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[Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review
- From: Andrew Tamis <andrew.tamis AT yale.edu>
- To: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
- Subject: [Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review
- Date: Wed, 22 Mar 2023 04:32:08 -0400
Hello Nihar,
Thank you for the nice comments, I have implemented them.
I have also received the theoretical predictions from Kyle Lee at MIT, which was normalized differently than my analysis: He normalized both the overall integral and x-axis scaling to Delta(R) rather than log_10(DeltaR). In order to make this comparable, I divided each of my bins by their equivalent length in DeltaR: changing my distribution from d(...)/d(Log_10(DeltaR)) to d(...)/d(DeltaR) and integrated them out to one in that space (Formula Updated on slide 5). Nothing changed about the analysis except for a scaling at the very end, so this is still the same data. Now that they are normalized the same way, I have included the comparisons with Kyle's theory calculations, normalizing his to the same area as mine within the region that they are plotted.
I have updated my plots and uploaded them to drupal here: Preliminary Plots for Energy-Energy Correlator Measurement in p+p Run12 | The STAR experiment (bnl.gov)
Slide 5->6: The lines are placed by eye, In this talk I have defined the DeltaR_Turnover as the leftmost edge of the bin which breaks the linear scaling behavior seen in the hadronization region. My previous slides were inconsistent about this, so I have corrected them. Because this region has some width there are other ways to calculate this, but I show that if one is consistent in a definition, the calculation will yield a value in the same order of magnitude for a given jet pT. The 3.6GeV isn't a set value, just showing that they are all of similar scale: so I have changed this to "2 to 3GeV" to make it less of a strong statement than asserting a value. This value is smaller because I changed the calculation from using average pT to the lower pT bound, which the scheme that the theoretical calculations I received followed.
Slide 9->11: I rephrased the sentence to say what they mean, leaving the abbreviations out, let me know if this works.
Slide 10->12: I rephrased it to "do not need to correct in addition to pT_Jet"
Slide 17->18: The geometric cutoff is due to it becoming more difficult to fit two particles into the cone once the deltaR reaches the jet radius, so an increased jet R allows for the measurement to push into larger deltaR, where we see the quark/gluon region continue.
Best,
Andrew
On Mon, Mar 20, 2023 at 3:31 AM Nihar Sahoo <nihar AT rcf.rhic.bnl.gov> wrote:
Hello Andrew,
Please find my comments on your nice presentation below.
___________
General comment/suggestion to all HP2023 and DIS2023 presenters:
1. Please make a Drupal page for all your preliminary plots and provide
us the link.
If you have already done that, please send us the link.
2. While preparing your analysis plots for "STAR preliminary" request,
please follow the guidance 1-7:
https://drupal.star.bnl.gov/STAR/pwg/common/Preliminary-figures
It saves our time.
_________
SLide:-2
t_f : mention "formation time"
SLide-5:
In plot:
Legend shows all blue, red, green markers are 15-20 GeV/c jet pT. I
think that is not the case. Please correct it. (Slide6)
As this is a PYTHIA study, I would strongly suggest to use open marker
here.
Because you have used the same marker style while plotting the data.
Otherwise it may confuse the audience.
Each dashed line:
Have you used the _expression_ "Lambda_QCD/jet Pt" to find the value of
Delta_R in the left plot?
If not, can you calculate what is the value if you use "ave jet pT" of
these three cases?
Slide6:
"< 𝑝𝑇 𝐽𝑒𝑡 >*∆𝑅𝑇𝑢𝑟𝑛𝑜𝑣𝑒𝑟 ~ 3.6 GeV" Not clear to me what this "3.6 GeV"
implies here?
Where do you get "DeltaR_turnover"? Have you calculated as I mentioned
above? Or just by eye?
SLide7:
"Experimental Measurment at STAR" -> "STAR detector" (all measurements
are experimental) (same on slide8)
You could show other colorful STAR detector pic.
"Must correct for inefficiencies …" ->" Must correct for detector
effects…"
Slide9
Mention what is "DeltaR_jet" and "DeltaR_track"?
Both left and right slide, X, Y axis labels are too small. Please
increase the size.
Put Unit on both the axises.
Slide10
Both left and right slide, X, Y axis labels are too small. Please
increase the size.
Put Unit and title on both the axises.
"..do not need to correct additionally to 𝒑𝑻𝑱𝒆𝒕 " -> I this we don't
need correction for EEC but "pTjet range" needs to be corrected. Is not
that?
Slide17:
"quark/gluon region continues longer before geometric cutoff" -> do you
understand why it is so?
Cheers
Nihar
On 2023-03-17 04:34, Andrew Tamis via Star-hp-l wrote:
> Hello Barbara,
>
> Thank you very much for the nice comments. I have implemented all of
> them and uploaded my new version, here are some notes on some of the
> changes
> -s6 Added a note that I calculate average Jet pT from PYTHIA spectra
> -s10 For the second part being more technical, i have now moved my
> GEANT statistical uncertainty explanation to a previous slide where I
> can talk about it in more detail, and changed some of the wording
>
> On Slide 16 I have included a comparison with the previous CMS result,
> showing that the <pT jet>*Rturnover produces something in the same
> order of magnitude, showing that this result is consistent. I believe
> this is significant, with how quickly the log axis moves and the
> ambiguity in declaring the start of the turnover region (If I say the
> previous bin on my plot is the start of the transition region I get
> 2.7GeV), please let me know how you think I should present this point.
>
> Let me know if you have any other suggestions.
>
> Best,
> Andrew
>
> On Wed, Mar 15, 2023 at 8:49 AM Barbara Trzeciak via Star-hp-l
> <star-hp-l AT lists.bnl.gov> wrote:
>
>> Hi Andrew,
>>
>> please find below my comments to your nice slides.
>>
>> - s2: clustered -> Clustered (to be consistent with other bullet
>> points)
>> - s3: add full reference to the right plot (same s4)
>> - s5,6: please improve the quality of the number values in the Jet
>> pT legend
>> - s5: "Curve normalized to integrate to" - you can make the font of
>> this bullet point a bit smaller, as it's a note
>> - s6: the arrows are displaced to the right from the dashed lines
>> - s6: when you calculate the turnover point, how do you get the
>> average jet pT for each range ? Do you use the PYTHIA spectra ?
>> - s6: you have twice "Average" in the equation, <p_T^Jet> shall be
>> enough.
>> - s6: higher Jet transverse -> higher jet transverse
>> - s7: I would suggest putting here a scheme of the STAR, with the
>> most important detectors marked.
>> - s7: I would remove this "triggers on and", you mention trigger at
>> the end of the sentence.
>> - s8: Add on the plots information about simulations, system,
>> energy. There's a line on the right side of the left plot.
>> - s8: right plot - add y-axis title, increase size of data points
>> and use different markers.
>> - s8: for Jet Pt -> x for Jet p_T
>> - s10: y-axis - add [%], improve quality of the legend, make the
>> lines wider and different styles, and I would decrease the y-axis
>> max so that all the contributions are visible. Add the "STAR
>> preliminary" label. I would suggest also using the same description
>> of the sys. unc. in the legend as you have on the previous slide.
>> - s10: I would suggest making bullet points to be consistent with
>> the style of other slides, and unify the font. Also, the second part
>> of the text on this slide sounds too technical, could you please
>> improve it and make a short point(s).
>> - s11: make the data point markers and font larger (e.g. you can
>> move the "STAR Preliminary" label up to have more space of the
>> text). The two plots look displayed relatively to each other. Same
>> for other result plots.
>> - s11: "Distribution moves " - this might not be clear. Maybe:
>> average of the distribution moves to lower angles ...
>> - s12: I would remove "Doing some estimations ...", remind instead
>> of the equation you show earlier
>> - s13, 14: make the style of the plots consistent with the previous
>> plots, increase the font size, etc. Also, you can merge from down
>> the lower ratio plots with the upper plots.
>> - s15: add a conclusion bullet
>> - s16: Mark here again to which region each colored band corresponds
>> to - as on slide 12.
>> - s16: Increase the font size of "Increasing R increases ... "
>> - s17: Increase the legend font size, and you don't need "Corrected
>> Data:"
>> - s17: Make the conclusion sentence standing out more, and remind
>> what is the Effect - transition region moves to smaller opening
>> angles with increasing jet pT
>> - s17: Higher Jet Radius -> higher jet radius
>> - Please consistently make all the slides' titles bold (or not bold)
>>
>> Cheers,
>> Barbara
>>
>> On Tue, Mar 14, 2023 at 2:34 AM webmaster--- via Star-hp-l
>> <star-hp-l AT lists.bnl.gov> wrote:
>>
>>> Dear Star-hp-l AT lists.bnl.gov members,
>>>
>>> Andrew Tamis (andrew.tamis AT yale.edu) has submitted a material for
>>> a review,
>>> please have a look:
>>> https://drupal.star.bnl.gov/STAR/node/62953
>>>
>>> Deadline: 2023-03-26
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster AT www.star.bnl.gov
>>> _______________________________________________
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[Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
webmaster, 03/13/2023
- <Possible follow-up(s)>
-
[Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
webmaster, 03/13/2023
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Barbara Trzeciak, 03/15/2023
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Andrew Tamis, 03/16/2023
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/20/2023
-
Message not available
-
[Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Andrew Tamis, 03/22/2023
- Re: [Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Nihar Sahoo, 03/22/2023
- Re: [Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Barbara Trzeciak, 03/22/2023
- Re: [Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Yi Yang, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Helen Caines, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Nihar Sahoo, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Nihar Sahoo, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Andrew Tamis, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Andrew Tamis, 03/24/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Barbara Trzeciak, 03/24/2023
- Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review, Yi Yang, 03/24/2023
-
[Star-hp-l] Fwd: STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Andrew Tamis, 03/22/2023
-
Message not available
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/20/2023
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Andrew Tamis, 03/16/2023
-
Re: [Star-hp-l] STAR presentation by Andrew Tamis for Hard Probes 2023 submitted for review,
Barbara Trzeciak, 03/15/2023
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