This third approach allowed us to refine the GGA5 AF QTL from 156-187 cM (31 cM) to a most probable location confidence interval of 166-173 cM (7 cM) (Table 1).
As can be seen, the most probable time is the interval of 0.3 0.4 s, so it is clearly smaller than the time step (h = 1 s).
This article explains why the particular methods in the manual were selected and describes the adjustments chosen to create a new, flexible method for calculating most probable numbers (MPNs), confidence intervals, and measures of improbability for up to 18 dilutions and up to 1020 tubes per dilution.
Since the ω values are sampled over the frequency domain of interest with a chosen interval, the most probable frequency from this set may have a close neighbour with even higher probability, but which fell between sampling points.
Removed markers were re-attached to the genetic map in the interval of most probable fit (e.g. minimum increase in the number of recombination events).
In these cases, intervals at most probable meta-QTL positions were chosen.
The conditional probability of the occurrence of R in an interval of R, the most probable value of R, and the mean expected value of R are calculated for the first time for the low, moderate, and high solar activity levels to study variations in these statistical parameters with latitude and solar activity.
From this distribution, we find the corresponding mapped interval that contains the most probable pixel value in the corresponding color channel, according to the indices of the dot patterns.
This distribution is known as the posterior, and the highest posterior density (HPD) interval refers to the most probable range of the parameter of interest, given the observed data.
We report the probability of the most probable path for each of the equally probable gene segment sets.
