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In 1968 Shirley Chisholm became the first Black woman elected to the United States Congress. In 1972 she launched a campaign for the Democratic presidential nomination, breaking another political barrier.
MORE →Reflects the personal views, recollections, and perspective of the author, Mike Davis.
This is a personal recollection on the Move fire on May 13, 1985

In frequentist inference, a confidence interval (CI) determines lower and upper bounds likely to contain (in repeated sampling) the true value of an unknown statistical parameter, such as a population mean.[1] Rather than reporting a single point estimate (e.g. "the average screen time is 3 hours per day"), a confidence interval provides an interval, such as from 2 hours to 4 hours.
A confidence interval is based on a pre-defined coverage probability, called confidence level, typically 95%. A 95% confidence level does not imply a 95% probability that the true parameter lies within a particular CI calculated from a sample (such interpretation would be associated with the credible interval in Bayesian inference). The confidence level instead reflects the long-run performance of the method used to generate the interval.[2][3] In other words, if the same sampling procedure were repeated 100 times from the same population, approximately 95 of the resulting intervals would be expected to contain the true population mean. The frequentist approach sees the true population mean as a fixed unknown constant, while the confidence interval is calculated using data from a random sample. Because the sample is random, the interval endpoints are random variables.
Let be a random sample from a probability distribution with statistical parameter . Here, is the quantity to be estimated, while includes other parameters (if any) that determine the distribution. A confidence interval for the parameter , with confidence level or coefficient , is an interval determined by random variables and with the property:
The number , which is typically large (e.g. 0.95), is sometimes given in the form (or as a percentage ), where is a small positive number, often 0.05. It means that the interval has a probability of covering the value of in repeated sampling.
Alternatively, some authors[4] simply require that
The confidence level can be described as "at least ". When it is known that the coverage probability can be strictly larger than for some parameter values, the confidence interval is called conservative, i.e., it errs on the safe side.
In many applications, confidence intervals that have exactly the required confidence level are hard to construct, but approximate intervals can be computed. The rule for constructing the interval may be accepted if
to an acceptable level of approximation.
There are many ways of calculating confidence intervals, and the best method depends on the situation. Two widely applicable methods are bootstrapping and the central limit theorem.[2] The latter method works only if the sample is large, since it entails calculating the sample mean and sample standard deviation and using the asymptotically standard normal quantity
where and are the population mean and the sample size, respectively.
Suppose is an independent sample from a normally distributed population with unknown parameters mean and variance Define the sample mean and unbiased sample variance as
Then the value
has a Student's t distribution with degrees of freedom.[5] This value is useful because its distribution does not depend on the values of the unobservable parameters and ; i.e., it is a pivotal quantity.
Suppose we wanted to calculate a 95% confidence interval for First, let be the 97.5th percentile of the distribution of . Then there is a 2.5% chance that will be less than and a 2.5% chance that it will be larger than (as the t distribution is symmetric about 0). In other words,
Consequently, by replacing with and re-arranging terms,
where is the probability measure for the sample .
It means that there is 95% probability with which this condition occurs in repeated sampling. After observing a sample, we find values for and for from which we compute the below interval, and we say it is a 95% confidence interval for the mean.
Various interpretations of a confidence interval can be given (taking the 95% confidence interval as an example in the following).

Confidence intervals and levels are frequently misunderstood, and published studies have shown that even professional scientists often misinterpret them.[9]
Contrary to common misconceptions, a 95% confidence level does not mean that:
For example, suppose a factory produces metal rods, and a random sample of 25 rods gives a 95% confidence interval of 36.8 to 39.0 mm for the population mean length.[12]
Instead, the 95% confidence level means that if we took 100 such samples, we would expect the true population mean to lie within approximately 95 of the calculated intervals.[1][10][11][12]

Interpreting confidence intervals is especially tricky when multiple groups are involved. Two common misconceptions are: that two groups are significantly different if their CIs "just touch," and that they differ when one group's CI excludes the other's mean. Neither of these is true in general, but even experienced researchers often make these mistakes.[13]
A confidence interval is used to estimate a population parameter, such as the mean. For example, the expected value of a fair six-sided die is 3.5. Based on repeated sampling, after computing many 95% confidence intervals, roughly 95% of them will contain 3.5 (and the width of the confidence interval shrinks with sample size).
A prediction interval, on the other hand, provides a range within which a future individual observation is expected to fall with a certain probability. In the case of a single roll of a fair six-sided die, an exact 95% prediction interval does not exist. However, there are exact 95% prediction intervals for rolling a twenty-sided die. One such interval is , since 95% of the time the roll will result in a 19 or less, and the remaining 5% will result in a 20.
The key distinction is that confidence intervals quantify uncertainty in estimating parameters, while prediction intervals quantify uncertainty in forecasting future observations.
In many common settings, such as estimating the mean of a normal distribution with known variance,[14] confidence intervals coincide with credible intervals under non-informative priors. In such cases, common misconceptions about confidence intervals (e.g. interpreting them as probability statements about the parameter) may yield practically correct conclusions.

Welch[15] presented an example which clearly shows the difference between the theory of confidence intervals and other theories of interval estimation (including Fisher's fiducial intervals and objective Bayesian intervals). Robinson[16] called this example "[p]ossibly the best known counterexample for Neyman's version of confidence interval theory." To Welch, it showed the superiority of confidence interval theory; to critics of the theory, it shows a deficiency. Here we present a simplified version.
Suppose that are independent observations from a uniform distribution. Then the optimal 50% confidence procedure for is[17]
A fiducial or objective Bayesian argument can be used to derive the interval estimate which is also a 50% confidence procedure. Welch showed that the first confidence procedure dominates the second, according to desiderata from confidence interval theory; for every , the probability that the first procedure contains is less than or equal to the probability that the second procedure contains . The average width of the intervals from the first procedure is less than that of the second. Hence, the first procedure is preferred under classical confidence interval theory.
However, when , intervals from the first procedure are guaranteed to contain the true value : Therefore, the nominal 50% confidence coefficient is unrelated to the uncertainty we should have that a specific interval contains the true value. The second procedure does not have this property.
Moreover, when the first procedure generates a very short interval, this indicates that are very close together and hence only offer the information in a single data point. Yet the first interval will exclude almost all reasonable values of the parameter due to its short width. The second procedure does not have this property.
The two counter-intuitive properties of the first procedure – 100% coverage when are far apart and almost 0% coverage when are close together – balance out to yield 50% coverage on average. However, despite the first procedure being optimal, its intervals offer neither an assessment of the precision of the estimate nor an assessment of the uncertainty one should have that the interval contains the true value.
This example is used to argue against naïve interpretations of confidence intervals. If a confidence procedure is asserted to have properties beyond that of the nominal coverage (such as relation to precision, or a relationship with Bayesian inference), those properties must be proved; they do not follow from the fact that a procedure is a confidence procedure.
Steiger[18] suggested a number of confidence procedures for common effect size measures in ANOVA. Morey et al.[10] point out that several of these confidence procedures, including the one for ω2, have the property that as the F statistic becomes increasingly small—indicating misfit with all possible values of ω2—the confidence interval shrinks and can even contain only the single value ω2 = 0; that is, the CI is infinitesimally narrow (this occurs when for a CI).
This behavior is consistent with the relationship between the confidence procedure and significance testing: as F becomes so small that the group means are much closer together than we would expect by chance, a significance test might indicate rejection for most or all values of ω2. Hence the interval will be very narrow or even empty (or, by a convention suggested by Steiger, containing only 0). However, this does not indicate that the estimate of ω2 is very precise. In a sense, it indicates the opposite: that the trustworthiness of the results themselves may be in doubt. This is contrary to the common interpretation of confidence intervals that they reveal the precision of the estimate.
Methods for calculating confidence intervals for the binomial proportion appeared from the 1920s.[19][20] The main ideas of confidence intervals in general were developed in the early 1930s,[21][22][23] and the first thorough and general account was given by Jerzy Neyman in 1937.[7]
Neyman described the development of the ideas as follows (reference numbers have been changed):[23]
[My work on confidence intervals] originated about 1930 from a simple question of Waclaw Pytkowski, then my student in Warsaw, engaged in an empirical study in farm economics. The question was: how to characterize non-dogmatically the precision of an estimated regression coefficient? ...
Pytkowski's monograph ... appeared in print in 1932.[24] It so happened that, somewhat earlier, Fisher published his first paper[25] concerned with fiducial distributions and fiducial argument. Quite unexpectedly, while the conceptual framework of fiducial argument is entirely different from that of confidence intervals, the specific solutions of several particular problems coincided. Thus, in the first paper in which I presented the theory of confidence intervals, published in 1934,[21] I recognized Fisher's priority for the idea that interval estimation is possible without any reference to Bayes' theorem and with the solution being independent from probabilities a priori. At the same time I mildly suggested that Fisher's approach to the problem involved a minor misunderstanding.
In medical journals, confidence intervals were promoted in the 1970s but only became widely used in the 1980s.[26] By 1988, medical journals were requiring the reporting of confidence intervals.[27]
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In frequentist inference, a confidence interval (CI) determines lower and upper bounds likely to contain (in repeated sampling) the true value of an unknown statistical parameter, such as a population mean. Rather than reporting a single point estimate (e.g. "the average screen time is 3 hours per day"), a confidence interval provides an interval, such as from 2 hours to 4 hours. A confidence interval is based on a pre-defined coverage probability, called confidence level, typically 95%. A 95% confidence level does not imply a 95% probability that the true parameter lies within a particular CI calculated from a sample (such interpretation would be associated with the credible interval in Bayesian inference). The confidence level instead reflects the long-run performance of the method used to generate the interval. In other words, if the same sampling procedure were repeated 100 times from the same population, approximately 95 of the resulting intervals would be expected to contain the true population mean. The frequentist approach sees the true population mean as a fixed unknown constant, while the confidence interval is calculated using data from a random sample. Because the sample is random, the interval endpoints are random variables.
The Challenger Deep is the deepest known point of the seabed of Earth, located in the western Pacific Ocean at the southern end of the Mariana Trench, in the ocean territory of the Federated States of Micronesia. The GEBCO Gazetteer of Undersea Feature Names indicates that the feature is situated at 11°22.4′N 142°35.5′E and has an approximated maximum depth of 5,962 to 6,020 fathoms (10,903 to 11,009 m; 35,772 to 36,120 ft) below sea level. A 2011 study placed the depth at 5,971 ± 5 fathoms (10,920 ± 9 m; 35,826 ± 30 ft) with a 2021 study revising the value to 10,935 ± 6 m (35,876 ± 20 ft) at a 95% confidence level. The depression is named after the British Royal Navy survey ships HMS Challenger, whose expedition of 1872–1876 first located it, and HMS Challenger II, whose expedition of 1950–1952 established its record-setting depth. The first descent by any vehicle was conducted by the United States Navy using the bathyscaphe Trieste in January 1960. As of July 2022, there were 27 people who have descended to the Challenger Deep.
In statistics, the 68–95–99.7 rule, also known as the empirical rule or 68–95–99.7 rule for a normal distribution and sometimes abbreviated 3sr or 3 σ, is a shorthand used to remember the percentage of values that lie within an interval estimate in a normal distribution: approximately 68%, 95%, and 99.7% of the values lie within one, two, and three standard deviations of the mean, respectively. In mathematical notation, these facts can be expressed as follows, where Pr() is the probability function, Χ is an observation from a normally distributed random variable, μ (mu) is the mean of the distribution, and σ (sigma) is its standard deviation: Pr ( μ − 1 σ ≤ X ≤ μ + 1 σ ) ≈ 68.27 % Pr ( μ − 2 σ ≤ X ≤ μ + 2 σ ) ≈ 95.45 % Pr ( μ − 3 σ ≤ X ≤ μ + 3 σ ) ≈ 99.73 % {\displaystyle {\begin{aligned}\Pr(\mu -1\sigma \leq X\leq \mu +1\sigma )&\approx 68.27\%\\\Pr(\mu -2\sigma \leq X\leq \mu +2\sigma )&\approx 95.45\%\\\Pr(\mu -3\sigma \leq X\leq \mu +3\sigma )&\approx 99.73\%\end{aligned}}} The usefulness of this heuristic depends especially on the question under consideration and the manner in which the data have been collected; most particularly the heuristic depends on the data genuinely being normally distributed: Among the many bell-shaped distributions often seen in real-life data, the normal distribution has notoriously "thin tails" – an unusual concentration of probability near its center. If the datum X is instead governed by one of the many similar-appearing and commonly encountered distributions that have "fatter tails" – with probability more spread-out – the significance would be lower for all three deviations from the mean. In the empirical sciences, the so-called three-sigma rule of thumb (or 3 σ rule) expresses a conventional heuristic that nearly all values are taken to lie within three standard deviations of the mean, and thus it is empirically useful to treat 99.7% probability as near certainty. In the social sciences, a result may be considered statistically significant (clear enough to warrant closer examination) if its confidence level is of the order of a two-sigma effect (95%), while in particle physics, there is a convention of requiring statistical significance of a five-sigma effect (99.99994% confidence) to qualify as a discovery. A weaker three-sigma rule can be derived from Chebyshev's inequality, stating that even for non-normally distributed variables, at least 88.8% of cases should fall within properly calculated three-sigma intervals. For unimodal distributions, the probability of being within three-sigma is at least 95% by the Vysochanskij–Petunin inequality. There may be certain assumptions for a distribution that force this probability to be at least 98%.
In statistics, Dixon's Q test, or simply the Q test, is used for identification and rejection of outliers. This assumes normal distribution and per Robert Dean and Wilfrid Dixon, and others, this test should be used sparingly and never more than once in a data set. To apply a Q test for bad data, arrange the data in order of increasing values and calculate Q as defined: Q = gap range {\displaystyle Q={\frac {\text{gap}}{\text{range}}}} Where gap is the absolute difference between the outlier in question and the closest number to it. If Q > Qtable, where Qtable is a reference value corresponding to the sample size and confidence level, then reject the questionable point. Note that only one point may be rejected from a data set using a Q test.
Before the 1921 destruction of Tulsa’s Greenwood District, Black residents had created a remarkable center of business and community life. The district included stores, professional offices, entertainment venues and homes owned by Black citizens. Understanding Greenwood means learning what was built—not only what was burned.
MORE →The Greenwood District.