Labor Cat.
|
Names
|
WBS Level 3
|
Tasks
|
WBS 2.1
|
WBS 2.2
|
WBS 2.3
|
WBS 2.4
|
WBS 2.5
|
WBS 2.6
|
Grand Total
|
Program Coordination
|
Detector Maintenance & Operations
|
Computing & Data Management
|
Data Processing & Simulation
|
Software
|
Calibration
|
|||||
KE
|
Xinhua Bai | 2.1.1 Administration
|
SDSMT Inst. Lead
|
0.30
|
0.30
|
|||||
2.1.4 E&O | Education & Outreach for neutrino astronomy and IceCube | 0.08
|
0.08
|
|||||||
2.2.4 Detector Monitoring | IceCube operation monitoring | 0.02
|
0.02
|
|||||||
2.5.3 Reconstruction & analysis | High energy cosmic rays, prompt leptons, fluctuations | 0.50
|
0.50
|
|||||||
2.1.2 Engineering and R&D Support | Detector development and testing | 0.10
|
0.10
|
|||||||
Bai, Xinhua Total | 0.48
|
0.02
|
0.50
|
1.00
|
||||||
GR1 a) | Emily Dvorak | 2.5.3 Reconstruction & physics analysis | IceTop-InIce combined reconstruction development and apply it to data analysis | 1.00 | 1.00 | |||||
Emily Dvorak Total | 1.00 | 1.00
|
||||||||
GR2 b) | Diana Silverio | 2.4.2 Simulation production | Prompt muon in UHE cosmic rays and neutrino flavor study | 0.50
|
0.50
|
|||||
2.5.3 Reconstruction & physics analysis | Prompt muon in UHE cosmic rays and neutrino flavor study | 0.50
|
0.50
|
|||||||
Diana Silverio Total | 0.50
|
0.50
|
1.00
|
|||||||
GR3 | To be recruited in 2019~20 | 2.4.2 Simulation study | Primary energy and mass sensitive parameters for non-contained EAS events | 0.70
|
0.70
|
|||||
2.5.3 Reconstruction & physics analysis | Cosmic ray composition and energy for non-contained EAS events | 0.30
|
0.30
|
|||||||
3rd PhD grad Total | 0.70
|
0.30
|
1.00
| |||||||
South Dakota School of Mines & Technology Total | 0.48
|
0.02
|
1.20
|
2.30
|
4.00
|
Note:
a) : Emily Dvorak will graduate in spring 2020. Funded by NSF
b) : Diana Silverio starts in 2019 summer. Grad 2 and 3 are in IceCube 2018 proposal.
SDSMT_MoU_SOW_2019.0429.docx