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Summary

Description
English: Design sensitivity of Advanced LIGO interferometer with major noise sources, maximum sensitivity is around 500 Hz
Date
Source https://link.springer.com/article/10.1007%2Fs41114-019-0018-y
Author Stefan L. Danilishin, Farid Ya. Khalili, Haixing Miao

Licensing

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Captions

Design sensitivity of Advanced LIGO interferometer with major noise sources, maximum sensitivity is around 500 Hz

29 April 2019

image/webp

53d25bc3298a615a0a3b63611a54e914393e1208

88,538 byte

545 pixel

765 pixel

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Date/TimeThumbnailDimensionsUserComment
current20:39, 13 January 2022Thumbnail for version as of 20:39, 13 January 2022765 × 545 (86 KB)DabedUploaded a work by Stefan L. Danilishin, Farid Ya. Khalili, Haixing Miao from https://link.springer.com/article/10.1007%2Fs41114-019-0018-y with UploadWizard

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