Is the pre-WMAP CMB data self-consistent?
Although individual observational groups vigorously test their datasets for systematic errors, the pre-WMAP CMB observational dataset has not yet been collectively tested. Under the assumption that the concordance model is the correct model, we have explored residuals of the observational data with respect to this model to see if any patterns emerge that can be identified with systematic errors. We found no significant trends associated with frequency, frequency channels, calibration source,...[Show more]
|Collections||ANU Research Publications|
|Source:||New Astronomy Reviews|
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