Noise in measurement applications is often assumed to be Gaussian due to the central limit theorem, which states that the sum or average of samples from any distribution will approximate a Gaussian distribution as sample size increases. Gauss developed this concept to analyze measurement errors in astronomy, demonstrating that random deviations from true values yield a Gaussian distribution. While real-world data rarely fits this model perfectly, it is generally accepted that noise can be approximated as Gaussian unless influenced by nonlinear biases or low sample sizes, where a Poisson distribution may be more appropriate. Discussions also highlight that while data may appear normally distributed, it can often be contaminated or follow other symmetric distributions. Understanding these nuances is crucial for accurate analysis in noise-based applications.