|
|
Notes |
Quantify fraction of noise in 5-50 Hz band
due to seismic motion |
*Phil Charlton (CIT)
Dick Greenwood (La Tech) Neven Simicevic (La Tech) |
|
Quantify correlations between GW and other channels | *Nelson Christensen (Carleton)
Adrian Ottewill (Dublin) Steve Penn (Syracuse) |
|
Quantify environmental correlations between sites | Nelson Christensen (Carleton)
Peter Fritschel (MIT) *Mike Landry (LHO) Soumya Mohanty (AEI) Adrian Ottewill (Dublin) Rauha Rahkola (Oregon) *Robert Schofield (Oregon) Julien Sylvestre (MIT) |
|
Identify & catalog environmental disturbances | Masahiro Ito (Oregon)
Soumya Mohanty (AEI) Steve Penn (Syracuse) Rauha Rahkola (Oregon) Peter Saulson (Syracuse) *Robert Schofield (Oregon) Julien Sylvestre (MIT) |
|
Quantify calibration stability & stationarity of data | Warren Johnson (LSU)
*Mike Landry (LHO) Luca Matone (CIT) Szabi Marka (CIT) Benoit Mours (Annecy) |
S,P |
Investigate angular fluctuations | *Gabriela Gonzalez (PSU)
Tiffany Summerscales (PSU) |
S,C |
Check data against detailed tidal prediction | *Fred Raab
David Strom (Oregon) |
|
Investigate source(s) of lock losses | Bill Butler (Rochester)
Dave Chin (Michigan) Dick Gustafson (Michigan) Masahiro Ito (Oregon) *Keith Riles (Michigan) |
S,C |
Quantify timing precision (intra- and inter-site) | Szabi Marka (CIT)
*Daniel Sigg (LHO) |
S,P |
Check data integrity end-to-end | *John Zweizig (CIT)
Peter Shawhan (CIT) |
|
Check data merging | Gabriela Gonzalez (PSU)
*Peter Shawhan (CIT) Patrick Sutton (PSU) |
|
Quantify strength and stability of line noise
in
GW channel |
[Bob Coldwell (Florida)]
*Sergey Klimenko (Florida) Soma Mukherjee (AEI) Bernard Whiting (Florida) |
|
Investigate occurrence and propagation of frequency noise | *Rana Adhikari (MIT)
Matteo Barsuglia (CNRS) Duncan Brown (UWM) Luca Matone (CIT) Andrea Vicere (CIT) |
S,P,C |
Explanation of notes in table:
* = Confirmed leader of investigation teamDescriptions of investigations:
S = Special conditions may be required at times during data run, perhaps dedicated shift
P = Special preparation may be needed before start of E2 run
C = Participation by a detector commissioner may be needed
[] = Not confirmed yet