A Primer for Spatial Econometrics
eBook - ePub

A Primer for Spatial Econometrics

With Applications in R

G. Arbia

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eBook - ePub

A Primer for Spatial Econometrics

With Applications in R

G. Arbia

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About This Book

This book aims at meeting the growing demand in the field by introducing the basic spatial econometrics methodologies to a wide variety of researchers. It provides a practical guide that illustrates the potential of spatial econometric modelling, discusses problems and solutions and interprets empirical results.

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Information

Year
2014
ISBN
9781137317940

1

The Classical Linear Regression Model

1.1 The basic linear regression model

Let us consider the following linear model
n y1 = n Xkk β1 + n ξ1 (1.1)
where
Image
is a vector of n observations of the dependent
variable y,
Image
a matrix of n observations on k – 1
non-stochastic exogenous regressors including a constant term,
Image
a vector of k unknown parameters to be estimated and
Image
a
vector of stochastic disturbances. We will assume throughout the book that the n observations refer to territorial units such as regions or countries.
The classical linear regression model assumes normality, identicity and independence of the stochastic disturbances conditional upon the k regressors. In short
ε | X ≈ i.i.d.N (0, σ2ε n In) (1.2)
n In being an n-by-n identity matrix. Equation (1.2) can also be written as:
E(Îľ | X) = 0(1.3)
E(ξξT | X) = σ2ξ n In (1.4)
Equation (1.3) corresponds to the assumption of exogeneity, Equation (1.4) to the assumption of spherical disturbances (Greene, 2011).
Furthermore it is assumed that the k regressors are not perfectly dependent on one another (full rank of matrix X). Under this set of hypotheses the Ordinary Least Squares fitting criterion (OLS) leads to the best linear unbiased estimators (BLUE) of the vector of parameters β, say
Image
OLS =
Image
. In fact the OLS criterion requires:
S(β) = eT e = min (1.5)
where e = y – X
Image
are the observed errors and eT indicates the transpose of e.
From Equation (1.5) we have:
Image
whence:
Image
OLS = (XT X)-1 XT y (1.6)
As said the OLS estimator is unbiased
E(
Image
OLS | X) = β (1.7)
with a variance
Var(
Image
OLS | X) = (XT X)–1σ2ε (1.8)
which achieves the minimum among all possible linear estimators (full efficiency) and tends to zero when n tends to infinity (weak consistency).
From the assumption of normality of the stochastic disturbances, normality of the estimators also follows:
Image
OLS | X ≈ N[β; (XT X)–1 σ2ε] (1.9)
Furthermore, from the assumption of normality of the stochastic disturbances, it also follows that the alternative estimators, based on the Maximum Likelihood criterion (ML), coincide with the OLS solution.
In fact, the single stochastic disturbance is distributed as:
Image
f being a density function, and consequently the likelihood of the observed sample is:
Image
(1.10)
from the assumption of independence of the disturbances. From (1.1) we have that
ε = y – Xβ (1.11)
hence (1.10) can be written as:
Image
(1.12)
and the log-likelihood as:
Image
(1.13)
The scores functions are defined as:
Image
(1.14)
and solving the system of k + 1 equations, we have:
Image
(1.15)
Thus, under the hypothesis of normality of residuals, the ML estimator of β coincides with the OLS estimator. The ML estimator of
Image
on the contrary differs from the unbiased estimator
Image
and it is biased, but asymptotically unbiased.
To ensure that the solution obtained is a maximum we consider the second derivatives:
Image
(1.16)
which can be arranged in the Fisher’s Information Matrix:
Image
(1.17)
which is positive definite.
The equivalence between the ML and the OLS estimators ensures that the solution found enjoys all the large sample properties of the ML estimators, that is to say: asymptotic normality, consistency, asymptotic unbiasedness, full efficiency with respect to a larger class of estimators other than the linear...

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