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
Parameters Distribution Fit to \(z=4.2\)
Parameters Distribution Fit to \(z=4.6\)
Parameters Distribution Fit to \(z=5.0\)
Power Spectrum
Power Spectrum Difference
Temperature
Effective Optical Depth
WDM Fit to Boera
Parameters Distribution Joint Fit to all redshifts
Parameters Distribution Fit to \(z=4.2\)
Parameters Distribution Fit to \(z=4.6\)
Parameters Distribution Fit to \(z=5.0\)
Power Spectrum
Power Spectrum Difference
Temperature
Effective Optical Depth
WDM Fit to Boera ( Data not corrected for instrument resolution )
Parameters Distribution Joint Fit to all redshifts
Parameters Distribution Fit to \(z=4.2\)
Parameters Distribution Fit to \(z=4.6\)
Parameters Distribution Fit to \(z=5.0\)
Power Spectrum
Power Spectrum Difference
Temperature
Effective Optical Depth