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Using COBE-DMR 4-year data, we find a general expression yielding thelikelihood distribution in the 3-dimensional parameter space spanned by thespectral index $n$, the spectral amplitude $a_{10}$ and the false-vacuumdensity parameter $\Omega_\Lambda$. Using such simple expression, the range ofpossible normalizations, within a given likelihood interval from top-likelihoodnormalization, is readily found, with fair approximation, for any model withtotal density parameter $\Omega_o = 1$ and assigned $n$ and $\Omega_\Lambda$.Comment: 19 pages, 7 figures. Added references. Accepted for publication in  Ap

Likelihood Distribution for Models with Cosmological Constant fromCOBEData