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Parameter estimation of inspiralling compact binaries in ground-based detectors: comparison between Monte Carlo simulations and the Fisher information matrix
National licenceIOP Institute of Physics | 2008| -
A template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model
National licenceIOP Institute of Physics | 2007| -
Searching for gravitational-wave signals emitted by eccentric compact binaries using a non-eccentric template bank: implications for ground-based detectors
National licenceIOP Institute of Physics | 2009| -
A template bank to search for gravitational waves from inspiralling compact binaries: I. Physical models
National licenceIOP Institute of Physics | 2006| -
Status of VIRGOPresented by F Frasconi for the Virgo Collaboration.
National licenceIOP Institute of Physics | 2004| -
Commissioning, characterization and operation of the dual-recycled GEO 600
National licenceIOP Institute of Physics | 2004| -
The VIRGO large mirrors: a challenge for low loss coatings
National licenceIOP Institute of Physics | 2004| -
Search for inspiralling binary events in the Virgo Engineering Run data
National licenceIOP Institute of Physics | 2004| -
The last-stage suspension of the mirrors for the gravitational wave antenna VirgoPresented by P Puppo.
National licenceIOP Institute of Physics | 2004| -
Results of the Virgo central interferometer commissioningPresented by F Bondu for the Virgo Collaboration.
National licenceIOP Institute of Physics | 2004| -
A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data
National licenceIOP Institute of Physics | 2004| -
The present status of the VIRGO Central Interferometer*
National licenceIOP Institute of Physics | 2002| -
Data analysis methods for non-Gaussian, nonstationary and nonlinear features and their application to VIRGO
National licenceIOP Institute of Physics | 2003| -
Search for gravitational-wave bursts in LIGO's third science run
National licenceIOP Institute of Physics | 2006|
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