Presentations
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M. Benacquista
Sources in the Medium Frequency Band
B. Berger
The View from NSF
G. Billingsley
Sapphire Test Masses: Lowering Thermoelastic Noise
J. Camp
LISA R&D
G. Cella
Reducing the Newtonian Noise Above and Below the Ground
M. Cerdonio
Dual GW Detector
D. Crooks
Frequency Dependent Loss in Coated Silica Substrates
R. DeSalvo
Sapphire Fibres: Effect of Surface Roughness on Thermal Conductivity
F. Fidecaro
High Frequency
L.S. Finn
Below, Between, and Beyond: Sources and Science
G. Gemme
Superconducting Cavities for Detection of High-Frequency GW
M. Hall
Sapphire Fibers: Effect of Surface Roughness on Thermal Conductivity
C. Hardham
Hydraulic Actuators for Advanced LIGO and LIGO I
J. Hough
Closing Remarks
W. Hua
Three DOF Active Isolation of Microseismic Peaks
V. Kalogera
Inspiral Rates for NS-WD Binaries
W. Kells
Thermal Lensing in LIGO
A. Krolak
Resolving Signals in the LISA Data
A. Kuhnert
The ST7 Interferometric Displacement Sensor: Progress Report
A. Melissinos
Detection of High-Frequency GW at LIGO
C. Miller
Intermediate-Mass BH and Gravitational Radiation
K. Numata
Numerical Calculation of Thermal Noise
K. Numata
Direct Measurement of Mirror Thermal Noise
D. Ottaway
QND in Advanced GW Detectors
S. Penn
Frequency-Dependent Loss in Coated Silica Substrates
S. Penn
Investigation of Mechanical Loss from Mirror Coatings in GW Interferometers
M. te Plate
The LISA Technology Package on SMART-2
F. Rasio
Gravitaional Wave Signals from Compact Binary Mergers
pdf with embedded animation
animation only
A. Rüdiger
GW Space Antennas Beyond LISA
S. Sato
Noise Experience of the 20m Run 1km Underground in the Kamioka Mine
[27Mb]
R. Schnabel
Squeezed Light Enchanced Michelson Interferometer
R. Schnabel
Manipulating the Quantum Noise: Squeezing, Entanglement and Teleportation
B. Schutz
The Case for Broadband High-Frequency Detectors
P. Sneddon
Investigations of Mechanical Loss from Mirror Coatings in GW Interferometers
M. Te Plate
The LISA Technology Package on SMART-2
M. Tinto
Optimal Time-Delay Interferometry for LISA
S. Wise
Linewidth-Broadened Fabry-Perot Cavities for Future GW Detectors
K. Yamamoto
Mechanical Loss of Optical Coating at Low Temperature
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06.09.2003
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