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star-hp-l - Re: [Star-hp-l] Dimuon and BHT1 at high luminosity in Run 23

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: "Ma, Rongrong" <marr AT bnl.gov>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] Dimuon and BHT1 at high luminosity in Run 23
  • Date: Mon, 19 Jun 2023 22:30:33 +0530

Hello Rongrong,

We do not have any hp physics proposal in the past BUR 23-25 documents for AuAu runs for Jet measurements except gamma trigger.

So I guess no one has plan also to analyze BHT2 trigger.

I am not sure who is interested in analyzing BHT1 trigger, but it
could at least serve as the bridge between MB and BHT2 triggers for
trigger bias evaluation
It is a good idea. If we need BHT with lower threshold , then BHT1 can serve the purpose.


Nihar


On 2023-06-19 21:36, Ma, Rongrong via Star-hp-l wrote:
Hello Isaac

For the HP-related triggers, what matters is the sampled luminosity
rather the number of events. Of course, the ideal case would be
sampling full luminosity, but as you noted the rates for dimuon and
BHT1 are too high. For BHT2 (Upsilon) and BHT3 (gamma+jet) triggers,
we should allocate enough bandwidths such that they can sample the
full luminosity.

One question: is the BHT2 trigger used for jet measurements in
general?

For the dimuon trigger, our plan is to tighten the trigger time window
cut and apply a pre-scale to reduce it to 1 kHz.

I am not sure who is interested in analyzing BHT1 trigger, but it
could at least serve as the bridge between MB and BHT2 triggers for
trigger bias evaluation.

Best
Rongrong

On Jun 16, 2023, at 5:38 PM, Mooney, Isaac via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hi all,

As I mentioned in the PWG meeting on the 8th, we’ve been asked to
give input on the prescales for HardProbes-related triggers for the
upcoming high-luminosity data-taking period. Specifically, due to
high rates from the dimuon and BHT1 triggers, these may require a
high prescale to limit their bandwidth. Our request is for analyzers
planning to use Run 23 data with these triggers to provide a desired
overall number of events for each trigger in order to meet the
physics goals for the analysis. If we assume a given number of weeks
of running, this then gives a rough estimate of the prescale we
should apply.

I’m also linking my slides from last week

(https://drupal.star.bnl.gov/STAR/system/files/TriggerRates100k_Run23.pdf)
with a few changes, including a rate table on the last slide
estimated by Akio, along with some back-of-the-envelope calculations
I added for the prescale of these two triggers.

Please let us know if you have any questions or input.

Thanks,
Isaac, Nihar, and Yi _______________________________________________
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