STAR Flow, Chirality and Vorticity PWG

[ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Jagbir
Fig.5 should be rebinned to be more visible, where we do not see if they are 
correlated or not. 
Is your Fig.6 (that was not in your QM poster) consistent with Fig.8 that was 
in the QM poster? 
This might be the case, though. Delta_gamma is defined to be gamma(OS) - 
gamma(SS), where 
the difference : blue (data) - red (shuffled) in SS has somewhat larger 
magnitude with negative 
sign than in OS for the top DBmax, while it is larger in OS than in SS for 
the middle to small 
DBmax region, which could be interesting. At the end of the figure caption of 
Fig.6, you say 
“for each centrality”, but it is mainly "for the mid-central collisions”, was 
this Fig.6 approved for 
preliminary in the last QM?, sorry I do not remember, since you did not store 
them in the database… 
In Fig.7, you say it’s linear, but it’s curving up to me. Why do you only 
show SS in this Fig.7? Since 
this is just for the top 10% of DBmax, so these 8 points are for the 8 
centrality bins? In Fig.9, why 
did you choose to show only the BG subtraction with shuffling, where you were 
showing both 
subtractions with shuffling and random flow for your QM poster. 
Best regards, ShinIchi

> 2020/12/14 16:43、jagbir <jagbir AT rcf.rhic.bnl.gov>のメール:
> 
> Dear all,
> 
> I tried to send email to FCV list earlier but for me, sometime its not 
> working. I am sorry if you recieved the same email again. I have updated 
> the delta gamma, gamma and fcme plot from QM-19 keeping only data and 
> charge reshuffle. Please let me know  for further comments and suggestions, 
> The link to the updated poster is:
> https://drupal.star.bnl.gov/STAR/node/53026
> 
> Thank you,
> Jagbir Singh
> 
> On 2020-12-14 09:24, jagbir via Star-fcv-l wrote:
>> Dear Prithwish,
>> I have updated the Db distribution plot ( QM-19 plot ).
>> I have updated the gamma  and delta gamma plots by removing the
>> correlated background.
>> I have re-plotted the f_cme plot from QM-19 containing the information
>> only from charge reshuffle background.
>> Please let me know about any further comments/suggestions.
>> The link to the updated poster is:
>> https://drupal.star.bnl.gov/STAR/node/53026
>> The poster presentation for DAE is on 15th December after lunch, i.e.,
>> 15 December midnight (BNL time).
>> Thank you,
>> Jagbir Singh
>> On 2020-12-13 09:29, Prithwish Tribedy wrote:
>>> Hi Jagbir,
>>>  Just to follow up on ShinIchi's suggestions. Since there's very
>>> little time before the conference and there are many questions --
>>> would it be possible for you to replace some of the new preliminary
>>> results with what you showed at the QM, in particular the plot on
>>> f_CME :
>>> https://drupal.star.bnl.gov/STAR/system/files/QM_Poster_Jagbir_v7.pdf
>>> But do include a para (or more) and details on your ongoing study with
>>> the STAR data. We need more time to show new plots but we can
>>> definitely update on the progress at this conference by saying a few
>>> words. This way we will be able to approve your poster presentation
>>> which is only 3-4 days away.
>>> Best,
>>> Prithwish
>>> On 2020-12-12 18:03, ShinIchi Esumi wrote:
>>>> Dear Jagbir
>>>> There has already been some preliminary plots that were shown in your 
>>>> poster
>>>> for the last QM, these results were different from this, so you can
>>>> not change/update
>>>> until you go to the final publication, unless there are some obvious
>>>> errors in the analysis,
>>>> which needs to be discussed in the PWG and cleared/agreed on what to
>>>> do. As Fuqiang
>>>> also pointed out, in addition to the unanswered questions, you did not
>>>> answer to my
>>>> questions/comments/suggestions yet…
>>>> Best regards, ShinIchi
>>>>> On Dec 13, 2020, at 4:26, Wang, Fuqiang <fqwang AT purdue.edu> wrote:
>>>>> Hi Jagbir, All,
>>>>> I'm very concerned about these results being presented outside STAR as 
>>>>> preliminary physics results. There are many unanswered questions (e.g. 
>>>>> my email several weeks ago was not answered) and many of the technical 
>>>>> issues people raised during your last CME focus group meeting 
>>>>> discussion need to be looked into (I will write in a separate email my 
>>>>> follow-up questions to your email to CMEfg yesterday). I would be fine 
>>>>> if your poster is to discuss a technical method to search for the CME, 
>>>>> but I'd be very worried that any physics results be presented as STAR 
>>>>> preliminary.
>>>>> Best regards,
>>>>> Fuqiang
>>>>>> -----Original Message-----
>>>>>> From: Star-fcv-l <star-fcv-l-bounces AT lists.bnl.gov> On Behalf Of 
>>>>>> jagbir via Star-
>>>>>> fcv-l
>>>>>> Sent: Wednesday, December 9, 2020 9:32 PM
>>>>>> To: STAR Flow, Chirality and Vorticity PWG <star-fcv-l AT lists.bnl.gov>;
>>>>>> ptribedy AT rcf.rhic.bnl.gov; esumi.shinichi.gn AT u.tsukuba.ac.jp;
>>>>>> jiangyong.jia AT stonybrook.edu
>>>>>> Subject: Re: [Star-fcv-l] STAR presentation by Jagbir Singh for DAE 
>>>>>> HEP 2020
>>>>>> submitted for review
>>>>>> Hi all,
>>>>>> Sorry for uploading the poster very late.
>>>>>> I request you to please review the poster and give your comments and
>>>>>> suggestions.
>>>>>> The conference is on 14 December.
>>>>>> the link to the poster is here below:
>>>>>> https://drupal.star.bnl.gov/STAR/node/53026
>>>>>> Thank you,
>>>>>> Regards,
>>>>>> Jagbir Singh
>>>>>> On 2020-12-09 23:33, webmaster--- via Star-fcv-l wrote:
>>>>>>> Dear star-fcv-l AT lists.bnl.gov members,
>>>>>>> Jagbir Singh (jagbir1593 AT gmail.com) has submitted a material for a
>>>>>>> review, please have a look:
>>>>>>> https://drupal.star.bnl.gov/STAR/node/53026
>>>>>>> ---
>>>>>>> If you have any problems with the review process, please contact
>>>>>>> webmaster AT www.star.bnl.gov
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