In this part, we present the construction of the diagram of Hubble of Nos 4 supernovæ remote having gained from measures to the filters corresponding to the filters B and V in their reference frame.
We initially have the results of the estimate of the parameters of their lightcurve.
In the second time, we present how, starting from the supernovæ close studied earlier, we build the diagram of Hubble their diagram of Hubble out of B.
Lastly, we present the estimates of the cosmological parameters deduced from these measurements.