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  1. STAR
    1. BTOW
      1. relative gains
      2. absolute gains + uncertainty
      3. Evaluate improvement in ET of 2x2/3x3 clustering vs. QCD-background rejection
    2. TPC
      1. identify reason for inefficiency at eta~0, but no replay of BFC
      2. compare TPC track position accuracy data/MC
    3. Vertex finder (PPV) vetting/debugging
      1. Q: is 3cm accuracy enough for x-section paper?
      2. acceptance correction when triggered on L2W trigger
    4. Trigger
      1. relative spin dependent lumi (based on BHT3 in muDst), QA
      2. absolute cross section from BHT3
        1. determine BHT3 cross section from Vernier scan
        2. estimate error, beam background contribution to BHT3 X-section
      3. vet BHT3 & BBC abs X-section previously used in STAR
      4. spin bits or bXing --> spin pattern mapping
    5. VPD ZDC local polarimeter
      1. magnitude non longitudinal beam polarization
    6. Simulations
      1. Vet MC/Data
      2. efficiency of W-algo used
    7. W-algo evaluation
      1. Background model for what's under the Jacobian peak
      2. acceptance corrections (will need input from TPC track position accuracy)
  2. RHIC Polarization
    1. pol pattern per fill
    2. CNI Polarization values, QA
  3. Theory
    1. get calculation done for our bins
    2. vary input PDFs, average sign
    3. effect of non longitudinal beam polarization
  4. Organization
    1. refine this list
    2. assemble .tex files with outline of the paper

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