Presents one-component KL as a lower-effort alternative to full KL for cosmic shear that simulations show is not yet competitive with WL for shallow HI radio surveys but could exceed WL for deeper spectroscopic surveys with stronger emission lines.
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Cosmic shear with one component and its application to future radio surveys
Presents one-component KL as a lower-effort alternative to full KL for cosmic shear that simulations show is not yet competitive with WL for shallow HI radio surveys but could exceed WL for deeper spectroscopic surveys with stronger emission lines.