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Summary

Description
English: Noise curves of the gravitational-wave detectors LISA and eLISA as a function of frequency together with the characteristic strains of the potential gravitational-wave signals they are to measure.
Date
Source http://www.ast.cam.ac.uk/~rhc26/sources/ (now http://rhcole.com/apps/GWplotter)
Author Christopher Moore, Robert Cole and Christopher Berry
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(Reusing this file)
http://www.ast.cam.ac.uk/~rhc26/sources/


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w:en:Creative Commons
attribution share alike
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.

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19 July 2013

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Date/TimeThumbnailDimensionsUserComment
current20:20, 15 April 2014Thumbnail for version as of 20:20, 15 April 20141,000 × 637 (94 KB)BobQQ{{subst:Upload marker added by en.wp UW}} {{Information |Description = {{en|Noise curves of the gravitational-wave detectors LISA and eLISA as a function of frequency together with the characteristic strains of the potential gravitational-wave signals...

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