Before exploring the results of the global fit in detail, some important general remarks about global fitting are discussed.
We allowed β to be a fitting parameter, with β ∼ 8 achieving the best global fit to the FECs for all three hairpin sequences.
Instead, we use what is called a global fit: If the cMSSM is true, it not only predicts a bunch of new particles, such as dark matter.
A global fit approach has been employed to obtain the spectral characteristics of the sources.
Global fit criteria are also found to support the detection of measurement misspecification.
The line corresponds to Equation 5, with k obtained by the global fit.
The line is the survival fraction modeled by Equation 4 using the parameters determined by the global fit (R = 0.96).
The Rasch model can be tested, not only with specific item fit values, but also with global fit statistics.
An improved global fit to the data was achieved through applying a unique technique utilizing the Fokker-Plank equation with a non-linear rigidity-dependent diffusion coefficient.
For the data of the awake group and the anesthetized group, independent fits were compared to a global fit that shared the rate of decay.
Several global fit measures were considered.
