1. IceCube Institutional Memorandum Of Understanding (MOU)
    2. Scope of Work
  1. Ohio State University
    1. James Beatty
    2. Ph.D Scientists (Faculty Scientist/Post Doc Grads): 4 (1 3 0)
    3. Faculty:
    4. Scientists and Post Docs:
    5. Students:
    6. General:

Last updated: April 22, 2013


IceCube Institutional Memorandum Of Understanding (MOU)


Scope of Work

 

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Ohio State University


James Beatty


Ph.D Scientists (Faculty Scientist/Post Doc Grads): 4 (1 3 0)

 

 

Labor Cat.
Names
WBS L3
Tasks
WBS 2.1
WBS 2.2
WBS 2.3
WBS 2.4
WBS 2.5
Grand Total
       
Program Management
Detector Maintenance & Operations
Computing & Data Management
Triggering & Filtering
Data Quality, Reconstruction & Simulation Tools
 
PO OSU PO Detector Monitoring Monitoring shifts  
0.02
     
0.02
    Education & Outreach Outreach
0.05
       
0.05
  OSU PO Total  
0.05
0.02
     
0.07
  ROTT, CARSTEN Physics Filters WIMP WG Co-Lead      
0.25
 
0.25
    Detector Monitoring Maintain good run list  
0.10
     
0.10
  ROTT, CARSTEN Total    
0.10
 
0.25
 
0.35
  PFENDNER, CARL Detector Monitoring Maintain good run list  
0.10
     
0.10
                   
  PFENDNER, CARL Total    
0.10
     
0.10
OSU Total    
0.05
0.22
 
0.25
 
0.52
 


Faculty:

Jim Beatty – 10% IceCube


Scientists and Post Docs:

Carsten Rott – WIMP-wg co-lead, Good Run List, data quality, outreach. Currently in transition into a faculty position at Sungkyunkwan University (SKKU) in Korea.

Carl Pfendner - Good Run List, data quality

Mike Stamatikos – GRB analysis tools, outreach – 10% IceCube (Swift, Fermi, ISS)


Students:

 

 

 


General:

Procedures and descriptions for the IceCube good run list have been developed by C.Rott. We are maintaining the good run list and perform associated long-term data-quality and stability tasks. We support integration of the good run list into i3live (C. Pfendner). We d evelop science analysis tools for correlated neutrino searches based upon electromagnetic parameters for each burst (M. Stamatikos).

Our analysis efforts are focused on Dark Matter searches and ultra-high energy neutrinos.

We use the Ohio Supercomputer Center (OSC) for data processing and to production of Monte Carlo event samples.

 

Note: The activities and staffing levels in this MoU are appropriate for the year beginning October 1, 2012.

 

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