1) PWGC preview

Title: Bulk properties of the system formed in Au+Au collisions at sqrt(sNN)=14.5 GeV using the STAR detector at RHIC
PWG: BulkCorr (primary) and LFSUPC (secondary) 
PAs: Debadeepti Mishra, Vipul Bairathi, Subhash Singha, Lokesh Kumar, Bedangadas Mohanty, Declan Keane

Target journal: PRC

webpage: http://www.star.bnl.gov/protected/bulkcorr/vipul/AuAu15GeV/PaperProposal/AnaWebpage/index.html
presentation: http://www.star.bnl.gov/protected/bulkcorr/vipul/AuAu15GeV/PaperProposal/PaperProposal_AuAu15GeV.pdf

analysis note: https://www.star.bnl.gov/protected/lfsupc/deepti/Papers/auau14p5GeV/ANALYSIS_NOTE_AuAu15GeV.pdf
https://www.star.bnl.gov/protected/bulkcorr/vipul/AuAu15GeV/ChrgPartv2Ana/Webpage/ananote/AnalysisNote_Chrgv2_v3.pdf 

- Brief introduction from the PWG conveners (5') [Nu]
- Paper proposal (15')  [Bedanga]
- Open discussions (35')
- Summary from the conveners' panel (5’)

2) Preliminary results vs plots
http://www.star.bnl.gov/HyperNews-star/protected/get/starpwgc/4364.html
Kolja: The thought was to take the original QM figure on the left side of slide 8 in https://drupal.star.bnl.gov/STAR/system/files/0823_aoyama_jetcorr.pdf and add background curves as shown in the blown up version on slide 9. The slide 9 picture may be a good _illustration_ of what I'm asking but it would be important to clarify that this is not the actual figure we're discussing. 

3) A few slides with highlight jet measurements from STAR - JetCorr/Spin

4) Search for volunteer checking BEMC status/calibration table, picoDst code maintainer, and embedding deputy

5) AOB 
https://drupal.star.bnl.gov/STAR/pwg/common/upcoming-conferences-deadlines