| lm {stats} | R Documentation |
Fitting Linear Models
Description
lm is used to fit linear models, including multivariate ones.
It can be used to carry out regression,
single stratum analysis of variance and
analysis of covariance (although aov may provide a more
convenient interface for these).
Usage
lm(formula, data, subset, weights, na.action,
method = "qr", model = TRUE, x = FALSE, y = FALSE, qr = TRUE,
singular.ok = TRUE, contrasts = NULL, offset, ...)
## S3 method for class 'lm'
print(x, digits = max(3L, getOption("digits") - 3L), ...)
Arguments
formula |
an object of class |
data |
an optional data frame, list or environment (or object
coercible by |
subset |
an optional vector specifying a subset of observations
to be used in the fitting process. (See additional details about how
this argument interacts with data-dependent bases in the
‘Details’ section of the |
weights |
an optional vector of weights to be used in the fitting
process. Should be |
na.action |
a function which indicates what should happen
when the data contain |
method |
the method to be used; for fitting, currently only
|
model, x, y, qr |
logicals. If |
singular.ok |
logical. If |
contrasts |
an optional list. See the |
offset |
this can be used to specify an a priori known
component to be included in the linear predictor during fitting.
This should be |
... |
For |
digits |
the number of significant digits to be
passed to |
Details
Models for lm are specified symbolically. A typical model has
the form response ~ terms where response is the (numeric)
response vector and terms is a series of terms which specifies a
linear predictor for response. A terms specification of the form
first + second indicates all the terms in first together
with all the terms in second with duplicates removed. A
specification of the form first:second indicates the set of
terms obtained by taking the interactions of all terms in first
with all terms in second. The specification first*second
indicates the cross of first and second. This is
the same as first + second + first:second.
If the formula includes an offset, this is evaluated and
subtracted from the response.
If response is a matrix a linear model is fitted separately by
least-squares to each column of the matrix and the result inherits from
"mlm" (“multivariate linear model”).
See model.matrix for some further details. The terms in
the formula will be re-ordered so that main effects come first,
followed by the interactions, all second-order, all third-order and so
on: to avoid this pass a terms object as the formula (see
aov and demo(glm.vr) for an example).
A formula has an implied intercept term. To remove this use either
y ~ x - 1 or y ~ 0 + x. See formula for
more details of allowed formulae.
Non-NULL weights can be used to indicate that
different observations have different variances (with the values in
weights being inversely proportional to the variances); or
equivalently, when the elements of weights are positive
integers w_i, that each response y_i is the mean of
w_i unit-weight observations (including the case that there
are w_i observations equal to y_i and the data have been
summarized). However, in the latter case, notice that within-group
variation is not used. Therefore, the sigma estimate and residual
degrees of freedom may be suboptimal; in the case of replication
weights, even wrong. Hence, standard errors and analysis of variance
tables should be treated with care.
lm calls the lower level functions lm.fit, etc,
see below, for the actual numerical computations. For programming
only, you may consider doing likewise.
All of weights, subset and offset are evaluated
in the same way as variables in formula, that is first in
data and then in the environment of formula.
Value
lm returns an object of class "lm" or for
multivariate (‘multiple’) responses of class c("mlm", "lm").
The functions summary and anova are used to
obtain and print a summary and analysis of variance table of the
results. The generic accessor functions coefficients,
effects, fitted.values and residuals extract
various useful features of the value returned by lm.
An object of class "lm" is a list containing at least the
following components:
coefficients |
a named vector of coefficients |
residuals |
the residuals, that is response minus fitted values. |
fitted.values |
the fitted mean values. |
rank |
the numeric rank of the fitted linear model. |
weights |
(only for weighted fits) the specified weights. |
df.residual |
the residual degrees of freedom. |
call |
the matched call. |
terms |
the |
contrasts |
(only where relevant) the contrasts used. |
xlevels |
(only where relevant) a record of the levels of the factors used in fitting. |
offset |
the offset used (missing if none were used). |
y |
if requested, the response used. |
x |
if requested, the model matrix used. |
model |
if requested (the default), the model frame used. |
na.action |
(where relevant) information returned by
|
In addition, non-null fits will have components assign,
effects and (unless not requested) qr relating to the linear
fit, for use by extractor functions such as summary and
effects.
Using time series
Considerable care is needed when using lm with time series.
Unless na.action = NULL, the time series attributes are
stripped from the variables before the regression is done. (This is
necessary as omitting NAs would invalidate the time series
attributes, and if NAs are omitted in the middle of the series
the result would no longer be a regular time series.)
Even if the time series attributes are retained, they are not used to
line up series, so that the time shift of a lagged or differenced
regressor would be ignored. It is good practice to prepare a
data argument by ts.intersect(..., dframe = TRUE),
then apply a suitable na.action to that data frame and call
lm with na.action = NULL so that residuals and fitted
values are time series.
Author(s)
The design was inspired by the S function of the same name described in Chambers (1992). The implementation of model formula by Ross Ihaka was based on Wilkinson & Rogers (1973).
References
Chambers, J. M. (1992) Linear models. Chapter 4 of Statistical Models in S eds J. M. Chambers and T. J. Hastie, Wadsworth & Brooks/Cole.
Wilkinson, G. N. and Rogers, C. E. (1973). Symbolic descriptions of factorial models for analysis of variance. Applied Statistics, 22, 392–399. doi:10.2307/2346786.
See Also
summary.lm for more detailed summaries and anova.lm for
the ANOVA table; aov for a different interface.
The generic functions coef, effects,
residuals, fitted, vcov.
predict.lm (via predict) for prediction,
including confidence and prediction intervals;
confint for confidence intervals of parameters.
lm.influence for regression diagnostics, and
glm for generalized linear models.
The underlying low level functions,
lm.fit for plain, and lm.wfit for weighted
regression fitting.
More lm() examples are available e.g., in
anscombe, attitude, freeny,
LifeCycleSavings, longley,
stackloss, swiss.
biglm in package biglm for an alternative
way to fit linear models to large datasets (especially those with many
cases).
Examples
require(graphics)
## Annette Dobson (1990) "An Introduction to Generalized Linear Models".
## Page 9: Plant Weight Data.
ctl <- c(4.17,5.58,5.18,6.11,4.50,4.61,5.17,4.53,5.33,5.14)
trt <- c(4.81,4.17,4.41,3.59,5.87,3.83,6.03,4.89,4.32,4.69)
group <- gl(2, 10, 20, labels = c("Ctl","Trt"))
weight <- c(ctl, trt)
lm.D9 <- lm(weight ~ group)
lm.D90 <- lm(weight ~ group - 1) # omitting intercept
anova(lm.D9)
summary(lm.D90)
opar <- par(mfrow = c(2,2), oma = c(0, 0, 1.1, 0))
plot(lm.D9, las = 1) # Residuals, Fitted, ...
par(opar)
### less simple examples in "See Also" above