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Quantifying Omitted Variable Bias in Nonlinear Instrumental Variable Estimators

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Quantifying Omitted Variable Bias in Nonlinear Instrumental Variable Estimators

abstractWe develop a framework for quantifying omitted variable bias (OVB) in nonlinear instrumental variable (IV) estimators, including the local average treatment effect (LATE), the LATE for the treated (LATT), and the partially linear IV model (PLIVM). Extending sensitivity analysis beyond linear settings, we derive bias decompositions, establish partial identification bounds, and construct OVB-adjusted confidence intervals. We estimate OVB bounds and conduct inference using double machine learning (DML), allowing flexible control for high-dimensional covariates. An application to the U.S. Job Training Partnership Act (JTPA) experiment shows that, at conventional significance levels, first-stage compliance estimates are robust to omitted variables, whereas intention-to-treat and treatment effects are more sensitive. Program impacts are robust and significant for females but fragile for males. \\\\ Keywords: Causal inference, Machine learning, Microeconometris, Sensitivity analysis, Partial identification\\

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Introduction

Instrumental variable (IV) estimators are widely used to address endogeneity, but their validity is compromised when relevant variables are omitted. This paper extends the results of CCNSS_2024 by quantifying omitted variable bias (OVB) in a broad class of IV estimators, including the partially linear IV model (PLIVM) and nonlinear estimators such as the local average treatment effect (LATE) and the local average treatment effect for the treated (LATT). Let $Z$ denote the instrumental variable, $X$ a set of observable covariates and $A$ a set of unobservable (or omitted) covariates. Define $W:=(Z,X,A)$ and $W_{s}:=(Z,X)$. Let $Y$ denote the outcome (dependent variable) and $D$ the treatment, which may be endogenous. Many IV estimators can be written in the following form:

equation[equation omitted — 81 chars of source]

where \[\lambda = E[\alpha(W)g_{Y}(W)] \text{ and }\gamma =E[\alpha(W)g_{D}(W)]. \] Inside the above expectations, $\alpha(W)$ is a weighting function, $g_{Y}(W)=E[Y|W]$ and $g_{D}(W)=E[D|W]$. When only $W_s$ is available, the short version of ((ref)) is given by

equation[equation omitted — 90 chars of source]

where \[ \lambda_s = E[\alpha_{s}(W_{s})g_{Ys}(W_{s})]\text{ and }\gamma_s = E[\alpha_{s}(W_{s})g_{Ds}(W_{s})] \] Again, inside the above expectations, $\alpha_{s}(W_{s})$ is a weighting and $g_{Ys}(W_{s})=E[Y|W_{s}]$ and $g_{Ds}(W_{s})=E[D|W_{s}]$. CCNSS_2024 refer to $\alpha(W)$ and $\alpha_{s}(W_s)$ as the long and short Riesz representers (RR).

We assume that with $W$, $\theta$ correctly identifies the interested parameter. However, with $W_s$, $\theta_s$ in general does not correctly identify the interested parameter. The central object of this paper are to characterize magnitude of the omitted variable bias (OVB) caused by using $\theta_s$: \[ |\text{Bias}| := |\theta - \theta_s|, \] and construct the OVB bounds for partially identifying $\theta$. We also will develop relevant statistical inference tools for the OVB analysis.

Many IV estimators admit the form of ((ref)), and we give several examples as follows.

Example 1 (PLIVM): Consider the omitted variable bias (OVB) of a partially linear instrumental variable (IV) regression. We assume that the dependent variable $Y$ and endogenous variable $D$ (can be continuous) have a form of partial linearity as follows:

align[align omitted — 98 chars of source]

Our goal is to estimate the coefficient $\theta$. Following CCNSS_2024, we will refer ((ref)) and ((ref)) as long versions of $Y$ and $D$ (since they are constructed with a completed set of variables $W$). Assume $E[u_{Y}|W]=0$ and $E[u_{D}|W]=0$, but $E[u_{Y}|D]\neq0$ and there is endogeneity. When endogeneity is present, $\theta$ can be identified with a two-stage procedure. At first, we rewrite $Y$ as a reduced form \[ Y=\lambda Z+k(X,A)+\varepsilon_{Y}, \] where $\lambda=\theta\gamma$, $k(X,A)=\theta h(X,A)+f(X,A)$ and $\varepsilon_{Y}=\theta u_{D}+u_{Y}.$ Note that $E[\varepsilon_{Y}|W]=0$, and then $\lambda$ and $\gamma$ can be identified as \[ \lambda =E[\alpha(W)g_{Y}(W)], \gamma =E[\alpha(W)g_{D}(W)], \] where

align*[align* omitted — 67 chars of source]

$g_{Y}(W)=E[Y|W]$ and $g_{D}(W)=E[D|W]$. Then we can have \[ \theta=\frac{\lambda}{\gamma}=\frac{E[\alpha(W) g_{Y}(W)]}{E[\alpha(W) g_{D}(W)]}, \]given that $\gamma\neq 0$. With $W_{s}:=(Z,X)$, the short versions of $Y$ and $D$ in ((ref)) and ((ref)) are given by

align[align omitted — 117 chars of source]

Following similar two-stage procedure above, the $\theta_{s}$ in short version ((ref)) can be identified as \[ \theta_{s}=\frac{\lambda_{s}}{\gamma_{s}}=\frac{E[\alpha_{s}(W_{s})g_{Ys}(W_{s})]}{E[\alpha_{s}(W_{s})g_{Ds}(W_{s})]}, \] given that $\gamma_s\neq 0$, where \[ \alpha_{s}(W_{s})=\frac{Z-E[Z|X]}{E[(Z-E[Z|X])^{2}]}, \] and $g_{Ys}(W_{s})=E[Y|W_{s}]$ and $g_{Ds}=E[D|W_{s}]$.

Example 2 (LATE): Consider the two-sided non-compliance framework. Let $Y_d$ denote the potential outcomes when the treatment variable $D=d$. Let $T\in \{AT,NT,C\}$ denote type of an individual, where $AT$ refer to the always taker, $NT$ refer to the never taker and $C$ refer to the complier. Under certain assumptions Frolich_2007, the local average treatment effect (average treatment effect of the complier group, LATE, IA_1994) \[\text{LATE}:= E[Y_{1}-Y_{0}|T=C]\] can be identified as

equation[equation omitted — 139 chars of source]

where ITT is the intention-to-treat effect and $P(T=C)$ is the probability that an individual is a complier. In the expectations, the weight function $\alpha(W)$ is given by: \[ \alpha(W) =\frac{Z}{\pi(X,A)}-\frac{1-Z}{1-\pi(X,A)}, \]where $\pi(X,A) =P(Z=1|X,A)$ is the propensity score function of the instrumental variable, and $g_{Y}(W)=E[Y|W]$ and $g_{D}(W)=E[D|W]$. Equation ((ref)) is a ratio of two inverse propensity score weighting estimands. The short version of $\theta$ is given by

equation[equation omitted — 157 chars of source]

where \[\alpha_{s}(W_{s}) =\frac{Z}{\pi_{s}(X)}-\frac{1-Z}{1-\pi_{s}(X)}, \pi_{s}(X) =P(Z=1|X),\] and $g_{Ys}(W_{s})=E[Y|W_{s}]$ and $g_{Ds}(W)=E[D|W_{s}]$.

Example 3 (LATT): The local average treatment effect on the treated (LATT) is defined as \[ \text{LATT} := E[Y_1-Y_0|T=C,D=1]. \]That is, LATE for the treated compliers. Under the same assumptions for identifying LATE, LATT can also be identified as $\theta = \lambda/\gamma$. But the weight functions $\alpha(W)$ and $\alpha(W_s)$ for LATT become

eqnarray[eqnarray omitted — 219 chars of source]

where $P_Z = P(Z=1)$. The function $g_Y(W)$, $g_{Y_s}(W_s)$, $g_D(W)$ and $g_{D_s}(W_s)$ are the same as in LATE.

The rest of the paper is organized as follows. Section 2 introduces the proposed method for OVB analysis of IV estimators, including the construction of OVB bounds, a set of statistical inference tools and a method for estimating them using double machine learning (DML). Section 3 applies the method to an empirical analysis of LATE and LATT using the classical JTPA data. Section 4 concludes.

Methodology

The OVB Bounds for $\lambda$ and $\gamma$

To quantify the OVB of $\theta_{s}\in \boldsymbol{\Theta}_s$, instead of directly calculating the OVB through comparing $\theta\in \boldsymbol{\Theta}$ and $\theta_s$, we exploit results from inference with weak instrument variables (section 13.3 in CHKSS_2024). A similar strategy, based on the Anderson–Rubin regression, was also adopted by CH_2025 to construct the OVB bound in a linear IV model. Suppose we would like to test $H_{0}:\theta=\theta_0$, where $\theta_0\in \boldsymbol{\Theta}_0\subseteq \boldsymbol{\Theta}$. Let $\phi_{t}:=\lambda-\gamma t$ and testing $H_{0}$ is equivalent to testing $H_{0}^{\prime}:\phi_{\theta_0}=0$. We next show that $\phi_{t}$ can be partially identified when the short version estimands $\lambda_s$ and $\gamma_s$ are used. To simplify the notations, we use $(\alpha,\alpha_s, g_Y, g_{Ys}, g_D, g_{Ds})$ to replace $(\alpha(W),\alpha_s(W_s), g_Y(W), g_{Ys}(W_s), g_D(W), g_{Ds}(W_s))$ in the following discussion.

At first, bias of $\lambda_{s}$ can be expressed as:

align[align omitted — 92 chars of source]

by using the result in CCNSS_2024. A key condition to achieving ((ref)) is that $E[g_{Y_s}(\alpha-\alpha_s)]=0$, which holds for LATE, LATT and PLIVM. With some calculations, we can have the following result for the squared bias of $\lambda_s$:

equation[equation omitted — 89 chars of source]

where $\rho_{Y}^{2}:=Cor^{2}(\alpha-\alpha_{s},g_{Y}-g_{Ys})$, $B_{Y}^{2}=C_{Y}^{2}C_{\alpha}^{2}S_{Y}^{2}$ and \[C_{Y}^{2} = \frac{E[(g_Y-g_{Y_s})^2]}{E[(Y-g_{Y_s})^2]}, C_{\alpha}^{2} = \frac{E[(\alpha - \alpha_s)^2]}{E[\alpha_{s}^{2}]}, S_{Y}^{2} = E[(Y-g_{Ys})^{2}]E[\alpha_{s}^{2}]=\sigma_{Y_{s}}^{2}v_{s}^{2}.\] $C_Y$ and $C_{\alpha}$ are referred to sensitivity parameters in the OVB analysis, and in practice, they can be specified by researchers according to domain knowledge of the empirical study. $S_{Y}^{2}$ can be directly estimated with data. With the above results, we can have

equation[equation omitted — 79 chars of source]

where $\lambda^{-}:=\lambda_{s}-|\rho_{Y}|B_{Y}$ and $\lambda^{+}:=\lambda_{s}+|\rho_{Y}|B_{Y}$ by using the fact that $C_Y$, $C_{\alpha}$ and $S_Y$ are all nonnegative. Similarly, for $\gamma$ and $\gamma_{s}$, by using the result in CCNSS_2024, we can have:

align[align omitted — 89 chars of source]

A key condition to achieving ((ref)) is that $E[g_{D_s}(\alpha-\alpha_s)]=0$, which holds for LATE, LATT and PLIVM. Then following similar procedures for deriving ((ref)), we can have:

equation[equation omitted — 87 chars of source]

where $\rho_{D}^{2}:=Cor^{2}(\alpha-\alpha_{s},g_{D}-g_{Ds})$, $B_{D}^{2}=C_{D}^{2}C_{\alpha}^{2}S_{D}^{2}$ and \[C_{D}^{2} = \frac{E[(g_D-g_{Ds})^2]}{E[(D-g_{Ds})^2]}, S_{D}^{2}= E[(D-g_{Ds})^{2}]E[\alpha_{s}^{2}] = \sigma_{Ds}^{2}v_{s}^{2}.\] Finally, it can be shown that

equation[equation omitted — 75 chars of source]

where $\gamma^{-}:=\gamma_{s}-|\rho_{D}|B_{D}$ and $\gamma^{+}:=\gamma_{s}+|\rho_{D}|B_{D}$ by using the fact that $C_D$, $C_{\alpha}$ and $S_D$ are all nonnegative.

Constructing the OVB Bound for $\theta$

Combining the above results yields the following partial identification result for $\phi_{t}$:

equation[equation omitted — 162 chars of source]

for $t\in \boldsymbol{\Theta}_0$. With some algebra, ((ref)) can be further rewritten as:

equation[equation omitted — 73 chars of source]

where

align*[align* omitted — 161 chars of source]

Using the result in ((ref)), we derive the following partial identification results for $\theta_0$.

theoremSuppose that $\theta=\theta_0$ and $\phi_{\theta_0} = \lambda - \gamma \theta_0$ satisfies ((ref)): $\phi_{\theta_0}^{-}\leq\phi_{\theta_0}\leq \phi_{\theta_0}^{+}$. \begin{enumerate} • When $(\gamma^{-},\gamma^{+})\in\mathbb{R}^{++}$: \begin{itemize} • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{++}$, then $\theta_0\in [\lambda^{-}/\gamma^{+},\lambda^{+}/\gamma^{-}].$ • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{--}$, then $\theta_0\in [\lambda^{-}/\gamma^{-},\lambda^{+}/\gamma^{+}].$ • If $\lambda^{-}$ and $\lambda^{+}$ have different signs, then $\theta_0\in [\lambda^{-}/\gamma^{-},\lambda^{+}/\gamma^{-}]$. \end{itemize} • When $(\gamma^{-},\gamma^{+})\in\mathbb{R}^{--}$: \begin{itemize} • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{++}$, then $\theta_0 \in [\lambda^{+}/\gamma^{+},\lambda^{-}/\gamma^{-}].$ • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{--}$, then $\theta_0 \in[\lambda^{+}/\gamma^{-},\lambda^{-}/\gamma^{+}].$ • If $\lambda^{+}$ and $\lambda^{-}$ have different signs, then $\theta_0 \in [\lambda^{+}/\gamma^{+},\lambda^{-}/\gamma^{+}]$. \end{itemize} • When $\gamma^{-}\neq 0$ and $\gamma^{+}\neq 0$ and they have different signs: \begin{itemize} • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{++}$, then $\theta_{0}\in (-\infty,\lambda^{-}/\gamma^{-}]\cup[\lambda^{-}/\gamma^{+},\infty).$ • If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{--}$, then $\theta_{0}\in(-\infty,\lambda^{+}/\gamma^{+}]\cup[\lambda^{+}/\gamma^{-},\infty)$. • If $\lambda^{+}$ and $\lambda^{-}$ have different signs, then $\theta_{0}\in\left(-\infty,\infty\right)$. \end{itemize} \end{enumerate}

To prove Theorem 1, note that if $\theta_{0}$ is the true value of $\theta$, $0\in [\phi_{\theta_{0}}^{-},\phi_{\theta_{0}}^{+}]$. This requires that both $\phi_{\theta_{0}}^{+}\geq0$ and $\phi_{\theta_{0}}^{-}\leq0$ hold. Therefore: \[ \theta_{0}\in\{t\in \boldsymbol{\Theta}_0:\{\phi_{t}^{+}\geq0\}\cap\{\phi_{t}^{-}\leq0\}\}. \] In addition, when $(\gamma^{-},\gamma^{+})\in\mathbb{R}^{++}$, if $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{++}$, $\theta_{0}>0$. If $(\lambda^{-},\lambda^{+})\in\mathbb{R}^{--}$, $\theta_{0}<0$. If $\lambda^{-}$ and $\lambda^{+}$ have different signs, $\theta_{0}\in[-c_1,c_2]$ where $(c_1,c_2)>0$ are some constants. Similar arguments can be applied to derive the OVB bounds of $\theta_0$ when $(\gamma^{-},\gamma^{+})\in\mathbb{R}^{--}$.

Let $(\hat{\lambda}^{-},\hat{\lambda}^{+},\hat{\gamma}^{-},\hat{\gamma}^{+})$ denote some estimates of $(\lambda^{-},\lambda^{+},\gamma^{-},\gamma^{+})$. In practice, we can apply the result of Theorem 1 to estimate the upper and lower bounds for $\theta_0$ using $(\hat{\lambda}^{-},\hat{\lambda}^{+},\hat{\gamma}^{-},\hat{\gamma}^{+})$. If the signs of $(\hat{\gamma}^{-},\hat{\gamma}^{+})$ are the same, the OVB bounds can be directly estimated following points 1. and 2. of Theorem 1. However, if $(\hat{\gamma}^{-},\hat{\gamma}^{+})$ have different signs, the situation becomes more complicated. According to point 3. of Theorem 1, when $(\gamma^{-},\gamma^{+})\neq (0,0)$ and have different signs, the partially identified set for $\theta_0$ is either (a) split into disjoint segments of the real line (when $(\lambda^{-},\lambda^{+})$ have the same sign); or (b) the entire real line (when $(\lambda^{-},\lambda^{+})$ have different signs). In case (a), zero is not included in the OVB bound; in (b), it is. These results, particularly case (a), are hard to be interpreted. Therefore for practically applying Theorem 1, we recommend first checking whether $(\hat{\gamma}^{-},\hat{\gamma}^{+})\neq (0,0)$ and have the same sign: $(\hat{\gamma}^{-},\hat{\gamma}^{+})\in\mathbb{R}^{++}$ or $(\hat{\gamma}^{-},\hat{\gamma}^{+})\in\mathbb{R}^{--}$. If this condition fails, we suggest stopping here and reporting that the first-stage estimation fails when the OVB is concerned. If the condition holds, we proceed with results of points 1. and 2. of Theorem 1 to construct the OVB bound for $\theta_0$.

Sensitivity Parameters in the OVB Analysis

The sensitivity parameters $C_{\alpha}$, $C_{Y}$ and $C_D$ play crucial roles in the OVB analysis. In this section, we elaborate on their properties and show that serve as measures of the strength of the omitted variable.

Let $R^{2}_{U_1\sim U_2}:=\text{Var}(U_2)/\text{Var}(U_1)$ denote the ratio of variances between two random variables $U_2$ and $U_1$. If $U_2=E[U_1|U_3]$ holds,

equation[equation omitted — 142 chars of source]

where $\eta_{U_1\sim U_3}^{2}$ denotes the non-parametric R-squared (Pearson's correlation ratio) between $U_1$ and $U_3$.

In the cases of PLIVM, LATE and LATT, we have $E[\alpha]=E[\alpha_{s}]=0$, and therefore $\text{Var}(\alpha)=E[\alpha^{2}]$ and $\text{Var}(\alpha_{s})=E[\alpha_{s}^{2}]$. Then using the fact that $E[\alpha_{s}(\alpha-\alpha_{s})]=0$, we also can have $E[(\alpha-\alpha_{s})^{2}]=E[\alpha^{2}]-E[\alpha_{s}^{2}]\geq0$ and express $C_{\alpha}^{2}$ as:

equation[equation omitted — 117 chars of source]

For LATE and LATT, since $E[\alpha|W_s] = \alpha_s$, we have $R_{\alpha\sim\alpha_{s}}^{2}=\eta_{\alpha\sim W_{s}}^{2}$, the nonparametric $R^{2}$ between $\alpha$ and $W_{s}$. However, $R_{\alpha\sim\alpha_{s}}^{2}=\eta_{\alpha\sim W_{s}}^{2}$ does not hold for PLIVM, since $E[\alpha|W_s] \neq \alpha_s$ for this case.

For LATE, using $\text{Var}(Z|X,A)=\pi(X,A)(1-\pi(X,A))$, we obtain $E[\alpha^{2}]=E\left[1/\text{Var}(Z|X,A)\right]$, which is the expected precision of prediction on $Z$ using $(X,A)$. Similarly, $E[\alpha_{s}^{2}]=E\left[1/\text{Var}(Z|X)\right].$ Therefore \[ 1-R^2_{\alpha\sim\alpha_s} =\frac{E\left[\frac{1}{\text{Var}(Z|X,A)}\right]-E\left[\frac{1}{\text{Var}(Z|X)}\right]}{E\left[\frac{1}{\text{Var}(Z|X,A)}\right]}, \]which quantifies the (absolute) decrease in expected prediction precision for $Z$ when $A$ is omitted in the model. Note that $1-R^2_{\alpha\sim\alpha_s}$ is bounded between 0 and 1. Using the result in ((ref)), we also have:

align*[align* omitted — 163 chars of source]

which represents the additional gain in expected prediction precision for $Z$ when $(X,A)$ are included into the model, relative to using $X$ alone. For PLIVM, $\alpha(W)=(Z-E[Z|A,X])/E[(Z-E[Z|A,X])^{2}]$ and $\alpha_{s}(W_{s})=(Z-E[Z|X])/E[(Z-E[Z|X])^{2}]$. Then it can be shown that $R_{\alpha\sim\alpha_{s}}^{2}=E[(Z-E[Z|A,X])^{2}]/E[(Z-E[Z|X])^{2}]$ and

align*[align* omitted — 157 chars of source]

which captures an increase in the MSE for predicting $Z$ when $A$ is absent in the model, relative to that for predicting $Z$ when both $(Z,A)$ present. In the second equality, $\eta_{Z\sim A|X}^{2} = 1-R^2_{\alpha\sim\alpha_s}$ is the nonparametric partial $R^{2}$ between $Z$ with $A$, conditional on $X$, which is defined as \[ \eta_{Z\sim A|X}^{2}:=\frac{E[\text{Var}(Z|X)]-E[\text{Var}(Z|A,X)]}{E[\text{Var}(Z|X)]}=\frac{\eta_{Z\sim A,X}^{2}-\eta_{Z\sim X}^{2}}{1-\eta_{Z\sim X}^{2}}. \] $\eta_{Z\sim A|X}^{2}$ captures the extra explanatory power that $A$ provides for $Z$, beyond what is already explained by $X$, relative to $1-\eta_{Z\sim X}^{2}$, the remaining unexplained variation of $Z$ after conditioning on $X$.

For $C_{Y}^{2}$ (or $C_{D}^{2}$), with the notations in ((ref)), we can express $C_{Y}^{2}$ as: \[C_{Y}^{2} = R^{2}_{Y-g_{Ys} \sim g_Y-g_{Ys}} \]using the identities $E[g_{Y}g_{Y_{s}}]=E[Yg_{Y_{s}}]=E[g_{Y_{s}}^{2}]$. Furthermore:

eqnarray*[eqnarray* omitted — 193 chars of source]

which is the nonparametric partial $R^{2}$ between $Y$ with $A$, conditional on $(Z,X)$. The quantity $\eta_{Y\sim A|Z,X}^{2}$ reflects the additional explanatory power of $A$ beyond what $(Z,X)$ already provides, relative to $1-\eta_{Y\sim Z,X}^{2}$, the unexplained variation in $Y$ given $(Z,X)$. Alternatively, $C_{Y}^{2}$ can also be interpreted as the proportional reduction in the MSE for predicting $Y$ when $A$ is additionally included into the model with $(Z,X)$, comparing to using $(Z,X)$ alone. Thus the sensitivity parameters $C_Y^{2}$, $C_D^{2}$ and $C_{\alpha}^{2}$ measure the gains in predictive accuracy for $Y$, $D$ and $Z$, respectively, when variable $A$ is included in the models given $X$.

To compute the OVB bounds in ((ref)), ((ref)) and ((ref)), we need to assign values to the sensitivity parameters $C_Y$, $C_{\alpha}$ and $C_D$. As discussed above, these parameters capture how the omitted variable $A$ affects the weight $\alpha$ and predictions for $Y$ and $D$, when only $(Z,X)$ are used. Therefore setting their values is equivalent to assessing the importance of the omitted variable $A$ in determining $\alpha$ and predicting $Y$ and $D$. Since the parameters of interest are constituted by the weight $\alpha$ and predictions on $Y$ and $D$, carefully selecting the values of the sensitivity parameters is crucial for quantifying the bias due to the omission of $A$. This can be done by leveraging the researcher’s domain knowledge, by estimating them from data through benchmarking analysis (see the discussion below), or by combining both approaches.

Finally, the sensitivity parameters $C_{\alpha}^{2}$, $C_Y^{2}$ and $C_D^{2}$ are all unit-free, as they are scaled by factors that eliminate dependence on measurement units. This scale-invariance ensures that the parameters are comparable across different variables and empirical contexts, regardless of their units of measurement. Since these parameters are derived from variance ratios (e.g., nonparametric R-squared), they quantify proportional improvements in predictive accuracy rather than absolute changes. This property facilitates meaningful interpretation, robust sensitivity analysis, and consistent calibration of parameter values—particularly when conducting simulations or assessing the importance of omitted variables whose scales may be unknown or heterogeneous. As a result, the unit-free nature of these sensitivity measures enhances both the generalizability and practical relevance of the OVB analysis.

Benchmarking Analysis

Following CH_2022 and CCNSS_2024, we conduct a benchmarking analysis by imposing a requirement that the explanatory power gained from including the omitted variable $A$ should be comparable to that obtained from specific observable variables. The primary objective of this analysis is to establish reasonable bounds for restricting the maximum values of the sensitivity parameters $C_{\alpha}^{2}$, $C_Y^{2}$ and $C_D^{2}$. To achieve this, we first show that $C_{\alpha}^{2}$, $C_{Y}^{2}$ and $C_{D}^{2}$ in the OVB bounds can be expressed as functions of the relative strength of the omitted variable $A$ comparable to other observable variables. Let $X_{-j}$ denote the set of all other observable variables when $X_{j}$ is excluded from $X$. Let $W_{-j}=(Z,X_{-j},A)$, $W_{s,-j}=(Z,X_{-j})$ and:

align*[align* omitted — 205 chars of source]

As before, we will use the abbreviations $\alpha_{s,-j}$, $g_{Ys,-j}$ and $g_{Ds,-j}$ to denote $\alpha_{s,-j}(W_{s,-j})$, $g_{Ys,-j}(W_{s,-j})$ and $g_{Ds,-j}(W_{s,-j})$. For $\alpha_{s}$, define the gain in explanatory power from including $X_{j}$, given $X_{-j}$ as: \[ 1-R_{\alpha_{s}\sim\alpha_{s,-j}}^{2}=1-\frac{E[\alpha_{s,-j}^{2}]}{E[\alpha_{s}^{2}]}. \] The gain in explanatory power from including $A$, $1-R_{\alpha\sim\alpha_{s}}^{2}$ can then be expressed as:

eqnarray[eqnarray omitted — 296 chars of source]

Note that $1-R_{\alpha\sim\alpha_{s,-j}}^{2}$ measures the gain in explanatory power from including $(A,X_{j})$, given $X_{-j}$. The numerator in ((ref)) therefore captures the extra explanatory power from including $A$ beyond that provided by $X_{j}$, given $X_{-j}$. Define the relative strength of $A$ to $X_{j}$ for $\alpha$ as:

equation[equation omitted — 157 chars of source]

which is a ratio of the extra gain in explanatory power from including $(X_j,A)$, compared to that from including $X_{j}$ only, given $X_{-j}$. Therefore the quantity $k_{\alpha}$ measures relative importance of $A$ compared to $X_{j}$ in explaining $\alpha$, given $X_{-j}$. A value $k_{\alpha}\leq1$ indicates that $A$ is relatively less important than $X_{j}$ for explaining $\alpha$, given $X_{-j}$. Furthermore, it can be shown that \[ 1-R_{\alpha\sim\alpha_{s}}^{2}=k_{\alpha}G_{\alpha}, \] where

equation*[equation* omitted — 127 chars of source]

is a quantity that can be estimated. This leads directly to:

equation*[equation* omitted — 153 chars of source]

For $C_{Y}^{2}$, at first note that\footnote{The same result and derivation are applied to $C_{D}^{2}$.}

eqnarray[eqnarray omitted — 243 chars of source]

by using the result $E(Y-g_Y)^{2}=E[Y^{2}]-E[g_{Y}^{2}]$. Equation ((ref)) captures the relative reduction in the mean squared error (MSE) in predicting $Y$ when including the omitted variable $A$. Following similar argument for deriving expression of $1-R_{\alpha\sim\alpha_{s}}^{2}$, we also have:

eqnarray[eqnarray omitted — 289 chars of source]

The numerator in ((ref)) represents the additional reduction in MSE in predicting $Y$ from including $(X_j,A)$, compared to that from including $X_{j}$ only, given $X_{-j}$. Define the relative strength of $A$ to $X_{j}$ for predicting $Y$ as

equation*[equation* omitted — 145 chars of source]

This yields

equation*[equation* omitted — 68 chars of source]

where

equation*[equation* omitted — 111 chars of source]

is a quantity that can be estimated.

Estimating $G_{\alpha}$ and $G_Y$ involves with estimating the variance ratios $R_{\alpha_s\sim\alpha_{s,-j}}^{2}$ and $R_{Y-g_{Ys,-j}\sim Y-g_{Ys}}^{2}$, which can be directly computed from available data. In addition, for estimating $\alpha_{s,-j}$ and $g_{Ys,-j}$, there is no restriction on the number of excluded variables $X_j$. That is, we may exclude a group of variables simultaneously if it is necessary.\footnote{For example, variables such as age are often represented categorically. In practice, we may exclude all age-related variables when estimating $\alpha_{s,-j}$ and $g_{Ys,-j}$. This approach is equivalent to treating $X_j$ as a vector that includes these age variables.} This flexibility facilitates a richer analysis on robustness of parameter estimations to the omitted variable bias.

Estimation and Inference for the OVB Bound

To estimate the OVB bound, we need to estimate $(\lambda_s, \gamma_s)$, the short version of $(\lambda,\gamma)$, as well as $(v^{2}_s,\sigma^{2}_{Y_s},\sigma^{2}_{D_s})$, along with the calibrated values of the sensitivity parameters $C_{\alpha}$, $C_Y$ and $C_D$ and correlation coefficients $|\rho_{Y}|$ and $|\rho_D|$. In our empirical application, we employ the double machine learning (DML) estimators combined with the median method CCDDHNR_2018 to estimate $(\lambda_s, \gamma_s, v^{2}_s,\sigma^{2}_{Y_s},\sigma^{2}_{D_s})$. The DML estimator integrates an estimator satisfying the Neyman orthogonality with K-fold cross fitting. We begin by introducing the former, which can be derived using the influence functions (IFs).

We first consider estimating the OVB bound for LATE. In this case, the IFs of $\lambda_{s}$ and $\gamma_s$ are given by:

equation[equation omitted — 150 chars of source]

where

eqnarray*[eqnarray* omitted — 289 chars of source]

By using the moment conditions $E[\psi_{\lambda_{s}}(Y,W_s)]=E[\psi_{\gamma_{s}}(D,W_s)]=0$, we identify:

equation[equation omitted — 108 chars of source]

It can be shown that the estimators based on the IFs ((ref)) satisfy Neyman orthogonality. Given that $\gamma_s\neq0$, the short version of $\theta$ is $\theta_{s}=\lambda_{s}/\gamma_{s}$, which can also be identified by solving the moment condition $E[\psi_{\theta_{s}}(Y,D,W_s)]=0$, where \[ \psi_{\theta_{s}}(Y,D,W_s)= \bar{\psi}(Y,W_s)-\bar{\psi}(D,W_s)\theta_s \]

For the case of LATT, the IFs for $\lambda_{s}$ and $\gamma_s$ are given by Hahn_1998:

equation[equation omitted — 189 chars of source]

where

eqnarray*[eqnarray* omitted — 341 chars of source]

Again, by setting $E[\psi_{\lambda_{s}}(Y,W_s)]=E[\psi_{\gamma_{s}}(D,W_s)]=0$, $\lambda_{s}$ and $\gamma_{s}$ can be identified as:

equation[equation omitted — 114 chars of source]

The estimators also satisfy Neyman orthogonality. Given that $\gamma_s\neq0$, the short version of $\theta$ is $\theta_{s}=\lambda_{s}/\gamma_{s}$, which can also be solved by using the moment condition $E[\tilde{\psi}_{\theta_{s}}]=0$, where \[ \psi_{\theta_{s}}(Y,D,W_s)= \tilde{\psi}(Y,W_s)-\tilde{\psi}(D,W_s)\theta_s. \]

For PLIVM in ((ref)) and ((ref)), we use the following IFs of $\lambda_{s}$ and $\gamma_s$ (Robinson style score functions) to estimate $\lambda_{s}$ and $\gamma_{s}$:

eqnarray[eqnarray omitted — 214 chars of source]

where $m(X):=E[Y|X]$, $r(X):=E[D|X]$ and $l(X):=E[Z|X]$. Setting $E[\psi_{\lambda_{s}}(Y,W_s)]=E[\psi_{\gamma_{s}}(D,W_s)]=0$ yields:

equation[equation omitted — 159 chars of source]

Given that $\gamma_s\neq 0$, the short version of $\theta$ is $\theta_{s}=\lambda_{s}/\gamma_{s}$, which can also be obtained with the moment condition $E[\psi_{\theta_{s}}(Y,D,W_s)]=0$, where \[ \psi_{\theta_{s}}(Y,D,W_s)=[Y-m(X)-\theta_{s}(D-r(X))][Z-l(X)] \] is a Robinson style score function for $\theta_{s}$ with $Z$ as the instrumental variable.

The sample analogues of ((ref)), ((ref)) and ((ref)) are used as estimators for estimating $\lambda_s$ and $\gamma_s$ in conjunction with K-fold cross-fitting (see Section 2.5.2). Inside these estimators, nuisance parameters, such as $\pi_{s}(X)$, $E[Y|Z=1,D]$ and $E[D|Z=1,X]$ etc., can be estimated using appropriate parametric or nonparametric models, potentially enhanced with various machine learning methods (e.g., random forest or the lasso), especially when the dimension of $X$ is large and/or their functional forms are complex. In our empirical application, we use random forest\footnote{The random forest is conducted with function ranger in R package ranger.} with K-fold cross-fitting to estimate these nuisance parameters. The estimate of the short version $\theta_s$ is crucial for the purposes of comparison and statistical inference in the empirical analysis. However, for estimating the OVB bounds for $\theta$ shown in Theorem 1, we only need estimates of $(\lambda_s, \gamma_s,v^{2}_s,\sigma^{2}_{Y_s},\sigma^{2}_{D_s})$, and estimating $\theta_s$ is not required.

Confidence Interval for the OVB Bound

We now turn to construction of confidence interval (C.I) for the OVB bound. The C.I. may serve as a measure to determine whether the statistical significance of the initial estimate persists after accounting for OVB. Let $\zeta_{Y,\alpha}=|\rho_{Y}|C_{Y}C_{\alpha}$ and $\zeta_{D,\alpha}=|\rho_{D}|C_{D}C_{\alpha}$. The influence functions (IFs) of $\lambda^{+}$ and $\lambda^{-}$ are given by CCNSS_2024:

equation*[equation* omitted — 158 chars of source]

where \[ \psi_{S_{Y}}=\frac{\sigma_{Y_{s}}^{2}\psi_{v_{s}^{2}}+v_{s}^{2}\psi_{\sigma_{Y_{s}}^{2}}}{2S_{Y}}, \] is the IF of $S_Y$ and \[\psi_{\sigma_{Ys}^{2}}= (Y-g_{Ys})^{2}-\sigma_{Ys}^{2}, \text{ } \psi_{v_{s}^{2}}=\alpha_{s}^{2}-v_{s}^{2}\] are IFs of $\sigma_{Ys}^{2}=E[(Y-g_{Ys})^{2}]$ and $v_{s}^{2}=E[\alpha_{s}^{2}]$. If the DML estimators for estimating $\lambda^{+}$ and $\lambda^{-}$, denoted by $\hat{\lambda}^{+}$ and $\hat{\lambda}^{-}$, satisfy certain regularity conditions CCDDHNR_2018, then $\hat{\lambda}^{+}$ and $\hat{\lambda}^{-}$ exhibit asymptotic normality: \[ \sqrt{n}(\hat{\lambda}^{+}-\lambda^{+}) \overset{a.}{\rightarrow} N\left(0,E\left[\psi_{\lambda^{+}}^{2}\right]\right), \sqrt{n}(\hat{\lambda}^{-}-\lambda^{-}) \overset{a.}{\rightarrow} N\left(0,E\left[\psi_{\lambda^{-}}^{2}\right]\right). \]Furthermore, the following one-sided covering properties hold: \[ \lim_{n\rightarrow\infty}P(\lambda^{+}\leq\hat{\lambda}^{+}_{1-\tau})\geq 1-\tau, \lim_{n\rightarrow\infty}P(\lambda^{-}\geq \hat{\lambda}^{-}_{\tau})\geq 1-\tau, \]where

equation[equation omitted — 229 chars of source]

and $\text{se}(\hat{\lambda}^{-}):=\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{-})/n}$ and $\text{se}(\hat{\lambda}^{+}):=\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{+})/n}$ are the standard errors of $\hat{\lambda}^{+}$ and $\hat{\lambda}^{-}$, and $\Phi^{-1}(1-\tau)$ denotes the $(1-\tau)$-th quantile of the standard normal distribution.\footnote{In the following, we assume that $\tau\leq 0.5$.}

For $(\gamma^{+}, \gamma^{-})$, we also have similar results. The IFs of $\gamma^{+}$ and $\gamma^{-}$ are given by: \[ \psi_{\gamma^{+}} =\psi_{\gamma_{s}}+\zeta_{D,\alpha}\psi_{S_D},\text{ } \psi_{\gamma^{-}} =\psi_{\gamma_{s}}-\zeta_{D,\alpha}\psi_{S_D}, \]where \[ \psi_{S_{D}} =\frac{\sigma_{D_{s}}^{2}\psi_{v_{s}^{2}}+v_{s}^{2}\psi_{\sigma_{D_{s}}^{2}}}{2S_{D}}, \]is the IF of $S_D$ and \[\psi_{\sigma_{Ds}^{2}}=(D-g_{Ds})^{2}-\sigma_{Ds}^{2}\] is the IF of $\sigma_{Ds}^{2}=E[(D-g_{Ds})^{2}]$. Again, if the DML estimators for estimating $\gamma^{+}$ and $\gamma^{-}$, denoted by $\hat{\gamma}^{+}$ and $\hat{\gamma}^{-}$, satisfy certain regularity conditions, the asymptotic normality of $\hat{\gamma}^{+}$ and $\hat{\gamma}^{-}$ holds: \[ \sqrt{n}(\hat{\gamma}^{+}-\gamma^{+}) \overset{a.}{\rightarrow} N\left(0,E\left[\psi_{\gamma^{+}}^{2}\right]\right), \sqrt{n}(\hat{\gamma}^{-}-\gamma^{-}) \overset{a.}{\rightarrow} N\left(0,E\left[\psi_{\gamma^{-}}^{2}\right]\right). \]Accordingly the following one-sided covering properties also hold: \[ \lim_{n\rightarrow\infty}P(\gamma^{+}\leq\hat{\gamma}^{+}_{1-\tau})\geq 1-\tau, \lim_{n\rightarrow\infty}P(\gamma^{-}\geq \hat{\gamma}^{-}_{\tau})\geq 1-\tau, \] where

equation[equation omitted — 220 chars of source]

and $\text{se}(\hat{\gamma}^{-}):=\sqrt{\widehat{\text{Var}}(\hat{\gamma}^{-})/n}$ and $\text{se}(\hat{\gamma}^{+}):=\sqrt{\widehat{\text{Var}}(\hat{\gamma}^{+})/n}$ are the standard errors of $\hat{\gamma}^{+}$ and $\hat{\gamma}^{-}$.

We now show the asymptotic results of $\hat{\phi}_{t}^{+}$ and $\hat{\phi}_{t}^{-}$, the plug-in estimators constructed using $(\hat{\lambda}^{+},\hat{\gamma}^{+},\hat{\gamma}^{-})$ and $(\hat{\lambda}^{-},\hat{\gamma}^{+},\hat{\gamma}^{-})$ for estimating $\phi_{t}^{+}$ and $\phi_{t}^{-}$ in ((ref)), under the assumptions that the parameters $(t,\rho_{Y},\rho_{D},C_{\alpha},C_{Y},C_{\alpha})$ are all fixed and some regularity conditions for the DML estimators hold. The derivations of the IFs of $\phi_{t}^{+}$ and $\phi_{t}^{-}$ and approximate variances of $\hat{\phi}_{t}^{+}$ and $\hat{\phi}_{t}^{-}$ relies using on the fact that $\phi_{t}^{+}$ and $\phi_{t}^{-}$ are linear functions of $(\lambda^{+}, \gamma^{+}, \gamma^{-})$ and $(\lambda^{-}, \gamma^{+}, \gamma^{-})$.

theoremAssume $(t,\rho_{Y},\rho_{D},C_{\alpha},C_{Y},C_{D})$ are all fixed. The influence functions of $\phi_{t}^{+}$ and $\phi_{t}^{-}$ are given by: \[ \psi_{\phi_{t}^{+}}=\mathbf{C}_{t}^{+\top}\boldsymbol{\psi},\psi_{\phi_{t}^{-}}=\mathbf{C}_{t}^{-\top}\boldsymbol{\psi}, \] where \begin{eqnarray*} \mathbf{C}_{t}^{+} & = & \left[1,-t,\left(\frac{\zeta_{Y,\alpha}\sigma_{Y_{s}}}{2v_{s}}+\frac{\zeta_{D,\alpha}\sigma_{D_{s}}|t|}{2v_{s}}\right),\frac{\zeta_{Y,\alpha}v_{s}}{2\sigma_{Y_{s}}},\frac{\zeta_{D,\alpha}v_{s}|t|}{2\sigma_{D_{s}}}\right]^{\top},\\ \mathbf{C}_{t}^{-} & = & \left[1,-t,-\left(\frac{\zeta_{Y,\alpha}\sigma_{Y_{s}}}{2v_{s}}+\frac{\zeta_{D,\alpha}\sigma_{D_{s}}|t|}{2v_{s}}\right),-\frac{\zeta_{Y,\alpha}v_{s}}{2\sigma_{Y_{s}}},-\frac{\zeta_{D,\alpha}v_{s}|t|}{2\sigma_{D_{s}}}\right]^{\top},\\ \boldsymbol{\psi} & = & \left[\psi_{\lambda s},\psi_{\gamma_{s}},\psi_{v_{s}^{2}},\psi_{\sigma_{Y_{s}}^{2}},\psi_{\sigma_{D_{s}}^{2}}\right]^{\top}. \end{eqnarray*} Suppose $(\lambda_{s},\gamma_{s},v_{s}^{2},\sigma_{Y_{s}}^{2},\sigma_{D_{s}}^{2})$ are all estimated with the DML estimators. If Assumption 4.2 (for PLIVM) or 5.2 (for LATE) in CCDDHNR_2018 holds, then \[ \sqrt{n}(\hat{\phi}_{t}^{+}-\phi_{t}^{+})\overset{a.}{\rightarrow}N\left(0,\mathbf{C}_{t}^{+\top}\boldsymbol{\Omega}\mathbf{C}_{t}^{+}\right),\sqrt{n}(\hat{\phi}_{t}^{-}-\phi_{t}^{-})\overset{a.}{\rightarrow}N\left(0,\mathbf{C}_{t}^{-\top}\boldsymbol{\Omega}\mathbf{C}_{t}^{-}\right), \] where $\boldsymbol{\Omega}=\mathbf{J}_{0}^{-1}E[\boldsymbol{\psi}\boldsymbol{\psi}^{\top}]\mathbf{J}_{0}^{-1}$is the approximate covariance matrix of these DML estimators and $\mathbf{J}_{0}$ is the Jacobian matrix.

In the case of PLIVM, $\mathbf{J}_0$ is a $5\times5$ diagonal matrix with diagonal elements: \[\left(-E\left[(Z-l(X))^{2}\right],-E\left[(Z-l(X))^{2}\right],-1,-1,-1\right).\] For LATE and LATT, $\mathbf{J}_{0}$ is a negative identity matrix, and the approximate variances of $\sqrt{n}(\hat{\phi}_{t}^{+}-\phi_{t}^{+})$ and $\sqrt{n}(\hat{\phi}_{t}^{-}-\phi_{t}^{-})$ can be simplified to $E[\psi_{\phi_{t}^{+}}^{2}]$ and $E[\psi_{\phi_{t}^{-}}^{2}]$.

We next show that the $(1-\tau)$ OVB-adjusted C.I. for $\theta$ can be constructed using the results in Theorem 2.

theoremLet $\hat{\phi}_{t,1-\tau}^{+}$ denote the upper bound of $(1-\tau)$ C.I. of $\phi_{t}^{+}$, and $\hat{\phi}_{t,\tau}^{-}$ denote the lower bound of $(1-\tau)$ C.I. of $\phi_{t}^{-}$, i.e., \[ \hat{\phi}_{t, 1-\tau}^{+} :=\hat{\phi}_{t}^{+}+\text{se}(\hat{\phi}_{t}^{+})\Phi^{-1}(1-\tau), \hat{\phi}_{t,\tau}^{-} :=\hat{\phi}_{t}^{-}-\text{se}(\hat{\phi}_{t}^{-})\Phi^{-1}(1-\tau), \]where $\text{se}(\hat{\phi}_{t}^{+}):=\sqrt{\widehat{\text{Var}}(\hat{\phi}_{t}^{+})/n}$ and $\text{se}(\hat{\phi}_{t}^{-}):=\sqrt{\widehat{\text{Var}}(\hat{\phi}_{t}^{-})/n}$ denote the standard errors of $\hat{\phi}_{t}^{+}$ and $\hat{\phi}_{t}^{-}$. The following one-sided covering properties hold: \[ \lim_{n\rightarrow\infty}P(\phi_{t}^{+}\leq\hat{\phi}_{t,1-\tau}^{+})\geq 1-\tau, \lim_{n\rightarrow\infty}P(\phi_{t}^{-}\geq\hat{\phi}_{t,\tau}^{-})\geq 1-\tau. \]Suppose \[ \left\{t\in \boldsymbol{\Theta}_0: \hat{\phi}_{t,1-\tau}^{+}\geq0 \right\}\neq \emptyset, \left\{t\in \boldsymbol{\Theta}_0:\hat{\phi}_{t,\tau}^{-}\leq0\right\}\neq \emptyset. \] If $\theta = \theta_0$, \begin{equation} P\left(\theta_{0}\in\left\{t\in \boldsymbol{\Theta}_0: \hat{\phi}_{t,1-\tau}^{+}\geq0 \right\} \right) \geq 1-\tau, P\left(\theta_{0}\in\left\{t\in \boldsymbol{\Theta}_0:\hat{\phi}_{t,\tau}^{-}\leq0\right\} \right)\geq 1-\tau. \end{equation}

Define \[ \text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]}:=[\hat{\lambda}_{\tau}^{-},\hat{\lambda}_{1-\tau}^{+}],\text{CI}_{1-2\tau}^{[\gamma^{-},\gamma^{+}]}:=[\hat{\gamma}_{\tau}^{-},\hat{\gamma}_{1-\tau}^{+}], \text{CI}_{1-2\tau}^{[\phi_{t}^{-},\phi_{t}^{+}]}:=\left[\hat{\phi}_{t,\tau}^{-},\hat{\phi}_{t,1-\tau}^{+}\right]. \] We then have the following results for coverage probability of the partial identification regions and interested parameters.

theorem\begin{align*} \lim_{n\rightarrow\infty}P(\lambda\inCI_{1-2\tau}^{[\lambda^{-},\lambda^{+}]})\geq\lim_{n\rightarrow\infty}P([\lambda^{-},\lambda^{+}]\inCI_{1-2\tau}^{[\lambda^{-},\lambda^{+}]})\geq 1-2\tau,\\ \lim_{n\rightarrow\infty}P(\gamma\inCI_{1-2\tau}^{[\gamma^{-},\gamma^{+}]})\geq\lim_{n\rightarrow\infty}P([\gamma^{-},\gamma^{+}]\inCI_{1-2\tau}^{[\gamma^{-},\gamma^{+}]})\geq 1-2\tau,\\ \lim_{n\rightarrow\infty}P(\phi_{t}\inCI_{1-2\tau}^{[\phi_{t}^{-},\phi_{t}^{+}]})\geq\lim_{n\rightarrow\infty}P\left(\left[{\phi}_{t}^{-},\phi_{t}^{+}\right]\inCI_{1-2\tau}^{[\phi_{t}^{-},\phi_{t}^{+}]}\right)\geq 1-2\tau. \end{align*}

As the product of the sensitivity parameters satisfies $\zeta_{Y,\alpha}\rightarrow 0$, the interval $\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]}$ converges to the (conventional) $(1-2\tau)$ C.I. for the short version parameter $\lambda_{s}$. Similarly, as $\zeta_{D,\alpha}\rightarrow 0$, $\text{CI}_{1-2\tau}^{[\gamma^{-},\gamma^{+}]}$ converges to the $(1-2\tau)$ C.I. for $\gamma_{s}$. For $\phi_{t}$ and $\theta_0$, assume that \[ \left\{t\in \boldsymbol{\Theta}_0: \hat{\phi}_{t,1-\tau}^{+}\geq0 \right\}\cap \left\{t\in \boldsymbol{\Theta}_0 :\hat{\phi}_{t,\tau}^{-}\leq0\right\}\neq \emptyset. \] Define

equation[equation omitted — 361 chars of source]

When both $\zeta_{Y,\alpha}\rightarrow 0$ and $\zeta_{D,\alpha}\rightarrow 0$ hold, $\text{CI}_{1-2\tau}^{[\phi_{t}^{-},\phi_{t}^{+}]}$ converges to the $(1-2\tau)$ C.I. for $\lambda_{s}-\gamma_{s}t$, and $\left[\hat{\theta}_{0,\tau}^{-},\hat{\theta}_{0,1-\tau}^{+}\right]$ converges to the interval obtained by inverting the positive and negative parts of the $(1-2\tau)$ C.I. for $\lambda_{s}-\gamma_{s}t$.

OVB-Adjusted Confidence Interval for the Interested Parameter

Theorem 4 appears to suggest that $\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]}$, $\text{CI}_{1-2\tau}^{[\gamma^{-},\gamma^{+}]}$ and $\text{CI}_{1-2\tau}^{[\phi_{t}^{-},\phi_{t}^{+}]}$, which provide valid $(1-2\tau)$ coverage for the OVB bounds, can be used directly as ($1-2\tau$) C.I.'s for $\lambda$, $\gamma$ and $\phi_{t}$ after accounting for OVB. However, these OVB-adjusted C.I.'s can be further improved to yield intervals. To illustrate this, we use $\lambda$ as an example (and the relevant results also hold for $\gamma$ and $\phi_{t}$).

Let $\Delta_{\lambda}=\lambda^{+}-\lambda^{-}$ denote the identification region of $\lambda$. In our framework, this is a constant and is not affected by sample size. If $\Delta_{\lambda}$ has a strictly positive length (i.e., $\lambda^{+}>\lambda^{-}$), it can be shown that

align[align omitted — 780 chars of source]

as $n\rightarrow\infty$. Hence \[\lim_{n\rightarrow\infty}P(\lambda\in\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]})\geq1-\tau.\] This result, established in a more general form by IM_2004, implies that a $(1-2\tau)$ C.I. for the OVB bounds $[\lambda^{-},\lambda^{+}]$ can be served as a $(1-\tau)$ C.I. for the true parameter $\lambda$.

The key condition for this result is the strict positivity of $\Delta_{\lambda}$. When $\Delta_{\lambda}$ is strictly positive, the true parameter $\lambda$ cannot be near both the upper bound $\lambda^{+}$ and lower bound $\lambda^{-}$ simultaneously. If $\lambda$ lies strictly inside the bounds, the non-coverage risk converges to zero asymptotically. If $\lambda$ is close to the lower (upper) bound, the risk that it exceeds the upper bound (falls short of the lower bound) is asymptotically negligible. Thus at least one of the second and third terms in ((ref)) vanishes asymptotically, ensuring coverage no smaller than the one-sided case.

However, $\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]}$ is not a uniformly valid $(1-\tau)$ C.I. for $\lambda$ over $\Delta_{\lambda}$. For instance, in the extreme scenario where $\Delta_{\lambda}=0$ (which cannot be ruled out in our case), $\lambda$ is point-identified ($\lambda=\lambda^{+}=\lambda^{-}$) and $\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]}$ reverts to a conventional $(1-2\tau)$ C.I.: $\lim_{n\rightarrow\infty}P(\lambda\in\text{CI}_{1-2\tau}^{[\lambda^{-},\lambda^{+}]})\geq1-2\tau$. That is, the asymptotic non-coverage risk becomes $1-2\tau$, making the C.I. too narrow.

To construct a uniformly valid $(1-\tau)$ OVB-adjusted C.I., we adopt the shrinkage method of Stoye_2009, which ensures that the C.I. is not narrower than the conventional C.I. as $\Delta_{\lambda}$ is close to zero. IM_2004 also provided a method to avoid the above difficulty based on the estimated size of the identification region $\hat{\Delta}_{\lambda}$ (see equation (7) in IM_2004). However, Stoye_2009 pointed out that Imben and Manski's approach implicitly relies on the superefficiency of $\hat{\Delta}_{\lambda}$: the estimation error of $\hat{\Delta}_{\lambda}$ must vanish fast enough (at least with rate $o_{p}(n^{-1/2})$) when $\Delta_{\lambda}$ is near zero. Such a requirement is too restrictive for our proposed DML estimator.

The shrinkage method of Stoye_2009 adjusts the estimator of the identification region and allows the estimation error of $\hat{\Delta}_{\lambda}$ can be with order $O_{p}(n^{-1/2})$. We again use $\lambda$ as an example to illustrate how to use this method to construct the OVB-adjusted C.I. for $\lambda$ as follows. Suppose there exists a sequence $\vartheta_{n}$ such that $\vartheta_{n}\rightarrow0$ and $\sqrt{n}\vartheta_{n}\rightarrow\infty$. Define \[ \hat{\Delta}_{\lambda}^{*}:=

cases\hat{\Delta}_{\lambda}, & if \hat{\Delta}_{\lambda}>\vartheta_{n},\\ 0, & Otherwise,

\] and \[ \hat{\rho}:=\widehat{\text{Corr}}(\hat{\lambda}^{+},\hat{\lambda}^{-})=\frac{\widehat{\text{Cov}}(\hat{\lambda}^{+},\hat{\lambda}^{-})}{\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{+})}\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{-})}}. \]The sequence $\vartheta_{n}$ controls the degree of shrinkage imposed on the initial estimator of the identification region. A slower decay of $\vartheta_{n}$ to zero indicates a less distortion from the shrinkage but a worsen accuracy of using the uniform normal approximation. The critical values for constructing the $(1-\tau)$ OVB-adjusted C.I., denoted by $z_{l}^{*}$ and $z_{u}^{*}$, are obtained from solving the following constrained minimization problem: \[ \min_{z_{l},z_{u}}z_{l}\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{-})}+z_{u}\sqrt{\widehat{\text{Var}}(\hat{\lambda}^{+})} \] subject to

align*[align* omitted — 344 chars of source]

where $(Z_{1},Z_{2})$ are two independent standard normal random variables. Then applying Proposition 3 of Stoye_2009 yields: \[ \lim_{n\rightarrow\infty}P(\lambda\in\text{CI}_{1-\tau}^{\lambda,*})\geq1-\tau, \] where \[ CI_{1-\tau}^{\lambda,*}=

cases\left[\hat{\lambda}^{+}-se(\hat{\lambda}^{-})z_{l}^{*},\hat{\lambda}^{+}+se(\hat{\lambda}^{+})z_{u}^{*}\right], & if \hat{\lambda}^{-}-se(\hat{\lambda}^{-})z_{l}^{*}\leq\hat{\lambda}^{+}+se(\hat{\lambda}^{+})z_{u}^{*},\\ \emptyset, & Otherwise,

\] is the $(1-\tau)$ OVB-adjusted C.I. for $\lambda$. Similar procedures can be applied to construct the $(1-\tau)$ OVB-adjusted C.I. for $\gamma$ and $\phi_{\theta_{0}}$. For $\theta_{0}$, we first can have that for $t\in\boldsymbol{\Theta}_{0}$, \[\lim_{n\rightarrow\infty}P(\phi_{t}\in\text{CI}_{1-\tau}^{\phi_{t},*})\geq1-\tau,\] where \[ CI_{1-\tau}^{\phi_{t},*}=

cases\left[\hat{\phi}_{t}^{-}-se(\hat{\phi}_{t}^{-})z_{l}^{\prime*},\hat{\phi}_{t}^{+}+se(\hat{\phi}_{t}^{+})z_{u}^{\prime*}\right], & if \hat{\phi}_{t}^{-}-se(\hat{\phi}_{t}^{-})z_{l}^{\prime*}\leq\hat{\phi}_{t}^{+}+se(\hat{\phi}_{t}^{+})z_{u}^{\prime*},\\ \emptyset, & Otherwise,

\] and $(z_{l}^{\prime*},z_{u}^{\prime*})$ are the solutions for the corresponding constrained minimization problem of Stoye's shrinkage method for $\phi_{t}$. If $\theta=\theta_{0}$, $\phi_{\theta_{0}}=0$, then we have:

equation[equation omitted — 188 chars of source]

Therefore $(1-\tau)$ OVB-adjusted C.I. for $\theta_{0}$ can be constructed accordingly.

K-Fold Cross-Fitting and the Median Method

In this section, we introduce two methods which can be adopted to further mitigate overfitting bias caused by machine learning estimators: K-fold cross-fitting and the median method CCDDHNR_2018. K-fold cross-fitting uses different parts of samples to repeatedly estimate and predict parameters: $(\lambda_s, \gamma_s,v^{2}_s,\sigma^{2}_{Y_s},\sigma^{2}_{D_s})$, and take an average of the predictions to form the final estimate of the parameter. Let $W_{s,i}=(Z_i,X_i)$ and $V_{s,i}=(Y_{i},D_{i},W_{s,i})$ denote the $i$-th available observation, $i=1,2,\ldots,n$. Below we illustrate the procedures for conducting the K-fold cross fitting on estimating $\theta_s=\lambda_s/\gamma_s$ with estimators based on ((ref)):

enumerate• Randomly split the $n$ samples into $K$ (mutually exclusive) subsamples of equal sample size $n_{k}=n/K$, $k=1,2,\ldots,K$. Let $I_{k}$, $k=1,2,\ldots,K$ denote the set of indices for the $K$ different subsamples. Let $I_{k}^{c}$, $k=1,2,\ldots,K$ denote the complement set of $I_{k}$: $I_{k}^{c}=\left\{ 1,2,\ldots,n\right\} \setminus I_{k}$. • For each $k$, estimate models of the nuisance parameters $\pi_s(X)$, $E[Y|W_s]$ and $E[D|W_s]$ with the available observations $V_{s,i}$, $i\in I_{k}^{c}$. Using the available observations $V_{s,i}$, $i\in I_{k}$ to obtain predictions of the nuisance parameters: $\hat{\pi}_s^{(k)}(X_i)$, $\hat{E}^{(k)}[Y_i|Z_i=1,X_i]$, $\hat{E}^{(k)}[Y_i|Z_i=0,X_i]$, $\hat{E}^{(k)}[D_i|Z_i=1,X_i]$ and $\hat{E}^{(k)}[D_i|Z_i=0,X_i]$. • For each $k$, compute the estimate of $\lambda_s$ and $\gamma_s$ using the predicted nuisance parameters of step 2 as \begin{equation*} \lambda_{s}^{(k)} = \frac{1}{n_{k}}\sum_{i\in I_{k}}\hat{\bar{\psi}}_{\lambda_{s}}^{(k)}(Y_{i},W_{s,i}), \gamma_{s}^{(k)} = \frac{1}{n_{k}}\sum_{i\in I_{k}}\hat{\bar{\psi}}_{\gamma_{s}}^{(k)}(D_i,W_{s,i}), \end{equation*}where \begin{eqnarray*} \hat{\bar{\psi}}_{\lambda_{s}}^{(k)}(Y_{i},W_{s,i}) & = & \frac{Z_{i}}{\hat{\pi}_{s}^{(k)}(X_{i})}(Y_{i}-\hat{E}^{(k)}[Y_{i}|Z_{i}=1,X_{i}])-\frac{1-Z_{i}}{1-\hat{\pi}_{s}^{(k)}(X_{i})}(Y_{i}-\hat{E}^{(k)}[Y_{i}|Z_{i}=0,X_{i}])+\\ & & \hat{E}^{(k)}[Y_{i}|Z_{i}=1,X_{i}]-\hat{E}^{(k)}[Y_{i}|Z_{i}=0,X_{i}],\\ \hat{\bar{\psi}}_{\gamma_{s}}^{(k)}(D_i,W_{s,i}) & = & \frac{Z_{i}}{\hat{\pi}_{s}^{(k)}(X_{i})}(D_{i}-\hat{E}^{(k)}[D_{i}|Z_{i}=1,X_{i}])-\frac{1-Z_{i}}{1-\hat{\pi}_{s}^{(k)}(X_{i})}(D_{i}-\hat{E}^{(k)}[D_{i}|Z_{i}=0,X_{i}])+\\ & & \hat{E}^{(k)}[D_{i}|Z_{i}=1,X_{i}]-\hat{E}^{(k)}[D_{i}|Z_{i}=0,X_{i}]. \end{eqnarray*} • Average $\hat{\lambda}_{s}^{(k)}$ and $\hat{\gamma}_{s}^{(k)}$ over $k=1,2,\ldots,K$ to obtain the estimates of $\lambda_s$ and $\gamma_s$: \[\hat{\lambda}_s=\frac{1}{K}\sum_{k=1}^{K}\hat{\lambda}_{s}^{(k)}, \hat{\gamma}_s=\frac{1}{K}\sum_{k=1}^{K}\hat{\gamma}_{s}^{(k)}.\]The estimate of $\theta_s$ is: \begin{equation} \hat{\theta}_s = \frac{\hat{\lambda}_s}{\hat{\gamma}_s}. \end{equation}

$\hat{\theta}_{s}$ in ((ref)) is referred to as DML2 estimator in CCDDHNR_2018 and is the equivalent to solving $\theta_{s}$ in the following equation: \[\frac{1}{K}\sum_{k=1}^{K}\left[\frac{1}{n_{k}}\sum_{i\in I_{k}}\hat{\bar{\psi}}_{\theta_{s}}^{(k)}(Y_{i},D_{i},W_{s,i})\right]=0,\]where \[\hat{\bar{\psi}}_{\theta_{s}}^{(k)}(Y_{i},D_{i},W_{s,i})=\hat{\bar{\psi}}_{\lambda_{s}}^{(k)}(Y_{i},W_{s,i})-\hat{\bar{\psi}}_{\gamma_{s}}^{(k)}(D_{i},W_{s,i})\theta_{s}.\]Alternatively, we may estimate $\theta_{s}$ by using DML1 estimator: $\hat{\theta}_{s}^{\prime}=1/K\sum_{k=1}^{K}\hat{\lambda}_{s}^{(k)}/\hat{\gamma}_{s}^{(k)}$, that is, taking an average of $\hat{\lambda}_{s}^{(k)}/\hat{\gamma}_{s}^{(k)}$, $k=1,\ldots,K$. In practice, DML2 estimator is more preferred than DML1 estimator, since the former generally has a more stable property than the latter and therefore demonstrates a better performance empirically CCDDHNR_2018.

Furthermore, to avoid uncertainty from sample splitting in the K-fold cross-fitting, we adopt the median method suggested in CCDDHNR_2018 to improve stability of our final estimates of $(\lambda_{s},\gamma_{s},v_{s}^{2},\sigma_{Y_{s}}^{2},\sigma_{D_{s}}^{2})$. To implement the median method, we first repeat the procedures of the K-fold cross-fitting $L$ times. Let $\hat{\boldsymbol{\xi}}^{l}$ denote a vector of the estimated parameters and $\hat{\mathbf{\Sigma}}^{l}$ denote the estimated approximate covariance matrix of $\sqrt{n}(\hat{\boldsymbol{\xi}}^{l}-\boldsymbol{\xi})$ (i.e., $\boldsymbol{\Omega}$ in Theorem 2), from the $l$th K-fold cross-fitting, $l=1,\ldots,L$. We use

equation[equation omitted — 124 chars of source]

as the final estimate of the parameters and

equation[equation omitted — 270 chars of source]

as the final estimate of the approximate covariance matrix.\footnote{The “Median” in ((ref)) chooses the median among the $L$ cross fittings for each of the estimated parameters , while in ((ref)), it chooses the matrix with median operator norm.}

Empirical Application with the JTPA Data

In this section, we demonstrate the usefulness of our proposed method for quantifying the OVB in nonlinear IV estimators through an empirical application. We perform an OVB analysis for LATE and LATT estimations in Title II programs of the Job Training Partnership Act (JTPA) in the US. The data consist of adult male and female workers who participated in these programs between November 1987 and September 1989. Following AAI_2002, we assume the observations are i.i.d. for estimation purposes. The outcome variable $Y$ is the total earnings in the 30 months. The treatment variable $D$ is a binary variable for enrollment in the JTPA services (1 = enrolled; 0 = not enrolled), while the instrumental variable $Z$ indicates whether the individual was offered such services (1 = offered; 0 = not offered). The exogenous covariates include age (age), which is a categorical variable, as well as a set of dummy variables: black (black), Hispanic (hispanic), high-school graduates (hsorged, including GED holders), marital status (married), AFDC receipt (adfc, for adult female workers only), whether the applicant worked at least 12 weeks in the 12 months preceding random assignment (\texttt{wkless13}), the original recommended service strategy: classroom training (\texttt{class_tr}), and OJT/JSA/other (\texttt{ojt_jsa}), and whether earnings data were from the second follow-up survey (\texttt{f2sms}). The total sample size is 11,204 (5,102 males and 6,102 females).

Although offers for the JTPA services were randomly assigned, only approximately 60% of those offered the services actually enrolled AAI_2002. This partial compliance raises potential endogeneity concerns, as treatment status may be self-selected and correlated with the potential outcomes. Since the offers were randomly assigned and were considered to likely influence participants' intention to enroll in the program, we use the offer assignment as the instrumental variable. While some individuals received services without being assigned, AAI_2002 note that this violation was rare (less than 2%) and thus unlikely to materially affect our estimates.

For LATE, Figure (ref) and (ref) present sensitivity contour plots for the lower bounds of the 97.5% confidence intervals (C.I.s) for $\lambda^{-}$ (left panel) and $\gamma^{-}$ (right panel) assuming $|\rho_Y|=|\rho_D|=1$. Figure (ref) corresponds to male workers and Figure (ref) to female workers. Each contour line shows the lower bound of the 97.5% C.I. when the product of $C_YC_{\alpha}$ (or $C_DC_{\alpha}$) equals to a specific value. For instance, consider the case of male workers. When $C_YC_{\alpha}$=4.55e-3 (i.e., $C_Y=0.1$ and $C_{\alpha} = 0.0455$), the contour line indicates that the lower bound of the 97.5% confidence interval for $\lambda^{-}$ roughly equals to -300.

The sensitivity parameters $C_Y C_{\alpha}$ and $C_D C_{\alpha}$ have a negative impact on the lower bounds of the C.I.s for $\lambda^{-}$ and $\gamma^{-}$. For the male workers, when $C_YC_{\alpha}=0$ (either $C_Y=0$ or $C_{\alpha} = 0$, or both), the lower bound is -114.99, suggesting that even without considering the OVB, the (short) estimate of $\lambda$ (ITT) is not statistically significant at the 5% level. In fact, the value for $C_Y C_{\alpha}$ to push the lower bound below zero is a slightly negative (roughly equals to -0.003), which is not feasible, since $C_Y C_{\alpha}$ is required to be nonnegative. For female workers, the corresponding threshold for $C_Y C_{\alpha}$ roughly equal to 0.019. In contrast, for $\gamma^{-}$, as shown in the right panels of Figures (ref) and (ref), the thresholds are much less stringent than those for $\lambda^{-}$. For both male and female workers, the criteria both exceed 0.65, indicating that estimates of $\gamma$ ($P(T=C)$) are much robust to the omitted variables compared to the estimates of $\lambda$ (ITT).

We next turn to the results of LATE estimation when considering the OVB. These results are obtained using the calibrated sensitivity parameters $C_{\alpha}$, $C_Y$ and $C_D$. To determine the calibrated value, we first estimate the sensitivity parameter separately for each covariate using the method introduced in the benchmarking analysis. We set the relative strength indicator $k_{\alpha} =k_Y= k_D = 1$, which implies that the omitted variable is assumed to be at least as important as any excluded covariate $X_j$ in predicting $(Y,D,Z)$, given the remaining covariates $X_{-j}$. In addition, we set $|\rho_Y| = |\rho_D| = 1$, which yields the maximal values of the estimated sensitivity parameters. Then the largest among these estimates is selected as the calibrated value of the sensitivity parameter. This maximum estimate (calibrated value of the sensitivity parameter) and associated covariate (denoted by $X_j^{*}$) are reported in Table (ref).\footnote{Here, the variable age represents all age-related categorical variables.} For LATE, the results indicate that if the omitted variable is as important as $X_j^{*}$, including it would enhance prediction precision for $Z$ by 1.9% ($0.138^2$) among male workers and 0.62% ($0.079^2$) among female workers. In the case of male workers, the reduction in MSE when predicting $Y$ and $D$ would be 2.2% and 0.18%, while for female workers, the corresponding reductions are 3.2% and 0.35%. Overall, the estimated influence of the omitted variable on the prediction of $(Y,D,Z)$ appears to be small in the case of LATE estimation.

The first three columns of Table (ref) present short estimates (those estimated with the available data) and their corresponding 95% C.I.s, and estimates of the OVB bounds for the parameters. Estimates of the OVB bounds for $\lambda$ and $\gamma$ are estimates of $(\lambda^{+},\lambda^{-})$ and $(\gamma^{+},\gamma^{-})$, while estimates of the OVB bounds for $\theta$ are estimates obtained from using the derived result in Theorem 1. From the table, the short estimates of $\gamma$ ($P(T=C)$) are statistically significant at the 5% level for both male and female workers. However, the significance of $\lambda$ (ITT) and $\theta$ (LATE) differs by gender: for female workers, both estimates remain statistically significant at the 5% level, while for male workers, they do not. When accounting for the OVB based on the calibrated sensitivity parameters, estimates of the OVB bounds suggest that the true LATE for the male workers lies within the range of 317 to 3,044 U.S. dollars, and for the female workers, the range is within 1,279 to 2,531 U.S. dollars.

The last column shows the estimated bounds $[\hat{\theta}^{-}_{0,\tau},\hat{\theta}^{+}_{0,1-\tau}]$ in ((ref)), $[\hat{\lambda}^{-}_{\tau},\hat{\lambda}^{+}_{1-\tau}]$ in ((ref)) and $[\hat{\gamma}^{-}_{\tau},\hat{\gamma}^{+}_{1-\tau}]$ in ((ref)) with $\tau = 0.025$, which are denoted by $\text{Low}_{0.025}$ and $\text{Up}_{0.975}$ in the table. Through Figure (ref), we illustrate how to practically use ((ref)) to obtain $[\hat{\theta}^{-}_{0,\tau},\hat{\theta}^{+}_{0,1-\tau}]$. Figure (ref) plots the estimated functions $\hat{\phi}_{t,0.975}^{+}$ and $\hat{\phi}_{t,0.025}^{-}$ over different values of $t$ based on the calibrated sensitivity parameters. Each function is segmented into two parts: one for $t\geq 0$ (solid line) and one for $t<0$ (dashed line). The two estimated functions are generally continuous in $t$ but not differentiable at $t=0$. Within the selected range of $t$ in the plots, both segments of the estimated functions decrease monotonically.

For the male workers, the plot shows that $\hat{\phi}_{t,0.975}^{+}\geq0$ if $t\leq4,916.2$, and $\hat{\phi}_{t,0.025}^{-}\leq0$ if $t\geq-1,551.26$. According to ((ref)), this implies that $[\hat{\theta}^{-}_{0,0.025},\hat{\theta}^{+}_{0,0.975}]= [-1,551.26, 4,916.20]$. For the female workers, applying the same logic yields $[\hat{\theta}^{-}_{0,0.025},\hat{\theta}^{+}_{0,0.975}]= [198.50, 3,625.84]$ based on the corresponding calibrated sensitivity parameters. From the results, it can be seen that as the uncertainty associated with OVB bound estimation is incorporated, the statistical significance results are align with those based on the point estimates. In particular, for female workers, the statistical significance of LATE (and ITT) estimate remains robustly stand after accounting for the OVB and uncertainty of the estimation.

For LATT, the relevant results are shown in Table (ref) and (ref) and Figure (ref) to (ref). The results are qualitatively similar as those for LATE. Specifically, the estimates of $\gamma$ are much robust to the omitted variables than the estimates of $\lambda$. For male workers, the threshold for $C_Y C_{\alpha}$ that brings the lower bound below zero roughly equals to -0.004. For female workers, the corresponding threshold is approximately 0.02. In contrast, the thresholds for $\gamma^{-}$, shown in the right panels of Figures (ref) and (ref), are much less stringent than those for $\lambda^{-}$. For both male and female workers, these thresholds are above 0.64, reinforcing the robustness of the estimated $\gamma$ to the omitted variables. Results of the OVB-adjusted estimates are again align with those of the point estimates. Importantly, the statistical significance of both $\lambda$ and LATT estimates for the female workers remains robust even after accounting for both the OVB and uncertainty in the estimation of its bounds.

Statistical Significance after Accounting for the OVB

Table (ref) to (ref) present the results for the $(1-\tau)$ OVB-adjusted confidence intervals for LATE and LATT constructed using the shrinkage method of Stoye_2009. We set the significance level $\tau=0.05$ (i.e., 95% C.I.) and the shrinkage factor as

equation[equation omitted — 137 chars of source]

where $\hat{\sigma}_{l}$ and $\hat{\sigma}_{u}$ denote the estimated standard deviations of the lower and upper OVB bounds. The shrinkage factor ((ref)) is the one (from the iterated law of logarithm) suggested in Stoye_2009, scaled by $\max\{\hat{\sigma}_{l},\hat{\sigma}_{u}\}$.

For $\lambda$ and $\gamma$, $(z_{l}^{*},z_{u}^{*})$ denote the critical values, $\hat{\Delta}^{*}$ denote the estimate of the identification region, and Min.Obj. denote the minimum value of the constrained minimization for Stoye's shrinkage method. To construct the $(1-\tau)$ OVB-adjusted C.I. for $\theta_{0}$ (LATE or LATT), we first compute $\text{C.I.}_{1-\tau}^{\phi_{t},*}$ for $t$ over a specified range, and then obtain the upper and lower bounds of the C.I. by inverting ((ref)). For $\theta_{0}$, the reported values of $(z_{l}^{*},z_{u}^{*})$, $\hat{\Delta}^{*}$ and Min.Obj. correspond to those for $\phi_{t}$, averaged over different values of $t$. Figure (ref) and (ref) show plots of the upper and lower bounds of $\text{C.I.}_{1-\tau}^{\phi_{t},*}$ as functions of $t$ for LATE and LATT.

From the two tables, we observe that at the 95% level, the statistical significance of $\theta_{0}$, $\lambda$ and $\gamma$ after accounting for OVB is qualitatively similar to the results obtained without OVB adjustment (i.e., the short estimates). For $\theta_{0}$ and $\lambda$, the 95% OVB-adjusted C.I.'s are narrower than the intervals $[\text{Low}_{0.025},\text{Up}_{0.975}]$ shown in previous tables. This is due to relatively large estimates of the identification regions for $\phi_{t}$ and $\lambda$, which lead to lower (one-sided) critical values. In our settings, the critical values used are almost equal to 1.645 or 1.96, corresponding to the 95% or 97.5% quantile of the standard normal distribution. This occurs because for each of $\phi_{t}$, $\lambda$ and $\gamma$, the estimated correlation between the estimated upper and lower OVB bounds is very close to one. As shown in Stoye_2009, in such a situation, the solved critical values for the $(1-\tau)$ OVB-adjusted C.I. are very close to $(1-\tau)$ (or $(1-2\tau)$) quantile of the standard normal distribution.

Conclusion

This paper develops a general framework for quantifying omitted variable bias (OVB) in nonlinear instrumental variable (IV) estimators. Extending the recent work of CCNSS_2024, we analyze a class of estimators — including the local average treatment effect (LATE), LATE on the treated (LATT), and the partially linear IV model (PLIVM) — that can be expressed as ratios of reduced-form and first-stage parameters. We derive bias decompositions for these parameters, establish partial identification bounds for the structural estimand, and construct statistical inference procedures that yield OVB-adjusted confidence intervals. Estimation is conducted via double machine learning and the median method CCDDHNR_2018. An empirical application to the U.S. Job Training Partnership Act (JTPA) experiment shows that estimates of the first-stage probability of compliance are robust to omitted variables, while intention-to-treat and treatment effect estimates are more sensitive. Specifically, female participants exhibit robust and statistically significant program impacts, whereas effects for males become fragile once OVB is or nor accounted for. Overall, this study provides a unified framework for sensitivity analysis of nonlinear IV estimators and offers practical tools for assessing the robustness of causal conclusions in applied research.