Seasonal seismic noise variations at the Sardinia site cause only minor changes in Einstein Telescope sensitivity and limit SNR impacts to a few percent for binary neutron star and intermediate mass black hole signals.
Grav.32, 074001 (2015)
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Unresolved compact binary coalescence background acts as additional noise that worsens Frequency-Hough sensitivity for continuous gravitational waves by 7-10% near 7 Hz under Einstein Telescope conditions.
citing papers explorer
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The impact of seasonality over the sensitivity of Einstein Telescope and the SNR of CBC signals at the Sardinia candidate site
Seasonal seismic noise variations at the Sardinia site cause only minor changes in Einstein Telescope sensitivity and limit SNR impacts to a few percent for binary neutron star and intermediate mass black hole signals.
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Impact of coalescence signals on the search for continuous gravitational waves with Einstein Telescope
Unresolved compact binary coalescence background acts as additional noise that worsens Frequency-Hough sensitivity for continuous gravitational waves by 7-10% near 7 Hz under Einstein Telescope conditions.