Confidence Interval Calculator
Compute confidence intervals for means (Z/t), proportions, and differences. Shows standard error, critical value, margin of error, and error-bar graph.
Compute confidence intervals for means (Z/t), proportions, and differences. Shows standard error, critical value, margin of error, and error-bar graph.
A confidence interval (CI) is a range of values that estimates an unknown population parameter with a specified level of confidence. Rather than providing a single point estimate (like a sample mean or proportion), a confidence interval acknowledges uncertainty and gives a plausible range where the true parameter is likely to fall. The "confidence level" (typically 90%, 95%, or 99%) represents the long-run frequency with which such intervals would contain the true parameter if we repeated the sampling process many times.
It's crucial to understand that a 95% confidence interval does NOT mean "there's a 95% probability the true parameter is in this interval." Once the interval is calculated, the parameter either is or isn't in it—the probability is either 0 or 1. What 95% means is: if we constructed confidence intervals from 100 random samples using the same method, approximately 95 of those intervals would contain the true parameter. This is a statement about the long-run performance of the method, not about a single interval.
When the population standard deviation σ is known and the sample size is large (n ≥ 30), or the population is normally distributed for any n, use the z-interval formula:
Where x̄ is the sample mean, zα/2 is the critical z-value (e.g., 1.96 for 95% confidence), σ is the population standard deviation, and n is the sample size. The term σ / √n is the standard error of the mean (SE), which measures the variability of the sample mean across different samples.
In practice, the population standard deviation σ is rarely known. When you only have the sample standard deviation s, use the t-interval formula:
Where tα/2, df is the critical t-value with degrees of freedom df = n - 1. The t-distribution accounts for the additional uncertainty from estimating σ with s. For small samples, the t-distribution has heavier tails than the normal distribution, resulting in wider confidence intervals. As n increases, the t-distribution approaches the normal distribution.
For a single proportion p̂ = x / n, the Wald (normal approximation) confidence interval is:
This formula works well when n is large and p̂ is not too close to 0 or 1. A common rule of thumb is np̂ ≥ 10 and n(1 - p̂) ≥ 10. However, the Wald interval has known problems with small samples or extreme proportions—it can produce intervals outside [0, 1] or have poor coverage (the actual confidence level is lower than the nominal level).
The Wilson score interval is a more reliable alternative to the Wald interval, especially for small samples or extreme proportions. It adjusts the center point and width of the interval to account for the discrete binomial distribution, resulting in better coverage properties. The Wilson interval never extends outside [0, 1] and provides more accurate confidence levels, particularly when p̂ is near 0, 0.5, or 1, or when n is small. Many statisticians recommend using Wilson by default for proportion intervals.
Two-Sample Mean Difference (Pooled t-Interval): When comparing means from two independent samples with equal variances, use the pooled standard deviation and the formula:
Where df = n₁ + n₂ - 2 and SEpooled combines the sample variances weighted by sample sizes. The pooled method assumes equal population variances (homoscedasticity), which should be verified with an F-test or Levene's test before use.
Two-Sample Mean Difference (Welch's t-Interval): When the assumption of equal variances is violated or uncertain, use Welch's t-interval, which does not pool variances and uses adjusted degrees of freedom (Welch-Satterthwaite approximation). Welch's method is more robust and is the default in many statistical software packages because it doesn't require the equal variances assumption.
Two-Sample Proportion Difference: For comparing two proportions p̂₁ and p̂₂, the confidence interval for the difference is:
This uses the Wald approach for differences. More sophisticated methods like the Wilson interval or exact methods (e.g., score interval) can be used for better coverage, especially with small samples or extreme proportions.
The point estimate is your best single-value estimate of the population parameter based on the sample data. For a single mean, it's x̄. For a proportion, it's p̂ = x / n. For differences, it's x̄₁ - x̄₂ or p̂₁ - p̂₂. The point estimate serves as the center of the confidence interval. While it's our best guess, it's subject to sampling variability—if we took a different sample, we'd get a different point estimate. The confidence interval quantifies this uncertainty.
The standard error measures the variability of the point estimate across different samples. It's the standard deviation of the sampling distribution of the estimator. For a mean: SE = s / √n (or σ / √n if σ is known). For a proportion: SE = √(p̂(1-p̂) / n). Smaller SE means the estimate is more precise—repeated samples would give point estimates clustered more tightly around the true parameter. SE decreases as sample size increases, following a 1/√n relationship. The SE is the key input to calculating the margin of error.
The critical value is the z or t multiplier corresponding to your chosen confidence level. For a 95% z-interval, it's 1.96. For a 95% t-interval with df = 20, it's approximately 2.086. The critical value determines how many standard errors you extend on each side of the point estimate to form the interval. Higher confidence levels require larger critical values (e.g., 99% uses 2.576 for z, wider than 95% at 1.96), resulting in wider intervals. The t critical value depends on degrees of freedom and converges to the z value as df increases.
The margin of error is the half-width of the confidence interval, calculated as ME = Critical Value × SE. It represents the maximum expected difference between the point estimate and the true parameter at the chosen confidence level. For example, if x̄ = 50 and ME = 3, you report "50 ± 3" or [47, 53]. The ME combines the precision of your estimate (SE) and the confidence you want (critical value). To reduce ME, you can either increase sample size (reducing SE) or accept lower confidence (reducing the critical value). Reporting the ME alongside the point estimate is a clear way to communicate uncertainty.
The confidence interval is the range [Point Estimate - ME, Point Estimate + ME], providing a plausible set of values for the true population parameter. A 95% CI means that if we repeated the sampling and interval construction process many times, 95% of the resulting intervals would contain the true parameter. It does NOT mean the parameter has a 95% probability of being in this specific interval—once calculated, the parameter is either in it or not. Use the CI to assess both statistical significance (does it exclude a null value like 0 or 1?) and practical significance (is the range narrow enough to inform decisions?).
The error-bar chart provides a visual representation of the confidence interval. The central point represents the point estimate, and the error bars extend to the lower and upper confidence limits. This makes it easy to visually assess:
When comparing two error bars, overlapping bars do NOT necessarily mean no significant difference—formal statistical tests or explicit difference intervals are needed for proper inference.
When constructing a CI for a difference (mean₁ - mean₂ or prop₁ - prop₂), special interpretation applies:
• Distributional Assumptions: Confidence interval formulas assume specific distributions (normal for means with large samples, t-distribution for small samples). Violations of these assumptions may produce invalid intervals.
• Random Sampling: Valid confidence intervals require random sampling from the population of interest. Convenience samples, self-selection, or non-random sampling may produce biased estimates that confidence intervals cannot correct.
• Independence: Observations must be independent. Clustered, repeated measures, or time-series data require specialized methods that account for correlation structures.
• Interpretation Caution: A 95% CI does NOT mean there is a 95% probability the true parameter falls within this specific interval. Rather, if we repeated sampling infinitely, 95% of such intervals would contain the true parameter.
Important Note: This calculator is strictly for educational and informational purposes only. It does not provide professional statistical consulting or research validation. Confidence intervals are commonly misinterpreted—the interval describes uncertainty about the parameter, not a range where future observations will fall. Results should be verified using professional statistical software (R, Python SciPy, SAS, SPSS) for research, academic, clinical, or business applications. Always consult qualified statisticians for important decisions, especially in medical research, clinical trials, quality control, or any context where interval estimates inform real-world actions. This tool cannot account for sampling bias, measurement error, missing data, or complex study designs.
The mathematical formulas and statistical concepts used in this calculator are based on established statistical theory and authoritative academic sources:
Common questions about confidence intervals, z vs t distributions, Wilson vs Wald methods, and sample size requirements.
Use z-intervals when the population standard deviation (σ) is known and the population is normal or n ≥ 30. In practice, σ is rarely known, so use t-intervals with the sample standard deviation (s) and degrees of freedom df = n - 1. The t-distribution accounts for the additional uncertainty from estimating σ with s. As sample size increases, the t-distribution converges to the normal distribution, so the difference becomes negligible for large samples (n > 100). When in doubt, use t—it's more conservative and appropriate for nearly all real-world scenarios.
The Wilson score interval has better coverage properties than the Wald interval, especially for small samples (n < 40) and extreme proportions (p̂ near 0 or 1). The Wald interval can produce intervals outside [0, 1], which is impossible for proportions, and the actual confidence level is often much lower than the nominal level (e.g., a 95% Wald interval might only achieve 88% coverage). Wilson adjusts both the center and width of the interval to account for the discrete binomial distribution, resulting in intervals that stay within [0, 1] and have coverage closer to the nominal level. Use Wilson by default unless you have a very large sample (n > 1000) and p̂ is well away from 0 and 1.
A 95% confidence interval means that if we repeated the sampling and interval construction process many times, approximately 95% of the resulting intervals would contain the true population parameter. It is NOT a statement about the probability that the true parameter is in this specific interval—once the interval is calculated, the parameter either is or isn't in it (probability 0 or 1). The 95% refers to the long-run performance of the method. Think of it this way: the method is reliable 95% of the time, but for any single interval, we don't know if it's one of the 95% that captured the parameter or one of the 5% that missed it. Use the interval to assess both statistical significance (does it exclude a null value?) and practical significance (is the range narrow enough to be useful?).
Use the pooled t-interval only when you have strong reason to believe the population variances are equal (σ₁² = σ₂²) and your study design supports this assumption (e.g., randomized controlled trial with balanced groups). Pooled intervals combine sample variances to get a single estimate, which can be more powerful (narrower interval) if the assumption is true. However, if variances differ, pooled intervals can be misleading—either too narrow or incorrectly centered. Welch's t-interval does not assume equal variances and uses adjusted degrees of freedom (Welch-Satterthwaite approximation). Because the equal variances assumption is often violated and can be hard to verify with small samples, Welch is the safer default choice and is used by default in most modern statistical software (R, Python, SPSS).
The confidence level (e.g., 95%, 99%) determines the critical value (z or t) used in the interval calculation. Higher confidence levels require larger critical values, resulting in wider intervals. The margin of error (ME) is the half-width of the confidence interval, calculated as ME = Critical Value × Standard Error. ME represents the maximum expected difference between the point estimate and the true parameter at the chosen confidence level. So confidence level controls how 'sure' you want to be (at the cost of precision), while ME quantifies the precision (how tight the interval is). For example, a 95% CI with ME = 3 means you're 95% confident the true parameter is within ±3 units of the point estimate. To reduce ME, you can increase sample size (reduces SE) or accept lower confidence (reduces critical value).
Sample size adequacy depends on your goals and the type of interval. For means with t-intervals, check if n ≥ 30 (Central Limit Theorem ensures approximate normality of the sampling distribution) or verify the population is approximately normal for smaller n using histograms or Q-Q plots. For proportions, the Wald interval requires np̂ ≥ 10 and n(1 - p̂) ≥ 10; Wilson relaxes this but still needs reasonably large n. For differences, each group should meet the respective criteria. Beyond meeting assumptions, evaluate whether your confidence interval is narrow enough for your purposes—if the ME is too large to make useful decisions, you need more data. Use the Sample Size & Power calculator to plan studies prospectively: specify your target margin of error or CI width, desired confidence level, and expected variability, and it will compute the required sample size.
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