Difference: Galery (1 vs. 3)

Revision 32011-03-05 - GergelyDebreczeni

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 SNR distribution of a 1.5 - 3.0 MSun component mass non-spinning, circular binary inspiral waveforms injected at 5 Mpc distance and reconstructed with a template bank of the same kind using simulated PSD at nominal detector
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sensitivity-fit.jpg
The noise curve of the Virgo detector in the 40 - 2048 Hz region with fitted model curve.
 . -- GergelyDebreczeni -


The RMKI Budapest Virgo Group

Revision 22010-12-15 - GergelyDebreczeni

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-- GergelyDebreczeni - 2010-12-10
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Home
What is Virgo ?
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CBwaves
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Computing activities
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Theory
Galery
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Archive
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Other GW groups

Images, figures, results of the group


snrdist-5Mpc-taylorf2.png
SNR distribution of a 1.5 - 3.0 MSun component mass non-spinning, circular binary inspiral waveforms injected at 5 Mpc distance and reconstructed with a template bank of the same kind using simulated PSD at nominal detector design sensitivity.
. -- GergelyDebreczeni -


The RMKI Budapest Virgo Group

Revision 12010-12-10 - GergelyDebreczeni

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META TOPICPARENT name="WebHome"
-- GergelyDebreczeni - 2010-12-10
 
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