lmInfl {reverseR} | R Documentation |
Checks and analyzes leave-one-out (LOO) p-values in linear regression
Description
This function calculates leave-one-out (LOO) p-values for all data points and identifies those resulting in "significance reversal", i.e. in the p-value of the model's slope traversing the user-defined \alpha
-level.
Usage
lmInfl(model, alpha = 0.05, method = c("pearson", "spearman"), verbose = TRUE, ...)
Arguments
model |
the linear model of class |
alpha |
the |
method |
select either parametric ( |
verbose |
logical. If |
... |
other arguments to |
Details
The algorithm
1) calculates the p-value of the full model (all points),
2) calculates a LOO-p-value for each point removed,
3) checks for significance reversal in all data points and
4) returns all models as well as classical influence.measures
with LOO-p-values, \Delta
p-values, slopes and standard errors attached.
If method = "spearman"
, p-values are based on Spearman Rank correlation, and the values given in the last column of the result matrix are Spearman's \rho
.
The idea of p-value influencers was first introduced by Belsley, Kuh & Welsch, and described as an influence measure pertaining directly to the change in t-statistics, that will "show whether the conclusions of hypothesis testing would be affected", termed dfstat in [1, 2, 3] or dfstud in [4]:
\rm{dfstat}_{ij} \equiv \frac{\hat{\beta}_j}{s\sqrt{(X'X)^{-1}_{jj}}}-\frac{\hat{\beta}_{j(i)}}{s_{(i)}\sqrt{(X'_{(i)}X_{(i)})^{-1}_{jj}}}
where \hat{\beta}_j
is the j-th estimate, s is the residual standard error, X is the design matrix and (i) denotes the i-th observation deleted.
dfstat, which for the regression's slope \beta_1
is the difference of t-statistics
\Delta t = t_{\beta1} - t_{\beta1(i)} = \frac{\beta_1}{\rm{s.e.(\beta_1)}} - \frac{\beta_1(i)}{\rm{s.e.(\beta_1(i)})}
is inextricably linked to the changes in p-value \Delta p
, calculated from
\Delta p = p_{\beta1} - p_{\beta1(i)} = 2\left(1-P_t(t_{\beta1}, \nu)\right) - 2\left(1-P_t(t_{\beta1(i)} , \nu-1)\right)
where P_t
is the Student's t cumulative distribution function with \nu
degrees of freedom, and where significance reversal is attained when \alpha \in [p_{\beta1}, p_{\beta1(i)}]
.
Interestingly, in linear regression the seemingly mandatory check of the influence of single data points on statistical inference is living in oblivion: apart from [1-4], there is, to the best of our knowledge, no reference to dfstat or \Delta p
in current literature on influence measures.
The influence output also includes the more recent Hadi's measure (column "hadi"):
H_i = \frac{p_{ii}}{1 - p_{ii}} + \frac{k}{1 - p_{ii}}\frac{d_i^2}{(1-d_i^2)}
where p_{ii}
are the diagonals of the hat matrix (leverages), k = 2
in univariate linear regression and d_i = e_i/\sqrt{\rm{SSE}}
.
Value
A list with the following items:
origModel |
the original model with all data points. |
finalModels |
a list of final models with the influencer(s) removed. |
infl |
a matrix with the original data, classical |
sel |
a vector with the influencers' indices. |
alpha |
the selected |
origP |
the original model's p-value. |
stab |
the stability measure, see |
Author(s)
Andrej-Nikolai Spiess
References
For dfstat / dfstud :
1. Regression diagnostics: Identifying influential data and sources of collinearity.
Belsley DA, Kuh E, Welsch RE.
John Wiley, New York, USA (2004).
2. Econometrics, 5ed.
Baltagi B.
Springer-Verlag Berlin, Germany (2011).
3. Growth regressions and what the textbooks don't tell you.
Temple J.
Bull Econom Res, 52, 2000, 181-205.
4. Robust Regression and Outlier Detection.
Rousseeuw PJ & Leroy AM.
John Wiley & Sons, New York, NY (1987).
Hadi's measure:
A new measure of overall potential influence in linear regression.
Hadi AS.
Comp Stat & Data Anal, 14, 1992, 1-27.
Examples
## Example #1 with single influencers and insignificant model (p = 0.115).
## Removal of #18 results in p = 0.0227!
set.seed(123)
a <- 1:20
b <- 5 + 0.08 * a + rnorm(20, 0, 1)
LM1 <- lm(b ~ a)
res1 <- lmInfl(LM1)
lmPlot(res1)
pvalPlot(res1)
inflPlot(res1)
slsePlot(res1)
stability(res1)
## Example #2 with multiple influencers and significant model (p = 0.0269).
## Removal of #2, #17, #18 or #20 result in crossing p = 0.05!
set.seed(125)
a <- 1:20
b <- 5 + 0.08 * a + rnorm(20, 0, 1)
LM2 <- lm(b ~ a)
res2 <- lmInfl(LM2)
lmPlot(res2)
pvalPlot(res2)
inflPlot(res2)
slsePlot(res2)
stability(res2)
## Large Example #3 with top 10 influencers and significant model (p = 6.72E-8).
## Not possible to achieve a crossing of alpha with any point despite strong noise.
set.seed(123)
a <- 1:100
b <- 5 + 0.08 * a + rnorm(100, 0, 5)
LM3 <- lm(b ~ a)
res3 <- lmInfl(LM3)
lmPlot(res3)
stability(res3)
## Example #4 with replicates and single influencer (p = 0.114).
## Removal of #58 results in p = 0.039.
set.seed(123)
a <- rep(1:20, each = 3)
b <- 5 + 0.08 * a + rnorm(20, 0, 2)
LM4 <- lm(b ~ a)
res4 <- lmInfl(LM4)
lmPlot(res4)
pvalPlot(res4)
inflPlot(res4)
slsePlot(res4)
stability(res4)
## As Example #1, but with weights.
## Removal of #18 results in p = 0.04747.
set.seed(123)
a <- 1:20
b <- 5 + 0.08 * a + rnorm(20, 0, 1)
LM5 <- lm(b ~ a, weights = 1:20)
res5 <- lmInfl(LM5)
lmPlot(res5)
stability(res5)