PROCEEDINGS VOLUME 4856
ASTRONOMICAL TELESCOPES AND INSTRUMENTATION | 22-28 AUGUST 2002
Gravitational-Wave Detection
ASTRONOMICAL TELESCOPES AND INSTRUMENTATION
22-28 August 2002
Waikoloa, Hawai'i, United States
Inertial Sensing and Drag-Free Spacecraft
Proc. SPIE 4856, Use of drag-free spacecraft in the detection of low-frequency gravitational radiation, 0000 (26 February 2003); doi: 10.1117/12.456760
Proc. SPIE 4856, Disturbance reduction system: testing technology for drag-free operation, 0000 (26 February 2003); doi: 10.1117/12.458565
Proc. SPIE 4856, Development of hardware for a drag-free control system, 0000 (26 February 2003); doi: 10.1117/12.458567
Proc. SPIE 4856, Position sensors for flight testing of LISA drag-free control, 0000 (26 February 2003); doi: 10.1117/12.458564
Proc. SPIE 4856, Electrostatic modeling for LISA, 0000 (26 February 2003); doi: 10.1117/12.456762
Proc. SPIE 4856, Charging of isolated proof masses in satellite experiments such as LISA, 0000 (26 February 2003); doi: 10.1117/12.461504
Interferometry
Proc. SPIE 4856, LISA phase measurement technique, 0000 (26 February 2003); doi: 10.1117/12.461497
Proc. SPIE 4856, LISA laser noise cancellation test using time-delayed interferometry, 0000 (26 February 2003); doi: 10.1117/12.461501
Proc. SPIE 4856, Bench-top interferometric test bed for LISA, 0000 (26 February 2003); doi: 10.1117/12.458563
Proc. SPIE 4856, LISA: pointing sensor development stand, 0000 (26 February 2003); doi: 10.1117/12.461499
Data and New Techniques
Proc. SPIE 4856, The Cassini gravitational wave experiment, 0000 (26 February 2003); doi: 10.1117/12.458566
Proc. SPIE 4856, Optical displacement sensor (ODS): an inertial reference sensor candidate for LISA, 0000 (26 February 2003); doi: 10.1117/12.461494
Proc. SPIE 4856, Preliminary studies of spherical proof masses in LISA drag-free satellites, 0000 (26 February 2003); doi: 10.1117/12.458562
Gravitational Wave Source Physics
Proc. SPIE 4856, Numerical relativity: maximizing the scientific payoff from gravitational wave detection, 0000 (26 February 2003); doi: 10.1117/12.459025
Proc. SPIE 4856, Gravitational waves from core collapse, 0000 (26 February 2003); doi: 10.1117/12.458864
Proc. SPIE 4856, A new method for estimating binary pulsar coalescence rates, 0000 (26 February 2003); doi: 10.1117/12.458969
Proc. SPIE 4856, Distribution of mass ratios in compact object binaries, 0000 (26 February 2003); doi: 10.1117/12.458968
Source Physics and Gravitation Wave Data Analysis
Proc. SPIE 4856, Probing the neutron star equation of state with gravitational wave detectors, 0000 (26 February 2003); doi: 10.1117/12.459021
Proc. SPIE 4856, Influence of the precession on the search of inspiral binaries with ground-based gravitational wave detectors, 0000 (26 February 2003); doi: 10.1117/12.459016
Proc. SPIE 4856, Analysis techniques for data from resonant-mass detectors, 0000 (26 February 2003); doi: 10.1117/12.459022
Proc. SPIE 4856, Search for gravitational waves in the galaxy with the five-bar network, 0000 (26 February 2003); doi: 10.1117/12.459023
Gravitational Wave Data Analysis
Proc. SPIE 4856, Analysis of data from interferometric gravitational-wave detectors, 0000 (26 February 2003); doi: 10.1117/12.459094
Proc. SPIE 4856, Data analysis with multiple detectors: plans and prospects for coordinated international analysis of interferometric detector data, 0000 (26 February 2003); doi: 10.1117/12.459051
Proc. SPIE 4856, A data analysis technique for detecting a stochastic background of gravitational radiation, 0000 (26 February 2003); doi: 10.1117/12.459018
Proc. SPIE 4856, Merits of coincident observation of energetic cosmic events by astronomical and gravity wave observatories, 0000 (26 February 2003); doi: 10.1117/12.459091
Gravitational Wave Detectors
Proc. SPIE 4856, Resonant detectors and interferometers can work together, 0000 (26 February 2003); doi: 10.1117/12.459052
Proc. SPIE 4856, Status of LIGO, 0000 (26 February 2003); doi: 10.1117/12.459097
The Future of Gravitational Wave Detectors
Proc. SPIE 4856, Advanced interferometer configurations, 0000 (26 February 2003); doi: 10.1117/12.459092
Proc. SPIE 4856, Second generation instruments for the Laser Interferometer Gravitational Wave Observatory (LIGO), 0000 (26 February 2003); doi: 10.1117/12.459090
Proc. SPIE 4856, Test mass materials for a new generation of gravitational wave detectors, 0000 (26 February 2003); doi: 10.1117/12.459019
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