[Brahms-l] Brahms minutes 02 March 07

From: Michael Murray <mjmurray_at_ku.edu>
Date: Fri, 2 Mar 2007 10:17:10 -0600
Minutes of BRAHMS Analysis meeting 23 Feb 2007
============================================== Submitted by Michael  
Murray

Slides are at http://indico.cern.ch/conferenceDisplay.py?confId=13148

Present: Michael, Selemon, Dipali, Hong Yan, Ramiro, JH Lee, Flemming  
Steve


Previous Action Items:
1) Please have a final check of Ionut's proceedings which will be  
submitted in a few hours. http://folk.uio.no/ionutca/ 
qm06_IA_proceeding_v3.pdf
    Done I guess
2)Dipali: Look into normalisation of background
    See this meeting

Agenda

09:30 	dau PID analysis (40') 	Ramiro Debbe
10:10 	Drift Velocity Calibration for T1 (20') 	SELEMON BEKELE
10:30 	phi->kk analysis (update) (20') 	Dipali Pal
10:50 	plans for analysis meeting (10') ( Paper   )	F.Videbaek
presentation and discussion of plans for analysis meetings,
as distributed before.


Action Items from this week:
Ramero: Understand the rescaling for group B runs
Explain the 20% difference between spectra from productions 3 and 2.

Selemon: Select only Trigger 2 and 6 and increase statistics for  
failing runs.
Dipali: Think about how to handle the normalization of events with 3  
and 4 kaons.

Next week: We should here from Nathalie and also Selemon will present  
CuCu spectra:

This week's minutes:
====================
Ramero: dAu PID:
================
He is using only the RICH and is using the 3rd set of DSTs. This set  
includes some more troublesome runs which have problems with the Z  
vertex.
Group A) No ADCs for INEL counter sigma = 10cm
Group B) cross talk, don't use INEL z vertex
Group C) Good vertex, sigma = 5cm.

Stratagies
a) Normalization INEL and Trig 5, pointing to vertex by tracking only.
b) These runs are useful for our negative pion distribution.use BB to  
get z vertex and normalization done with trig 1. Will correct for  
lower efficiency of BB detectors.
He finds this factor in good runs.
FV notes that this correction factor depends slightly on the vertex  
bin. Note scaling factor for polarity B seems to be different from  
polarity A. With fudged scaling factor he can get a nice agreement  
with spectra.

When comparing to DSTs from production 2 he find an increase of 20%  
for both pi+ and pi-. This could be due to tracking efficiencies  
caused by a difference in maps.
A new PRL will
To concentrate on measurements performed at 4 degrees.
Spectra: min bias 0-30% 30-60% and 60-80% for pion kaons and protons.
(Note on a semilog plot one cannot see the difference in centrality  
between the spectra).

RdAu for the most central set. We may be able to highlight the  
physics behind meson baryon difference, as well as the “standard”  
discussion about evolution and multiple scattering.
We appear to have a decent data sample of p+Au events tagged with a  
single neutron in the right ZDC. There may be interesting physics in  
that measurement.

Action Items: Understand the rescaling for group B runs
Explain the 20% difference between spectra from productions 3 and 2.

Then he can make p,pbar spectra and work on a paper draft.

Centrality Dependence: Hong Yang will



Flemming:Schedule and preserving analysis info
==============================================
3/9 Selemon: CuCu spectra and Nathalia -
3/16 Catalin: AuAu high pt Flemming: pp 62 GeV
3/23 Truls: auau,cucu 62 JH: Spin at 62 and 200 GeV
3/30 Steve: v2 analysis

We need to make our results widely available and easily understandable.
Data should be saved as simple root historgrams with easily  
identifable names.

Spectrum specification :
Each spectrum analysis should deliver spectra (invariant yields as  
root directories with
simple names, and titles) (ptalso mt?),
Centrality CuCu (0-10, 10-20, 20-30, 30-40,40-60,60-80) -  Selemon
Centrality AuAu (0-10, 10-20, 20-50, 40-60) - Catalin
Centrality dAu (0-30, 30-60, 60-80) those were used in multiplicity  
papers.
Rapidity bins (dy = 0.2) HY - dA, pp
What are the appropriate centrality scales, dy and dpt. In general  
ones should try to stick
to something like dy-0.1, dpt=50 MeV/c, coarser binning at higher  
rapidities
Dipali Mixed event normalization factor.
========================================
Previous scheme
Mix K+/-'s from an event with K-/+'s from the next
10 events within same centrality and vertex.
Normalize above φ mass range ( 1.1 < M < 1.5
GeV)
Normalization factor, R = Σ(Measured) / Σ(Mixed)
within above mass range
R should be ~0.05, but we found it ~0.03

The weakness of this method is that the mixed events may not all contain
two kaons. She now requires two kaons for all events that are used in  
the background. This gives a much better normalization factor.
Action Item: Think about events with 3 and 4 kaons and discuss  
offline with JH.

Selemon: Drift Velocity calibration of T1
==========================================
One horizontal  calibration fiber seems to be dead.
Many calibrations fail because of "Inconsistent number of fit points"
Some runs seem to have low statistics, Selemon only uses 5 sequences  
but he may need more. Flemming reported that he should select only  
events with triggers 2 and 6, ie something hitting the spectrometer.
In supermon the hit distributions for the calibration fibers seem to  
be missing but this may be simply that the ADC threshold was wrong.
Action Item: Select only Trigger 2 and 6 and increase statistics for  
failing runs.





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Received on Fri Mar 02 2007 - 11:18:54 EST

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