Quote by marcus
We seem to be coming from widely different places. The matter content has been measured. The standard LambdaCDM model gives the simplest good fit to the data and Lambda has been measured. From my perspective the distance to the cosmic event horizon is knownas I recall some 15 billion ly.

Here again I would say that we "measure" supernova luminosities and redshifts, CMB photon redshifts etc. Then we fit a certain model to these measurements to determine model parameters, like lambda. Likewise, we do not observe acceleration, except within this certain mathematical framework (and indeed you can find some (unrealistic) models which fit the supernovae and CMB data (BAO gives enough tension to rule the simple models out) which are locally decelerating everywhere). In these models you would not have a cosmic event horizon at all.
I think the Lineweaver article is very reasonable, but I also felt like there should be a proviso that this relies heavily on the assumptions put into the standard cosmological model.