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Fitting the Universe

In this section we will use our apparatus developed with the use of Maxima, Maple, Mathematica, Fortran and Gnuplot to fit data for the expanding Universe, as I have promised at the beginning of this section.

Right now, I don't have this data in hand, although I have some other data that illutrates the measurements of the so-called deceleration parameter.

For the time being let us put this section on-hold and proceed to the next section that sums up what we have learnt about Fortran, Gnuplot, and some important aspects of numerical computing so far (quite a lot actually).

By the time this sub-section comes up during the course, I should already have some more material here.

Zdzislaw Meglicki