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K. Arun , B.R. Iyer, B.S. Sathyaprakash and P. Sundarajan

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. Sensitivity of the instruments. Span of the interferometers.

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K. Arun , B.R. Iyer, B.S. Sathyaprakash and P. Sundarajan

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

  2. Sensitivity of the instruments GWDAW-9, Annecy

  3. 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 GWDAW-9, Annecy

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

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

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

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

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

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

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