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star-gpc-355-l - Re: [Star-gpc-355-l] Acceptance LK18767WR Collaboration

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Subject: STAR GPC #355

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Re: [Star-gpc-355-l] Acceptance LK18767WR Collaboration

Chronological Thread  
    < Chronological >       < Thread >
  • From: James Dunlop <dunlop AT bnl.gov>
  • To: "Feng, Yicheng" <feng216 AT purdue.edu>
  • Cc: James Dunlop <dunlop AT bnl.gov>, STAR GPC #355 <star-gpc-355-l AT lists.bnl.gov>, Fuqiang Wang <fqwang AT purdue.edu>
  • Subject: Re: [Star-gpc-355-l] Acceptance LK18767WR Collaboration
  • Date: Tue, 4 Jun 2024 14:48:13 -0400
Go ahead unless you hear something by COB today

On Jun 4, 2024, at 2:47 PM, Feng, Yicheng <feng216 AT purdue.edu> wrote:

Hi GPC, 

Just a kind reminder. 
I sent an email last Thursday for comments on the "key image and blurb". 
If you do not have any further comments, I plan to send them to starpapers-l. 

Thank you,
Yicheng for the PAs
From: Star-gpc-355-l <star-gpc-355-l-bounces AT lists.bnl.gov> on behalf of Feng, Yicheng via Star-gpc-355-l <star-gpc-355-l AT lists.bnl.gov>
Sent: Thursday, May 30, 2024 6:29 PM
To: STAR GPC #355 <star-gpc-355-l AT lists.bnl.gov>
Cc: Feng, Yicheng <feng216 AT purdue.edu>; Wang, Fuqiang <fqwang AT purdue.edu>
Subject: [Star-gpc-355-l] Fw: Acceptance LK18767WR Collaboration
 
---- External Email: Use caution with attachments, links, or sharing data ----

Hi GPC, 

The short paper of isobar CME baseline has been accepted by PRResearch. 
The journal asks for a "Key image" and "Blurb"(1 or 2 sentences) to show on their webpage: 

We drafted a blurb with 2 sentences: 
The anticipated chiral magnetic effect (CME)-related charge separation was not measured to be larger in ${^{96}_{44}\text{Ru}}+{^{96}_{44}\text{Ru}}$ than in ${^{96}_{40}\text{Zr}}+{^{96}_{40}\text{Zr}}$ collisions because the flow-induced backgrounds do not fully cancel due to nuclear structure differences between the two isobar nuclei. Properly taking this, as well as the next-level nonflow-related backgrounds, into account, the charge separation results are consistent between the isobar systems and an upper limit of 10% CME signal is extracted at 95% confidence level. 

We tried to make an image by ourselves, which can be found through the drupal links below: 
As a reference, the previous BNL news for isobar blind analysis has a cartoon: https://www.bnl.gov/newsroom/news.php?a=119062

If you have any comments, please let us know. 
After you think they are ready, we will also send them to starpapers-l.

Sincerely,
Yicheng for the PAs

From: prresearch AT aps.org <prresearch AT aps.org>
Sent: Monday, May 27, 2024 6:05 PM
To: Feng, Yicheng <feng216 AT purdue.edu>
Subject: Acceptance LK18767WR Collaboration
 
[You don't often get email from prresearch AT aps.org. Learn why this is important at https://aka.ms/LearnAboutSenderIdentification ]

---- External Email: Use caution with attachments, links, or sharing data ----


Re: LK18767WR
    Upper limit on the chiral magnetic effect in isobar collisions at the
    relativistic heavy-ion collider
    by The STAR Collaboration and Yicheng Feng

Dear Dr. Feng,

We are pleased to inform you that your manuscript has been accepted
for publication as a Letter in Physical Review Research.

Your manuscript will now be prepared for the production process, so
please do not send a revised manuscript or figures at this time unless
requested. If any issues arise, we will contact you.

Otherwise, you should receive page proofs in one to two weeks after
your manuscript is received by our production vendor. For up-to-date
information on the editorial and production status of your manuscript,
see https://nam04.safelinks.protection.outlook.com/?url="https%3A%2F%2Fauthors.aps.org%2FSubmissions%2Fstatus%2F&data=05%7C02%7Cfeng216%40purdue.edu%7Ca3c17eff1d9d4f3b066e08dc7e992878%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638524443485727143%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C0%7C%7C%7C&sdata=06ADx58MJlJWX2BiSID7%2BKFsJFWRtckjxpE0JVRnACY%3D&reserved=0.

Yours sincerely,

Juan-Jose Lietor-Santos
Chief Editor
Physical Review Research
Email: prresearch AT aps.org
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Re: LK18767WR
    Upper limit on the chiral magnetic effect in isobar collisions at the
    relativistic heavy-ion collider
    by The STAR Collaboration and Yicheng Feng

Dear Dr. Feng,

Your article will be accompanied by a Blurb and a Key Image, when it
appears online. We would appreciate if you could provide us with these
at your earliest convenience, by replying to this email.

The Blurb should be about one to two sentences, preferably written in
the third person, that summarize the main advance of the article in
its area of research. Please refrain from claims of novelty,
significance, or from speculations about future developments. We
strongly favor factual texts that objectively state the science
presented in the paper. You may consult recently published articles in
our webpage for examples and guidance on our preferred style for
Blurbs. We may edit or rewrite any text for consistency.

As for the Key Image, we would ask for one that is clear and
captivating (avoid plots). It is meant to catch the eye and convey the
main theme of the work, in broad strokes, not to explain
quantitatively the key scientific result. We would ask for an
approximately square, aesthetically pleasing, and simple image.
Ideally, it should be 400 x 400 pixels (PNG preferred). Be sure that
the figure you supply is either your own and original or has the
appropriate copyright clearance.

We look forward to hearing from you.

Yours sincerely,

Juan-Jose Lietor-Santos
Chief Editor
Physical Review Research
Email: prresearch AT aps.org
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