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.