# Binomial proportion confidence interval

In statistics, a **binomial proportion confidence interval** is a confidence interval for the probability of success calculated from the outcome of a series of success–failure experiments (Bernoulli trials). In other words, a binomial proportion confidence interval is an interval estimate of a success probability *p* when only the number of experiments *n* and the number of successes *n _{S}* are known.

There are several formulas for a binomial confidence interval, but all of them rely on the assumption of a binomial distribution. In general, a binomial distribution applies when an experiment is repeated a fixed number of times, each trial of the experiment has two possible outcomes (success and failure), the probability of success is the same for each trial, and the trials are statistically independent. Because the binomial distribution is a discrete probability distribution (i.e., not continuous) and difficult to calculate for large numbers of trials, a variety of approximations are used to calculate this confidence interval, all with their own tradeoffs in accuracy and computational intensity.

A simple example of a binomial distribution is the set of various possible outcomes, and their probabilities, for the number of heads observed when a coin is flipped ten times. The observed binomial proportion is the fraction of the flips that turn out to be heads. Given this observed proportion, the confidence interval for the true probability of the coin landing on heads is a range of possible proportions, which may or may not contain the true proportion. A 95% confidence interval for the proportion, for instance, will contain the true proportion 95% of the times that the procedure for constructing the confidence interval is employed.^{[1]}

## Contents

## Normal approximation intervalEdit

A commonly used formula for a binomial confidence interval relies on approximating the distribution of error about a binomially-distributed observation, , with a normal distribution.^{[2]} This approximation is based on the central limit theorem and is unreliable when the sample size is small or the success probability is close to 0 or 1.^{[3]}

Using the normal approximation, the success probability *p* is estimated as

or the equivalent

where is the proportion of successes in a Bernoulli trial process, measured with trials yielding successes and failures, and is the quantile of a standard normal distribution (i.e., the probit) corresponding to the target error rate . For a 95% confidence level, the error , so and .

An important theoretical derivation of this confidence interval involves the inversion of a hypothesis test. Under this formulation, the confidence interval represents those values of the population parameter that would have large *p*-values if they were tested as a hypothesized population proportion. The collection of values, , for which the normal approximation is valid can be represented as

where is the quantile of a standard normal distribution. Since the test in the middle of the inequality is a Wald test, the normal approximation interval is sometimes called the Wald interval, but it was first described by Pierre-Simon Laplace in 1812.^{[4]}

## Wilson score intervalEdit

The Wilson score interval is an improvement over the normal approximation interval in that the actual coverage probability is closer to the nominal value. It was developed by Edwin Bidwell Wilson (1927).^{[5]}

Wilson gave the confidence limits as solutions of both equations

after transforming it into quadratic equations. Hence the success probability *p* is estimated as

or the equivalent

Intuitively, the center value of this interval is the weighted average of and , with receiving greater weight as the sample size increases. This interval has good properties even for a small number of trials and/or an extreme probability.

In most cases Wilsons equations can be solved numerically using the fixed-point iteration

with .

The Wilson interval can be derived from Pearson's chi-squared test with two categories. The resulting interval,

can then be solved for to produce the Wilson score interval. The test in the middle of the inequality is a score test.

### Wilson score interval with continuity correctionEdit

The Wilson interval may be modified by employing a continuity correction, in order to align the minimum coverage probability, rather than the average probability, with the nominal value.

Just as the Wilson interval mirrors Pearson's chi-squared test, the Wilson interval with continuity correction mirrors the equivalent Yates' chi-squared test.

The following formulae for the lower and upper bounds of the Wilson score interval with continuity correction are derived from Newcombe (1998).^{[6]}

However, if *p* = 0, must be taken as 0; if *p* = 1, is then 1.

## Jeffreys intervalEdit

The *Jeffreys interval* has a Bayesian derivation, but it has good frequentist properties. In particular, it has coverage properties that are similar to those of the Wilson interval, but it is one of the few intervals with the advantage of being *equal-tailed* (e.g., for a 95% confidence interval, the probabilities of the interval lying above or below the true value are both close to 2.5%). In contrast, the Wilson interval has a systematic bias such that it is centred too close to *p* = 0.5.^{[7]}

The Jeffreys interval is the Bayesian credible interval obtained when using the non-informative Jeffreys prior for the binomial proportion *p*. The Jeffreys prior for this problem is a Beta distribution with parameters (1/2, 1/2). After observing *x* successes in *n* trials, the posterior distribution for *p* is a Beta distribution with parameters (*x* + 1/2, *n* – *x* + 1/2).

When *x* ≠0 and *x* ≠ *n*, the Jeffreys interval is taken to be the 100(1 – *α*)% equal-tailed posterior probability interval, i.e., the *α* / 2 and 1 – *α* / 2 quantiles of a Beta distribution with parameters (*x* + 1/2, *n* – *x* + 1/2). These quantiles need to be computed numerically, although this is reasonably simple with modern statistical software.

In order to avoid the coverage probability tending to zero when *p* → 0 or 1, when *x* = 0 the upper limit is calculated as before but the lower limit is set to 0, and when *x* = *n* the lower limit is calculated as before but the upper limit is set to 1.^{[3]}

## Clopper–Pearson intervalEdit

The Clopper–Pearson interval is an early and very common method for calculating binomial confidence intervals.^{[8]} This is often called an 'exact' method, but that is because it is based on the cumulative probabilities of the binomial distribution (i.e., exactly the correct distribution rather than an approximation), but the intervals are not exact in the way that one might assume: the discontinuous nature of the binomial distribution precludes any interval with exact coverage for all population proportions. The Clopper–Pearson interval can be written as

or equivalently,

with

where 0 ≤ *x* ≤ *n* is the number of successes observed in the sample and Bin(*n*; *θ*) is a binomial random variable with *n* trials and probability of success *θ*.

Equivalently we can say that the Clopper–Pearson interval is with confidence level if is the infimum of those such that the following tests of hypothesis succeed with significance :

1. H_{0}: with H_{A}:

2. H_{0}: with H_{A}: .

Because of a relationship between the binomial distribution and the beta distribution, the Clopper–Pearson interval is sometimes presented in an alternate format that uses quantiles from the beta distribution.

where *x* is the number of successes, *n* is the number of trials, and *B*(*p*; *v*,*w*) is the *p*th quantile from a beta distribution with shape parameters *v* and *w*.

When is either or , closed-form expressions for the interval bounds are available: when the interval is and when it is .^{[9]}

The beta distribution is, in turn, related to the F-distribution so a third formulation of the Clopper–Pearson interval can be written using F quantiles:

where *x* is the number of successes, *n* is the number of trials, and *F*(*c*; *d*_{1}, *d*_{2}) is the *c* quantile from an F-distribution with *d*_{1} and *d*_{2} degrees of freedom.^{[10]}

The Clopper–Pearson interval is an exact interval since it is based directly on the binomial distribution rather than any approximation to the binomial distribution. This interval never has less than the nominal coverage for any population proportion, but that means that it is usually conservative. For example, the true coverage rate of a 95% Clopper–Pearson interval may be well above 95%, depending on *n* and *θ*. Thus the interval may be wider than it needs to be to achieve 95% confidence. In contrast, it is worth noting that other confidence bounds may be narrower than their nominal confidence width, i.e., the normal approximation (or "standard") interval, Wilson interval,^{[5]} Agresti–Coull interval,^{[10]} etc., with a nominal coverage of 95% may in fact cover less than 95%.^{[3]}

## Agresti–Coull intervalEdit

The Agresti–Coull interval is also another approximate binomial confidence interval.^{[10]}

Given successes in trials, define

and

Then, a confidence interval for is given by

where is the quantile of a standard normal distribution, as before. For example, for a 95% confidence interval, let , so and . If we use 2 instead of 1.96 for , this is the "add 2 successes and 2 failures" interval in Agresti and Coull's 1998 paper "Approximate is Better than 'Exact' for Interval Estimation of Binomial Proportions." ^{[10]}

## Arcsine transformationEdit

Let *X* be the number of successes in *n* trials and let *p* = *X*/*n*. The variance of *p* is

Using the arc sine transform the variance of the arcsine of *p*^{1/2} is^{[11]}

So, the confidence interval itself has the following form:

where is the quantile of a standard normal distribution.

This method may be used to estimate the variance of *p* but its use is problematic when *p* is close to 0 or 1.

*t*_{a} transformEdit

This section does not cite any sources. (July 2017) (Learn how and when to remove this template message) |

Let *p* be the proportion of successes. For 0 ≤ *a* ≤ 2,

This family is a generalisation of the logit transform which is a special case with *a* = 1 and can be used to transform a proportional data distribution to an approximately normal distribution. The parameter *a* has to be estimated for the data set.

## Special casesEdit

The rule of three is used to provide a simple way of stating an approximate 95% confidence interval for *p*, in the special case that no successes ( ) have been observed.^{[12]} The interval is (0,3/*n*).

By symmetry, one could expect for only successes ( ), the interval is (1 − 3/*n*,1).

## Comparison of different intervalsEdit

There are several research papers that compare these and other confidence intervals for the binomial proportion.^{[2]}^{[6]}^{[13]}^{[14]} Both Agresti and Coull (1998)^{[10]} and Ross (2003)^{[15]} point out that exact methods such as the Clopper–Pearson interval may not work as well as certain approximations.

Many of these intervals can be calculated in R using packages like binom.

## See alsoEdit

## ReferencesEdit

**^**Sullivan, Lisa (2017-10-27). "Confidence Intervals".*Boston University School of Public Health*.- ^
^{a}^{b}Wallis, Sean A. (2013). "Binomial confidence intervals and contingency tests: mathematical fundamentals and the evaluation of alternative methods" (PDF).*Journal of Quantitative Linguistics*.**20**(3): 178–208. doi:10.1080/09296174.2013.799918. - ^
^{a}^{b}^{c}Brown, Lawrence D.; Cai, T. Tony; DasGupta, Anirban (2001). "Interval Estimation for a Binomial Proportion".*Statistical Science*.**16**(2): 101–133. CiteSeerX 10.1.1.50.3025. doi:10.1214/ss/1009213286. MR 1861069. Zbl 1059.62533. **^**Laplace, Pierre Simon (1812).*Théorie analytique des probabilités*(in French). p. 283.- ^
^{a}^{b}Wilson, E. B. (1927). "Probable inference, the law of succession, and statistical inference".*Journal of the American Statistical Association*.**22**: 209–212. doi:10.1080/01621459.1927.10502953. JSTOR 2276774. - ^
^{a}^{b}Newcombe, R. G. (1998). "Two-sided confidence intervals for the single proportion: comparison of seven methods".*Statistics in Medicine*.**17**(8): 857–872. doi:10.1002/(SICI)1097-0258(19980430)17:8<857::AID-SIM777>3.0.CO;2-E. PMID 9595616. **^**Cai, TT (2005). "One-sided confidence intervals in discrete distributions".*Journal of Statistical Planning and Inference*.**131**: 63–88. doi:10.1016/j.jspi.2004.01.005.**^**Clopper, C.; Pearson, E. S. (1934). "The use of confidence or fiducial limits illustrated in the case of the binomial".*Biometrika*.**26**: 404–413. doi:10.1093/biomet/26.4.404.**^**Thulin, Måns (2014-01-01). "The cost of using exact confidence intervals for a binomial proportion".*Electronic Journal of Statistics*.**8**(1): 817–840. doi:10.1214/14-EJS909. ISSN 1935-7524.- ^
^{a}^{b}^{c}^{d}^{e}Agresti, Alan; Coull, Brent A. (1998). "Approximate is better than 'exact' for interval estimation of binomial proportions".*The American Statistician*.**52**: 119–126. doi:10.2307/2685469. JSTOR 2685469. MR 1628435. **^**Shao J (1998) Mathematical statistics. Springer. New York, New York, USA**^**Steve Simon (2010) "Confidence interval with zero events", The Children's Mercy Hospital, Kansas City, Mo. (website: "Ask Professor Mean at Stats topics or Medical Research Archived October 15, 2011, at the Wayback Machine)**^**Reiczigel, J (2003). "Confidence intervals for the binomial parameter: some new considerations" (PDF).*Statistics in Medicine*.**22**: 611–621. doi:10.1002/sim.1320.**^**Sauro J., Lewis J.R. (2005) "Comparison of Wald, Adj-Wald, Exact and Wilson intervals Calculator".*Proceedings of the Human Factors and Ergonomics Society, 49th Annual Meeting (HFES 2005)*, Orlando, FL, pp. 2100–2104**^**Ross, T. D. (2003). "Accurate confidence intervals for binomial proportion and Poisson rate estimation".*Computers in Biology and Medicine*.**33**: 509–531. doi:10.1016/S0010-4825(03)00019-2.