A review of sampling distributions and the univariate Gaussian

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Outline

  • The following topics will be covered in this lecture:
    • Sample statistics
    • Sample random variables
    • Sampling distributions
    • The univariate Gaussian distribution
    • Properties of the univariate Gaussian
    • The central limit theorem

Sample statistics

  • The goal statistics is to use a numerical summary of data from a small, representative sample to say something general about the larger, unobservable population or phenomena.

  • The measures of the population are referred to as parameters.

  • Parameters are generally unknown and unknowable.

    • For example, we cannot exactly compute the mean sea-surface temperature globally, as it is impossible to take all such measurements.
  • However, if we have a representative sample, we can compute the sample mean.

    • Numerical values like the sample mean computed from data are referred to as statistics.
  • The sample mean will almost surely not equal population mean, due to the natural variation (sampling error) that occurs in any given sample.

    • However, if we have a good probabilistic model for the population, we can use the sample statistic to estimate the general, unknown population parameter.
  • RVs and probability distributions give us the model for estimating population parameters.

  • Note: we can only “find” the parameters exactly in very simple examples like games of chance.

  • Generally, we will have to be satisfied with estimates of the parameters that are uncertain, but also include measures of “how uncertain”.

Sample mean

  • Suppose we have a sample of \( n \) total measurements of some RV \( X \).

    • We will denote these measurements \( x_1, x_2, \cdots, x_n \in \mathbb{R} \), where these refer to fixed numerical values.
    • These may correspond to the value that \( X \) attains upon \( n \) independently replicated trials.
The (arithmetic sample) mean
Given measurements \( x_1,\cdots,x_n \) of the RV \( X \), we say that the sample mean is defined \[ \text{Sample mean} = \hat{x} = \frac{x_1 +x_2 +\cdots + x_n}{n}= \frac{\sum_{i=1}^n x_i}{n} \]
  • We remark that \( \hat{x} \) is a fixed numerical value depending on the particular sequence of outcomes \( x_1,\cdots, x_n \) observed.

    • Due to this fact, with respect to a new sample of size \( n \), we may attain a new value for the sample mean.

Sample variance and standard deviation

  • We can similarly define the sample variance and standard deviation as follows
Sample standard deviation
Given measurements \( x_1,\cdots,x_n \) of the RV \( X \), we say that the sample standard deviation \[ \hat{\sigma} = \sqrt{\frac{\sum_{i=1}^n\left(x_i - \hat{x}\right)^2}{n-1}} \]
  • Note that the numerator in the above accounts for the fact that one degree of freedom has been utilized in the computation of \( \hat{x} \).
Sample variance
Given measurements \( x_1,\cdots,x_n \) of the RV \( X \), we say that the sample variance \[ \hat{\sigma}^2 = \frac{\sum_{i=1}^n\left(x_i - \hat{x}\right)^2}{n-1} \]
  • For the same reasons discussed for the sample mean, the sample standard deviation and variance will tend to differ depending on the particular sequence of outcomes \( x_1,\cdots, x_n \) measured.

  • This discrepancy is what we call sampling error, in which the random variation in a sample of a fixed size \( n \) upon replication produces differences in the computation of a statistic.

  • For this reason, we may also consider a probabilistic model for the sample statistic, depending on the replication of measurements.

Sample random variables

  • Specifically, suppose that we want to obtain an estimate of a population parameter, where the population is modeled with a RV \( X \).

  • We know that before the data are collected, the observations are considered to be RVs,

    • i.e., we treat an independent sequence of measurements of \( X \),

    \[ X_1, X_2, \cdots , X_n \]

    • as RVs all drawn from a parent distribution \( X \sim P \) (where the CDF will define the distribution).
    Random sample
    The RVs \( X_1 , X_2, \cdots , X_n \) are a random sample of size \( n \) if the \( X_i \)’s are independent RVs and every \( X_i \) has the same probability distribution.
  • We then say that the measurements we obtain are possible outcomes of the sample variables \( \{X_i\}_{i=1}^n \);

    • particularly, if we make a computation of the sample mean, \[ \hat{X} = \frac{1}{n} \sum_{i=1}^n X_i \]

    the above is treated as a RV (a linear combination of RVs) which has a random outcome, dependent on the realizations of the \( X_i \).

Sampling distributions

  • More generally, any function of the observations, i.e., any statistic, is also modeled as a RV.
Point estimators
Let \( \{X_j\}_{j=1}^n \) be a random sample. Let \( \theta \) be a parameter of the parent population, defined by the CDF \( P \). If \( h \) is a general function used to compute some statistic estimating \( \theta \), we thus define the RV \[ \hat{\Theta} = h(X_1, \cdots, X_n) \] to be a point estimator for \( \theta \).
  • We call the probability distribution of a statistic or estimator as above a sampling distribution.

    Sampling Distribution
    The probability distribution of a statistic is called a sampling distribution.
  • In this framework, we will distinguish then between the estimator (a random variable) and the numerical value it might attain on a sample of measurements.

    Point estimate
    A point estimate of some population parameter \( \theta \) is a single numerical value
    \[ \hat{\theta} = h(x_1, \cdots,x_n) \] attained as a particular realization of the RV \( \hat{\Theta} \).

Sampling distributions

  • The notion of the “center” of the sampling distribution can be useful as a general criteria for estimators.

  • Formally, we say that \( \hat{\Theta} \) is an unbiased estimator of \( \theta \) if the expected value of \( \hat{\Theta} \) is equal to \( \theta \).

  • This is equivalent to saying that the mean of the sampling distribution of \( \hat{\Theta} \) is equal to \( \theta \).

Bias of an Estimator
The point estimator \( \hat{\Theta} \) is an unbiased estimator for the parameter \( \theta \) if \[ \mathbb{E}\left[\hat{\Theta}\right] = \theta \] If the estimator is not unbiased, then the difference \[ \mathbb{E}\left[\hat{\Theta}\right] - \theta \] is called the bias of the estimator \( \hat{\Theta} \). When an estimator is unbiased, the bias is zero; that is, \[ \begin{align} \mathbb{E}\left[\hat{\Theta}\right] - \theta &= \theta - \theta \\ &=0 \end{align} \]
  • If we consider the expected value to represent the average value over infinite replications;

    • the above says that “over infinite replications of a random sample of size \( n \), the average value of the point estimator \( \hat{\Theta} \) will equal the true population parameter \( \theta \)”.

Sampling distributions

  • Both of the
    1. sample mean \[ \hat{X}= \frac{1}{n}\sum_{i=1}^n X_i; \] and
    2. sample variance \[ \hat{\sigma}^2 = \frac{\sum_{i=1}^n \left(X_i - \hat{X}\right)^2}{n-1} \]
  • are unbiased estimators, i.e., \[ \begin{align} \mathbb{E}\left[\hat{X}\right] = \overline{x}, & & \mathbb{E}\left[\hat{\sigma}^2\right] = \sigma^2. \end{align} \]

  • However, there are theoretical reasons that we can use to show that the sample standard deviation is a biased estimator of the population standard deviation, i.e.,

    \[ \mathbb{E}\left[ \hat{\sigma}\right] \leq \sigma \]

    and it consistently underestimates the true standard deviation.

  • The bias tends to be small, however, and it is still the most practical estimate most of the time for the population standard deviation.

Sampling distributions

  • Recalling that the expected value gives the center of mass of the probability distribution, we should also be interested in the spread of the sampling distribution.

  • As noted before, the variance is a “natural” measure of spread mathematically for theoretical reasons, but it is in the units squared of the original units.

  • For this reason, when we talk about the spread of an estimator's sampling distribution, we typically discuss the standard error.

    The standard error
    Let \( \hat{\Theta} \) be a point estimator of \( \theta \). The standard error error of \( \hat{\Theta} \) is its standard deviation given by \[ \sigma_\hat{\Theta} = \sqrt{\mathrm{var}\left(\hat{\Theta}\right)}. \] If the standard error involves unknown parameters that can be estimated, substitution of those values into the equation above produces an estimated standard error denoted \( \hat{\sigma}_\hat{\Theta} \). It is also common to write the standard error as \( \mathrm{SE}\left(\hat{\Theta}\right) \).
  • With these constructions in mind, we will now introduce one of the most fundamental results of classical statistics.

  • This result establishes the normal or Gaussian distribution in its central importance among distributions.

The univariate Gaussian distribution

  • The Gaussian distribution is considered the most prominent distribution in statistics.
  • It is a continuous probability distribution that has a bell-shaped probability density function.
  • The Gaussian distribution arises from the central limit theorem (CLT),
    • under weak conditions, the sum of a large number of RVs drawn from the same distribution is distributed approximately normally irrespective of the form of the original distribution.
  • This gives mathematical justification to why we see normally distributed data quite often in practice; as was noted by Henri Poincare
  • “Everybody believes in the exponential law of errors [i.e., the normal / Gaussian distribution]: the experimenters, because they think it can be proved by mathematics; and the mathematicians, because they believe it has been established by observation.” — Poincare, Henri “Calcul Des Probabilités.”
  • In addition to the ubiquity of the normal distribution, it can be easily manipulated analytically in equations,
    • this enables one to derive a large number of results in explicit form.
  • Due to these two aspects, the normal distribution is used extensively in theory and practice.

The univariate Gaussian distribution continued

  • Unlike how we defined the density function \( p \) and used this to compute \( \overline{x} \) and \( \sigma \) formerly, we will reverse this for the normal.
  • That is, we will use \( \overline{x} \) and \( \sigma \) to define the density of the normal and parametrize the distribution.
  • Let us use the following notation for compactness where \[ \exp(x) = e^{x}. \]
  • The univariate Gaussian distribution
    Let the Gaussian RV \( X \) have mean \( \overline{x} \) and standard deviation \( \sigma \). The probability density function is given as \[ \begin{align} p(x) = \frac{1}{\sqrt{2\pi}\sigma}\exp\left(-\frac{\left(x - \overline{x}\right)^2}{2\sigma^2}\right). \end{align} \] We will write \( X \sim N\left(\overline{x}, \sigma^2\right) \) to denote that \( X \) has the density described above.
  • Recall how we considered \( \overline{x} \) to be a measure of center and \( \sigma \) a measure of spread.
  • If we vary these two values, we can change the center of mass and the spread of the normal distribution:
Shapes of the normal density.
  • In the case that \( \overline{x}=0 \) and \( \sigma=1 \), we denote \( N(0, 1) \) to be the standard normal distribution.

The univariate Gaussian distribution continued

  • Another useful property of the family of Gaussian distributions is that it is closed under linear transformations.
Closure of the Gaussian under linear transformations
Let \( X_1 \) and \( X_2 \) be independent, Gaussian RVs defined \[ \begin{align} X_1\sim N\left(\overline{x}_1 , \sigma_1^2 \right) & & X_2 \sim N\left(\overline{x}_2, \sigma_2^2 \right). \end{align} \] Then for \( a,b,c \in \mathbb{R} \), the linear combination satisfies \[ aX_1 + bX_2 + c \sim N\left(a \overline{x}_1 + b\overline{x}_2 + c, a^2 \sigma_1^2 + b^2 \sigma_2^2\right) \]
  • This is actually a general property of the family of stable distributions.

  • The closure property above implies that a Gaussian variable can always be “standardized” as,

    \[ \begin{align} X \sim N(\overline{x}, \sigma^2) && \Rightarrow && \frac{X - \overline{x}}{\sigma} \sim N(0, 1). \end{align} \]

  • The closure of the Gaussian under linear transformations has extremely important implications, when we introduce a mechanistic model later.

  • This is at the basis of results for estimators defined in a class of models known as Gauss-Markov models.

    • We will return to this subject shortly.

Central limit theorem

  • Suppose that a random sample of size \( n \) is taken from a normal population with mean \( \overline{x} \) and variance \( \sigma^2 \).

  • By definition of a random sample each observation in this sample, say, \( X_1, X_2, \cdots, X_n \), is a normally and independently distributed RV with mean \( \overline{x} \) and variance \( \sigma^2 \).

  • We conclude that, due to closure of the Gaussian, the sample mean

    \[ \hat{X}= \frac{X_1 + X_2 + \cdots + X_n}{n} \]

    has a normal distribution with mean

    \[ \begin{align} \mathbb{E}\left[\hat{X}\right] &= \frac{\mathbb{E}\left[X_1\right] + \cdots + \mathbb{E}\left[X_n\right]}{n} = \overline{x} \end{align} \]

    • and variance

    \[ \sigma^2_\hat{X}:= \mathbb{E}\left[\left(\hat{X} - \overline{x}\right)^2\right] = \frac{\sigma^2 + \sigma^2 + \cdots + \sigma^2}{n^2} = \frac{\sigma^2}{n} \]

Central limit theorem continued

  • More generally, if we are sampling from a population that has an unknown probability distribution, the sampling distribution of the sample mean will still be approximately Gaussian with mean \( \overline{x} \) and variance \( \frac{\sigma^2}{n} \) if the sample size \( n \) is large.

  • This is one of the most useful theorems in statistics, called the central limit theorem:

    The central limit theorem (CLT)
    Let \( X_1 , X_2 , \cdots , X_n \) be a random sample of size \( n \) taken from a population with mean \( \overline{x} \) and finite variance \( \sigma^2 \) and \( \hat{X} \) be the sample mean. Then the limiting form of the distribution of \[ Z = \frac{\hat{X} - \overline{x}}{\frac{\sigma}{\sqrt{n}}} \] as \( n \rightarrow \infty \) is the standard normal distribution.
  • Put another way, for \( n \) sufficiently large, \( \hat{X} \) has approximately a \( N\left(\overline{x}, \frac{\sigma^2}{n}\right) \) distribution – this says the following.

    • Suppose we take a sample of size \( n \) and compute the sample mean \( \hat{x} \).
    • Then suppose we replicate this sample and record the observed realizations for the sample mean \( \hat{x}_1, \hat{x}_2, \cdots \).
    • If the sample size \( n \) is large, these data points \( \hat{x}_1, \cdots \) will be approximately bell shaped with the following properties:
      • the bell will be centered approximately at \( \overline{x} \), the true population mean;
      • the spread of the data around the center will be given by approximately by the standard deviation \( \frac{\sigma}{\sqrt{n}} \).
    • Particularly, if \( n \) is very large, the observed sample means will tend to be very close to the center (the true mean).

Central limit theorem continued

  • As a visualization of the concept, suppose that we have a random sample indexed by \( j \) \[ X_{1,j}, \cdots, X_{n,j}, \] where \( j \) refers to the replication number.
  • We will make replications for \( j=1,\cdots,m \) and get a RV for sample mean indexed by \( j \), \[ \hat{X}_j = \frac{1}{n}\sum_{i=1}^n X_{i,j}. \]
  • When we observe a realization of \( \hat{X}_j=\hat{x}_j \) or respectively the sample \[ X_{1,j}=x_{1,j}, \cdots, X_{n,j}=x_{n,j}, \] we record these fixed numerical values.
Central limit theorem

Courtesy of Mathieu ROUAUD, CC BY-SA 4.0, via Wikimedia Commons

  • The measurements \( X_{i,j} \) may be distributed according to any underlying distribution with mean \( \overline{x} \) and standard deviation \( \sigma \).
  • However, if \( n \) is large, the \( \hat{X}_j \) is approximately normal with mean \( \overline{x} \) and standard deviation \( \frac{\sigma}{\sqrt{n}} \).
  • The sample mean replications, defined by the realizations of \( x_{i,j} \), will have approximately a bell shaped frequency, centered approximately at \( \overline{x} \).
  • The spread of the data will be approximately \( \frac{\sigma}{\sqrt{n}} \).
  • Particularly, as \( n\rightarrow \infty \), the spread shrinks to zero, so that we get a better and better estimate (more peaked bell shape) with large sample sizes.