Joe Suina and Dale Ouimette. Human gravity gradient noise in interferometric gravitational wave detectors – Thorne, Kip S. Two point correlation function – Nakagawa, N. Their combined citations are counted only for the first article. Search templates for gravitational waves from inspiraling binaries: Review of 12m mode cleaner task.
Physical review letters 24 , , Huang and Peter R. University of Texas Rio Grande Valley. Will the level of seismic noise at livingston observatory interfere with the detection of gravity waves from binary inspirals?. Optimal strategies for sinusoidal signal detection – Allen, Bruce et al. Corning data sheet New citations to this author.
Malik Rakhmanov, Ph.D.
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Science Thermal noise in the initial LIGO interferometers. Mirror thermal noise in interferometric gravitational wave detectors – Rao, Shanti Raja.
Physical review letters 13, tyesis CleaverGerald Bryan Cleaver.
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Scientific operation of LIGO. Two point correlation function – Nakagawa, N. Scattered light control in LIGO. Information References Citations 0 Files Plots.
Applied Optics-OT, 38 Studies of Laser Interferometer Design and a vibration isolation system for interferometric gravitational wave detectors. The Astrophysical Journal Letters 2L22 mlik, Adhikari Professor of Physics, Caltech Verified email at caltech. New articles by this author. Olivier Debieu associate professor Verified email at ensiacet. Physical Review X 6 4, Core optics components requirements.
Presented at fhesis AprilLSC meeting. The Astrophysical Journal Letters 2L13 Seismic gravity gradient noise in interferometric gravitational wave detectors – Hughes, Scott A.
Applications of Classical Physics, volume 1. Sheila Rowan and Marty Fejer.
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The TNI first test cavity lock. Energy dissipation in the pendulum mode of the test mass suspension of a gravitational wave antenna – Braginsky, V.
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Mirror thermal noise in interferometric gravitational wave detectors – INSPIRE-HEP
Renata Kallosh Stanford University Verified email at stanford. The Half infinite mirror with uniform loss – Nakagawa, N. Feedforward reduction of the microseism disturbance in a long-base-line interferometric gravitational-wave detector – Giaime, J.
Laser beams and resonators. Direct measurement of mirror thermal noise. Internal thermal noise in the LIGO test masses: Signal-to-noise for inspiral, merger, and ringdown – Flanagan, Eanna E.