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Status of GEO600

Status of GEO600. Benno Willke for the GEO600 team. Aspen Meeting Aspen CO, January 2005 LIGO-G050030-00-Z. Sensitivity Improvements. Transition Commissioning - Observing. overnight runs Aug04 – Jan05: 1405h (duty cycle: 93.7%). Central Building. Tube / Trench.

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Status of GEO600

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  1. Status of GEO600 Benno Willke for the GEO600 team Aspen Meeting Aspen CO, January 2005 LIGO-G050030-00-Z

  2. Sensitivity Improvements

  3. Transition Commissioning - Observing overnight runs Aug04 – Jan05: 1405h (duty cycle: 93.7%)

  4. Central Building

  5. Tube / Trench

  6. Clean Room / Control Room

  7. Reaction Pendulum

  8. GEO600 optical layout 600m Attenuated to 6W interferometer with dual recycling mode cleaner 12W laser 1% Transmission detector

  9. HPD lock + New MI+SR servo SR bench scattering Sensitivity progress (highlights) Typical S3

  10. Sensitivity – Jan 2005 h(f) [1/sqrt(Hz)] Frequency [Hz]

  11. Sensitivity Change with Heater Power

  12. Amplitude Noise Coupling

  13. PRC 72 * D ( 765Hz) 72 * D ( 765Hz) 119* D (1.26kHz) 119* D (1.26kHz) SRC broad- band 1.86kHz 2.3kHz 1.1kHz 2.2kHz SRC detuned to 1.1 kHz -119 * f -72 * f 0 72 * f 119 * f PRC PRC PRC PRC SR-sidebands SR-sidebands SR-sidebands carrier MI-sidebands broadband 1.1kHz detuned 2kHz detuned Unbalanced Sidebands

  14. Optical Gain

  15. Calibration

  16. optical On-line optical TF measurements P and Q CAL actuator

  17. Calibration progress • On-line calibration of both output quadratures HP and HQ • Work on optimal combination is underway • Estimation of optical parameters in real-time in control room • On-line calibration leads to overnight runs

  18. Combining HP and HQ - result • HQ’ contains almost no signal compared to HP’ • Where noise behaves like cal lines, we have apparent displacement • Useful diagnostic for noise hunting (?)

  19. Overnight Runs – Jan 14th

  20. Noise Projections

  21. Summary & Outlock • GEO600 runs with dual-recycling on large baseline detector including calibration • sensitivity improved by two orders of magnitude since S3-I • data taking over night and on weekends with high duty cycle • next steps: • LSC–S4 science run • increase injected power • increase power recycling gain • improve noise models and increase sensitivity • convert GEO into observatory • GEO-HF

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