Blog of Plots for the Phi Meson Spin Alignment Study

Correction Note:drupal.star.bnl.gov/STAR/system/files/Correction.pdf

FCV Presentations:
Spin Alignment Figure Request/Update FCV 05/15/24:drupal.star.bnl.gov/STAR/system/files/SQM_9.pdf
Spin Alignment Correction Procedure II: drupal.star.bnl.gov/STAR/system/files/SpinAlignmentFCV050124_1.pdf
Spin Alignment Correction Procedure: drupal.star.bnl.gov/STAR/system/files/SpinAlignmentFCV041724__.pdf
Progress Summary: 02/21/24: drupal.star.bnl.gov/STAR/system/files/FCV_Meeting_022124_4.pdf

Previous Presentations for QA with Xin: 
QA Meeting 02/07/24: drupal.star.bnl.gov/STAR/system/files/PrimarySubEventCheck020724.pdf
QA/Analysis Meeting slide 01/13/24: drupal.star.bnl.gov/STAR/system/files/QA_Update011324_0.pdf
QA Meeting 01/12/24: drupal.star.bnl.gov/STAR/system/files/QA_Update011224_0.pdf
QA Meeting 11/30/23: drupal.star.bnl.gov/STAR/system/files/ProgressReportQA113023_0.pdf
QA Meeting 11/17/23: drupal.star.bnl.gov/STAR/system/files/QA_Meeting111723_2.pdf
QA Meeting 10/13/23: drupal.star.bnl.gov/STAR/system/files/QA_Meeting101623_0.pdf

Pre-QM 23 Presentations:
QM 2023 Poster: drupal.star.bnl.gov/STAR/system/files/CWR-QM2023_poster_6e.pdf
Raw Yield and Inv Mass Check (FCV) : drupal.star.bnl.gov/STAR/system/files/RawYieldAndInvMassCheckpdf.pdf
QM Preliminary Request (FCV): drupal.star.bnl.gov/STAR/system/files/PreliminaryRequest_3.pdf
Update for QM FCV 0801623 - 081723: drupal.star.bnl.gov/STAR/blog/cwrobertson/Spin-Alingment-Update-QM-Poster-FCV-Meeting-0816-0817
Toy Model Presentation II  062123 for FCV: drupal.star.bnl.gov/STAR/system/files/FCV062123.pdf
Toy Model Presentation I 053123 for FCV: drupal.star.bnl.gov/STAR/system/files/Fcv053122_SpinAlingmentToyModel.pdf 
First presentation at FCV 040523: drupal.star.bnl.gov/STAR/blog/cwrobertson/Phi-Meson-Slides-FCV-Meeting-040523

Current Results: 
<cos> toy model/folding fits:drupal.star.bnl.gov/STAR/system/files/QA_Meeting111723_fits.pdf
slides 13-19: fits of our data folding/toy model study of the phi meson kinematic effect on rho00
slide 13 real phi, smeared kinematic, <cos> fits

Momentum/Rapidity Dependence/Phi Meson Angle Dependence:
Run11 200 GeV: drupal.star.bnl.gov/STAR/system/files/RhoMomentumDepdence112623.pdf
slide 2: cuts and binning details
slide 3: raw results
slides 4+: progress plots <cos> and mass plots

Eta/Rapidity Dependence:
Run 11 200 GeV:  drupal.star.bnl.gov/STAR/system/files/Run11Rapid110923.pdf
slide 3-5: run 11 200 GeV data results 
slide 6: real and rotate pair <cos> comparison vs. y 
slides 7-8: folding <cos> 
slide 8-12: initial data scaling (cyan) and intial correction green/cyan vs. y
slides 14-19: data folding with and without eta_k cut 
Cyan data in these plots are from data scaling without Y dependence. They are from our inclusive data scaling we used before QM.
Run 11 200 GeV, Additional Slides: drupal.star.bnl.gov/STAR/system/files/Run11Rapid112023.pdf
Slides 7-9: centrality 20-60% |Y| results
Slides 23- 26: Rapidity dependent weighting and scaling test

Comparison of Our Raw Rho00 vs. Centrality and Pt  Results with Published/Analysis Note  (10/03/23) 
drupal.star.bnl.gov/STAR/system/files/RawRhoCentAndPt_new.pdf
-Run 14 200 GeV, Run 11 200 GeV, 62, 39, 27, 19.6, and 11.5 GeV 

Comparison with GPC Analysis Note for Strange Hadron Study (09/22/23)  QA 
drupal.star.bnl.gov/STAR/system/files/AnalysisNoteComparison.pdf
-Includes our Phi Meson pt spectra for each centrality, compared with published 

200 GeV Run11 QA Plots (09/22/23):
drupal.star.bnl.gov/STAR/system/files/200GeV_Run11_QA_Plots.pdf
s2-9: Mass dist in each cos theta bin, for each pt bin
s11-18: Mass dist in each cos that bin / sum of cos theta bins, for each pt bin 
s19: Mass dist in each pt bin / mass dist in Sum Pt Bins 
s20: Mass dist in each pt bin 
s21: <cos> vs. Mass in each pt bin / Sum Pt Bins 

200 GeV Run14 QA Plots (10/03/23) :
drupal.star.bnl.gov/STAR/system/files/200GeV_Run14_QA_Plots_0.pdf
s2-9: Mass dist in each cos theta bin, for each pt bin
s11-18: Mass dist in each cos that bin / sum of cos theta bins, for each pt bin 
s19: Mass dist in each pt bin / mass dist in Sum Pt Bins 
s20: Mass dist in each pt bin 
s21: <cos> vs. Mass in each pt bin / Sum Pt Bins 

62 GeV QA Plots(09/22/23)
drupal.star.bnl.gov/STAR/system/files/62GeV_QA_Plots.pdf
s2: Mass dist in each Pt Bin
s3: Mass dist in each Pt Bin / Sum Pt Bin
s4: <cos> vs. mass in each pt bin / Sum Pt Bin
s5: <cos> vs. mass in each pt bin / <cos> vs. mass 200 GeV
s6: Mass dist  in each pt bin / 200 GeV in each pt bin

39 GeV QA Plots(09/22/23)
drupal.star.bnl.gov/STAR/system/files/39GeV_QA_Plots.pdf
s2: Mass dist in each Pt Bin
s3: Mass dist in each Pt Bin / Sum Pt Bin
s4 :Mass dist  in each pt bin / 200 GeV in each pt bin
s5: <cos> vs. mass in each pt bin / Sum Pt Bin
s6: <cos> vs. mass in each pt bin / <cos> 200 GeV in each pt bin

27 GeV Run18 QA Plots (09/22/23):
drupal.star.bnl.gov/STAR/system/files/27GeV_Run18_QA_Plots.pdf
s2-9: Mass dist in each cos theta bin, for each pt bin
s11-18: Mass dist in each cos that bin / sum of cos theta bins, for each pt bin 
s19: Mass dist in each pt bin / mass dist in Sum Pt Bins 
s20: Mass dist in each pt bin 
s21: <cos> vs. Mass in each pt bin / Sum Pt Bins 

19.6 GeV QA Plots (09/27/23):
drupal.star.bnl.gov/STAR/system/files/19GeV_QA_Plots.pdf
s2: Mass dist in each Pt Bin
s3: Mass dist in each Pt Bin / Sum Pt Bin
s4 :Mass dist  in each pt bin / 200 GeV in each pt bin
s5: <cos> vs. mass in each pt bin / Sum Pt Bin
s6: <cos> vs. mass in each pt bin / <cos> 200 GeV in each pt bin

11.5 GeV QA Plots (09/27/23):
drupal.star.bnl.gov/STAR/system/files/11GeV_QA_Plots.pdf
Have less plots than the other energies, because I didn't run the cos theta bin method at this energy
Also did not make plots of 11.5 GeV /200 GeV, because we ran this energy with more pt bins as a check.
Would require some rebinning and technical work to make those plots