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abstract
has been analyzed under the assumption of a Gaussian autocorrelation function (Cheng et al.,1994). The variety of possible power spectra and the presence of small scale ($\leq$ 15 arcminutes) structure in these data which is spectrally consistent with a Planck function has motivated the exploration of additional models. We present the results of extending our prior analysis to a flat spectral model as well as a family of CDM models.
