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Statistics & Probability Statistical Inference Syllabus
The Statistical Inference syllabus for Statistics & Probability in full: 7 chapters and 27 topics, every one listed below, plus 50 Statistical Inference flashcards with answers.
Statistical Inference syllabus: all 7 chapters
Expand any chapter to see its topics and sub-topics.
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Point and Interval Estimation
4 topics- Point Estimators and Their Properties
- Confidence Intervals for a Mean
- Confidence Intervals for a Proportion
- Margin of Error and Sample Size
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Hypothesis Testing Fundamentals
5 topics- Null and Alternative Hypotheses
- Type I and Type II Errors
- Significance Level and P-Values
- Statistical Power
- One-Tailed vs Two-Tailed Tests
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Tests for Means
3 topics- One-Sample z-Test and t-Test
- Two-Sample t-Tests
- Assumptions and Diagnostics
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Tests for Proportions and Variance
4 topics- One and Two Proportion z-Tests
- Chi-Square Goodness-of-Fit
- Chi-Square Test of Independence
- Tests for Variance
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Analysis of Variance (ANOVA)
4 topics- One-Way ANOVA
- Two-Way ANOVA
- Post-Hoc Tests
- ANOVA Assumptions
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Nonparametric Methods
4 topics- Mann-Whitney U Test
- Wilcoxon Signed-Rank Test
- Kruskal-Wallis Test
- Spearman Rank Correlation
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Resampling Methods
3 topics- Bootstrap
- Permutation Tests
- Cross-Validation
Statistics & Probability Statistical Inference flashcards — 50 questions with answers
What is a point estimator, and how does it differ from a point estimate?
A point estimator is a statistic (a rule/function of the sample data) used to infer an unknown population parameter, e.g. $\bar{X}$ for $\mu$. A point estimate is the single numerical value the estimator takes for a specific sample. The estimator is the random variable; the estimate is one realized number.
Define an unbiased estimator.
An estimator $\hat{\theta}$ is unbiased for $\theta$ if its expected value equals the parameter: $E(\hat{\theta}) = \theta$. The bias is $\text{Bias}(\hat{\theta}) = E(\hat{\theta}) - \theta$, so unbiasedness means zero bias for all sample sizes.
Why is the sample variance defined with $n-1$ in the denominator rather than $n$?
Dividing by $n-1$ makes the sample variance unbiased for the population variance: $E\left(\frac{1}{n-1}\sum (X_i-\bar{X})^2\right) = \sigma^{2}$. Using $n$ underestimates $\sigma^{2}$ because deviations are taken about $\bar{X}$ (which minimizes them), costing one degree of freedom.
What does it mean for an estimator to be consistent?
An estimator $\hat{\theta}_n$ is consistent if it converges in probability to the parameter as the sample grows: for every $\varepsilon>0$, $P(|\hat{\theta}_n - \theta| > \varepsilon) \to 0$ as $n \to \infty$. Roughly, the estimate gets arbitrarily close to $\theta$ with more data.
How is the efficiency of an unbiased estimator judged, and what is the MSE decomposition?
Among unbiased estimators, the more efficient one has the smaller variance. Overall accuracy is measured by mean squared error: $$\text{MSE}(\hat{\theta}) = \text{Var}(\hat{\theta}) + \left[\text{Bias}(\hat{\theta})\right]^{2}.$$ A minimum-variance unbiased estimator is the most efficient unbiased choice.
What is the confidence interval for a population mean $\mu$ when the population standard deviation $\sigma$ is known?
$$\bar{x} \pm z_{\alpha/2}\,\frac{\sigma}{\sqrt{n}}$$ where $z_{\alpha/2}$ is the standard-normal critical value (e.g. $1.96$ for 95%). Valid when the population is normal or $n$ is large (CLT).
What is the confidence interval for a mean $\mu$ when $\sigma$ is unknown?
$$\bar{x} \pm t_{\alpha/2,\,n-1}\,\frac{s}{\sqrt{n}}$$ using the sample standard deviation $s$ and the $t$-distribution with $n-1$ degrees of freedom. The $t$ critical value exceeds the corresponding $z$ value to account for extra uncertainty in estimating $\sigma$.
What is the correct interpretation of a 95% confidence interval?
If we repeatedly drew samples and built an interval each time by the same method, about 95% of those intervals would contain the true parameter. It does NOT mean there is a 95% probability that this particular interval contains $\mu$ — the parameter is fixed, and a given interval either contains it or not.
State the large-sample (Wald) confidence interval for a population proportion $p$.
$$\hat{p} \pm z_{\alpha/2}\sqrt{\frac{\hat{p}(1-\hat{p})}{n}}$$ where $\hat{p} = x/n$ is the sample proportion and $\sqrt{\hat{p}(1-\hat{p})/n}$ is the standard error of $\hat{p}$.
What conditions justify the normal-approximation confidence interval for a proportion?
Independent observations (e.g. random sample, and $n \leq 10\%$ of the population) and a large enough sample so the sampling distribution is approximately normal: typically $n\hat{p} \geq 10$ and $n(1-\hat{p}) \geq 10$ (some texts use $\geq 5$).
Define the margin of error in a confidence interval.
The margin of error is the half-width of the interval: $E = (\text{critical value}) \times (\text{standard error})$. For a mean with known $\sigma$, $E = z_{\alpha/2}\,\frac{\sigma}{\sqrt{n}}$; for a proportion, $E = z_{\alpha/2}\sqrt{\frac{\hat{p}(1-\hat{p})}{n}}$.
How does the required sample size for estimating a mean depend on the desired margin of error $E$?
Solving $E = z_{\alpha/2}\,\frac{\sigma}{\sqrt{n}}$ gives $$n = \left(\frac{z_{\alpha/2}\,\sigma}{E}\right)^{2}.$$ Halving $E$ quadruples $n$, and $n$ grows with the square of the confidence critical value; always round up.
What sample size is needed to estimate a proportion within margin $E$, and what value maximizes it?
$$n = \frac{z_{\alpha/2}^{2}\,\hat{p}(1-\hat{p})}{E^{2}}.$$ With no prior estimate, use the conservative $\hat{p} = 0.5$, which maximizes $\hat{p}(1-\hat{p}) = 0.25$ and thus the required $n$. Round up.
How do the null hypothesis $H_0$ and alternative hypothesis $H_a$ differ?
$H_0$ is the default claim of no effect/no difference, always stated with equality (e.g. $\mu = \mu_0$). $H_a$ is the researcher's claim of an effect, stated with $\neq$, $<$, or $>$. Testing seeks evidence to reject $H_0$ in favor of $H_a$; we never 'prove' $H_0$.
What is a Type I error and how is its probability denoted?
A Type I error is rejecting a true null hypothesis (a 'false positive'). Its probability equals the significance level: $P(\text{Type I}) = \alpha$.
What is a Type II error and how is its probability denoted?
A Type II error is failing to reject a false null hypothesis (a 'false negative'). Its probability is denoted $\beta$, and $1-\beta$ is the power of the test.
How are the Type I and Type II error rates related as you change the decision threshold?
For a fixed sample size, lowering $\alpha$ (stricter rejection rule) raises $\beta$, and vice versa — there is a trade-off. Both can be reduced simultaneously only by increasing the sample size $n$.
What is the significance level $\alpha$ of a hypothesis test?
$\alpha$ is the pre-chosen threshold for the maximum tolerable probability of a Type I error — the probability of rejecting $H_0$ when it is true. Common choices are $0.05$, $0.01$, and $0.10$; it defines the size of the rejection region.
Define the p-value of a hypothesis test.
The p-value is the probability, assuming $H_0$ is true, of obtaining a test statistic at least as extreme as the one observed (in the direction of $H_a$). A small p-value means the observed data would be unlikely under $H_0$.
State the p-value decision rule for a significance level $\alpha$.
If $p \leq \alpha$, reject $H_0$ (result is statistically significant). If $p > \alpha$, fail to reject $H_0$. Note: a p-value is NOT the probability that $H_0$ is true, nor the probability the result occurred by chance.
Show the other 30 Statistical Inference flashcards
Define the statistical power of a test.
Power is the probability of correctly rejecting a false null hypothesis: $$\text{Power} = 1 - \beta = P(\text{reject } H_0 \mid H_0 \text{ false}).$$ It measures the test's ability to detect a true effect.
List four factors that increase the power of a statistical test.
(1) Larger sample size $n$; (2) larger true effect size (bigger departure from $H_0$); (3) larger significance level $\alpha$ (less strict); (4) smaller variability $\sigma$. Using a one-tailed test (when appropriate) also raises power.
Compare one-tailed and two-tailed tests, including how the rejection region is placed.
A two-tailed test ($H_a: \theta \neq \theta_0$) splits $\alpha$ into both tails ($\alpha/2$ each) and detects deviations in either direction. A one-tailed test ($H_a: \theta > \theta_0$ or $<\theta_0$) puts all $\alpha$ in one tail, giving more power to detect an effect in that specified direction only.
Write the test statistic for a one-sample z-test for a mean.
$$z = \frac{\bar{x} - \mu_0}{\sigma/\sqrt{n}}$$ used when $\sigma$ is known (or $n$ is large) and the sampling distribution of $\bar{x}$ is approximately normal.
Write the test statistic and degrees of freedom for a one-sample t-test for a mean.
$$t = \frac{\bar{x} - \mu_0}{s/\sqrt{n}}, \qquad df = n-1$$ used when $\sigma$ is unknown and estimated by the sample standard deviation $s$.
Give the pooled two-sample t-test statistic used when equal population variances are assumed.
$$t = \frac{(\bar{x}_1-\bar{x}_2)-(\mu_1-\mu_2)}{s_p\sqrt{\frac{1}{n_1}+\frac{1}{n_2}}}, \quad s_p^{2}=\frac{(n_1-1)s_1^{2}+(n_2-1)s_2^{2}}{n_1+n_2-2}$$ with $df = n_1+n_2-2$.
What is Welch's two-sample t-test and when is it preferred?
Welch's test compares two means without assuming equal variances: $$t = \frac{\bar{x}_1-\bar{x}_2}{\sqrt{\frac{s_1^{2}}{n_1}+\frac{s_2^{2}}{n_2}}}$$ with df from the Welch–Satterthwaite approximation. It is preferred (and is the default) whenever the two group variances or sample sizes differ.
When is a paired (dependent-samples) t-test used, and what is its test statistic?
It is used when observations are naturally paired (e.g. before/after on the same subjects). You analyze the differences $d_i$: $$t = \frac{\bar{d} - \mu_{d,0}}{s_d/\sqrt{n}}, \qquad df = n-1,$$ where $n$ is the number of pairs.
State the key assumptions of one-sample and two-sample t-tests.
(1) Random/independent sampling; (2) the data (or, for two samples, each group; for paired, the differences) come from an approximately normal population, with robustness improving as $n$ grows via the CLT; (3) for the pooled two-sample test, equal population variances (homogeneity).
What diagnostics check the normality and variance assumptions before a t-test or ANOVA?
Normality: histograms, normal Q–Q plots (points near the line), and tests like Shapiro–Wilk. Equal variance (homoscedasticity): compare group spreads/boxplots or use Levene's or the F-test. Also check independence and screen for outliers that distort means and variances.
Write the one-proportion z-test statistic.
$$z = \frac{\hat{p} - p_0}{\sqrt{\frac{p_0(1-p_0)}{n}}}$$ Note the standard error uses the hypothesized $p_0$ (not $\hat{p}$), since it is computed assuming $H_0$ is true.
Write the two-proportion z-test statistic and its pooled proportion.
$$z = \frac{\hat{p}_1-\hat{p}_2}{\sqrt{\hat{p}(1-\hat{p})\left(\frac{1}{n_1}+\frac{1}{n_2}\right)}}, \quad \hat{p}=\frac{x_1+x_2}{n_1+n_2}$$ The pooled $\hat{p}$ is used because $H_0: p_1=p_2$ assumes a common proportion.
Give the chi-square goodness-of-fit test statistic and its degrees of freedom.
$$\chi^{2} = \sum \frac{(O_i - E_i)^{2}}{E_i}, \qquad df = k - 1$$ where $O_i$ and $E_i$ are observed and expected counts across $k$ categories. It tests whether a categorical variable follows a specified distribution.
How are expected counts computed in a chi-square goodness-of-fit test?
For each category, $E_i = n\,p_i$, where $n$ is the total sample size and $p_i$ is the proportion specified by $H_0$ for that category. The test requires all expected counts to be sufficiently large (commonly $E_i \geq 5$).
Give the chi-square test-of-independence statistic and its degrees of freedom.
$$\chi^{2} = \sum \frac{(O - E)^{2}}{E}, \qquad df = (r-1)(c-1)$$ for an $r \times c$ contingency table. It tests whether two categorical variables are associated (dependent).
How is each expected cell count computed in a chi-square test of independence?
$$E_{ij} = \frac{(\text{row } i \text{ total})\times(\text{column } j \text{ total})}{\text{grand total}}.$$ This is the count expected if the row and column variables were independent.
What are the main assumptions/conditions for chi-square tests on counts?
(1) Data are counts (frequencies) from a random sample; (2) observations are independent; (3) categories are mutually exclusive and exhaustive; (4) expected counts are large enough — a common rule is all $E_i \geq 5$ (or at least 80% of cells $\geq 5$).
State the chi-square test statistic and df for a test about a single population variance.
$$\chi^{2} = \frac{(n-1)s^{2}}{\sigma_0^{2}}, \qquad df = n-1$$ used to test $H_0: \sigma^{2} = \sigma_0^{2}$. It requires the population to be (approximately) normal, an assumption to which this test is quite sensitive.
What test compares two population variances, and what is its statistic?
The F-test: $$F = \frac{s_1^{2}}{s_2^{2}}$$ with $df_1 = n_1-1$ and $df_2 = n_2-1$. Under $H_0: \sigma_1^{2}=\sigma_2^{2}$ it follows an F-distribution; it assumes both populations are normal.
State the hypotheses of a one-way ANOVA.
$H_0: \mu_1 = \mu_2 = \cdots = \mu_k$ (all group means equal) versus $H_a:$ at least one mean differs. It compares $k$ group means simultaneously using one categorical factor.
Give the one-way ANOVA F statistic in terms of mean squares.
$$F = \frac{\text{MSB}}{\text{MSW}} = \frac{SSB/(k-1)}{SSW/(N-k)}$$ where MSB is mean square between groups (signal) and MSW is mean square within groups (noise). Large $F$ suggests between-group differences exceed within-group variation.
State the sum-of-squares partition in one-way ANOVA.
Total variation splits into between-group and within-group parts: $$SST = SSB + SSW,$$ i.e. $\sum(x_{ij}-\bar{x})^{2} = \sum n_j(\bar{x}_j-\bar{x})^{2} + \sum(x_{ij}-\bar{x}_j)^{2}.$
What are the degrees of freedom for the F-test in a one-way ANOVA with $k$ groups and $N$ total observations?
Between groups (numerator): $df_1 = k-1$. Within groups / error (denominator): $df_2 = N-k$. Total: $df_{\text{total}} = N-1 = (k-1)+(N-k)$.
List the assumptions of ANOVA.
(1) Independent random samples/observations; (2) each group's population is approximately normal; (3) homogeneity of variance — all groups share a common variance $\sigma^{2}$. ANOVA is fairly robust to mild normality violations, especially with balanced designs.
What is the purpose of a two-way ANOVA and what factors does it examine?
Two-way ANOVA tests the effect of two categorical factors on a continuous response simultaneously. It examines two main effects (one per factor) and their interaction effect, partitioning variance into these components plus error.
What does an interaction effect mean in a two-way ANOVA?
An interaction means the effect of one factor on the response depends on the level of the other factor. Graphically, the lines in an interaction (means) plot are non-parallel. If interaction is significant, main effects must be interpreted cautiously.
What is the standard error of the sample mean, and why does it matter?
$$SE(\bar{x}) = \frac{\sigma}{\sqrt{n}} \quad (\text{estimated by } s/\sqrt{n}).$$ It quantifies the sampling variability of $\bar{x}$ and shrinks as $\sqrt{n}$ grows, forming the denominator of z/t statistics and the basis of margins of error.
Why is the Central Limit Theorem important for inference about a mean?
The CLT states that for large $n$, the sampling distribution of $\bar{x}$ is approximately normal with mean $\mu$ and standard deviation $\sigma/\sqrt{n}$, regardless of the population's shape. This justifies using z/t procedures and normal-based confidence intervals even for non-normal populations.
Why can't a two-tailed hypothesis test 'accept' the null hypothesis?
Failing to reject $H_0$ only means the data provide insufficient evidence against it — absence of evidence is not evidence of absence. The null may still be false with the test simply lacking power, so we say 'fail to reject,' never 'accept.'
After a significant one-way ANOVA, what is needed to identify which means differ, and why?
A post-hoc multiple-comparison procedure (e.g. Tukey's HSD, Bonferroni, Scheffé). ANOVA's F-test only signals that at least one mean differs, not which; post-hoc tests compare pairs while controlling the inflated family-wise Type I error from many comparisons.
Statistics & Probability Statistical Inference FAQ
What is in the Statistics & Probability Statistical Inference syllabus?
Statistics & Probability Statistical Inference is split into 7 chapters: Point and Interval Estimation, Hypothesis Testing Fundamentals, Tests for Means, Tests for Proportions and Variance, Analysis of Variance (ANOVA), Nonparametric Methods and Resampling Methods. Together they contain 27 topics.
How many chapters are in Statistics & Probability Statistical Inference?
7 chapters, containing 27 topics. The largest chapter is Hypothesis Testing Fundamentals, with 5 topics.
Are there flashcards for Statistics & Probability Statistical Inference?
Yes — a 50-card Statistical Inference deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.