ET is a “design study” supported by the European Commission under the Framework Programme 7 (FP7) It is a ~3 years project supported by EC with about.
False alarm rate statistics
Koji Arai – LIGO Laboratory / Caltech LIGO-G1401147-v2.
Testing the black hole no-hair theorem using LIGO extreme mass ratio inspiral events Jonathan Gair, IoA Cambridge “Testing gravity in the next decade”
INDIAN PARTICIPATION IN GRAVITATIONAL WAVE DETECTORS AND TELESCOPES : An Assessment of opportunity and readiness C. S. Unnikrishnan DHEP/Gravitation Group.
Tests of the Newton gravity law at various distances V.N.Rudenko. SAI.MSU, INR RAS Precision Physics & Fundamental Physical Constants, (Dubna, December.
What can gravitational waves tell us about neutron stars? Ben Owen TeV 2006 @ UW MadisonAugust 30, 2006.
The Virgo detector: status and first experimental results Nicolas Arnaud NIKHEF June 20 th, 2003.
What can gravitational waves tell us about neutron stars?
Testing the black hole no-hair theorem using LIGO extreme mass ratio inspiral events
[email protected] | , October 28 2009 LIGO Document ID: LIGO-G0900981 Multivariate Veto Analysis for Real-time Gravitational Wave.
Excess Mechanical Loss From Dielectric Mirror Coatings on Interferometer Test Masses