Consider the following regression model $$ y=\beta _{1}x_{1}+\beta _{2}x_{2}+u $$ where $x_{1}$ and $x_{2}$ are two random variables and $u$ is a disturbance term. I simulate the model drawing $x_{1}$, $x_{2}$ and $u$ from a standard normal distribution (mean 0 and standard deviation of 1) and making the two regressors $x_{1}$ and $x_{2}$ correlated with correlation coefficient of $0.995$. I set $\beta _{1}=\beta _{2}=0.5$.
The high correlation gives obvious problems visible in the large swings of the estimated coefficients in the table below. What strikes me, however, is that their sum ($\hat{\beta}_{1}+\hat{\beta}_{2}$) seems rather stable and centers around the true sum of 1. The table below shows the coefficients and their sum for five different draws.
(1) | (2) | (3) | (4) | (5) | |
---|---|---|---|---|---|
beta1 | -0.445 | 0.$_{.}$467 | 0.966 | 0.538 | 0.189 |
beta2 | 1.451 | 0.505 | -0.0443 | 0.479 | 0.862 |
beta1+beta2 | 1.006 | 0.972 | 1.013 | 1.012 | 1.051 |
When one coefficient goes up, the other seems to go down.
Question: Is this something well known? Does this have a name?
This could as well be trivial, but it seems that this may somehow be related to the fact that while OLS gives inconsistent estimates when the regressors are highly correlated, it still allows us to predict $y$ fairly well. I am referring to what Diebold calls p-consistency. See for example
The full table with the estimation results of the five regressions is
| | y | y | y | y | y | |-----|------------------|----------------|------------------|---------------|--| |x1_1 |-0.445 (0.310) | | | | | |x2_1 |1.451*** (0.308) | | | | | |x1_2 | | 0.467 (0.313) | | | | |x2_2 | | 0.505 (0.313) | | | | |x1_3 | | | 0.966** (0.326) | | | |x2_3 | | | 0.0443 (0.328) | | | |x1_4 | | | | 0.538 (0.320)| | |x2_4 | | | | 0.479 (0.319)| | |x1_5 | | | | | 0.189 (0.312) | |x2_5 | | | | | 0.862** (0.312)| |N | 1000 | 1000 | 1000 | 1000 | 1000 | |R-sq | 0.5114 | 0.4926 | 0.4861 | 0.5155 | 0.5467 | Standard errors in parentheses
- p<0.05, ** p<0.01, *** p<0.001