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
Matthias Tartarin(TDLI/SJTU)
Description
点击链接入会,或添加至会议列表:
https://cern.zoom.us/j/4042031778
10:00
→
10:05
Introduction & Announcements
Meeting's note: After the meeting
Today's focus:
[1st project/analysis: XXX ]:
item 1
sub-item 1
sub-item 2
item 2
[...]
[2nd project/analysis: XXX ]:
item 1
item 2
[...]
[...]
Plans:
[optional: indicate which project/analysis it refers to] item 1
[optional: indicate which project/analysis it refers to] item 2
10:05
→
10:15
Status10m
Speaker:
Kang Yu(TDLI, SJTU)
10:15
→
10:25
Status10m
Speaker:
Linjing Duan(TDLI, SJTU)
Today's focus:
[CEPC Zvvy nTGC]:
cross-checked the fitting results with Danning: the 1D results look fine, while the 2D results still need theory discussion.
I have drafted the theoretical framework section of the paper.
discussed with Yuning and helped complete the CEPCSW environment setup and run the full simulation workflow successfully.
Plans:
plan to finalize the systematics part by defining the signal and background uncertainties and implementing the corresponding nuisance parameters in the fit.
plan to draft the simulation section of the paper
10:25
→
10:35
Status10m
Speaker:
Jun Wei Lok(TDLI, SJTU)
10:35
→
10:45
Status10m
Speaker:
Zelin Yan(TDLI, SJTU)
10:45
→
10:55
Status10m
Speaker:
Bai-Hong Zhou(TDLI, SJTU)
10:55
→
11:05
Status10m
Speaker:
Xuliang Zhu(TDLI, SJTU)
11:05
→
11:15
Status10m
Speaker:
Zhiyu Zhao(TDLI, SJTU)
11:15
→
11:25
Status10m
Speaker:
Haidar Mas'ud Alfanda(TDLI, SJTU)
11:25
→
11:35
Status10m
Speaker:
Matthias Tartarin(TDLI, SJTU)
11:35
→
12:30
REU: Undergrad Research Discussions
11:35
Status5m
Speaker:
Peixu Teng(SPA, SJTU)
11:40
Status5m
Speaker:
Zhijing Zhang(CCNU & TDLI/SJTU)
Today’s focus:
Gain a detailed understanding of the basic structure and working principle of the ECAL in STCF through the CDR.
Test the energy and time resolution of 1 GeV electrons under background‑free conditions.
Plans:
Use OSCAR to simulate the energy response of photons from 0.1 GeV to 3.5 GeV, and obtained the energy, time, and position resolution curves.