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Subject: STAR Flow, Chirality and Vorticity PWG
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- From: cebra <cebra AT physics.ucdavis.edu>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Cc: Mathias Labonte <mlabonte AT ucdavis.edu>
- Subject: Re: [Star-fcv-l] 3.2 GeV Efficiency issue?
- Date: Mon, 18 Dec 2023 16:14:40 -0600
Hi Cameron,
The 3.2 GeV FXT embedding request that I had submitted used and eta range from -2.4 to 0.0.
That embedding sample should cover the region about which you are concerned. Note that for the
high pT tracks we have never seen any change in tracking performance above 1.5 GeV, so it is really
not efficient use of embedding resources to embed to high pT. There ought to be another 3.2 GeV
proton embedding sample that have the full eta coverage.
You are correct that the FXT acceptance extends beyond rapidity or eta of -2.0, and embedding requests
that do not cover the full acceptance of the TPC in FXT mode are not the best use of resources as they
will need to be redone with a complete coverage.
Regards, Daniel
On 2023-12-18 15:24, Cameron Racz via Star-fcv-l wrote:
Hello convenors,
I was recently doing some work on how I apply the 3.2 GeV FXT TPC
efficiency values to my analyses at 3.5, 3.9, and 4.5 GeV (since that
was the plan I knew of since Quark Matter) and I noticed that the
embedding does not fully cover the TPC in rapidity. I am using
embedding ID 20221601
(https://drupal.star.bnl.gov/STAR/starsimrequests/2022/Apr/23/FXT-AuAu-32-GeV-2019-proton)
I have attached here a 2D plot I made that shows all of the protons I
have that DON’T match up to a TPC efficiency. Essentially, the empty
region that has been cut out is the embedding/efficiency region. I was
concerned about the yellow band at low pT in rapidity between -0.8 and
0 since all of those protons are being thrown out with no
efficiencies.
I think this comes from the fact that the embedding used "-2 <
rapidity < 0 (LAB rapidity)” when the actual eta distribution of the
TPC at 3.2 extends a little past -2.0 (I also attach here a picture of
an eta distribution of all the good TPC tracks I found in my
analysis).
I just wanted to bring this to your attention in case it was an
unknown issue. Is there a way that this could be fixed, or are there
other embeddings planned that would sort of overwrite this one and fix
this issue soon?
Thank you,
Cameron Racz
Ph.D. Candidate
Heavy-ion Physics Group
University of California, Riverside
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[Star-fcv-l] 3.2 GeV Efficiency issue?,
Cameron Racz, 12/18/2023
- Re: [Star-fcv-l] 3.2 GeV Efficiency issue?, cebra, 12/18/2023
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