Propagating spatially varying multiplicative shear bias to cosmological parameter estimation for stage-IV weak-lensing surveys
We consider the bias introduced by a spatially varying multiplicative shear bias (<i>m</i>-bias) on tomographic cosmic shear angular power spectra. To compute the bias in the power spectra, we estimate the mode-coupling matrix associated with an <i>m</i>-bias map using a comp...
Autori principali: | Cragg, C, Duncan, CAJ, Miller, L, Alonso, D |
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Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
Oxford University Press
2022
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