The package fixest
provides a family of functions to
perform estimations with multiple fixed-effects. The two main functions
are feols
for linear models and feglm
for
generalized linear models. In addition, the function femlm
performs direct maximum likelihood estimation, and feNmlm
extends the latter to allow the inclusion of non-linear in parameters
right-hand-sides. Finally, the functions fepois
and
fenegbin
are aliases for Poisson and negative binomial
fixed-effect estimations. Each of these functions supports any number of
fixed-effects and is implemented with full fledged multi-threading in
C++. Functions feols
and feglm
further support
variables with varying slopes.
This package is currently (Feb. 2020) the fastest software available to perform fixed-effects estimations. See the project’s homepage for a set of benchmarks.
The standard-errors of the estimates can be easily and intuitively clustered (up to four-way).
The function etable
allows to seamlessly export the
results of multiple estimations into either a data.frame, or into a
Latex table.
The main features of the package are illustrated in this vignette. The theory used to obtain the fixed-effects is based on Berge (2018), “Efficient estimation of maximum likelihood models with multiple fixed-effects: the R package FENmlm.” CREA Discussion Papers, 13.
This example deals with international trade, which is a setup that usually requires performing estimations with many fixed-effects. We estimate a very simple gravity model in which we are interested in finding out the negative effect of geographic distance on trade. The sample data consists of European trade extracted from Eurostat. Let’s load the data contained in the package:
This data is a sample of bilateral importations between EU15 countries from 2007 and 2016. The data is further broken down according to 20 product categories. Here is a sample of the data:
Destination | Origin | Product | Year | dist_km | Euros |
---|---|---|---|---|---|
LU | BE | 1 | 2007 | 139.5719 | 2966697 |
BE | LU | 1 | 2007 | 139.5719 | 6755030 |
LU | BE | 2 | 2007 | 139.5719 | 57078782 |
BE | LU | 2 | 2007 | 139.5719 | 7117406 |
LU | BE | 3 | 2007 | 139.5719 | 17379821 |
BE | LU | 3 | 2007 | 139.5719 | 2622254 |
The dependent variable of the estimation will be the level of trade between two countries while the independent variable is the geographic distance between the two countries. To obtain the elasticity of geographic distance net of the effects of the four fixed-effects, we estimate the following:
\(E\left(Trade_{i,j,p,t}\right)=\gamma_{i}^{Exporter}\times\gamma_{j}^{Importer}\times\gamma_{p}^{Product}\times\gamma_{t}^{Year}\times Distance_{ij}^{\beta}\),
where the subscripts \(i\), \(j\), \(p\) and \(t\) stand respectively for the exporting country, the importing country, the type of product and the year, and the \(\gamma_{v}^{c}\) are fixed-effects for these groups. Here \(\beta\) is the elasticity of interest.
Note that when you use the Poisson/Negative Binomial families, this relationship is in fact linear because the right hand side is exponentialized to avoid negative values for the Poisson parameter. This leads to the equivalent relation:1
\(E\left(Trade_{i,j,p,t}\right)=\exp\left(\gamma_{i}^{Exporter}+\gamma_{j}^{Importer}+\gamma_{p}^{Product}+\gamma_{t}^{Year}+\beta\times \ln Distance_{ij}\right)\).
The estimation of this model using a Poisson likelihood is as follows:
The function fepois
is actually an alias to the function
feglm
with family = poisson
. The results can
be shown directly with the print
method:
print(gravity_pois)
#> Poisson estimation, Dep. Var.: Euros
#> Observations: 38,325
#> Fixed-effects: Origin: 15, Destination: 15, Product: 20, Year: 10
#> Standard-errors: Clustered (Origin)
#> Estimate Std. Error z value Pr(>|z|)
#> log(dist_km) -1.52787 0.115678 -13.208 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -7.025e+11 Adj. Pseudo R2: 0.764032
#> BIC: 1.405e+12 Squared Cor.: 0.612021
The print
reports the coefficient estimates and
standard-errors as well as some other information. Among the quality of
fit information, the squared-correlation corresponds to the correlation
between the dependent variable and the expected predictor; it reflects
somehow the idea of R-square in OLS estimations. Note that the
estimation is performed using parallel computing which you can control
using the argument nthreads
(see the “multi-threading”
section for more details).
To cluster the standard-errors, we can simply use the argument
vcov
of the summary
method. Let’s say we want
to cluster the standard-errors according to the first two fixed-effects
(i.e. the Origin and Destination variables). Then we
just have to do:
summary(gravity_pois, vcov = "twoway")
#> Poisson estimation, Dep. Var.: Euros
#> Observations: 38,325
#> Fixed-effects: Origin: 15, Destination: 15, Product: 20, Year: 10
#> Standard-errors: Clustered (Origin & Destination)
#> Estimate Std. Error z value Pr(>|z|)
#> log(dist_km) -1.52787 0.130734 -11.6869 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -7.025e+11 Adj. Pseudo R2: 0.764032
#> BIC: 1.405e+12 Squared Cor.: 0.612021
The clustering can be done on one, two, three or up to four
variables. If the estimation includes fixed-effects, then by default the
clustering will be done using these fixed-effects, in the original
order. This is why the Origin and Destination
variables were used for the two-way clustering in the previous example.
If, instead, you wanted to perform one-way clustering on the
Product variable, you need to provide it in a formula or use
the argument cluster
:
# Three ways to summon clustering on the Product variable
summary(gravity_pois, vcov = ~Product)
summary(gravity_pois, cluster = "Product")
summary(gravity_pois, cluster = ~Product)
Both produce the same results:
summary(gravity_pois, cluster = ~Product)
#> Poisson estimation, Dep. Var.: Euros
#> Observations: 38,325
#> Fixed-effects: Origin: 15, Destination: 15, Product: 20, Year: 10
#> Standard-errors: Clustered (Product)
#> Estimate Std. Error z value Pr(>|z|)
#> log(dist_km) -1.52787 0.098294 -15.544 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -7.025e+11 Adj. Pseudo R2: 0.764032
#> BIC: 1.405e+12 Squared Cor.: 0.612021
Note that you can always cluster the standard-errors, even when the estimation contained no fixed-effect:
gravity_simple = fepois(Euros ~ log(dist_km), trade)
# We use a formula to specify the variables used for two way clustering
# (note that the values of the variables are fetched directly in the original database)
summary(gravity_simple, ~Origin + Destination)
#> Poisson estimation, Dep. Var.: Euros
#> Observations: 38,325
#> Standard-errors: Clustered (Origin & Destination)
#> Estimate Std. Error z value Pr(>|z|)
#> (Intercept) 24.70889 1.124768 21.96798 < 2.2e-16 ***
#> log(dist_km) -1.02896 0.158022 -6.51145 7.4429e-11 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -2.426e+12 Adj. Pseudo R2: 0.185023
#> BIC: 4.852e+12 Squared Cor.: 0.055107
Finally, the standard-errors can also be computed at estimation time,
you simply need to add the vcov
argument:
fepois(Euros ~ log(dist_km), trade, vcov = ~Product)
#> Poisson estimation, Dep. Var.: Euros
#> Observations: 38,325
#> Standard-errors: Clustered (Product)
#> Estimate Std. Error z value Pr(>|z|)
#> (Intercept) 24.70889 0.330044 74.8654 < 2.2e-16 ***
#> log(dist_km) -1.02896 0.045954 -22.3909 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -2.426e+12 Adj. Pseudo R2: 0.185023
#> BIC: 4.852e+12 Squared Cor.: 0.055107
Talking about standard-errors… there are more than clustered standard-errors that can be computed… and there are many ways to achieve the same thing… and many shortcuts to know. So before you leave don’t forget to have a look at the section describing how to use the vcov argument!
Now we estimate the same relationship by OLS. We need to put the left hand side in logarithm (since the right-hand-side is not exponentialized):
Of course you can use different families in feglm
,
exactly as in glm
.
To get the estimation for the fixed-effects Negative Binomial:
Now let’s say that we want a compact overview of the results of
several estimations. The best way is to use the function
etable
. This function summarizes the results of several
fixest
estimations into a data.frame. To see the
fixed-effects results with the three different likelihoods, we just have
to type:
etable(gravity_pois, gravity_negbin, gravity_ols,
vcov = "twoway", headers = c("Poisson", "Negative Binomial", "Gaussian"))
gravity_pois | gravity_negbin | gravity_ols | ||
---|---|---|---|---|
1 | Poisson | Negative Binomial | Gaussian | |
3 | ||||
4 | log(dist_km) | -1.528*** (0.1307) | -1.711*** (0.1773) | -2.170*** (0.1714) |
5 | Fixed-Effects: | —————— | —————— | —————— |
6 | Origin | Yes | Yes | Yes |
7 | Destination | Yes | Yes | Yes |
8 | Product | Yes | Yes | Yes |
9 | Year | Yes | Yes | Yes |
10 | _______________ | __________________ | __________________ | __________________ |
11 | Family | Poisson | Neg. Bin. | OLS |
12 | S.E.: Clustered | by: Orig. & Dest. | by: Orig. & Dest. | by: Orig. & Dest. |
13 | Observations | 38,325 | 38,325 | 38,325 |
14 | Squared Cor. | 0.61202 | 0.43760 | 0.70558 |
15 | Pseudo R2 | 0.76403 | 0.03473 | 0.23640 |
16 | BIC | 1.4e+12 | 1,293,786.1 | 151,977.2 |
17 | Over-dispersion | – | 0.54877 | – |
We added the argument vcov="twoway"
to cluster the
standard-errors for all estimations. As can be seen this function gives
an overview of the estimates and standard-errors, as well as some
quality of fit measures. The argument headers
is used to
add information on each estimation column.
In the previous example, we directly added the estimation results as
arguments of the function etable
. But the function also
accepts lists of estimations. Let’s give an example. Say you want to see
the influence of the introduction of fixed-effects on the estimate of
the elasticity of distance. You can do it with the following code where
we use the argument fixef
to include fixed-effects (instead
of inserting them directly in the formula):
gravity_subfe = list()
all_FEs = c("Year", "Destination", "Origin")
for(i in 0:3){
gravity_subfe[[i+1]] = fepois(Euros ~ log(dist_km), trade, fixef = all_FEs[0:i])
}
The previous code performs 4 estimations with an increasing number of
fixed-effects and store their results into the list named
gravity_subfe
. To show the results of all 4 estimations,
it’s easy:
model 1 | model 2 | model 3 | model 4 | |
---|---|---|---|---|
Dependent Var.: | Euros | Euros | Euros | Euros |
Constant | 24.71*** (1.125) | |||
log(dist_km) | -1.029*** (0.1580) | -1.029*** (0.1581) | -1.226*** (0.2045) | -1.518*** (0.1282) |
Fixed-Effects: | —————— | —————— | —————— | —————— |
Year | No | Yes | Yes | Yes |
Destination | No | No | Yes | Yes |
Origin | No | No | No | Yes |
_______________ | __________________ | __________________ | __________________ | __________________ |
S.E.: Clustered | by: Orig. & Dest. | by: Orig. & Dest. | by: Orig. & Dest. | by: Orig. & Dest. |
Observations | 38,325 | 38,325 | 38,325 | 38,325 |
Squared Cor. | 0.05511 | 0.05711 | 0.16420 | 0.38479 |
Pseudo R2 | 0.18502 | 0.18833 | 0.35826 | 0.59312 |
BIC | 4.85e+12 | 4.83e+12 | 3.82e+12 | 2.42e+12 |
We have a view of the 4 estimations, all reporting two-way clustered
standard-errors thanks to the use of the argument
cluster
.
Note that since version 0.8.0, multiple estimations can be performed
at once without requiring loops. Let’s replicate the previous example
using fixest
stepwise functions:
The previous line of code performs 4 estimations. The function
csw0
is the key here, it means: cumulative stepwise
starting with the empty element. Starting with the empty element,
each new estimation adds a new element in the csw0()
function, quite like the previous loop. Then you can consider the
results, here res_multi
, as a list of results, although
with specific methods to easily access each element.
Stepwise functions can be applied to the linear right-hand-side and
to the fixed-effects, you can also have multiple dependent variables and
perform split sample estimations with the argument split
.
All of this is detailed in the dedicated vignette: Multiple
estimations.
So far we have seen how to report the results of multiple estimations
on the R console. Now, using the same function etable
, we
can also export the results to high quality Latex tables. We just need
to provide the argument tex = TRUE
:
# with two-way clustered SEs
etable(res_multi, cluster = ~Origin+Destination, tex = TRUE)
#> \begingroup
#> \centering
#> \begin{tabular}{lcccc}
#> \tabularnewline \midrule \midrule
#> Dependent Variable: & \multicolumn{4}{c}{Euros}\\
#> Model: & (1) & (2) & (3) & (4)\\
#> \midrule
#> \emph{Variables}\\
#> Constant & 24.71$^{***}$ & & & \\
#> & (1.125) & & & \\
#> log(dist\_km) & -1.029$^{***}$ & -1.029$^{***}$ & -1.226$^{***}$ & -1.518$^{***}$\\
#> & (0.1580) & (0.1581) & (0.2045) & (0.1282)\\
#> \midrule
#> \emph{Fixed-effects}\\
#> Year & & Yes & Yes & Yes\\
#> Destination & & & Yes & Yes\\
#> Origin & & & & Yes\\
#> \midrule
#> \emph{Fit statistics}\\
#> Observations & 38,325 & 38,325 & 38,325 & 38,325\\
#> Squared Correlation & 0.05511 & 0.05711 & 0.16420 & 0.38479\\
#> Pseudo R$^2$ & 0.18502 & 0.18833 & 0.35826 & 0.59312\\
#> BIC & $4.85\times 10^{12}$ & $4.83\times 10^{12}$ & $3.82\times 10^{12}$ & $2.42\times 10^{12}$\\
#> \midrule \midrule
#> \multicolumn{5}{l}{\emph{Clustered (Origin \& Destination) standard-errors in parentheses}}\\
#> \multicolumn{5}{l}{\emph{Signif. Codes: ***: 0.01, **: 0.05, *: 0.1}}\\
#> \end{tabular}
#> \par\endgroup
The user can export the Latex table directly into a file (argument
file
), add a title (arg. title
) and a label to
the table (arg. label
). Note that when the argument
file
is present, the Latex format becomes the default
(i.e. tex = TRUE
by default).
The coefficients can be renamed easily (arg. dict
), some
can be dropped (arg. drop
) and they can be easily reordered
with regular expressions (arg. order
).
The significance codes can easily be changed (arg.
signifCode
) and all quality of fit information can be
customized (argument fitstat
). Among others, the number of
fixed-effect per fixed-effect dimension can also be displayed using the
argument fixef_sizes
.
Consider the following example of the exportation of two tables:
# we set the dictionary once and for all
myDict = c("log(dist_km)" = "$\\ln (Distance)$", "(Intercept)" = "Constant")
# 1st export: we change the signif code and drop the intercept
etable(res_multi, signifCode = c("a" = 0.01, "b" = 0.05),
drop = "Const", dict = myDict, file = "Estimation Tables.tex",
replace = TRUE, title = "First export -- normal Standard-errors")
# 2nd export: clustered S-E + distance as the first coefficient
etable(res_multi, cluster = ~Product, order = "Dist",
dict = myDict, file = "Estimation Tables.tex",
title = "Second export -- clustered standard-errors (on Product variable)")
In this example, two tables containing the results of the 4
estimations are directly exported to a Latex table into the file
“Estimation Tables.tex”. First take notice (again) that we do not
need to use the argument tex=TRUE
since when the
argument file
is present, the Latex format becomes the
default. The file is re-created in the first exportation thanks to the
argument replace = TRUE
.
To change the variable names in the Latex table, we use the argument
dict
. The variable myDict
is the dictionary we
use to rename the variables, it is simply a named vector. The original
name of the variables correspond to the names of myDict
while the new names of the variables are the values of this vector. Any
variable that matches the names of myDict
will be replaced
by its value. Thus we do not care of the order of appearance of the
variables in the estimation results.
In the first export, the coefficient of the intercept is dropped by
using drop = "Const"
(could be anything such that
grepl(drop[1], "Constant")
is TRUE). In the second, the
coefficient of the distance is put before the intercept (which is kept)
thanks to the argument order
. Note that the actions
performed by the arguments drop
or order
are
performed after the renaming takes place with the
argument dict
.
Note that you can completely customize the style of the table by
using the style
and postprocessing
arguments,
please have a look at the dedicated vignette: Exporting
estimation tables.
To obtain the fixed-effects of the estimation, the function
fixef
must be performed on the results. This function
returns a list containing the fixed-effects coefficients for each
dimension. The summary
method helps to have a quick
overview:
fixedEffects = fixef(gravity_pois)
summary(fixedEffects)
#> Fixed_effects coefficients
#> Origin Destination Product Year
#> Number of fixed-effects 15 15 20 10
#> Number of references 0 1 1 1
#> Mean 23.3 3.09 0.0129 0.157
#> Standard-deviation 1.28 1.11 1.36 0.113
#>
#> COEFFICIENTS:
#> Origin: AT BE DE DK ES
#> 22.51 23.56 24.71 23.44 24.97 ... 10 remaining
#> -----
#> Destination: AT BE DE DK ES
#> 2.436 2.696 4.323 2.451 4.043 ... 10 remaining
#> -----
#> Product: 1 2 3 4 5
#> 0 1.414 0.6562 1.449 -1.521 ... 15 remaining
#> -----
#> Year: 2007 2008 2009 2010 2011
#> 0 0.06912 0.005225 0.07331 0.163 ... 5 remaining
We can see that the fixed-effects are balanced across the dimensions.
Indeed, apart from the first dimension, only one coefficient per
fixed-effect needs to be set as reference (i.e. fixed to 0) to avoid
collinearity across the different fixed-effects dimensions. This ensures
that the fixed-effects coefficients can be compared within a given
fixed-effect dimension. Had there be strictly more than one reference
per fixed-effect dimension, their interpretation would have not been
possible at all. If this was the case though, a warning message would
have been prompted. Note that the mean values are meaningless per se,
but give a reference points to which compare the fixed-effects within a
dimension. Let’s look specifically at the Year
fixed-effects:
fixedEffects$Year
#> 2007 2008 2009 2010 2011 2012
#> 0.000000000 0.069122284 0.005225473 0.073308208 0.163013386 0.192605170
#> 2013 2014 2015 2016
#> 0.230629376 0.242605404 0.282800683 0.310325692
Finally, the plot
method helps to distinguish the most
notable fixed-effects:
For each dimension, the fixed-effects are first centered, then sorted, and finally the most notable (i.e. highest and lowest) are reported. The exponential of the coefficient is reported in the right hand side to simplify the interpretation for models with log-link (as the Poisson model). As we can see from the country of destination fixed-effects, trade involving France (FR), Italy (IT) and Germany (DE) as destination countries is more than 2.7 times higher than the EU15 average. Further, the highest heterogeneity come from the product category, where trade in product 4 (dairy products) is roughly 2.7 times the average while product 14 (vegetable plaiting materials) represents a negligible fraction of the average.
Note however that the interpretation of the fixed-effects must be taken with extra care. In particular, here the fixed-effects can be interpreted only because they are perfectly balanced.
The version 0.10.0 of fixest
introduced the argument
vcov
. This argument is highly versatile and single-handedly
manages how the standard-errors are computed (note that you can find
many example in summary.fixest
help pages). This argument can be many things, so bear with me, and now,
let’s start trying to describe it!
So far (version 0.10.0), six types of standard-errors can be computed, here are their keywords and a brief description:
iid
: assumes that the error variance is spherical,
i.e. errors are homoskedastic and not correlated (independent and
identically distributed errors have a spherical error
variance).
hetero
: assumes that errors are heteroskedastic
(White correction).
cluster
, twoway
: clustered SEs, assumes
that errors are correlated within the cluster groups.
NW
, newey_west
: Newey and West (1987)
SEs for time series or panel data, assumes heteroskedastic and serially
correlated errors.
DK
, driscoll_kraay
: Driscoll and Kraay
(1998) SEs for panel data, assumes cross-sectionally and serially
correlated errors.
conley
: Conley (1999) SEs for cross-sections,
assumes spatially correlated errors.
The most basic uses of the vcov
argument are:
with a character scalar: vcov = "vcov_type"
(ex:
vcov = "hetero"
).
with a formula of the form:
vcov = vcov_type ~ variables
where the variables are used
to compute the SEs (ex: vcov = DK ~ period
).
Most of the VCOV types need the information on some variables to be computed. For these types, one then needs to use a formula to inform on these variables. Let’s give a first example:
data(base_did)
est = feols(y ~ x1, base_did)
# Note that there is partial matching enabled (newey = newey_west)
summary(est, newey ~ id + period)
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Standard-errors: Newey-West (L=1)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.988753 0.174111 11.4223 1.1709e-06 ***
#> x1 0.983110 0.052699 18.6551 1.6762e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.89686 Adj. R2: 0.262357
Here we queried Newey-West SEs and provided the panel identifiers in the right of the formula. Had we used the keyword only, that would have led to an error:
summary(est, "newey_west")
#> Error in vcov.fixest(object, vcov = vcov, ssc = ssc, forceCovariance = forceCovariance, : To compute the Newey-West VCOV, we need a variable for the time. Since you didn't provide it in the formula, we typically deduce it from the 'panel.id' identifiers. PROBLEM: no 'panel.id' was set in this estimation. Please provide it in the formula.
But, huh what does the error message says? That the time
variable can be deduced? Indeed, that’s the thing: the algorithm tries
hard to provide sensible default values for the user. Let’s now try with
panel identifiers set at estimation time:
est_panel = feols(y ~ x1, base_did, panel.id = ~id + period)
summary(est_panel, "newey_west")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Standard-errors: Newey-West (L=1)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.988753 0.174111 11.4223 1.1709e-06 ***
#> x1 0.983110 0.052699 18.6551 1.6762e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.89686 Adj. R2: 0.262357
Oh, now it works! However I can see some shade of disappointment in
your eyes: since we need to add panel.id = ~id + period
we
end up with more typing! Well, I’m not done: typically we tend to make
many estimations with the same data set, so it may be useful to set some
characteristics globally. This can be done with the
setFixest_estimation()
function:
setFixest_estimation(panel.id = ~id + period)
est_implicit = feols(y ~ x1, base_did)
summary(est_implicit, "newey_west")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Standard-errors: Newey-West (L=1)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.988753 0.174111 11.4223 1.1709e-06 ***
#> x1 0.983110 0.052699 18.6551 1.6762e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.89686 Adj. R2: 0.262357
Although the exact same two lines of code led to an error a few paragraphs ago, now it works fine.
Here is another example of implicit deduction:
summary(est_implicit, "cluster")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Standard-errors: Clustered (id)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.988753 0.194352 10.2327 < 2.2e-16 ***
#> x1 0.983110 0.046789 21.0115 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.89686 Adj. R2: 0.262357
The SEs are clustered at the unit identifier of the panel. Note that even if fixed-effects are present, the panel identifier takes precedence for clustering:
feols(y ~ x1 | period, base_did, "cluster")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: period: 10
#> Standard-errors: Clustered (id)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.997536 0.045721 21.818 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.5526 Adj. R2: 0.357059
#> Within R2: 0.297883
Of course, if the panel identifier is missing, the automatic clustering falls back to the first fixed-effect present:
# Removing the panel
setFixest_estimation(reset = TRUE)
feols(y ~ x1 | period, base_did, "cluster")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: period: 10
#> Standard-errors: Clustered (period)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.997536 0.050264 19.8458 9.7207e-09 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.5526 Adj. R2: 0.357059
#> Within R2: 0.297883
Talking about clustered SEs, note that this is such a common
operation that the empty keyword is equivalent to clustered SEs, so that
vcov = ~id + period
would lead to SEs clustered by
id
and period
:
feols(y ~ x1 | period, base_did, ~id + period)
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: period: 10
#> Standard-errors: Clustered (id & period)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.997536 0.047498 21.0015 5.8984e-09 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.5526 Adj. R2: 0.357059
#> Within R2: 0.297883
Finally, a last example using Conley SEs:
data(quakes)
feols(depth ~ mag, quakes, "conley")
#> OLS estimation, Dep. Var.: depth
#> Observations: 1,000
#> Standard-errors: Conley (90km)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 881.625 110.6727 7.96606 4.4465e-15 ***
#> mag -123.421 20.1746 -6.11765 1.3619e-09 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 209.6 Adj. R2: 0.052245
In this case the latitude and longitude are deduced from the
variables names in the data set used for the estimation (here these are
"lat"
and "long"
). Note that, for convenience,
an automatic distance cutoff is deduced from the data but is not likely
to be the most appropriate! But how to pass your own cutoff as a
parameter? That’s what we’ll see in the next section!
Some VCOVs require parameters: for example in the Newey-West VCOV, you need to provide the number of lags to consider. Although it is automatically deduced via a rule of thumb, the user is likely to want to use (or test) other values. To provide these extra parameters, you have two solutions:
use helper functions which have the same name as the VCOV
keywords (ex: NW
or newey_west
are two
functions).
use dedicated VCOV functions (ex: vcov_NW
).
We now cover these two methods in turn. Helper functions can be seen as supercharged keywords: they are used in place of the VCOV keywords but also accept arguments. Here are two examples:
feols(y ~ x1 | period, base_did, NW(2) ~ id + period)
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: period: 10
#> Standard-errors: Newey-West (L=2)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.997536 0.049344 20.2159 8.2589e-09 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.5526 Adj. R2: 0.357059
#> Within R2: 0.297883
feols(depth ~ mag, quakes, conley(200, distance = "spherical"))
#> OLS estimation, Dep. Var.: depth
#> Observations: 1,000
#> Standard-errors: Conley (200km)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 881.625 128.2426 6.87467 1.0937e-11 ***
#> mag -123.421 22.8950 -5.39074 8.7582e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 209.6 Adj. R2: 0.052245
In the first example, we use the helper function NW()
directly in the formula, exactly where the VCOV type would be. The first
(and only) argument of NW()
is the number of lags. On the
right hand side of the formula, we give the variables used to identify
the unit and the time variables, as usual.
In the second example, we use no formula but directly the helper
function conley()
for which we provide two arguments: the
cutoff (first argument) and how the distance should be computed. The
latitude and longitude are still deduced from the data. If it could not
be deduced, we would have to provide a formula giving them, like in the
previous example.
There are also dedicated VCOV functions which work in a more standard way. Let’s redo the same two examples with them:
feols(y ~ x1 | period, base_did, vcov_NW("id", "period", lag = 2))
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: period: 10
#> Standard-errors: Newey-West (L=2)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.997536 0.049344 20.2159 8.2589e-09 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.5526 Adj. R2: 0.357059
#> Within R2: 0.297883
feols(depth ~ mag, quakes, vcov_conley(lat = "lat", lon = "long",
cutoff = 200, distance = "spherical"))
#> OLS estimation, Dep. Var.: depth
#> Observations: 1,000
#> Standard-errors: Conley (200km)
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 881.625 128.2426 6.87467 1.0937e-11 ***
#> mag -123.421 22.8950 -5.39074 8.7582e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 209.6 Adj. R2: 0.052245
Contrary to the helper functions: a) these functions cannot be used in a formula, b) they accept the variables to compute the SEs as arguments. They provide an alternative way to specify the VCOV.
The value of the SEs can (sometimes quite surprisingly) be impacted
by the type of small sample correction (SSC) applied. In
fixest
you can monitor the SSC with the function
ssc()
. Details on how the SSCs are computed can be found in
the dedicated vignette: On
standard-errors – here we detail only the implementation.
Most fixest
functions accept an ssc
argument that you can readily use. Here’s an example:
est = feols(y ~ x1 | id, base_did)
est_up = feols(y ~ x1 | id, base_did, ssc = ssc(fixef.K = "full"))
est_down = feols(y ~ x1 | id, base_did, ssc = ssc(adj = FALSE, cluster.adj = FALSE))
etable(est, est_up, est_down)
#> est est_up est_down
#> Dependent Var.: y y y
#>
#> x1 0.9615*** (0.0481) 0.9615*** (0.0507) 0.9615*** (0.0478)
#> Fixed-Effects: ------------------ ------------------ ------------------
#> id Yes Yes Yes
#> _______________ __________________ __________________ __________________
#> S.E.: Clustered by: id by: id by: id
#> Observations 1,080 1,080 1,080
#> R2 0.38715 0.38715 0.38715
#> Within R2 0.26507 0.26507 0.26507
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Instead of providing the argument ssc
, you can instead
add the ssc
call directly within the formula of the
vcov
. In this case you should simply add it as a variable.
We now replicate the previous example using a list of several VCOVs in
etable
(that’s the only function that accepts lists in the
argument vcov
):
etable(est, vcov = list(~id, ~id + ssc(fixef.K = "full"),
~id + ssc(adj = FALSE, cluster.adj = FALSE)))
#> est est.1 est.2
#> Dependent Var.: y y y
#>
#> x1 0.9615*** (0.0481) 0.9615*** (0.0507) 0.9615*** (0.0478)
#> Fixed-Effects: ------------------ ------------------ ------------------
#> id Yes Yes Yes
#> _______________ __________________ __________________ __________________
#> S.E.: Clustered by: id by: id by: id
#> Observations 1,080 1,080 1,080
#> R2 0.38715 0.38715 0.38715
#> Within R2 0.26507 0.26507 0.26507
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
You can also tweak iid
or hetero
SEs using
a formula:
feols(y ~ x1 | id, base_did, iid ~ ssc(adj = FALSE))
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: id: 108
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.961525 0.048741 19.7272 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.46555 Adj. R2: 0.318981
#> Within R2: 0.265068
feols(y ~ x1 | id, base_did, hetero ~ ssc(adj = FALSE))
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: id: 108
#> Standard-errors: Heteroskedasticity-robust
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.961525 0.050226 19.1438 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.46555 Adj. R2: 0.318981
#> Within R2: 0.265068
Finally, we’re approaching the end of the tour of the
vcov
argument. That argument can also accept:
a matrix, which will be used as the VCOV (possibly useful in specific contexts)
a function to be applied to a fixest
object to
compute the VCOV.
The matrix case needs no explanation, let’s have a few lines on the function. You can provide custom functions to compute the VCOV:
summary(est, vcov = sandwich::vcovHC, type = "HC1")
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: id: 108
#> Standard-errors: vcovHC
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.961525 0.050226 19.1438 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.46555 Adj. R2: 0.318981
#> Within R2: 0.265068
The argument type
here is not an argument of
summary
but is passed directly to the function
vcovHC
. Note that in estimations you can still pass
functions but they must not accept extra arguments. Hence creating you
own wrapper function may be necessary:
feols(y ~ x1 | id, base_did, vcov = function(x) sandwich::vcovHC(x, type = "HC1"))
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: id: 108
#> Standard-errors: vcovHC(x, type = "HC1")
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.961525 0.050226 19.1438 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 4.46555 Adj. R2: 0.318981
#> Within R2: 0.265068
Two stage least square estimations can be performed by simply adding in the formula the link between the endogenous and the instrumental variables. Let’s have an example.
base = iris
names(base) = c("y", "x1", "x_endo_1", "x_inst_1", "fe")
set.seed(2)
base$x_inst_2 = 0.2 * base$y + 0.2 * base$x_endo_1 + rnorm(150, sd = 0.5)
base$x_endo_2 = 0.2 * base$y - 0.2 * base$x_inst_1 + rnorm(150, sd = 0.5)
est_iv = feols(y ~ x1 | x_endo_1 + x_endo_2 ~ x_inst_1 + x_inst_2, base)
est_iv
#> TSLS estimation - Dep. Var.: y
#> Endo. : x_endo_1, x_endo_2
#> Instr. : x_inst_1, x_inst_2
#> Second stage: Dep. Var.: y
#> Observations: 150
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.831380 0.411435 4.45121 1.6844e-05 ***
#> fit_x_endo_1 0.444982 0.022086 20.14744 < 2.2e-16 ***
#> fit_x_endo_2 0.639916 0.307376 2.08186 3.9100e-02 *
#> x1 0.565095 0.084715 6.67051 4.9180e-10 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.398842 Adj. R2: 0.761653
#> F-test (1st stage), x_endo_1: stat = 903.2 , p < 2.2e-16 , on 2 and 146 DoF.
#> F-test (1st stage), x_endo_2: stat = 3.25828, p = 0.041268, on 2 and 146 DoF.
#> Wu-Hausman: stat = 6.79183, p = 0.001518, on 2 and 144 DoF.
So we’ve just performed a two stage least squares estimation. The
formula coming after the pipe,
x_endo_1 + x_endo_2 ~ x_inst_1 + x_inst_2
, describes the
endogenous variables (on the left) and the instruments (on the
right).
By default, three statistics are displayed: the F-test from the first stage (weak instrument test), the Wu-Hausman endogeneity test and the overidentifying restrictions (Sargan) test. Note that the Sargan statistic appears only when relevant (i.e. when # instr. > # endo. vars., not the case here).
You can use the fitstat
command to summon other kind of
tests, notably Wald tests on the first/second stages:
fitstat(est_iv, ~ ivf1 + ivwald1 + ivf2 + ivwald2, cluster = "fe")
#> F-test (1st stage), x_endo_1: stat = 903.2 , p < 2.2e-16 , on 2 and 146 DoF.
#> F-test (1st stage), x_endo_2: stat = 3.25828, p = 0.041268, on 2 and 146 DoF.
#> Wald (1st stage), x_endo_1 : stat = 1,482.6 , p < 2.2e-16 , on 2 and 146 DoF, VCOV: Clustered (fe).
#> Wald (1st stage), x_endo_2 : stat = 2.22157, p = 0.112092, on 2 and 146 DoF, VCOV: Clustered (fe).
#> F-test (2nd stage): stat = 194.2 , p < 2.2e-16 , on 2 and 146 DoF.
#> Wald (2nd stage): stat = 539,363.2 , p < 2.2e-16 , on 2 and 146 DoF, VCOV: Clustered (fe).
As the Wald test relies on a given variance-covariance matrix, you
can pass extra arguments to fitstat
, as the argument
cluster
in the previous example, to specify which type of
VCOV matrix is desired.
Note that you can display the statistics that you wish when printing by changing the default print values:
setFixest_print(fitstat = ~ . + ivwald2)
est_iv
#> TSLS estimation - Dep. Var.: y
#> Endo. : x_endo_1, x_endo_2
#> Instr. : x_inst_1, x_inst_2
#> Second stage: Dep. Var.: y
#> Observations: 150
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 1.831380 0.411435 4.45121 1.6844e-05 ***
#> fit_x_endo_1 0.444982 0.022086 20.14744 < 2.2e-16 ***
#> fit_x_endo_2 0.639916 0.307376 2.08186 3.9100e-02 *
#> x1 0.565095 0.084715 6.67051 4.9180e-10 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.398842 Adj. R2: 0.761653
#> F-test (1st stage), x_endo_1: stat = 903.2 , p < 2.2e-16 , on 2 and 146 DoF.
#> F-test (1st stage), x_endo_2: stat = 3.25828, p = 0.041268, on 2 and 146 DoF.
#> Wu-Hausman: stat = 6.79183, p = 0.001518, on 2 and 144 DoF.
#> Wald (2nd stage): stat = 224.0 , p < 2.2e-16 , on 2 and 146 DoF, VCOV: IID.
In the previous code, fitstat = ~ . + ivwald2
means that
we want to add the second stage Wald test to the existing printed
statistics (represented here by the point).
Now what about adding some fixed-effects? That’s of course possible, you need to add them after the first right-hand-side, as follows:
est_iv_fe = feols(y ~ x1 | fe | x_endo_1 + x_endo_2 ~ x_inst_1 + x_inst_2, base)
est_iv_fe
#> TSLS estimation - Dep. Var.: y
#> Endo. : x_endo_1, x_endo_2
#> Instr. : x_inst_1, x_inst_2
#> Second stage: Dep. Var.: y
#> Observations: 150
#> Fixed-effects: fe: 3
#> Standard-errors: Clustered (fe)
#> Estimate Std. Error t value Pr(>|t|)
#> fit_x_endo_1 0.666671 0.106558 6.25640 0.024608 *
#> fit_x_endo_2 0.413839 0.177769 2.32796 0.145344
#> x1 0.451680 0.153375 2.94495 0.098553 .
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.327938 Adj. R2: 0.836626
#> Within R2: 0.585907
#> F-test (1st stage), x_endo_1: stat = 21.6 , p = 6.151e-9, on 2 and 146 DoF.
#> F-test (1st stage), x_endo_2: stat = 4.78816, p = 0.00968 , on 2 and 146 DoF.
#> Wu-Hausman: stat = 1.31408, p = 0.271968, on 2 and 142 DoF.
#> Wald (2nd stage): stat = 19.6 , p = 2.941e-8, on 2 and 146 DoF, VCOV: Clustered (fe).
To access the first stage(s), you can use the summary method:
summary(est_iv_fe, stage = 1)
#> IV: First stage: x_endo_1
#> TSLS estimation - Dep. Var.: x_endo_1
#> Endo. : x_endo_1, x_endo_2
#> Instr. : x_inst_1, x_inst_2
#> First stage: Dep. Var.: x_endo_1
#> Observations: 150
#> Fixed-effects: fe: 3
#> Standard-errors: Clustered (fe)
#> Estimate Std. Error t value Pr(>|t|)
#> x_inst_1 0.705992 0.485614 1.45381 0.28320
#> x_inst_2 0.202337 0.143302 1.41196 0.29346
#> x1 0.189320 0.135622 1.39594 0.29751
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.346509 Adj. R2: 0.959865
#> Within R2: 0.338407
#> F-test (1st stage): stat = 21.6, p = 6.151e-9, on 2 and 146 DoF.
#>
#> IV: First stage: x_endo_2
#> TSLS estimation - Dep. Var.: x_endo_2
#> Endo. : x_endo_1, x_endo_2
#> Instr. : x_inst_1, x_inst_2
#> First stage: Dep. Var.: x_endo_2
#> Observations: 150
#> Fixed-effects: fe: 3
#> Standard-errors: Clustered (fe)
#> Estimate Std. Error t value Pr(>|t|)
#> x_inst_1 -0.546745 0.081370 -6.71920 0.02144 *
#> x_inst_2 0.183092 0.083446 2.19415 0.15946
#> x1 0.153198 0.089148 1.71847 0.22785
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.51208 Adj. R2: 0.040133
#> Within R2: 0.063919
#> F-test (1st stage): stat = 4.78816, p = 0.00968, on 2 and 146 DoF.
When summary
shall return more than one element, the
object returned is not a regular fixest
object but a
fixest_multi
object. These kind of objects are covered in
the vignette: Multiple
estimations. You can display the first and second stages in a table
with etable
:
etable(summary(est_iv_fe, stage = 1:2), fitstat = ~ . + ivfall + ivwaldall.p)
#> summary(est_..1 summary(est_iv..2 summary(est_i..3
#> Dependent Var.: x_endo_1 x_endo_2 y
#>
#> x_inst_1 0.7060 (0.4856) -0.5467* (0.0814)
#> x_inst_2 0.2023 (0.1433) 0.1831 (0.0834)
#> x1 0.1893 (0.1356) 0.1532 (0.0891) 0.4517. (0.1534)
#> x_endo_1 0.6667* (0.1066)
#> x_endo_2 0.4138 (0.1778)
#> Fixed-Effects: --------------- ----------------- ----------------
#> fe Yes Yes Yes
#> _______________________ _______________ _________________ ________________
#> S.E.: Clustered by: fe by: fe by: fe
#> Observations 150 150 150
#> R2 0.96121 0.07234 0.84211
#> Within R2 0.33841 0.06392 0.58591
#> F-test (IV only) 21.581 4.7882 8.3352
#> Wald (IV only), p-value 2.29e-9 1.32e-9 2.94e-8
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Here we use stage = 1:2
to get all first stage
regressions followed by the second stage. Using stage = 2:1
would have done the opposite.
Now some explanations regarding fitstat
. The suffix
all
concerns IV only and means the following: if it’s a
first stage regression, then the first-stage F-stat is displayed,
otherwise it’s the second stage F-stat. The suffix .p
is
used in ivwaldall.p
to access the p-value and not the
statistic. Finally, you can permanently set which fit statistic to
display in etable
by using setFixest_etable
,
like for example
setFixest_etable(fitstat = ~ . + ivfall + ivwaldall.p)
.
Most R users will be familiar with the base expansion operators for
creating model interaction terms, e.g. x1*x2
,
x1:x2
, and x1/x2
. These base operators all
work with fixest
models. However, the package also provides
its own specialized syntax for creating interaction terms and combining
variables. Relative to the base methods, these fixest
methods offer significant performance gains and synergies with the
package’s other functions. To balance performance and convenience, the
exact syntax depends on whether the interaction involves fixed-effects
or not. Here we walk through both categories, further providing examples
of common use-cases.
There are two reasons why we would want to interact variables in the
fixed-effects slot. First, we may simply wish to combine fixed-effects
(e.g. firm × country effects). Second, we wish to allow for varying
slopes (e.g. a time trend for each firm). Let us consider each in turn,
using a lightly modified version of the iris
dataset:
# Our base data for this section
base = iris
names(base) = c("y", paste0("x", 1:3), "fe1")
# Create another "fixed-effect"
base$fe2 = rep(letters[1:5], 30)
head(base)
#> y x1 x2 x3 fe1 fe2
#> 1 5.1 3.5 1.4 0.2 setosa a
#> 2 4.9 3.0 1.4 0.2 setosa b
#> 3 4.7 3.2 1.3 0.2 setosa c
#> 4 4.6 3.1 1.5 0.2 setosa d
#> 5 5.0 3.6 1.4 0.2 setosa e
#> 6 5.4 3.9 1.7 0.4 setosa a
fe1^fe2^fe3...
)Say we want to “combine” the two fixed-effect variables
fe1
and fe2
to create a brand new fixed-effect
variable. We can do it simply via fixest
’s special
^
operator:
est_comb = feols(y ~ x1 | fe1^fe2, base)
est_comb
#> OLS estimation, Dep. Var.: y
#> Observations: 150
#> Fixed-effects: fe1^fe2: 15
#> Standard-errors: Clustered (fe1^fe2)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.782815 0.119465 6.55267 1.2854e-05 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.406785 Adj. R2: 0.729861
#> Within R2: 0.280234
The ^
operator does the same thing as
paste0(species, "_", fe)
, but is more convenient and
significantly faster for large datasets. You can still extract the
fixed-effects the same way:
fixef(est_comb)[[1]]
#> setosa_a setosa_b setosa_c setosa_d setosa_e versicolor_a
#> 2.443630 2.384084 2.164943 2.296256 2.323630 3.713320
#> versicolor_b versicolor_c versicolor_d versicolor_e virginica_a virginica_b
#> 3.800694 4.003367 3.745539 3.575086 4.513272 3.986351
#> virginica_c virginica_d virginica_e
#> 4.423725 4.216804 4.159382
Note further that more than two fixed-effects can be combined in
exactly the same manner (e.g. fe1^fe2^fe3
), and the syntax
carries over to multivariate clustering too
(e.g. cluster = ~fe1^fe2^fe3
).
fe[x]
)You can introduce variables with varying slopes directly into the
fixed-effects part of the formula using square brackets
([]
). Recall that varying slopes allow us to flexibly
control for heterogeneous effects across groups. Common real-life
examples could be the inclusion of time trends for each observational
unit (e.g. country), or allowing for the effect of some control variable
(e.g. income) to be moderated by a fixed-effect (e.g. gender). Here we
demonstrate by continuing with our simple dataset.
head(base)
#> y x1 x2 x3 fe1 fe2
#> 1 5.1 3.5 1.4 0.2 setosa a
#> 2 4.9 3.0 1.4 0.2 setosa b
#> 3 4.7 3.2 1.3 0.2 setosa c
#> 4 4.6 3.1 1.5 0.2 setosa d
#> 5 5.0 3.6 1.4 0.2 setosa e
#> 6 5.4 3.9 1.7 0.4 setosa a
Say we want to estimate y
as a function of
x1
, but controlling for x2
. Moreover, we think
that the slope coefficient of our x2
control variable
should be allowed to vary by the fe1
fixed-effect variable.
We can do this as follows:
est_vs = feols(y ~ x1 | fe1[x2], base)
est_vs
#> OLS estimation, Dep. Var.: y
#> Observations: 150
#> Fixed-effects: fe1: 3
#> Varying slopes: x2 (fe1): 3
#> Standard-errors: Clustered (fe1)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.450006 0.156731 2.8712 0.10292
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.298706 Adj. R2: 0.863506
#> Within R2: 0.178944
If you want to see the slopes for x2
, just use the
function fixef
:
summary(fixef(est_vs))
#> Fixed-effects/Slope coefficients
#> fe1 x2 (slopes: fe1)
#> Number of fixed-effects/slopes 3 3
#> Number of references 0 0
#> Mean 1.7 0.639
#> Standard-deviation 1.32 0.262
#>
#> COEFFICIENTS:
#> fe1: setosa versicolor virginica
#> 2.926 1.879 0.3068
#> -----
#> x2 (slopes: fe1): setosa versicolor virginica
#> 0.3677 0.6598 0.8903
Note that this produces the same result as
feols(y ~ x1 + fe1/x2, base)
, but is much more performant
for large datasets. The trade-off from the fe1[x2]
method
is that we lose the ability to estimate confidence intervals on the
resulting slope coefficients. This should be fine in cases where we are
just trying to control for some confounding or nuisance parameters. If
you are interested in conducting statistical inference on the resulting
slope coefficients and require confidence intervals, then you should use
the slower fe1/x2
approach instead.
The preceding interaction examples all took place in the
fixed-effects slot (i.e. after the |
). Underneath the hood,
methods like fe1^fe2
and fe1[x2]
use numerical
shortcuts that greatly speed up computation. This comes at the cost of
being able to do richer inference with the interacted terms —
e.g. construct confidence intervals — since they are swept out of the
model at estimation time. In many cases, this should prove to be a
perfectly acceptable trade-off. After all, the primary motivation for
estimating fixed-effects models in the first place is to remove the
confounding effect of such “nuisance” parameters.
Yet, there are equally many cases where we do want to retain full
inferential information about interaction terms. For example, in a
difference-in-differences (DiD) research design. Here too
fixest
offers its own specialized syntax for combining
terms in the model formula: i()
.
As we shall see, i()
is more versatile than just
creating interaction terms. It is also able to coerce individual
variables to a factor and, compared to base R factor()
,
does so in a way that allows for better synergies with other
fixest
functions like etable
and
coefplot
/iplot
. This will allow us to perform
some common estimation tasks much more easily.
We now illustrate the main uses of i()
with the help of
some examples.
i()
The function i()
accepts the arguments ref
,
and keep
which are used to identify which levels to keep.
Here’s an example how to use them:
data(airquality)
res_i1 = feols(Ozone ~ Solar.R + i(Month), airquality)
res_i2 = feols(Ozone ~ Solar.R + i(Month, ref = 8), airquality)
res_i3 = feols(Ozone ~ Solar.R + i(Month, keep = 5:6), airquality)
etable(res_i1, res_i2, res_i3, dict = c("6" = "June", "Month::5" = "May"),
order = c("Int|May", "Mon"))
#> res_i1 res_i2
#> Dependent Var.: Ozone (ppb) Ozone (ppb)
#>
#> May -36.90*** (8.201)
#> Month = June 5.069 (10.98) -31.83** (11.05)
#> Month = 7 31.04*** (8.018) -5.861 (8.146)
#> Month = 8 36.90*** (8.201)
#> Month = 9 8.912 (7.763) -27.99*** (7.845)
#> Constant 3.219 (7.919) 40.12*** (7.828)
#> Solar Radiation (Langleys) 0.1148*** (0.0300) 0.1148*** (0.0300)
#> __________________________ __________________ __________________
#> S.E. type IID IID
#> Observations 111 111
#> R2 0.31974 0.31974
#> Adj. R2 0.28735 0.28735
#>
#> res_i3
#> Dependent Var.: Ozone (ppb)
#>
#> May -24.50*** (6.936)
#> Month = June -19.46. (10.46)
#> Month = 7
#> Month = 8
#> Month = 9
#> Constant 25.82*** (6.681)
#> Solar Radiation (Langleys) 0.1253*** (0.0311)
#> __________________________ __________________
#> S.E. type IID
#> Observations 111
#> R2 0.22452
#> Adj. R2 0.20278
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Now that we’ve seen the basic i()
functionality with a
single variable, let’s see how it can be put to use in an interaction
context. We will consider two DiD examples of increasing complexity.
To illustrate i()
’s interaction functionality, we will
estimate treatment effects over time in a simple DiD setup.
Consider the following dataset where some individuals (identified by
the variable id
) receive a treatment and others do not (as
represented by the variable treat
). The treatment takes
effect from period
6 onward. The data look like this:
# Sample data illustrating the DiD
data(base_did)
head(base_did)
#> y x1 id period post treat
#> 1 2.87530627 0.5365377 1 1 0 1
#> 2 1.86065272 -3.0431894 1 2 0 1
#> 3 0.09416524 5.5768439 1 3 0 1
#> 4 3.78147485 -2.8300587 1 4 0 1
#> 5 -2.55819959 -5.0443544 1 5 0 1
#> 6 1.72873240 -0.6363849 1 6 1 1
The empirical approach that we will use here is the canonical two-way
fixed effects (TWFE) model that should be familiar to many empirical
researchers. In a regression context, TWFE essentially amounts to an
interaction between our treat
and period
variables. This is easily done using the
i(fact_var, num_var, reference)
syntax:
# Estimation of treatment × period effects
# We also add individual and period fixed-effects:
est_did = feols(y ~ x1 + i(period, treat, 5) | id + period, base_did)
est_did
#> OLS estimation, Dep. Var.: y
#> Observations: 1,080
#> Fixed-effects: id: 108, period: 10
#> Standard-errors: Clustered (id)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.973490 0.045678 21.311868 < 2.2e-16 ***
#> period::1:treat -1.403045 1.110267 -1.263701 2.0908e-01
#> period::2:treat -1.247511 1.093145 -1.141213 2.5633e-01
#> period::3:treat -0.273206 1.106935 -0.246813 8.0553e-01
#> period::4:treat -1.795721 1.087974 -1.650518 1.0177e-01
#> period::6:treat 0.784452 1.028388 0.762798 4.4726e-01
#> period::7:treat 3.598897 1.101563 3.267081 1.4609e-03 **
#> period::8:treat 3.811766 1.247502 3.055519 2.8366e-03 **
#> period::9:treat 4.731426 1.097113 4.312617 3.6041e-05 ***
#> period::10:treat 6.606229 1.120494 5.895817 4.4031e-08 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 3.83653 Adj. R2: 0.48783
#> Within R2: 0.389628
Here, i(period, treat, 5)
creates a set of interact
terms: One treat
dummy for each period
, but
excluding period 5 as a reference. While the explicit reference period
is optional, note that we need a reference to avoid the collinearity
problem posed by the id
fixed effects. More to the point,
for this DiD analysis we are interested in whether the treatment
generated a sustained impact on our outcome variable relative to the
control group. This makes period 5 (immediately prior to treatment) the
obvious choice to use as our relative anchor. It also demonstrates an
advantage that i()
’s syntax offers over the equivalent base
treat*factor(period)
expansion, which would automatically
use period 1 as a reference. Of course, we could specify the levels of
factor(period)
ahead of time. But this is rather tedious,
whereas i()
allows us to do so concisely on the fly.
To display the treatment effects on a graph, we can use the function
iplot
:
The function iplot
reports the coefficients of variables
created with i()
, and only them. In case you wanted to
display all the coefficients, including x1
, you can use the
function coefplot
instead.
Note that the content of this section is only valid for
fixest
version 0.9.0 or later.
Despite TWFE’s long-standing popularity for DiD designs, recent research has a shone a light on the biases that it can introduce under differential timing. For example, under staggered treatment or policy rollout.
For staggered DiD analyzes, fixest
provides the
sunab
function for implementing the unbiased method of Sun and Abraham
(2020) — hereafter: SA20. The method is based on the estimation of
treated cohort x time to treatment
dummies which are later
aggregated to obtain the average treatment for the treated (ATT) for
each period (or for the full post treatment period).
(Aside: Note that we use time to treatment
rather than
just time
, because we need to account for the staggered
treatment via a relative time measure.)
Let’s walk through an example with the base_stagg
data
set, where (a) different cohorts get the treatment at different periods,
and (b) the effect of the treatment is cohort-specific and increasing
over time. Let’s have a first look at the data:
data(base_stagg)
head(base_stagg)
#> id year year_treated time_to_treatment treated treatment_effect_true
#> 2 90 1 2 -1 1 0
#> 3 89 1 3 -2 1 0
#> 4 88 1 4 -3 1 0
#> 5 87 1 5 -4 1 0
#> 6 86 1 6 -5 1 0
#> 7 85 1 7 -6 1 0
#> x1 y
#> 2 -1.0947021 0.01722971
#> 3 -3.7100676 -4.58084528
#> 4 2.5274402 2.73817174
#> 5 -0.7204263 -0.65103066
#> 6 -3.6711678 -5.33381664
#> 7 -0.3152137 0.49562631
Note that the variable year_treated
is set to 1000
(i.e. above the maximum value of year
) for the never
treated. Here’s a quick visual depiction of the data. Again, notice the
staggered treatment rollout and time-varying intensity.
With our data in hand, let’s move on to the estimations. We’ll implement two DiD models:
# "Naive" TWFE DiD (note that the time to treatment for the never treated is -1000)
# (by using ref = c(-1, -1000) we exclude the period just before the treatment and
# the never treated)
res_twfe = feols(y ~ x1 + i(time_to_treatment, ref = c(-1, -1000)) | id + year, base_stagg)
# To implement the Sun and Abraham (2020) method,
# we use the sunab(cohort, period) function
res_sa20 = feols(y ~ x1 + sunab(year_treated, year) | id + year, base_stagg)
Let’s compare our results in plot form:
# Plot the two TWFE results
iplot(list(res_twfe, res_sa20), sep = 0.5)
# Add the true results
att_true = tapply(base_stagg$treatment_effect_true, base_stagg$time_to_treatment, mean)[-1]
points(-9:8, att_true, pch = 15, col = 4)
legend("topleft", col = c(1, 4, 2), pch = c(20, 15, 17),
legend = c("TWFE", "Truth", "Sun & Abraham (2020)"))
As we can see, the TWFE results suffer from varying degrees of bias due to the staggered rollout. In contrast, the aggregated SA20 results do a much better job of consistently estimating the true effects.
As a final example, here’s how to get the average treatment effect for the treated (ATT):
# The full ATT
summary(res_sa20, agg = "att")
#> OLS estimation, Dep. Var.: y
#> Observations: 950
#> Fixed-effects: id: 95, year: 10
#> Standard-errors: Clustered (id)
#> Estimate Std. Error t value Pr(>|t|)
#> x1 0.994678 0.018378 54.12293 < 2.2e-16 ***
#> ATT -1.133749 0.205070 -5.52858 2.882e-07 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.921817 Adj. R2: 0.887984
#> Within R2: 0.876406
This time the aggregation of the coefficients is operated across each cohort for non-negative time to treatment. Note that the estimated ATT compares favourably with the true value of -1.
Under the hood, the sunab()
function creates
cohort x time to treatment
interactions with the function
i()
, the coefficients are then aggregated at the
appropriate level with the function aggregate.fixest
. To
obtain the coefficients for each
cohort x time to treatment
, one simply needs to remove the
aggregation:
# Full disaggregation (you could have used summary instead of etable)
head(etable(res_sa20, agg = FALSE), 20)
#> res_sa20
#> Dependent Var.: y
#>
#> x1 0.9947*** (0.0184)
#> year = -9 x cohort = 10 0.3518 (0.3591)
#> year = -8 x cohort = 9 0.0339 (0.4714)
#> year = -8 x cohort = 10 -0.1919 (0.3529)
#> year = -7 x cohort = 8 -0.5894 (0.7369)
#> year = -7 x cohort = 9 0.8730. (0.4934)
#> year = -7 x cohort = 10 0.0195 (0.6034)
#> year = -6 x cohort = 7 -0.0421 (0.8657)
#> year = -6 x cohort = 8 -0.6576 (0.5733)
#> year = -6 x cohort = 9 0.8777 (0.5333)
#> year = -6 x cohort = 10 -0.4036 (0.3474)
#> year = -5 x cohort = 6 -0.6580 (0.9134)
#> year = -5 x cohort = 7 -0.3170 (0.6979)
#> year = -5 x cohort = 8 -0.2382 (0.4697)
#> year = -5 x cohort = 9 0.3015 (0.6042)
#> year = -5 x cohort = 10 -0.5648 (0.4632)
#> year = -4 x cohort = 5 -0.9835 (0.6345)
#> year = -4 x cohort = 6 0.3604 (0.8583)
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Now we present some other features of the package:
It can be useful, to tidy up the workflow or simply for convenience,
to define formula macros: i.e. macro variables each representing several
variables. This package offers two functions to deal with that:
setFixest_fml
to set macro variables globally, and
xpd
to create a formula with macro variables either
globally defined or defined at run time.
Here is an example:
base = iris
names(base) = c("y", "x1", "x2", "x3", "species")
# Defining the macro variables
setFixest_fml(..ctrl = ~poly(x2, 2) + poly(x3, 2))
# Accessing them
xpd(y ~ x1 + ..ctrl)
#> y ~ x1 + poly(x2, 2) + poly(x3, 2)
# Definition at run time
vars = c("x2", "x2^2", "x3")
for(i in 1:3){
print(xpd(y ~ x1 + ..ctrl, ..ctrl = vars[1:i]))
}
#> y ~ x1 + x2
#> y ~ x1 + x2 + x2^2
#> y ~ x1 + x2 + x2^2 + x3
Macro variables must start with two dots. As seen in the example,
once set globally they can be directly accessed with xpd
.
In the example, xpd
redefines the formula at run-time by
having a character vector as input.
All fixest
estimations call xpd
internally
if appropriate. This means that the following code works just fine:
feols(y ~ x1 + ..ctrl, base)
#> OLS estimation, Dep. Var.: y
#> Observations: 150
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 4.122797 0.233398 17.66423 < 2.2e-16 ***
#> x1 0.562757 0.075897 7.41470 9.5941e-12 ***
#> poly(x2, 2)1 12.601293 1.782973 7.06758 6.2621e-11 ***
#> poly(x2, 2)2 1.635558 0.589023 2.77673 6.2216e-03 **
#> poly(x3, 2)1 -2.757047 1.725003 -1.59829 1.1217e-01
#> poly(x3, 2)2 -1.055565 0.668027 -1.58012 1.1627e-01
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.30128 Adj. R2: 0.862108
The function xpd
also accepts regular expression macros
of the form ..("regex")
(or regex("regex")
).
If these macros are encountered and provided a character
vector/data.frame is in the argument data
, then all
variables names matching the regular expression will be placed in the
formula.
data(longley)
xpd(Armed.Forces ~ Population + regex("GNP|ployed"), data = longley)
#> Armed.Forces ~ Population + GNP.deflator + GNP + Unemployed +
#> Employed
Again, since xpd
is called internally, the following
works:
feols(Armed.Forces ~ Population + regex("GNP|ployed"), longley)
#> OLS estimation, Dep. Var.: Armed.Forces
#> Observations: 16
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 4403.682352 4091.847594 1.076209 0.307112
#> Population -22.844324 32.671302 -0.699217 0.500356
#> GNP.deflator 7.638472 12.347773 0.618611 0.550003
#> GNP 3.150533 3.554170 0.886433 0.396201
#> Unemployed -0.591649 0.389005 -1.520928 0.159248
#> Employed -50.059800 25.348299 -1.974878 0.076522 .
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 36.1 Adj. R2: 0.569345
The special operator .[]
can be used in
fixest
formulas to replace the enclosed item by its value
in the current environment. Let’s give an example:
base = setNames(iris, c("y", "x1", "x2", "x3", "species"))
i = 2:3
z = "i(species)"
feols(y ~ x.[i] + .[z], base)
#> OLS estimation, Dep. Var.: y
#> Observations: 150
#> Standard-errors: IID
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 3.682982 0.107403 34.291343 < 2.2e-16 ***
#> x2 0.905946 0.074311 12.191282 < 2.2e-16 ***
#> x3 -0.005995 0.156260 -0.038368 9.6945e-01
#> species::versicolor -1.598362 0.205706 -7.770113 1.3154e-12 ***
#> species::virginica -2.112647 0.304024 -6.948940 1.1550e-10 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> RMSE: 0.333482 Adj. R2: 0.832221
What just happened? When .[]
is encountered in a
formula, its value is evaluated and inserted verbatim in the formula.
Further, when the value in brackets is a vector, as many variables are
added in the model. That’s why x.[i]
led to
x2 + x3
. Of course, numbers can be used directly:
x.[2:3]
would have led to the same result.
Variable names in which .[]
is in the middle of the name
can also be created, but it has to be nested:
How does it work? .[stuff]
evaluates stuff
and if stuff is a string literal, the function dsb
, which
expands anything in .[]
, is applied. In the previous
example, dsb("x.[i]_sq")
leads to the vector
c("x1_sq", "x2_sq", "x3_sq")
. Then vector is then
aggregated with a sum due to the initial .[]
, leading to
x1_sq + x2_sq + x3_sq
being inserted in the formula.
By default, when stuff
is a vector, the aggregation is
done with a sum. But in some instances, it can be interesting to
aggregate with commas: e.g. when you want to perform a stepwise
estimation. To summon comma-aggregation, place a comma right after the
opening square bracket. Here’s an example:
etable(feols(y ~ csw(x.[, 1:3]), base))
#> feols(y ~ csw(..1 feols(y ~ csw(x..2 feols(y ~ csw(x...3
#> Dependent Var.: y y y
#>
#> Constant 6.526*** (0.4789) 2.249*** (0.2480) 1.856*** (0.2508)
#> x1 -0.2234 (0.1551) 0.5955*** (0.0693) 0.6508*** (0.0667)
#> x2 0.4719*** (0.0171) 0.7091*** (0.0567)
#> x3 -0.5565*** (0.1275)
#> _______________ _________________ __________________ ___________________
#> S.E. type IID IID IID
#> Observations 150 150 150
#> R2 0.01382 0.84018 0.85861
#> Adj. R2 0.00716 0.83800 0.85571
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Finally, there is a special shortcut to facilitate multiple
estimations with variable names stored in a vector. If vars
is a vector of variable names, just use .[vars]
in the LHS
to perform a multiple estimation:
vars = c("x1", "x2", "x3") # Equiv. to: dsb("x.[1:3]")
etable(feols(.[vars] ~ i(species), base))
#> feols(.[vars] ~ ..1 feols(.[vars] ..2 feols(.[vars] ~..3
#> Dependent Var.: x1 x2 x3
#>
#> Constant 3.428*** (0.0480) 1.462*** (0.0609) 0.2460*** (0.0289)
#> species = versicolor -0.6580*** (0.0679) 2.798*** (0.0861) 1.080*** (0.0409)
#> species = virginica -0.4540*** (0.0679) 4.090*** (0.0861) 1.780*** (0.0409)
#> ____________________ ___________________ _________________ __________________
#> S.E. type IID IID IID
#> Observations 150 150 150
#> R2 0.40078 0.94137 0.92888
#> Adj. R2 0.39263 0.94057 0.92792
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Some methods have been created to easily deal with leads and lags in
a panel setting. First is shown the various ways of how to deal with it
in a fixest
estimation, then how to create a panel data
set, last is described a general way to create lead and lag
variables.
There are two ways to provide leads and/or lags in a
fixest
estimation. Either “on-the-fly” by using the
argument panel.id
, either by setting up a panel data set
with the function panel
(useful if you run multiple models
needing lags and/or leads), described in the next subsection.
To set up the panel on-the-fly, you need to use the
panel.id
argument, which will give you access to the
functions f
and l
to create leads and lags,
respectively. Let’s give an example, using the previous data set, where
we use lags and leads of the explanatory and dependent variables.
est1 = feols(y ~ l(x1, 0:1), base_did, panel.id = ~id+period)
est2 = feols(f(y) ~ l(x1, -1:1), base_did, panel.id = ~id+period)
est3 = feols(l(y) ~ l(x1, 0:3), base_did, panel.id = ~id+period)
etable(est1, est2, est3, order = "f", drop = "Int")
#> est1 est2 est3
#> Dependent Var.: y f(y,1) l(y,1)
#>
#> f(x1,1) 0.9940*** (0.0542)
#> Constant 2.235*** (0.2032) 2.464*** (0.2233) 2.196*** (0.2110)
#> x1 0.9948*** (0.0487) 0.0081 (0.0592) -0.0534 (0.0545)
#> l(x1,1) 0.0410 (0.0558) 0.0157 (0.0640) 0.9871*** (0.0551)
#> l(x1,2) 0.0220 (0.0580)
#> l(x1,3) 0.0102 (0.0639)
#> _______________ __________________ __________________ __________________
#> S.E.: Clustered by: id by: id by: id
#> Observations 972 864 756
#> R2 0.26558 0.25697 0.25875
#> Adj. R2 0.26406 0.25438 0.25480
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
First of all, the value of panel.id
corresponds to panel
identifiers: first comes the variable identifying the panel-individuals,
then comes the variables identifying the time. In the example, the
panel.id
came in the form of a one-sided formula, but it
could equivalently be equal to panel.id = c("id", "period")
or panel.id = "id,period"
.
As we can see, in the first estimation, a lag is created with the
function l
. The second argument of the function consists of
a vector giving the lags we want. In this case, l(x1, 0:1)
means we want x1
and the first lag of x1
. This
argument accepts negative values which give leads, as shown in the
second estimation where l(x1, -1:1)
means that we want the
first lead of x1
, x1
, then its first lag. In
this example, we also use the first lead of y
as a
dependent variable with f(y)
.
You can set up a panel data set with the function panel
.
There are between two and three advantages of doing so. First, if you
have to estimate many models with leads and/or lags, setting up a panel
gives you access to the lagging functions, f
and
l
, without having to provide the panel.id
argument we’ve seen in the previous subsection. Second, even when you
estimate models with a sub-selection of the panel data, the data set is
still a proper panel, meaning you can still use the lagging functions.
Finally, and only if you are a data.table
user, you can use
the lagging functions to create new variables.
Let’s repeat the previous example, now with a panel data set:
# setting up the panel
pdat = panel(base_did, ~id + period)
# Now the panel.id argument is not required
est1 = feols(y ~ l(x1, 0:1), pdat)
est2 = feols(f(y) ~ l(x1, -1:1), pdat)
# You can use sub selections of the panel data
est_sub = feols(y ~ l(x1, 0:1), pdat[!pdat$period %in% c(2, 4)])
etable(est1, est2, est_sub, order = "f", drop = "Int")
#> est1 est2 est_sub
#> Dependent Var.: y f(y,1) y
#>
#> f(x1,1) 0.9940*** (0.0542)
#> Constant 2.235*** (0.2032) 2.464*** (0.2233) 3.691*** (0.3085)
#> x1 0.9948*** (0.0487) 0.0081 (0.0592) 1.013*** (0.0707)
#> l(x1,1) 0.0410 (0.0558) 0.0157 (0.0640) -0.0063 (0.0779)
#> _______________ __________________ __________________ _________________
#> S.E.: Clustered by: id by: id by: id
#> Observations 972 864 540
#> R2 0.26558 0.25697 0.26258
#> Adj. R2 0.26406 0.25438 0.25983
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Last, if you also use data.table
, let’s give an example
of lead/lag creation:
library(data.table)
pdat_dt = panel(as.data.table(base_did), ~id+period)
# we create a lagged value of the variable x1
pdat_dt[, x1_l1 := l(x1)]
# Now
pdat_dt[, c("x1_l1_fill0", "y_f2") := .(l(x1, fill = 0), f(y, 2))]
head(pdat_dt)
#> y x1 id period post treat x1_l1 x1_l1_fill0
#> <num> <num> <int> <int> <num> <num> <num> <num>
#> 1: 2.87530627 0.5365377 1 1 0 1 NA 0.0000000
#> 2: 1.86065272 -3.0431894 1 2 0 1 0.5365377 0.5365377
#> 3: 0.09416524 5.5768439 1 3 0 1 -3.0431894 -3.0431894
#> 4: 3.78147485 -2.8300587 1 4 0 1 5.5768439 5.5768439
#> 5: -2.55819959 -5.0443544 1 5 0 1 -2.8300587 -2.8300587
#> 6: 1.72873240 -0.6363849 1 6 1 1 -5.0443544 -5.0443544
#> y_f2
#> <num>
#> 1: 0.09416524
#> 2: 3.78147485
#> 3: -2.55819959
#> 4: 1.72873240
#> 5: 6.28423629
#> 6: 4.76688778
If you just want to create a single lag/lead variable, a simple and
fast method has been implemented: lag.formula
. Let’s give
an example:
base_lag = base_did
# we create a lagged value of the variable x1
base_lag$x1.l1 = lag(x1 ~ id + period, 1, base_lag)
head(base_lag)
#> y x1 id period post treat x1.l1
#> 1 2.87530627 0.5365377 1 1 0 1 NA
#> 2 1.86065272 -3.0431894 1 2 0 1 0.5365377
#> 3 0.09416524 5.5768439 1 3 0 1 -3.0431894
#> 4 3.78147485 -2.8300587 1 4 0 1 5.5768439
#> 5 -2.55819959 -5.0443544 1 5 0 1 -2.8300587
#> 6 1.72873240 -0.6363849 1 6 1 1 -5.0443544
The first two arguments are mandatory. The formula informs on the variable to be lagged (on the left hand side), and the two panel identifiers. Note that the time index must appear second. The second argument tells how much lags we want. Using negative values gives leads. Finally the last argument informs on where to find the variables.
In case you use the popular package data.table
, you can
create lagged variables very simply:
The function feNmlm
is similar to femlm
but
allows to have non-linear in parameters right-hand-sides (RHS). First an
example without fixed-effects, the one with fixed-effects is given
later. Let’s say we want to estimate the following relation with a
Poisson model:
\(E\left(z_i\right) = a\times x_i + b\times y_i\).
In fact, this type of model is non-linear in the context of a Poisson model because the sum is embedded within the log:
\(E\left(z_i\right) = \exp\left(\log\left(a\times x_i + b\times y_i\right)\right)\).
So let’s estimate such a relation. (Note that you can estimate this relation with GLM and identity link, but I carry on for the example.) First we generate the data:
# Generating data:
n = 1000
# x and y: two positive random variables
x = rnorm(n, 1, 5)**2
y = rnorm(n, -1, 5)**2
# E(z) = 2*x + 3*y and some noise
z = rpois(n, 2*x + 3*y) + rpois(n, 1)
base = data.frame(x, y, z)
To estimate the non-linear relationship, we need to use the argument
NL.fml
where we put the non-linear part. We also have to
provide starting values with the argument NL.start
.
Finally, to ensure the RHS can be evaluated in any situation, we add
lower bounds for the parameters with the argument
lower
.
result_NL = feNmlm(z~0, base, NL.fml = ~ log(a*x + b*y), NL.start = list(a=1, b=1), lower = list(a=0, b=0))
Note that the arguments NL.start
and lower
are named lists. Setting lower = list(a=0, b=0)
means that
the optimization algorithm will never explore parameters for \(a\) and \(b\) that are lower than 0. The results
obtained can be interpreted similarly to results with linear RHS. We can
see them with a print:
print(result_NL)
#> Non-linear ML estimation, family = Poisson, Dep. Var.: z
#> Observations: 1,000
#> Standard-errors: IID
#> Estimate Std. Error z value Pr(>|z|)
#> a 2.02334 0.011217 180.383 < 2.2e-16 ***
#> b 3.02817 0.012684 238.736 < 2.2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#> Log-Likelihood: -3,596.8 Adj. Pseudo R2: 0.942674
#> BIC: 7,207.5 Squared Cor.: 0.993353
We can see that we obtain coefficients close to the generating values.
Adding fixed-effects is identical to the linear case. The user must only be well aware of the functional form. Indeed, the fixed-effects must enter the estimation linearly. This means that the previous equation with one set of fixed-effects writes:
\(E\left(z_i\right) = \gamma_{id_i} \left( a\times x_i + b\times y_i \right)\),
where \(id_i\) is the class of observation \(i\) and \(\gamma\) is the vector of fixed-effects. Here the fixed-effects are in fact linear because in the context of the Poisson model we estimate:
\(E\left(z_i\right) = \exp\left(\gamma_{id_i}+\log\left(a\times x_i + b\times y_i\right)\right)\).
Further, remark that there exists an infinity of values of \(\gamma^{\prime}\), \(a^{\prime}\) and \(b^{\prime}\) such that:
\(\gamma_{k} \left( a\times x_i + b\times y_i \right) = \gamma_{k}^{\prime} \left(a^{\prime}\times x_i + b^{\prime}\times y_i \right),\forall i,k\).
An example is \(\gamma^{\prime}_{k} = 2\times \gamma_k\), \(a^{\prime} = a/2\) and \(b^{\prime} = b/2\). Thus estimating this relation directly will lead to a problem to uniquely identify the coefficients. To circumvent this problem, we just have to fix one of the coefficient, this will ensure that we uniquely identify them.
Let’s generate this relation:
# the class of each observation
id = sample(20, n, replace = TRUE)
base$id = id
# the vector of fixed-effects
gamma = rnorm(20)**2
# the new vector z_bis
z_bis = rpois(n, gamma[id] * (2*x + 3*y)) + rpois(n, 1)
base$z_bis = z_bis
Now we estimate it with the fixed-effects while fixing one of the coefficients (we fix \(a\) to its true value but it could be any value):
# we add the fixed-effect in the formula
result_NL_fe = feNmlm(z_bis~0|id, base, NL.fml = ~ log(2*x + b*y), NL.start = list(b=1), lower = list(b=0))
# The coef should be around 3
coef(result_NL_fe)
#> b
#> 3.024891
# the gamma and the exponential of the fixed-effects should be similar
rbind(gamma, exp(fixef(result_NL_fe)$id[as.character(1:20)]))
#> 1 2 3 4 5 6 7
#> gamma 2.679535 0.1707382 0.7294981 0.6375940 0.002920490 2.202472 0.08203791
#> 2.670332 0.1831774 0.7519754 0.6240016 0.008805172 2.220800 0.08548657
#> 8 9 10 11 12 13 14
#> gamma 1.501218 1.262652 1.515043 1.681641 0.1949462 1.095457 1.0023382
#> 1.454965 1.276599 1.493300 1.705419 0.1975139 1.104186 0.9971681
#> 15 16 17 18 19 20
#> gamma 0.3743722 2.606235 0.5238710 0.1428949 0.4871731 0.1550584
#> 0.3896577 2.609243 0.5372464 0.1433603 0.4910665 0.1629123
As we can see, we obtain the “right” estimates.
The package fixest
integrates multi-platform parallelism
to hasten the estimation process. By default it makes use of 50% of all
available threads. To change the number of threads used, just use the
argument nthreads
:
# Sample of results:
# 1 nthreads: 3.13s
system.time(fenegbin(Euros ~ log(dist_km)|Origin+Destination+Product+Year, trade, nthreads = 1))
# 2 nthreads: 1.82s
system.time(fenegbin(Euros ~ log(dist_km)|Origin+Destination+Product+Year, trade, nthreads = 2))
# 4 nthreads: 1.17s
system.time(fenegbin(Euros ~ log(dist_km)|Origin+Destination+Product+Year, trade, nthreads = 4))
As you can see, the efficiency of increasing the number of threads is not 1 to 1. Two threads do not divide the computing time by 2, nor four threads by 4. However it still reduces significantly the computing time, which might be valuable for large sample estimations.
You can permanently set the number of threads used by
fixest
using setFixest_nthreads(nthreads)
.
Note that you can permanently set this number at the project level by
using the argument save:
setFixest_nthreads(nthreads, save = TRUE)
. This way you
won’t need to re-set the number of threads whenever you restart
R.
Since the \(\gamma\) are parameters, I omit to put them in logarithmic form.↩︎