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Good modeling will constrain the possible values of the parameters being used so that they reflect known physics, but bad 'curve fitting' doesn't limit itself to physical realities.
Current efforts in observational cosmology focus on measuring the most accurate possible values of Hubble's constant and of critical density.
There are three possible values of η: 1. (η < 1).
Three possible values of the overlap parameters are considered.
All possible values of ΣCI range from 1 to 63.
The set of possible values of is given as (31).
The possible values of β are described in [6].
Given the event M = m, the set of possible values of x changes to X ( m ) ≜ { possible values of x : M = m } ⊆ X.
The posterior most possible values of modal parameters and their uncertainties were estimated through Bayesian inference.
The possible values of these elements were also determined for use in the experimentation process.
We obtained all possible values of the parameters μ, β and λ [33].
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