STAR Flow, Chirality and Vorticity PWG

[Muhammad Farhan Taseer <mfarhan_taseer AT yahoo.com>]

Hi Subhash,

Thank you for your nice comments. I have updated the proceedings as per your suggestions. The latest version can be found at the following link:  "https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurement-charge-dependent-directed-flow-STAR-Beam-Energy-Scan-BES-II-AuA-2"

Precisely speaking, I have addressed you comments as:

l#43: in Au+Au collisions --> in peripheral Au+Au collisions

Answer: Implemented

The X-axis in Fig-4 should be smaller case p_{T}

Answer: Implemented

l#77: "is observed at lower BES-II energies (7.7 – 19.6 GeV) in Au+Au 

collisions"

--> is observed in BES-II Au+Au collisions at s_NN = 7.7 – 19.6 GeV.

Answer: Implemented

Regards

Muhammad Farhan Taseer

Institute of Modern Physics,

CAS, Lanzhou, China.

On Wednesday, 28 August 2024 at 02:44:53 pm GMT+8, webmaster AT star.bnl.gov <webmaster AT star.bnl.gov> wrote:

Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material 

originally submitted by Muhammad Farhan Taseer ( mfarhan_taseer AT yahoo.com ) 

at

https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurement-charge-dependent-directed-flow-STAR-Beam-Energy-Scan-BES-II-AuA-2

Comment:

Dear Farhan,

Nice proceedings. For record, I sign off with following additional 

suggestions.

l#43: in Au+Au collisions --> in peripheral Au+Au collisions

The X-axis in Fig-4 should be smaller case p_{T}

l#77: "is observed at lower BES-II energies (7.7 – 19.6 GeV) in Au+Au 

collisions"

--> is observed in BES-II Au+Au collisions at s_NN = 7.7 – 19.6 GeV.

---

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