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The Taylor Rule and Interval Forecast for Exchange Rates

Jian Wang and Jason J. Wu*

NOTE: International Finance Discussion Papers are preliminary materials circulated to stimulate discussion and critical comment. References in publications to International Finance Discussion Papers (other than an acknowledgment that the writer has had access to unpublished material) should be cleared with the author or authors. Recent IFDPs are available on the Web at http://www.federalreserve.gov/pubs/ifdp/. This paper can be downloaded without charge from the Social Science Research Network electronic library at http://www.ssrn.com/.


Abstract:

This paper attacks the Meese-Rogoff (exchange rate disconnect) puzzle from a different perspective: out-of-sample interval forecasting. Most studies in the literature focus on point forecasts. In this paper, we apply Robust Semi-parametric (RS) interval forecasting to a group of Taylor rule models. Forecast intervals for twelve OECD exchange rates are generated and modified tests of Giacomini and White (2006) are conducted to compare the performance of Taylor rule models and the random walk. Our contribution is twofold. First, we find that in general, Taylor rule models generate tighter forecast intervals than the random walk, given that their intervals cover out-of-sample exchange rate realizations equally well. This result is more pronounced at longer horizons. Our results suggest a connection between exchange rates and economic fundamentals: economic variables contain information useful in forecasting the distributions of exchange rates. The benchmark Taylor rule model is also found to perform better than the monetary and PPP models. Second, the inference framework proposed in this paper for forecast-interval evaluation, can be applied in a broader context, such as inflation forecasting, not just to the models and interval forecasting methods used in this paper.

Keywords: Exchange rate disconnect puzzle, exchange rate forecast, interval forecasting

JEL classification: F31, C14, C53


1.  Introduction

Recent studies explore the role of monetary policy rules, such as Taylor rules, in exchange rate determination. They find empirical support in these models for the linkage between exchange rates and economic fundamentals. Our paper extends this literature from a different perspective: interval forecasting. We find that the Taylor rule models can outperform the random walk, especially at long horizons, in forecasting twelve OECD exchange rates based on relevant out-of-sample interval forecasting criteria. The benchmark Taylor rule model is also found to perform relatively better than the standard monetary model and the purchasing power parity (PPP) model.

In a seminal paper, Meese and Rogoff (1983) find that economic fundamentals - such as the money supply, trade balance and national income - are of little use in forecasting exchange rates. They show that existing models cannot forecast exchange rates better than the random walk in terms of out-of-sample forecasting accuracy. This finding suggests that exchange rates may be determined by something purely random rather than economic fundamentals. Meese and Rogoff's (1983) finding has been named the Meese-Rogoff puzzle in the literature.

In defending fundamental-based exchange rate models, various combinations of economic variables and econometric methods have been used in attempts to overturn Meese and Rogoff's finding. For instance, Mark (1995) finds greater exchange rate predictability at longer horizons.1Groen (2000) and Mark and Sul (2001) detect exchange rate predictability by using panel data. Kilian and Taylor (2003) find that exchange rates can be predicted from economic models at horizons of 2 to 3 years after taking into account the possibility of nonlinear exchange rate dynamics. Faust, Rogers, and Wright (2003) find that the economic models consistently perform better using real-time data than revised data, though they do not perform better than the random walk.

Recently, there is a growing strand of literature that uses Taylor rules to model exchange rate determination. Engel and West (2005) derive the exchange rate as present-value asset price from a Taylor rule model. They also find a positive correlation between the model-based exchange rate and the actual real exchange rate between the US dollar and the Deutschmark (Engel and West, 2006). Mark (2007) examines the role of Taylor-rule fundamentals for exchange rate determination in a model with learning. In his model, agents use least-square learning rules to acquire information about the numerical values of the model's coefficients. He finds that the model is able to capture six major swings of the real Deutschemark-Dollar exchange rate from 1973 to 2005. Molodtsova and Papell (2008) find significant short-term out-of-sample predictability of exchange rates with Taylor-rule fundamentals for 11 out of 12 currencies vis-á-vis the U.S. dollar over the post-Bretton Woods period. Molodtsova, Nikolsko-Rzhevskyy, and Papell (2008) find evidence of out-of-sample predictability for the dollar/mark nominal exchange rate with forecasts based on Taylor rule fundamentals using real-time data, but not revised data.

Our paper joins the above literature of Taylor-rule exchange rate models. However, we addresses the Meese and Rogoff puzzle from a different perspective: interval forecasting. A forecast interval captures not only the expected future value of the exchange rate, but a range in which the exchange rate may lie with a certain probability, given a set of predictors available at the time of forecast. Our contribution to the literature is twofold. First, we find that for twelve OECD exchange rates, the Taylor rule models in general generate tighter forecast intervals than the random walk, given that their intervals cover the realized exchange rates (statistically) equally well. This finding suggests an intuitive connection between exchange rates and economic fundamentals beyond point forecasting: the use of economic variables as predictors help narrow down the range in which future exchange rates may lie, compared to random walk forecast intervals which are essentially based on unconditional distributions of exchange rates. Second, we propose an inference framework for cross-model comparison of out-of-sample forecast intervals. The proposed framework can be used for forecast-interval evaluation in a broader context, not just for the models and methods used in this paper. For instance, the framework can also be used to evaluate out-of-sample inflation forecasting.

As we will discuss later, we in fact derive forecast intervals from estimates of the distribution of changes in the exchange rate. Hence, in principle, evaluations across models can be done based on distributions instead of forecast intervals. However, focusing on interval forecasting performance allows us to compare models in two dimensions that are more relevant to practitioners: empirical coverage and length.

While the literature on interval forecasting for exchange rates is sparse, several authors have studied out-of-sample exchange rate density forecasts, from which interval forecasts can be derived. Diebold, Hahn and Tay (1999) use the RiskMetrics model of JP Morgan (1996) to compute half-hour-ahead density forecasts for Deutschmark/Dollar and Yen/Dollar returns. Christoffersen and Mazzotta (2005) provide option-implied one-day-ahead density and interval forecasts for four major exchange rates. Boero and Marrocu (2004) obtain one-day-ahead density forecasts for the Euro nominal effective exchange rate using the self-exciting threshold autoregressive (SETAR) models. Sarno and Valente (2005) evaluate the exchange rate density forecasting performance of the Markov-switching vector equilibrium correction model that is developed by Clarida, Sarno, Taylor and Valente (2003). They find that information from the term structure of forward premia help the model to outperform the random walk in forecasting the out-of-sample densities of the spot exchange rate. More recently, Hong, Li and Zhao (2007) construct half-hour-ahead density forecasts for Euro/Dollar and Yen/Dollar exchange rates using a comprehensive set of univariate time series models that capture fat tails, time-varying volatility and regime switches.

There are several common features across the studies listed above, which make them different from our paper. First, the focus of the above studies is not to make connections between the exchange rate and economic fundamentals. These studies use high frequency data, which are not available for most conventional economic fundamentals. For instance, Diebold, Hahn and Tay (1999) and Hong, Li and Zhao (2007) use intra-day data. With the exception of Sarno and Valente (2005), all the studies focus only on univariate time series models. Second, these studies do not consider multi-horizon-ahead forecasts, perhaps due to the fact that their models are often highly nonlinear. Iterating nonlinear density models multiple horizons ahead is analytically difficult, if not infeasible. Lastly, the above studies assume that the densities are analytically defined for a given model. The semi-parametric method used in this paper does not impose such restrictions.

Our choice of semi-parametric method is motivated by the difficulty of using macroeconomic models in exchange rate interval forecasting: these models typically do not describe the future distributions of exchange rates. For instance, the Taylor rule models considered in this paper do not describe any features of the data beyond the conditional means of future exchange rates. We address this difficulty by applying Robust Semi-parametric forecast intervals (from hereon RS forecast intervals) of Wu (2007).2 This method is useful since it does not require the model be correctly specified, or contain parametric assumptions about the future distribution of exchange rates.

We apply RS forecast intervals to a set of Taylor rule models that differ in terms of the assumptions on policy and interest rate smoothing rules. Following Molodtsova and Papell (2008), we include twelve OECD exchange rates (relative to the US dollar) over the post-Bretton Woods period in our dataset. For these twelve exchange rates, the out-of-sample RS forecast intervals at different forecast horizons are generated from the Taylor rule models and then compared with those of the random walk. The empirical coverages and lengths of forecast intervals are used as the evaluation criteria. Our empirical coverage and length tests are modified from Giacomini and White's (2006) predictive accuracy tests in the case of rolling but fixed-size estimation samples.

For a given nominal coverage (probability), the empirical coverage of forecast intervals derived from a forecasting model is the probability that the out-of-sample realizations (exchange rates) lie in the intervals. The length of the intervals is a measure of its tightness: the distance between its upper and lower bound. In general, the empirical coverage is not the same as its nominal coverage. Significantly missing the nominal coverage indicates poor quality of the model and intervals. One certainly wants the forecast intervals to contain out-of-sample realizations as close as possible to the probability they target. Most evaluation methods in the literature focus on comparing empirical coverages across models, following the seminal work of Christoffersen (1998). Following this literature, we first test whether forecast intervals of the Taylor rule models and the random walk have equally accurate empirical coverages. The model with more accurate coverages is considered the better model. In the cases where equal coverage accuracy cannot be rejected, we further test whether the lengths of forecast intervals are the same. The model with tighter forecast intervals provides more useful information about future values of the data, and hence is considered as a more useful forecasting model.

It is also important to establish what this paper is not attempting. First, the inference procedure does not carry the purpose of finding the correct model specification. Rather, inference is on how useful models are in generating forecast intervals, measured in terms of empirical coverages and lengths. Second, this paper does not consider the possibility that there might be alternatives to RS forecast intervals for the exchange rate models we consider. Some models might perform better if parametric distribution assumptions (e.g. the forecast errors are conditionally heteroskedastic and $ t-$distributed) or other assumptions (e.g. the forecast errors are independent of the predictors) are added. One could presumably estimate the forecast intervals differently based on the same models, and then compare those with the RS forecast intervals, but this is out of the scope of this paper. As we described, we choose RS method for its robustness and flexibility achieved by the semi-parametric approach.

Our benchmark Taylor rule model is from Engel and West (2005) and Engel, Wang, and Wu (2008). For the purpose of comparison, several alternative Taylor rule models are also considered. These setups have been studied by Molodtsova and Papell (2008) and Engel, Mark, and West (2007). In general, we find that the Taylor rule models perform better than the random walk model, especially at long horizons: the models either have more accurate empirical coverages than the random walk, or in cases of equal coverage accuracy, the models have tighter forecast intervals than the random walk. The evidence of exchange rate predictability is much weaker in coverage tests than in length tests. In most cases, the Taylor rule models and the random walk have statistically equally accurate empirical coverages. So, under the conventional coverage test, the random walk model and the Taylor rule models perform equally well. However, the results of length tests suggest that Taylor rule fundamentals are useful in generating tighter forecasts intervals without losing accuracy in empirical coverages.

We also consider two other popular models in the literature: the monetary model and the model of purchasing power parity (PPP). Based on the same criteria, both models are found to perform better than the random walk in interval forecasting. As with the Taylor rule models, most evidence of exchange rate predictability comes from the length test: economic models have tighter forecast intervals than the random walk given statistically equivalent coverage accuracy. The monetary model performs slightly worse than the benchmark Taylor rule model and the PPP model. The benchmark Taylor rule model performs better than the PPP model at short horizons and equally well at long horizons.

Our findings suggest that exchange rate movements are linked to economic fundamentals. However, we acknowledge that the Meese-Rogoff puzzle remains difficult to understand. Although Taylor rule models offer statistically significant length reductions over the random walk, the reduction of length is quantitatively small. Forecasting exchange rates remains a difficult task in practice. There are some impressive advances in the literature, but most empirical findings remain fragile. As mentioned in Cheung, Chinn, and Pascual (2005), forecasts from economic fundamentals may work well for some currencies during certain sample periods but not for other currencies or sample periods. Engel, Mark, and West (2007) recently show that a relatively robust finding is that exchange rates are more predictable at longer horizons, especially when using panel data. We find greater predictability at longer horizons in our exercise. It would be of interest to investigate connections between our findings and theirs.

Several recent studies have attacked the puzzle from a different angle: there are reasons that economic fundamentals cannot forecast the exchange rate, even if the exchange rate is determined by these fundamentals. Engel and West (2005) show that existing exchange rate models can be written in a present-value asset-pricing format. In these models, exchange rates are determined not only by current fundamentals but also by expectations of what the fundamentals will be in the future. When the discount factor is large (close to one), current fundamentals receive very little weight in determining the exchange rate. Not surprisingly, the fundamentals are not very useful in forecasting. Nason and Rogers (2008) generalize the Engel-West theorem to a class of open-economy dynamic stochastic general equilibrium (DSGE) models. Other factors such as parameter instability and mis-specification (for instance, Rossi 2005) may also play important roles in understanding the puzzle. It is interesting to investigate conditions under which we can reconcile our findings with these studies.

The remainder of this paper is organized as follows. Section two describes the forecasting models we use, as well as the data. In section three, we illustrate how the RS forecast intervals are constructed from a given model. We also propose loss criteria to evaluate the quality of the forecast intervals, and test statistics that are based on Giacomini and White (2006). Section four presents results of out-of-sample forecast evaluation. Finally, section five contains concluding remarks.


2.  Models and Data

Seven models are considered in this paper. Let $ m=1,2,...,7$ be the index of these models and the first model be the benchmark model. A general setup of the models takes the form of

$\displaystyle s_{t+h}-s_{t}=\alpha_{m,h}+\beta^{\prime}_{m,h}\mathbf{X}_{m,t}+\varepsilon _{m,t+h},$ (1)

where $ s_{t+h}-s_{t}$ is $ h$-period changes of the (log) exchange rate, and $ \mathbf{X}_{m,t}$ contains economic variables that are used in model $ m$. Following the literature of long-horizon regressions, both short- and long-horizon forecasts are considered. Models differ in economic variables that are included in matrix $ \mathbf{X}_{m,t}$. In the benchmark model,

$\displaystyle \mathbf{X}_{1,t}\equiv\left[ \begin{array}[c]{ccc} \pi_{t}-\pi_{t}^{\ast} & y_{t}^{gap}-y_{t}^{gap\ast} & q_{t}\\ & & \end{array} \right] ,$    

where $ \pi_{t}$ ( $ \pi_{t}^{\ast}$) is the inflation rate, and $ y_{t}^{gap}$ ( $ y_{t}^{gap\ast}$) is output gap in the home (foreign) country. The real exchange rate $ q_{t}$ is defined as $ q_{t}\equiv s_{t}+p_{t}^{\ast}-p_{t}$, where $ p_{t}$ ( $ p_{t}^{\ast}$) is the (log) consumer price index in the home (foreign) country. This setup is motivated by the Taylor rule model in Engel and West (2005) and Engel, Wang, and Wu (2008). The next subsection describes this benchmark Taylor rule model in detail.

We also consider the following models that have been studied in the literature:

  • Model 2:
  • : \begin{displaymath}\mathbf{X}_{2,t}\equiv\left[ \begin{array}[c]{cc} \pi_{t}-\pi_{t}^{\ast} & y_{t}^{gap}-y_{t}^{gap\ast}\ & \end{array}\right] \end{displaymath}
  • Model 3:
  • : \begin{displaymath}\mathbf{X}_{3,t}\equiv\left[ \begin{array}[c]{ccc} \pi_{t}-\pi_{t}^{\ast} & y_{t}^{gap}-y_{t}^{gap\ast} & i_{t-1}-i_{t-1}^{\ast }\ & & \end{array}\right] \end{displaymath} ,

    where $ i_{t}$ ( $ i_{t}^{\ast}$) is the short-term interest rate in the home (foreign) country.

  • Model 4:
  • : \begin{displaymath}\mathbf{X}_{4,t}\equiv\left[ \begin{array}[c]{cccc} \pi_{t}-\pi_{t}^{\ast} & y_{t}^{gap}-y_{t}^{gap\ast} & q_{t} & i_{t-1} -i_{t-1}^{\ast}\ & & & \end{array}\right] \end{displaymath}
  • Model 5:
  • : $ \mathbf{X}_{5,t}\equiv q_{t}$
  • Model 6:
  • : \begin{displaymath}\mathbf{X}_{6,t}\equiv\left[ \begin{array}[c]{c} s_{t}-\left[ (m_{t}-m_{t}^{\ast})-(y_{t}-y_{t}^{\ast})\right] \ \end{array}\right] \end{displaymath},

    where $ m_{t}$ ( $ m_{t}^{\ast}$) is the money supply and $ y_{t}$ ( $ y_{t}^{\ast}$)

    is total output in the home (foreign) country.

     

  • Model 7:
  • : $ \mathbf{X}_{7,t}\equiv0$

    Models 2-4 are the Taylor rule models studied in Molodtsova and Papell (2008). Model 2 can be considered as the constrained benchmark model in which PPP always holds. Molodtsova and Papell (2008) include interest rate lags in models 3 and 4 to take into account potential interest rate smoothing rules of the central bank. Model 5 is the purchasing power parity (PPP) model and model 6 is the monetary model. Both models have been widely used in the literature. See Molodtsova and Papell (2008) for the PPP model and Mark (1995) for the monetary model. Model 7 is the driftless random walk model ( $ \alpha _{7,h}\equiv0$).3 Given a date $ \tau$ and horizon $ h$, the objective is to estimate the forecast distribution of $ s_{\tau+h}-s_{\tau}$ conditional on $ \mathbf{X}_{m,\tau}$, and subsequently build forecast intervals from the estimated forecast distribution. Before moving to the econometric method, we first describe the Taylor rule model that motivates the setup of our benchmark model.

    2.1  Benchmark Taylor Rule Model

    Our benchmark model is the Taylor rule model that is derived in Engel and West (2005) and Engel, Wang, and Wu (2008). Following Molodtsova and Papell (2008), we focus on models that depend only on current levels of inflation and output gap.4 The Taylor rule in the home country takes the form of

    $\displaystyle \bar{i}_{t}=\bar{i}+\delta_{\pi}(\pi_{t}-\bar{\pi})+\delta_{y}y_{t} ^{gap}+u_{t},$ (2)

    where $ \bar{i}_{t}$ is the central bank's target for short-term interest rate at time $ t$, $ \bar{i}$ is the equilibrium long-run rate, $ \pi_{t}$ is the inflation rate, $ \bar{\pi}$ is the target inflation rate, and $ y_{t}^{gap}$ is output gap. The foreign country is assumed to follow a symmetric Taylor rule. In addition, we follow Engel and West (2005) to assume that the foreign country targets the exchange rate in its Taylor rule:

    $\displaystyle \bar{i}_{t}^{\ast}=\bar{i}+\delta_{\pi}(\pi_{t}^{\ast}-\bar{\pi})+\delta _{y}y_{t}^{gap\ast}+\delta_{s}(s_{t}-\bar{s}_{t})+u_{t}^{\ast} ,$ (3)

    where $ \bar{s}_{t}$ is the targeted exchange rate. Assume that the foreign country targets the PPP level of the exchange rate: $ \bar{s}_{t}=p_{t} -p_{t}^{\ast}$, where $ p_{t}$ and $ p_{t}^{\ast}$ are logarithms of the home and foreign aggregate prices. In equation (3), we assume that the policy parameters take the same values in the home and foreign countries. To simplify our presentation, we assume that the home and foreign countries have the same long-run inflation and interest rates. Such restrictions have been relaxed in our econometric model after we include a constant term in estimations.

    We do not consider interest rate smoothing in our benchmark model. That is, the actual interest rate ($ i_{t}$) is identical to the target rate in the benchmark model:

    $\displaystyle i_{t}=\bar{i}_{t}.$ (4)

    Molodtsova and Papell (2008) consider the following interest rate smoothing rule:

    $\displaystyle i_{t}=(1-\rho)\bar{i}_{t}+\rho i_{t-1}+\nu_{t},$ (5)

    where $ \rho$ is the interest rate smoothing parameter. We include these setups in models 3 and 4. Note that our estimation methods do not require the monetary policy shock $ u_{t}$ and the interest rate smoothing shock $ \nu_{t}$ to satisfy any assumptions, aside from smoothness of their distributions when conditioned on predictors.

    Substituting the difference of equations (2) and (3) to Uncovered Interest-rate Parity (UIP), we have

    $\displaystyle s_{t}=E_{t}\left\{ (1-b)\sum_{j=0}^{\infty }b^{j}(p_{t+j}-p^{*}_{t+j})-b\sum_{j=0}^{\infty}b^{j}\left[ \delta_{y} (y^{gap}_{t+j}-y_{t+j}^{gap\ast})+\delta_{\pi}(\pi_{t+j}-\pi^{*}_{t+j})\right] \right\} ,$ (6)

    where the discount factor $ b=\frac{1}{1+\delta_{s}}$. Under some conditions, the present value asset pricing format in equation (6) can be written into an error-correction form:5

    $\displaystyle s_{t+h}-s_{t}=\alpha_{h}+\beta _{h}z_{t}+\varepsilon_{t+h},$ (7)

    where the deviation of the exchange rate from its equilibrium level is defined as:

    $\displaystyle z_{t}=s_{t}-p_{t}+p_{t}^{\ast}+\frac{b}{1-b}\left[ \delta_{y}(y_{t}^{gap}-y_{t}^{gap\ast})+\delta_{\pi}(\pi_{t}-\pi_{t}^{\ast })\right] .$ (8)

    We use equation (7) as our benchmark setup in calculating h-horizon-ahead out-of-sample forecasting intervals. According to equation (8), the matrix $ \mathbf{X} _{1,t}$ in equation (1) includes economic variables $ q_{t}\equiv s_{t}+p_{t}^{\ast}-p_{t}$, $ y_{t}^{gap}-y_{t}^{gap\ast}$, and $ \pi_{t}-\pi_{t}^{\ast}$.

    2.2  Data

    The forecasting models and the corresponding forecast intervals are estimated using monthly data for twelve OECD countries. The United States is treated as the foreign country in all cases. For each country we synchronize the beginning and end dates of the data across all models estimated. The twelve countries and periods considered are: Australia (73:03-06:6), Canada (75:01-06:6), Denmark (73:03-06:6), France (77:12-98:12), Germany (73:03-98:12), Italy (74:12-98:12), Japan (73:03-06:6), Netherlands (73:03-98:12), Portugal (83:01-98:12), Sweden (73:03-04:11), Switzerland (75:09-06:6), and the United Kingdom (73:03-06:4).

    The data is taken from Molodtsova and Papell (2008).6 With the exception of interest rates, the data is transformed by taking natural logs and then multiplied by 100. The nominal exchange rates are end-of-month rates taken from the Federal Reserve Bank of St. Louis database. Output data $ y_{t}$ are proxied by Industrial Production (IP) from the International Financial Statistics (IFS) database. IP data for Australia and Switzerland are only available at quarterly frequency, and hence are transformed from quarterly to monthly observations using the quadratic-match average option in Eviews 4.0 by Molodtsova and Papell (2008). Following Engel and West (2006), the output gap $ y_{t}^{gap}$ is calculated by quadratically de-trending the industrial production for each country.

    Prices data $ p_{t}$ are proxied by Consumer Price Index (CPI) from the IFS database. Again, CPI for Australia is only available at quarterly frequency and quadratic-match average is used to impute monthly observations. Inflation rates are calculated by taking the first differences of the logs of CPIs. Money market rate from IFS (or "call money rate") is used as a measure of the short-term interest rate set by the central bank. Finally, M1 is used to measure the money supply for most countries. M0 for the UK, and M2 for Italy and Netherlands is used due to the unavailability of M1 data.


    3.  Econometric Method

    For a given model $ m$, the objective is to estimate from equation (1) the distribution of $ s_{\tau +h}-s_{\tau}$ conditional on data $ \mathbf{X}_{m,\tau}$ that is observed up to time $ \tau$. This is the $ h$-horizon-ahead forecast distribution of the exchange rate, from which the corresponding forecast interval can be derived. For a given $ \alpha$, the forecast interval of coverage $ \alpha \in(0,1)$ is an interval in which $ s_{\tau+h}-s_{\tau}$ is supposed to lie with a probability of $ \alpha$.

    Models $ m=1,...,7$ in equation (1) provide only point forecasts of $ s_{\tau+h}-s_{\tau}$. In order to construct forecast intervals for a given model, we apply robust semi-parametric (RS) forecast intervals to all models. The nominal $ \alpha$-coverage forecast interval of $ s_{\tau +h}-s_{\tau}$ conditional on $ \mathbf{X}_{m,\tau}$ can be obtained by the following three-step procedure:

    Step 1.
    Estimate model $ m$ by OLS and obtain residuals $ \widehat{\varepsilon}_{m,t+h}\equiv s_{t+h}-s_{t}-\widehat{\alpha} _{m,h}+\widehat{\beta}^{^{\prime}}_{m,h}\mathbf{X}_{m,t}$ , for $ t=1,...,\tau -h$.
    Step 2.
    For a range of values of $ \varepsilon$ (sorted residuals $ \{\widehat{\varepsilon}_{m,t+h}\}_{t=1}^{\tau-h}$), estimate the conditional distribution of $ \varepsilon_{m,\tau+h}\vert\mathbf{X}_{m,\tau}$ by
    $\displaystyle \widehat{P}(\varepsilon_{m,\tau+h}\le\varepsilon\vert\mathbf{X}_{m,\tau} )\equiv\frac{\sum_{t=1}^{\tau-h}1(\widehat{\varepsilon}_{m,t+h}\le\varepsilon) \mathbf{K}_{b}(\mathbf{X}_{m,t}-\mathbf{X}_{m,\tau})}{\sum_{t=1}^{\tau -h}\mathbf{K}_{b}(\mathbf{X}_{m,t}-\mathbf{X}_{m,\tau})},$ q (9)

    where $ \mathbf{K}_{b}(\mathbf{X}_{m,t}-\mathbf{X}_{m,\tau})\equiv b^{-d}\mathbf{K}((\mathbf{X}_{m,t}-\mathbf{X}_{m,\tau})/b)$ , $ \mathbf{K} (\cdot)$ is a multivariate Gaussian kernel with dimension same as that of $ \mathbf{X}_{m,t}$, and $ b$ is the smoothing parameter or bandwidth.7
    Step 3.
    Find the $ (1-\alpha)/2$ and $ (1+\alpha)/2$ quantiles of the estimated distribution, which are denoted by $ \widehat{\varepsilon }_{m,h}^{(1-\alpha)/2}$ and $ \widehat{\varepsilon}_{m,h}^{(1+\alpha)/2}$. The estimate of the $ \alpha$-coverage forecast interval for $ s_{\tau+h}-s_{\tau}$ conditional on $ \mathbf{X}_{m,\tau}$ is
    $\displaystyle \widehat{I}^{\alpha}_{m,\tau+h}\equiv(\widehat{\beta}_{m,h}^{\prime} \mathbf{X}_{m,\tau}+\widehat{\varepsilon}_{m,h}^{(1-\alpha)/2}, \widehat {\beta}_{m,h}^{\prime}\mathbf{X}_{m,\tau}+\widehat{\varepsilon}_{m,h} ^{(1+\alpha)/2})$ (10)

    For each model $ m$, the above method uses the forecast models in equation (1) to estimate the location of the forecast distribution, while nonparametric kernel distribution estimate is used to estimate the shape. As a result, the interval obtained from this method is semi-parametric. Wu (2007) shows that under some weak regularity conditions, this method always consistently estimates the forecast distribution,8 and hence the forecast intervals, of $ s_{\tau+h}-s_{\tau}$ conditional on $ \mathbf{X} _{m,\tau}$, regardless of the quality of model $ m$. That is, the forecast intervals are robust. Stationarity of economic variables is one of those regularity conditions. In our models, exchange rate differences, interest rates and inflation rates are well-known to be stationary, while empirical tests for real exchange rates and output gaps generate mixed results. These results may be driven by the difficulty of distinguishing a stationary but persistent variable from a non-stationary one. In this paper, we take the stationarity of these variables as given.

    Model seven is the random walk model. The estimator in equation (9) becomes the Empirical Distribution Function (EDF) of the exchange rate innovations. Under regularity conditions, equation (9) consistently estimates the unconditional distribution of $ s_{\tau+h}-s_{\tau}$, and can be used to form forecast intervals for $ s_{\tau+h}$. The forecast intervals of economic models and the random walk are compared. Our interest is to test whether RS forecast intervals based on economic models are more accurate than those based on the random walk model. We focus on the empirical coverage and the length of forecast intervals in our tests.

    Following Christoffersen (1998) and related work, the first standard we use is the empirical coverage. The empirical coverage should be as close as possible to the nominal coverage ($ \alpha$). Significantly missing the nominal coverage indicates the inadequacy of the model and predictors for the given sample size. For instance, if 90% forecast intervals calculated from a model contain only 50% of out-of-sample observations, the model can hardly be identified as useful for interval forecasting. This case is called under-coverage. In contrast, over-coverage implies that the intervals could be reduced in length (or improved in tightness), but the forecast interval method and model are unable to do that for the given sample size. An economic model is said to outperform the random walk if its empirical coverage is more accurate than that of the random walk.

    On the other hand, the empirical coverage of an economic model may be equally accurate as that of the random walk model, but the economic model has tighter forecast intervals than the random walk. We argue that the lengths of forecast intervals signify the informativeness of the intervals given that these intervals have equally accurate empirical coverages. In this case, the economic model is also considered to outperform the random walk in forecasting exchange rates. The empirical coverage and length tests are conducted at both short and long horizons for six economic models relative to the random walk for each of the twelve OECD exchange rates.

    We use tests that are applications of the unconditional predictive accuracy inference framework of Giacomini and White (2006). Unlike the tests of Diebold and Mariano (1995) and West (1996), our forecast evaluation tests do not focus the asymptotic features of the forecasts. Rather, in the spirit of Giacomini and White (2006), we are comparing the population features of forecasts generated by rolling samples of fixed sample size. This contrasts the traditional forecast evaluation methods in that although it uses asymptotic approximations to do the testing, the inference is not on the asymptotic properties of forecasts, but on their population finite sample properties. We acknowledge that the philosophy of this inference framework remains a point of contention, but it does tackle three important evaluation difficulties in this paper. First, it allows for evaluation of forecast intervals that are not parametrically derived. The density evaluation methods developed in well-known studies such as Diebold, Gunther, Tay (1998), Corradi and Swanson (2006a) and references within Corradi and Swanson (2006b) require that the forecast distributions be parametrically specified. Giacomini and White's (2006) method overcomes this challenge by allowing comparisons among parametric, semi-parametric and nonparametric forecasts. As a result, in the cases of semi-parametric and nonparametric forecasts, it also allows comparison of models with predictors of different dimensions, as evident in our exercise. Second, by comparing finite sample properties of RS forecast intervals derived from different models, we avoid rejecting models that are mis-specified,9 but are nonetheless good approximations useful for forecasting. Finally, we can individually (though not jointly) test whether the forecast intervals differ in terms of empirical coverages and lengths, for the given estimation sample, and not confined to focus only on empirical coverages or holistic properties of forecast distribution such as probability integral transform.

    3.1  Test of Equal Empirical Coverages

    Suppose the sample size available to the researcher is $ T$ and all data are collected in a vector $ \mathbf{W}_{t}$. Our inference procedure is based on a rolling estimation scheme, with the size of the rolling window fixed while $ T\rightarrow\infty$. Let $ T=R+N$ and $ R$ be the size of the rolling window. For each horizon $ h$ and model $ m$, a sequence of $ N(h)=N+1-h$ $ \alpha $-coverage forecast intervals are generated using rolling data: $ \{\mathbf{W} _{t}\}_{t=1}^{R}$ for forecast for date $ R+h$, $ \{\mathbf{W}_{t}\}_{t=2} ^{R+1}$ for forecast for date $ R+h+1$, and so on, until forecast for date $ T$ is generated using $ \{\mathbf{W}_{t}\}_{t=N(h)}^{R+N(h)-1}$.

    Under this fixed-sample-size rolling scheme, for each finite $ h$ we have $ N(h)$ observations to compare the empirical coverages and lengths across $ m$ models ( $ m=1, 2,...,7$). By fixing $ R$, we allow the finite sample properties of the forecast intervals to be preserved as $ T\rightarrow\infty$. Thus, the forecast intervals and the associated forecast losses are simply functions of a finite and fixed number of random variables. We are interested in approximating the population moments of these objects by taking $ N(h)\rightarrow\infty$. A loose analogy would be finding the finite-sample properties of a certain parameter estimator when sample size is fixed at $ R$, by a bootstrap with an arbitrarily large number of bootstrap replications.

    We conduct individual tests for the empirical coverages and lengths. In each test, we define a corresponding forecast loss, propose a test statistic and derive its asymptotic distribution. As defined in equation (10), let $ \widehat{I}^{\alpha}_{m,\tau+h}$ be the $ h-$horizon ahead RS forecast interval of model $ m$ with a nominal coverage of $ \alpha$. For out-of-sample forecast evaluation, we require $ \widehat{I}^{\alpha}_{m,\tau+h}$ to be constructed using data from $ t=\tau-R+1$ to $ t=\tau$. The coverage accuracy loss is defined as

    $\displaystyle CL_{m,h}^{\alpha}=\left[ P(Y_{\tau+h}\in\widehat{I}^{\alpha}_{m,\tau +h})-\alpha\right] ^{2}.$ (11)

    For economic models ($ m=1,...,6$), the goal is to compare the coverage accuracy loss of RS forecast intervals of model $ m$ with that of the random walk ($ m=7$). The null and alternative hypotheses are:

    $\displaystyle H_{0}$ $\displaystyle : \Delta CL_{m,h}^{\alpha}\equiv CL_{7,h}^{\alpha}-CL_{m,h}^{\alpha }=0$
    $\displaystyle H_{A}$ $\displaystyle : \Delta CL_{m,h}^{\alpha}\ne0.$

    Define the sample analog of the coverage accuracy loss in equation (11):

    $\displaystyle \widehat{CL}_{m,h}^{\alpha}=\left( N(h)^{-1}\sum_{\tau=R}^{T-h}1(Y_{\tau+h} \in\widehat{I}^{\alpha}_{m,\tau+h})-\alpha\right) ^{2},$

    where $ 1(Y_{\tau+h}\in\widehat{I}^{\alpha}_{m,\tau+h})$ is an index function that equals one when $ Y_{\tau+h}\in\widehat{I}^{\alpha}_{m,\tau+h}$, and equals zero otherwise. Applying the asymptotic test of Giacomini and White (2006) to the sequence $ \{1(Y_{\tau+h}\in\widehat{I}^{\alpha}_{m,\tau +h})\}_{\tau=R}^{T-h}$ and applying the Delta method, we can show that

    $\displaystyle \sqrt{N(h)}(\Delta\widehat{CL}_{m,h}^{\alpha}-\Delta CL_{m,h}^{\alpha })\overset{d}{\rightarrow}N(0,\Gamma_{m,h}^{^{\prime}}\Omega_{m,h}\Gamma _{m,h}),$ (12)

    where $ \overset{d}{\rightarrow}$ denotes convergence in distribution, and $ \Omega_{m,h}$ is the long-run covariance matrix between $ 1(Y_{\tau+h} \in\widehat{I}^{\alpha}_{m,\tau+h})$ and $ 1(Y_{\tau+h}\in\widehat{I}^{\alpha }_{7,\tau+h})$. The matrix $ \Gamma_{m,h}$ is defined as:

    $\displaystyle \Gamma_{m,h}\equiv\left[ \begin{array}[c]{cc} 2\left( P\left( Y_{\tau+h}\in\widehat{I}^{\alpha}_{m,\tau+h}\right) -\alpha\right) & 2\left( P\left( Y_{\tau+h}\in\widehat{I}^{\alpha}_{7,\tau +h}\right) -\alpha\right) \end{array} \right] ^{\prime}.$

    $ \Gamma_{m,h}$ can be estimated consistently by its sample analog $ \widehat{\Gamma}_{m,h}$, while $ \Omega_{m,h}$ can be estimated by some HAC estimator $ \widehat{\Omega}_{m,h}$, such as Newey and West (1987).10The test statistic for coverage test is defined as:

    $\displaystyle Ct_{m,h}^{\alpha}\equiv\frac{\sqrt{N(h)}\Delta\widehat{CL}_{m,h}^{\alpha} }{\sqrt{\widehat{\Gamma}_{m,h}^{^{\prime}}\widehat{\Omega}_{m,h} \widehat{\Gamma}_{m,h}}}\overset{d}{\rightarrow}N(0,1)$ (13)

    3.2  Test of Equal Empirical Lengths

    Define the length loss as:

    $\displaystyle LL^{\alpha}_{m,h}\equiv E\left[ leb\left( \widehat{I}^{\alpha}_{m,\tau +h}\right) \right] ,$ (14)

    where $ leb(\cdot)$ is the Lesbesgue measure. To compare the length loss of RS forecast intervals of economic models $ m=1, 2,...,6$ with that of the random walk ($ m=7)$, the null and alternative hypotheses are:

    $\displaystyle H_{0}$ $\displaystyle : \Delta LL_{m,h}^{\alpha}\equiv LL_{7,h}^{\alpha}-LL_{m,h}^{\alpha }=0$
    $\displaystyle H_{A}$ $\displaystyle : \Delta LL_{m,h}^{\alpha}\ne0.$

    The sample analog of the length loss for model $ m$ is defined as:

    $\displaystyle \widehat{LL}_{m,h}^{\alpha}=N(h)^{-1}\sum_{\tau=R}^{T-h}leb(\widehat {I}^{\alpha}_{m,\tau+h}).$

    Directly applying the test of Giacomini and White (2006), we have

    $\displaystyle \sqrt{N(h)}(\Delta\widehat{LL}_{m,h}^{\alpha}-\Delta LL_{m,h}^{\alpha })\overset{d}{\rightarrow}N(0,\Sigma_{m,h}),$ (15)

    where $ \Sigma_{m,h}$ is the long-run variance of $ leb\left( \widehat {I}^{\alpha}_{7,\tau+h}\right) -leb\left( \widehat{I}^{\alpha}_{m,\tau +h}\right) $ . Let $ \widehat{\Sigma}_{m,h}$ be the HAC estimator of $ \Sigma_{m,h}$. The test statistic for empirical length is defined as:

    $\displaystyle Lt_{m,h}^{\alpha}\equiv\frac{\sqrt{N(h)}\Delta\widehat{LL}_{m,h}^{\alpha} }{\sqrt{\widehat{\Sigma}_{m,h}}}\overset{d}{\rightarrow}N(0,1).$ (16)

    3.3  Discussion

    The coverage accuracy loss function is symmetric in our paper. In practice, an asymmetric loss function may be better when looking for an exchange rate forecast model to help make policy or business decisions. Under-coverage is arguably a more severe problem than over-coverage in practical situations. However, the focus of this paper is the disconnect between economic fundamentals and the exchange rate. Our goal is to investigate which model comes closer to the data: the random walk or fundamental-based models. It is not critical in this case whether coverage inaccuracy comes from the under- or over-coverage. We acknowledge that the use of symmetric coverage loss remains a caveat, especially since we are using the coverage accuracy test as a pre-test for the tests of length. Clearly, there is a tradeoff between the empirical coverage and the length of forecast intervals. Given the same center,11 intervals with under-coverage have shorter lengths than intervals with over-coverage. In this case, the length test is in favor of models that systematically under-cover the targeted nominal coverage when compared to a model that systematically over-covers. This problem cannot be detected by the coverage accuracy test with symmetric loss function because over- and under-coverage are treated equally. However, our results in section 4 show that there is no evidence of systematic under-coverage for the economic models considered in this paper. For instance, in Table 1, one-month-ahead ($ h=1$) forecast interval over-covers the nominal coverage (90%) for nine out of twelve exchange rates.12 Note that under-coverage does not guarantee shorter intervals either in our paper, because forecast intervals of different models usually have different centers.13

    As we have mentioned, comparisons across models can also be done at the distribution level. We choose interval forecasts for two reasons. First, interval forecasts have been widely used and reported by the practitioners. For instance, the Bank of England calculates forecast intervals of inflation in its inflation reports. Second, compared to evaluation metrics for density forecasts, the empirical coverage and length loss functions of interval forecasts, and the subsequent interpretations of test rejection/acceptance are more intuitive.


    4.  Results

    We apply RS forecast intervals for each model for a given nominal coverage of $ \alpha=0.9$. There is no particular reason why we chose 0.9 as the nominal coverage. Some auxiliary results show that our qualitative findings do not depend on the choice of $ \alpha$. Due to different sample sizes across countries, we choose different sizes for the rolling window ($ R$) for different countries. Our rule is very simple: for countries with $ T\ge300$, we choose $ R=200$, otherwise we set $ R=150$.14 Again, from our experience, tampering with $ R$ does not change the qualitative results unless $ R$ is chosen to be unusually big or small.

    For time horizons $ h=1,3,6,9,12$ and models $ m=1,...,7$, we construct a sequence of $ N(h)$ 90% forecast intervals $ \{\widehat{I}^{0.9}_{m,\tau +h}\}_{\tau=R}^{T-h}$ for the $ h$-horizon change of the exchange rate $ s_{t+h}-s_{t}$. Then we compare economic models and the random walk by computing empirical coverages, lengths and test statistics $ Ct_{m,h}^{0.9}$ and $ Lt_{m,h}^{0.9}$ as described in section 3. We first report the results of our benchmark model. After that, results of alternative models are reported and discussed.

    4.1  Results of Benchmark Model

    Table 1 shows results of the benchmark Taylor rule model. For each time horizon $ h$ and exchange rate, the first column (Cov.) reports the empirical coverage for the given nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals (the distance between upper and lower bounds). The length is multiplied by 100 and therefore expressed in terms of the percentage change of the exchange rate. For instance, the length of the one-month-ahead forecast interval for the Australian dollar is $ 7.114$. On average, the distance between the upper and lower bound of the one-month-ahead forecast interval for the Australian dollar is $ 7.114$% change of the Australian dollar against the US dollar. We use superscripts $ a$, $ b$, and $ c$ to denote that the null hypothesis of equal empirical coverage accuracy/length is rejected in favor of the Taylor rule model at a confidence level of 10%, 5%, and 1% respectively. Superscripts $ x$, $ y$, and $ z$ are used for rejections in favor of the random walk analogously.

    We summarize our findings in three panels. In the first panel ((1) Coverage Test), the row of "Model Better" reports the number of exchange rates that the Taylor rule model has more accurate empirical coverages than the random walk. The row of "RW Better" reports the number of exchange rates for which the random walk outperforms the Taylor rule model under the same criterion. In the second panel ((2) Length Test Given Equal Coverage Accuracy), a better model is the one with tighter forecast intervals given equal coverage accuracy. In the last panel ((1)+(2)), a better model is the one with either more accurate coverages, or tighter forecast intervals given equal coverage accuracy.

    For most exchange rates and time horizons, the Taylor rule model and the random walk model have statistically equally accurate empirical coverages. The null hypothesis of equal coverage accuracy is rejected in only nine out of sixty tests (one rejection at horizon 3, two rejections at horizons 6 and 9, and four at horizon 12). All nine rejections are in favor of the Taylor rule model. That is, the empirical coverage of the Taylor rule model is closer to the nominal coverage than those of the random walk. However, based on the number of rejections (9) in a total of sixty tests, there is no strong evidence that the Taylor rule model can generate more accurate empirical coverages than the random walk. The coverage tests at horizon twelve have more rejections in favor of the Taylor rule model than that at short horizons ($ h=1,3$). However, this pattern in coverage tests does not exist in other models that will be discussed in next subsection.

    In cases where the Taylor rule model and the random walk have equally accurate empirical coverages, the Taylor rule model generally has equal or significantly tighter forecast intervals than the random walk. In forty-one out of fifty-one cases, the null hypothesis of equally tight forecast intervals is rejected in favor of the Taylor rule model. In contrast, the null hypothesis is rejected in only two cases in favor of the random walk. The evidence of exchange rate predictability is more pronounced at longer horizons. At horizons nine and twelve ($ h=9, 12$), for cases where empirical coverage accuracies between the random walk and the Taylor rule model are statistically equivalent, the Taylor rule model has significantly tighter forecast intervals than the random walk.

    As for each individual exchange rate, the benchmark Taylor rule model works best for the Canadian dollar, the French Franc, the Deutschmark, and the Swedish Krona: for all time horizons, the model has tighter forecast intervals than the random walk, while their empirical coverages are statistically equally accurate. The Taylor rule model performs better than the random walk in most horizons for remaining exchange rates except the Japanese yen, for which the Taylor rule model outperforms the random walk only at long horizons.

    4.2  Results of Alternative Models

    Five alternative economic models are also compared with the random walk: three alternative Taylor rule models that are studied in Molodtsova and Papell (2008), the PPP model, and the monetary model. Tables 2-6 report results of these alternative models.

    In general, results of coverage tests do not show strong evidence that economic models can generate more accurate coverages than the random walk at either short or long horizons. Though the benchmark Taylor rule model shows a sign of long-horizon predictability based on coverage accuracy tests, there is no clear evidence for such a pattern in any other models. However, after considering length tests, we find that economic models perform better than the random walk, especially at long horizons. The Taylor rule model four (Table 4) and the PPP model (Table 5) perform the best among alternative models. Results of these two models are very similar to that of the benchmark Taylor rule model. At horizon twelve, both models outperform the random walk for all twelve exchange rates under our out-of-sample forecast interval evaluation criteria. The performance of the Taylor rule model two (Table 2) and three (Table 3) is relatively less impressive than other models, but still for about half of exchange rates, the economic models outperform the random walk at several horizons in out-of-sample interval forecasts.

    Comparing the benchmark Taylor rule model, the PPP model and the monetary model, the performance of the monetary model (Table 6) is slightly worse than the other two models at long horizons. Compared to the Taylor rule and PPP models, the monetary model outperforms the random walk for a smaller number of exchange rates at horizons 6, 9, and 12. The Taylor rule model and the monetary model perform relatively better than the PPP model at short horizons. Overall, the benchmark Taylor rule model seems to perform slightly better than the monetary and PPP models. Molodtsova and Papell (2008) find similar results in their point forecasts.

    4.3  Discussion

    After Mark (1995) first documents exchange rate predictability at long horizons, long-horizon exchange rate predictability has become a very active area in the literature. With panel data, Engel, Mark, and West (2007) recently show that the long-horizon predictability of the exchange rate is relatively robust in the exchange rate forecasting literature. We find similar results in our interval forecasts. The evidence of long-horizon predictability seems robust across different models and currencies when both empirical coverage and length tests are used. At horizon twelve, all economic models outperform the random walk for seven exchange rates: the Australia dollar, Canadian dollar, Italian Lira, Japanese yen, Portuguese escudo, Swedish krona, and the British pound in the sense that interval lengths of economic models are smaller than those of the random walk, given equivalent coverage accuracy. This is true only for the Italian Lira at horizon one. We also notice that there is no clear evidence of long-horizon predictability based on the tests of empirical coverage accuracy only.

    Molodtsova and Papell (2008) find strong out-of-sample exchange rate predictability for Taylor rule models even at the short horizon. In our paper, the evidence for exchange rate predictability at short horizons is not very strong. This finding may be a result of some assumptions we have used to simplify our computation. For instance, an $ \alpha$-coverage forecast interval will always be constructed using the $ (1-\alpha)/2$ and $ (1+\alpha)/2$ quantiles. Alternatively, we can choose quantiles that minimize the length of intervals, given the nominal coverage.15 We have also assumed symmetric Taylor rules. Relaxing these assumptions may help us find exchange rate predictability at short horizons. In addition, the development of more powerful testing methods may also be helpful. The evidence of exchange rate predictability in Molodtsova and Papell (2008) is partly driven by the testing method recently developed by Clark and West (2006, 2007). We acknowledge that whether or not short-horizon results can be improved remains an interesting question, but do not pursue this in the current paper. The purpose of this paper is to show the connection between the exchange rate and economic fundamentals from an interval forecasting perspective. Predictability either at short- or long-horizons will serve this purpose.

    Though we find that economic fundamentals are helpful for forecasting exchange rates, we acknowledge that exchange rate forecasting in practice is still a difficult task. The forecast intervals from economic models are statistically tighter than those of the random walk, but they remain fairly wide. For instance, the distance between the upper and lower bound of three-month-ahead forecast intervals is usually a 20% change of the exchange rates. Figures 1-3 show forecast intervals generated by the benchmark Taylor rule model and the random walk for the British pound, the Deutschmark, and the Japanese yen at different horizons.16 To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been re-centered so that they have the same center as the forecast intervals of the Taylor rule model. In these figures, the Taylor rule model has tighter forecast intervals, especially at the horizon of 12 months, than the random walk. However, the difference is quantitatively small.


    5.  Conclusion

    There is a growing strand of literature that uses Taylor rules to model exchange rate movements. Our paper contributes to the literature by showing that Taylor rule fundamentals are useful in forecasting distribution of exchange rates. We apply Robust Semi-parametric forecast intervals of Wu (2007) to a group of Taylor models for twelve OECD exchange rates. The forecast intervals generated by the Taylor rule models are in general tighter than those of the random walk, given that these intervals cover the realized exchange rates equally well. The evidence of exchange rate predictability is more pronounced at longer horizons, a result that echoes previous long-horizon studies such as Mark (1995). The benchmark Taylor rule model is also found to perform better than the monetary and PPP models based on out-of-sample interval forecasts.

    Though we find some empirical support for the connection between the exchange rate and economic fundamentals, we acknowledge that the detected connection is weak. The reductions of the lengths of forecast intervals are quantitatively small, though they are statistically significant. Forecasting exchange rates remains a difficult task in practice. Engel and West (2005) argue that as the discount factor gets closer to one, present value asset pricing models place greater weight on future fundamentals. Consequently, current fundamentals have very weak forecasting power and exchange rates appear to follow approximately a random walk. Under standard assumptions in Engel and West (2005), the Engel-West theorem does not imply that exchange rates are more predictable at longer horizons, or economic models can outperform the random walk in forecasting exchange rates based on out-of-sample interval forecasts. However, modifications to these assumptions may be able to reconcile the Engel-West explanation with empirical findings of exchange rate predictability. For instance, Engel, Wang, and Wu (2008) find that when there exist stationary but persistent unobservable fundamentals, for example risk premium, the Engel-West explanation predicts long-horizon exchange rate predictability in point forecasts, though the exchange rate still approximately follows a random walk at short horizons. It would also be of interest to study conditions under which our findings in interval forecasts can be reconciled with the Engel-West theorem.

    We believe other issues, such as parameter instability (Rossi, 2005), nonlinearity (Kilian and Taylor, 2003), real time data (Faust, Rogers, and Wright, 2003, Molodtsova, Nikolsko-Rzhevskyy, and Papell, 2008), are all contributing to the Meese-Rogoff puzzle. Panel data are also found helpful in detecting exchange rate predictability, especially at long horizons. For instance, see Mark and Sul (2001) and Engel, Mark, and West (2007). It would be interesting to incorporate these studies into interval forecasting. We leave these extensions for future research.

    Table 1: Panel 1 - Results of Benchmark Taylor Rule Model.
     Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.895

    7.114

    0.888

    14.283c

    0.923

    20.286c

    0.927

    24.468c

    0.915

    28.016c

    Canadian Dollar

    0.808

    3.446c

    0.789

    6.351c

    0.808

    8.586c

    0.817

    10.321c

    0.801

    12.614c

    Danish Kroner

    0.920

    8.668c

    0.939

    17.415c

    0.949

    26.087

    0.969

    30.776c

    0.968

    36.962c

    French Franc

    0.912

    8.921c

    0.920

    17.674c

    0.928c

    26.007c

    0.957

    29.924c

    0.934

    36.883c

    Deutschmark

    0.927

    8.851c

    0.879

    18.634c

    0.894

    27.923c

    0.960a

    33.734c

    0.969

    38.374c

    Italian Lira

    0.906

    8.754c

    0.875

    18.305

    0.910

    26.788c

    0.862

    34.785c

    0.890a

    39.958c

    Japanese Yen

    0.915

    9.633z

    0.909

    19.765

    0.902

    28.497c

    0.932

    33.793c

    0.883

    37.333c

    Dutch Guilder

    0.917

    8.821

    0.907

    18.649c

    0.933

    27.649c

    0.951a

    31.117c

    0.959a

    40.737c

    Portuguese Escudo

    0.901

    8.205z

    0.913a

    17.899

    0.879c

    22.431c

    0.825

    25.959c

    0.883c

    32.464c

    Swedish Krona

    0.844

    7.448c

    0.860

    15.405c

    0.874

    23.930c

    0.861

    30.827c

    0.834

    37.432c

    Swiss Franc

    0.935

    9.759c

    0.946

    20.036

    0.982

    27.682c

    0.994

    32.837c

    0.956

    38.728c

    British Pound

    0.919

    8.429

    0.923

    16.570c

    0.906

    23.623c

    0.884

    27.849c

    0.903c

    30.814c

    Note: �h denotes forecast horizons for monthly data. �For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. �Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 1: Panel 2 - Results of Benchmark Taylor Rule Model, Coverage Test
     h=1h=3h=6h=9h=12
    Model Better 01224
    RW Better 00000

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 1: Panel 3 - Results of Benchmark Taylor Rule Model, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 7 8 9 10 8
    RW Better 2 0 0 0 0

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 1: Panel 4 - Results of Benchmark Taylor Rule Model, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 7 9 11 12 12
    RW Better 2 0 0 0 0

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Table 2: Panel 1 - Results of Benchmark Taylor Rule Model Two.
     Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.884

    7.146y

    0.899

    15.086c

    0.918

    20.902a

    0.880

    26.222c

    0.856

    30.677c

    Canadian Dollar

    0.825

    3.442c

    0.783

    6.362c

    0.820

    8.815c

    0.846

    10.610c

    0.813

    13.216c

    Danish Kroner

    0.925

    8.756c

    0.934

    17.791c

    0.959

    27.511z

    0.963

    32.956

    0.947

    40.387

    French Franc

    0.922

    8.840c

    0.920

    18.740

    0.949c

    29.161c

    0.936

    34.994c

    0.868

    41.330c

    Deutschmark

    0.936

    9.005

    0.879

    19.489

    0.952

    29.658

    0.941a

    38.006

    0.980

    44.355z

    Italian Lira

    0.920

    9.095b

    0.882

    18.558

    0.910

    27.464c

    0.908

    37.325c

    0.921

    43.005c

    Japanese Yen

    0.915

    9.565

    0.914

    19.752

    0.912

    29.618

    0.937

    36.834

    0.942

    44.455b

    Dutch Guilder

    0.908

    8.645c

    0.897

    18.983c

    0.971

    29.391b

    0.990

    38.867z

    0.980

    46.650z

    Portuguese Escudo

    0.916

    7.956

    0.957

    17.924z

    0.909c

    24.196c

    0.889

    28.533z

    0.883a

    35.338c

    Swedish Krona

    0.861

    7.575

    0.860

    15.679c

    0.851

    24.916c

    0.849

    31.108c

    0.823

    40.458c

    Swiss Franc

    0.947

    10.008

    0.928

    20.379y

    0.976

    29.578c

    0.988

    37.858

    0.962

    44.675z

    British Pound

    0.919

    8.614z

    0.933

    17.302c

    0.922

    26.196c

    0.937

    31.371a

    0.957

    37.239c

    Note: –h denotes forecast horizons for monthly data. –For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. –Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 2: Panel 2 - Results of Benchmark Taylor Rule Model Two, Coverage Test
      h=1 h=3 h=6 h=9 h=12
    Model Better 0 0 2 1 1
    RW Better 0 0 0 0 0

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 2: Panel 3 - Results of Benchmark Taylor Rule Model Two, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 5 6 7 6 7
    RW Better 2 2 1 2 3

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 2: Panel 4 - Results of Benchmark Taylor Rule Model Two, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 5 6 9 7 8
    RW Better 2 2 1 2 3

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Table 3: Panel 1 - Results of Benchmark Taylor Rule Model. Three
     Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.884

    7.163y

    0.893

    14.925c

    0.881

    21.067

    0.869

    25.590c

    0.835

    28.714c

    Canadian Dollar

    0.831

    3.453b

    0.789

    6.402c

    0.808

    8.764c

    0.846

    10.644c

    0.795

    12.592c

    Danish Kroner

    0.925

    8.794b

    0.924

    17.831c

    0.959

    27.536z

    0.963

    33.251

    0.942

    40.036a

    French Franc

    0.941

    8.880c

    0.880

    18.389c

    0.876c

    28.548b

    0.915

    35.443a

    0.813

    41.350c

    Deutschmark

    0.945

    9.042

    0.897

    19.642z

    0.914

    29.677

    0.901c

    37.291a

    0.878

    44.520y

    Italian Lira

    0.906

    8.831c

    0.868

    18.064c

    0.902

    27.430c

    0.877

    37.364c

    0.803

    41.499c

    Japanese Yen

    0.905

    9.181c

    0.873

    18.910c

    0.881

    25.700c

    0.927

    31.259c

    0.894

    37.049c

    Dutch Guilder

    0.927

    8.910

    0.907

    19.204a

    0.942

    29.637

    0.951a

    36.896c

    0.959

    46.321z

    Portuguese Escudo

    0.930

    7.961

    0.928

    16.808c

    0.909c

    24.059b

    0.873

    27.868

    0.917b

    34.980c

    Swedish Krona

    0.861

    7.375c

    0.843

    15.096c

    0.886

    24.770c

    0.849

    31.044c

    0.817

    38.468c

    Swiss Franc

    0.965

    9.959

    0.934

    20.433y

    0.957

    29.418c

    0.926c

    37.130

    0.911

    43.546

    British Pound

    0.919

    8.537

    0.939

    17.397b

    0.927

    25.809c

    0.926

    30.749c

    0.968

    36.825c

    Note: –h denotes forecast horizons for monthly data. –For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. –Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 3: Panel 2 - Results of Benchmark Taylor Rule Model Three, Coverage Test
      h=1 h=3 h=6 h=9 h=12
    Model Better 0 0 2 2 1
    RW Better 0 0 0 0 0

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 3: Panel 3 - Results of Benchmark Taylor Rule Model Three, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 4 5 5 7 8
    RW Better 0 2 1 0 2

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 3: Panel 4 - Results of Benchmark Taylor Rule Model Three, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 4 5 7 8 9
    RW Better 0 2 0 0 2

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Table 4: Panel 1 - Results of Benchmark Taylor Rule Model Four.
      Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.895

    7.119

    0.888

    14.409c

    0.902

    20.359c

    0.911

    24.165c

    0.872

    27.492c

    Canadian Dollar

    0.814

    3.425c

    0.777

    6.332c

    0.744

    8.490c

    0.769

    10.177c

    0.759

    12.043c

    Danish Kroner

    0.920

    8.703c

    0.929

    17.534c

    0.964

    26.025

    0.984x

    30.891c

    0.963

    36.443c

    French Franc

    0.931

    9.065c

    0.860

    17.422c

    0.938c

    25.950c

    0.883

    30.016c

    0.791

    35.192c

    Deutschmark

    0.945

    8.866c

    0.888

    18.839c

    0.894

    26.803c

    0.911c

    32.839c

    0.929

    38.699c

    Italian Lira

    0.891

    8.663c

    0.838

    17.575c

    0.865

    26.307c

    0.777

    33.602c

    0.756

    38.890c

    Japanese Yen

    0.905

    9.160c

    0.863

    18.708c

    0.861

    24.386c

    0.869

    28.730c

    0.851

    31.697c

    Dutch Guilder

    0.936

    8.797

    0.897

    18.368c

    0.914

    26.700c

    0.931c

    29.974c

    0.929c

    37.481c

    Portuguese Escudo

    0.901

    8.183y

    0.884b

    16.237b

    0.909c

    22.354c

    0.905

    25.896c

    0.917

    30.329c

    Swedish Krona

    0.861

    7.382c

    0.854

    15.095c

    0.869

    23.340c

    0.820

    30.370c

    0.805

    36.487c

    Swiss Franc

    0.965

    9.644c

    0.940

    19.782a

    0.957

    27.332c

    0.975

    31.004c

    0.956

    35.362c

    British Pound

    0.904

    8.464

    0.923

    16.287c

    0.854

    23.394c

    0.825

    27.333c

    0.855

    29.796c

    Note: –h denotes forecast horizons for monthly data. –For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. –Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 4: Panel 2 - Results of Benchmark Taylor Rule Model Four, Coverage Test
      h=1 h=3 h=6 h=9 h=12
    Model Better 0 0 2 2 2
    RW Better 0 0 0 1 0

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 4: Panel 3 - Results of Benchmark Taylor Rule Model Four, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 8 1 9 9 10
    RW Better 1 0 0 0 0

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 4: Panel 4 - Results of Benchmark Taylor Rule Model Four, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 8 11 11 11 12
    RW Better 1 0 0 1 0

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Table 5: Panel 1 - Results of Purchasing Power Parity Model.
     Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.895

    7.114z

    0.883

    15.558

    0.912

    21.311

    0.880

    26.120c

    0.856

    30.316c

    Canadian Dollar

    0.808

    3.513

    0.811

    6.929

    0.814

    9.669b

    0.828

    11.912a

    0.789

    15.303c

    Danish Kroner

    0.925

    8.735b

    0.929

    18.253

    0.938

    25.891c

    0.969

    32.151b

    0.952

    38.019c

    French Franc

    0.922

    8.918c

    0.940

    18.137c

    0.979

    26.944c

    0.936

    31.597c

    0.824

    37.655c

    Deutschmark

    0.936

    9.079

    0.935

    18.797c

    0.942

    27.588c

    1.000

    33.585c

    0.990

    39.821c

    Italian Lira

    0.913

    8.794c

    0.875

    18.600

    0.887

    26.619c

    0.954

    36.347c

    0.953

    42.926c

    Japanese Yen

    0.920

    9.662z

    0.899

    19.903

    0.912

    28.691c

    0.932

    33.973c

    0.899

    38.568c

    Dutch Guilder

    0.936

    8.830

    0.935

    18.904c

    0.952

    27.902c

    1.000

    33.468c

    0.990

    40.045c

    Portuguese Escudo

    0.901

    8.049

    0.913a

    17.818

    0.909c

    23.033c

    0.841

    25.579c

    0.900c

    32.050c

    Swedish Krona

    0.861

    7.541c

    0.876

    16.089

    0.886

    24.345c

    0.855

    31.744a

    0.799

    37.943c

    Swiss Franc

    0.941

    9.884c

    0.946

    19.709c

    0.988

    28.110c

    0.988

    33.301c

    0.981

    39.887c

    British Pound

    0.934

    8.643z

    0.939

    17.317c

    0.938

    25.283c

    0.952

    29.418c

    0.930

    32.964c

    Note: –h denotes forecast horizons for monthly data. –For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. –Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 5: Panel 2 - Results of Purchasing Power Parity Model, Coverage Test
      h=1 h=3 h=6 h=9 h=12
    Model Better 0 1 1 0 1
    RW Better 0 0 0 0 0

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 5: Panel 3 - Results of Purchasing Power Parity Model, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 5 5 10 12 11
    RW Better 3 0 0 0 0

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 5: Panel 4 - Results of Purchasing Power Parity Model, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 5 6 11 12 12
    RW Better 3 0 0 0 0

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Table 6: Panel 1 - Results of Monetary Model.
      Cov. h=1 Leng. h=1 Cov. h=3 Leng. h=3 Cov. h=6 Leng. h=6 Cov. h=9 Leng. h=9 Cov. h=12 Leng. h=12

    Australian Dollar

    0.869

    7.089

    0.853

    15.357

    0.840

    21.353

    0.822

    25.707c

    0.766

    30.099c

    Canadian Dollar

    0.791

    3.529

    0.783

    6.854

    0.779

    9.903

    0.787

    12.336

    0.747

    15.176c

    Danish Kroner

    0.905

    8.771b

    0.893

    18.049

    0.871

    26.413

    0.864

    31.655b

    0.856

    38.564c

    French Franc

    0.922

    8.830c

    0.910

    18.346c

    0.949b

    26.794c

    0.957

    32.389c

    0.956

    38.113c

    Deutschmark

    0.936

    8.944a

    0.897

    18.615c

    0.875

    27.610c

    0.901c

    33.223c

    0.908

    40.409c

    Italian Lira

    0.913

    9.001c

    0.882

    18.445b

    0.925

    26.613c

    0.954

    34.968c

    0.945

    41.395c

    Japanese Yen

    0.920

    9.542

    0.919

    19.374c

    0.871

    28.312c

    0.864

    33.401c

    0.814

    38.149c

    Dutch Guilder

    0.917

    8.753a

    0.916

    19.384a

    0.962

    29.149b

    0.970

    38.173

    0.908c

    43.896c

    Portuguese Escudo

    0.916

    8.073

    0.957

    17.811

    0.985

    24.971z

    0.968

    28.026

    1.000

    34.598c

    Swedish Krona

    0.856

    7.460c

    0.837

    15.587c

    0.823

    22.536c

    0.826

    28.641c

    0.781

    33.112c

    Swiss Franc

    0.929

    9.910

    0.868

    19.539c

    0.793

    26.827c

    0.745

    31.797c

    0.722

    36.189c

    British Pound

    0.929

    8.398c

    0.928

    17.355c

    0.896

    25.383c

    0.884

    30.600c

    0.850

    34.251c

    Note: –h denotes forecast horizons for monthly data. –For each horizon (h), the first column (Cov.) reports empirical coverages given a nominal coverage of 90%. The second column (Leng.) reports the length of forecast intervals in terms of percentage change of the exchange rate. Empirical coverages and lengths are averages across N(h) out-of-sample trials. –Superscripts a, b, c in the column of Cov. (Leng.) denote rejections of equal coverage accuracy (equal length) in favor of the economic model at a 10%, 5% and 1% confidence level respectively. Superscripts x, y, z are defined analogously for rejections in favor of the random walk.

    Table 6: Panel 2 - Results of Monetary Model, Coverage Test
      h=1 h=3 h=6 h=9 h=12
    Model Better 0 0 1 1 1
    RW Better 0 0 0 0 0

    Note: In this panel, a better model is the one with more accurate empirical coverages. RW is the abbreviation of Random Walk.

    Table 6: Panel 3 - Results of Monetary Model, Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 7 8 8 8 11
    RW Better 0 0 1 0 0

    Note: In this panel, a better model is the one with tighter forecast intervals given equal coverage accuracy.

    Table 6: Panel 4 - Results of Monetary Model, Coverage Test and Length Test Given Equal Coverage Accuracy
      h=1 h=3 h=6 h=9 h=12
    Model Better 7 8 8 9 12
    RW Better 0 0 1 0 0

    Note: In this panel, a better model is the one with either more accurate coverages or tighter forecast intervals given equal coverage accuracy.

    Figure 1a.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (British Pound), 1-month-ahead forecast

    Data for Figure 1a immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1989M12143.690.60990.66290.61030.6638
    1990M1144.980.6010.65310.60120.6538
    1990M2145.690.58120.63140.58120.6322
    1990M3153.310.56640.6150.56590.6155
    1990M4158.460.59090.64180.59080.6427
    1990M5154.040.58780.63820.58620.6377
    1990M6153.700.57270.6220.57220.6224
    1990M7149.040.56090.60940.56110.6104
    1990M8147.460.52850.57640.53030.5769
    1990M9138.440.50320.54810.50450.5491
    1990M10129.590.50910.55450.51030.5555
    1990M11129.220.4910.53490.4930.5366
    1990M12133.890.48510.52860.48830.5315
    1991M1133.700.49640.54070.49910.5432
    1991M2130.540.49260.53670.49580.5397
    1991M3137.390.48550.5290.48840.5316
    1991M4137.110.52440.57170.52660.5736
    1991M5138.220.54790.5970.54820.5971
    1991M6139.750.55430.6040.55640.6061
    1991M7137.830.57960.63220.58140.6334
    1991M8136.820.57870.63130.58080.6327
    1991M9134.300.56830.620.56960.6205
    1991M10130.770.55480.60530.55550.6052
    1991M11129.630.55560.60630.55670.6064
    1991M12128.040.53750.5860.5390.5871
    1992M1125.460.52330.57080.52490.5718
    1992M2127.700.52810.57610.53020.5776
    1992M3132.860.53740.58620.53950.5877
    1992M4133.540.55460.60480.55640.6062
    1992M5130.770.5450.59440.5460.5948
    1992M6126.840.53020.57840.530.5774
    1992M7125.880.51640.56350.51710.5633
    1992M8126.230.49930.54480.50020.5449
    1992M9122.600.49260.53730.49360.5377
    1992M10121.170.51810.56550.51940.5661
    1992M11123.880.57820.63150.58030.6338
    1992M12124.040.62640.6840.62820.6861
    1993M1124.990.61690.67360.61840.6754
    1993M2120.760.62520.68260.62590.6835
    1993M3117.020.66230.72320.66630.7294
    1993M4112.410.65350.71360.65620.7183
    1993M5110.340.61750.67470.62040.6798
    1993M6107.410.61620.67310.61920.6768
    1993M7107.690.63370.69190.63540.6945
    1993M8103.770.63850.69710.64080.7004
    1993M9105.570.63910.69770.64260.7024
    1993M10107.020.62540.68260.62840.6869
    1993M11107.880.63650.69460.63790.6973
    1993M12109.910.64430.70310.64710.7074
    1994M1111.440.6390.69720.64260.7024
    1994M2106.300.6410.69940.64220.7019
    1994M3105.100.64350.70220.64780.7081
    1994M4103.480.63920.69750.64230.7021
    1994M5103.750.63940.69770.64650.7067
    1994M6102.530.6320.68970.63710.6964
    1994M798.450.62620.68340.62790.6863
    1994M899.940.61890.67550.61960.6773
    1994M998.770.61810.67460.62190.6792
    1994M1098.350.60850.66420.61240.6688
    1994M1198.040.59360.6480.59710.6521
    1994M12100.180.60070.65570.60360.6592
    1995M199.770.61060.66640.61530.672
    1995M298.240.60860.66430.60910.6652
    1995M390.520.60770.66330.61020.6664
    1995M483.690.59750.65220.59940.6546
    1995M585.110.59220.64640.59670.6517
    1995M684.640.60110.65610.60420.6599
    1995M787.400.59980.65480.60150.6568
    1995M894.740.60.6550.60130.6567
    1995M9100.550.6090.66480.61220.6686
    1995M10100.840.6120.66810.61530.6719
    1995M11101.940.60860.66430.60790.6638
    1995M12101.850.6110.66690.61390.6704
    1996M1105.750.61720.67360.62260.68
    1996M2105.790.62710.68440.62740.6852
    1996M3105.940.62220.67750.62480.6819
    1996M4107.200.62690.6820.62840.6859
    1996M5106.340.6310.68650.6330.6909
    1996M6108.960.63260.68840.63340.6914
    1996M7109.190.6230.67790.62250.6795
    1996M8107.870.62060.67520.61790.6745
    1996M9109.930.6180.67250.61920.6758
    1996M10112.410.61470.6690.61550.6718
    1996M11112.300.60650.65990.6050.6603
    1996M12113.980.57730.62990.5770.6301
    1997M1117.910.57560.6280.57640.6295
    1997M2122.960.5790.63160.57830.6316
    1997M3122.770.59070.64410.590.6444
    1997M4125.640.59740.65120.59590.6508
    1997M5119.190.58920.64190.58870.6429
    1997M6114.290.58870.64120.58770.6418
    1997M7115.380.5850.63730.58310.6368
    1997M8117.930.5770.62860.57450.6274
    1997M9120.890.60070.65480.59820.6532
    1997M10121.060.60340.65760.5990.6528
    1997M11125.380.59360.64690.58740.6401
    1997M12129.730.57440.62630.56790.6189
    1998M1129.550.58270.63570.57790.6298
    1998M2125.850.59410.64760.58670.6391
    1998M3129.080.58820.64050.58460.6367
    1998M4131.750.58090.63230.57710.6286
    1998M5134.900.57480.62570.57360.6248
    1998M6140.330.59010.64310.58550.6378
    1998M7140.790.58750.63990.58120.6331
    1998M8144.680.58950.64190.58360.6357
    1998M9134.480.59290.64560.58690.6393
    1998M10121.050.57510.62640.57010.621
    1998M11120.290.57330.6240.56610.6166
    1998M12117.070.58380.63550.57740.629
    1999M1113.290.58010.63140.57410.6253
    1999M2116.670.59040.64250.58140.6332
    1999M3119.470.59520.64770.58930.6419
    1999M4119.770.59740.650.59160.6444
    1999M5122.000.60230.65530.59610.6493
    1999M6120.720.59890.65140.59370.6467
    1999M7119.330.60670.66010.60130.655
    1999M8113.230.61620.67060.6090.6633
    1999M9106.880.60210.6550.59730.6506
    1999M10105.970.5950.64730.59040.6431
    1999M11104.650.58430.63580.57880.6305
    1999M12102.580.59680.64940.59190.6447
    2000M1105.300.59970.65240.59460.6477
    2000M2109.390.59320.64530.58470.6369
    2000M3106.310.60470.6580.59950.653
    2000M4105.630.6130.6670.60710.6613
    2000M5108.320.60880.66250.60620.6603
    2000M6106.130.64030.69670.63570.6925
    2000M7108.210.6410.69730.63550.6923
    2000M8108.080.64270.69950.63620.6931
    2000M9106.840.64760.70520.64420.7018
    2000M10108.440.67220.73160.6690.7288
    2000M11109.010.66520.7240.66120.7203
    2000M12112.210.67380.73390.67270.7329
    2001M1116.670.65690.71590.65570.7143
    2001M2116.230.65430.71340.64910.7072
    2001M3121.510.65910.71950.66030.7194
    2001M4123.770.66330.72420.6640.7233
    2001M5121.770.66650.72820.66850.7282
    2001M6122.350.66930.73110.67240.7324
    2001M7124.500.68140.74440.68410.7452
    2001M8121.370.67590.73590.67790.7379
    2001M9118.610.66140.71860.66740.7257
    2001M10121.450.65160.70810.65530.7126
    2001M11122.410.65640.71330.66150.7193
    2001M12127.590.66540.72170.66840.7265
    2002M1132.680.66110.71710.66580.7237
    2002M2133.640.66720.72370.67010.7283
    2002M3131.060.67420.72790.67460.7331
    2002M4130.770.67420.72790.67440.7329
    2002M5126.380.66380.71650.66510.7228
    2002M6123.290.65620.70840.65860.7145
    2002M7117.900.64810.69970.6480.703
    2002M8118.990.61690.66870.61660.6701
    2002M9121.080.62330.67580.62440.6787
    2002M10123.910.61380.66560.61660.6702
    2002M11121.610.61540.66730.61610.6697
    2002M12121.890.60980.66110.61080.6638
    2003M1118.810.60360.65440.6050.6575
    2003M2119.340.59580.64610.59330.6448
    2003M3118.690.59820.64870.59680.6487
    2003M4119.900.60710.65870.60640.6591
    2003M5117.370.6060.65760.60970.6627
    2003M6118.330.59170.64060.59150.6429
    2003M7118.700.58130.62920.57780.6279
    2003M8118.660.5940.64260.59160.643
    2003M9114.800.60380.65360.60320.6544
    2003M10109.500.59460.64370.59520.6456
    2003M11109.180.57330.6210.57290.6211
    2003M12107.740.56910.61660.56930.6172
    2004M1106.270.54920.59510.54930.5955
    2004M2106.710.53280.57760.52670.5713
    2004M3108.520.51860.56260.51490.5586
    2004M4107.660.53020.57490.52650.5712
    2004M5112.200.53460.57990.53320.5785
    2004M6109.430.54110.58690.53830.584
    2004M7109.490.5290.57390.52630.5706
    2004M8110.230.52370.56810.52180.5657
    2004M9110.090.52980.57480.52850.573
    2004M10108.780.53770.58330.53630.5815
    2004M11104.700.53650.58060.53370.5769
    2004M12103.810.52020.56310.51850.5605
    2005M1103.340.49950.54150.50020.5408
    2005M2104.940.51690.55970.51320.5544
    2005M3105.250.51320.55530.51120.5517
    2005M4 107.19        
    2005M5106.60    
    2005M6108.75    
    2005M7111.95    
    2005M8110.61    

     

    Figure 1b.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (British Pound), 6-month-ahead forecast

    Data for Figure 1b immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M50.59620.5720.74040.56380.738
    1990M60.58470.56060.72570.55530.7269
    1990M70.55250.54060.69940.53690.7029
    1990M80.52600.53250.69030.52270.6843
    1990M90.53210.55490.71670.54570.7144
    1990M100.51400.580.74770.54150.7089
    1990M110.50910.54480.70120.52860.6919
    1990M120.52030.52550.67590.51840.6785
    1991M10.51690.50040.64330.48990.6413
    1991M20.50910.48090.62090.46630.6104
    1991M30.54900.48460.62620.47080.6175
    1991M40.57150.4680.60730.45420.5965
    1991M50.58010.4520.59250.44520.5908
    1991M60.60620.46220.60560.4550.6039
    1991M70.60560.45550.59670.4520.5999
    1991M80.59380.45410.59480.44520.5909
    1991M90.57920.48520.63570.48010.6372
    1991M100.58030.51590.67620.49980.6633
    1991M110.56190.5120.67150.50730.6733
    1991M120.54730.53540.70250.530.7037
    1992M10.55280.53250.69980.52950.7055
    1992M20.56250.5280.69410.51920.6919
    1992M30.58010.51880.68170.50650.6749
    1992M40.56930.51910.68060.50750.6762
    1992M50.55260.50270.65660.49130.6548
    1992M60.53910.48930.6430.47850.6377
    1992M70.52150.49050.64390.48340.6441
    1992M80.51460.49750.65370.49180.6554
    1992M90.54160.51180.67250.50730.676
    1992M100.60500.50690.66660.49780.6633
    1992M110.65500.49790.65550.48320.6439
    1992M120.64470.48270.63550.47140.6281
    1993M10.65250.46860.61570.4560.6076
    1993M20.69470.46310.60790.450.5996
    1993M30.68410.48230.63040.47350.631
    1993M40.64740.5290.69130.5290.705
    1993M50.64610.57210.74480.57270.7638
    1993M60.66300.56580.73850.56380.7551
    1993M70.66870.57650.75010.57060.7644
    1993M80.67050.59390.77430.60740.8167
    1993M90.65580.59190.77060.59820.8086
    1993M100.66560.56410.73320.56610.7651
    1993M110.67530.56190.72980.5650.7636
    1993M120.67060.5780.75010.57980.7836
    1994M10.67010.57940.75120.58470.7903
    1994M20.67600.57650.7470.58630.7925
    1994M30.67030.56810.73320.57340.7751
    1994M40.67460.58060.74890.5820.7867
    1994M50.66480.58230.75070.59050.7981
    1994M60.65520.57670.74370.58640.7925
    1994M70.64650.5830.75180.5860.792
    1994M80.64840.57780.74540.59110.799
    1994M90.63850.57730.74560.58610.7922
    1994M100.62250.56830.73460.58990.7973
    1994M110.62920.56630.73230.58130.7857
    1994M120.64160.57110.73870.57290.7744
    1995M10.63510.5660.73210.56540.7641
    1995M20.63610.55980.72410.5670.7664
    1995M30.62490.5510.71270.55830.7547
    1995M40.62220.54080.69980.54430.7357
    1995M50.63000.54820.70970.55020.7437
    1995M60.62700.5520.71450.5610.7582
    1995M70.62690.56210.72840.55530.7506
    1995M80.63820.55660.72210.55630.7519
    1995M90.64140.54910.7130.54650.7386
    1995M100.63380.53820.69880.5440.7353
    1995M110.64000.54860.71240.55080.7445
    1995M120.64910.55210.7170.54830.7411
    1996M10.65410.55130.71510.54820.7409
    1996M20.65100.55550.72050.55810.7543
    1996M30.65480.55950.72040.56090.7581
    1996M40.65960.56580.72650.55420.749
    1996M50.66000.55950.71860.55960.7564
    1996M60.64870.55930.71850.56760.7672
    1996M70.64390.5760.74020.5720.7731
    1996M80.64520.56560.72720.56930.7694
    1996M90.64130.56890.73140.57260.7739
    1996M100.63040.57550.73960.57680.7796
    1996M110.60160.57880.74460.57710.78
    1996M120.60100.57570.74140.56720.7667
    1997M10.60300.57730.74380.5630.761
    1997M20.61520.56740.73120.56420.7625
    1997M30.62130.56490.72790.56080.758
    1997M40.61380.56330.7240.55120.7451
    1997M50.61270.54320.69790.5260.711
    1997M60.60790.54040.69110.52550.7103
    1997M70.59900.54630.69650.52720.7126
    1997M80.62360.55880.71190.53790.727
    1997M90.62450.56780.72230.54320.7343
    1997M100.61240.55970.71150.53670.7254
    1997M110.59210.56040.71190.53570.7241
    1997M120.60250.55930.71150.53160.7185
    1998M10.61160.55240.70260.52380.7079
    1998M20.60950.57780.73430.54530.7332
    1998M30.60170.58430.7430.54610.7316
    1998M40.59800.57850.7360.53550.7172
    1998M50.61040.57050.72490.51770.6905
    1998M60.60590.57610.73160.52690.7021
    1998M70.60840.58950.74970.53480.7127
    1998M80.61190.58040.73810.53290.7101
    1998M90.59440.57660.73080.52610.7011
    1998M100.59020.57110.72250.52290.6968
    1998M110.60200.60050.75870.53380.7113
    1998M120.59850.59590.75220.52980.706
    1999M10.60610.59060.74480.5320.7089
    1999M20.61440.60390.76130.5350.713
    1999M30.61680.58530.73750.51980.6926
    1999M40.62150.59250.74680.51610.6877
    1999M50.61900.59550.75070.52640.7015
    1999M60.62700.58840.74260.52340.6974
    1999M70.63490.6050.76290.530.7062
    1999M80.62270.59770.75550.53720.7159
    1999M90.61550.59550.75410.53930.7187
    1999M100.60340.60220.76380.54350.7242
    1999M110.61710.59640.74960.54130.7213
    1999M120.61990.60040.75420.54820.7305
    2000M10.60960.61190.76860.55520.7398
    2000M20.62500.59110.74280.54450.7256
    2000M30.63300.5830.73280.53820.7172
    2000M40.63200.57990.72910.52770.7031
    2000M50.66270.58620.73720.53960.7191
    2000M60.66260.59260.74550.5420.7223
    2000M70.66330.59750.75270.53310.7103
    2000M80.67160.59350.74940.54650.7283
    2000M90.69750.60250.76120.55340.7375
    2000M100.68940.59410.75130.55260.7364
    2000M110.70140.62130.78550.57950.7722
    2000M120.68360.62320.78760.57940.7721
    2001M10.67680.62930.7950.580.7729
    2001M20.68850.62150.78490.58730.7826
    2001M30.69230.64020.810.60990.8128
    2001M40.69700.63450.79980.60280.8032
    2001M50.70100.63150.7950.61330.8173
    2001M60.71330.62040.77490.59770.7964
    2001M70.70680.62150.77630.59180.7884
    2001M80.69580.61050.76060.6020.802
    2001M90.68320.6120.75520.60530.7888
    2001M100.68960.61030.74970.60940.7782
    2001M110.69660.60760.74590.6130.7796
    2001M120.69380.61580.75190.62370.7932
    2002M10.69820.61290.74830.6180.786
    2002M20.70290.59420.72570.60840.7738
    2002M30.70270.59430.72550.60370.7597
    2002M40.69300.59820.72990.61020.7669
    2002M50.68500.6060.73890.61750.7746
    2002M60.67400.60020.73170.61750.7716
    2002M70.64250.60790.74120.62180.7765
    2002M80.65070.60810.74160.6270.7816
    2002M90.64250.60910.74240.62690.7815
    2002M100.64210.59910.73080.61820.7707
    2002M110.63650.59160.72170.61110.7618
    2002M120.63040.6010.73320.60130.7495
    2003M10.61820.57940.7070.57320.7145
    2003M20.62190.57920.70660.58050.7236
    2003M30.63190.56910.69460.57320.7146
    2003M40.63540.57230.69970.57280.714
    2003M50.61640.56730.69470.56780.7078
    2003M60.60210.56270.6850.56240.701
    2003M70.61650.56840.68950.55150.6875
    2003M80.62740.56310.68110.55480.6916
    2003M90.61900.56640.68640.56370.7027
    2003M100.59550.55520.67250.56680.7065
    2003M110.59180.55490.67210.54990.6854
    2003M120.57090.55420.67070.53790.6695
    2004M10.54780.55660.67580.55310.6856
    2004M20.53550.56350.6840.56640.6977
    2004M30.54760.55530.67410.55890.6884
    2004M40.55460.54330.65860.53770.6623
    2004M50.55990.54360.65840.53430.6581
    2004M60.54710.53060.64390.51550.6349
    2004M70.54240.53060.64590.49140.6091
    2004M80.54940.51780.63090.48050.5955
    2004M90.55750.52090.63610.49130.609
    2004M100.55320.51990.6360.49760.6167
    2004M110.53740.52980.64750.50550.6226
    2004M120.51850.51910.6380.49860.6084
    2005M10.53200.51420.63290.49440.6031
    2005M20.52990.52020.63750.50070.6109
    2005M30.52510.52520.64360.50810.62
    2005M40.52740.52820.64730.50420.6151
    2005M50.53880.51080.62780.48980.5976
    2005M60.55010.49350.60640.47260.5766
    2005M70.57120.51830.6370.48490.5916
    2005M80.55730.51070.62790.4830.5893
    2005M90.55360.510.62730.47860.584

     

    Figure 1c.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (British Pound), 12-month-ahead forecast

    Data for Figure 1c immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M110.50910.5640.81060.53160.8054
    1990M120.52030.55280.79460.52360.7933
    1991M10.51690.53490.76770.50630.7671
    1991M20.50910.52830.75690.49290.7468
    1991M30.54900.54810.78480.51460.7797
    1991M40.57150.57610.82520.51060.7736
    1991M50.58010.54450.78060.49840.7551
    1991M60.60620.530.76080.48880.7405
    1991M70.60560.50520.72760.46190.6998
    1991M80.59380.4920.71090.43970.6662
    1991M90.57920.4930.71590.44480.6739
    1991M100.58030.47840.6920.42450.651
    1991M110.56190.46550.6750.4180.6448
    1991M120.54730.47120.69690.42720.659
    1992M10.55280.46280.68360.42440.6547
    1992M20.56250.46670.68280.4180.6449
    1992M30.58010.48940.71980.45080.6954
    1992M40.56930.51820.76190.46930.7239
    1992M50.55260.5040.74240.47630.7348
    1992M60.53910.52290.77030.49770.7677
    1992M70.52150.51590.75990.49720.767
    1992M80.51460.51550.75850.48750.7521
    1992M90.54160.50770.75020.47550.7336
    1992M100.60500.50840.75210.47650.7351
    1992M110.65500.49410.73010.46130.7117
    1992M120.64470.48730.71650.44930.6887
    1993M10.65250.48760.71860.45380.6943
    1993M20.69470.49370.72260.46180.7034
    1993M30.68410.50590.73840.47630.7255
    1993M40.64740.5050.73590.46740.7119
    1993M50.64610.50080.71720.45370.6911
    1993M60.66300.48580.69280.44260.6733
    1993M70.66870.47210.66490.42810.6477
    1993M80.67050.4660.65650.42250.6391
    1993M90.65580.47960.67310.44460.6726
    1993M100.66560.51450.72270.49670.7514
    1993M110.67530.550.7680.53770.8134
    1993M120.67060.54370.76120.52940.8008
    1994M10.67010.55040.7780.53570.8104
    1994M20.67600.55870.79350.57040.8628
    1994M30.67030.55790.79160.56170.8497
    1994M40.67460.53820.76250.53150.804
    1994M50.66480.53410.75650.53050.8024
    1994M60.65520.54670.77790.54440.8235
    1994M70.64650.54640.77730.5490.8351
    1994M80.64840.54220.77280.55050.8437
    1994M90.63850.53630.7640.53840.8252
    1994M100.62250.54630.77790.54650.8376
    1994M110.62920.54550.77660.55440.8498
    1994M120.64160.54160.77090.55060.8438
    1995M10.63510.54670.77810.55020.8432
    1995M20.63610.54050.76920.5550.8507
    1995M30.62490.54120.77010.55030.8434
    1995M40.62220.5330.75810.55390.8489
    1995M50.63000.53210.75670.54580.8365
    1995M60.62700.53910.76220.53790.8245
    1995M70.62690.53450.75550.53080.8136
    1995M80.63820.52860.74710.53240.816
    1995M90.64140.5210.73640.52420.8035
    1995M100.63380.51460.72740.51110.7833
    1995M110.64000.52050.73640.51660.7918
    1995M120.64910.52290.73940.52670.8073
    1996M10.65410.53430.75620.52140.7992
    1996M20.65100.52940.74950.52230.8005
    1996M30.65480.52680.74220.51310.7864
    1996M40.65960.51640.72720.51080.7829
    1996M50.66000.52590.740.51720.7927
    1996M60.64870.53110.74680.51480.7891
    1996M70.64390.52880.74320.51470.7888
    1996M80.64520.5320.74780.5240.8032
    1996M90.64130.53480.75030.52670.8072
    1996M100.63040.54260.75870.52030.7975
    1996M110.60160.53450.74740.52550.8053
    1996M120.60100.53260.74490.5330.8168
    1997M10.60300.54690.7650.5370.8231
    1997M20.61520.53740.7520.53450.8192
    1997M30.62130.53810.75360.53760.824
    1997M40.61380.55090.77150.54160.83
    1997M50.61270.55430.77560.54190.8305
    1997M60.60790.55580.77350.53260.8163
    1997M70.59900.55770.77460.52870.8103
    1997M80.62360.54990.76420.52970.8119
    1997M90.62450.54970.76290.52660.807
    1997M100.61240.54790.7610.51760.7933
    1997M110.59210.53530.7440.49390.757
    1997M120.60250.53460.74130.49340.7562
    1998M10.61160.53770.74540.4950.7587
    1998M20.60950.55070.76330.5050.7741
    1998M30.60170.55930.77520.51010.7759
    1998M40.59800.55310.76620.50390.7622
    1998M50.61040.55420.76730.5030.7575
    1998M60.60590.55440.76750.49910.7508
    1998M70.60840.54620.75730.49180.7383
    1998M80.61190.57120.79310.5120.7671
    1998M90.59440.58070.80650.51270.7667
    1998M100.59020.57870.80360.50280.7516
    1998M110.60200.57920.80420.48610.7173
    1998M120.59850.58610.81350.49470.7296
    1999M10.60610.59550.82640.50220.7407
    1999M20.61440.59180.82120.50040.738
    1999M30.61680.58410.81390.4940.7286
    1999M40.62150.58370.81650.4910.7241
    1999M50.61900.61450.85940.50120.7392
    1999M60.62700.6050.84580.49750.7337
    1999M70.63490.59480.83180.49950.7368
    1999M80.62270.61810.86380.50240.741
    1999M90.61550.59840.8330.4880.7198
    1999M100.60340.60260.8340.48460.7147
    1999M110.61710.5980.83020.49430.7277
    1999M120.61990.58810.81580.49140.7235
    2000M10.60960.59580.82670.49760.7326
    2000M20.62500.58810.81610.50440.7427
    2000M30.63300.58330.80870.50640.7456
    2000M40.63200.58920.81680.51030.7513
    2000M50.66270.58340.80840.50820.7483
    2000M60.66260.58460.81010.51470.7578
    2000M70.66330.5930.8220.52130.7674
    2000M80.67160.57560.79460.51130.7528
    2000M90.69750.56890.78260.50540.744
    2000M100.68940.57010.7840.49540.7294
    2000M110.70140.57420.7890.50670.7459
    2000M120.68360.58280.80080.5090.7493
    2001M10.67680.58770.80540.50050.7369
    2001M20.68850.58110.79560.51310.7555
    2001M30.69230.58780.79680.51960.7651
    2001M40.69700.58380.7750.51890.7639
    2001M50.70100.60420.79870.54410.8011
    2001M60.71330.60510.78560.5440.7895
    2001M70.70680.61070.78730.54460.783
    2001M80.69580.60340.77480.55150.7921
    2001M90.68320.62020.79020.57270.8218
    2001M100.68960.61110.77370.5660.806
    2001M110.69660.60640.76870.57590.8175
    2001M120.69380.59690.75240.56120.7968
    2002M10.69820.59110.74420.55570.7888
    2002M20.70290.58240.73220.56520.8024
    2002M30.70270.5840.73310.56840.8069
    2002M40.69300.58640.73450.57220.8124
    2002M50.68500.58460.73030.57560.8171
    2002M60.67400.58970.73550.58560.8314
    2002M70.64250.58820.73270.58030.8238
    2002M80.65070.5740.71480.57470.811
    2002M90.64250.57330.71460.56750.7963
    2002M100.64210.57640.71850.57650.8038
    2002M110.63650.580.72290.58240.8119
    2002M120.63040.57730.71910.5820.8087
    2003M10.61820.58080.72320.59290.8138
    2003M20.62190.57980.72180.59990.8192
    2003M30.63190.58110.72320.59980.8191
    2003M40.63540.5730.71360.59150.8078
    2003M50.61640.56570.70540.58470.7984
    2003M60.60210.5860.7290.57530.7856
    2003M70.61650.56550.70240.54840.7489
    2003M80.62740.56160.69530.55540.7584
    2003M90.61900.55590.68850.54840.7489
    2003M100.59550.55740.69190.5480.7483
    2003M110.59180.5560.68980.54320.7419
    2003M120.57090.55110.68510.53810.7348
    2004M10.54780.55660.6920.52770.7206
    2004M20.53550.55090.68480.53080.7249
    2004M30.54760.5520.68410.53930.7365
    2004M40.55460.54520.67630.54230.7405
    2004M50.55990.54780.68110.52610.7184
    2004M60.54710.54740.68120.51390.7017
    2004M70.54240.54720.68020.53090.7186
    2004M80.54940.55150.68530.54180.7312
    2004M90.55750.54780.68070.53640.7215
    2004M100.55320.53970.67060.51610.6941
    2004M110.53740.54460.67660.51280.6898
    2004M120.51850.53960.66990.49480.6654
    2005M10.53200.53650.66870.47470.6385
    2005M20.52990.52990.66330.46250.6242
    2005M30.52510.52740.66110.47290.6383
    2005M40.52740.52880.66320.47890.6464
    2005M50.53880.53430.67040.48350.6526
    2005M60.55010.52790.6630.47240.6376
    2005M70.57120.52870.6640.46840.6322
    2005M80.55730.53270.66880.47440.6403
    2005M90.55360.53430.6710.48140.6498
    2005M100.56650.53680.67430.47770.6447
    2005M110.57640.52670.66240.46410.6264
    2005M120.57280.51790.65320.44780.6044
    2006M10.56540.52990.66930.45940.6201
    2006M20.57210.52390.6620.45760.6177
    2006M30.57330.52490.66370.45350.6121
    2006M40.56560.51920.65770.45540.6147

     

    Figure 2a.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Deutschmark), 1-month-ahead forecast

    Data for Figure 2a immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1989M121.73781.73991.89891.73721.9062
    1990M11.69141.65221.80511.64971.8101
    1990M21.67581.59991.7461.60621.7619
    1990M31.70531.59831.74261.59871.7456
    1990M41.68631.61661.76281.62681.7762
    1990M51.66301.61081.75791.60871.7565
    1990M61.68321.58291.72741.58651.7322
    1990M71.63751.59391.73781.60581.7529
    1990M81.57021.54921.68981.56221.7054
    1990M91.57011.48081.61531.4981.6343
    1990M101.52381.48121.61611.49781.6341
    1990M111.48571.44411.57561.45371.586
    1990M121.49821.39911.52621.41741.5464
    1991M11.50911.41631.54531.42931.5594
    1991M21.48051.42061.55021.43961.5707
    1991M31.61221.39971.52721.41241.541
    1991M41.70271.52491.6621.5381.679
    1991M51.71991.62341.77411.62431.7736
    1991M61.78281.63931.79151.64081.7916
    1991M71.78521.70291.86141.70081.8571
    1991M81.74351.72331.88381.7031.8595
    1991M91.69331.65781.8111.66331.8161
    1991M101.68931.6091.75711.61541.7639
    1991M111.62081.63311.78331.61161.7596
    1991M121.56301.54311.68541.54621.6883
    1992M11.57881.48571.62271.49111.6281
    1992M21.61861.50471.64321.50621.6446
    1992M31.66161.54041.68251.54421.6857
    1992M41.64931.57971.7221.58521.7305
    1992M51.62251.57521.71651.57351.7177
    1992M61.57261.54691.68571.54791.6898
    1992M71.49141.4971.63211.50021.6377
    1992M81.44751.4211.55451.41621.5532
    1992M91.45141.37361.50161.37451.5074
    1992M101.48511.37551.50481.37821.5115
    1992M111.58751.41061.54311.41031.5467
    1992M121.58221.51471.65851.50761.6537
    1993M11.61441.5111.65391.50251.6481
    1993M21.64141.55781.70611.53311.6817
    1993M31.64661.5731.7231.55861.7097
    1993M41.59641.56911.71841.56361.7151
    1993M51.60711.52561.67061.5161.663
    1993M61.65471.53321.67911.52611.674
    1993M71.71571.58221.73331.57131.7236
    1993M81.69441.64581.8031.62921.7871
    1993M91.62191.60961.76361.6091.7649
    1993M101.64051.54221.68961.54021.6894
    1993M111.70051.5581.7071.55781.7088
    1993M121.71051.62271.77731.61481.7713
    1994M11.74261.6341.78981.62431.7818
    1994M21.73551.66871.82831.65481.8152
    1994M31.69091.65981.81821.64811.8078
    1994M41.69841.61081.76381.60581.7614
    1994M51.65651.61971.77361.61281.7692
    1994M61.62711.58561.73581.5731.7255
    1994M71.56741.55211.69821.54511.6949
    1994M81.56461.49991.64081.48841.6326
    1994M91.54911.49481.63551.48571.6297
    1994M101.51951.47471.61451.47111.6137
    1994M111.53961.44961.58721.4431.5828
    1994M121.57161.47091.61091.4621.6037
    1995M11.53021.50331.64691.49241.6371
    1995M21.50221.4651.60331.45311.5939
    1995M31.40611.44051.57571.42651.5647
    1995M41.38121.34141.47081.33481.4646
    1995M51.40961.31861.44581.31131.4388
    1995M61.40121.34941.47681.33861.4683
    1995M71.38861.34211.46831.33061.4595
    1995M81.44561.33211.45731.31861.4464
    1995M91.46011.38521.51511.37271.5058
    1995M101.41431.39811.52961.38651.5209
    1995M111.41731.35411.4811.3431.4731
    1995M121.44061.36081.48821.34591.4764
    1996M11.46351.38591.51541.36811.5007
    1996M21.46691.41.53121.38971.5244
    1996M31.47761.40971.54321.39311.5281
    1996M41.50441.41361.54741.40311.5391
    1996M51.53241.43981.57761.42861.5671
    1996M61.52821.46811.60951.45511.5962
    1996M71.50251.4651.60651.45121.5919
    1996M81.48261.44041.57941.42681.565
    1996M91.50801.41971.55651.40791.5443
    1996M101.52771.44251.58151.4321.5708
    1996M111.51181.46151.60121.45081.5911
    1996M121.55251.44651.58391.43561.5744
    1997M11.60471.49591.63021.47431.6169
    1997M21.67471.54761.68621.52381.6711
    1997M31.69461.61171.75561.59031.7444
    1997M41.71191.62811.77341.60911.7651
    1997M51.70481.64421.7911.62561.7832
    1997M61.72771.64551.79171.61881.7757
    1997M71.79391.66061.80751.64071.7997
    1997M81.84001.72891.88241.70351.8686
    1997M91.78621.76741.92581.74731.9167
    1997M101.75751.71171.86371.69621.8595
    1997M111.73231.68371.83381.6691.8296
    1997M121.77881.66411.81281.64511.8034
    1998M11.81651.711.86121.68911.8513
    1998M21.81231.73721.89321.7251.8906
    1998M31.82721.73391.89191.7211.8863
    1998M41.81321.74071.90181.73521.9018
    1998M51.77531.73951.89031.73191.8872
    1998M61.79281.70571.85381.69571.8478
    1998M71.79761.72031.86971.71241.866
    1998M81.78691.72511.87491.7171.8711
    1998M91.69901.71191.86051.70681.8599
    1998M101.63811.62761.77161.61531.7683
    1998M111.68271.56661.70731.55741.7049
    1998M121.66981.6161.75911.59981.7514

     

    Figure 2b.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Deutschmark), 6-month-ahead forecast

    Data for Figure 2b immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M51.66301.60492.13311.5732.106
    1990M61.68321.54842.05621.49531.9999
    1990M71.63751.45711.93561.45541.9466
    1990M81.57021.48171.96951.4421.9286
    1990M91.57011.45961.94081.46731.9517
    1990M101.52381.49521.96121.45091.93
    1990M111.48571.4521.90051.43091.9033
    1990M121.49821.42591.86411.44831.9265
    1991M11.50911.38951.82181.4091.8742
    1991M21.48051.31311.72231.35111.7971
    1991M31.61221.31591.72671.35091.797
    1991M41.70271.33431.74861.31111.744
    1991M51.71991.2411.62861.27841.7005
    1991M61.78281.28981.69391.28921.7148
    1991M71.78521.26181.65961.29851.7272
    1991M81.74351.28131.68521.27391.6945
    1991M91.69331.33591.75281.38721.8452
    1991M101.68931.4561.91081.46511.9488
    1991M111.62081.48041.96711.47991.9794
    1991M121.56301.55212.06521.5342.0639
    1992M11.57881.68472.23881.5362.0687
    1992M21.61861.51422.0111.50022.0348
    1992M31.66161.4681.94921.4571.9762
    1992M41.64931.65272.19451.45351.9715
    1992M51.62251.46231.9411.39461.8916
    1992M61.57261.39091.8531.34491.8241
    1992M71.49141.41841.89471.35851.8426
    1992M81.44751.42821.90961.39281.8891
    1992M91.45141.43771.9211.42981.9392
    1992M101.48511.46331.95741.41921.925
    1992M111.58751.42941.91171.39611.8936
    1992M121.58221.38081.84631.35311.8353
    1993M11.61441.34021.7911.28331.7405
    1993M21.64141.26761.69431.24551.6893
    1993M31.64661.2631.68551.24881.6938
    1993M41.59641.30091.73741.27791.7333
    1993M51.60711.42341.90161.3661.8528
    1993M61.65471.42631.90351.36141.8465
    1993M71.71571.55092.06961.38921.8842
    1993M81.69441.51322.02291.41231.9155
    1993M91.62191.47141.96751.41681.9217
    1993M101.64051.44991.93861.37371.8632
    1993M111.70051.44781.93581.38281.8755
    1993M121.71051.50792.0161.42381.9311
    1994M11.74261.5832.11611.47622.0023
    1994M21.73551.49371.99661.45791.9774
    1994M31.69091.43841.92231.39561.8929
    1994M41.69841.44441.93041.41161.9146
    1994M51.65651.53062.04541.46321.9846
    1994M61.62711.54982.07091.47181.9963
    1994M71.56741.59812.13521.49952.0338
    1994M81.56461.58132.11161.49332.0255
    1994M91.54911.50652.00931.4551.9735
    1994M101.51951.52512.03141.46141.9822
    1994M111.53961.52112.02321.42531.9332
    1994M121.57161.46581.94261.41.8989
    1995M11.53021.43341.90541.34861.8292
    1995M21.50221.41621.8841.34621.8259
    1995M31.40611.38181.8371.3331.808
    1995M41.38121.36951.82391.30751.7734
    1995M51.40961.3961.85881.32471.7968
    1995M61.40121.4391.911.35231.8342
    1995M71.38861.40481.86591.31671.7859
    1995M81.44561.39021.84161.29251.7531
    1995M91.46011.29291.71181.20991.641
    1995M101.41431.27731.69071.18851.612
    1995M111.41731.30121.72111.21291.6451
    1995M121.44061.29651.71691.20561.6353
    1996M11.46351.29551.71671.19481.6206
    1996M21.46691.33041.76311.24381.6871
    1996M31.47761.3381.77291.25631.704
    1996M41.50441.30051.72341.21691.6505
    1996M51.53241.32271.75291.21961.6542
    1996M61.52821.35421.7941.23961.6814
    1996M71.50251.33941.7721.25921.708
    1996M81.48261.37491.81671.26231.7121
    1996M91.50801.35661.7911.27141.7244
    1996M101.52771.38621.82731.29451.7558
    1996M111.51181.4161.86681.31851.7884
    1996M121.55251.4181.86951.3151.7835
    1997M11.60471.39761.84251.29281.7535
    1997M21.67471.37231.80771.27571.7303
    1997M31.69461.38631.82571.29761.76
    1997M41.71191.40721.85351.31461.783
    1997M51.70481.39451.83481.30081.7644
    1997M61.72771.441.8951.33591.8119
    1997M71.79391.48981.96021.38071.8727
    1997M81.84001.53132.01681.44091.9544
    1997M91.78621.53722.02251.45811.9776
    1997M101.75751.54642.03761.4731.9838
    1997M111.73231.57962.0851.46681.9735
    1997M121.77881.56382.0621.48661.9774
    1998M11.81651.64682.15381.54362.0352
    1998M21.81231.66582.16321.58332.0865
    1998M31.82721.60172.06921.5372.024
    1998M41.81321.5772.03371.51231.9852
    1998M51.77531.57692.03341.49061.9568
    1998M61.79281.62422.09411.53052.0091
    1998M71.79761.62372.09381.5632.0518
    1998M81.78691.6272.09871.55942.0471
    1998M91.69901.61672.08561.57222.0639
    1998M101.63811.62082.09111.56022.0481
    1998M111.68271.60312.06841.52762.0053
    1998M121.66981.60792.07271.54262.0251

     

    Figure 2c.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Deutschmark), 12-month-ahead forecast

    Data for Figure 2c immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M111.48571.4462.16261.38782.1567
    1990M121.49821.39322.08331.31782.0481
    1991M11.50911.34012.00371.28271.9935
    1991M21.48051.35082.01981.27091.9751
    1991M31.61221.3482.01581.29322.0097
    1991M41.70271.35932.03841.27881.9873
    1991M51.71991.32841.99321.26111.9599
    1991M61.78281.31841.97731.27651.9838
    1991M71.78521.28561.92651.24181.93
    1991M81.74351.22911.83881.19081.8506
    1991M91.69331.22751.83351.19071.8504
    1991M101.68931.22581.82841.15561.7959
    1991M111.62081.17071.73411.12671.751
    1991M121.56301.18481.76411.13621.7658
    1992M11.57881.16211.72961.14441.7786
    1992M21.61861.17111.73381.12281.7449
    1992M31.66161.21871.8161.22261.9001
    1992M41.64931.2961.92861.29122.0067
    1992M51.62251.3141.95511.30432.0271
    1992M61.57261.35332.01351.3522.1012
    1992M71.49141.41822.11161.35382.1039
    1992M81.44751.33831.99541.32222.0548
    1992M91.45141.31721.96971.28421.9957
    1992M101.48511.37622.05741.28111.9909
    1992M111.58751.29151.93111.22911.9102
    1992M121.58221.25381.87471.18531.8421
    1993M11.61441.27451.9061.19731.8608
    1993M21.64141.3011.9451.22751.9077
    1993M31.64661.32651.98121.26011.9583
    1993M41.59641.33681.99641.25081.9439
    1993M51.60711.31511.96351.23051.9123
    1993M61.65471.27721.90881.19261.8534
    1993M71.71571.2351.84741.1311.7577
    1993M81.69441.19061.78091.09771.7059
    1993M91.62191.191.77621.10061.7105
    1993M101.64051.21681.82051.12631.7503
    1993M111.70051.31.9461.20391.8711
    1993M121.71051.30451.95181.19991.8647
    1994M11.74261.36182.03721.22431.9027
    1994M21.73551.3672.04541.24471.9344
    1994M31.69091.35412.02941.24871.9406
    1994M41.69841.32871.99141.21071.8816
    1994M51.65651.33061.99421.21871.894
    1994M61.62711.37052.0541.25481.9501
    1994M71.56741.4262.13211.30112.022
    1994M81.56461.38742.07161.28491.9969
    1994M91.54911.34722.0091.231.9115
    1994M101.51951.35762.02561.24411.9334
    1994M111.53961.40922.10291.28962.0041
    1994M121.57161.42192.12061.29722.016
    1995M11.53021.45962.17471.32152.0538
    1995M21.50221.45372.16441.31612.0454
    1995M31.40611.41182.10111.28241.9929
    1995M41.38121.42122.11451.2882.0017
    1995M51.40961.41212.09881.25621.9523
    1995M61.40121.37962.0511.23391.9176
    1995M71.38861.35172.00751.18861.8473
    1995M81.44561.34842.00371.18651.8439
    1995M91.46011.32511.96481.17481.8258
    1995M101.41431.31341.94881.15231.7909
    1995M111.41731.33531.97671.16751.8145
    1995M121.44061.3652.01981.19181.8522
    1996M11.46351.35141.99521.16041.8034
    1996M21.46691.3291.96421.13921.7704
    1996M31.47761.26691.87381.06631.6572
    1996M41.50441.24251.85471.04751.6279
    1996M51.53241.25821.87311.0691.6613
    1996M61.52821.25911.87431.06261.6514
    1996M71.50251.24981.8591.05311.6366
    1996M81.48261.29791.93261.09631.7037
    1996M91.50801.3031.94021.10731.7208
    1996M101.52771.29441.92421.07251.6668
    1996M111.51181.29291.92011.07491.6705
    1996M121.55251.30281.93521.09251.6979
    1997M11.60471.3151.95381.10981.7248
    1997M21.67471.3221.9641.11251.7289
    1997M31.69461.33411.98041.12051.7414
    1997M41.71191.35952.01711.14091.773
    1997M51.70481.36282.021.16211.806
    1997M61.72771.36792.0281.15891.8011
    1997M71.79391.36282.02121.13941.7707
    1997M81.84001.33971.98861.12431.7473
    1997M91.78621.35052.00441.14361.7773
    1997M101.75751.36652.02621.15861.7973
    1997M111.73231.3512.00141.14651.7786
    1997M121.77881.3592.01311.17741.8265
    1998M11.81651.39462.06441.21691.8784
    1998M21.81231.43992.12791.271.9576
    1998M31.82721.45632.13421.28511.9682
    1998M41.81321.45912.12981.29821.9693
    1998M51.77531.46492.12681.29281.9589
    1998M61.79281.45242.10211.31021.9814
    1998M71.79761.49732.16711.36042.0573
    1998M81.78691.54172.2541.39542.1145
    1998M91.69901.50632.18671.35462.0548
    1998M101.63811.482.151.33282.0218
    1998M111.68271.47172.14041.31381.9929
    1998M121.66981.50162.17921.34892.0462

     

    Figure 3a.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Japanese Yen), 1-month-ahead forecast

    Data for Figure 3a immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1989M12143.69137.1448150.3042135.8702149.366
    1990M1144.98137.0572150.1959136.0333149.5454
    1990M2145.69138.3936151.6314137.2494150.8823
    1990M3153.31139.0866152.3841137.9236151.6234
    1990M4158.46146.6827160.6354145.1402159.9882
    1990M5154.04151.6278165.9187150.0097165.3559
    1990M6153.70147.417161.4377145.8239160.7419
    1990M7149.04146.9849161.1507145.5035159.9562
    1990M8147.46142.2518156.0701141.0903155.1046
    1990M9138.44140.3027154.2165139.6026153.4539
    1990M10129.59131.1932144.3835130.8171144.0557
    1990M11129.22122.5274134.9261122.4619134.855
    1990M12133.89122.3886134.7416122.1073134.4645
    1991M1133.70126.9561139.8379126.5199139.3237
    1991M2130.54126.7481139.5959126.3429139.1288
    1991M3137.39123.6171136.2016123.3591135.843
    1991M4137.11130.1833143.4535129.8266142.9793
    1991M5138.22129.8952143.1449129.5672142.6936
    1991M6139.75131.0981144.4562130.6079143.8398
    1991M7137.83132.6852146.2326132.0658145.4453
    1991M8136.82130.782144.1128130.2427143.4376
    1991M9134.30129.7122142.9256129.2954142.3943
    1991M10130.77127.3166140.3002126.9128139.7702
    1991M11129.63123.5467136.1673123.569136.0878
    1991M12128.04122.755135.2936122.4986134.9089
    1992M1125.46121.3312133.7332120.989133.2464
    1992M2127.70118.7918130.9355118.5577130.5688
    1992M3132.86120.9751133.3118120.6749132.9004
    1992M4133.54125.7367138.524125.5495138.2689
    1992M5130.77126.1439138.9549126.1914138.9758
    1992M6126.84123.6608136.3031123.569136.0878
    1992M7125.88120.1263132.4361119.8571131.9997
    1992M8126.23119.3691131.5722118.9496131.0004
    1992M9122.60119.3371131.5382119.2831131.3677
    1992M10121.17115.9207127.7959115.8504127.5872
    1992M11123.88114.63126.3828114.5029126.1031
    1992M12124.04117.1965129.206117.0616128.921
    1993M1124.99117.1537129.2048117.2138129.0887
    1993M2120.76118.3556130.3984118.1081130.0735
    1993M3117.02114.2326125.9636114.1142125.6751
    1993M4112.41110.5448121.905110.5757121.778
    1993M5110.34106.04116.9426106.2293116.9913
    1993M6107.41104.3046115.0288104.2717114.8354
    1993M7107.69101.5958112.0406101.5042111.7875
    1993M8103.77101.609112.0558101.7684112.0786
    1993M9105.5798.0503108.12998.062107.9966
    1993M10107.0299.7681110.025399.7633109.8702
    1993M11107.88101.3172111.7358101.1293111.3747
    1993M12109.91102.1469112.6526101.9416112.2692
    1994M1111.44103.7283114.2849103.8658114.3884
    1994M2106.30105.3095116.0551105.3091115.9779
    1994M3105.10100.5524110.7573100.454110.631
    1994M4103.4899.1887109.222599.3153109.3769
    1994M5103.7597.6774107.540597.7878107.6947
    1994M6102.5397.9322107.884598.0424107.975
    1994M798.4597.1121107.036496.8923106.7084
    1994M899.9493.1883102.728593.028102.4526
    1994M998.7794.3563103.998794.4433104.0113
    1994M1098.3593.2214102.747393.3355102.7912
    1994M1198.0492.6616102.154792.935102.3502
    1994M12100.1892.7087102.243292.6473102.0334
    1995M199.7794.7109104.411994.6703104.2613
    1995M298.2494.3687104.068494.2829103.8347
    1995M390.5293.1143102.693593102.2376
    1995M483.6985.585794.405685.695594.2075
    1995M585.1178.841286.963779.059487.095
    1995M684.6480.250788.537780.398988.5706
    1995M787.4079.870888.031379.957988.076
    1995M894.7482.590591.039882.566290.9491
    1995M9100.5589.528698.756189.496598.593
    1995M10100.8494.8839104.68194.9927104.9307
    1995M11101.9495.4478105.313895.259105.2249
    1995M12101.8596.3677106.282796.3031106.0913
    1996M1105.7596.1693106.050496.2164105.9959
    1996M2105.79100.1183110.412999.903110.0572
    1996M3105.94100.1107110.400599.943110.1012
    1996M4107.20100.1748110.4614100.083110.2555
    1996M5106.34101.2044111.6215101.271111.5642
    1996M6108.96100.4388110.7321100.454110.6642
    1996M7109.19103.0411113.5438102.9352113.3862
    1996M8107.87103.2287113.739103.1516113.6246
    1996M9109.93101.9811112.3662101.9008112.2468
    1996M10112.41103.7504114.3077103.8451114.3884
    1996M11112.30106.203117.0035106.1974116.9797
    1996M12113.98106.268117.0627106.0913116.8627
    1997M1117.91107.7368118.645107.8995118.6052
    1997M2122.96111.5738122.8637111.62122.6948
    1997M3122.77116.3477128.1381116.4079127.9705
    1997M4125.64116.0634127.8241116.2217127.7659
    1997M5119.19118.0081129.999118.9377130.7517
    1997M6114.29112.3734123.9277112.832124.0395
    1997M7115.38107.9781119.0616108.1912118.9377
    1997M8117.93109.1976120.4083109.2239120.073
    1997M9120.89111.3451122.7849111.6423122.7316
    1997M10121.06113.7762125.4698114.4456125.8134
    1997M11125.38114.2197125.9511114.606125.9897
    1997M12129.73118.6781130.869118.6882130.4774
    1998M1129.55122.415135.0145122.8176135.0169
    1998M2125.85122.3367134.922122.6457134.828
    1998M3129.08118.8284131.018119.1401130.9742
    1998M4131.75121.5706134.0612122.1928134.3301
    1998M5134.90124.2904137.0916124.7236137.1123
    1998M6140.33127.2105140.3396127.7021140.3866
    1998M7140.79132.9272146.6644132.8473146.0428
    1998M8144.68133.49147.289133.2864146.5256
    1998M9134.48136.9805151.1832136.9615150.5658
    1998M10121.05126.39139.4667127.0397139.9381
    1998M11120.29113.383125.1976114.2284125.9645
    1998M12117.07113.0988124.8832113.511125.1734
    1999M1113.29110.2031121.6818110.4762121.8268
    1999M2116.67106.9306117.9395106.9114117.8721
    1999M3119.47110.014121.3704110.0902121.3768
    1999M4119.77112.554124.1653112.7418124.3002
    1999M5122.00112.8164124.4674113.024124.6114
    1999M6120.72114.6104126.2066115.1229126.9255
    1999M7119.33113.6874125.1962113.9204125.5997
    1999M8113.23112.8048124.2021112.7305124.1512
    1999M9106.88106.3352117.0174106.9648117.8014
    1999M10105.97100.6024110.7098100.8869111.1966
    1999M11104.6599.5617109.6013100.033110.2555
    1999M12102.5898.9207108.904998.7805108.875
    2000M1105.3096.6317106.370396.8245106.7191
    2000M2109.3999.2742109.346199.3948109.5521
    2000M3106.31103.6896114.2491103.2548113.8065
    2000M4105.63100.4624110.6755100.3536110.6088
    2000M5108.3299.0885109.159899.7034109.8922
    2000M6106.13101.8785112.156102.2479112.6967
    2000M7108.21100.4251110.6095100.1831110.421
    2000M8108.08102.268112.6512102.1457112.584
    2000M9106.84101.3201111.6058102.0232112.449
    2000M10108.44101.0619111.3277100.8465111.1522
    2000M11109.01102.1351112.5001102.3604112.8207
    2000M12112.21102.8055113.245102.8941113.4089
    2001M1116.67105.3585116.0631105.9217116.7459
    2001M2116.23110.0807121.49110.1232121.3768
    2001M3121.51109.802121.0614109.7165120.9165
    2001M4123.77114.3424126.172114.6977126.4188
    2001M5121.77116.2528128.27116.8277128.7664
    2001M6122.35114.4249126.5201114.9388126.6845
    2001M7124.50115.037127.2639115.4919127.2941
    2001M8121.37116.5541128.9739117.519129.5284
    2001M9118.61113.2041125.2614114.5601126.2672
    2001M10121.45111.7232123.1354111.9553123.3962
    2001M11122.41113.2307124.8044114.6404126.3556
    2001M12127.59114.8505126.5979115.5496127.3577
    2002M1132.68118.8042131.4102120.4338132.7808
    2002M2133.64124.2441137.4541125.236138.0754
    2002M3131.06125.6902139.0484126.141139.0731
    2002M4130.77122.6819135.7181123.7174136.4011
    2002M5126.38122.2512135.2525123.4332136.0878
    2002M6123.29117.9296130.4507119.3905131.5254
    2002M7117.90115.6443127.8922116.4661128.3037
    2002M8118.99111.0714122.8514111.3747122.6948
    2002M9121.08111.6028123.4421112.4041123.8288
    2002M10123.91114.0112125.7751114.6289126.0149
    2002M11121.61116.862128.9033117.3077128.9597
    2002M12121.89114.3845126.1665115.1229126.5579
    2003M1118.81114.5082126.3267115.388126.8493
    2003M2119.34112.4318124.0381112.4715123.6432
    2003M3118.69113.413125.0666113.0353124.2008
    2003M4119.90112.0637123.5696112.4153123.5196
    2003M5117.37112.4222123.9644113.5678124.786
    2003M6118.33110.19121.5344111.1633122.1439
    2003M7118.70111.8546123.2355112.0786123.1127
    2003M8118.66112.0936123.4951112.4265123.4949
    2003M9114.80111.9399123.316112.3928123.4579
    2003M10109.50108.3948119.4097108.7335119.4383
    2003M11109.18103.1588113.6451103.7102113.9204
    2003M12107.74103.2173113.6914103.5754113.5905
    2004M1106.27101.4557111.7814102.207112.0898
    2004M2106.71100.9333111.1857100.8163110.5646
    2004M3108.52101.1693111.4677101.2305111.0188
    2004M4107.66102.8155113.2199102.9455112.8997
    2004M5112.20101.8971112.202102.1355112.0113
    2004M6109.43106.357117.0372106.442116.9329
    2004M7109.49103.8684113.785103.8347114.0458
    2004M8110.23103.9626113.8367104.4282114.1028
    2004M9110.09104.4655114.3732105.1408114.8814
    2004M10108.78104.3049114.1881105.0042114.7321
    2004M11104.70103.1904112.9815103.7516113.3636
    2004M12103.8199.5597109.067999.8631109.1147
    2005M1103.3498.6076108.035399.0178108.1912
    2005M2104.9498.4622107.865398.5634107.6947
    2005M3105.25100.4329109.9926100.093109.1802
    2005M4107.19100.3011109.8516100.3837109.4973
    2005M5106.60102.2425111.9461102.2376111.5196
    2005M6108.75100.8962110.4973101.6769110.9079
    2005M7111.95103.5451113.4482103.7309113.1484
    2005M8110.61106.7007116.8631106.7831116.4777
    2005M9111.24105.264115.3071105.4988115.0768
    2005M10114.87106.3474116.4835106.1019115.7346
    2005M11118.45109.1451119.4848109.563119.51
    2005M12118.46112.01122.5664112.9788123.2359
    2006M1115.48111.7955122.1451112.9901123.2359
    2006M2117.86110.413120.5558110.1453120.085
    2006M3117.28112.5427122.8268112.4153122.5599
    2006M4117.07111.7563121.9831111.8658121.9608
    2006M5111.73111.9335122.1922111.6646121.7415
    2006M6114.63106.1331115.9514106.5698116.1869

     

    Figure 3b.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Japanese Yen), 6-month-ahead forecast

    Data for Figure 3b immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M5154.04126.5472171.9341118.5696160.5973
    1990M6153.70125.2612170.1406118.712160.7901
    1990M7149.04126.4843171.7585119.7732162.2276
    1990M8147.46126.815171.2492120.3615163.0244
    1990M9138.44133.277180.0206126.6592171.2972
    1990M10129.59136.6261185.0265130.9087177.0443
    1990M11129.22133.7383180.8796127.2559172.1042
    1990M12133.89134.3002181.6167126.9762171.726
    1991M1133.70130.809176.8975123.125166.5174
    1991M2130.54129.4392174.9506121.8268164.7617
    1991M3137.39120.7606163.0848114.3656154.671
    1991M4137.11112.4895151.8927106.155144.7923
    1991M5138.22111.7187150.9232105.8476144.373
    1991M6139.75114.3646153.4259109.6726149.5903
    1991M7137.83113.0787151.925109.5192149.381
    1991M8136.82110.3666148.0935106.9327145.8531
    1991M9134.30114.8958154.0108112.539153.4999
    1991M10130.77115.1056154.4195112.3142153.1932
    1991M11129.63116.8139156.7761113.2163154.4237
    1991M12128.04118.9457159.6412114.48156.1473
    1992M1125.46117.3254157.502112.8997153.9919
    1992M2127.70116.4048156.4145112.0786152.8719
    1992M3132.86114.6656153.9692110.0132150.0547
    1992M4133.54110.3883148.0732107.1147146.1013
    1992M5130.77110.5288148.4431106.1868144.8357
    1992M6126.84109.4923147.1243104.8782143.0508
    1992M7125.88106.8164143.6438102.7707140.1762
    1992M8126.23108.481145.9819104.6059142.6794
    1992M9122.60111.8873150.6733108.8314148.4428
    1992M10121.17111.6999150.5394109.3879149.2018
    1992M11123.88110.6138149.2283107.1147146.1013
    1992M12124.04108.06145.8709103.897141.7124
    1993M1124.99107.8631145.6424103.1104140.6395
    1993M2120.76106.9894144.4981103.3995141.0339
    1993M3117.02103.8831140.3355100.4239136.9752
    1993M4112.41103.2573139.488399.2558135.3819
    1993M5110.34105.4319142.3876101.4737138.4072
    1993M6107.41104.9019141.5134101.6057138.5872
    1993M7107.69106.6669143.9181102.3809139.6445
    1993M8103.77102.793138.664398.9189134.9224
    1993M9105.5799.7553134.464295.8515130.7386
    1993M10107.0295.4726128.703292.0839125.5997
    1993M11107.8894.5428127.066790.387123.2852
    1993M12109.9192.5148124.195587.988120.013
    1994M1111.4491.6733123.144188.217120.3254
    1994M2106.3089.0754119.51485.0041115.9432
    1994M3105.1090.3351121.221286.4789117.9546
    1994M4103.4892.1319123.569587.663119.5698
    1994M5103.7592.8297124.49288.3671120.5302
    1994M6102.5393.4006125.246690.0351122.8053
    1994M798.4595.1951127.578191.2862124.5117
    1994M899.9491.5529122.425587.0776118.7713
    1994M998.7790.0621120.384486.0906117.425
    1994M1098.3588.6525118.566984.7665115.619
    1994M1198.0488.9276119.132884.9871115.92
    1994M12100.1888.7033118.90783.9902114.5601
    1995M199.7785.0085113.995980.6404109.9912
    1995M298.2485.1437114.186881.8673111.6646
    1995M390.5284.181112.74980.907110.3547
    1995M483.6983.4181111.587281.2475109.8812
    1995M585.1184.178112.519581.1501109.5411
    1995M684.6485.8576114.64483.0464111.9329
    1995M787.4086.7068115.205382.7066111.475
    1995M894.7485.4649113.340681.4346109.7604
    1995M9100.5579.1169104.144475.0384101.1394
    1995M10100.8472.03695.464969.373293.5036
    1995M11101.9473.386996.659170.548595.0877
    1995M12101.8572.482395.666170.161594.415
    1996M1105.7574.547198.839872.450297.4072
    1996M2105.7980.0589106.448678.5315105.5622
    1996M3105.9484.2908112.254783.3543112.0449
    1996M4107.2085.4273114.331483.588112.3816
    1996M5106.3486.0601115.865384.5041113.8976
    1996M6108.9686.0144115.83884.4281113.966
    1996M7109.1990.2576121.506187.663118.3327
    1996M8107.8790.2467121.668687.6981118.38
    1996M9109.9390.1027121.657687.8209118.5459
    1996M10112.4190.9335123.27488.8634119.7732
    1996M11112.3090.343122.342888.1465118.7476
    1996M12113.9892.7838125.477990.3237121.6807
    1997M1117.9192.8799125.448890.5136121.9364
    1997M2122.9691.8122123.950989.416120.4579
    1997M3122.7793.1062125.62391.1221122.7562
    1997M4125.6495.2381128.471693.1862125.5369
    1997M5119.1995.481128.583893.0931125.4115
    1997M6114.2996.1425129.817494.4811127.2814
    1997M7115.3899.5392134.328897.7389131.6702
    1997M8117.93103.7282139.7992101.9314137.593
    1997M9120.89103.2951139.2933101.7684137.373
    1997M10121.06104.1555140.3126104.1466140.5833
    1997M11125.38100.3373135.083198.8002133.3664
    1997M12129.7396.9513130.587494.7366127.881
    1998M1129.5598.0285132.146595.6408129.1016
    1998M2125.8599.8793134.930697.7585131.9602
    1998M3129.08101.9423136.3365100.2132135.1115
    1998M4131.75102.4976136.8599100.3536135.2061
    1998M5134.90106.1825141.7347103.9282140.0221
    1998M6140.33109.4348146.1606107.544144.9951
    1998M7140.79109.3473146.128107.3935144.9661
    1998M8144.68106.6326142.5158104.3238140.8225
    1998M9134.48109.1187145.7877106.9969144.4307
    1998M10121.05111.4806148.8975109.213147.4221
    1998M11120.29113.9107152.4394111.8211150.9427
    1998M12117.07118.3852158.6411116.3264157.0242
    1999M1113.29118.8181159.341116.7109157.5432
    1999M2116.67122.3459164.2871119.929161.8872
    1999M3119.47114.2203152.7245111.475150.295
    1999M4119.77103.9364138.6279100.3436135.2872
    1999M5122.00103.0983136.873499.7134134.4376
    1999M6120.72100.099132.906497.0474130.8432
    1999M7119.3396.687127.875893.5972126.6212
    1999M8113.2398.1602130.221795.4879130.3861
    1999M9106.8899.9288132.727597.7878133.5265
    1999M10105.97100.0689132.869598.0326133.8607
    1999M11104.65101.9217135.23399.8531136.3466
    1999M12102.58101.2602134.227698.8101134.9224
    2000M1105.30100.3604133.177797.6705133.3664
    2000M2109.3995.6659126.882492.6751126.5453
    2000M3106.3191.0664120.66987.4791119.4503
    2000M4105.6390.1092119.589986.7387118.4392
    2000M5108.3289.1164118.572685.6526116.9563
    2000M6106.1387.0437115.921783.9566114.6404
    2000M7108.2188.8145118.367786.1853117.6836
    2000M8108.0891.7752122.290889.5323122.2539
    2000M9106.8489.5391119.543887.0167118.8188
    2000M10108.4489.0509118.99886.4529118.049
    2000M11109.0191.1302121.566888.6592121.0617
    2000M12112.2189.8777119.95286.8689118.617
    2001M1116.6791.1593121.718188.5706120.9407
    2001M2116.2390.9983121.462688.4644120.7956
    2001M3121.5190.0906119.984587.4441119.4025
    2001M4123.7791.2234121.492888.7568121.1949
    2001M5121.7791.9352122.03489.2195121.8268
    2001M6122.3594.5181124.846791.8448125.4115
    2001M7124.5097.3128.03595.4879130.3861
    2001M8121.3796.9839127.056195.1353129.9046
    2001M9118.6199.9774131.11899.4545135.9653
    2001M10121.45101.3019132.5279101.3014138.9758
    2001M11122.4199.8105130.672299.6635136.7289
    2001M12127.59100.155130.5393100.1431137.3868
    2002M1132.68100.8215131.0986101.9008139.7982
    2002M2133.6498.6228128.051299.3352136.2784
    2002M3131.0697.6201126.284997.0766133.1798
    2002M4130.7798.7388127.33899.4048136.3738
    2002M5126.3899.5688128.3102100.1932137.4555
    2002M6123.29101.8414131.4407104.4282143.2656
    2002M7117.90105.0004137.1861109.6069148.9782
    2002M8118.99105.613138.1444110.7749150.0547
    2002M9121.08104.3139136.3466109.3223147.1717
    2002M10123.91104.5984136.6671109.0929146.8336
    2002M11121.61102.2895133.1046106.0171141.911
    2002M12121.89101.0627131.3248104.1571138.4349
    2003M1118.8197.7554127.1707100.1631132.3831
    2003M2119.3498.1064127.7883101.099133.6066
    2003M3118.6999.7366129.8777103.0382135.9653
    2003M4119.90101.7145132.5327106.2931139.1427
    2003M5117.37100.3467130.782104.3134136.5512
    2003M6118.33100.7549131.3324104.5536136.8657
    2003M7118.7098.6095128.5949101.911133.4064
    2003M8118.6698.7963128.8288102.3706134.0081
    2003M9114.8098.2868128.1687101.8092133.273
    2003M10109.5099.1609129.3144102.8529134.6394
    2003M11109.1897.5554127.2198100.6753131.7887
    2003M12107.7498.1913128.0256101.5042132.8738
    2004M1106.2798.3694128.577101.8193133.2864
    2004M2106.7198.3625128.7925101.7888133.2464
    2004M3108.5295.68125.326598.4747128.9081
    2004M4107.6691.9363120.339193.9253122.9527
    2004M5112.2091.7817120.096793.6533122.5967
    2004M6109.4390.657118.495292.416120.9769
    2004M7109.4989.77117.168591.1585119.3309
    2004M8110.2389.999117.451491.533119.8211
    2004M9110.0991.0782118.939593.2515121.8511
    2004M10108.7890.296118.049192.5177120.8923
    2004M11104.7093.439122.108196.4187125.9897
    2004M12103.8191.3371119.378594.0381122.879
    2005M1103.3491.3434119.422294.0851122.9404
    2005M2104.9491.7328119.919494.7271123.7793
    2005M3105.2591.6662119.885294.604123.6185
    2005M4107.1990.951119.003693.4756122.1439
    2005M5106.6088.247115.475389.9721117.566
    2005M6108.7587.5134114.522689.2106116.5709
    2005M7111.9587.2688114.125688.8012116.0359
    2005M8110.6188.625115.865790.1793117.8367
    2005M9111.2488.4136115.568790.4412118.1789
    2005M10114.8789.6973117.226692.1115120.3615
    2005M11118.4588.7022115.894891.6063119.7014
    2005M12118.4690.761118.566393.4569122.1195
    2006M1115.4893.0582121.759596.2068125.7128
    2006M2117.8691.9929120.535595.0497123.6185
    2006M3117.2892.7904121.751295.593124.3251
    2006M4117.0794.7149124.256898.7114128.3807
    2006M5111.7396.896127.4209101.7888132.3831
    2006M6114.6396.7553127.3269101.799132.3963

     

    Figure 3c.  Forecast Intervals of Benchmark Taylor Rule and Random Walk (Japanese Yen), 12-month-ahead forecast

    Data for Figure 3c immediately follows

    Note: To facilitate graphical comparisons, the 6- and 12-month-ahead forecast intervals of the random walk have been relocated such that they have the same center as the intervals of the Taylor rule model.

    DateRealizationTaylor Rule 5%Taylor Rule 95%RW 5%RW 95%
    1990M11129.22119.9269189.1412101.8499167.2016
    1990M12133.89119.0975187.9188101.9722167.4023
    1991M1133.70120.0614189.4829102.8838168.8988
    1991M2130.54120.2957189.7437103.3891169.7285
    1991M3137.39126.1044198.7747108.7988179.5404
    1991M4137.11128.6518202.5936112.449185.8983
    1991M5138.22126.0977199.0752109.3113180.7112
    1991M6139.75125.5027198.5642109.0711180.314
    1991M7137.83122.6752193.6962105.7629174.845
    1991M8136.82121.1749191.3707104.6478173.0015
    1991M9134.30113.7143179.128698.2387162.4061
    1991M10130.77107.5264168.731191.9643152.0334
    1991M11129.63106.8016167.600691.6979151.5931
    1991M12128.04108.534169.630795.0117157.0713
    1992M1125.46106.8953167.776194.8788156.8516
    1992M2127.70104.6625164.22992.6381153.1473
    1992M3132.86107.2349168.275397.4949161.1765
    1992M4133.54106.3819166.242797.3001160.8545
    1992M5130.77107.1213166.668398.0816162.1465
    1992M6126.84108.8759168.66399.1764163.9563
    1992M7125.88106.8214165.35397.8074161.6931
    1992M8126.23105.8252163.662797.096160.517
    1992M9122.60104.8871162.055795.3067157.559
    1992M10121.17101.345156.564192.7957153.4078
    1992M11123.88102.4156158.105191.9919152.079
    1992M12124.04102.2723157.333490.8582150.2048
    1993M1124.99100.1645154.056289.0324147.1864
    1993M2120.76101.6537156.064890.6223149.8148
    1993M3117.02104.1865159.666194.2829155.8665
    1993M4112.41103.6534158.362894.765156.6635
    1993M5110.34103.7239158.597992.7957153.4078
    1993M6107.41101.5174155.480790.0081148.7995
    1993M7107.69101.6095155.443989.3267147.6729
    1993M8103.77100.4867153.734889.5771148.087
    1993M9105.5797.1502149.342786.9993143.8254
    1993M10107.0297.4055150.048985.9873142.1524
    1993M11107.8899.2957153.036887.9088145.329
    1993M12109.9198.493152.005988.0232145.518
    1994M1111.44100.2269154.644188.6947146.6282
    1994M2106.3096.6196149.178985.6955141.6699
    1994M3105.1094.4201145.863783.0381137.2769
    1994M4103.4890.1753139.190179.7742131.881
    1994M5103.7589.3975137.7178.3041129.4507
    1994M6102.5388.0407135.968876.2258126.0149
    1994M798.4586.6753134.379176.4242126.3429
    1994M899.9484.8642131.863973.6409121.7415
    1994M998.7785.7114133.310874.9184123.8536
    1994M1098.3587.4345136.106875.9443125.5495
    1994M1198.0487.7933136.714176.5543126.5579
    1994M12100.1888.0434136.772577.9993128.9468
    1995M199.7789.9991139.672279.0832130.7386
    1995M298.2485.8894133.665575.4372124.7111
    1995M390.5285.0029131.013474.5821123.2975
    1995M483.6984.2589128.857673.6703121.4011
    1995M585.1186.5461129.453574.7912121.7172
    1995M684.6486.7195128.393674.7388120.2893
    1995M787.4083.5581123.585771.758115.4919
    1995M894.7484.8298122.964572.8498117.249
    1995M9100.5584.1623121.948371.9952115.8736
    1995M10100.8483.2353120.448271.6863115.3764
    1995M11101.9484.0288121.435171.4644115.0193
    1995M12101.8585.3146123.153573.0249117.5307
    1996M1105.7586.3606124.562572.7261117.0499
    1996M2105.7984.2589121.452171.6075115.2496
    1996M3105.9477.4991111.833665.9832106.1974
    1996M4107.2069.7317102.605161.001698.1798
    1996M5106.3470.8602104.652862.035199.8431
    1996M6108.9670.238103.777561.694898.6028
    1996M7109.1972.4342106.165863.7074101.6057
    1996M8107.8777.3663113.074369.0548109.6288
    1996M9109.9381.2467118.392573.2956116.1869
    1996M10112.4181.9867119.570473.5011115.6999
    1996M11112.3082.4019119.858674.3066116.7109
    1996M12113.9881.893118.823374.2398116.501
    1997M1117.9185.7119124.263277.0843120.9648
    1997M2122.9685.6593124.216477.1152121.0132
    1997M3122.7785.4524124.01277.2232121.2919
    1997M4125.6485.7739125.675178.1398123.0019
    1997M5119.1985.2217126.228677.5095122.8667
    1997M6114.2987.3307131.196679.424126.6719
    1997M7115.3887.1891131.229279.5909127.205
    1997M8117.9386.2233129.716378.6258125.6625
    1997M9120.8987.0336130.952780.126128.0601
    1997M10121.0688.7809133.452481.941130.9611
    1997M11125.3889.2273133.994881.8591130.8302
    1997M12129.7389.4459134.435683.0797132.7808
    1998M1129.5592.1231138.403985.9444137.3593
    1998M2125.8595.63143.900189.6309143.2512
    1998M3129.0895.1319142.892989.4876143.0222
    1998M4131.7595.835144.210191.5788147.0393
    1998M5134.9092.7928139.35486.8776139.491
    1998M6140.3390.3624135.865183.3043133.7537
    1998M7140.7991.2778137.371584.0994135.0304
    1998M8144.6892.9861140.115285.9615138.0202
    1998M9134.4895.057143.14588.12141.4859
    1998M10121.0595.8515144.960388.2435141.6841
    1998M11120.2999.6553149.797691.3867146.7309
    1998M12117.07102.443153.765394.5662151.8358
    1999M1113.29101.9087153.280294.4339151.6234
    1999M2116.67100.073150.52491.7346147.2895
    1999M3119.47102.2854153.730294.0851151.0635
    1999M4119.77103.7301157.417396.0338154.1922
    1999M5122.00106.1261159.639498.3271157.8744
    1999M6120.72109.0931164.0652102.2888164.2353
    1999M7119.33108.7053163.8753102.6269164.7781
    1999M8113.23111.8497169.238105.4567169.5588
    1999M9106.88106.2428160.503998.0228157.6063
    1999M10105.9798.3217148.338288.2347141.8684
    1999M11104.6597.5761146.855987.6805140.9775
    1999M12102.5895.3679143.04185.3363137.2083
    2000M1105.3092.3543138.008482.5827132.7808
    2000M2109.3994.3502140.571285.0382136.7289
    2000M3106.3195.9133142.670487.0863140.0221
    2000M4105.6396.3669143.168987.3043140.3726
    2000M5108.3297.6358145.746288.9256142.9793
    2000M6106.1396.5183143.183487.9968141.4859
    2000M7108.2194.9051140.646886.9819139.8541
    2000M8108.0891.6146135.196782.5331132.7012
    2000M9106.8487.6588129.103777.9058125.2611
    2000M10108.4487.1514128.472277.2464124.2008
    2000M11109.0186.1511127.092776.2792122.6457
    2000M12112.2184.7047125.066474.7687120.2172
    2001M1116.6786.38127.599576.7536123.4085
    2001M2116.2388.3445130.339379.7343128.2011
    2001M3121.5186.3646127.587777.494124.5989
    2001M4123.7786.4851128.242876.9919123.7917
    2001M5121.7787.5732130.786678.9567126.9508
    2001M6122.3586.1428127.497777.3623124.3873
    2001M7124.5086.7698125.931178.8778126.824
    2001M8121.3787.6861127.313878.7832126.6719
    2001M9118.6186.064123.255277.8746125.211
    2001M10121.4587.4853125.319579.0436127.0906
    2001M11122.4188.4658123.390779.4557127.7532
    2001M12127.5991.0381124.288681.7937131.5122
    2002M1132.6892.2676125.651685.0382136.7289
    2002M2133.6491.7911124.269784.7241136.2239
    2002M3131.0693.7488126.910688.5706142.4085
    2002M4130.7794.441126.674990.2154145.0531
    2002M5126.3893.4343125.621588.7568142.7079
    2002M6123.2993.0479125.977889.1839143.3946
    2002M7117.9093.7099126.854490.7492145.9115
    2002M8118.9992.9194125.696288.4644142.2378
    2002M9121.0891.3919124.064186.4529139.0036
    2002M10123.9192.4352125.488394.0663142.3374
    2002M11121.6192.6413126.150795.8036143.4663
    2002M12121.8994.5935128.9616100.9676149.5304
    2003M1118.8196.4432131.7778105.4461155.4929
    2003M2119.3497.1343133.1306106.6337156.6165
    2003M3118.6996.8017132.4609104.7315153.6074
    2003M4119.9097.668133.3781105.7523153.2545
    2003M5117.3796.668131.3118103.1413148.1166
    2003M6118.3396.3946130.3061101.1293144.4885
    2003M7118.7094.2765127.1896.9214138.1721
    2003M8118.6694.2317127.470498.1307139.4491
    2003M9114.8095.4371129.080699.953141.911
    2003M10109.5097.0536130.9072102.2888145.2273
    2003M11109.1895.7842129.4644100.3837142.5225
    2003M12107.7496.3846130.1341101.3419142.8507
    2004M1106.2794.5969127.751598.7805139.2401
    2004M2106.7194.633127.959199.226139.8681
    2004M3108.5293.9993127.10998.6817139.101
    2004M4107.6694.5641127.882499.6935140.5271
    2004M5112.2093.3974126.29297.5827137.5517
    2004M6109.4393.9791127.075298.3861138.6843
    2004M7109.4993.9196127.195399.6436139.1149
    2004M8110.2394.7317127.373299.893139.0731
    2004M9110.0992.8407124.454996.66134.5452
    2004M10108.7889.5846120.162892.3975128.3293
    2004M11104.7089.5739120.048192.4622127.9577
    2004M12103.8188.5943118.654791.2406126.2672
    2005M1103.3487.7321117.431789.9991124.5491
    2005M2104.9488.1639117.998390.3689125.0608
    2005M3105.2588.8312118.947691.8999127.1796
    2005M4107.1987.9718117.857891.1768126.1788
    2005M5106.6090.4506121.106595.0212131.4991
    2005M6108.7588.5691118.588992.6751128.2524
    2005M7111.9588.5522118.634292.7215128.3165
    2005M8110.6188.8437118.994893.3541129.192
    2005M9111.2488.7335118.909193.2328129.0242
    2005M10114.8788.2904118.319192.1207127.4852
    2005M11118.4586.0486115.324988.6681122.7071
    2005M12118.4685.5127114.603287.9176121.6685
    2006M1115.4885.147114.114187.5141121.1101
    2006M2117.8686.1565115.373888.8723122.9896
    2006M3117.2885.9235115.045589.1304123.3468
    2006M4117.0786.7376116.166590.7765125.6248
    2006M5111.7386.0627115.278290.2786124.9358
    2006M6114.6387.6359117.638392.1023127.4597

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    Nason, J. and J. Rogers (2008) "Exchange Rates and Fundamentals: A Generalization," International Finance Discussion Papers, Number 948, Board of Governors of the Federal Reserve System.

    Newey, W. K. and K. D. West (1987) "A Simple, Positive Semi-definite, Heteroskedasticity and Autocorrelation Consistent Covariance Matrix" Econometrica 55, 703-708.

    Rossi, B. (2005) "Testing Long-horizon Predictive Ability with High Persistence, and the Meese-Rogoff Puzzle," International Economic Review 46(1), 61-92.

    Sarno, L. and G. Valente (2005) "Empirical Exchange Rate Models and Currency Risk: Some Evidence from Density Forecasts," Journal of International, Money and Finance 24(2), 363-385.

    West, K. D. (1996) "Asymptotic Inference About Predictive Ability," Econometrica 64, 1067-1084.

    Wu, J. J. (2007) "Robust Semiparametric Forecast Intervals," Manuscript, the Federal Reserve Board.


    APPENDIX

    A.1  Monetary and Taylor Rule Models

    In this section, we describe the monetary and Taylor rule models used in the paper.

    A.1.1  Monetary Model

    Assume the money market clearing condition in the home country is

    $\displaystyle m_t=p_t+\gamma y_t-\alpha i_t+v_t,$

    where $ m_t$ is the log of money supply, $ p_t$ is the log of aggregate price, $ i_t$ is the nominal interest rate, $ y_t$ is the log of output, and $ v_t$ is money demand shock. A symmetric condition holds in the foreign country and we use an asterisk in subscript to denote variables in the foreign country. Subtracting foreign money market clearing condition from the home, we have

    $\displaystyle i_t-i_t^\ast=\frac{1}{\alpha}\left[-(m_t-m_t^\ast)+(p_t-p_t^\ast)+\gamma(y_t-y_t^\ast)+(v_t-v_t^\ast)\right].$ (A.1.1)

    The nominal exchange rate is equal to its purchasing power value plus the real exchange rate:

    $\displaystyle s_t=p_t-p_t^\ast+q_t.$ (A.1.2)

    The uncovered interest rate parity in financial market takes the form

    $\displaystyle E_ts_{t+1}-s_t=i_t-i_t^\ast+\rho_t,$ (A.1.3)

    where $ \rho_t$ is the uncovered interest rate parity shock. Substituting equations (A.1.1) and (A.1.2) into (A.1.3), we have

    $\displaystyle s_t=(1-b)\left[m_t-m_t^\ast-\gamma(y_t-y_t^\ast)+q_t-(v_t-v_t^\ast)\right]-b\rho_t+bE_ts_{t+1},$ (A.1.4)

    where $ b=\alpha/(1+\alpha)$. Solving $ s_t$ recursively and applying "no-bubbles" condition, we have

    $\displaystyle s_t=E_t\left\{(1-b)\sum_{j=0}^\infty b^j\left[m_{t+j}-m_{t+1}^\ast-\gamma(y_{t+j}-y_{t+1}^\ast)+q_{t+1}-(v_{t+j}-v_{t+j}^\ast)\right]-b\sum_{j=1}^\infty b^{j}\rho_{t+j}\right\}.$ (A.1.5)

    In the standard monetary model, such as Mark (1995), purchasing power parity ($ q_t=0$) and uncovered interest rate parity hold ($ \rho_t=0$). Furthermore, it is assumed that the money demand shock is zero ( $ v_t=v_t^\ast=0$) and $ \gamma=1$. Equation (A.1.5) reduces to

    $\displaystyle s_{t}=E_{t}\left\{(1-b)\sum_{j=0}^{\infty}b^{j}\left(m_{t+j}-m^{*}_{t+j}-(y_{t+j}-y^{*}_{t+j})\right)\right\}.$

    A.1.2  Taylor Rule Model

    We follow Engel and West (2005) to assume that both countries follow the Taylor rule and the foreign country targets the exchange rate in its Taylor rule. The interest rate differential is

    $\displaystyle i_t-i_t^\ast=\delta_s(s_t-\bar{s}_t^\ast)+\delta_y(y_t^{gap}-y_t^{gap\ast })+\delta_\pi(\pi_t-\pi_t^{\ast})+v_t-v_t^\ast,$ (A.1.6)

    where $ \bar{s}_t^\ast$ is the targeted exchange rate. Assume that monetary authorities target the PPP level of the exchange rate: $ \bar{s}_t^\ast=p_t-p_t^\ast$. Substituting this condition and the interest rate differential to the UIP condition, we have

    $\displaystyle s_t=(1-b)(p_t-p_t^\ast)-b\left[\delta_y(y_t^{gap}-y_t^{gap\ast })+\delta_\pi(\pi_t-\pi_t^{\ast})+v_t-v_t^\ast\right]-b\rho_t+bE_ts_{t+1},$ (A.1.7)

    where $ b=\frac{1}{1+\delta_s}$. Assuming that uncovered interest rate parity hold ($ \rho_t=0$) and monetary shocks are zero, equation (A.1.7)) reduces to the benchmark Taylor rule model in our paper:

    $\displaystyle s_{t}=E_{t}\left\{(1-b)\sum_{j=0}^{\infty}b^{j}(p_{t+j}-p^{*}_{t+j})-b\sum_{j=0}^{\infty}b^{j}(\delta_{y}(y^{gap}_{t+j}-y_{t+j}^{gap*})+\delta_{\pi}(\pi_{t+j}-\pi^{*}_{t+j}))\right\}.$

     

    A.2  Long-horizon Regressions

    In this section, we derive long-horizon regressions for the monetary model and the benchmark Taylor rule model.

    A.2.1  Monetary Model

    In the monetary model,

    $\displaystyle s_{t}=E_{t}\left\{(1-b)\sum_{j=0}^{\infty}b^{j}\left(m_{t+j}-m^{*}_{t+j}-(y_{t+j}-y^{*}_{t+j})\right)\right\},$

    where $ m_{t}$ and $ y_{t}$ are logarithms of domestic money stock and output, respectively. The superscript $ *$ denotes the foreign country. Money supplies ($ m_t$ and $ m_t^*$) and total outputs ($ y_t$ and $ y_t^*$) are usually I(1) variables. The general form considered in Engel, Wang, and Wu(2008) is:

    $\displaystyle s_{t}$ $\displaystyle =$ $\displaystyle (1-b)\sum_{j=0}^{\infty}b^{j}E_{t}\alpha^{'}\mathbf{D}_{t}$  
    $\displaystyle (I_{n}-\Phi(L))\Delta\mathbf{D}_{t}$ $\displaystyle =$ $\displaystyle \varepsilon_{t}$ (A.2.1)
    $\displaystyle E(\varepsilon_{t+j}\vert\varepsilon_{t},\varepsilon_{t-1},...)$ $\displaystyle \equiv$ $\displaystyle E_{t}(\varepsilon_{t+j})=0, \forall j\ge 1,$  

    where $ n$ is the dimension of $ \mathbf{D}_{t}$ and $ I_n$ is an $ n\times n$ identity matrix. $ L$ is the lag operator and $ \Phi(L)=\phi_{1}L+\phi_{2}L^{2}+...+\phi_{p}L^{p}$. Assume $ \Phi(1)$ is non-diagonal and the covariance matrix of $ \varepsilon_t$ is given by $ \Omega=E_t[\varepsilon_t\varepsilon_t']$. We assume that the change of fundamentals follows a VAR(p) process in our setup. From proposition 1 of Engel, Wang, Wu (2008), we know that for a fixed discount factor $ b$ and $ p\ge 2$,

    $\displaystyle s_{t+h}-s_{t}=\beta_{h}z_{t}+\delta^{'}_{0,h}\Delta\mathbf{D}_{t}+...+\delta^{'}_{p-2,h}\Delta\mathbf{D}_{t-p+2}+\zeta_{t+h}$

    is a correctly specified regression where the regressors and errors do not correlate. In the case of $ p=1$, the long-horizon regressions reduces to

    $\displaystyle s_{t+h}-s_{t}=\beta_{h}z_{t}+\zeta_{t+h}.$

    Following the literature, for instance Mark (1995), we do not include $ \Delta\mathbf{D}_{t}$ and its lags in our long-horizon regressions. The monetary model can be written in the form of (A.2.1) by setting $ \mathbf{D}_{t}=[m_{t}\quad m^{*}_{t}\quad y_{t}\quad y^{*}_{t}]'$ , $ \alpha=[1\quad -1\quad -1\quad 1]'$. By definition, $ z_{t}=s_{t}-(m_{t}-m^{*}_{t})+(y_{t}-y^{*}_{t})$. This corresponds to $ \beta_{m,h}=1$, $ \mathbf{X}_{m,t} =s_{t}-(m_{t}-m^{*}_{t})+(y_{t}-y^{*}_{t})$ in equation (1) of section 3.

    A.2.2  Taylor Rule Model

    In the Taylor rule model,

    $\displaystyle s_{t}=E_{t}\left\{(1-b)\sum_{j=0}^{\infty}b^{j}(p_{t+j}-p^{*}_{t+j})-b\sum_{j=0}^{\infty}b^{j}(\delta_{y}(y^{gap}_{t+j}-y_{t+j}^{gap*})+\delta_{\pi}(\pi_{t+j}-\pi^{*}_{t+j}))\right\},$

    where $ p_{t}$, $ y^{gap}_{t}$ and $ \pi_{t}$ are domestic aggregate price, output gap and inflation rate, respectively. $ \delta_{y}$ and $ \delta_{\pi}$ are coefficients of the Taylor rule model. The aggregate prices $ p_t$ and $ p_t^\ast$ are usually I(1) variables. Inflation and output gap are more likely to be I(0). Engel, Wang, and Wu (2008) consider a setup which includes both stationary and non-stationary variables:

    $\displaystyle s_t=(1-b)\sum_{j=0}^\infty b^jE_t\left[f_{1t+j}\right]$ $\displaystyle +b\sum_{j=0}^\infty b^jE_t\left[f_{2t+j}+u_{2t+j}\right]$
    $\displaystyle f_{1t}$ $\displaystyle =\alpha_1'\mathbf{D_t}\sim I(1)$    
    $\displaystyle f_{2t}$ $\displaystyle =\alpha_2'\mathbf{\Delta D_t}\sim I(0)$    
    $\displaystyle u_{2t}$ $\displaystyle =\alpha_3'\mathbf{\Delta D_t}\sim I(0)$    
    $\displaystyle (I_{n}$ $\displaystyle -\Phi(L))\Delta\mathbf{X}_{t}=\varepsilon_{t},$ (A.2.2)

    where $ f_{1t}$ and $ f_{2t}$ ($ u_{2t}$) are observable (unobservable) fundamentals. $ \Delta\mathbf{D}_{t}$ is the first difference of $ \mathbf{D}_{t}$, which contains I(1) economic variables.17 From proposition 2 of Engel, Wang, and Wu (2008), we know that for a fixed discount factor $ b$ and $ h\ge 2$,

    $\displaystyle s_{t+h}-s_{t}=\tilde{\beta}_{h}z_{t}+\sum_{k=0}^{p-1}\tilde{\delta}^{'}_{k,h}\Delta\mathbf{D}_{t-k}+\tilde{\zeta}_{t+h}$ (A.2.3)

    is a correctly specified regression, where the regressors and errors do not correlate. In the case of $ p=1$, the long-horizon regressions reduces to

    $\displaystyle s_{t+h}-s_{t}=\tilde{\beta}_{h}z_{t}+\tilde{\zeta}_{t+h}.$

    The Taylor rule model can be written into the form of (A.2.2) by setting

    $\displaystyle \mathbf{D}_{t}=\left[p_{t}\quad p^{*}_{t}\quad \sum_{s=-\infty}^t y^{gap}_{s}\quad \sum_{s=-\infty}^ty^{gap*}_s,\sum_{s=-\infty}^t\pi_{s}\quad \sum_{s=-\infty}^t\pi^{*}_{s}\right]'.$

    By definition, $ z_{t}=s_t-p_{t}+p^{*}_{t}+\frac{b}{1-b}(\delta_{y}(y^{gap}_{t}-y^{gap*}_{t})+\delta_{\pi}(\pi_{t}-\pi^{*}_{t}))$ . This corresponds to $ \beta_{m,h}=[1\quad \frac{b}{1-b}\delta_y\quad \frac{b}{1-b}\delta_\pi]$ and $ \mathbf{X}_{m,t}=[q_t\quad y_t^{gap}-y_t^{gap*}\quad \pi_t-\pi_t^*]$ , where $ q_t=s_t-p_{t}+p^{*}_{t}$ is the real exchange rate. $ \beta_{m,h}$ and $ \mathbf{X}_{m,t}$ can be defined differently. For instance, $ \beta_{m,h}=1$ and $ \mathbf{X}_{m,t}=s_t-p_{t}+p^{*}_{t}+\frac{b}{1-b}(\delta_{y}(y^{gap}_{t}-y^{gap*}_{t})+\delta_{\pi}(\pi_{t}-\pi^{*}_{t}))$ . Our results do not change qualitatively under this alternative setup.


    Footnotes

    *  We thank Menzie Chinn, Charles Engel, Bruce Hansen, Mark Wynne, and Ken West for invaluable discussions. We would also like to thank seminar participants at the Dallas Fed for helpful comments. All views are those of the authors and do not necessarily reflect the views of the Federal Reserve Bank of Dallas, the Board of Governors or the Federal Reserve System. All GAUSS programs are available upon request. Email: [email protected] Address: Research Department, Federal Reserve Bank of Dallas, 2200 N. Pearl Street, Dallas, TX 75201 Phone: (214) 922-6471. Email: [email protected] Address: Board of Governors of the Federal Reserve System, 20th and C Streets, Washington, D.C. 20551 Phone: (202) 452-2556.  Return to text

    1.  Chinn and Meese (1995), and MacDonald and Taylor (1994) find similar results. However, the long-horizon exchange rate predictability in Mark (1995) has been challenged by Kilian (1999) and Berkowitz and Giorgianni (2001) in succeeding studies. Return to text

    2.  For brevity, we omit RS and simply say forecast intervals when we believe that it causes no confusion. Return to text

    3.  We also tried the random walk with a drift. It does not change our results. Return to text

    4.  Clarida, Gali, and Gertler (1998) find empirical support for forward looking Taylor rules. Forward looking Taylor rules are ruled out because they require forecasts of predictors, which creates additional complications in out-of-sample forecasting. Return to text

    5.  See appendix for more detail. While the long-horizon regression format of the benchmark Taylor model is derived directly from the underlying Taylor rule model, this is not the case for the models with interest rate smoothing (models 3 and 4). Molodtsova and Papell (2007) only consider the short-horizon regression for the Taylor rule models. We include long-horizon regressions of these models only for the purpose of comparison. Return to text

    6.  We thank the authors for the data, which we downloaded from David Papell's website. For the exact line numbers and sources of the data, see the data appendix of Molodtsova and Papell (2008). Return to text

    7.  We choose $ b$ using the method of Hall, Wolff, and Yao (1999). Return to text

    8.  It is consistent in the sense of convergence in probability as the estimation sample size goes to infinity. Return to text

    9.  While RS intervals remedy mis-specifications asymptotically, it does not guarantee such corrections in a given finite sample. Return to text

    10.  We use Newey and West (1987) for our empirical work, with a window width of 12. Return to text

    11.  Center here means the half way point between the upper and lower bound for a given interval. Return to text

    12.  These nine exchange rates are the Danish Kroner, the French Franc, the Deutschmark, the Italian Lira, the Japanese Yen, the Dutch Guilder, the Portuguese Escudo, the Swiss Franc, and the British pound. Similar results hold at other horizons. Return to text

    13.  When comparing the intervals for $ S_{\tau+h} - S_{\tau}$, the random walk model builds the forecast interval around 0, while economic model $ m$ build it around $ \widehat{\beta}^{^{\prime}}_{m,h}\mathbf{X}_{m,\tau}$ Return to text

    14.  The only exception is Portugal, where only 192 data points were available. In this case, we choose R = 120. Return to text

    15.  See Wu (2007) for more discussions. Return to text

    16.  Figures in other countries show similar patterns. Results are available upon request. Return to text

    17.  To incorporate I(0) economic variables, $ \mathbf{D}_{t}$ contains the levels of I(1) variables and the summation of I(0) variables from negative infinity to time $ t$Return to text


    This version is optimized for use by screen readers. Descriptions for all mathematical expressions are provided in LaTex format. A printable pdf version is available. Return to text

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