Sampling Distributions and Point Estimation Comprehensive Study Notes

Foundations of Population and Sample Statistics

To understand sampling distributions, one must distinguish between a population and a sample space. A population refers to the entire group of interest, while a sample is a subset of that population. Within this framework, a population parameter is a fixed numerical value describing a characteristic of the population, whereas a sample statistic is a value calculated from sample data used to estimate that parameter. For instance, in parameter estimation, statistics are utilized to gauge the effectiveness of pilot training or psychotherapy programs. A core objective involves using the sample standard deviation (ss) to estimate the population standard deviation (σ\sigma).

Several fundamental questions guide the study of these distributions: What is a sampling distribution? What is the standard error? What is the principle of maximum likelihood? What is bias in a statistical sense? What is a confidence interval? What is the central limit theorem? Additionally, why is the number 1.961.96 considered a significant value in this field?

The Mechanics of Sampling Distributions

A sampling distribution is a probability distribution of a statistic obtained through all possible samples of a fixed size (NN). Because every sample drawn from a population contains different observed values, the resulting sample means will vary. To generate a sampling distribution, the following process is followed: First, a sample of size NN (such as 55, 1010, or 10001000) is taken from the population. Second, a statistic, such as the mean (xˉ\bar{x}), is computed and recorded. Third, this process is repeated infinitely for large populations. Finally, the resulting distribution of the statistic over these repeated samples is plotted.

Consider an example involving a supervisor with six employees whose years of experience are 22, 44, 66, 66, 77, and 88. The population mean for these six elements is μ=5.5\mu = 5.5. If two employees are chosen randomly (n=2n = 2) without replacement, the first observation has a probability of 1/61/6 and the second has a probability of 1/51/5. There are 1515 possible combinations, such as (2,42,4) with a mean of 33, (2,62,6) with a mean of 44, and (7,87,8) with a mean of 7.57.5. The probabilities for each sample mean are as follows: P(3)=1/15P(3) = 1/15, P(4)=2/15P(4) = 2/15, P(4.5)=1/15P(4.5) = 1/15, P(5)=3/15P(5) = 3/15, P(5.5)=1/15P(5.5) = 1/15, P(6)=2/15P(6) = 2/15, P(6.5)=2/15P(6.5) = 2/15, P(7)=2/15P(7) = 2/15, and P(7.5)=1/15P(7.5) = 1/15.

In a second example, consider a population of six elements (1,2,3,4,5,61, 2, 3, 4, 5, 6) where samples of size 22 are selected with replacement. This implies each element has a 1/61/6 chance of being selected, resulting in 3636 possible outcomes ranging from (1,11,1) with a mean of 11 to (6,66,6) with a mean of 66. While there is only one way to achieve a mean of 11, there are six different combinations that result in a mean of 3.53.5. The sampling distribution illustrates the specific relationship between the probability of a statistic and the statistic's numerical value for all possible samples of size NN.

Quantitative Properties of the Sample Mean and Standard Error

The mean of the sampling distribution is defined by the expected value of the sample mean. For a set of independent observations, the expected value of the sample mean is equal to the population mean:

E(Xˉ)=E(1n(X1+X2+...+Xn))=μE(\bar{X}) = E\left(\frac{1}{n}(X_1 + X_2 + ... + X_n)\right) = \mu

The variance of the sampling distribution is calculated as:

Var(Xˉ)=Var(X1+X2+...+Xnn)=σ2nVar(\bar{X}) = Var\left(\frac{X_1 + X_2 + ... + X_n}{n}\right) = \frac{\sigma^2}{n}

The standard deviation of the sampling distribution is specifically referred to as the Standard Error (σxˉ\sigma_{\bar{x}}). When individuals are selected independently, it is expressed as:

σxˉ=σn\sigma_{\bar{x}} = \frac{\sigma}{\sqrt{n}}

If observations are not selected independently, a finite population correction must be applied to the variance:

Var(Xˉ)=σ2n×N−nN−1Var(\bar{X}) = \frac{\sigma^2}{n} \times \frac{N - n}{N - 1}

The Central Limit Theorem and Standard Normal Applications

The Central Limit Theorem (CLT) states that the sampling distribution of means becomes normal as the sample size (NN) increases, regardless of the shape of the original distribution. This principle also applies to other statistics, such as variance, and dictates that binomial distributions become normal as NN increases.

Whenever a sampling distribution of the mean follows a normal distribution, we can compute the standardized normal variable ZZ using the formula:

Z=xˉ−μσxˉ=xˉ−μσ/nZ = \frac{\bar{x} - \mu}{\sigma_{\bar{x}}} = \frac{\bar{x} - \mu}{\sigma / \sqrt{n}}

Example Case Study: A spark plug manufacturer claims spark plug lives are normally distributed with a mean of 60,000 miles60,000\,miles and a standard deviation of 4000 miles4000\,miles. A random sample of 1616 plugs yields an average life of 58,500 miles58,500\,miles. To find the probability of finding a sample mean of this value or less, we first calculate the standard error:

σxˉ=400016=1000\sigma_{\bar{x}} = \frac{4000}{\sqrt{16}} = 1000

Then we calculate the ZZ-score:

P(xˉ<58,500)=P(Z<58,500−60,0001000)P(\bar{x} < 58,500) = P\left(Z < \frac{58,500 - 60,000}{1000}\right)

P(Z<−1.50)=0.0668P(Z < -1.50) = 0.0668

Acceptance Intervals and Sample Proportions

An acceptance interval is a range within which a sample mean has a high probability of occurring, given a known population mean and variance. If a sample mean falls within this interval, we accept the conclusion that the sample originated from that population. The interval is calculated as:

μ±Zα/2σxˉ\mu \pm Z_{\alpha/2} \sigma_{\bar{x}}

In the context of Bernoulli and binomial distributions, the probability of success is denoted as PP. The sample proportion (pp) is used to make inferences about the population proportion. Let XX be the number of successes in a sample of nn observations; the sample proportion is p=X/np = X/n. Because pp is the mean of a set of independent random variables, the Central Limit Theorem allows us to model it as a normally distributed random variable for large sample sizes.

For a binomial distribution, the mean and variance of the sample proportion are:

E(p)=PE(p) = P

Var(p)=P(1−P)nVar(p) = \frac{P(1 - P)}{n}

The standard normal variable for proportions is:

Z=p−PσpZ = \frac{p - P}{\sigma_p}

Example Case Study: A sample of 270270 homes is taken to estimate the proportion with unsafe wiring. If the true population proportion is P=0.2P = 0.2, the probability that the sample proportion falls between 16%16\% and 24%24\% is calculated by first finding the standard error of the proportion:

σp=0.2(0.8)270=0.024\sigma_p = \sqrt{\frac{0.2(0.8)}{270}} = 0.024

P(0.16<p<0.24)=P(0.16−0.20.024<Z<0.24−0.20.024)=0.9050P(0.16 < p < 0.24) = P\left(\frac{0.16 - 0.2}{0.024} < Z < \frac{0.24 - 0.2}{0.024}\right) = 0.9050

The Chi-Square Distribution and Sample Variance

Consider a random sample of nn observations from a population with an unknown mean (μ\mu) and unknown variance (σ2\sigma^2). While the population variance is σ2=E(X−μ)2\sigma^2 = E(X - \mu)^2, the sample variance is calculated as:

s2=∑i=1n(xi−xˉ)2n−1s^2 = \frac{\sum_{i=1}^{n} (x_i - \bar{x})^2}{n - 1}

The expected value of the sample variance is equal to the population variance: E(s2)=σ2E(s^2) = \sigma^2. For a normally distributed population, the ratio of the sample and population variance follows a chi-square distribution with n−1n - 1 degrees of freedom (vv):

χ(n−1)2=(n−1)s2σ2=∑i=1n(xi−xˉ)2σ2\chi_{(n-1)}^2 = \frac{(n-1)s^2}{\sigma^2} = \frac{\sum_{i=1}^n (x_i - \bar{x})^2}{\sigma^2}

The chi-square distribution is defined only for positive values. Its mean and variance are linked to the degrees of freedom:

E(χv2)=vE(\chi_v^2) = v

Var(χv2)=2vVar(\chi_v^2) = 2v

Further proof shows that because E[(n−1)s2/σ2]=n−1E[(n - 1)s^2 / \sigma^2] = n - 1, then Var(s2)=2σ4/(n−1)Var(s^2) = 2\sigma^4 / (n - 1). When reading chi-square tables, specific values are denoted as χα,v2\chi_{\alpha, v}^2. For example, with v=39v = 39 degrees of freedom, a value corresponding to a 0.050.05 upper tail would be written as P(χ392>K)=0.05P(\chi_{39}^2 > K) = 0.05.

Example Case Study: Shirley Mendez, a quality assurance manager at Green Valley Foods, wants to ensure the variation in package weights is limited. For a sample of n=20n = 20, she seeks an upper limit for the ratio s2/σ2s^2 / \sigma^2 such that the probability of being above the limit is 0.0250.025. Using the chi-square table for v=19v = 19 and α=0.025\alpha = 0.025, the value is 32.85232.852. The limit (kuk_u) is found via:

P(χ192>19×ku)=0.025P(\chi_{19}^2 > 19 \times k_u) = 0.025

19×ku=32.85219 \times k_u = 32.852

ku=32.85219=1.729k_u = \frac{32.852}{19} = 1.729

This indicates that with 97.5%97.5\% probability, the ratio of sample variance to population variance will be below 1.7291.729.