Optimizing electron-beam lithography via smaller beam step size and avoiding main-field stitching reduces random and systematic frequency scatter four-fold in superconducting microstrip resonators.
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Simulations of an SKA-Mid survey predict detection of 1.5e4 star-forming galaxies to z~7 with thermal SFR uncertainties of 0.1 dex, enabling constraints on cosmic star formation rate density.
citing papers explorer
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Enhanced electron-beam lithography to reduce the frequency scatter of 200-400 GHz superconducting microstrip resonators for on-chip filterbank spectrometers
Optimizing electron-beam lithography via smaller beam step size and avoiding main-field stitching reduces random and systematic frequency scatter four-fold in superconducting microstrip resonators.
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Tracing the Star Formation History of the Universe through Thermal Free-Free Emission with the SKA
Simulations of an SKA-Mid survey predict detection of 1.5e4 star-forming galaxies to z~7 with thermal SFR uncertainties of 0.1 dex, enabling constraints on cosmic star formation rate density.