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star-fcv-l - Re: [Star-fcv-l] [Star-pwgc-l] [Starprod-l] auau 19.6GeV run 2019 sample for QA

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: EMAIL-SDU <xuqh AT email.sdu.edu.cn>
  • To: "Van Buren, Gene" <gene AT bnl.gov>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] [Star-pwgc-l] [Starprod-l] auau 19.6GeV run 2019 sample for QA
  • Date: Sun, 12 Sep 2021 15:13:11 +0800

Hi Gene,

I can understand this for low pT tracks, but a bit hard to understand this
for track at pT>2 GeV. It is true that it is happening with a tiny
probability though.

Thanks,

Qinghua

> 2021年9月11日 上午12:15,Van Buren, Gene via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> 写道:
>
> Hi, all
>
> CA can include more than 1 hit on a pad row onto any track as it crosses
> that row.
>
> -Gene
>
>> On Sep 10, 2021, at 7:33 AM, ShinIchi Esumi via Star-fcv-l
>> <star-fcv-l AT lists.bnl.gov> wrote:
>>
>> Dear Xingrui
>> Thanks for the plots, you've mentioned that number of hits in the TPC
>> are exceeding more than the number of pad in radial direction, is this
>> not allowed if the track is curling up by the B-fields especially for the
>> low
>> pT tracks, so can you plot the 2D-correlation plot between "number of tpc
>> hits in one track" vs (pT, eta and phi) for both (global and primary
>> tracks)?
>> Thank you very much. You can also ask for a time slot in the parallel
>> Session, is you like to show and discuss this with other people in the
>> PWG...
>> Best regards, ShinIchi
>>
>>> On Sep 10, 2021, at 17:50, xgou <xgou AT rcf.rhic.bnl.gov> wrote:
>>>
>>> Dear all,
>>>
>>> We have taken a quick look QA at AuAu19.6GeV_2019.
>>> You can find my slides here:
>>> https://drupal.star.bnl.gov/STAR/blog/xgou/quick-qa-auau19gev2019
>>> Thanks.
>>>
>>> Best regards,
>>> Xingrui
>>>
>>>
>>>> Dear FCV PWG colleagues
>>>> This is a good news for people looking for 19.6GeV production. Please
>>>> take a look.
>>>> I hope we do not have to stop anymore and continue ...
>>>> Best regards, ShinIchi
>>>>> Begin forwarded message:
>>>>> From: Rongrong Ma via Star-pwgc-l <star-pwgc-l AT lists.bnl.gov>
>>>>> Subject: [Star-pwgc-l] Fwd: [Starprod-l] auau 19.6GeV run 2019
>>>>> sample for QA
>>>>> Date: September 1, 2021 2:16:27 JST
>>>>> To: STAR PWG Convener List <star-pwgc-l AT lists.bnl.gov>
>>>>> Reply-To: Rongrong Ma <marr AT bnl.gov>, STAR PWG Convener List
>>>>> <star-pwgc-l AT lists.bnl.gov>
>>>>> Dear Conveners
>>>>> The new test sample for 19.6 GeV is available now. Please provide
>>>>> feedback on data quality as quickly as possible. Thanks!
>>>>> Best
>>>>> Rongrong
>>>>>> Begin forwarded message:
>>>>>> From: didenko via Starprod-l <starprod-l AT lists.bnl.gov>
>>>>>> Subject: [Starprod-l] auau 19.6GeV run 2019 sample for QA
>>>>>> Date: August 31, 2021 at 12:47:44 PM EDT
>>>>>> To: starprod-l AT lists.bnl.gov
>>>>>> Reply-To: didenko <didenko AT rcf.rhic.bnl.gov>, discussion list for
>>>>>> all aspects of STAR's offline data production
>>>>>> <starprod-l AT lists.bnl.gov>
>>>>>> Dear All,
>>>>>> auau 19.6GeV run 2019 data sample for days 62-65 have been
>>>>>> produced with
>>>>>> updated calibrations, chain options and SL21c library.
>>>>>> Current statistics is 135M st_physics stream data and 1.8M st_mtd
>>>>>> stream data.
>>>>>> MuDst & picoDst files are written on NFS.
>>>>>> You can use next FileCatalog query to get list of files and
>>>>>> locations:
>>>>>> get_file_list.pl -keys path,filename -cond
>>>> trgsetupname=production_19GeV_2019,production=P21ic,filetype=daq_reco_picoDst,filename~st_physics,storage=nfs
>>>>>> -limit 0 -delim "/"
>>>>>> Pl look at the data sample for QA and give us feedback.
>>>>>> Thanks, Lidia.
>>>>>> _______________________________________________
>>>>>> Starprod-l mailing list
>>>>>> Starprod-l AT lists.bnl.gov
>>>>>> https://lists.bnl.gov/mailman/listinfo/starprod-l
>>>>> _______________________________________________
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