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Произведение коэффициента стьюдента на ошибку генерального среднего называют

В отличие от критериев
Розенбаума и Манна-Уитни критерий t
Стьюдента является параметрическим,
т. е. основан на определении основных
статистических показателей – средних
значений в каждой выборке (и)
и их дисперсий (s2x
и s2y),
рассчитываемых по стандартным формулам
(см. раздел 5).

Использование критерия
Стьюдента предполагает соблюдение
следующих условий:

  1. Распределения значений
    для обеих выборок должны соответствовать
    закону нормального распределения (см.
    раздел 6).

  2. Суммарный объем выборок
    должен быть не менее 30 (для β1
    = 0,95) и не менее 100 (для β2
    = 0,99).

  3. Объемы двух выборок
    не должны существенно отличаться друг
    от друга (не более чем в 1,5 ÷ 2 раза).

Идея критерия Стьюдента
достаточно проста. Предположим, что
значения переменных в каждой из выборок
распределяются по нормальному закону,
т. е. мы имеем дело с двумя нормальными
распределениями, отличающимися друг
от друга по средним значениям и дисперсии
(соответственно
и,и,
см. рис. 7.1).

sx

sy

Рис.
7.1. Оценка различий между двумя независимыми
выборками:
и
средние значения выборок x
и y;
sx

и sy

стандартные отклонения

Нетрудно понять, что
различия между двумя выборками будут
тем больше, чем больше разность между
средними значениями и чем меньше их
дисперсии (или стандартные отклонения).

В
случае независимых выборок коэффициент
Стьюдента определяют по формуле:

(7.2)

где nx
и ny
– соответственно численность выборок
x
и y.

После вычисления
коэффициента Стьюдента в таблице
стандартных (критических) значений t
(см. Приложение, табл. Х) находят величину,
соответствующую числу степеней свободы
n
= n
x
+ ny
– 2, и сравнивают
ее с рассчитанной по формуле. Если tэксп.
£
tкр.,
то гипотезу о достоверности различий
между выборками отвергают, если же
tэксп.
> tкр.,
то ее принимают. Другими словами, выборки
достоверно отличаются друг от друга,
если вычисленный по формуле коэффициент
Стьюдента больше табличного значения
для соответствующего уровня значимости.

В рассмотренной нами
ранее задаче вычисление средних значений
и дисперсий дает следующие значения:
xср.
= 38,5; σх2
= 28,40; уср.
= 36,2; σу2
= 31,72.

Можно видеть, что
среднее значение тревожности в группе
девушек выше, чем в группе юношей. Тем
не менее эти различия настолько
незначительны, что вряд ли они являются
статистически значимыми. Разброс
значений у юношей, напротив, несколько
выше, чем у девушек, но различия между
дисперсиями также невелики.

Подставляем
значения в формулу:

Вывод

tэксп.
= 1,14 < tкр.
= 2,05 (β1
= 0,95). Различия между двумя сравниваемыми
выборками не являются статистически
достоверными. Данный вывод вполне
согласуется с таковым, полученным при
использовании критериев Розенбаума и
Манна-Уитни.

Другой
способ определения различий между двумя
выборками по критерию Стьюдента состоит
в вычислении доверительного интервала
стандартных отклонений. Доверительным
интервалом называется среднеквадратичное
(стандартное) отклонение, деленное на
корень квадратный из объема выборки и
умноженное на стандартное значение
коэффициента Стьюдента для n
– 1 степеней свободы (соответственно,
и).

Примечание

Величина
=mx
называется
среднеквадратичной ошибкой (см. раздел
5). Следовательно, доверительный интервал
есть среднеквадратичная ошибка,
умноженная на коэффициент Стьюдента
для данного объема выборки, где число
степеней свободы ν = n
– 1, и заданного уровня значимости.

Две
независимые друг от друга выборки
считаются достоверно различающимися,
если доверительные интервалы для этих
выборок не перекрываются друг с другом.
В нашем случае мы имеем для первой
выборки 38,5 ± 2,84, для второй 36,2 ± 3,38.

Следовательно,
случайные вариации xi
лежат в диапазоне 35,66 ¸
41,34, а вариации yi
– в диапазоне 32,82 ¸
39,58. На основании этого можно констатировать,
что различия между выборками x
и y
статистически недостоверны (диапазоны
вариаций перекрываются друг с другом).
При этом следует иметь в виду, что ширина
зоны перекрытия в данном случае не имеет
значения (важен лишь сам факт перекрытия
доверительных интервалов).

Метод
Стьюдента для зависимых друг от друга
выборок (например, для сравнения
результатов, полученных при повторном
тестировании на одной и той же выборке
испытуемых) используют достаточно
редко, поскольку для этих целей существуют
другие, более информативные статистические
приемы (см. раздел 10). Тем не менее, для
данной цели в первом приближении можно
использовать формулу Стьюдента следующего
вида:

(7.3)

Полученный результат
сравнивают с табличным значением для
n
– 1 степеней свободы, где n
– число пар значений x
и y.
Результаты сравнения интерпретируются
точно так же, как и в случае вычисления
различий между двумя независимыми
выборками.

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Коэффициенты Стьюдента

Коэффициенты Стьюдента

Кванти́ли (проценти́ли) распределе́ния Стью́дента (коэффициенты Стьюдента) — числовые характеристики, широко используемые в задачах математической статистики таких как построение доверительных интервалов и проверка статистических гипотез.

Содержание

  • 1 Определение
  • 2 Замечания
  • 3 Таблица квантилей
    • 3.1 Пример
  • 4 См. также

Определение

Пусть Fn — функция распределения Стьюдента t(n) с n степенями свободы, и alpha in [0,1]. Тогда α-квантилью этого распределения называется число tα,n такое, что

F_nleft(t_{alpha,n}right) = alpha.

Замечания

F_n^{-1}(alpha) = t_{alpha,n}.
  • Функция F^{-1}_n не имеет простого представления. Однако, возможно вычислить её значения численно.
  • Распределение t(n) симметрично. Следовательно,
t1 − α,n = − tα,n.

Таблица квантилей

Нижеприведённая таблица получена с помощью функции tinv пакета tα,n, необходимо найти строку, соответствующую нужному n, и колонку, соответствующую нужному α. Искомое число находится в таблице на их пересечении.

Пример

t0.2,4 = 0.2707;
t0.8,4 = − t0.2,4 = − 0.2707.

См. также

  • Распределение Стьюдента;
  • Доверительный интервал для математического ожидания нормальной выборки.

Квантили tα,n

two-tailed test 1-0.9/2 1-0.8/2 1-0.7/2 1-0.6/2 1-0.5/2 1-0.4/2 1-0.3/2 1-0.2/2 1-0.1/2 1-0.05/2 1-0.02/2
one-tailed test 1-0.9 1-0.8 1-0.7 1-0.6 1-0.5 1-0.4 1-0.3 1-0.2 1-0.1 1-0.05 1-0.02
1 0.1584 0.3249 0.5095 0.7265 1.0000 1.3764 1.9626 3.0777 6.3138 12.7062 31.8205
2 0.1421 0.2887 0.4447 0.6172 0.8165 1.0607 1.3862 1.8856 2.9200 4.3027 6.9646
3 0.1366 0.2767 0.4242 0.5844 0.7649 0.9785 1.2498 1.6377 2.3534 3.1824 4.5407
4 0.1338 0.2707 0.4142 0.5686 0.7407 0.9410 1.1896 1.5332 2.1318 2.7764 3.7469
5 0.1322 0.2672 0.4082 0.5594 0.7267 0.9195 1.1558 1.4759 2.0150 2.5706 3.3649
6 0.1311 0.2648 0.4043 0.5534 0.7176 0.9057 1.1342 1.4398 1.9432 2.4469 3.1427
7 0.1303 0.2632 0.4015 0.5491 0.7111 0.8960 1.1192 1.4149 1.8946 2.3646 2.9980
8 0.1297 0.2619 0.3995 0.5459 0.7064 0.8889 1.1081 1.3968 1.8595 2.3060 2.8965
9 0.1293 0.2610 0.3979 0.5435 0.7027 0.8834 1.0997 1.3830 1.8331 2.2622 2.8214
10 0.1289 0.2602 0.3966 0.5415 0.6998 0.8791 1.0931 1.3722 1.8125 2.2281 2.7638
11 0.1286 0.2596 0.3956 0.5399 0.6974 0.8755 1.0877 1.3634 1.7959 2.2010 2.7181
12 0.1283 0.2590 0.3947 0.5386 0.6955 0.8726 1.0832 1.3562 1.7823 2.1788 2.6810
13 0.1281 0.2586 0.3940 0.5375 0.6938 0.8702 1.0795 1.3502 1.7709 2.1604 2.6503
14 0.1280 0.2582 0.3933 0.5366 0.6924 0.8681 1.0763 1.3450 1.7613 2.1448 2.6245
15 0.1278 0.2579 0.3928 0.5357 0.6912 0.8662 1.0735 1.3406 1.7531 2.1314 2.6025
16 0.1277 0.2576 0.3923 0.5350 0.6901 0.8647 1.0711 1.3368 1.7459 2.1199 2.5835
17 0.1276 0.2573 0.3919 0.5344 0.6892 0.8633 1.0690 1.3334 1.7396 2.1098 2.5669
18 0.1274 0.2571 0.3915 0.5338 0.6884 0.8620 1.0672 1.3304 1.7341 2.1009 2.5524
19 0.1274 0.2569 0.3912 0.5333 0.6876 0.8610 1.0655 1.3277 1.7291 2.0930 2.5395
20 0.1273 0.2567 0.3909 0.5329 0.6870 0.8600 1.0640 1.3253 1.7247 2.0860 2.5280
21 0.1272 0.2566 0.3906 0.5325 0.6864 0.8591 1.0627 1.3232 1.7207 2.0796 2.5176
22 0.1271 0.2564 0.3904 0.5321 0.6858 0.8583 1.0614 1.3212 1.7171 2.0739 2.5083
23 0.1271 0.2563 0.3902 0.5317 0.6853 0.8575 1.0603 1.3195 1.7139 2.0687 2.4999
24 0.1270 0.2562 0.3900 0.5314 0.6848 0.8569 1.0593 1.3178 1.7109 2.0639 2.4922
25 0.1269 0.2561 0.3898 0.5312 0.6844 0.8562 1.0584 1.3163 1.7081 2.0595 2.4851
26 0.1269 0.2560 0.3896 0.5309 0.6840 0.8557 1.0575 1.3150 1.7056 2.0555 2.4786
27 0.1268 0.2559 0.3894 0.5306 0.6837 0.8551 1.0567 1.3137 1.7033 2.0518 2.4727
28 0.1268 0.2558 0.3893 0.5304 0.6834 0.8546 1.0560 1.3125 1.7011 2.0484 2.4671
29 0.1268 0.2557 0.3892 0.5302 0.6830 0.8542 1.0553 1.3114 1.6991 2.0452 2.4620
30 0.1267 0.2556 0.3890 0.5300 0.6828 0.8538 1.0547 1.3104 1.6973 2.0423 2.4573
31 0.1267 0.2555 0.3889 0.5298 0.6825 0.8534 1.0541 1.3095 1.6955 2.0395 2.4528
32 0.1267 0.2555 0.3888 0.5297 0.6822 0.8530 1.0535 1.3086 1.6939 2.0369 2.4487
33 0.1266 0.2554 0.3887 0.5295 0.6820 0.8526 1.0530 1.3077 1.6924 2.0345 2.4448
34 0.1266 0.2553 0.3886 0.5294 0.6818 0.8523 1.0525 1.3070 1.6909 2.0322 2.4411
35 0.1266 0.2553 0.3885 0.5292 0.6816 0.8520 1.0520 1.3062 1.6896 2.0301 2.4377
36 0.1266 0.2552 0.3884 0.5291 0.6814 0.8517 1.0516 1.3055 1.6883 2.0281 2.4345
37 0.1265 0.2552 0.3883 0.5289 0.6812 0.8514 1.0512 1.3049 1.6871 2.0262 2.4314
38 0.1265 0.2551 0.3882 0.5288 0.6810 0.8512 1.0508 1.3042 1.6860 2.0244 2.4286
39 0.1265 0.2551 0.3882 0.5287 0.6808 0.8509 1.0504 1.3036 1.6849 2.0227 2.4258
40 0.1265 0.2550 0.3881 0.5286 0.6807 0.8507 1.0500 1.3031 1.6839 2.0211 2.4233
41 0.1264 0.2550 0.3880 0.5285 0.6805 0.8505 1.0497 1.3025 1.6829 2.0195 2.4208
42 0.1264 0.2550 0.3880 0.5284 0.6804 0.8503 1.0494 1.3020 1.6820 2.0181 2.4185
43 0.1264 0.2549 0.3879 0.5283 0.6802 0.8501 1.0491 1.3016 1.6811 2.0167 2.4163
44 0.1264 0.2549 0.3878 0.5282 0.6801 0.8499 1.0488 1.3011 1.6802 2.0154 2.4141
45 0.1264 0.2549 0.3878 0.5281 0.6800 0.8497 1.0485 1.3006 1.6794 2.0141 2.4121
46 0.1264 0.2548 0.3877 0.5281 0.6799 0.8495 1.0483 1.3002 1.6787 2.0129 2.4102
47 0.1263 0.2548 0.3877 0.5280 0.6797 0.8493 1.0480 1.2998 1.6779 2.0117 2.4083
48 0.1263 0.2548 0.3876 0.5279 0.6796 0.8492 1.0478 1.2994 1.6772 2.0106 2.4066
49 0.1263 0.2547 0.3876 0.5278 0.6795 0.8490 1.0475 1.2991 1.6766 2.0096 2.4049
50 0.1263 0.2547 0.3875 0.5278 0.6794 0.8489 1.0473 1.2987 1.6759 2.0086 2.4033
100 0.1260 0.2540 0.3864 0.5261 0.6770 0.8452 1.0418 1.2901 1.6602 1.9840 2.3642
1000 0.1257 0.2534 0.3854 0.5246 0.6747 0.8420 1.0370 1.2824 1.6464 1.9623 2.3301

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Полезное

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  • Процентили распределения Стьюдента — Квантили (процентили) распределения Стьюдента (коэффициенты Стьюдента)  числовые характеристики, широко используемые в задачах математической статистики таких как построение доверительных интервалов и проверка статистических гипотез. Содержание 1 …   Википедия

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Доверительные интервалы

Общий обзор

Доверительный интервал для среднего

Доверительный интервал для пропорции

Интерпретация доверительных интервалов

Общий обзор

Взяв выборку из популяции, мы получим точечную оценку интересующего нас параметра и вычислим стандартную ошибку для того, чтобы указать точность оценки.

Однако, для большинства случаев стандартная ошибка как такова не приемлема. Гораздо полезнее объединить эту меру точности с интервальной оценкой для параметра популяции.

Это можно сделать, используя знания о теоретическом распределении вероятности выборочной статистики (параметра) для того, чтобы вычислить доверительный интервал (CI – Confidence Interval, ДИ – Доверительный интервал) для параметра.

Вообще, доверительный интервал расширяет оценки в обе стороны некоторой величиной, кратной стандартной ошибке (данного параметра); два значения (доверительные границы), определяющие интервал, обычно отделяют запятой и заключают в скобки.

Доверительный интервал для среднего

Использование нормального распределения

Выборочное среднее имеет нормальное распределение, если объем выборки большой, поэтому можно применить знания о нормальном распределении при рассмотрении выборочного среднего.

В частности, 95% распределения выборочных средних находится в пределах 1,96 стандартных отклонений (SD) среднего популяции.

Когда у нас есть только одна выборка, мы называем это стандартной ошибкой среднего (SEM)  и вычисляем 95% доверительного интервала для среднего следующим образом:

Если повторить этот эксперимент несколько раз, то интервал будет содержать истинное среднее популяции в 95% случаев.

Обычно это доверительный интервал как, например, интервал значений, в пределах которого с доверительной вероятностью 95% находится истинное  среднее популяции (генеральное среднее).

Хотя это не вполне строго (среднее в популяции есть фиксированное значение и поэтому не может иметь вероятность, отнесённую к нему) таким образом интерпретировать доверительный интервал, но концептуально это удобнее для понимания.

Использование t-распределения

Можно использовать нормальное распределение, если знать  значение дисперсии в популяции. Кроме того, когда объем выборки небольшой, выборочное среднее отвечает нормальному распределению, если данные, лежащие в основе популяции, распределены нормально.

Если данные, лежащие в основе популяции, распределены ненормально и/или неизвестна генеральная дисперсия (дисперсия в популяции), выборочное  среднее подчиняется t-распределению Стьюдента.

Вычисляем 95% доверительный интервал для генерального среднего в популяции следующим образом:

где   — процентная точка (процентиль) t-распределения Стьюдента с (n-1) степенями свободы, которая даёт двухстороннюю вероятность 0,05.

Вообще, она обеспечивает более широкий интервал, чем при использовании нормального распределения, поскольку учитывает дополнительную неопределенность, которую вводят, оценивая стандартное отклонение популяции и/или из-за небольшого объёма выборки.

Когда объём выборки большой (порядка 100 и более), разница между двумя распределениями (t-Стьюдента и нормальным) незначительна. Тем не менее всегда используют t-распределение при вычислении доверительных интервалов, даже если объем выборки большой.

Обычно указывают 95% ДИ. Можно вычислить другие доверительные интервалы, например 99% ДИ для среднего.

Вместо произведения стандартной ошибки и табличного значения t-распределения, которое соответствует двусторонней вероятности 0,05, умножают её (стандартную ошибку) на значение, которое соответствует двусторонней вероятности 0,01. Это более широкий доверительный интервал, чем в случае 95%, поскольку он отражает увеличенное доверие к тому, что интервал действительно включает среднее популяции.

Доверительный интервал для пропорции

Выборочное распределение пропорций имеет биномиальное распределение. Однако если объём выборки n разумно большой, тогда выборочное распределение пропорции приблизительно нормально со средним .

Оцениваем выборочным отношением p=r/n (где r– количество индивидуумов в выборке с интересующими нас характерными особенностями), и стандартная ошибка оценивается:

95% доверительный интервал для пропорции оценивается:

Если объём выборки небольшой (обычно когда np или n(1-p) меньше 5), тогда необходимо использовать биномиальное распределение для того, чтобы вычислить точные доверительные интервалы.

Заметьте, что если p выражается в процентах, то (1-p) заменяют на (100-p).

Интерпретация доверительных интервалов

При интерпретации доверительного интервала нас интересуют следующие вопросы:

Насколько широк доверительный интервал?

Широкий доверительный интервал указывает на то, что оценка неточна; узкий указывает на точную оценку.

Ширина доверительного интервала зависит от размера стандартной ошибки, которая, в свою очередь, зависит от объёма выборки и при рассмотрении числовой переменной от изменчивости данных дают более широкие доверительные интервалы, чем исследования многочисленного набора данных немногих переменных.

Включает ли ДИ какие-либо значения, представляющие особенный интерес?

Можно проверить, ложится ли вероятное значение для параметра популяции в пределы доверительного интервала. Если да, то результаты согласуются с этим вероятным значением. Если нет, тогда маловероятно (для 95% доверительного интервала шанс почти 5%), что параметр имеет это значение.

Связанные определения:
Доверительный интервал
Доверительный предел
Коэффициент доверия
Оценка
Оценочная функция
Свободный от распределения доверительный интервал

В начало

Содержание портала

This article is about the mathematics of Student’s t-distribution. For its uses in statistics, see Student’s t-test.

Student’s t

Probability density function

Student t pdf.svg

Cumulative distribution function

Student t cdf.svg

Parameters nu >0 degrees of freedom (real)
Support {displaystyle xin (-infty ,infty )}
PDF textstylefrac{Gamma left(frac{nu+1}{2} right)} {sqrt{nupi},Gamma left(frac{nu}{2} right)} left(1+frac{x^2}{nu} right)^{-frac{nu+1}{2}}!
CDF

begin{matrix}
     frac{1}{2} + x Gamma left( frac{nu+1}{2} right)  times\[0.5em]
     frac{,_2F_1 left ( frac{1}{2},frac{nu+1}{2};frac{3}{2};
           -frac{x^2}{nu} right)}
     {sqrt{pinu},Gamma left(frac{nu}{2}right)}
     end{matrix}

where 2F1 is the hypergeometric function

Mean 0 for nu > 1, otherwise undefined
Median 0
Mode 0
Variance textstylefrac{nu}{nu-2} for nu > 2, ∞ for 1 < nu le 2, otherwise undefined
Skewness 0 for nu > 3, otherwise undefined
Ex. kurtosis textstylefrac{6}{nu-4} for nu > 4, ∞ for 2 < nu le 4, otherwise undefined
Entropy

{displaystyle {begin{matrix}{frac {nu +1}{2}}left[psi left({frac {1+nu }{2}}right)-psi left({frac {nu }{2}}right)right]\[0.5em]+ln {left[{sqrt {nu }}Bleft({frac {nu }{2}},{frac {1}{2}}right)right]},{scriptstyle {text{(nats)}}}end{matrix}}}

  • ψ: digamma function,
  • B: beta function
MGF undefined
CF

textstylefrac{K_{nu/2} left(sqrt{nu}|t|right)
                    cdot left(sqrt{nu}|t| right)^{nu/2}}
                    {Gamma(nu/2)2^{nu/2-1}} for nu >0

  • K_nu(x): modified Bessel function of the second kind[1]

In probability and statistics, Student’s t-distribution (or simply the t-distribution) is any member of a family of continuous probability distributions that arise when estimating the mean of a normally distributed population in situations where the sample size is small and the population’s standard deviation is unknown. It was developed by English statistician William Sealy Gosset under the pseudonym «Student».

The t-distribution plays a role in a number of widely used statistical analyses, including Student’s t-test for assessing the statistical significance of the difference between two sample means, the construction of confidence intervals for the difference between two population means, and in linear regression analysis. Student’s t-distribution also arises in the Bayesian analysis of data from a normal family.

If we take a sample of n observations from a normal distribution, then the t-distribution with nu=n-1 degrees of freedom can be defined as the distribution of the location of the sample mean relative to the true mean, divided by the sample standard deviation, after multiplying by the standardizing term {sqrt {n}}. In this way, the t-distribution can be used to construct a confidence interval for the true mean.

The t-distribution is symmetric and bell-shaped, like the normal distribution. However, the t-distribution has heavier tails, meaning that it is more prone to producing values that fall far from its mean. This makes it useful for understanding the statistical behavior of certain types of ratios of random quantities, in which variation in the denominator is amplified and may produce outlying values when the denominator of the ratio falls close to zero. The Student’s t-distribution is a special case of the generalized hyperbolic distribution.

History and etymology[edit]

Statistician William Sealy Gosset, known as «Student»

In statistics, the t-distribution was first derived as a posterior distribution in 1876 by Helmert[2][3][4] and Lüroth.[5][6][7] The t-distribution also appeared in a more general form as Pearson Type IV distribution in Karl Pearson’s 1895 paper.[8]

In the English-language literature, the distribution takes its name from William Sealy Gosset’s 1908 paper in Biometrika under the pseudonym «Student».[9] One version of the origin of the pseudonym is that Gosset’s employer preferred staff to use pen names when publishing scientific papers instead of their real name, so he used the name «Student» to hide his identity. Another version is that Guinness did not want their competitors to know that they were using the t-test to determine the quality of raw material.[10][11]

Gosset worked at the Guinness Brewery in Dublin, Ireland, and was interested in the problems of small samples – for example, the chemical properties of barley where sample sizes might be as few as 3. Gosset’s paper refers to the distribution as the «frequency distribution of standard deviations of samples drawn from a normal population». It became well known through the work of Ronald Fisher, who called the distribution «Student’s distribution» and represented the test value with the letter t.[12][13]

How Student’s distribution arises from sampling[edit]

Let {textstyle X_{1},ldots ,X_{n}} be independently and identically drawn from the distribution {mathcal {N}}(mu ,sigma ^{2}), i.e. this is a sample of size n from a normally distributed population with expected mean value mu and variance sigma ^{2}.

Let

{displaystyle {bar {X}}={frac {1}{n}}sum _{i=1}^{n}X_{i}}

be the sample mean and let

{displaystyle S^{2}={frac {1}{n-1}}sum _{i=1}^{n}(X_{i}-{bar {X}})^{2}}

be the (Bessel-corrected) sample variance. Then the random variable

{displaystyle {frac {{bar {X}}-mu }{sigma /{sqrt {n}}}}}

has a standard normal distribution (i.e. normal with expected mean 0 and variance 1), and the random variable

{displaystyle {frac {{bar {X}}-mu }{S/{sqrt {n}}}}}

i.e where S has been substituted for sigma , has a Student’s t-distribution with n-1 degrees of freedom. Since {textstyle S} has replaced {textstyle sigma ,} the only unobservable quantity in this expression is {textstyle mu ,} so this can be used to derive confidence intervals for {textstyle mu .} The numerator and the denominator in the preceding expression are statistically independent random variables despite being based on the same sample {textstyle X_{1},ldots ,X_{n}}. This can be seen by observing that {textstyle operatorname {cov} ({overline {X}},,X_{i}-{overline {X}})=0,} and recalling that {textstyle {overline {X}}} and {textstyle X_{i}-{overline {X}}} are both linear combinations of the same set of i.i.d. normally distributed random variables.

Definition[edit]

Probability density function[edit]

Student’s t-distribution has the probability density function (PDF) given by

{displaystyle f(t)={frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}left(1+{frac {t^{2}}{nu }}right)^{-(nu +1)/2},}

where nu is the number of degrees of freedom and Gamma is the gamma function. This may also be written as

{displaystyle f(t)={frac {1}{{sqrt {nu }},mathrm {B} ({frac {1}{2}},{frac {nu }{2}})}}left(1+{frac {t^{2}}{nu }}right)^{-(nu +1)/2},}

where B is the Beta function. In particular for integer valued degrees of freedom  nu we have:

For {displaystyle nu >1} even,

{displaystyle {frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}={frac {(nu -1)(nu -3)cdots 5cdot 3}{2{sqrt {nu }}(nu -2)(nu -4)cdots 4cdot 2,}}cdot }

For {displaystyle nu >1} odd,

{displaystyle {frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}={frac {(nu -1)(nu -3)cdots 4cdot 2}{pi {sqrt {nu }}(nu -2)(nu -4)cdots 5cdot 3,}}cdot !}

The probability density function is symmetric, and its overall shape resembles the bell shape of a normally distributed variable with mean 0 and variance 1, except that it is a bit lower and wider. As the number of degrees of freedom grows, the t-distribution approaches the normal distribution with mean 0 and variance 1. For this reason {nu } is also known as the normality parameter.[14]

The following images show the density of the t-distribution for increasing values of nu . The normal distribution is shown as a blue line for comparison. Note that the t-distribution (red line) becomes closer to the normal distribution as nu increases.

1 degree of freedom

2 degrees of freedom

3 degrees of freedom

5 degrees of freedom

10 degrees of freedom

30 degrees of freedom

Cumulative distribution function[edit]

The cumulative distribution function (CDF) can be written in terms of I, the regularized
incomplete beta function. For t > 0,[15]

{displaystyle F(t)=int _{-infty }^{t}f(u),du=1-{tfrac {1}{2}}I_{x(t)}left({tfrac {nu }{2}},{tfrac {1}{2}}right),}

where

x(t) = frac{nu}{{t^2+nu}}.

Other values would be obtained by symmetry. An alternative formula, valid for t^2 < nu, is[15]

{displaystyle int _{-infty }^{t}f(u),du={tfrac {1}{2}}+t{frac {Gamma left({tfrac {1}{2}}(nu +1)right)}{{sqrt {pi nu }},Gamma left({tfrac {nu }{2}}right)}},{}_{2}F_{1}left({tfrac {1}{2}},{tfrac {1}{2}}(nu +1);{tfrac {3}{2}};-{tfrac {t^{2}}{nu }}right),}

where 2F1 is a particular case of the hypergeometric function.

For information on its inverse cumulative distribution function, see quantile function § Student’s t-distribution.

Special cases[edit]

Certain values of nu give a simple form for Student’s t-distribution.

nu PDF CDF notes
1 {displaystyle {frac {1}{pi (1+t^{2})}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}arctan(t)} See Cauchy distribution
2 {displaystyle {frac {1}{2{sqrt {2}}left(1+{frac {t^{2}}{2}}right)^{3/2}}}} {displaystyle {frac {1}{2}}+{frac {t}{2{sqrt {2}}{sqrt {1+{frac {t^{2}}{2}}}}}}}
3 {displaystyle {frac {2}{pi {sqrt {3}}left(1+{frac {t^{2}}{3}}right)^{2}}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}{left[{frac {1}{sqrt {3}}}{frac {t}{1+{frac {t^{2}}{3}}}}+arctan left({frac {t}{sqrt {3}}}right)right]}}
4 {displaystyle {frac {3}{8left(1+{frac {t^{2}}{4}}right)^{5/2}}}} {displaystyle {frac {1}{2}}+{frac {3}{8}}{frac {t}{sqrt {1+{frac {t^{2}}{4}}}}}{left[1-{frac {1}{12}}{frac {t^{2}}{1+{frac {t^{2}}{4}}}}right]}}
5 {displaystyle {frac {8}{3pi {sqrt {5}}left(1+{frac {t^{2}}{5}}right)^{3}}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}{left[{frac {t}{{sqrt {5}}left(1+{frac {t^{2}}{5}}right)}}left(1+{frac {2}{3left(1+{frac {t^{2}}{5}}right)}}right)+arctan left({frac {t}{sqrt {5}}}right)right]}}
infty {displaystyle {frac {1}{sqrt {2pi }}}e^{-t^{2}/2}} {displaystyle {frac {1}{2}}{left[1+operatorname {erf} left({frac {t}{sqrt {2}}}right)right]}} See Normal distribution, Error function

How the t-distribution arises[edit]

Sampling distribution[edit]

Let x_{1},ldots ,x_{n} be the numbers observed in a sample from a continuously distributed population with expected value mu . The sample mean and sample variance are given by:

{displaystyle {begin{aligned}{bar {x}}&={frac {x_{1}+cdots +x_{n}}{n}},\[5pt]s^{2}&={frac {1}{n-1}}sum _{i=1}^{n}(x_{i}-{bar {x}})^{2}.end{aligned}}}

The resulting t-value is

 t = frac{bar{x} - mu}{s/sqrt{n}}.

The t-distribution with n-1 degrees of freedom is the sampling distribution of the t-value when the samples consist of independent identically distributed observations from a normally distributed population. Thus for inference purposes t is a useful «pivotal quantity» in the case when the mean and variance {displaystyle (mu ,sigma ^{2})} are unknown population parameters, in the sense that the t-value has then a probability distribution that depends on neither mu nor sigma ^{2}.

Bayesian inference[edit]

In Bayesian statistics, a (scaled, shifted) t-distribution arises as the marginal distribution of the unknown mean of a normal distribution, when the dependence on an unknown variance has been marginalized out:[16]

{displaystyle {begin{aligned}p(mu mid D,I)=&int p(mu ,sigma ^{2}mid D,I),dsigma ^{2}\=&int p(mu mid D,sigma ^{2},I),p(sigma ^{2}mid D,I),dsigma ^{2},end{aligned}}}

where D stands for the data {x_i}, and I represents any other information that may have been used to create the model. The distribution is thus the compounding of the conditional distribution of mu given the data and sigma ^{2} with the marginal distribution of sigma ^{2} given the data.

With n data points, if uninformative, or flat, the location prior {displaystyle p(mu mid sigma ^{2},I)={text{const}}} can be taken for μ, and the scale prior {displaystyle p(sigma ^{2}mid I)propto 1/sigma ^{2}} can be taken for σ2, then Bayes’ theorem gives

{displaystyle {begin{aligned}p(mu mid D,sigma ^{2},I)&sim N({bar {x}},sigma ^{2}/n),\p(sigma ^{2}mid D,I)&sim operatorname {Scale-inv-} chi ^{2}(nu ,s^{2}),end{aligned}}}

a normal distribution and a scaled inverse chi-squared distribution respectively, where nu = n - 1 and

s^{2}=sum {frac  {(x_{i}-{bar  {x}})^{2}}{n-1}}.

The marginalization integral thus becomes

{displaystyle {begin{aligned}p(mu mid D,I)&propto int _{0}^{infty }{frac {1}{sqrt {sigma ^{2}}}}exp left(-{frac {1}{2sigma ^{2}}}n(mu -{bar {x}})^{2}right)cdot sigma ^{-nu -2}exp(-nu s^{2}/2sigma ^{2}),dsigma ^{2}\&propto int _{0}^{infty }sigma ^{-nu -3}exp left(-{frac {1}{2sigma ^{2}}}left(n(mu -{bar {x}})^{2}+nu s^{2}right)right),dsigma ^{2}.end{aligned}}}

This can be evaluated by substituting {displaystyle z=A/2sigma ^{2}}, where {displaystyle A=n(mu -{bar {x}})^{2}+nu s^{2}}, giving

{displaystyle dz=-{frac {A}{2sigma ^{4}}},dsigma ^{2},}

so

{displaystyle p(mu mid D,I)propto A^{-(nu +1)/2}int _{0}^{infty }z^{(nu -1)/2}exp(-z),dz.}

But the z integral is now a standard Gamma integral, which evaluates to a constant, leaving

{displaystyle {begin{aligned}p(mu mid D,I)&propto A^{-(nu +1)/2}\&propto left(1+{frac {n(mu -{bar {x}})^{2}}{nu s^{2}}}right)^{-(nu +1)/2}.end{aligned}}}

This is a form of the t-distribution with an explicit scaling and shifting that will be explored in more detail in a further section below. It can be related to the standardized t-distribution by the substitution

{displaystyle t={frac {mu -{bar {x}}}{s/{sqrt {n}}}}.}

The derivation above has been presented for the case of uninformative priors for mu and sigma ^{2}; but it will be apparent that any priors that lead to a normal distribution being compounded with a scaled inverse chi-squared distribution will lead to a t-distribution with scaling and shifting for {displaystyle P(mu mid D,I)}, although the scaling parameter corresponding to {displaystyle {frac {s^{2}}{n}}} above will then be influenced both by the prior information and the data, rather than just by the data as above.

Characterization[edit]

As the distribution of a test statistic[edit]

Student’s t-distribution with nu degrees of freedom can be defined as the distribution of the random variable T with[15][17]

{displaystyle T={frac {Z}{sqrt {V/nu }}}=Z{sqrt {frac {nu }{V}}},}

where

  • Z is a standard normal with expected value 0 and variance 1;
  • V has a chi-squared distribution (χ2-distribution) with nu degrees of freedom;
  • Z and V are independent;

A different distribution is defined as that of the random variable defined, for a given constant μ, by

(Z+mu)sqrt{frac{nu}{V}}.

This random variable has a noncentral t-distribution with noncentrality parameter μ. This distribution is important in studies of the power of Student’s t-test.

Derivation[edit]

Suppose X1, …, Xn are independent realizations of the normally-distributed, random variable X, which has an expected value μ and variance σ2. Let

overline{X}_n = frac{1}{n}(X_1+cdots+X_n)

be the sample mean, and

{displaystyle S_{n}^{2}={frac {1}{n-1}}sum _{i=1}^{n}left(X_{i}-{overline {X}}_{n}right)^{2}}

be an unbiased estimate of the variance from the sample. It can be shown that the random variable

V = (n-1)frac{S_n^2}{sigma^2}

has a chi-squared distribution with nu = n - 1 degrees of freedom (by Cochran’s theorem).[18] It is readily shown that the quantity

{displaystyle Z=left({overline {X}}_{n}-mu right){frac {sqrt {n}}{sigma }}}

is normally distributed with mean 0 and variance 1, since the sample mean {overline {X}}_{n} is normally distributed with mean μ and variance σ2/n. Moreover, it is possible to show that these two random variables (the normally distributed one Z and the chi-squared-distributed one V) are independent. Consequently[clarification needed] the pivotal quantity

{textstyle Tequiv {frac {Z}{sqrt {V/nu }}}=left({overline {X}}_{n}-mu right){frac {sqrt {n}}{S_{n}}},}

which differs from Z in that the exact standard deviation σ is replaced by the random variable Sn, has a Student’s t-distribution as defined above. Notice that the unknown population variance σ2 does not appear in T, since it was in both the numerator and the denominator, so it canceled. Gosset intuitively obtained the probability density function stated above, with nu equal to n − 1, and Fisher proved it in 1925.[12]

The distribution of the test statistic T depends on nu , but not μ or σ; the lack of dependence on μ and σ is what makes the t-distribution important in both theory and practice.

As a maximum entropy distribution[edit]

Student’s t-distribution is the maximum entropy probability distribution for a random variate X for which {displaystyle operatorname {E} (ln(nu +X^{2}))} is fixed.[19][clarification needed][better source needed]

Properties[edit]

Moments[edit]

For nu > 1, the raw moments of the t-distribution are

{displaystyle operatorname {E} (T^{k})={begin{cases}0&k{text{ odd}},quad 0<k<nu \{frac {1}{{sqrt {pi }}Gamma left({frac {nu }{2}}right)}}left[Gamma left({frac {k+1}{2}}right)Gamma left({frac {nu -k}{2}}right)nu ^{frac {k}{2}}right]&k{text{ even}},quad 0<k<nu .\end{cases}}}

Moments of order nu or higher do not exist.[20]

The term for 0 < k < nu, k even, may be simplified using the properties of the gamma function to

{displaystyle operatorname {E} (T^{k})=nu ^{frac {k}{2}},prod _{i=1}^{k/2}{frac {2i-1}{nu -2i}}qquad k{text{ even}},quad 0<k<nu .}

For a t-distribution with nu degrees of freedom, the expected value is 0 if {displaystyle nu >1}, and its variance is frac{nu}{nu-2} if nu>2. The skewness is 0 if nu > 3 and the excess kurtosis is frac{6}{nu-4} if nu > 4.

Monte Carlo sampling[edit]

There are various approaches to constructing random samples from the Student’s t-distribution. The matter depends on whether the samples are required on a stand-alone basis, or are to be constructed by application of a quantile function to uniform samples; e.g., in the multi-dimensional applications basis of copula-dependency.[citation needed] In the case of stand-alone sampling, an extension of the Box–Muller method and its polar form is easily deployed.[21] It has the merit that it applies equally well to all real positive degrees of freedom, ν, while many other candidate methods fail if ν is close to zero.[21]

Integral of Student’s probability density function and p-value[edit]

The function A(t | ν) is the integral of Student’s probability density function, f(t) between −t and t, for t ≥ 0. It thus gives the probability that a value of t less than that calculated from observed data would occur by chance. Therefore, the function A(t | ν) can be used when testing whether the difference between the means of two sets of data is statistically significant, by calculating the corresponding value of t and the probability of its occurrence if the two sets of data were drawn from the same population. This is used in a variety of situations, particularly in t-tests. For the statistic t, with ν degrees of freedom, A(t | ν) is the probability that t would be less than the observed value if the two means were the same (provided that the smaller mean is subtracted from the larger, so that t ≥ 0). It can be easily calculated from the cumulative distribution function Fν(t) of the t-distribution:

{displaystyle A(tmid nu )=F_{nu }(t)-F_{nu }(-t)=1-I_{frac {nu }{nu +t^{2}}}left({frac {nu }{2}},{frac {1}{2}}right),}

where Ix is the regularized incomplete beta function (ab).

For statistical hypothesis testing this function is used to construct the p-value.

Generalized Student’s t-distribution[edit]

In terms of scaling parameter σ̂ or σ̂2[edit]

Student’s t distribution can be generalized to a three parameter location-scale family, introducing a location parameter {hat {mu }} and a scale parameter {hat {sigma }}, through the relation

{displaystyle X={hat {mu }}+{hat {sigma }}T}

or

{displaystyle T={frac {X-{hat {mu }}}{hat {sigma }}}}

This means that {displaystyle {frac {x-{hat {mu }}}{hat {sigma }}}} has a classic Student’s t distribution with nu degrees of freedom.

The resulting non-standardized Student’s t-distribution has a density defined by:[22]

{displaystyle p(xmid nu ,{hat {mu }},{hat {sigma }})={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}}){sqrt {pi nu }}{hat {sigma }},}}left(1+{frac {1}{nu }}left({frac {x-{hat {mu }}}{hat {sigma }}}right)^{2}right)^{-(nu +1)/2}}

Here, {hat {sigma }} does not correspond to a standard deviation: it is not the standard deviation of the scaled t distribution, which may not even exist; nor is it the standard deviation of the underlying normal distribution, which is unknown. {hat {sigma }} simply sets the overall scaling of the distribution. In the Bayesian derivation of the marginal distribution of an unknown normal mean {hat {mu }} above, {hat {sigma }} as used here corresponds to the quantity {displaystyle {s/{sqrt {n}}}}, where

{displaystyle s^{2}=sum {frac {(x_{i}-{bar {x}})^{2}}{n-1}}.,}

Equivalently, the distribution can be written in terms of {hat {sigma }}^{2}, the square of this scale parameter:

{displaystyle p(xmid nu ,{hat {mu }},{hat {sigma }}^{2})={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}}){sqrt {pi nu {hat {sigma }}^{2}}}}}left(1+{frac {1}{nu }}{frac {(x-{hat {mu }})^{2}}{{hat {sigma }}^{2}}}right)^{-(nu +1)/2}}

Other properties of this version of the distribution are:[22]

{displaystyle {begin{aligned}operatorname {E} (X)&={hat {mu }}&{text{  for }}nu >1\operatorname {var} (X)&={hat {sigma }}^{2}{frac {nu }{nu -2}}&{text{  for }}nu >2\operatorname {mode} (X)&={hat {mu }}end{aligned}}}

This distribution results from compounding a Gaussian distribution (normal distribution) with mean mu and unknown variance, with an inverse gamma distribution placed over the variance with parameters a = nu/2 and {displaystyle b=nu {hat {sigma }}^{2}/2}. In other words, the random variable X is assumed to have a Gaussian distribution with an unknown variance distributed as inverse gamma, and then the variance is marginalized out (integrated out). The reason for the usefulness of this characterization is that the inverse gamma distribution is the conjugate prior distribution of the variance of a Gaussian distribution. As a result, the non-standardized Student’s t-distribution arises naturally in many Bayesian inference problems. See below.

Equivalently, this distribution results from compounding a Gaussian distribution with a scaled-inverse-chi-squared distribution with parameters nu and {hat {sigma }}^{2}. The scaled-inverse-chi-squared distribution is exactly the same distribution as the inverse gamma distribution, but with a different parameterization, i.e. {displaystyle nu =2a,;{hat {sigma }}^{2}={frac {b}{a}}}.

This version of the t-distribution can be useful in financial modeling. For example, Platen and Sidorowicz found that among the family of generalized hyperbolic distributions, this form of the t-distribution with about 4 degrees of freedom was the best fit for the (log) return of many worldwide stock indices.[23]

In terms of inverse scaling parameter λ[edit]

An alternative parameterization in terms of an inverse scaling parameter lambda (analogous to the way precision is the reciprocal of variance), defined by the relation {displaystyle lambda ={frac {1}{{hat {sigma }}^{2}}},}. The density is then given by:[24]

{displaystyle p(xmid nu ,{hat {mu }},lambda )={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}})}}left({frac {lambda }{pi nu }}right)^{1/2}left(1+{frac {lambda (x-{hat {mu }})^{2}}{nu }}right)^{-(nu +1)/2}.}

Other properties of this version of the distribution are:[24]

{displaystyle {begin{aligned}operatorname {E} (X)&={hat {mu }}&&{text{  for }}nu >1\[5pt]operatorname {var} (X)&={frac {1}{lambda }}{frac {nu }{nu -2}}&&{text{  for }}nu >2\[5pt]operatorname {mode} (X)&={hat {mu }}end{aligned}}}

This distribution results from compounding a Gaussian distribution with mean {hat {mu }} and unknown precision (the reciprocal of the variance), with a gamma distribution placed over the precision with parameters a = nu/2 and b = nu/(2lambda). In other words, the random variable X is assumed to have a normal distribution with an unknown precision distributed as gamma, and then this is marginalized over the gamma distribution.

[edit]

  • If X has a Student’s t-distribution with degree of freedom nu then X2 has an F-distribution: {displaystyle X^{2}sim mathrm {F} left(nu _{1}=1,nu _{2}=nu right)}
  • The noncentral t-distribution generalizes the t-distribution to include a location parameter. Unlike the nonstandardized t-distributions, the noncentral distributions are not symmetric (the median is not the same as the mode).
  • The discrete Student’s t-distribution is defined by its probability mass function at r being proportional to:[25]

    {displaystyle prod _{j=1}^{k}{frac {1}{(r+j+a)^{2}+b^{2}}}quad quad r=ldots ,-1,0,1,ldots .}

    Here a, b, and k are parameters. This distribution arises from the construction of a system of discrete distributions similar to that of the Pearson distributions for continuous distributions.[26]

  • One can generate Student-t samples by taking the ratio of variables from the normal distribution and the square-root of χ2-distribution. If we use instead of the normal distribution, e.g., the Irwin–Hall distribution, we obtain over-all a symmetric 4-parameter distribution, which includes the normal, the uniform, the triangular, the Student-t and the Cauchy distribution. This is also more flexible than some other symmetric generalizations of the normal distribution.
  • t-distribution is an instance of ratio distributions.

Bayesian inference: prior distribution for the degrees of the freedom[edit]

Suppose that {displaystyle x=(x_{1},cdots ,x_{N})} represents N number of independently and identically distributed samples drawn from the Student t-distribution

{displaystyle t_{nu }(x)={frac {Gamma left({frac {nu +1}{2}}right)}{{sqrt {nu pi }}Gamma left({frac {nu }{2}}right)}}left(1+{frac {x^{2}}{nu }}right)^{-{frac {nu +1}{2}}},quad xin mathbb {R} .}

With a choice a prior for the degrees of freedom nu , denoted as {displaystyle pi (nu )}, Bayesian inference seeks to evaluate the posterior distribution

{displaystyle pi (nu |{textbf {x}})={frac {prod t_{nu }(x_{i})cdot pi (nu )}{int prod t_{nu }(x_{i})cdot pi (nu )dnu }},quad nu in mathbb {R} ^{+}.}

Mean squared error comparison between Bayes estimators based on the four priors and maximum likelihood estimator for the degrees of the freedom. Data is simulated from the student t distribution with the degrees of freedom nu _{0} varying from 0 to 25 with the sample size {displaystyle N=30} (left) and {displaystyle N=100} (right). Lower value for MSE implies better accuracy.[27]

Some popular choices of the priors are:

  • Jeffreys prior [28]

{displaystyle pi _{J}(nu )propto left({frac {nu }{nu +3}}right)^{1/2}left(psi 'left({frac {nu }{2}}right)-psi 'left({frac {nu +1}{2}}right)-{frac {2(nu +3)}{nu (nu +1)^{2}}}right)^{1/2},quad nu in mathbb {R} ^{+},}
where psi '(x) represents trigamma function.

  • Exponential prior [29]

{displaystyle pi _{E}(nu )=Ga(nu |1,0.1)=exp(nu |0.1)={frac {1}{10}}e^{-nu /10},quad nu in mathbb {R} ^{+}}

  • Gamma prior [30]

{displaystyle pi _{G}(nu )=Ga(nu |2,0.1)={frac {nu }{100}}e^{-nu /10},quad nu in mathbb {R} ^{+}}

  • Log-normal prior [31]

{displaystyle pi _{L}(nu )=logN(nu |1,1)={frac {1}{nu {sqrt {2pi }}}}exp left[-{frac {(log nu -1)^{2}}{2}}right],quad nu in mathbb {R} ^{+}}

The right panels show the result of the numerical experiments. The Bayes estimator based on the Jeffreys prior {displaystyle pi _{J}(nu )} results in relatively lower Mean Squared Error (MSE ) then the Maximum Likelihood Estimator (MLE) over the values {displaystyle nu _{0}in (0,25)}. It is important to note that no Bayes estimator dominates other estimators over the interval {displaystyle (0,25)}. In other words, each Bayes estimator has its own region where the estimator is non-inferior to others.

Uses[edit]

In frequentist statistical inference[edit]

Student’s t-distribution arises in a variety of statistical estimation problems where the goal is to estimate an unknown parameter, such as a mean value, in a setting where the data are observed with additive errors. If (as in nearly all practical statistical work) the population standard deviation of these errors is unknown and has to be estimated from the data, the t-distribution is often used to account for the extra uncertainty that results from this estimation. In most such problems, if the standard deviation of the errors were known, a normal distribution would be used instead of the t-distribution.

Confidence intervals and hypothesis tests are two statistical procedures in which the quantiles of the sampling distribution of a particular statistic (e.g. the standard score) are required. In any situation where this statistic is a linear function of the data, divided by the usual estimate of the standard deviation, the resulting quantity can be rescaled and centered to follow Student’s t-distribution. Statistical analyses involving means, weighted means, and regression coefficients all lead to statistics having this form.

Quite often, textbook problems will treat the population standard deviation as if it were known and thereby avoid the need to use the Student’s t-distribution. These problems are generally of two kinds: (1) those in which the sample size is so large that one may treat a data-based estimate of the variance as if it were certain, and (2) those that illustrate mathematical reasoning, in which the problem of estimating the standard deviation is temporarily ignored because that is not the point that the author or instructor is then explaining.

Hypothesis testing[edit]

A number of statistics can be shown to have t-distributions for samples of moderate size under null hypotheses that are of interest, so that the t-distribution forms the basis for significance tests. For example, the distribution of Spearman’s rank correlation coefficient ρ, in the null case (zero correlation) is well approximated by the t distribution for sample sizes above about 20.[citation needed]

Confidence intervals[edit]

Suppose the number A is so chosen that

Pr(-A < T < A)=0.9,

when T has a t-distribution with n − 1 degrees of freedom. By symmetry, this is the same as saying that A satisfies

Pr(T < A) = 0.95,

so A is the «95th percentile» of this probability distribution, or  A=t_{(0.05,n-1)}. Then

{displaystyle Pr left(-A<{frac {{overline {X}}_{n}-mu }{S_{n}/{sqrt {n}}}}<Aright)=0.9,}

and this is equivalent to

Prleft(overline{X}_n - A frac{S_n}{sqrt{n}} < mu < overline{X}_n + Afrac{S_n}{sqrt{n}}right) = 0.9.

Therefore, the interval whose endpoints are

overline{X}_npm Afrac{S_n}{sqrt{n}}

is a 90% confidence interval for μ. Therefore, if we find the mean of a set of observations that we can reasonably expect to have a normal distribution, we can use the t-distribution to examine whether the confidence limits on that mean include some theoretically predicted value – such as the value predicted on a null hypothesis.

It is this result that is used in the Student’s t-tests: since the difference between the means of samples from two normal distributions is itself distributed normally, the t-distribution can be used to examine whether that difference can reasonably be supposed to be zero.

If the data are normally distributed, the one-sided (1 − α)-upper confidence limit (UCL) of the mean, can be calculated using the following equation:

{displaystyle mathrm {UCL} _{1-alpha }={overline {X}}_{n}+t_{alpha ,n-1}{frac {S_{n}}{sqrt {n}}}.}

The resulting UCL will be the greatest average value that will occur for a given confidence interval and population size. In other words, {overline {X}}_{n} being the mean of the set of observations, the probability that the mean of the distribution is inferior to UCL1−α is equal to the confidence level 1 − α.

Prediction intervals[edit]

The t-distribution can be used to construct a prediction interval for an unobserved sample from a normal distribution with unknown mean and variance.

In Bayesian statistics[edit]

The Student’s t-distribution, especially in its three-parameter (location-scale) version, arises frequently in Bayesian statistics as a result of its connection with the normal distribution. Whenever the variance of a normally distributed random variable is unknown and a conjugate prior placed over it that follows an inverse gamma distribution, the resulting marginal distribution of the variable will follow a Student’s t-distribution. Equivalent constructions with the same results involve a conjugate scaled-inverse-chi-squared distribution over the variance, or a conjugate gamma distribution over the precision. If an improper prior proportional to σ−2 is placed over the variance, the t-distribution also arises. This is the case regardless of whether the mean of the normally distributed variable is known, is unknown distributed according to a conjugate normally distributed prior, or is unknown distributed according to an improper constant prior.

Related situations that also produce a t-distribution are:

  • The marginal posterior distribution of the unknown mean of a normally distributed variable, with unknown prior mean and variance following the above model.
  • The prior predictive distribution and posterior predictive distribution of a new normally distributed data point when a series of independent identically distributed normally distributed data points have been observed, with prior mean and variance as in the above model.

Robust parametric modeling[edit]

The t-distribution is often used as an alternative to the normal distribution as a model for data, which often has heavier tails than the normal distribution allows for; see e.g. Lange et al.[32] The classical approach was to identify outliers (e.g., using Grubbs’s test) and exclude or downweight them in some way. However, it is not always easy to identify outliers (especially in high dimensions), and the t-distribution is a natural choice of model for such data and provides a parametric approach to robust statistics.

A Bayesian account can be found in Gelman et al.[33] The degrees of freedom parameter controls the kurtosis of the distribution and is correlated with the scale parameter. The likelihood can have multiple local maxima and, as such, it is often necessary to fix the degrees of freedom at a fairly low value and estimate the other parameters taking this as given. Some authors[citation needed] report that values between 3 and 9 are often good choices. Venables and Ripley[citation needed] suggest that a value of 5 is often a good choice.

Student’s t-process[edit]

For practical regression and prediction needs, Student’s t-processes were introduced, that are generalisations of the Student t-distributions for functions. A Student’s t-process is constructed from the Student t-distributions like a Gaussian process is constructed from the Gaussian distributions. For a Gaussian process, all sets of values have a multidimensional Gaussian distribution. Analogously, X(t) is a Student t-process on an interval I=[a,b] if the correspondent values of the process {displaystyle X(t_{1}),...,X(t_{n})} ({displaystyle t_{i}in I}) have a joint multivariate Student t-distribution.[34] These processes are used for regression, prediction, Bayesian optimization and related problems. For multivariate regression and multi-output prediction, the multivariate Student t-processes are introduced and used.[35]

Table of selected values[edit]

The following table lists values for t-distributions with ν degrees of freedom for a range of one-sided or two-sided critical regions. The first column is ν, the percentages along the top are confidence levels, and the numbers in the body of the table are the {displaystyle t_{alpha ,n-1}} factors described in the section on confidence intervals.

The last row with infinite ν gives critical points for a normal distribution since a t-distribution with infinitely many degrees of freedom is a normal distribution. (See Related distributions above).

One-sided 75% 80% 85% 90% 95% 97.5% 99% 99.5% 99.75% 99.9% 99.95%
Two-sided 50% 60% 70% 80% 90% 95% 98% 99% 99.5% 99.8% 99.9%
1 1.000 1.376 1.963 3.078 6.314 12.706 31.821 63.657 127.321 318.309 636.619
2 0.816 1.080 1.386 1.886 2.920 4.303 6.965 9.925 14.089 22.327 31.599
3 0.765 0.978 1.250 1.638 2.353 3.182 4.541 5.841 7.453 10.215 12.924
4 0.741 0.941 1.190 1.533 2.132 2.776 3.747 4.604 5.598 7.173 8.610
5 0.727 0.920 1.156 1.476 2.015 2.571 3.365 4.032 4.773 5.893 6.869
6 0.718 0.906 1.134 1.440 1.943 2.447 3.143 3.707 4.317 5.208 5.959
7 0.711 0.896 1.119 1.415 1.895 2.365 2.998 3.499 4.029 4.785 5.408
8 0.706 0.889 1.108 1.397 1.860 2.306 2.896 3.355 3.833 4.501 5.041
9 0.703 0.883 1.100 1.383 1.833 2.262 2.821 3.250 3.690 4.297 4.781
10 0.700 0.879 1.093 1.372 1.812 2.228 2.764 3.169 3.581 4.144 4.587
11 0.697 0.876 1.088 1.363 1.796 2.201 2.718 3.106 3.497 4.025 4.437
12 0.695 0.873 1.083 1.356 1.782 2.179 2.681 3.055 3.428 3.930 4.318
13 0.694 0.870 1.079 1.350 1.771 2.160 2.650 3.012 3.372 3.852 4.221
14 0.692 0.868 1.076 1.345 1.761 2.145 2.624 2.977 3.326 3.787 4.140
15 0.691 0.866 1.074 1.341 1.753 2.131 2.602 2.947 3.286 3.733 4.073
16 0.690 0.865 1.071 1.337 1.746 2.120 2.583 2.921 3.252 3.686 4.015
17 0.689 0.863 1.069 1.333 1.740 2.110 2.567 2.898 3.222 3.646 3.965
18 0.688 0.862 1.067 1.330 1.734 2.101 2.552 2.878 3.197 3.610 3.922
19 0.688 0.861 1.066 1.328 1.729 2.093 2.539 2.861 3.174 3.579 3.883
20 0.687 0.860 1.064 1.325 1.725 2.086 2.528 2.845 3.153 3.552 3.850
21 0.686 0.859 1.063 1.323 1.721 2.080 2.518 2.831 3.135 3.527 3.819
22 0.686 0.858 1.061 1.321 1.717 2.074 2.508 2.819 3.119 3.505 3.792
23 0.685 0.858 1.060 1.319 1.714 2.069 2.500 2.807 3.104 3.485 3.767
24 0.685 0.857 1.059 1.318 1.711 2.064 2.492 2.797 3.091 3.467 3.745
25 0.684 0.856 1.058 1.316 1.708 2.060 2.485 2.787 3.078 3.450 3.725
26 0.684 0.856 1.058 1.315 1.706 2.056 2.479 2.779 3.067 3.435 3.707
27 0.684 0.855 1.057 1.314 1.703 2.052 2.473 2.771 3.057 3.421 3.690
28 0.683 0.855 1.056 1.313 1.701 2.048 2.467 2.763 3.047 3.408 3.674
29 0.683 0.854 1.055 1.311 1.699 2.045 2.462 2.756 3.038 3.396 3.659
30 0.683 0.854 1.055 1.310 1.697 2.042 2.457 2.750 3.030 3.385 3.646
40 0.681 0.851 1.050 1.303 1.684 2.021 2.423 2.704 2.971 3.307 3.551
50 0.679 0.849 1.047 1.299 1.676 2.009 2.403 2.678 2.937 3.261 3.496
60 0.679 0.848 1.045 1.296 1.671 2.000 2.390 2.660 2.915 3.232 3.460
80 0.678 0.846 1.043 1.292 1.664 1.990 2.374 2.639 2.887 3.195 3.416
100 0.677 0.845 1.042 1.290 1.660 1.984 2.364 2.626 2.871 3.174 3.390
120 0.677 0.845 1.041 1.289 1.658 1.980 2.358 2.617 2.860 3.160 3.373
0.674 0.842 1.036 1.282 1.645 1.960 2.326 2.576 2.807 3.090 3.291
One-sided 75% 80% 85% 90% 95% 97.5% 99% 99.5% 99.75% 99.9% 99.95%
Two-sided 50% 60% 70% 80% 90% 95% 98% 99% 99.5% 99.8% 99.9%

Calculating the confidence interval

Let’s say we have a sample with size 11, sample mean 10, and sample variance 2. For 90% confidence with 10 degrees of freedom, the one-sided t-value from the table is 1.372. Then with confidence interval calculated from

{displaystyle {overline {X}}_{n}pm t_{alpha ,nu }{frac {S_{n}}{sqrt {n}}},}

we determine that with 90% confidence we have a true mean lying below

{displaystyle 10+1.372{frac {sqrt {2}}{sqrt {11}}}=10.585.}

In other words, 90% of the times that an upper threshold is calculated by this method from particular samples, this upper threshold exceeds the true mean.

And with 90% confidence we have a true mean lying above

{displaystyle 10-1.372{frac {sqrt {2}}{sqrt {11}}}=9.414.}

In other words, 90% of the times that a lower threshold is calculated by this method from particular samples, this lower threshold lies below the true mean.

So that at 80% confidence (calculated from 100% − 2 × (1 − 90%) = 80%), we have a true mean lying within the interval

{displaystyle left(10-1.372{frac {sqrt {2}}{sqrt {11}}},10+1.372{frac {sqrt {2}}{sqrt {11}}}right)=(9.414,10.585).}

Saying that 80% of the times that upper and lower thresholds are calculated by this method from a given sample, the true mean is both below the upper threshold and above the lower threshold is not the same as saying that there is an 80% probability that the true mean lies between a particular pair of upper and lower thresholds that have been calculated by this method; see confidence interval and prosecutor’s fallacy.

Nowadays, statistical software, such as the R programming language, and functions available in many spreadsheet programs compute values of the t-distribution and its inverse without tables.

See also[edit]

Notes[edit]

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  23. ^ Platen, Eckhard & Sidorowicz, Renata (March 2007). «Empirical Evidence on Student-t Log Returns of Diversified World Stock Indices» (PDF). Quantitative Finance Research Center. ISSN 1441-8010. Archived from the original (PDF) on 2019-04-30. Retrieved 2022-03-22.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  24. ^ a b Bishop, C.M. (2006). Pattern Recognition and Machine Learning. New York, NY: Springer. ISBN 9780387310732.
  25. ^ Ord JK (1972). Families of Frequency Distributions. London: Griffin. ISBN 9780852641378. See Table 5.1.{{cite book}}: CS1 maint: postscript (link)
  26. ^ Ord JK (1972). «Chapter 5». Families of frequency distributions. London: Griffin. ISBN 9780852641378.
  27. ^ Lee, Se Yoon (2022). «The Use of a Log-Normal Prior for the Student t-Distribution». Axioms. 11 (9): 462. doi:10.3390/axioms11090462.
  28. ^ Fonseca, T.C.; Ferreira, M.A.; Migon, H.S. (2008). «Objective Bayesian analysis for the Student-t regression model». Biometrika. 95 (2): 325–333. doi:10.1093/biomet/asn001.
  29. ^ Fernández, C.; Steel, M.F. (1998). «On Bayesian modeling of fat tails and skewness». J. Am. Stat. Assoc.
  30. ^ Juárez, M.A.; Steel, M.F. (2010). «Model-based clustering of non-Gaussian panel data based on skew-t distributions». J. Bus. Econ. Stat. 28: 52–66. doi:10.1198/jbes.2009.07145. S2CID 10091669.
  31. ^ Lee, Se Yoon (2022). «The Use of a Log-Normal Prior for the Student t-Distribution». Axioms. 11 (9): 462. doi:10.3390/axioms11090462.
  32. ^ Lange KL, Little RJ, Taylor JM (1989). «Robust Statistical Modeling Using the t Distribution» (PDF). J. Am. Stat. Assoc. 84 (408): 881–896. doi:10.1080/01621459.1989.10478852. JSTOR 2290063.
  33. ^ Gelman AB, Carlin JB, Stern HS, et al. (2014). «Computationally efficient Markov chain simulation». Bayesian Data Analysis. Boca Raton, Florida: CRC Press. p. 293. ISBN 9781439898208.
  34. ^ Shah, Amar; Wilson, Andrew Gordon; Ghahramani, Zoubin (2014). «Student-t processes as alternatives to Gaussian processes» (PDF). JMLR. 33 (Proceedings of the 17th International Conference on Artificial Intelligence and Statistics (AISTATS) 2014, Reykjavik, Iceland): 877–885. arXiv:1402.4306.
  35. ^ Chen, Zexun; Wang, Bo; Gorban, Alexander N. (2019). «Multivariate Gaussian and Student-t process regression for multi-output prediction». Neural Computing and Applications. 32 (8): 3005–3028. arXiv:1703.04455. doi:10.1007/s00521-019-04687-8.
  36. ^ Sun, Jingchao; Kong, Maiying; Pal, Subhadip (22 June 2021). «The Modified-Half-Normal distribution: Properties and an efficient sampling scheme». Communications in Statistics — Theory and Methods: 1–23. doi:10.1080/03610926.2021.1934700. ISSN 0361-0926. S2CID 237919587.

References[edit]

  • Senn, S.; Richardson, W. (1994). «The first t-test». Statistics in Medicine. 13 (8): 785–803. doi:10.1002/sim.4780130802. PMID 8047737.
  • Hogg RV, Craig AT (1978). Introduction to Mathematical Statistics (4th ed.). New York: Macmillan. ASIN B010WFO0SA.
  • Venables, W. N.; Ripley, B. D. (2002). Modern Applied Statistics with S (Fourth ed.). Springer.
  • Gelman, Andrew; John B. Carlin; Hal S. Stern; Donald B. Rubin (2003). Bayesian Data Analysis (Second ed.). CRC/Chapman & Hall. ISBN 1-58488-388-X.

External links[edit]

  • «Student distribution», Encyclopedia of Mathematics, EMS Press, 2001 [1994]
  • Earliest Known Uses of Some of the Words of Mathematics (S) (Remarks on the history of the term «Student’s distribution»)
  • Rouaud, M. (2013), Probability, Statistics and Estimation (PDF) (short ed.) First Students on page 112.
  • Student’s t-Distribution, Archived 2021-04-10 at the Wayback Machine ck12

This article is about the mathematics of Student’s t-distribution. For its uses in statistics, see Student’s t-test.

Student’s t

Probability density function

Student t pdf.svg

Cumulative distribution function

Student t cdf.svg

Parameters nu >0 degrees of freedom (real)
Support {displaystyle xin (-infty ,infty )}
PDF textstylefrac{Gamma left(frac{nu+1}{2} right)} {sqrt{nupi},Gamma left(frac{nu}{2} right)} left(1+frac{x^2}{nu} right)^{-frac{nu+1}{2}}!
CDF

begin{matrix}
     frac{1}{2} + x Gamma left( frac{nu+1}{2} right)  times\[0.5em]
     frac{,_2F_1 left ( frac{1}{2},frac{nu+1}{2};frac{3}{2};
           -frac{x^2}{nu} right)}
     {sqrt{pinu},Gamma left(frac{nu}{2}right)}
     end{matrix}

where 2F1 is the hypergeometric function

Mean 0 for nu > 1, otherwise undefined
Median 0
Mode 0
Variance textstylefrac{nu}{nu-2} for nu > 2, ∞ for 1 < nu le 2, otherwise undefined
Skewness 0 for nu > 3, otherwise undefined
Ex. kurtosis textstylefrac{6}{nu-4} for nu > 4, ∞ for 2 < nu le 4, otherwise undefined
Entropy

{displaystyle {begin{matrix}{frac {nu +1}{2}}left[psi left({frac {1+nu }{2}}right)-psi left({frac {nu }{2}}right)right]\[0.5em]+ln {left[{sqrt {nu }}Bleft({frac {nu }{2}},{frac {1}{2}}right)right]},{scriptstyle {text{(nats)}}}end{matrix}}}

  • ψ: digamma function,
  • B: beta function
MGF undefined
CF

textstylefrac{K_{nu/2} left(sqrt{nu}|t|right)
                    cdot left(sqrt{nu}|t| right)^{nu/2}}
                    {Gamma(nu/2)2^{nu/2-1}} for nu >0

  • K_nu(x): modified Bessel function of the second kind[1]

In probability and statistics, Student’s t-distribution (or simply the t-distribution) is any member of a family of continuous probability distributions that arise when estimating the mean of a normally distributed population in situations where the sample size is small and the population’s standard deviation is unknown. It was developed by English statistician William Sealy Gosset under the pseudonym «Student».

The t-distribution plays a role in a number of widely used statistical analyses, including Student’s t-test for assessing the statistical significance of the difference between two sample means, the construction of confidence intervals for the difference between two population means, and in linear regression analysis. Student’s t-distribution also arises in the Bayesian analysis of data from a normal family.

If we take a sample of n observations from a normal distribution, then the t-distribution with nu=n-1 degrees of freedom can be defined as the distribution of the location of the sample mean relative to the true mean, divided by the sample standard deviation, after multiplying by the standardizing term {sqrt {n}}. In this way, the t-distribution can be used to construct a confidence interval for the true mean.

The t-distribution is symmetric and bell-shaped, like the normal distribution. However, the t-distribution has heavier tails, meaning that it is more prone to producing values that fall far from its mean. This makes it useful for understanding the statistical behavior of certain types of ratios of random quantities, in which variation in the denominator is amplified and may produce outlying values when the denominator of the ratio falls close to zero. The Student’s t-distribution is a special case of the generalized hyperbolic distribution.

History and etymology[edit]

Statistician William Sealy Gosset, known as «Student»

In statistics, the t-distribution was first derived as a posterior distribution in 1876 by Helmert[2][3][4] and Lüroth.[5][6][7] The t-distribution also appeared in a more general form as Pearson Type IV distribution in Karl Pearson’s 1895 paper.[8]

In the English-language literature, the distribution takes its name from William Sealy Gosset’s 1908 paper in Biometrika under the pseudonym «Student».[9] One version of the origin of the pseudonym is that Gosset’s employer preferred staff to use pen names when publishing scientific papers instead of their real name, so he used the name «Student» to hide his identity. Another version is that Guinness did not want their competitors to know that they were using the t-test to determine the quality of raw material.[10][11]

Gosset worked at the Guinness Brewery in Dublin, Ireland, and was interested in the problems of small samples – for example, the chemical properties of barley where sample sizes might be as few as 3. Gosset’s paper refers to the distribution as the «frequency distribution of standard deviations of samples drawn from a normal population». It became well known through the work of Ronald Fisher, who called the distribution «Student’s distribution» and represented the test value with the letter t.[12][13]

How Student’s distribution arises from sampling[edit]

Let {textstyle X_{1},ldots ,X_{n}} be independently and identically drawn from the distribution {mathcal {N}}(mu ,sigma ^{2}), i.e. this is a sample of size n from a normally distributed population with expected mean value mu and variance sigma ^{2}.

Let

{displaystyle {bar {X}}={frac {1}{n}}sum _{i=1}^{n}X_{i}}

be the sample mean and let

{displaystyle S^{2}={frac {1}{n-1}}sum _{i=1}^{n}(X_{i}-{bar {X}})^{2}}

be the (Bessel-corrected) sample variance. Then the random variable

{displaystyle {frac {{bar {X}}-mu }{sigma /{sqrt {n}}}}}

has a standard normal distribution (i.e. normal with expected mean 0 and variance 1), and the random variable

{displaystyle {frac {{bar {X}}-mu }{S/{sqrt {n}}}}}

i.e where S has been substituted for sigma , has a Student’s t-distribution with n-1 degrees of freedom. Since {textstyle S} has replaced {textstyle sigma ,} the only unobservable quantity in this expression is {textstyle mu ,} so this can be used to derive confidence intervals for {textstyle mu .} The numerator and the denominator in the preceding expression are statistically independent random variables despite being based on the same sample {textstyle X_{1},ldots ,X_{n}}. This can be seen by observing that {textstyle operatorname {cov} ({overline {X}},,X_{i}-{overline {X}})=0,} and recalling that {textstyle {overline {X}}} and {textstyle X_{i}-{overline {X}}} are both linear combinations of the same set of i.i.d. normally distributed random variables.

Definition[edit]

Probability density function[edit]

Student’s t-distribution has the probability density function (PDF) given by

{displaystyle f(t)={frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}left(1+{frac {t^{2}}{nu }}right)^{-(nu +1)/2},}

where nu is the number of degrees of freedom and Gamma is the gamma function. This may also be written as

{displaystyle f(t)={frac {1}{{sqrt {nu }},mathrm {B} ({frac {1}{2}},{frac {nu }{2}})}}left(1+{frac {t^{2}}{nu }}right)^{-(nu +1)/2},}

where B is the Beta function. In particular for integer valued degrees of freedom  nu we have:

For {displaystyle nu >1} even,

{displaystyle {frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}={frac {(nu -1)(nu -3)cdots 5cdot 3}{2{sqrt {nu }}(nu -2)(nu -4)cdots 4cdot 2,}}cdot }

For {displaystyle nu >1} odd,

{displaystyle {frac {Gamma ({frac {nu +1}{2}})}{{sqrt {nu pi }},Gamma ({frac {nu }{2}})}}={frac {(nu -1)(nu -3)cdots 4cdot 2}{pi {sqrt {nu }}(nu -2)(nu -4)cdots 5cdot 3,}}cdot !}

The probability density function is symmetric, and its overall shape resembles the bell shape of a normally distributed variable with mean 0 and variance 1, except that it is a bit lower and wider. As the number of degrees of freedom grows, the t-distribution approaches the normal distribution with mean 0 and variance 1. For this reason {nu } is also known as the normality parameter.[14]

The following images show the density of the t-distribution for increasing values of nu . The normal distribution is shown as a blue line for comparison. Note that the t-distribution (red line) becomes closer to the normal distribution as nu increases.

1 degree of freedom

2 degrees of freedom

3 degrees of freedom

5 degrees of freedom

10 degrees of freedom

30 degrees of freedom

Cumulative distribution function[edit]

The cumulative distribution function (CDF) can be written in terms of I, the regularized
incomplete beta function. For t > 0,[15]

{displaystyle F(t)=int _{-infty }^{t}f(u),du=1-{tfrac {1}{2}}I_{x(t)}left({tfrac {nu }{2}},{tfrac {1}{2}}right),}

where

x(t) = frac{nu}{{t^2+nu}}.

Other values would be obtained by symmetry. An alternative formula, valid for t^2 < nu, is[15]

{displaystyle int _{-infty }^{t}f(u),du={tfrac {1}{2}}+t{frac {Gamma left({tfrac {1}{2}}(nu +1)right)}{{sqrt {pi nu }},Gamma left({tfrac {nu }{2}}right)}},{}_{2}F_{1}left({tfrac {1}{2}},{tfrac {1}{2}}(nu +1);{tfrac {3}{2}};-{tfrac {t^{2}}{nu }}right),}

where 2F1 is a particular case of the hypergeometric function.

For information on its inverse cumulative distribution function, see quantile function § Student’s t-distribution.

Special cases[edit]

Certain values of nu give a simple form for Student’s t-distribution.

nu PDF CDF notes
1 {displaystyle {frac {1}{pi (1+t^{2})}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}arctan(t)} See Cauchy distribution
2 {displaystyle {frac {1}{2{sqrt {2}}left(1+{frac {t^{2}}{2}}right)^{3/2}}}} {displaystyle {frac {1}{2}}+{frac {t}{2{sqrt {2}}{sqrt {1+{frac {t^{2}}{2}}}}}}}
3 {displaystyle {frac {2}{pi {sqrt {3}}left(1+{frac {t^{2}}{3}}right)^{2}}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}{left[{frac {1}{sqrt {3}}}{frac {t}{1+{frac {t^{2}}{3}}}}+arctan left({frac {t}{sqrt {3}}}right)right]}}
4 {displaystyle {frac {3}{8left(1+{frac {t^{2}}{4}}right)^{5/2}}}} {displaystyle {frac {1}{2}}+{frac {3}{8}}{frac {t}{sqrt {1+{frac {t^{2}}{4}}}}}{left[1-{frac {1}{12}}{frac {t^{2}}{1+{frac {t^{2}}{4}}}}right]}}
5 {displaystyle {frac {8}{3pi {sqrt {5}}left(1+{frac {t^{2}}{5}}right)^{3}}}} {displaystyle {frac {1}{2}}+{frac {1}{pi }}{left[{frac {t}{{sqrt {5}}left(1+{frac {t^{2}}{5}}right)}}left(1+{frac {2}{3left(1+{frac {t^{2}}{5}}right)}}right)+arctan left({frac {t}{sqrt {5}}}right)right]}}
infty {displaystyle {frac {1}{sqrt {2pi }}}e^{-t^{2}/2}} {displaystyle {frac {1}{2}}{left[1+operatorname {erf} left({frac {t}{sqrt {2}}}right)right]}} See Normal distribution, Error function

How the t-distribution arises[edit]

Sampling distribution[edit]

Let x_{1},ldots ,x_{n} be the numbers observed in a sample from a continuously distributed population with expected value mu . The sample mean and sample variance are given by:

{displaystyle {begin{aligned}{bar {x}}&={frac {x_{1}+cdots +x_{n}}{n}},\[5pt]s^{2}&={frac {1}{n-1}}sum _{i=1}^{n}(x_{i}-{bar {x}})^{2}.end{aligned}}}

The resulting t-value is

 t = frac{bar{x} - mu}{s/sqrt{n}}.

The t-distribution with n-1 degrees of freedom is the sampling distribution of the t-value when the samples consist of independent identically distributed observations from a normally distributed population. Thus for inference purposes t is a useful «pivotal quantity» in the case when the mean and variance {displaystyle (mu ,sigma ^{2})} are unknown population parameters, in the sense that the t-value has then a probability distribution that depends on neither mu nor sigma ^{2}.

Bayesian inference[edit]

In Bayesian statistics, a (scaled, shifted) t-distribution arises as the marginal distribution of the unknown mean of a normal distribution, when the dependence on an unknown variance has been marginalized out:[16]

{displaystyle {begin{aligned}p(mu mid D,I)=&int p(mu ,sigma ^{2}mid D,I),dsigma ^{2}\=&int p(mu mid D,sigma ^{2},I),p(sigma ^{2}mid D,I),dsigma ^{2},end{aligned}}}

where D stands for the data {x_i}, and I represents any other information that may have been used to create the model. The distribution is thus the compounding of the conditional distribution of mu given the data and sigma ^{2} with the marginal distribution of sigma ^{2} given the data.

With n data points, if uninformative, or flat, the location prior {displaystyle p(mu mid sigma ^{2},I)={text{const}}} can be taken for μ, and the scale prior {displaystyle p(sigma ^{2}mid I)propto 1/sigma ^{2}} can be taken for σ2, then Bayes’ theorem gives

{displaystyle {begin{aligned}p(mu mid D,sigma ^{2},I)&sim N({bar {x}},sigma ^{2}/n),\p(sigma ^{2}mid D,I)&sim operatorname {Scale-inv-} chi ^{2}(nu ,s^{2}),end{aligned}}}

a normal distribution and a scaled inverse chi-squared distribution respectively, where nu = n - 1 and

s^{2}=sum {frac  {(x_{i}-{bar  {x}})^{2}}{n-1}}.

The marginalization integral thus becomes

{displaystyle {begin{aligned}p(mu mid D,I)&propto int _{0}^{infty }{frac {1}{sqrt {sigma ^{2}}}}exp left(-{frac {1}{2sigma ^{2}}}n(mu -{bar {x}})^{2}right)cdot sigma ^{-nu -2}exp(-nu s^{2}/2sigma ^{2}),dsigma ^{2}\&propto int _{0}^{infty }sigma ^{-nu -3}exp left(-{frac {1}{2sigma ^{2}}}left(n(mu -{bar {x}})^{2}+nu s^{2}right)right),dsigma ^{2}.end{aligned}}}

This can be evaluated by substituting {displaystyle z=A/2sigma ^{2}}, where {displaystyle A=n(mu -{bar {x}})^{2}+nu s^{2}}, giving

{displaystyle dz=-{frac {A}{2sigma ^{4}}},dsigma ^{2},}

so

{displaystyle p(mu mid D,I)propto A^{-(nu +1)/2}int _{0}^{infty }z^{(nu -1)/2}exp(-z),dz.}

But the z integral is now a standard Gamma integral, which evaluates to a constant, leaving

{displaystyle {begin{aligned}p(mu mid D,I)&propto A^{-(nu +1)/2}\&propto left(1+{frac {n(mu -{bar {x}})^{2}}{nu s^{2}}}right)^{-(nu +1)/2}.end{aligned}}}

This is a form of the t-distribution with an explicit scaling and shifting that will be explored in more detail in a further section below. It can be related to the standardized t-distribution by the substitution

{displaystyle t={frac {mu -{bar {x}}}{s/{sqrt {n}}}}.}

The derivation above has been presented for the case of uninformative priors for mu and sigma ^{2}; but it will be apparent that any priors that lead to a normal distribution being compounded with a scaled inverse chi-squared distribution will lead to a t-distribution with scaling and shifting for {displaystyle P(mu mid D,I)}, although the scaling parameter corresponding to {displaystyle {frac {s^{2}}{n}}} above will then be influenced both by the prior information and the data, rather than just by the data as above.

Characterization[edit]

As the distribution of a test statistic[edit]

Student’s t-distribution with nu degrees of freedom can be defined as the distribution of the random variable T with[15][17]

{displaystyle T={frac {Z}{sqrt {V/nu }}}=Z{sqrt {frac {nu }{V}}},}

where

  • Z is a standard normal with expected value 0 and variance 1;
  • V has a chi-squared distribution (χ2-distribution) with nu degrees of freedom;
  • Z and V are independent;

A different distribution is defined as that of the random variable defined, for a given constant μ, by

(Z+mu)sqrt{frac{nu}{V}}.

This random variable has a noncentral t-distribution with noncentrality parameter μ. This distribution is important in studies of the power of Student’s t-test.

Derivation[edit]

Suppose X1, …, Xn are independent realizations of the normally-distributed, random variable X, which has an expected value μ and variance σ2. Let

overline{X}_n = frac{1}{n}(X_1+cdots+X_n)

be the sample mean, and

{displaystyle S_{n}^{2}={frac {1}{n-1}}sum _{i=1}^{n}left(X_{i}-{overline {X}}_{n}right)^{2}}

be an unbiased estimate of the variance from the sample. It can be shown that the random variable

V = (n-1)frac{S_n^2}{sigma^2}

has a chi-squared distribution with nu = n - 1 degrees of freedom (by Cochran’s theorem).[18] It is readily shown that the quantity

{displaystyle Z=left({overline {X}}_{n}-mu right){frac {sqrt {n}}{sigma }}}

is normally distributed with mean 0 and variance 1, since the sample mean {overline {X}}_{n} is normally distributed with mean μ and variance σ2/n. Moreover, it is possible to show that these two random variables (the normally distributed one Z and the chi-squared-distributed one V) are independent. Consequently[clarification needed] the pivotal quantity

{textstyle Tequiv {frac {Z}{sqrt {V/nu }}}=left({overline {X}}_{n}-mu right){frac {sqrt {n}}{S_{n}}},}

which differs from Z in that the exact standard deviation σ is replaced by the random variable Sn, has a Student’s t-distribution as defined above. Notice that the unknown population variance σ2 does not appear in T, since it was in both the numerator and the denominator, so it canceled. Gosset intuitively obtained the probability density function stated above, with nu equal to n − 1, and Fisher proved it in 1925.[12]

The distribution of the test statistic T depends on nu , but not μ or σ; the lack of dependence on μ and σ is what makes the t-distribution important in both theory and practice.

As a maximum entropy distribution[edit]

Student’s t-distribution is the maximum entropy probability distribution for a random variate X for which {displaystyle operatorname {E} (ln(nu +X^{2}))} is fixed.[19][clarification needed][better source needed]

Properties[edit]

Moments[edit]

For nu > 1, the raw moments of the t-distribution are

{displaystyle operatorname {E} (T^{k})={begin{cases}0&k{text{ odd}},quad 0<k<nu \{frac {1}{{sqrt {pi }}Gamma left({frac {nu }{2}}right)}}left[Gamma left({frac {k+1}{2}}right)Gamma left({frac {nu -k}{2}}right)nu ^{frac {k}{2}}right]&k{text{ even}},quad 0<k<nu .\end{cases}}}

Moments of order nu or higher do not exist.[20]

The term for 0 < k < nu, k even, may be simplified using the properties of the gamma function to

{displaystyle operatorname {E} (T^{k})=nu ^{frac {k}{2}},prod _{i=1}^{k/2}{frac {2i-1}{nu -2i}}qquad k{text{ even}},quad 0<k<nu .}

For a t-distribution with nu degrees of freedom, the expected value is 0 if {displaystyle nu >1}, and its variance is frac{nu}{nu-2} if nu>2. The skewness is 0 if nu > 3 and the excess kurtosis is frac{6}{nu-4} if nu > 4.

Monte Carlo sampling[edit]

There are various approaches to constructing random samples from the Student’s t-distribution. The matter depends on whether the samples are required on a stand-alone basis, or are to be constructed by application of a quantile function to uniform samples; e.g., in the multi-dimensional applications basis of copula-dependency.[citation needed] In the case of stand-alone sampling, an extension of the Box–Muller method and its polar form is easily deployed.[21] It has the merit that it applies equally well to all real positive degrees of freedom, ν, while many other candidate methods fail if ν is close to zero.[21]

Integral of Student’s probability density function and p-value[edit]

The function A(t | ν) is the integral of Student’s probability density function, f(t) between −t and t, for t ≥ 0. It thus gives the probability that a value of t less than that calculated from observed data would occur by chance. Therefore, the function A(t | ν) can be used when testing whether the difference between the means of two sets of data is statistically significant, by calculating the corresponding value of t and the probability of its occurrence if the two sets of data were drawn from the same population. This is used in a variety of situations, particularly in t-tests. For the statistic t, with ν degrees of freedom, A(t | ν) is the probability that t would be less than the observed value if the two means were the same (provided that the smaller mean is subtracted from the larger, so that t ≥ 0). It can be easily calculated from the cumulative distribution function Fν(t) of the t-distribution:

{displaystyle A(tmid nu )=F_{nu }(t)-F_{nu }(-t)=1-I_{frac {nu }{nu +t^{2}}}left({frac {nu }{2}},{frac {1}{2}}right),}

where Ix is the regularized incomplete beta function (ab).

For statistical hypothesis testing this function is used to construct the p-value.

Generalized Student’s t-distribution[edit]

In terms of scaling parameter σ̂ or σ̂2[edit]

Student’s t distribution can be generalized to a three parameter location-scale family, introducing a location parameter {hat {mu }} and a scale parameter {hat {sigma }}, through the relation

{displaystyle X={hat {mu }}+{hat {sigma }}T}

or

{displaystyle T={frac {X-{hat {mu }}}{hat {sigma }}}}

This means that {displaystyle {frac {x-{hat {mu }}}{hat {sigma }}}} has a classic Student’s t distribution with nu degrees of freedom.

The resulting non-standardized Student’s t-distribution has a density defined by:[22]

{displaystyle p(xmid nu ,{hat {mu }},{hat {sigma }})={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}}){sqrt {pi nu }}{hat {sigma }},}}left(1+{frac {1}{nu }}left({frac {x-{hat {mu }}}{hat {sigma }}}right)^{2}right)^{-(nu +1)/2}}

Here, {hat {sigma }} does not correspond to a standard deviation: it is not the standard deviation of the scaled t distribution, which may not even exist; nor is it the standard deviation of the underlying normal distribution, which is unknown. {hat {sigma }} simply sets the overall scaling of the distribution. In the Bayesian derivation of the marginal distribution of an unknown normal mean {hat {mu }} above, {hat {sigma }} as used here corresponds to the quantity {displaystyle {s/{sqrt {n}}}}, where

{displaystyle s^{2}=sum {frac {(x_{i}-{bar {x}})^{2}}{n-1}}.,}

Equivalently, the distribution can be written in terms of {hat {sigma }}^{2}, the square of this scale parameter:

{displaystyle p(xmid nu ,{hat {mu }},{hat {sigma }}^{2})={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}}){sqrt {pi nu {hat {sigma }}^{2}}}}}left(1+{frac {1}{nu }}{frac {(x-{hat {mu }})^{2}}{{hat {sigma }}^{2}}}right)^{-(nu +1)/2}}

Other properties of this version of the distribution are:[22]

{displaystyle {begin{aligned}operatorname {E} (X)&={hat {mu }}&{text{  for }}nu >1\operatorname {var} (X)&={hat {sigma }}^{2}{frac {nu }{nu -2}}&{text{  for }}nu >2\operatorname {mode} (X)&={hat {mu }}end{aligned}}}

This distribution results from compounding a Gaussian distribution (normal distribution) with mean mu and unknown variance, with an inverse gamma distribution placed over the variance with parameters a = nu/2 and {displaystyle b=nu {hat {sigma }}^{2}/2}. In other words, the random variable X is assumed to have a Gaussian distribution with an unknown variance distributed as inverse gamma, and then the variance is marginalized out (integrated out). The reason for the usefulness of this characterization is that the inverse gamma distribution is the conjugate prior distribution of the variance of a Gaussian distribution. As a result, the non-standardized Student’s t-distribution arises naturally in many Bayesian inference problems. See below.

Equivalently, this distribution results from compounding a Gaussian distribution with a scaled-inverse-chi-squared distribution with parameters nu and {hat {sigma }}^{2}. The scaled-inverse-chi-squared distribution is exactly the same distribution as the inverse gamma distribution, but with a different parameterization, i.e. {displaystyle nu =2a,;{hat {sigma }}^{2}={frac {b}{a}}}.

This version of the t-distribution can be useful in financial modeling. For example, Platen and Sidorowicz found that among the family of generalized hyperbolic distributions, this form of the t-distribution with about 4 degrees of freedom was the best fit for the (log) return of many worldwide stock indices.[23]

In terms of inverse scaling parameter λ[edit]

An alternative parameterization in terms of an inverse scaling parameter lambda (analogous to the way precision is the reciprocal of variance), defined by the relation {displaystyle lambda ={frac {1}{{hat {sigma }}^{2}}},}. The density is then given by:[24]

{displaystyle p(xmid nu ,{hat {mu }},lambda )={frac {Gamma ({frac {nu +1}{2}})}{Gamma ({frac {nu }{2}})}}left({frac {lambda }{pi nu }}right)^{1/2}left(1+{frac {lambda (x-{hat {mu }})^{2}}{nu }}right)^{-(nu +1)/2}.}

Other properties of this version of the distribution are:[24]

{displaystyle {begin{aligned}operatorname {E} (X)&={hat {mu }}&&{text{  for }}nu >1\[5pt]operatorname {var} (X)&={frac {1}{lambda }}{frac {nu }{nu -2}}&&{text{  for }}nu >2\[5pt]operatorname {mode} (X)&={hat {mu }}end{aligned}}}

This distribution results from compounding a Gaussian distribution with mean {hat {mu }} and unknown precision (the reciprocal of the variance), with a gamma distribution placed over the precision with parameters a = nu/2 and b = nu/(2lambda). In other words, the random variable X is assumed to have a normal distribution with an unknown precision distributed as gamma, and then this is marginalized over the gamma distribution.

[edit]

  • If X has a Student’s t-distribution with degree of freedom nu then X2 has an F-distribution: {displaystyle X^{2}sim mathrm {F} left(nu _{1}=1,nu _{2}=nu right)}
  • The noncentral t-distribution generalizes the t-distribution to include a location parameter. Unlike the nonstandardized t-distributions, the noncentral distributions are not symmetric (the median is not the same as the mode).
  • The discrete Student’s t-distribution is defined by its probability mass function at r being proportional to:[25]

    {displaystyle prod _{j=1}^{k}{frac {1}{(r+j+a)^{2}+b^{2}}}quad quad r=ldots ,-1,0,1,ldots .}

    Here a, b, and k are parameters. This distribution arises from the construction of a system of discrete distributions similar to that of the Pearson distributions for continuous distributions.[26]

  • One can generate Student-t samples by taking the ratio of variables from the normal distribution and the square-root of χ2-distribution. If we use instead of the normal distribution, e.g., the Irwin–Hall distribution, we obtain over-all a symmetric 4-parameter distribution, which includes the normal, the uniform, the triangular, the Student-t and the Cauchy distribution. This is also more flexible than some other symmetric generalizations of the normal distribution.
  • t-distribution is an instance of ratio distributions.

Bayesian inference: prior distribution for the degrees of the freedom[edit]

Suppose that {displaystyle x=(x_{1},cdots ,x_{N})} represents N number of independently and identically distributed samples drawn from the Student t-distribution

{displaystyle t_{nu }(x)={frac {Gamma left({frac {nu +1}{2}}right)}{{sqrt {nu pi }}Gamma left({frac {nu }{2}}right)}}left(1+{frac {x^{2}}{nu }}right)^{-{frac {nu +1}{2}}},quad xin mathbb {R} .}

With a choice a prior for the degrees of freedom nu , denoted as {displaystyle pi (nu )}, Bayesian inference seeks to evaluate the posterior distribution

{displaystyle pi (nu |{textbf {x}})={frac {prod t_{nu }(x_{i})cdot pi (nu )}{int prod t_{nu }(x_{i})cdot pi (nu )dnu }},quad nu in mathbb {R} ^{+}.}

Mean squared error comparison between Bayes estimators based on the four priors and maximum likelihood estimator for the degrees of the freedom. Data is simulated from the student t distribution with the degrees of freedom nu _{0} varying from 0 to 25 with the sample size {displaystyle N=30} (left) and {displaystyle N=100} (right). Lower value for MSE implies better accuracy.[27]

Some popular choices of the priors are:

  • Jeffreys prior [28]

{displaystyle pi _{J}(nu )propto left({frac {nu }{nu +3}}right)^{1/2}left(psi 'left({frac {nu }{2}}right)-psi 'left({frac {nu +1}{2}}right)-{frac {2(nu +3)}{nu (nu +1)^{2}}}right)^{1/2},quad nu in mathbb {R} ^{+},}
where psi '(x) represents trigamma function.

  • Exponential prior [29]

{displaystyle pi _{E}(nu )=Ga(nu |1,0.1)=exp(nu |0.1)={frac {1}{10}}e^{-nu /10},quad nu in mathbb {R} ^{+}}

  • Gamma prior [30]

{displaystyle pi _{G}(nu )=Ga(nu |2,0.1)={frac {nu }{100}}e^{-nu /10},quad nu in mathbb {R} ^{+}}

  • Log-normal prior [31]

{displaystyle pi _{L}(nu )=logN(nu |1,1)={frac {1}{nu {sqrt {2pi }}}}exp left[-{frac {(log nu -1)^{2}}{2}}right],quad nu in mathbb {R} ^{+}}

The right panels show the result of the numerical experiments. The Bayes estimator based on the Jeffreys prior {displaystyle pi _{J}(nu )} results in relatively lower Mean Squared Error (MSE ) then the Maximum Likelihood Estimator (MLE) over the values {displaystyle nu _{0}in (0,25)}. It is important to note that no Bayes estimator dominates other estimators over the interval {displaystyle (0,25)}. In other words, each Bayes estimator has its own region where the estimator is non-inferior to others.

Uses[edit]

In frequentist statistical inference[edit]

Student’s t-distribution arises in a variety of statistical estimation problems where the goal is to estimate an unknown parameter, such as a mean value, in a setting where the data are observed with additive errors. If (as in nearly all practical statistical work) the population standard deviation of these errors is unknown and has to be estimated from the data, the t-distribution is often used to account for the extra uncertainty that results from this estimation. In most such problems, if the standard deviation of the errors were known, a normal distribution would be used instead of the t-distribution.

Confidence intervals and hypothesis tests are two statistical procedures in which the quantiles of the sampling distribution of a particular statistic (e.g. the standard score) are required. In any situation where this statistic is a linear function of the data, divided by the usual estimate of the standard deviation, the resulting quantity can be rescaled and centered to follow Student’s t-distribution. Statistical analyses involving means, weighted means, and regression coefficients all lead to statistics having this form.

Quite often, textbook problems will treat the population standard deviation as if it were known and thereby avoid the need to use the Student’s t-distribution. These problems are generally of two kinds: (1) those in which the sample size is so large that one may treat a data-based estimate of the variance as if it were certain, and (2) those that illustrate mathematical reasoning, in which the problem of estimating the standard deviation is temporarily ignored because that is not the point that the author or instructor is then explaining.

Hypothesis testing[edit]

A number of statistics can be shown to have t-distributions for samples of moderate size under null hypotheses that are of interest, so that the t-distribution forms the basis for significance tests. For example, the distribution of Spearman’s rank correlation coefficient ρ, in the null case (zero correlation) is well approximated by the t distribution for sample sizes above about 20.[citation needed]

Confidence intervals[edit]

Suppose the number A is so chosen that

Pr(-A < T < A)=0.9,

when T has a t-distribution with n − 1 degrees of freedom. By symmetry, this is the same as saying that A satisfies

Pr(T < A) = 0.95,

so A is the «95th percentile» of this probability distribution, or  A=t_{(0.05,n-1)}. Then

{displaystyle Pr left(-A<{frac {{overline {X}}_{n}-mu }{S_{n}/{sqrt {n}}}}<Aright)=0.9,}

and this is equivalent to

Prleft(overline{X}_n - A frac{S_n}{sqrt{n}} < mu < overline{X}_n + Afrac{S_n}{sqrt{n}}right) = 0.9.

Therefore, the interval whose endpoints are

overline{X}_npm Afrac{S_n}{sqrt{n}}

is a 90% confidence interval for μ. Therefore, if we find the mean of a set of observations that we can reasonably expect to have a normal distribution, we can use the t-distribution to examine whether the confidence limits on that mean include some theoretically predicted value – such as the value predicted on a null hypothesis.

It is this result that is used in the Student’s t-tests: since the difference between the means of samples from two normal distributions is itself distributed normally, the t-distribution can be used to examine whether that difference can reasonably be supposed to be zero.

If the data are normally distributed, the one-sided (1 − α)-upper confidence limit (UCL) of the mean, can be calculated using the following equation:

{displaystyle mathrm {UCL} _{1-alpha }={overline {X}}_{n}+t_{alpha ,n-1}{frac {S_{n}}{sqrt {n}}}.}

The resulting UCL will be the greatest average value that will occur for a given confidence interval and population size. In other words, {overline {X}}_{n} being the mean of the set of observations, the probability that the mean of the distribution is inferior to UCL1−α is equal to the confidence level 1 − α.

Prediction intervals[edit]

The t-distribution can be used to construct a prediction interval for an unobserved sample from a normal distribution with unknown mean and variance.

In Bayesian statistics[edit]

The Student’s t-distribution, especially in its three-parameter (location-scale) version, arises frequently in Bayesian statistics as a result of its connection with the normal distribution. Whenever the variance of a normally distributed random variable is unknown and a conjugate prior placed over it that follows an inverse gamma distribution, the resulting marginal distribution of the variable will follow a Student’s t-distribution. Equivalent constructions with the same results involve a conjugate scaled-inverse-chi-squared distribution over the variance, or a conjugate gamma distribution over the precision. If an improper prior proportional to σ−2 is placed over the variance, the t-distribution also arises. This is the case regardless of whether the mean of the normally distributed variable is known, is unknown distributed according to a conjugate normally distributed prior, or is unknown distributed according to an improper constant prior.

Related situations that also produce a t-distribution are:

  • The marginal posterior distribution of the unknown mean of a normally distributed variable, with unknown prior mean and variance following the above model.
  • The prior predictive distribution and posterior predictive distribution of a new normally distributed data point when a series of independent identically distributed normally distributed data points have been observed, with prior mean and variance as in the above model.

Robust parametric modeling[edit]

The t-distribution is often used as an alternative to the normal distribution as a model for data, which often has heavier tails than the normal distribution allows for; see e.g. Lange et al.[32] The classical approach was to identify outliers (e.g., using Grubbs’s test) and exclude or downweight them in some way. However, it is not always easy to identify outliers (especially in high dimensions), and the t-distribution is a natural choice of model for such data and provides a parametric approach to robust statistics.

A Bayesian account can be found in Gelman et al.[33] The degrees of freedom parameter controls the kurtosis of the distribution and is correlated with the scale parameter. The likelihood can have multiple local maxima and, as such, it is often necessary to fix the degrees of freedom at a fairly low value and estimate the other parameters taking this as given. Some authors[citation needed] report that values between 3 and 9 are often good choices. Venables and Ripley[citation needed] suggest that a value of 5 is often a good choice.

Student’s t-process[edit]

For practical regression and prediction needs, Student’s t-processes were introduced, that are generalisations of the Student t-distributions for functions. A Student’s t-process is constructed from the Student t-distributions like a Gaussian process is constructed from the Gaussian distributions. For a Gaussian process, all sets of values have a multidimensional Gaussian distribution. Analogously, X(t) is a Student t-process on an interval I=[a,b] if the correspondent values of the process {displaystyle X(t_{1}),...,X(t_{n})} ({displaystyle t_{i}in I}) have a joint multivariate Student t-distribution.[34] These processes are used for regression, prediction, Bayesian optimization and related problems. For multivariate regression and multi-output prediction, the multivariate Student t-processes are introduced and used.[35]

Table of selected values[edit]

The following table lists values for t-distributions with ν degrees of freedom for a range of one-sided or two-sided critical regions. The first column is ν, the percentages along the top are confidence levels, and the numbers in the body of the table are the {displaystyle t_{alpha ,n-1}} factors described in the section on confidence intervals.

The last row with infinite ν gives critical points for a normal distribution since a t-distribution with infinitely many degrees of freedom is a normal distribution. (See Related distributions above).

One-sided 75% 80% 85% 90% 95% 97.5% 99% 99.5% 99.75% 99.9% 99.95%
Two-sided 50% 60% 70% 80% 90% 95% 98% 99% 99.5% 99.8% 99.9%
1 1.000 1.376 1.963 3.078 6.314 12.706 31.821 63.657 127.321 318.309 636.619
2 0.816 1.080 1.386 1.886 2.920 4.303 6.965 9.925 14.089 22.327 31.599
3 0.765 0.978 1.250 1.638 2.353 3.182 4.541 5.841 7.453 10.215 12.924
4 0.741 0.941 1.190 1.533 2.132 2.776 3.747 4.604 5.598 7.173 8.610
5 0.727 0.920 1.156 1.476 2.015 2.571 3.365 4.032 4.773 5.893 6.869
6 0.718 0.906 1.134 1.440 1.943 2.447 3.143 3.707 4.317 5.208 5.959
7 0.711 0.896 1.119 1.415 1.895 2.365 2.998 3.499 4.029 4.785 5.408
8 0.706 0.889 1.108 1.397 1.860 2.306 2.896 3.355 3.833 4.501 5.041
9 0.703 0.883 1.100 1.383 1.833 2.262 2.821 3.250 3.690 4.297 4.781
10 0.700 0.879 1.093 1.372 1.812 2.228 2.764 3.169 3.581 4.144 4.587
11 0.697 0.876 1.088 1.363 1.796 2.201 2.718 3.106 3.497 4.025 4.437
12 0.695 0.873 1.083 1.356 1.782 2.179 2.681 3.055 3.428 3.930 4.318
13 0.694 0.870 1.079 1.350 1.771 2.160 2.650 3.012 3.372 3.852 4.221
14 0.692 0.868 1.076 1.345 1.761 2.145 2.624 2.977 3.326 3.787 4.140
15 0.691 0.866 1.074 1.341 1.753 2.131 2.602 2.947 3.286 3.733 4.073
16 0.690 0.865 1.071 1.337 1.746 2.120 2.583 2.921 3.252 3.686 4.015
17 0.689 0.863 1.069 1.333 1.740 2.110 2.567 2.898 3.222 3.646 3.965
18 0.688 0.862 1.067 1.330 1.734 2.101 2.552 2.878 3.197 3.610 3.922
19 0.688 0.861 1.066 1.328 1.729 2.093 2.539 2.861 3.174 3.579 3.883
20 0.687 0.860 1.064 1.325 1.725 2.086 2.528 2.845 3.153 3.552 3.850
21 0.686 0.859 1.063 1.323 1.721 2.080 2.518 2.831 3.135 3.527 3.819
22 0.686 0.858 1.061 1.321 1.717 2.074 2.508 2.819 3.119 3.505 3.792
23 0.685 0.858 1.060 1.319 1.714 2.069 2.500 2.807 3.104 3.485 3.767
24 0.685 0.857 1.059 1.318 1.711 2.064 2.492 2.797 3.091 3.467 3.745
25 0.684 0.856 1.058 1.316 1.708 2.060 2.485 2.787 3.078 3.450 3.725
26 0.684 0.856 1.058 1.315 1.706 2.056 2.479 2.779 3.067 3.435 3.707
27 0.684 0.855 1.057 1.314 1.703 2.052 2.473 2.771 3.057 3.421 3.690
28 0.683 0.855 1.056 1.313 1.701 2.048 2.467 2.763 3.047 3.408 3.674
29 0.683 0.854 1.055 1.311 1.699 2.045 2.462 2.756 3.038 3.396 3.659
30 0.683 0.854 1.055 1.310 1.697 2.042 2.457 2.750 3.030 3.385 3.646
40 0.681 0.851 1.050 1.303 1.684 2.021 2.423 2.704 2.971 3.307 3.551
50 0.679 0.849 1.047 1.299 1.676 2.009 2.403 2.678 2.937 3.261 3.496
60 0.679 0.848 1.045 1.296 1.671 2.000 2.390 2.660 2.915 3.232 3.460
80 0.678 0.846 1.043 1.292 1.664 1.990 2.374 2.639 2.887 3.195 3.416
100 0.677 0.845 1.042 1.290 1.660 1.984 2.364 2.626 2.871 3.174 3.390
120 0.677 0.845 1.041 1.289 1.658 1.980 2.358 2.617 2.860 3.160 3.373
0.674 0.842 1.036 1.282 1.645 1.960 2.326 2.576 2.807 3.090 3.291
One-sided 75% 80% 85% 90% 95% 97.5% 99% 99.5% 99.75% 99.9% 99.95%
Two-sided 50% 60% 70% 80% 90% 95% 98% 99% 99.5% 99.8% 99.9%

Calculating the confidence interval

Let’s say we have a sample with size 11, sample mean 10, and sample variance 2. For 90% confidence with 10 degrees of freedom, the one-sided t-value from the table is 1.372. Then with confidence interval calculated from

{displaystyle {overline {X}}_{n}pm t_{alpha ,nu }{frac {S_{n}}{sqrt {n}}},}

we determine that with 90% confidence we have a true mean lying below

{displaystyle 10+1.372{frac {sqrt {2}}{sqrt {11}}}=10.585.}

In other words, 90% of the times that an upper threshold is calculated by this method from particular samples, this upper threshold exceeds the true mean.

And with 90% confidence we have a true mean lying above

{displaystyle 10-1.372{frac {sqrt {2}}{sqrt {11}}}=9.414.}

In other words, 90% of the times that a lower threshold is calculated by this method from particular samples, this lower threshold lies below the true mean.

So that at 80% confidence (calculated from 100% − 2 × (1 − 90%) = 80%), we have a true mean lying within the interval

{displaystyle left(10-1.372{frac {sqrt {2}}{sqrt {11}}},10+1.372{frac {sqrt {2}}{sqrt {11}}}right)=(9.414,10.585).}

Saying that 80% of the times that upper and lower thresholds are calculated by this method from a given sample, the true mean is both below the upper threshold and above the lower threshold is not the same as saying that there is an 80% probability that the true mean lies between a particular pair of upper and lower thresholds that have been calculated by this method; see confidence interval and prosecutor’s fallacy.

Nowadays, statistical software, such as the R programming language, and functions available in many spreadsheet programs compute values of the t-distribution and its inverse without tables.

See also[edit]

Notes[edit]

  1. ^ Hurst, Simon. «The Characteristic Function of the Student t Distribution». Financial Mathematics Research Report No. FMRR006-95, Statistics Research Report No. SRR044-95. Archived from the original on February 18, 2010.
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  5. ^ Lüroth J (1876). «Vergleichung von zwei Werten des wahrscheinlichen Fehlers». Astron. Nachr. 87 (14): 209–20. Bibcode:1876AN…..87..209L. doi:10.1002/asna.18760871402.
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  15. ^ a b c Johnson NL, Kotz S, Balakrishnan N (1995). «Chapter 28». Continuous Univariate Distributions. Vol. 2 (2nd ed.). Wiley. ISBN 9780471584940.
  16. ^ Gelman AB, Carlin JS, Rubin DB, et al. (1997). Bayesian Data Analysis (2nd ed.). Boca Raton: Chapman & Hall. p. 68. ISBN 9780412039911.
  17. ^ Hogg RV, Craig AT (1978). Introduction to Mathematical Statistics (4th ed.). New York: Macmillan. ASIN B010WFO0SA. Sections 4.4 and 4.8{{cite book}}: CS1 maint: postscript (link)
  18. ^ Cochran WG (1934). «The distribution of quadratic forms in a normal system, with applications to the analysis of covariance». Math. Proc. Camb. Philos. Soc. 30 (2): 178–191. Bibcode:1934PCPS…30..178C. doi:10.1017/S0305004100016595. S2CID 122547084.
  19. ^ Park SY, Bera AK (2009). «Maximum entropy autoregressive conditional heteroskedasticity model». J. Econom. 150 (2): 219–230. doi:10.1016/j.jeconom.2008.12.014.
  20. ^ Casella G, Berger RL (1990). Statistical Inference. Duxbury Resource Center. p. 56. ISBN 9780534119584.
  21. ^ a b Bailey RW (1994). «Polar Generation of Random Variates with the t-Distribution». Math. Comput. 62 (206): 779–781. Bibcode:1994MaCom..62..779B. doi:10.2307/2153537. JSTOR 2153537.
  22. ^ a b Jackman, S. (2009). Bayesian Analysis for the Social Sciences. Wiley Series in Probability and Statistics. Wiley. p. 507. doi:10.1002/9780470686621. ISBN 9780470011546.
  23. ^ Platen, Eckhard & Sidorowicz, Renata (March 2007). «Empirical Evidence on Student-t Log Returns of Diversified World Stock Indices» (PDF). Quantitative Finance Research Center. ISSN 1441-8010. Archived from the original (PDF) on 2019-04-30. Retrieved 2022-03-22.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  24. ^ a b Bishop, C.M. (2006). Pattern Recognition and Machine Learning. New York, NY: Springer. ISBN 9780387310732.
  25. ^ Ord JK (1972). Families of Frequency Distributions. London: Griffin. ISBN 9780852641378. See Table 5.1.{{cite book}}: CS1 maint: postscript (link)
  26. ^ Ord JK (1972). «Chapter 5». Families of frequency distributions. London: Griffin. ISBN 9780852641378.
  27. ^ Lee, Se Yoon (2022). «The Use of a Log-Normal Prior for the Student t-Distribution». Axioms. 11 (9): 462. doi:10.3390/axioms11090462.
  28. ^ Fonseca, T.C.; Ferreira, M.A.; Migon, H.S. (2008). «Objective Bayesian analysis for the Student-t regression model». Biometrika. 95 (2): 325–333. doi:10.1093/biomet/asn001.
  29. ^ Fernández, C.; Steel, M.F. (1998). «On Bayesian modeling of fat tails and skewness». J. Am. Stat. Assoc.
  30. ^ Juárez, M.A.; Steel, M.F. (2010). «Model-based clustering of non-Gaussian panel data based on skew-t distributions». J. Bus. Econ. Stat. 28: 52–66. doi:10.1198/jbes.2009.07145. S2CID 10091669.
  31. ^ Lee, Se Yoon (2022). «The Use of a Log-Normal Prior for the Student t-Distribution». Axioms. 11 (9): 462. doi:10.3390/axioms11090462.
  32. ^ Lange KL, Little RJ, Taylor JM (1989). «Robust Statistical Modeling Using the t Distribution» (PDF). J. Am. Stat. Assoc. 84 (408): 881–896. doi:10.1080/01621459.1989.10478852. JSTOR 2290063.
  33. ^ Gelman AB, Carlin JB, Stern HS, et al. (2014). «Computationally efficient Markov chain simulation». Bayesian Data Analysis. Boca Raton, Florida: CRC Press. p. 293. ISBN 9781439898208.
  34. ^ Shah, Amar; Wilson, Andrew Gordon; Ghahramani, Zoubin (2014). «Student-t processes as alternatives to Gaussian processes» (PDF). JMLR. 33 (Proceedings of the 17th International Conference on Artificial Intelligence and Statistics (AISTATS) 2014, Reykjavik, Iceland): 877–885. arXiv:1402.4306.
  35. ^ Chen, Zexun; Wang, Bo; Gorban, Alexander N. (2019). «Multivariate Gaussian and Student-t process regression for multi-output prediction». Neural Computing and Applications. 32 (8): 3005–3028. arXiv:1703.04455. doi:10.1007/s00521-019-04687-8.
  36. ^ Sun, Jingchao; Kong, Maiying; Pal, Subhadip (22 June 2021). «The Modified-Half-Normal distribution: Properties and an efficient sampling scheme». Communications in Statistics — Theory and Methods: 1–23. doi:10.1080/03610926.2021.1934700. ISSN 0361-0926. S2CID 237919587.

References[edit]

  • Senn, S.; Richardson, W. (1994). «The first t-test». Statistics in Medicine. 13 (8): 785–803. doi:10.1002/sim.4780130802. PMID 8047737.
  • Hogg RV, Craig AT (1978). Introduction to Mathematical Statistics (4th ed.). New York: Macmillan. ASIN B010WFO0SA.
  • Venables, W. N.; Ripley, B. D. (2002). Modern Applied Statistics with S (Fourth ed.). Springer.
  • Gelman, Andrew; John B. Carlin; Hal S. Stern; Donald B. Rubin (2003). Bayesian Data Analysis (Second ed.). CRC/Chapman & Hall. ISBN 1-58488-388-X.

External links[edit]

  • «Student distribution», Encyclopedia of Mathematics, EMS Press, 2001 [1994]
  • Earliest Known Uses of Some of the Words of Mathematics (S) (Remarks on the history of the term «Student’s distribution»)
  • Rouaud, M. (2013), Probability, Statistics and Estimation (PDF) (short ed.) First Students on page 112.
  • Student’s t-Distribution, Archived 2021-04-10 at the Wayback Machine ck12

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