Multi-band EBL intensity mapping cross-correlated with cosmic shear and galaxy clustering recovers IHL, IGL, and EoR parameters with 10-35% smaller uncertainties than intensity mapping alone.
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B-mode null tests for UNIONS-3500 cosmic shear pass after galaxy size cuts and stellar masking, with an oscillatory pattern from additive shear bias suppressed by excluding CCD angular scales.
Cross-covariances and cross-correlations between Euclid spectroscopic and photometric probes have negligible impact on cosmological parameter constraints.
citing papers explorer
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Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
Multi-band EBL intensity mapping cross-correlated with cosmic shear and galaxy clustering recovers IHL, IGL, and EoR parameters with 10-35% smaller uncertainties than intensity mapping alone.
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UNIONS-3500 Weak Lensing: II. B-mode validation for cosmic shear
B-mode null tests for UNIONS-3500 cosmic shear pass after galaxy size cuts and stellar masking, with an oscillatory pattern from additive shear bias suppressed by excluding CCD angular scales.
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Euclid preparation: 6x2 pt analysis of Euclid's spectroscopic and photometric data sets
Cross-covariances and cross-correlations between Euclid spectroscopic and photometric probes have negligible impact on cosmological parameter constraints.