The calling sequence for call_t is:
result = calc_t(z,,
,H0=x,w=y,/year)
where x is a value for the hubble constant and y is a value for w (
). For ``normal'' physics, use w = -1 (see section IA above). z can be a scalar or an array. If it is scalar, result is a scalar lookback time. If z is an array, result is an array with the corresponding lookback time for each z value in the array. The parameters
,
must be specified, whereas H0 and w can be omitted (for the effects of this, see section IC below). H0 has to be given in terms of
.
If omitted, H0 is internally set to 1 so the function returns as result the lookback time in terms of H0 (see eq. 2). If w is omitted, it is internally set to -1. If the keyword /year is used, the result is given in years instead of seconds (see section IC below).