and so on. The last field gives the lookback time in terms of the fraction of the age of the Universe when the light was emitted. For example, if this number is 0.14, the light was emitted when the Universe was only 14 percent of its present age (with the age depending on the Hubble and deceleration parameters that were input).
Usage: Use the sliders to enter values for the Hubble constant and the deceleration parameter. Then the recessional velocity, distance, look-back time in years, and the fraction of the age of the Universe corresponding to when the light was emitted are calculated for each redshift input in the top field.