Consider the order latex($p$) VAR representation for the latex($1\times m$) vector of observed variables latex($y_t$):

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where latex($u_t\sim \mathcal N\left( 0,\Sigma_u\right)$). Let latex($z_t$) be the latex($mp\times 1$) vector latex($\left[y_{t-1}',...,y_{t-p}'\right]'$) and define latex($\mathbf{A}=\left[\mathbf A_1',...,\mathbf A_p'\right]'$), the VAR representation can then be written in matrix form as:

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where latex($Y = (y_1',\dots,y_T')'$), latex($Z = (z_1',\dots,z_T')'$) and latex($\mathcal U = (u_1',\dots,u_T')'$).

Dummy observations prior for the VAR can be constructed using the VAR likelihood function for latex($\mathcal T = [\lambda T]$) artificial data simulated with the DSGE latex($\left( Y^{\ast },Z^{\ast}\right)$), combined with diffuse priors. The prior is then given by:

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implying that latex($\Sigma$) follows an inverted Wishart distribution and latex($\mathbf A$) conditional on latex($\Sigma$) is gaussian. Assuming that observables are covariance stationary, Del Negro and Schorfheide use the DSGE theoretical autocovariance matrices for a given latex($n\times 1$) vector of model parameters latex($\theta$), denoted latex($\Gamma_{YY}\left( \theta \right)$), latex($\Gamma_{ZY}\left( \theta \right)$), latex($\Gamma_{YZ}\left( \theta\right)$), latex($\Gamma_{ZZ}\left( \theta \right)$) instead of the (artificial) sample moments latex(${Y^*}'Y^*$), latex(${Z^*}'Y^*$), latex(${Y^*}'Z^*$), latex(${Z^*}'Z^*$). In addition, the latex($p$)-th order VAR approximation of the DSGE provides the first moment of the prior distributions through the population least-square regression:

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Conditional on the deep parameters of the DSGE latex($\theta $) and latex($\lambda$), the priors for the VAR parameters are given by:

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where latex($\Gamma_{ZZ}(\theta)$) is assumed to be non singular and latex($\lambda \geq \frac{mp+m}{T}$) for the priors to be proper\footnote{Note that it

\textit{a priori} density of $\mathbf A$ is defined by $n+1$ parameters ($\theta$ and $\lambda$), which is likely to be less than $mp$ (the VAR number of parameters). If we have a one-to-one relationship (no identification issues) between $(\theta,\lambda)$ and $\mathbf A$ it will be a good idea to estimate $(\theta,\lambda)$ instead of $\mathbf A$, \textit{ie} to estimate fewer free parameters. To do so, \cite{DS2004} complete the prior by specifying a prior distribution over the structural model's deep parameters: $p_0(\theta)$. We still have to set the weight of the structural prior, $\lambda$. \citeauthor{DS2004} choose the value of $\lambda$ that maximizes the marginal density. They estimate a limited number of DSGE-VAR models with different values of $\lambda$. For each model they also estimate the marginal density and select the model (\textit{ie} the value of $\lambda$) with highest marginal density. In the present paper, we estimate directly $\lambda$ as another parameter, instead of doing a loop over the values of this parameter\footnote{In this regard, the approach followed by

$\lambda$, which is assumed to be independent from $\theta$. Finally, the DSGE-VAR model has the following prior structure: \begin{equation}\tag{P3}\label{prior3} p_0\left( \mathbf A,\Sigma, \theta, \lambda \right) = p_0\left( \mathbf A, \Sigma \mid \theta ,\lambda \right) \times p_0\left( \theta \right) \times p_0\left( \lambda \right) \end{equation} where $p_0\left(\mathbf A, \Sigma \mid \theta ,\lambda \right)$ is defined by [\ref{prior1a},\ref{prior1b}] and \equaref{prior2}.}\newline

\par{The posterior distribution, may be factorized in the following way: \begin{equation}\tag{Q3}\label{posterior1} p\left( \mathbf A, \Sigma , \theta , \lambda \mid \mathcal Y_T\right) = p\left(\mathbf A, \Sigma \mid \mathcal Y_T, \theta, \lambda\right) \times p\left( \theta ,\lambda \mid \mathcal Y_T\right) \end{equation} where $\mathcal Y_T$ stands for the sample. A closed form expression for the first density function on the right hand side of \equaref{posterior1} is available. Conditional on $\theta $ and $\lambda$, [\ref{prior1a},\ref{prior1b}] and \equaref{prior2} define a conjugate prior for the VAR model, so its posterior density has to belong to the same family: the distribution of $\mathbf A$ conditional on $\Sigma$, $\theta$, $\lambda$ and the sample is matric-variate normal, and the distribution of $\Sigma$ conditional on $\theta$, $\lambda$ and the sample is inverted Wishart. More formally, we have: \begin{equation}\tag{Q2}\label{posterior2}

(\lambda+1)T-mp-m\right)

\end{equation} where: \begin{subequations}%\tag{Q1}\label{posterior3}

\end{subequations} with: \[ V(\theta,\lambda) = \lambda T~\Gamma_{ZZ}(\theta) +Z'Z \] Not surprisingly, we find that the posterior mean of $\mathbf A$ is a convex combination of $A^*(\theta)$, the prior mean, and of the OLS estimate of $\mathbf A$. When $\lambda$ goes to infinity the posterior mean shrinks towards the prior mean, \textit{ie} the projection of the DSGE model onto the VAR($p$).\newline We do not have a closed form expression for the joint posterior density of $\theta $ and $\lambda$ (the second term on the right hand side of \equaref{posterior1}). So the posterior distribution of $(\theta,\lambda)$ is recovered from an MCMC algorithm, as described in \cite[appendix B]{DS2004}, except that we do estimate $\lambda$ as the deep parameters $\theta$.\footnote{This can be done with

\par{All in all, this estimation procedure allows to select the

\par{Notice that, when $\lambda$ is closer to its lowest possible