LIGO-G040336-00-Z Detector Characterization Summary - 2004.8.19K. Riles - University of Michigan 1 Summary of the Detector Characterization Sessions Keith.

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LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of the Detector Characterization Sessions Keith Riles (University of Michigan) LIGO Scientific Collaboration Meeting LIGO Hanford Observatory August 16-19, 2004

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 2 Presentations in DC Sessions Can’t do justice to all of these in this brief summary Will just try to hit the highlights Agenda Lots of interesting talks!

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 3 S4 Planning Pre-S4 engineering runs approaching fast New DMT monitors should be ready for 24/7 running at observatories in Mid-September: More reliable shakedown of monitors More guidance to commissioners on astrophysical issues (e.g, if IFO’s unacceptably glitchy, need time to find sources)  Time is running out!

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 4 Looking ahead to S4 - Scimons Making scimons more effective – discussions underway Longer shift blocks with fewer different scimons (more cost-effective for groups, allows better training; longer-term goal: more LSC students/postdocs at sites) More focus on astrophysical figures of merit More focus on data quality flagging in the control room Groups should make requests for special consideration early – to avoid later use of scimon-swaps

LIGO-G Z S4 Planning Looking ahead to S4 Analysis Feedback First line of defense against astrophysically crappy data: SenseMonitor & other monitors of “expected” sensitivities Next line of defense: DataQual, glitchmon, & other generic glitch finders Next line of defense: BurstMon (& other monitors of realistic astrophysical sensitivity) Last line of defense Quasi-online analysis jobs using actual inspiral template banks, burst ETG’s, etc.  DASWG purview [ volunteers welcome! see Patrick Brady ]

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 6 More on DMT issues Glad to see new astrophysical FOM and other DMT monitors  THANKS! But we need more monitors of known artifacts (see Fred’s list) Embarrassing that we STILL don’t have an airplane monitor! (effects first seen in E1(!) engineering run – April 2000) Upcoming detector investigation camp will have sessions on DMT monitors, including how to write them, with template examplesdetector investigation camp