In her paper Boera reports two measurements of the powers spectrum, one of the is corrected for instrument resolution.
Using the corrected measurement to do the fit:
CDM Fit to Boera
Parameters Distribution Joint Fit to all redshifts
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Parameters Distribution Fit to \(z=4.2\)
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Parameters Distribution Fit to \(z=4.6\)
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Parameters Distribution Fit to \(z=5.0\)
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Power Spectrum
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Power Spectrum Difference
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Temperature
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Effective Optical Depth
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WDM Fit to Boera
Parameters Distribution Joint Fit to all redshifts
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Parameters Distribution Fit to \(z=4.2\)
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Parameters Distribution Fit to \(z=4.6\)
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Parameters Distribution Fit to \(z=5.0\)
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Power Spectrum
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Power Spectrum Difference
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Temperature
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Effective Optical Depth
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WDM Fit to Boera ( Data not corrected for instrument resolution )
Parameters Distribution Joint Fit to all redshifts
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Parameters Distribution Fit to \(z=4.2\)
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Parameters Distribution Fit to \(z=4.6\)
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Parameters Distribution Fit to \(z=5.0\)
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Power Spectrum
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Power Spectrum Difference
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Temperature
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Effective Optical Depth
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