https://www.selleckchem.com/pr....oducts/ide397-gsk-43
Measuring the faint polarization signal of the cosmic microwave background (CM not only requires high optical throughput and instrument sensitivity but also control over systematic effects. Polarimetric cameras or receivers used in this setting often employ dielectric vacuum windows, filters, or lenses to appropriately prepare light for detection by cooled sensor arrays. These elements in the optical chain are typically designed to minimize reflective losses and hence improve sensitivity while minimizing potential imaging a
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