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Light Field Camera Calibration
Light Field Camera Calibration. Finally, the targets y are computed by drawing randomly from a gaussian with the desired covariance and mean and adding gaussian noise with standard deviation exp(hyp.lik). The standard normal distribution has zero mean and unit standard deviation.

Finally, the targets y are computed by drawing randomly from a gaussian with the desired covariance and mean and adding gaussian noise with standard deviation exp(hyp.lik). The second parameter, σ, is the standard deviation. Binary function to apply, specified as a function handle.
The Standard Normal Distribution Has Zero Mean And Unit Standard Deviation.
Binary function to apply, specified as a function handle. Fun must support scalar expansion, such that if a or b is a scalar, then c is the result of applying the scalar to every. For more information, see compatible array sizes for basic operations.
The Normal Inverse Function Is.
Ordinarily, we would only directly call the gp function. The first parameter, µ, is the mean. The second parameter, σ, is the standard deviation.
The Above Code Is A Bit Special Because We Explicitly Call The Mean And Covariance Functions (In Order To Generate Samples From A Gp);
Finally, the targets y are computed by drawing randomly from a gaussian with the desired covariance and mean and adding gaussian noise with standard deviation exp(hyp.lik).
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