Confidence Intervals for the Mean

Learning Objectives

1. Define confidence interval
2. State why a confidence interval is not the probability the interval contains the parameter

Say you were interested in the mean weight of 10-year-old girls living in the United States. Since it would have been impractical to weigh all the 10-year-old girls in the United States, you took a sample of 16 and found that the mean weight was 90 pounds. This sample mean of 90 is a point estimate of the population mean. A point estimate by itself is of limited usefulness because it does not reveal the uncertainty associated with the estimate; you do not have a good sense of how far this sample mean may be from the population mean. For example, can you be confident that the population mean is within 5 pounds of 90? You simply do not know.

Confidence intervals provide more information than point estimates. Confidence intervals for means are intervals constructed using a procedure (presented in the next section) that will contain the population mean a specified proportion of the time, typically either 95% or 99% of the time. These intervals are referred to as 95% and 99% confidence intervals respectively. An example of a 95% confidence interval is shown below:

$72.85 < μ < 107.15$

There is good reason to believe that the population mean lies between these two bounds of 72.85 and 107.15 since 95% of the time confidence intervals contain the true mean.

If repeated samples were taken and the 95% confidence interval computed for each sample, 95% of the intervals would contain the population mean. Naturally, 5% of the intervals would not contain the population mean.

It is natural to interpret a 95% confidence interval as an interval with a 0.95 probability of containing the population mean. However, the proper interpretation is not that simple. One problem is that the computation of a confidence interval does not take into account any other information you might have about the value of the population mean. For example, if numerous prior studies had all found sample means above 110, it would not make sense to conclude that there is a 0.95 probability that the population mean is between 72.85 and 107.15. What about situations in which there is no prior information about the value of the population mean? Even here the interpretation is complex. The problem is that there can be more than one procedure that produces intervals that contain the population parameter 95% of the time. Which procedure produces the "true" 95% confidence interval? Although the various methods are equal from a purely mathematical point of view, the standard method of computing confidence intervals has two desirable properties: each interval is symmetric about the point estimate and each interval is contiguous. Recall from the introductory section in the chapter on probability that, for some purposes, probability is best thought of as subjective. It is reasonable, although not required by the laws of probability, that one adopt a subjective probability of 0.95 that a 95% confidence interval, as typically computed, contains the parameter in question.

Confidence intervals can be computed for various parameters, not just the mean. For example, later in this chapter you will see how to compute a confidence interval for $ρ$, the population value of Pearson's $r$, based on sample data.

Source: David M. Lane , https://onlinestatbook.com/2/estimation/confidence.html
This work is in the Public Domain.

Learning Objectives

1. Use the inverse normal distribution calculator to find the value of z to use for a confidence interval
2. Compute a confidence interval on the mean when σ is known
3. Determine whether to use a t distribution or a normal distribution
4. Compute a confidence interval on the mean when σ is estimated

When you compute a confidence interval on the mean, you compute the mean of a sample in order to estimate the mean of the population. Clearly, if you already knew the population mean, there would be no need for a confidence interval. However, to explain how confidence intervals are constructed, we are going to work backwards and begin by assuming characteristics of the population. Then we will show how sample data can be used to construct a confidence interval.

Assume that the weights of 10-year-old children are normally distributed with a mean of 90 and a standard deviation of 36. What is the sampling distribution of the mean for a sample size of 9? Recall from the section on the sampling distribution of the mean that the mean of the sampling distribution is μ and the standard error of the mean is

For the present example, the sampling distribution of the mean has a mean of 90 and a standard deviation of 36/3 = 12. Note that the standard deviation of a sampling distribution is its standard error. Figure 1 shows this distribution. The shaded area represents the middle 95% of the distribution and stretches from 66.48 to 113.52. These limits were computed by adding and subtracting 1.96 standard deviations to/from the mean of 90 as follows:

90 - (1.96)(12) = 66.48
90 + (1.96)(12) = 113.52

The value of 1.96 is based on the fact that 95% of the area of a normal distribution is within 1.96 standard deviations of the mean; 12 is the standard error of the mean.

Figure 1. The sampling distribution of the mean for N=9. The middle 95% of the distribution is shaded.

Figure 1 shows that 95% of the means are no more than 23.52 units (1.96 standard deviations) from the mean of 90. Now consider the probability that a sample mean computed in a random sample is within 23.52 units of the population mean of 90. Since 95% of the distribution is within 23.52 of 90, the probability that the mean from any given sample will be within 23.52 of 90 is 0.95. This means that if we repeatedly compute the mean (M) from a sample, and create an interval ranging from $M - 23.52$ to $M + 23.52$, this interval will contain the population mean 95% of the time. In general, you compute the 95% confidence interval for the mean with the following formula:

Lower limit = $M - Z_{.95σM}$

Upper limit = $M + Z_{.95σM}$

where Z.95 is the number of standard deviations extending from the mean of a normal distribution required to contain 0.95 of the area and σM is the standard error of the mean.

If you look closely at this formula for a confidence interval, you will notice that you need to know the standard deviation ($σ$) in order to estimate the mean. This may sound unrealistic, and it is. However, computing a confidence interval when σ is known is easier than when σ has to be estimated, and serves a pedagogical purpose. Later in this section we will show how to compute a confidence interval for the mean when σ has to be estimated.

Suppose the following five numbers were sampled from a normal distribution with a standard deviation of 2.5: 2, 3, 5, 6, and 9. To compute the 95% confidence interval, start by computing the mean and standard error:


$M = (2 + 3 + 5 + 6 + 9)/5 = 5$.
$σ_M = \dfrac{2.5}{\sqrt 5} = 1.118$.


$Z_{.95}$ can be found using the normal distribution calculator and specifying that the shaded area is 0.95 and indicating that you want the area to be between the cutoff points. As shown in Figure 2, the value is 1.96. If you had wanted to compute the 99% confidence interval, you would have set the shaded area to 0.99 and the result would have been 2.58.

Figure 2. 95% of the area is between -1.96 and 1.96.

Normal Distribution Calculator

The confidence interval can then be computed as follows:

Lower limit = $5 - (1.96)(1.118)= 2.81$
Upper limit = $5 + (1.96)(1.118)= 7.19$

You should use the t distribution rather than the normal distribution when the variance is not known and has to be estimated from sample data. When the sample size is large, say 100 or above, the t distribution is very similar to the standard normal distribution. However, with smaller sample sizes, the t distribution is leptokurtic, which means it has relatively more scores in its tails than does the normal distribution. As a result, you have to extend farther from the mean to contain a given proportion of the area. Recall that with a normal distribution, 95% of the distribution is within 1.96 standard deviations of the mean. Using the t distribution, if you have a sample size of only 5, 95% of the area is within 2.78 standard deviations of the mean. Therefore, the standard error of the mean would be multiplied by 2.78 rather than 1.96.

The values of t to be used in a confidence interval can be looked up in a table of the t distribution. A small version of such a table is shown in Table 1. The first column, $df$, stands for degrees of freedom, and for confidence intervals on the mean, $df$ is equal to $N - 1$, where $N$ is the sample size.

Table 1. Abbreviated t table.

Learning Objectives

1. State the difference between the shape of the $t$ distribution and the normal distribution
2. State how the difference between the shape of the $t$ distribution and normal distribution is affected by the degrees of freedom
3. Use a $t$ table to find the value of $t$ to use in a confidence interval
4. Use the $t$ calculator to find the value of $t$ to use in a confidence interval

In the introduction to normal distributions it was shown that 95% of the area of a normal distribution is within 1.96 standard deviations of the mean. Therefore, if you randomly sampled a value from a normal distribution with a mean of 100, the probability it would be within $1.96σ$ of 100 is 0.95. Similarly, if you sample $N$ values from the population, the probability that the sample mean ($M$) will be within $1.96 σ_M$ of 100 is 0.95.

Now consider the case in which you have a normal distribution but you do not know the standard deviation. You sample $N$ values and compute the sample mean ($M$) and estimate the standard error of the mean ($σ_M)$ with $s_M$. What is the probability that $M$ will be within $1.96 s_M$ of the population mean ($μ$)? This is a difficult problem because there are two ways in which $M$ could be more than $1.96 s_M$ from $μ$: (1) $M$ could, by chance, be either very high or very low and (2) $s_M$ could, by chance, be very low. Intuitively, it makes sense that the probability of being within 1.96 standard errors of the mean should be smaller than in the case when the standard deviation is known (and cannot be underestimated). But exactly how much smaller? Fortunately, the way to work out this type of problem was solved in the early 20th century by W. S. Gosset who determined the distribution of a mean divided by an estimate of its standard error. This distribution is called the Student's $t$ distribution or sometimes just the $t$ distribution. Gosset worked out the $t$ distribution and associated statistical tests while working for a brewery in Ireland. Because of a contractual agreement with the brewery, he published the article under the pseudonym "Student". That is why the $t$ test is called the "Student's $t$ test".

The $t$ distribution is very similar to the normal distribution when the estimate of variance is based on many degrees of freedom, but has relatively more scores in its tails when there are fewer degrees of freedom. Figure 1 shows t distributions with 2, 4, and 10 degrees of freedom and the standard normal distribution. Notice that the normal distribution has relatively more scores in the center of the distribution and the t distribution has relatively more in the tails. The t distribution is therefore leptokurtic. The $t$ distribution approaches the normal distribution as the degrees of freedom increase.

Figure 1. A comparison of $t$ distributions with 2, 4, and 10 $df$ and the standard normal distribution. The distribution with the lowest peak is the 2 $df$ distribution, the next lowest is 4 $df$, the lowest after that is 10 $df$, and the highest is the standard normal distribution.

Since the t distribution is leptokurtic, the percentage of the distribution within 1.96 standard deviations of the mean is less than the 95% for the normal distribution. Table 1 shows the number of standard deviations from the mean required to contain 95% and 99% of the area of the t distribution for various degrees of freedom. These are the values of $t$ that you use in a confidence interval. The corresponding values for the normal distribution are 1.96 and 2.58 respectively. Notice that with few degrees of freedom, the values of t are much higher than the corresponding values for a normal distribution and that the difference decreases as the degrees of freedom increase. The values in Table 1 can be obtained from the "Find t for a confidence interval" calculator.

Table 1. Abbreviated t table.

Learning Objectives

1. State the assumptions for computing a confidence interval on the difference between means
2. Compute a confidence interval on the difference between means
3. Format data for computer analysis

It is much more common for a researcher to be interested in the difference between means than in the specific values of the means themselves. We take as an example the data from the "Animal Research" case study. In this experiment, students rated (on a 7-point scale) whether they thought animal research is wrong. The sample sizes, means, and variances are shown separately for males and females in Table 1.

As you can see, the females rated animal research as more wrong than did the males. This sample difference between the female mean of 5.35 and the male mean of 3.88 is 1.47. However, the gender difference in this particular sample is not very important. What is important is the difference in the population. The difference in sample means is used to estimate the difference in population means. The accuracy of the estimate is revealed by a confidence interval.

In order to construct a confidence interval, we are going to make three assumptions:

1. The two populations have the same variance. This assumption is called the assumption of homogeneity of variance.
2. The populations are normally distributed.
3. Each value is sampled independently from each other value.

The consequences of violating these assumptions are discussed in a later section. For now, suffice it to say that small-to-moderate violations of assumptions 1 and 2 do not make much difference.

A confidence interval on the difference between means is computed using the following formula:

Lower Limit = $M_1 - M_2 - (t_{CL})(S_{M_1-M_2})$
Upper Limit = $M_1 - M_2 + (t_{CL})(S_{M_1-M_2})$

where $M_1 - M_2$ is the difference between sample means, $t_{CL}$ is the t for the desired level of confidence, and $S_{M_1-M_2}$  is the estimated standard error of the difference between sample means. The meanings of these terms will be made clearer as the calculations are demonstrated.

We continue to use the data from the "Animal Research" case study and will compute a confidence interval on the difference between the mean score of the females and the mean score of the males. For this calculation, we will assume that the variances in each of the two populations are equal.

The first step is to compute the estimate of the standard error of the difference between means $(S_{M_1-M_2})$. Recall from the relevant section in the chapter on sampling distributions that the formula for the standard error of the difference in means in the population is:

$\sigma _{M_1 - M_2} = \sqrt{\dfrac{ \sigma_1^2 }{n_1} + \dfrac{\sigma_2^2 }{n_2}} = \sqrt{\dfrac{ \sigma^2 }{n} + \dfrac{\sigma^2 }{n}} = \sqrt{\dfrac{ 2 \sigma^2 }{n}}$

In order to estimate this quantity, we estimate $σ^2$ and use that estimate in place of $σ^2$. Since we are assuming the population variances are the same, we estimate this variance by averaging our two sample variances. Thus, our estimate of variance is computed using the following formula:

where MSE is our estimate of σ². In this example,

$MSE = (2.743 + 2.985)/2 = 2.864$.

Note that MSE stands for "mean square error" and is the mean squared deviation of each score from its group's mean.

Since $n$ (the number of scores in each condition) is 17,

$S_{M_1-M_2}=\sqrt {\dfrac{2MSE}{n}}= \sqrt{\dfrac{(2)(2.864)}{17}} = 0.5805$.

The next step is to find the t to use for the confidence interval ($t_{CL}$). To calculate $t_{CL}$, we need to know the degrees of freedom. The degrees of freedom is the number of independent estimates of variance on which MSE is based. This is equal to $(n_1 - 1) + (n_2 - 1)$ where $n_1$ is the sample size of the first group and $n_2$ is the sample size of the second group. For this example, $n_1= n_2 = 17$. When $n_1= n_2$, it is conventional to use "$n$" to refer to the sample size of each group. Therefore, the degrees of freedom is 16 + 16 = 32.

From either the above calculator or a $t$ table, you can find that the $t$ for a 95% confidence interval for $32 df$ is 2.037.

We now have all the components needed to compute the confidence interval. First, we know the difference between means:

$M_1 - M_2 = 5.353 - 3.882 = 1.471$

We know the standard error of the difference between means is

 $S_{M_1-M_2}= 0.5805$

and that the $t$ for the 95% confidence interval with $32 df$ is

$t_{CL} = 2.037$

Therefore, the 95% confidence interval is

Lower Limit = $1.471 - (2.037)(0.5805) = 0.29$

Upper Limit = $1.471 + (2.037)(0.5805) = 2.65$

We can write the confidence interval as:

where $μ_f$ is the population mean for females and $μ_m$ is the population mean for males. This analysis provides evidence that the mean for females is higher than the mean for males, and that the difference between means in the population is likely to be between 0.29 and 2.65.

Formatting data for Computer Analysis

Most computer programs that compute $t$ tests require your data to be in a specific form. Consider the data in Table 2.

Here there are two groups, each with three observations. To format these data for a computer program, you normally have to use two variables: the first specifies the group the subject is in and the second is the score itself. For the data in Table 2, the reformatted data look as follows:

To use Analysis Lab to do the calculations, you would copy the data and then

1. Click the "Enter/Edit User Data" button. (You may be warned that for security reasons you must use the keyboard shortcut for pasting data).
2. Paste your data.
3. Click "Accept Data".
4. Set the Dependent Variable to Y.
5. Set the Grouping Variable to G.
6. Click the t-test confidence interval button.

The 95% confidence interval on the difference between means extends from -4.267 to 0.267.

Computations for Unequal Sample Sizes (optional)

The calculations are somewhat more complicated when the sample sizes are not equal. One consideration is that MSE, the estimate of variance, counts the sample with the larger sample size more than the sample with the smaller sample size. Computationally this is done by computing the sum of squares error (SSE) as follows:

where $M_1$ is the mean for group 1 and $M_2$ is the mean for group 2. Consider the following small example:

$M_1 = 4$ and $M_2 = 3$.

$SSE = (3-4)^2 + (4-4)^2 + (5-4)^2 + (2-3)^2 + (4-3)^2 = 4$

Then, MSE is computed by: $MSE = SSE/df$

where the degrees of freedom ($df$) is computed as before:
$df = (n_1 -1) + (n_2 -1) = (3-1) + (2-1) = 3$.
$MSE = SSE/df = 4/3 = 1.333$.

The formula

$S_{M_1-M_2} = \sqrt {\dfrac{2MSE}{n}}$

is replaced by

$S_{M_1-M_2} = \sqrt {\dfrac{2MSE}{n_h}}$

where $n_h$ is the harmonic mean of the sample sizes and is computed as follows:

$n_h = \dfrac{2}{1/n_1 + 1/n_2} = \dfrac{2}{1/3+1/2} = 2.4$

and

$S_{M_1-M_2} = \sqrt {\dfrac{(2)(1.333)}{2.4}} = 1.054$.


$t_{CL}$ for 3 $df$ and the 0.05 level = 3.182.

Therefore the 95% confidence interval is

Lower Limit = $1 - (3.182)(1.054)= -2.35$

Upper Limit = $1 + (3.182)(1.054)= 4.35$

We can write the confidence interval as:

$-2.35 ≤ μ_1 - μ_2 ≤ 4.35$