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Asia/Shanghai
Tsung-Dao Lee Institute/N6F-N630 - Smart Classroom (Tsung-Dao Lee Institute)
Tsung-Dao Lee Institute/N6F-N630 - Smart Classroom
Tsung-Dao Lee Institute
Also at Room 603, New Science Building #5, Minhang Campus
15
Description
点击链接入会，或添加至会议列表：
https://cern.zoom.us/j/4042031778
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Speaker: Bai-Hong Zhou (TDLI, SJTU)
Today's focus:
[ssWW]:- Produced signal samples with systematics;
- Use TrexFitter to obtain the new significance results
- For LL, (exp) sig is 2.0, for LX: (exp) sig is 7.1;
- Larger than expected, due to lack of fake samples;
[Hyy*]:
- Updated all the combined results with new workspace provided;
- Draw the m_lly plots for the best fit;
[DarkSHINE FastSimu]:
- Used the H5 provided by Xuliang to migrate Qibin's Calo-VQ to DarkSHINE experiment;
- The detector struction changes have done;
Plans:
[ssWW]:
- Check the systematics impact for ParT;
- Add the WZ CR to trex fitter process;
[Hyy*]:
- Derive the delta mu results for each systenatics;
[DarkSHINE FastSimu]:
- Use Calo-VQ to see the fast simulation results in DarkSHINE experiment;
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Speaker: Zhiyu Zhao (TDLI, SJTU)
Today's focus:
[STCF EMC]:- A timing resolution of 600 ps for MIPs has already been achieved with pure CsI crystals. Since the crystals themselves are relatively large in volume (about 6*6*28 cm^3), the USTC professor suggested me to study the consistency of the timing resolution for particles incident at different positions.
- Using cosmic rays, I studied the crystal’s response to particles hitting different positions along the crystal’s length. I found that：
- The timing resolution is better at positions closer to the sensor
- The closer the impact point is to the sensor, the larger the signal amplitude and the shorter the detection time. This suggests that timing information may be used to infer where the energy is deposited within the crystal.
- I built a simple setup to collect cosmic-ray particles incident along the crystal’s length. In this configuration, the energy deposition is larger, but the event rate is very low, so long-term running is needed to collect sufficient data.
[DarkSHINE ECAL Prototype]:
- Investigate the mechanical structure of the similar crystal prototype designs, such as CRINLIN, CEPC ScW ECAL, CMS MTD BTL. Plan to discuss with USTC professor.
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Speaker: Matthias Tartarin (TDLI, SJTU)
Today's focus:
[Hyy*]:- Prepared and presented the slides for the Unblinding request (for the Photons sub-group meeting Yesterday).
[ZZy]:
- Prepared small updates to the Run-3 ZZy TDLI prepration slides:
- Already included small updates on some plots of interests: Using raw datasets for Zy background (for comparison), and added the "most probable candidate" ZZ pile-up sample to the reproduction of Figure 8.2 (<- I will put them in the Appendix, the ZZ contribution is maybe a bit large).
- Will include the update from Linjing to the slides, when available (about list of available MC sample; and the update on signal XS scaling).
- ttH candidate sample changed: Lijing modified the sample .txt file, and I re-submitted the sample to the chain (grid/download/merge/plot production) these last two days: OK.
- ttH candidate sample changed: Lijing modified the sample .txt file, and I re-submitted the sample to the chain (grid/download/merge/plot production) these last two days: OK.
- Already included small updates on some plots of interests: Using raw datasets for Zy background (for comparison), and added the "most probable candidate" ZZ pile-up sample to the reproduction of Figure 8.2 (<- I will put them in the Appendix, the ZZ contribution is maybe a bit large).
- Began to read again the Run-2 INT note to anticipate future discussions. Will take more time for this.
Plans:
- No clear tasks. I am up-to-date on the different items, and will continue in that direction.
- [ZZy]: Will have the last meeting before presentation with Linjing this afternoon. After that I will circulate final slides to the group.
- [VBS kappa_lambda]: Could not update this work last week ; Still on the to-do list high priority.
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