Minutes of Detector Characterization Teleconference (November 12, 2004)

Present:

Caltech: Peter Shawhan, Patrick Sutton, John Zweizig
Carleton: Nelson Christensen
CSUDH: Ken Ganezer
Florida: Sergey Klimenko
Hobart: Steve Penn
LHO: Dick Gustafson, Mike Landry, Greg Mendell, Fred Raab, Vern Sandberg, Robert Schofield
LLO: Natalia Zotov
Loyola: Marc Cenac, John Whelan
LSU: Gaby Gonzalez
Michigan: Keith Riles
Oregon: Ray Frey, David Strom   



E11 Preparations:


S3 Calibration Status (Mike Landry, Gaby Gonzalez)
Mike summarized the status of the S3 calibration for all three IFO's, giving a talk that had been prepared for the LSC meeting last weekend but was not given, for lack of time. He mentioned that the review committee has been supplemented by John Zweizig, given the committee's workload. Briefly, most of the modelling has now been reviewed successfully, with a small number of tasks to be completed. Validation is nearly complete for Xavi's demodulation technique for determining alpha/beta, and validation of his h(t) frames has begun. An example of the agreement between modelling, measurements, and fits was shown for one dewhitening filter. Cross checks include computing imaginary parts of coefficients that should be real but may not be if modelling is wrong, time evolution of imaginary components, and consistency between calibration determined by a ~150 Hz injected line and the usual ~900 Hz line. Cross checks work very well for H1 and H2, but there is a tiny discrepancy (~1 degree phase) in L1 for the ~900 Hz line. Final results are expected in 2 weeks (again!). Although old S3-era calibrations were used for M5, updated calibrations will be performed for E11 (see above). For S4, the same DC calibration methods will be used, but others may also be explored to beat down the dominant systemic uncertainty. The plan is to have good reference measurements in place <i>before</i> the run starts to allow reliable online calibration and data analysis. There will also be real-time comparisons for different methods to obtain coefficients. By then the photon calibrator should be ready for testing as a cross check.


A.O.B.