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| Description |
English: Noise curves of the gravitational-wave detectors LIGO and Advanced LIGO as a function of frequency together with the characteristic strains of the potential gravitational-wave signals they are designed to measure. |
| Date | |
| Source | http://www.ast.cam.ac.uk/~rhc26/sources/ |
| Author | Christopher Moore, Robert Cole and Christopher Berry |
| Permission (Reusing this file) |
http://www.ast.cam.ac.uk/~rhc26/sources/ |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 16:36, 20 April 2014 | | 1,000 × 637 (61 KB) | BobQQ | {{subst:Upload marker added by en.wp UW}} {{Information |Description = {{en|Noise curves of the gravitational-wave detectors LIGO and Advanced LIGO as a function of frequency together with the characteristic strains of the potential gravitational-wave... |
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