NS/V noise NS/H noise NS/H earthquakes The use of a very dense seismic array to characterize the Cavola, Northern Italy, active landslide body. By P. Bordoni.
LIGO-G030270-00-D Advanced LIGO: Mechanical Systems, Systems Tests and Installation Dennis Coyne PAC-14 Review, 5 June 2003.
Stable levelling and locking methods applicable for borehole very broad band seismic sensors including tilt meters presented at SUPERSITES COORDINATION.
VSR1 summary - post VSR1 Commissioning plans E. Tournefier (LAPP-CNRS) LSC-Virgo meeting Oct 22 nd, 2007.
LIGO-G 020169 -00-D 1 Requirements Environment and constraints Performance requirements Functional requirements.
There is a time for ultra seismic accuracy but that comes after we have located something exciting enough to look at. Since migration before stack almost.
Actuation Electronics For (Near) Future Detectors Alberto Gennai [email protected].
1 Gravitational wave interferometer OPTICS François BONDU CNRS UMR 6162 ARTEMIS, Observatoire de la Côte d’Azur, Nice, France EGO, Cascina, Italy May 2006.
Status of Virgo Gabriele Vajente INFN Pisa and Scuola Normale Superiore di Pisa On behalf of the Virgo Collaboration 11 th Gravitational Wave Data Analysis.
Several Fun Research Projects at NAOJ for the Future GW Detectors LIGO Seminar @ Caltech Aug. 8, 2006 Seiji Kawamura National Astronomical Observatory.
Optical Coating Development for the Advanced LIGO Gravitational Wave Antennas Gregory Harry LIGO/MIT - On Behalf of the Coating Working Group - University.
E.T. Design Study & European roadmaps Michele Punturo/Harald Lück.
