R/D.L.R
In cosmoFns: Functions for Cosmological Distances, Times, Luminosities, Etc

D.L <-
function(z, omega.m = 0.27, omega.lambda = 0.73, H.0 = 71) {
    D.M(z, omega.m=omega.m, omega.lambda=omega.lambda, H.0=H.0)*(1+z)
}

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cosmoFns documentation built on May 9, 2022, 9:10 a.m.

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