms Analysis Meeting 02 April 2010 ================================================ Ramiro, Chellis, JH, FV, Steve, Kris, Michael Agenda and slides at http://indico.cern.ch/conferenceDisplay.py?confId=89928 Ramiro dAu Analysis =================== He has produced pi,k,p, spectra from dst2spec, ie Flemming's package. He has min bias and 0-30%, 30_60%, 60_80%. He is trying to push beyound 2.0GeV and so has corrected his spectra for contamination. To create dN/dy's over a wide rapidity spectrum he has fit a Levi function using "Combined Fits" macro that was developed for the pp analysis. T = T0 + ay + by^2 and the same for the p0 parameter. Getting the dN/dy versus rapidity he thinks he has some problems at 12 and 8 degree, ie rapidity 2-3. There was also some discussion on the error values. There are significant fluctuation around the general curve and he thinks that a first fit that uses only settings with good low Pt data should be used. Then use all data where you allow just the dN/dy to be free. For the protons he has fit to exponentials in Mt. He tends to have good coverage at low Pt so this helps with the dN/dy. At high Pt he may have contamination from pions and kaons. d/p Michael =========== The main topic was the discussion of the summary which is now perhaps too long. The distinction between radial and elliptic flow should be noted. There were several small comments on the text and unfortunately a few gremlins crept into the figures. These should be fixed this weekend so we can hopefully announce the paper soon. pp paper: Flemming and Kris =========================== Flemming quickly went through the draft pp paper, with special emphasis on the figures. There were several suggestions for improving the clarity of the figures and a few questions on the data and fits. _______________________________________________ Brahms-l mailing list Brahms-l_at_lists.bnl.gov https://lists.bnl.gov/mailman/listinfo/brahms-lReceived on Fri Apr 02 2010 - 13:12:13 EDT
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