- drach09's home page
- Posts
- 2022
- 2020
- June (1)
- 2019
- 2018
- 2017
- 2016
- 2015
- 2014
- December (13)
- November (2)
- October (5)
- September (2)
- August (8)
- July (9)
- June (7)
- May (5)
- April (4)
- March (4)
- February (1)
- January (2)
- 2013
- December (2)
- November (8)
- October (5)
- September (12)
- August (5)
- July (2)
- June (3)
- May (4)
- April (8)
- March (10)
- February (9)
- January (11)
- 2012
- 2011
- October (1)
- My blog
- Post new blog entry
- All blogs
2019 Isobar Analysis Blinding Status Page
Updated on Sat, 2019-10-05 15:32. Originally created by drach09 on 2019-06-12 08:39.
This page gives the current status of the 2019 blind analysis of isobar data, as outlined in the Analysis Blinding Committee recommendation adopted by STAR.
Step-1: Mixed-species Reference
Estimated Completion Date: October 13, 2019 (based on CME-focus meeting discussion, September 30)
From the recommendation:
- Analysis code and time-dependent Q/A will be tuned on this reference sample, committed to the analysis code repository, and kept unchanged at this stage. Among other aspects, this step will enable extraction of time-dependent spectra for Q/A, detection of time-dependent anomalies, detection of secondary decays, and measurement of peak widths relevant to momentum resolution. The step will also enable detection of beam backgrounds, provided they are strictly time-dependent over periods greater than the time between switching species.
- After the step-1 data are available, blind-data analysts will estimate a timeline for completing the necessary analyses for partial un-blinding and advancing to step-2. Based on this input from the analysts, management will approve a date for partial un-blinding. Analysts will present regular updates to document progress. Regardless of progress, un-blinding will occur no earlier than the original estimate unless all blind analyses are deemed ready to proceed by STAR Management. Based upon the progress reports, un-blinding may be delayed to ensure the quality of the final results.
- Prior to the first un-blinding step, analysts will prepare a detailed note documenting the procedures, cuts, corrections, systematic uncertainties, and criteria for any future run-by-run cuts and corrections
- Prior to each un-blinding step, analysts will provide analysis code for vetting and Q/A by the GPC in addition to the standard vetting within the physics working groups.
- When the GPC is satisfied that an analysis is ready for un-blinding, analysts will present the status of their analyses to the physics working group conveners and the physics analysis coordinator. As the un-blinding date approaches, analysts discuss with STAR management any need for delays to un-blinding to ensure the quality of results. If an unresolved disagreement exists between analysts, the decision to un-blind or extend the date will lie with STAR management.
Initial Steps: Mock Data Challenge
Completed, March 21, 2019
Links to studies (also available at the CME Focus page)
- Step-1 Mock Data ("mixed" blind data)
- Step-2 Mock Data (“unmixed” blind data)
- Fully unblind Mock Data
»
- drach09's blog
- Login or register to post comments