Calculates the confidence interval of the best power fit for an input data set.
If the noise of y is Gaussian-distributed, you must fit the observations with the Power mode of the Curve Fitting node using the Least Square method to obtain the amplitude and power.
Level of certainty for the confidence interval. confidence level must be greater than 0 and less than 1.
Default: 0.95, which means the probability that the best fit falls between lower bound and upper bound is 95%.
Dependent values. y must contain at least four points.
Independent values. x must be the same size as y.
Weights for the observations.
weight must be the same size as y. weight also must contain non-zero elements. If an element in weight is less than 0, this node uses the absolute value of the element. If you do not wire an input to weight, this node sets all elements of weight to 1.
Amplitude of the fitted model.
Error conditions that occur before this node runs. The node responds to this input according to standard error behavior.
Default: No error
Power of the fitted model.
Upper bound of the confidence interval.
Lower bound of the confidence interval.
Confidence radius of the amplitude of the fitted model.
Confidence radius of the power of the fitted model.
Error information. The node produces this output according to standard error behavior.
In the following illustration, the region between the upper and lower confidence bounds is the confidence interval.
Where This Node Can Run:
Desktop OS: Windows
FPGA: Not supported