Why the Joint Limit Matters
With a strong instrument, reduced-form coefficients become increasingly precise around their population values. Under a local-to-zero instrument sequence, however, the population slopes themselves shrink at the same rate as their sampling uncertainty. The limiting behavior is therefore described not by two separate approximations, but by a joint distribution that keeps both the local signal and the covariance between the estimates.
That covariance matters because the reduced-form outcome and endogenous-regressor equations share a source of variation. In particular, the outcome’s reduced-form error contains both the structural error and the first-stage error. If those errors are correlated, the covariance between the reduced-form estimates reflects that correlation.
Model and Reduced-Form Coefficients
Consider a scalar model with one instrument and no intercept or controls. The equations for observation \(i\) in a sample of size \(n\) are
Here \(y_i\) is the outcome, \(x_i\) is the endogenous regressor, \(z_i\) is the instrument, \(\beta\) is the structural parameter, and \(u_i\) and \(v_i\) are the structural and first-stage errors. The coefficient \(\pi_n\) is allowed to vary with sample size.
Use the following assumptions throughout. The triples \((z_i,u_i,v_i)\) are independent and identically distributed across observations, with a common distribution that does not depend on \(n\). The instrument is independent of the error pair \((u_i,v_i)\), and
Write \(\sigma_u^2=\operatorname{Var}(u_i)\), \(\sigma_v^2=\operatorname{Var}(v_i)\), and \(\sigma_{uv}=\operatorname{Cov}(u_i,v_i)\). Allow \(\sigma_{uv}\ne 0\). Assume there is a \(\delta>0\) for which \(E|z_i|^{2+\delta}\), \(E|u_i|^{2+\delta}\), and \(E|v_i|^{2+\delta}\) are finite. Finally, take the local-to-zero sequence
where \(c\) is a fixed real number. Independence of \(z_i\) from the errors and their zero means imply \(E[y_i\mid z_i]=\beta\pi_n z_i\) and \(E[x_i\mid z_i]=\pi_n z_i\). Thus the stated population reduced-form slopes are also the conditional mean slopes.
Worked Example: Writing the Two Reduced Forms
Suppose \(x_i=(1.2/\sqrt n)z_i+v_i\) and \(y_i=2x_i+u_i\). Substituting the first equation into the second gives
The coefficient of \(z_i\) is \(1.2/\sqrt n\) in the \(x_i\) equation and \(2.4/\sqrt n\) in the \(y_i\) equation. The corresponding reduced-form errors are \(v_i\) and \(2v_i+u_i\), not \(v_i\) and \(u_i\). The latter distinction determines the covariance of the two coefficient estimates.
The Joint Reduced-Form Limit
The joint limit has a simple structure: the local sequence contributes a fixed shift to the limiting mean, while the error variances and covariance determine the limiting covariance matrix.
Equivalently, after centering at the population reduced-form coefficients,
Derivation of the Joint Limit
First substitute \(x_i=\pi_nz_i+v_i\) into the outcome equation. The two sample slopes can then be written exactly as their population coefficients plus ratios of error-weighted instrument sums:
Define the vector \(\xi_i=z_i(\beta v_i+u_i,\ v_i)^\mathsf{T}\). Its mean is zero. Independence of \(z_i\) and \((u_i,v_i)\) gives its covariance:
The covariance calculation itself also shows why the structural error correlation cannot be discarded. The outcome reduced-form error is \(\beta v_i+u_i\); its covariance with the regressor reduced-form error \(v_i\) is \(\beta\sigma_v^2+\sigma_{uv}\). In particular, this covariance is not generally zero even when \(u_i\) and \(v_i\) are uncorrelated.
Worked Example: Computing the Full Limit Covariance
Let \(\beta=2\), \(Q=4\), \(\sigma_u^2=9\), \(\sigma_v^2=4\), and \(\sigma_{uv}=3\). These error moments are admissible: the determinant of their covariance matrix is \(9(4)-3^2=27>0\). The variance of the outcome reduced-form error is
Its covariance with the regressor reduced-form error is
Thus the limiting covariance matrix is
For \(c=1.5\), the limiting mean is \((\beta c,c)^\mathsf{T}=(3,1.5)^\mathsf{T}\). The full limit is therefore a bivariate normal with that mean and the covariance matrix above. Its off-diagonal entry, \(2.75\), records the dependence between the two reduced-form coefficient estimates.
How Error Correlation Changes the Result
The formula contains \(\sigma_{uv}\) in both the outcome variance and the cross-covariance. Its effect is not limited to the off-diagonal entry: because the outcome reduced-form error combines \(u_i\) and \(\beta v_i\), their covariance also changes that error’s variance. The next calculation isolates this point.
Worked Example: A Negative Structural Error Covariance
Suppose \(\beta=1.5\), \(Q=1\), \(\sigma_u^2=4\), \(\sigma_v^2=1\), and \(\sigma_{uv}=-0.5\). The error covariance matrix is valid because its determinant is \(4(1)-(-0.5)^2=3.75>0\). The outcome reduced-form error variance is
and the cross-covariance is
The limiting covariance matrix is therefore \(\begin{pmatrix}4.75&1\\1&1\end{pmatrix}\). If the errors were incorrectly treated as uncorrelated, the cross-covariance would be reported as \(1.5\), and the outcome variance as \(6.25\). Both entries would be wrong.
The Local Shift and Covariance Structure
The sequence parameter \(c\) appears in the mean of the uncentered joint limit, not in its covariance. For example, changing \(c\) from \(0\) to \(2\) shifts the limit’s mean from \((0,0)^\mathsf{T}\) to \((2\beta,2)^\mathsf{T}\), while leaving the covariance matrix unchanged under the maintained assumptions. Thus the sequence describes how much signal remains on the sampling scale; the error distribution describes the joint sampling variation.
A useful check on the covariance formula is that it must be positive semidefinite. Let \(\Sigma\) denote the covariance matrix in the theorem. Direct expansion gives
To verify the determinant, expand the numerator before dividing by \(Q^2\):
The right-hand side is nonnegative because the covariance matrix of \((u_i,v_i)^\mathsf{T}\) is positive semidefinite. The diagonal entries of \(\Sigma\) are variances divided by \(Q>0\), so they are nonnegative as well. For a symmetric \(2\)-by-\(2\) matrix these conditions imply positive semidefiniteness. This check also shows that the determinant does not depend on \(\beta\): transforming the error pair into \((\beta v_i+u_i,v_i)\) changes its individual variances and covariance, but preserves its determinant.
Common Mistake
- Wrong reasoning: “The outcome equation is \(y_i=\beta x_i+u_i\), so the reduced-form outcome error is just \(u_i\). I can use \(\sigma_u^2\) for its variance and ignore the covariance with the first-stage error.”
- Correction: Substituting \(x_i=\pi_nz_i+v_i\) gives \(y_i=\beta\pi_nz_i+(\beta v_i+u_i)\). The reduced-form outcome error is \(\beta v_i+u_i\). Its variance and covariance with \(v_i\) must be calculated from that expression, retaining \(\sigma_{uv}\).
- Another common error: Centering both estimates at zero in the local sequence without accounting for their local means. For the uncentered scaled estimates, the correct mean is \((\beta c,c)^\mathsf{T}\); it is zero only when \(c=0\).
The joint reduced-form limit is a key input for later weak-instrument analysis. Working with both coefficients together preserves their dependence and makes the local signal explicit. Treating the estimates as independent, or replacing the reduced-form error by the structural error alone, loses information already present in the model.
Check Your Understanding
Try these questions using the assumptions and notation above.
- Under the local sequence \(\pi_n=c/\sqrt n\), what is the limiting mean of \((\sqrt n\,\hat{\gamma}_{y,n},\sqrt n\,\hat{\gamma}_{x,n})^\mathsf{T}\)?
- Why does the reduced-form outcome error equal \(\beta v_i+u_i\), rather than \(u_i\)?
- Write the limiting cross-covariance of the two scaled reduced-form estimates and identify where structural error correlation enters.
- If \(\sigma_{uv}=0\), is the cross-covariance necessarily zero? Explain using its formula.
- Why does changing \(c\) affect the uncentered limiting mean but not the limiting covariance under the stated assumptions?