Analysis and comparison of main sources limiting the Virgo and GEO sensitivities: control noise
Analysis and comparison of main sources limiting the Virgo and GEO sensitivities: diffused light and acoustic couplings
Analysis and comparison of main sources limiting the Virgo and GEO sensitivities: detectors long term behavior
Comparison of characterization methodologies: noise non stationarity monitor
Comparison of characterization methodologies: automatic noise budget
Comparison of characterization methodologies: detector automation and operation procedures
Reciprocal exchange of software tools: discuss tools, identify possible benefits of the exchange
Reciprocal exchange of software tools: study compatibility and implementation of the HACR algorithm at Virgo
The beam centering project
The alignment simulations project: the controllability using row vector orientation
Row angles as a measure for the sensing matrix quality
A Fabry Perot Cavity example
The VIRGO Layout
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