Basic Prerequisites: Statistics & Inference (t-test, CLT, Type I/II error) and 03 · Abnormal Returns & CAR.
1. Intuition & Practical Objective
An event study is not finished when it computes a CAR - it must decide whether that CAR is statistically distinguishable from zero or could be a draw from noise. This page covers the test statistic, its assumptions, its power (ability to detect real abnormal performance), and the two inferential traps (cross-correlation and event-period variance) that break it.
The test statistic is the CAR divided by an estimate of its standard deviation (Kothari–Warner eq. 5):
where and is the variance of the one-period mean abnormal return (estimated from the estimation-window time series). Under the null of zero abnormal performance, is approximately unit normal. Two design facts matter more than the formula (Kothari–Warner §3.6):
- Short horizons are well-specified and powerful; long horizons are poorly specified with low power.
- Power depends on sample size, firm volatility, and whether the abnormal performance is concentrated in a known window. A 10% abnormal return on a known single day is detected with 100% power by just 6 stocks; spread over 6 months, 200 stocks detect it only 65% of the time (Kothari–Warner §3.6.4).
2. Mathematical Ground Truth & Derivations
The test statistic (Kothari–Warner eq. 5–6). For the CAR over window with periods:
is estimated from the time series of portfolio (mean) abnormal returns in the estimation window, so it automatically captures cross-sectional dependence across firms (Brown–Warner 1985 eq. 5 uses the same “portfolio excess return” approach).
Cross-correlation inflation (Kothari–Warner eq. 10). If the sample firms’ abnormal returns are positively correlated (event-date clustering, common industry), the true SE is larger than the independence-based one by:
where is the average pairwise correlation. At and , this is - the t-stat is overstated by ~73%. This is why long-horizon tests that ignore cross-dependence “reject the null far more often than the size of the test” (Kothari–Warner §4.4.2).
Power. Power = . For a cross-sectional mean abnormal return with SE , the power of a two-sided 5% test is approximately
Power rises with (sample size) and falls with (firm volatility). Crucially, power is high only if abnormal performance is concentrated in a precisely-known window (Table 2, Kothari–Warner §3.6.1).
3. Computational Implementation - the test, its traps, and power
Stdlib only. Three experiments: (a) the cross-correlation inflation factor; (b) the event-period-variance over-rejection trap; (c) power vs sample size.
Reading the output. (a) The factor reproduces Kothari–Warner’s headline number exactly: - a ~73% overstatement of significance from even mild cross-dependence. (b) When the event-day variance doubles (Beaver 1968: volatility rises around earnings announcements), a naive 5% test rejects the null 16.5% of the time - a badly misspecified test. (c) Detecting a 1% abnormal return with average-volatility firms needs a large sample: ~200 firms for 76% power. For a concentrated signal, power is dramatically better - Kothari–Warner report 6 firms detect a 10% one-day abnormal return with 100% power.
4. Failure Modes & First-Principles Breakdowns
- The joint-test problem (the deepest one). Every event-study test is a joint test of “abnormal returns are zero” and “the expected-return model is correct.” A rejection can mean either. Short windows make the model component negligible (~0.05% daily expected return); long windows are dominated by it (Kothari–Warner §3.5.1).
- Event-period variance increase. Volatility rises around events, so estimation-window SEs understate event-period variability and the test over-rejects (Experiment b: 5% → 16.5%). Remedies: use event-period cross-sectional variance, nonparametric rank tests (Corrado 1989).
- Cross-correlation / clustering. Ignoring event-date clustering inflates the t-stat by up to ~1.7× (Experiment a). The portfolio-time-series SE handles cross-sectional dependence; calendar-time portfolios handle it for long horizons.
- Low power at long horizons. Even huge cumulative abnormal performance (25% over 5 years, 200 firms) is detected under 50% of the time (Jegadeesh–Karceski 2004). Long-window “no result” is often just low power.
- Non-normality / skewness of BHARs. Long-horizon BHARs are right-skewed; the t-distribution is then asymmetric with mean below zero under the null (Brav 2000). Use skewness-adjusted or bootstrap t-stats.
5. References
- Kothari & Warner (2007), Econometrics of Event Studies, Handbook of Corporate Finance
- Brown & Warner (1985), Using Daily Stock Returns, JFE 14(1)
- Brown & Warner (1980), Measuring Security Price Performance, JFE 8(3)
- Corrado (1989), A Nonparametric Test for Abnormal Security-Price Performance in Event Studies, JFE 23(2)
- Jegadeesh & Karceski (2004), Long-Term Performance Evaluation, Working Paper
6. Connected Graph Bridges
- Back: 03 · Abnormal Returns & CAR · Index Hub
- Forward: 05 · Failure Modes · 06 · Advanced Extensions
- Base: Statistics & Inference (t-tests, power, CLT) · Bayesian Statistics
- Practice: Backtesting Hygiene (multiple-testing caveat on significance thresholds)