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sphenix-cold-qcd-l - Re: [[Sphenix-cold-qcd-l] ] Vernier Scan Instruction

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  • From: Ralf Seidl <rseidl AT rcf.rhic.bnl.gov>
  • To: sphenix-cold-qcd-l AT lists.bnl.gov
  • Subject: Re: [[Sphenix-cold-qcd-l] ] Vernier Scan Instruction
  • Date: Wed, 10 Jul 2024 16:35:13 +0900

Dear Itaru, all,

I had sent Jamie a list of relevant PHENIX ANs at the begin of the run when we started discussing the Vernier scans. I cannot share the notes here, but many people can obtain them directly. If someone does not have access to the PHENIX pages, please contact me as we can now share PHENIX notes on a case by case level upon PHENIX Spokesperson approval.

AN688 ( 200_62GeV)
AN888 (500GeV)
AN597 (62GeV)

Generally, I agree with Sasha on the triggers. From my recollection we required a fixed number of events rather than a fixed time in the later Vernier scans due to the significantly lower rates at large displacements. The 5 minute scans are more like the short scans that Angelika often does for CAD at the end of fills while we preferred to have more data.

Cheers,

Ralf

On 2024-07-10 12:52, Aidala, Christine wrote:
Dear Itaru and all,

I quickly tried looking for explicit instructions on how to take the
Vernier scan data from PHENIX days, but I couldn't find them, either.
In case it is helpful, I did find a 2005 "PHENIX Focus" didactic talk
by Dave Kawall on how to measure absolute luminosity at RHIC.

Christine

--
Christine A. Aidala
Professor, Department of Physics 
University of Michigan

-----Original Message-----
From: sphenix-cold-qcd-l-request AT lists.bnl.gov
<sphenix-cold-qcd-l-request AT lists.bnl.gov> On Behalf Of Alexander
Bazilevsky
Sent: Tuesday, July 9, 2024 8:50 PM
To: sphenix-cold-qcd-l AT lists.bnl.gov
Subject: Re: [[Sphenix-cold-qcd-l] ] Vernier Scan Instruction

Hi Itaru ans All,

Some correction to my proposal.
After looking more careful in the vernier scan analyses we did in the
past, I found that the vertex distribution evolution vs different beam
displacements was studied with ZDC triggers (as its efficiency is not
z-dependent, unlike BBC/MBD which is z-dependent), so we'd better
increase the collected statistics for ZDC-Coincidence. So, my
corrected proposal for scaledowns:

CLOCK: 10k
MBD N&S >= 1: 10
ZDC Coincidence: 0

(actually almost the same as we run it in PHENIX)

and if we can afford collecting also single-side triggers (just in case):

ZDC-North and ZDC-South: 100
MBD S >= 1 and MBD N >= 1: 500

Regards,
Sasha.

On 7/9/24 9:51 AM, Alexander Bazilevsky wrote:
Thanks, Itaru, for compiling the info!

Besides the scaler (GL1P) data, we also need event data: as a maximal
set - for all triggers included in GL1P, and as a minimal set - for
MBD coincidence trigger and CLOCK (e.g. to study vertex distribution
at each beam position to understand the hour glass effect).

Since during the vernier scan run our rates vary by a few orders of
magnitude, we can not set up reasonable trigger scaledowns which would
provide both good life time and good DAQ rate at each step. Therefore
we used to release the scaledowns for triggers we collect to saturate
the DAQ rate regardless the life time (with the goal to collect as
many as possible of triggers we want).

So, I suggest the following scale downs:

CLOCK: 10k
MBD N&S >= 1: 0
ZDC Coincidence: 0

Not sure how useful could be the one-side trigger data, but if we can
afford enabling them, I'd suggest the scaledowns:
ZDC-North and ZDC-South: 10
MBD S >= 1 and MBD N >= 1: 50

In this configuration, the major bandwidth will be occupied by CLOCK
and MBD N&S, and only a few % for all other triggers (not necessary,
but may be useful).

Regards,
Sasha.



On 7/9/24 5:01 AM, Itaru Nakagawa wrote:
Dear Sasha and Ralf,

 Here is the draft instruction for the vernier scan. Unfortunately I
cannot find any instruction of the data taking in PHENIX, but here is
what I think is the procedure. Please have a look and send me feedback.

Best regards,

-itaru



--
Alexander Bazilevsky
Brookhaven National Laboratory, Bldg. 510D, 2-232 Upton, NY 11973 Tel:
631-344-3712
Email: shura AT bnl.gov
-------------------------------------------------



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