Difference: Galery (2 vs. 3)

Revision 32011-03-05 - GergelyDebreczeni

Line: 1 to 1
 
META TOPICPARENT name="WebHome"

Home
What is Virgo ?
People
CBwaves
GPU_inspiral
Computing activities
Analysis activities
Theory
Galery
Publications
Events
Useful links
Getting started
TDK/BSc/MSc/PhD
Archive
Contact
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
Changed:
<
<		design sensitivity.
>
>		design sensitivity.
 
Added:
>
>		 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
View topic | History: r3 < r2 < r1 | More topic actions...
 
This site is powered by the TWiki collaboration platform Powered by Perl This site is powered by the TWiki collaboration platformCopyright &© by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback