The Astrophysical Journal · 1995 · 38 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsCosmologyRadio AstronomyCosmic Microwave BackgroundObservational CosmologyAnisotropy MeasurementsCmb Angular Correlation FunctionCmb BispectrumCosmic Microwave Background AnisotropiesCosmic Variance EstimationGaussianity Of Cmb FluctuationsSignal-to-noise RatioSignal-to-noise Ratio Analysis
We compute the three-point temperature correlation function of the COBE Differential Microwave Radiometer (DMR) 2 year sky maps to search for evidence of non-Gaussian temperature fluctuations. We detect three-point correlations in our sky with a substantially higher signal-to-noise ratio than from the first-year data. However, the magnitude of the signal is consistent with the level of cosmic variance expected from Gaussian fluctuations, even when the low-order multipole moments, up to l = 9, are filtered from the data. These results do not strongly constrain most existing models of structure formation, but the absence of intrinsic three-point correlations on large angular scales is an important consistency test for such models.