1. Parameter Estimation Using 3.5 post-Newtonian Inspiral Waveforms GWDAW, December 15-18, 2004, Annecy K. Arun, B.R. Iyer, B.S. Sathyaprakash and P. Sundarajan

2. 2 GWDAW-9, Annecy Sensitivity of the instruments

3. 3 GWDAW-9, Annecy Span of the interferometers Detectors have the best sensitivity to black hole binaries with mass in the range 10-200 M  Initial LIGO and Virgo have similar sensitivities for binaries in the range 10-50 M  Advanced LIGO has a span of 15 times greater than Initial LIGO/VIRGO or an event rate 3000 times larger

4. 4 GWDAW-9, Annecy Parameter Estimation at Constant SNR: Coalescence Time

5. 5 GWDAW-9, Annecy Parameter Estimation at Constant SNR: Chirp Mass

6. 6 GWDAW-9, Annecy Parameter Estimation at Constant SNR: Mass Ratio

7. 7 GWDAW-9, Annecy Parameter Estimation at Constant Distance: Coalescence Time

8. 8 GWDAW-9, Annecy Parameter Estimation at Constant Distance: Chirp Mass

9. 9 GWDAW-9, Annecy Parameter Estimation at Constant Distance: Mass Ratio