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[ascl:2007.020] pygwinc: Gravitational Wave Interferometer Noise Calculator

pygwinc processes and plots noise budgets for ground-based gravitational wave detectors. Its primary feature is a collection of mostly analytic noise calculation functions for various sources of noise affecting detectors, including quantum and seismic noise, mirror coating and substrate thermal noise, suspension fiber thermal noise, and residual gas noise. It is also a generalized noise budgeting tool that allows users to create arbitrary noise budgets for any experiment, not just ground-based GW detectors, using measured or analytically calculated data.

Code site:
https://git.ligo.org/gwinc/pygwinc
Used in:
https://ui.adsabs.harvard.edu/abs/2020arXiv200708550J https://ui.adsabs.harvard.edu/abs/2019PhRvD..99l4043T
Bibcode:
2020ascl.soft07020R

Views: 256

ascl:2007.020
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