This is an introduction to R (“GNU S”), a language and environment for statistical computing and graphics. R is similar to the award-winning 1 S system, which was developed at Bell Laboratories by John Chambers et al. It provides a wide variety of statistical and graphical techniques (linear and nonlinear modelling, statistical tests, time series analysis, classification, clustering, . ).
This manual provides information on data types, programming elements, statistical modelling and graphics.
This manual is for R, version 4.4.1 (2024-06-14).
Copyright © 1990 W. N. Venables
Copyright © 1992 W. N. Venables & D. M. Smith
Copyright © 1997 R. Gentleman & R. Ihaka
Copyright © 1997, 1998 M. Maechler
Copyright © 1999–2024 R Core Team
Permission is granted to make and distribute verbatim copies of this manual provided the copyright notice and this permission notice are preserved on all copies.
Permission is granted to copy and distribute modified versions of this manual under the conditions for verbatim copying, provided that the entire resulting derived work is distributed under the terms of a permission notice identical to this one.
Permission is granted to copy and distribute translations of this manual into another language, under the above conditions for modified versions, except that this permission notice may be stated in a translation approved by the R Core Team.
This introduction to R is derived from an original set of notes describing the S and S-PLUS environments written in 1990–2 by Bill Venables and David M. Smith when at the University of Adelaide. We have made a number of small changes to reflect differences between the R and S programs, and expanded some of the material.
We would like to extend warm thanks to Bill Venables (and David Smith) for granting permission to distribute this modified version of the notes in this way, and for being a supporter of R from way back.
Comments and corrections are always welcome. Please address email correspondence to R-help@R-project.org.
Most R novices will start with the introductory session in Appendix A. This should give some familiarity with the style of R sessions and more importantly some instant feedback on what actually happens.
Many users will come to R mainly for its graphical facilities. See Graphical procedures, which can be read at almost any time and need not wait until all the preceding sections have been digested.
R is an integrated suite of software facilities for data manipulation, calculation and graphical display. Among other things it has
The term “environment” is intended to characterize it as a fully planned and coherent system, rather than an incremental accretion of very specific and inflexible tools, as is frequently the case with other data analysis software.
R is very much a vehicle for newly developing methods of interactive data analysis. It has developed rapidly, and has been extended by a large collection of packages. However, most programs written in R are essentially ephemeral, written for a single piece of data analysis.
R can be regarded as an implementation of the S language which was developed at Bell Laboratories by Rick Becker, John Chambers and Allan Wilks, and also forms the basis of the S-PLUS systems.
The evolution of the S language is characterized by four books by John Chambers and coauthors. For R, the basic reference is The New S Language: A Programming Environment for Data Analysis and Graphics by Richard A. Becker, John M. Chambers and Allan R. Wilks. The new features of the 1991 release of S are covered in Statistical Models in S edited by John M. Chambers and Trevor J. Hastie. The formal methods and classes of the methods package are based on those described in Programming with Data by John M. Chambers. See References, for precise references.
There are now a number of books which describe how to use R for data analysis and statistics, and documentation for S/S-PLUS can typically be used with R, keeping the differences between the S implementations in mind. See What documentation exists for R? in R FAQ .
Our introduction to the R environment did not mention statistics, yet many people use R as a statistics system. We prefer to think of it of an environment within which many classical and modern statistical techniques have been implemented. A few of these are built into the base R environment, but many are supplied as packages. There are about 25 packages supplied with R (called “standard” and “recommended” packages) and many more are available through the CRAN family of Internet sites (via https://CRAN.R-project.org) and elsewhere. More details on packages are given later (see Packages).
Most classical statistics and much of the latest methodology is available for use with R, but users may need to be prepared to do a little work to find it.
There is an important difference in philosophy between S (and hence R) and the other main statistical systems. In S a statistical analysis is normally done as a series of steps, with intermediate results being stored in objects. Thus whereas SAS and SPSS will give copious output from a regression or discriminant analysis, R will give minimal output and store the results in a fit object for subsequent interrogation by further R functions.
The most convenient way to use R is at a graphics workstation running a windowing system. This guide is aimed at users who have this facility. In particular we will occasionally refer to the use of R on an X window system although the vast bulk of what is said applies generally to any implementation of the R environment.
Most users will find it necessary to interact directly with the operating system on their computer from time to time. In this guide, we mainly discuss interaction with the operating system on UNIX machines. If you are running R under Windows or macOS you will need to make some small adjustments.
Setting up a workstation to take full advantage of the customizable features of R is a straightforward if somewhat tedious procedure, and will not be considered further here. Users in difficulty should seek local expert help.
When you use the R program it issues a prompt when it expects input commands. The default prompt is ‘ > ’, which on UNIX might be the same as the shell prompt, and so it may appear that nothing is happening. However, as we shall see, it is easy to change to a different R prompt if you wish. We will assume that the UNIX shell prompt is ‘ $ ’.
In using R under UNIX the suggested procedure for the first occasion is as follows:
$ mkdir work $ cd work
Further R sessions are simple.
$ cd work $ R
To use R under Windows the procedure to follow is basically the same. Create a folder as the working directory, and set that in the Start In field in your R shortcut. Then launch R by double clicking on the icon.
Readers wishing to get a feel for R at a computer before proceeding are strongly advised to work through the introductory session given in A sample session.
R has an inbuilt help facility similar to the man facility of UNIX. To get more information on any specific named function, for example solve , the command is
> help(solve)
An alternative is
> ?solve
For a feature specified by special characters, the argument must be enclosed in double or single quotes, making it a “character string”: This is also necessary for a few words with syntactic meaning including if , for and function .
> help("[[")
Either form of quote mark may be used to escape the other, as in the string "It's important" . Our convention is to use double quote marks for preference.
On most R installations help is available in HTML format by running
> help.start()
which will launch a Web browser that allows the help pages to be browsed with hyperlinks. On UNIX, subsequent help requests are sent to the HTML -based help system. The ‘Search Engine and Keywords’ link in the page loaded by help.start() is particularly useful as it is contains a high-level concept list which searches though available functions. It can be a great way to get your bearings quickly and to understand the breadth of what R has to offer.
The help.search command (alternatively ?? ) allows searching for help in various ways. For example,
> ??solve
Try ?help.search for details and more examples.
The examples on a help topic can normally be run by
> example(topic)
Windows versions of R have other optional help systems: use
> ?help
for further details.
Technically R is an expression language with a very simple syntax. It is case sensitive as are most UNIX based packages, so A and a are different symbols and would refer to different variables. The set of symbols which can be used in R names depends on the operating system and country within which R is being run (technically on the locale in use). Normally all alphanumeric symbols are allowed 2 (and in some countries this includes accented letters) plus ‘ . ’ and ‘ _ ’, with the restriction that a name must start with ‘ . ’ or a letter, and if it starts with ‘ . ’ the second character must not be a digit. Names are effectively unlimited in length.
Elementary commands consist of either expressions or assignments. If an expression is given as a command, it is evaluated, printed (unless specifically made invisible), and the value is lost. An assignment also evaluates an expression and passes the value to a variable but the result is not automatically printed.
Commands are separated either by a semi-colon (‘ ; ’), or by a newline. Elementary commands can be grouped together into one compound expression by braces (‘ < ’ and ‘ >’). Comments can be put almost 3 anywhere, starting with a hash mark (‘ # ’), everything to the end of the line is a comment.
If a command is not complete at the end of a line, R will give a different prompt, by default
on second and subsequent lines and continue to read input until the command is syntactically complete. This prompt may be changed by the user. We will generally omit the continuation prompt and indicate continuation by simple indenting.
Command lines entered at the console are limited 4 to about 4095 bytes (not characters).
Under many versions of UNIX and on Windows, R provides a mechanism for recalling and re-executing previous commands. The vertical arrow keys on the keyboard can be used to scroll forward and backward through a command history. Once a command is located in this way, the cursor can be moved within the command using the horizontal arrow keys, and characters can be removed with the DEL key or added with the other keys. More details are provided later: see The command-line editor.
The recall and editing capabilities under UNIX are highly customizable. You can find out how to do this by reading the manual entry for the readline library.
Alternatively, the Emacs text editor provides more general support mechanisms (via ESS , Emacs Speaks Statistics) for working interactively with R. See R and Emacs in R FAQ .
If commands 5 are stored in an external file, say commands.R in the working directory work , they may be executed at any time in an R session with the command
> source("commands.R")
For Windows Source is also available on the File menu. The function sink ,
> sink("record.lis")
will divert all subsequent output from the console to an external file, record.lis . The command
> sink()
restores it to the console once again.
The entities that R creates and manipulates are known as objects. These may be variables, arrays of numbers, character strings, functions, or more general structures built from such components.
During an R session, objects are created and stored by name (we discuss this process in the next section). The R command
> objects()
(alternatively, ls() ) can be used to display the names of (most of) the objects which are currently stored within R. The collection of objects currently stored is called the workspace.
To remove objects the function rm is available:
> rm(x, y, z, ink, junk, temp, foo, bar)
All objects created during an R session can be stored permanently in a file for use in future R sessions. At the end of each R session you are given the opportunity to save all the currently available objects. If you indicate that you want to do this, the objects are written to a file called .RData 6 in the current directory, and the command lines used in the session are saved to a file called .Rhistory .
When R is started at later time from the same directory it reloads the workspace from this file. At the same time the associated commands history is reloaded.
It is recommended that you should use separate working directories for analyses conducted with R. It is quite common for objects with names x and y to be created during an analysis. Names like this are often meaningful in the context of a single analysis, but it can be quite hard to decide what they might be when the several analyses have been conducted in the same directory.
R operates on named data structures. The simplest such structure is the numeric vector, which is a single entity consisting of an ordered collection of numbers. To set up a vector named x , say, consisting of five numbers, namely 10.4, 5.6, 3.1, 6.4 and 21.7, use the R command
This is an assignment statement using the function c() which in this context can take an arbitrary number of vector arguments and whose value is a vector got by concatenating its arguments end to end. 7
A number occurring by itself in an expression is taken as a vector of length one.
Notice that the assignment operator (‘
Assignment can also be made using the function assign() . An equivalent way of making the same assignment as above is with:
> assign("x", c(10.4, 5.6, 3.1, 6.4, 21.7))
Assignments can also be made in the other direction, using the obvious change in the assignment operator. So the same assignment could be made using
> c(10.4, 5.6, 3.1, 6.4, 21.7) -> x
If an expression is used as a complete command, the value is printed and lost 8 . So now if we were to use the command
the reciprocals of the five values would be printed at the terminal (and the value of x , of course, unchanged).
The further assignment
would create a vector y with 11 entries consisting of two copies of x with a zero in the middle place.
Vectors can be used in arithmetic expressions, in which case the operations are performed element by element. Vectors occurring in the same expression need not all be of the same length. If they are not, the value of the expression is a vector with the same length as the longest vector which occurs in the expression. Shorter vectors in the expression are recycled as often as need be (perhaps fractionally) until they match the length of the longest vector. In particular a constant is simply repeated. So with the above assignments the command
generates a new vector v of length 11 constructed by adding together, element by element, 2*x repeated 2.2 times, y repeated just once, and 1 repeated 11 times.
The elementary arithmetic operators are the usual + , - , * , / and ^ for raising to a power. In addition all of the common arithmetic functions are available. log , exp , sin , cos , tan , sqrt , and so on, all have their usual meaning. max and min select the largest and smallest elements of a vector respectively. range is a function whose value is a vector of length two, namely c(min(x), max(x)) . length(x) is the number of elements in x , sum(x) gives the total of the elements in x , and prod(x) their product.
Two statistical functions are mean(x) which calculates the sample mean, which is the same as sum(x)/length(x) , and var(x) which gives
sum((x-mean(x))^2)/(length(x)-1)
or sample variance. If the argument to var() is an n-by-p matrix the value is a p-by-p sample covariance matrix got by regarding the rows as independent p-variate sample vectors.
sort(x) returns a vector of the same size as x with the elements arranged in increasing order; however there are other more flexible sorting facilities available (see order() or sort.list() which produce a permutation to do the sorting).
Note that max and min select the largest and smallest values in their arguments, even if they are given several vectors. The parallel maximum and minimum functions pmax and pmin return a vector (of length equal to their longest argument) that contains in each element the largest (smallest) element in that position in any of the input vectors.
For most purposes the user will not be concerned if the “numbers” in a numeric vector are integers, reals or even complex. Internally calculations are done as double precision real numbers, or double precision complex numbers if the input data are complex.
To work with complex numbers, supply an explicit complex part. Thus
sqrt(-17)
will give NaN and a warning, but
sqrt(-17+0i)
will do the computations as complex numbers.
R has a number of facilities for generating commonly used sequences of numbers. For example 1:30 is the vector c(1, 2, …, 29, 30) . The colon operator has high priority within an expression, so, for example 2*1:15 is the vector c(2, 4, …, 28, 30) . Put n
The construction 30:1 may be used to generate a sequence backwards.
The function seq() is a more general facility for generating sequences. It has five arguments, only some of which may be specified in any one call. The first two arguments, if given, specify the beginning and end of the sequence, and if these are the only two arguments given the result is the same as the colon operator. That is seq(2,10) is the same vector as 2:10 .
Arguments to seq() , and to many other R functions, can also be given in named form, in which case the order in which they appear is irrelevant. The first two arguments may be named from= value and to= value ; thus seq(1,30) , seq(from=1, to=30) and seq(to=30, from=1) are all the same as 1:30 . The next two arguments to seq() may be named by= value and length= value , which specify a step size and a length for the sequence respectively. If neither of these is given, the default by=1 is assumed.
> seq(-5, 5, by=.2) -> s3
generates in s3 the vector c(-5.0, -4.8, -4.6, …, 4.6, 4.8, 5.0) . Similarly
generates the same vector in s4 .
The fifth argument may be named along= vector , which is normally used as the only argument to create the sequence 1, 2, …, length( vector ) , or the empty sequence if the vector is empty (as it can be).
A related function is rep() which can be used for replicating an object in various complicated ways. The simplest form is
which will put five copies of x end-to-end in s5 . Another useful version is
which repeats each element of x five times before moving on to the next.
As well as numerical vectors, R allows manipulation of logical quantities. The elements of a logical vector can have the values TRUE , FALSE , and NA (for “not available”, see below). The first two are often abbreviated as T and F , respectively. Note however that T and F are just variables which are set to TRUE and FALSE by default, but are not reserved words and hence can be overwritten by the user. Hence, you should always use TRUE and FALSE .
Logical vectors are generated by conditions. For example
> temp 13
sets temp as a vector of the same length as x with values FALSE corresponding to elements of x where the condition is not met and TRUE where it is.
The logical operators are < , , >= , == for exact equality and != for inequality. In addition if c1 and c2 are logical expressions, then c1 & c2 is their intersection (“and”), c1 | c2 is their union (“or”), and !c1 is the negation of c1 .
Logical vectors may be used in ordinary arithmetic, in which case they are coerced into numeric vectors, FALSE becoming 0 and TRUE becoming 1 . However there are situations where logical vectors and their coerced numeric counterparts are not equivalent, for example see the next subsection.
In some cases the components of a vector may not be completely known. When an element or value is “not available” or a “missing value” in the statistical sense, a place within a vector may be reserved for it by assigning it the special value NA . In general any operation on an NA becomes an NA . The motivation for this rule is simply that if the specification of an operation is incomplete, the result cannot be known and hence is not available.
The function is.na(x) gives a logical vector of the same size as x with value TRUE if and only if the corresponding element in x is NA .
Notice that the logical expression x == NA is quite different from is.na(x) since NA is not really a value but a marker for a quantity that is not available. Thus x == NA is a vector of the same length as x all of whose values are NA as the logical expression itself is incomplete and hence undecidable.
Note that there is a second kind of “missing” values which are produced by numerical computation, the so-called Not a Number, NaN , values. Examples are
> Inf - Inf
which both give NaN since the result cannot be defined sensibly.
In summary, is.na(xx) is TRUE both for NA and NaN values. To differentiate these, is.nan(xx) is only TRUE for NaN s.
Missing values are sometimes printed as when character vectors are printed without quotes.
Character quantities and character vectors are used frequently in R, for example as plot labels. Where needed they are denoted by a sequence of characters delimited by the double quote character, e.g., "x-values" , "New iteration results" .
Character strings are entered using either matching double ( " ) or single ( ' ) quotes, but are printed using double quotes (or sometimes without quotes). They use C-style escape sequences, using \ as the escape character, so \ is entered and printed as \\ , and inside double quotes " is entered as \" . Other useful escape sequences are \n , newline, \t , tab and \b , backspace—see ?Quotes for a full list.
Character vectors may be concatenated into a vector by the c() function; examples of their use will emerge frequently.
The paste() function takes an arbitrary number of arguments and concatenates them one by one into character strings. Any numbers given among the arguments are coerced into character strings in the evident way, that is, in the same way they would be if they were printed. The arguments are by default separated in the result by a single blank character, but this can be changed by the named argument, sep= string , which changes it to string , possibly empty.
> labsmakes labs into the character vector
c("X1", "Y2", "X3", "Y4", "X5", "Y6", "X7", "Y8", "X9", "Y10")Note particularly that recycling of short lists takes place here too; thus c("X", "Y") is repeated 5 times to match the sequence 1:10 . 9
2.7 Index vectors; selecting and modifying subsets of a data set ¶
Subsets of the elements of a vector may be selected by appending to the name of the vector an index vector in square brackets. More generally any expression that evaluates to a vector may have subsets of its elements similarly selected by appending an index vector in square brackets immediately after the expression.
Such index vectors can be any of four distinct types.
A logical vector. In this case the index vector is recycled to the same length as the vector from which elements are to be selected. Values corresponding to TRUE in the index vector are selected and those corresponding to FALSE are omitted. For example
creates (or re-creates) an object y which will contain the non-missing values of x , in the same order. Note that if x has missing values, y will be shorter than x . Also
> (x+1)[(!is.na(x)) & x>0] -> z> x[1:10]selects the first 10 elements of x (assuming length(x) is not less than 10). Also> c("x","y")[rep(c(1,2,2,1), times=4)]> fruit names(fruit) lunchAn indexed expression can also appear on the receiving end of an assignment, in which case the assignment operation is performed only on those elements of the vector. The expression must be of the form vector[ index_vector ] as having an arbitrary expression in place of the vector name does not make much sense here.
> x[is.na(x)]replaces any missing values in x by zeros and
has the same effect as
2.8 Other types of objects ¶
Vectors are the most important type of object in R, but there are several others which we will meet more formally in later sections.
The entities R operates on are technically known as objects. Examples are vectors of numeric (real) or complex values, vectors of logical values and vectors of character strings. These are known as “atomic” structures since their components are all of the same type, or mode, namely numeric 10 , complex, logical, character and raw.
Vectors must have their values all of the same mode. Thus any given vector must be unambiguously either logical, numeric, complex, character or raw. (The only apparent exception to this rule is the special “value” listed as NA for quantities not available, but in fact there are several types of NA ). Note that a vector can be empty and still have a mode. For example the empty character string vector is listed as character(0) and the empty numeric vector as numeric(0) .
R also operates on objects called lists, which are of mode list. These are ordered sequences of objects which individually can be of any mode. lists are known as “recursive” rather than atomic structures since their components can themselves be lists in their own right.
The other recursive structures are those of mode function and expression. Functions are the objects that form part of the R system along with similar user written functions, which we discuss in some detail later. Expressions as objects form an advanced part of R which will not be discussed in this guide, except indirectly when we discuss formulae used with modeling in R.
By the mode of an object we mean the basic type of its fundamental constituents. This is a special case of a “property” of an object. Another property of every object is its length. The functions mode( object ) and length( object ) can be used to find out the mode and length of any defined structure 11 .
Further properties of an object are usually provided by attributes( object ) , see Getting and setting attributes. Because of this, mode and length are also called “intrinsic attributes” of an object.
For example, if z is a complex vector of length 100, then in an expression mode(z) is the character string "complex" and length(z) is 100 .
R caters for changes of mode almost anywhere it could be considered sensible to do so, (and a few where it might not be). For example with
> digitsafter which digits is the character vector c("0", "1", "2", …, "9") . A further coercion, or change of mode, reconstructs the numerical vector again:
Now d and z are the same. 12 There is a large collection of functions of the form as. something () for either coercion from one mode to another, or for investing an object with some other attribute it may not already possess. The reader should consult the different help files to become familiar with them.
3.2 Changing the length of an object ¶
An “empty” object may still have a mode. For example
makes e an empty vector structure of mode numeric. Similarly character() is a empty character vector, and so on. Once an object of any size has been created, new components may be added to it simply by giving it an index value outside its previous range. Thus
now makes e a vector of length 3, (the first two components of which are at this point both NA ). This applies to any structure at all, provided the mode of the additional component(s) agrees with the mode of the object in the first place.
This automatic adjustment of lengths of an object is used often, for example in the scan() function for input. (see The scan() function.)
Conversely to truncate the size of an object requires only an assignment to do so. Hence if alpha is an object of length 10, then
> alphamakes it an object of length 5 consisting of just the former components with even index. (The old indices are not retained, of course.) We can then retain just the first three values by
> length(alpha)and vectors can be extended (by missing values) in the same way.
3.3 Getting and setting attributes ¶
The function attributes( object ) returns a list of all the non-intrinsic attributes currently defined for that object. The function attr( object , name ) can be used to select a specific attribute. These functions are rarely used, except in rather special circumstances when some new attribute is being created for some particular purpose, for example to associate a creation date or an operator with an R object. The concept, however, is very important.
Some care should be exercised when assigning or deleting attributes since they are an integral part of the object system used in R.
When it is used on the left hand side of an assignment it can be used either to associate a new attribute with object or to change an existing one. For example
> attr(z, "dim")allows R to treat z as if it were a 10-by-10 matrix.
3.4 The class of an object ¶
All objects in R have a class, reported by the function class . For simple vectors this is just the mode, for example "numeric" , "logical" , "character" or "list" , but "matrix" , "array" , "factor" and "data.frame" are other possible values.
A special attribute known as the class of the object is used to allow for an object-oriented style 13 of programming in R. For example if an object has class "data.frame" , it will be printed in a certain way, the plot() function will display it graphically in a certain way, and other so-called generic functions such as summary() will react to it as an argument in a way sensitive to its class.
To remove temporarily the effects of class, use the function unclass() . For example if winter has the class "data.frame" then
> winterwill print it in data frame form, which is rather like a matrix, whereas
> unclass(winter)will print it as an ordinary list. Only in rather special situations do you need to use this facility, but one is when you are learning to come to terms with the idea of class and generic functions.
Generic functions and classes will be discussed further in Classes, generic functions and object orientation, but only briefly.
4 Ordered and unordered factors ¶
A factor is a vector object used to specify a discrete classification (grouping) of the components of other vectors of the same length. R provides both ordered and unordered factors. While the “real” application of factors is with model formulae (see Contrasts), we here look at a specific example.
Suppose, for example, we have a sample of 30 tax accountants from all the states and territories of Australia 14 and their individual state of origin is specified by a character vector of state mnemonics as
> stateNotice that in the case of a character vector, “sorted” means sorted in alphabetical order.
A factor is similarly created using the factor() function:
> statefThe print() function handles factors slightly differently from other objects:
> statef [1] tas sa qld nsw nsw nt wa wa qld vic nsw vic qld qld sa [16] tas sa nt wa vic qld nsw nsw wa sa act nsw vic vic act Levels: act nsw nt qld sa tas vic waTo find out the levels of a factor the function levels() can be used.
> levels(statef) [1] "act" "nsw" "nt" "qld" "sa" "tas" "vic" "wa"4.2 The function tapply() and ragged arrays ¶
To continue the previous example, suppose we have the incomes of the same tax accountants in another vector (in suitably large units of money)
> incomesTo calculate the sample mean income for each state we can now use the special function tapply() :
> incmeansgiving a means vector with the components labelled by the levels
act nsw nt qld sa tas vic wa 44.500 57.333 55.500 53.600 55.000 60.500 56.000 52.250The function tapply() is used to apply a function, here mean() , to each group of components of the first argument, here incomes , defined by the levels of the second component, here statef 15 , as if they were separate vector structures. The result is a structure of the same length as the levels attribute of the factor containing the results. The reader should consult the help document for more details.
Suppose further we needed to calculate the standard errors of the state income means. To do this we need to write an R function to calculate the standard error for any given vector. Since there is an builtin function var() to calculate the sample variance, such a function is a very simple one liner, specified by the assignment:
> stdError(Writing functions will be considered later in Writing your own functions. Note that R’s a builtin function sd() is something different.) After this assignment, the standard errors are calculated by
> incsterand the values calculated are then
> incster act nsw nt qld sa tas vic wa 1.5 4.3102 4.5 4.1061 2.7386 0.5 5.244 2.6575As an exercise you may care to find the usual 95% confidence limits for the state mean incomes. To do this you could use tapply() once more with the length() function to find the sample sizes, and the qt() function to find the percentage points of the appropriate t-distributions. (You could also investigate R’s facilities for t-tests.)
The function tapply() can also be used to handle more complicated indexing of a vector by multiple categories. For example, we might wish to split the tax accountants by both state and sex. However in this simple instance (just one factor) what happens can be thought of as follows. The values in the vector are collected into groups corresponding to the distinct entries in the factor. The function is then applied to each of these groups individually. The value is a vector of function results, labelled by the levels attribute of the factor.
The combination of a vector and a labelling factor is an example of what is sometimes called a ragged array, since the subclass sizes are possibly irregular. When the subclass sizes are all the same the indexing may be done implicitly and much more efficiently, as we see in the next section.
4.3 Ordered factors ¶
The levels of factors are stored in alphabetical order, or in the order they were specified to factor if they were specified explicitly.
Sometimes the levels will have a natural ordering that we want to record and want our statistical analysis to make use of. The ordered() function creates such ordered factors but is otherwise identical to factor . For most purposes the only difference between ordered and unordered factors is that the former are printed showing the ordering of the levels, but the contrasts generated for them in fitting linear models are different.
5 Arrays and matrices ¶
An array can be considered as a multiply subscripted collection of data entries, for example numeric. R allows simple facilities for creating and handling arrays, and in particular the special case of matrices.
A dimension vector is a vector of non-negative integers. If its length is k then the array is k-dimensional, e.g. a matrix is a 2-dimensional array. The dimensions are indexed from one up to the values given in the dimension vector.
A vector can be used by R as an array only if it has a dimension vector as its dim attribute. Suppose, for example, z is a vector of 1500 elements. The assignment
> dim(z)gives it the dim attribute that allows it to be treated as a 3 by 5 by 100 array.
Other functions such as matrix() and array() are available for simpler and more natural looking assignments, as we shall see in The array() function.
The values in the data vector give the values in the array in the same order as they would occur in FORTRAN, that is “column major order,” with the first subscript moving fastest and the last subscript slowest.
For example if the dimension vector for an array, say a , is c(3,4,2) then there are 3 * 4 * 2 = 24 entries in a and the data vector holds them in the order a[1,1,1], a[2,1,1], …, a[2,4,2], a[3,4,2] .
Arrays can be one-dimensional: such arrays are usually treated in the same way as vectors (including when printing), but the exceptions can cause confusion.
5.2 Array indexing. Subsections of an array ¶
Individual elements of an array may be referenced by giving the name of the array followed by the subscripts in square brackets, separated by commas.
More generally, subsections of an array may be specified by giving a sequence of index vectors in place of subscripts; however if any index position is given an empty index vector, then the full range of that subscript is taken.
Continuing the previous example, a[2,,] is a 4 * 2 array with dimension vector c(4,2) and data vector containing the values
c(a[2,1,1], a[2,2,1], a[2,3,1], a[2,4,1], a[2,1,2], a[2,2,2], a[2,3,2], a[2,4,2])in that order. a[,,] stands for the entire array, which is the same as omitting the subscripts entirely and using a alone.
For any array, say Z , the dimension vector may be referenced explicitly as dim(Z) (on either side of an assignment).
Also, if an array name is given with just one subscript or index vector, then the corresponding values of the data vector only are used; in this case the dimension vector is ignored. This is not the case, however, if the single index is not a vector but itself an array, as we next discuss.
5.3 Index matrices ¶
As well as an index vector in any subscript position, a matrix may be used with a single index matrix in order either to assign a vector of quantities to an irregular collection of elements in the array, or to extract an irregular collection as a vector.
A matrix example makes the process clear. In the case of a doubly indexed array, an index matrix may be given consisting of two columns and as many rows as desired. The entries in the index matrix are the row and column indices for the doubly indexed array. Suppose for example we have a 4 by 5 array X and we wish to do the following:
In this case we need a 3 by 2 subscript array, as in the following example.
> x Generate a 4 by 5 array. > x [,1] [,2] [,3] [,4] [,5] [1,] 1 5 9 13 17 [2,] 2 6 10 14 18 [3,] 3 7 11 15 19 [4,] 4 8 12 16 20 > i i # i
is a 3 by 2 index array. [,1] [,2] [1,] 1 3 [2,] 2 2 [3,] 3 1 > x[i] # Extract those elements [1] 9 6 3 > x[i] Replace those elements by zeros. > x [,1] [,2] [,3] [,4] [,5] [1,] 1 5 0 13 17 [2,] 2 0 10 14 18 [3,] 0 7 11 15 19 [4,] 4 8 12 16 20 >
Negative indices are not allowed in index matrices. NA and zero values are allowed: rows in the index matrix containing a zero are ignored, and rows containing an NA produce an NA in the result.
As a less trivial example, suppose we wish to generate an (unreduced) design matrix for a block design defined by factors blocks ( b levels) and varieties ( v levels). Further suppose there are n plots in the experiment. We could proceed as follows:
> Xb Xv ib iv Xb[ib] Xv[iv] XTo construct the incidence matrix, N say, we could use
However a simpler direct way of producing this matrix is to use table() :
Index matrices must be numerical: any other form of matrix (e.g. a logical or character matrix) supplied as a matrix is treated as an indexing vector.
5.4 The array() function ¶
As well as giving a vector structure a dim attribute, arrays can be constructed from vectors by the array function, which has the form
> Z data_vector, dim_vector)For example, if the vector h contains 24 or fewer, numbers then the command
would use h to set up 3 by 4 by 2 array in Z . If the size of h is exactly 24 the result is the same as
However if h is shorter than 24, its values are recycled from the beginning again to make it up to size 24 (see Mixed vector and array arithmetic. The recycling rule) but dim(h)
makes Z an array of all zeros.
At this point dim(Z) stands for the dimension vector c(3,4,2) , and Z[1:24] stands for the data vector as it was in h , and Z[] with an empty subscript or Z with no subscript stands for the entire array as an array.
Arrays may be used in arithmetic expressions and the result is an array formed by element-by-element operations on the data vector. The dim attributes of operands generally need to be the same, and this becomes the dimension vector of the result. So if A , B and C are all similar arrays, then
makes D a similar array with its data vector being the result of the given element-by-element operations. However the precise rule concerning mixed array and vector calculations has to be considered a little more carefully.
5.4.1 Mixed vector and array arithmetic. The recycling rule ¶
The precise rule affecting element by element mixed calculations with vectors and arrays is somewhat quirky and hard to find in the references. From experience we have found the following to be a reliable guide.
An important operation on arrays is the outer product. If a and b are two numeric arrays, their outer product is an array whose dimension vector is obtained by concatenating their two dimension vectors (order is important), and whose data vector is got by forming all possible products of elements of the data vector of a with those of b . The outer product is formed by the special operator %o% :
An alternative is
The multiplication function can be replaced by an arbitrary function of two variables. For example if we wished to evaluate the function f(x; y) = cos(y)/(1 + x^2) over a regular grid of values with x- and y-coordinates defined by the R vectors x and y respectively, we could proceed as follows:
In particular the outer product of two ordinary vectors is a doubly subscripted array (that is a matrix, of rank at most 1). Notice that the outer product operator is of course non-commutative. Defining your own R functions will be considered further in Writing your own functions.
As an artificial but cute example, consider the determinants of 2 by 2 matrices [a, b; c, d] where each entry is a non-negative integer in the range 0, 1, . 9, that is a digit.
The problem is to find the determinants, ad - bc, of all possible matrices of this form and represent the frequency with which each value occurs as a high density plot. This amounts to finding the probability distribution of the determinant if each digit is chosen independently and uniformly at random.
A neat way of doing this uses the outer() function twice:
> d fr plot(fr, xlab="Determinant", ylab="Frequency")
Notice that plot() here uses a histogram like plot method, because it “sees” that fr is of class "table" . The “obvious” way of doing this problem with for loops, to be discussed in Grouping, loops and conditional execution, is so inefficient as to be impractical.
It is also perhaps surprising that about 1 in 20 such matrices is singular.
The function aperm(a, perm) may be used to permute an array, a . The argument perm must be a permutation of the integers , where k is the number of subscripts in a . The result of the function is an array of the same size as a but with old dimension given by perm[j] becoming the new j -th dimension. The easiest way to think of this operation is as a generalization of transposition for matrices. Indeed if A is a matrix, (that is, a doubly subscripted array) then B given by
is just the transpose of A . For this special case a simpler function t() is available, so we could have used B
As noted above, a matrix is just an array with two subscripts. However it is such an important special case it needs a separate discussion. R contains many operators and functions that are available only for matrices. For example t(X) is the matrix transpose function, as noted above. The functions nrow(A) and ncol(A) give the number of rows and columns in the matrix A respectively.
The operator %*% is used for matrix multiplication. An n by 1 or 1 by n matrix may of course be used as an n-vector if in the context such is appropriate. Conversely, vectors which occur in matrix multiplication expressions are automatically promoted either to row or column vectors, whichever is multiplicatively coherent, if possible, (although this is not always unambiguously possible, as we see later).
If, for example, A and B are square matrices of the same size, then
> A * B
is the matrix of element by element products and
> A %*% B
is the matrix product. If x is a vector, then
> x %*% A %*% x
is a quadratic form. 16
The function crossprod() forms “cross products”, meaning that crossprod(X, y) is the same as t(X) %*% y but the operation is more efficient. If the second argument to crossprod() is omitted it is taken to be the same as the first.
The meaning of diag() depends on its argument. diag(v) , where v is a vector, gives a diagonal matrix with elements of the vector as the diagonal entries. On the other hand diag(M) , where M is a matrix, gives the vector of main diagonal entries of M . This is the same convention as that used for diag() in MATLAB. Also, somewhat confusingly, if k is a single numeric value then diag(k) is the k by k identity matrix!
Solving linear equations is the inverse of matrix multiplication. When after
only A and b are given, the vector x is the solution of that linear equation system. In R,
> solve(A,b)
solves the system, returning x (up to some accuracy loss). Note that in linear algebra, formally x = A^ %*% b where A^ denotes the inverse of A , which can be computed by
solve(A)
but rarely is needed. Numerically, it is both inefficient and potentially unstable to compute x
The quadratic form x %*% A^ %*% x which is used in multivariate computations, should be computed by something like 17 x %*% solve(A,x) , rather than computing the inverse of A .
The function eigen(Sm) calculates the eigenvalues and eigenvectors of a symmetric matrix Sm . The result of this function is a list of two components named values and vectors . The assignment
will assign this list to ev . Then ev$val is the vector of eigenvalues of Sm and ev$vec is the matrix of corresponding eigenvectors. Had we only needed the eigenvalues we could have used the assignment:
> evalsevals now holds the vector of eigenvalues and the second component is discarded. If the expression
> eigen(Sm)is used by itself as a command the two components are printed, with their names. For large matrices it is better to avoid computing the eigenvectors if they are not needed by using the expression
> evals5.7.4 Singular value decomposition and determinants ¶
The function svd(M) takes an arbitrary matrix argument, M , and calculates the singular value decomposition of M . This consists of a matrix of orthonormal columns U with the same column space as M , a second matrix of orthonormal columns V whose column space is the row space of M and a diagonal matrix of positive entries D such that M = U %*% D %*% t(V) . D is actually returned as a vector of the diagonal elements. The result of svd(M) is actually a list of three components named d , u and v , with evident meanings.
If M is in fact square, then, it is not hard to see that
> absdetMcalculates the absolute value of the determinant of M . If this calculation were needed often with a variety of matrices it could be defined as an R function
> absdetafter which we could use absdet() as just another R function. As a further trivial but potentially useful example, you might like to consider writing a function, say tr() , to calculate the trace of a square matrix. [Hint: You will not need to use an explicit loop. Look again at the diag() function.]
R has a builtin function det to calculate a determinant, including the sign, and another, determinant , to give the sign and modulus (optionally on log scale),
5.7.5 Least squares fitting and the QR decomposition ¶
The function lsfit() returns a list giving results of a least squares fitting procedure. An assignment such as
gives the results of a least squares fit where y is the vector of observations and X is the design matrix. See the help facility for more details, and also for the follow-up function ls.diag() for, among other things, regression diagnostics. Note that a grand mean term is automatically included and need not be included explicitly as a column of X . Further note that you almost always will prefer using lm(.) (see Linear models) to lsfit() for regression modelling.
Another closely related function is qr() and its allies. Consider the following assignments
> Xplus b fit resThese compute the orthogonal projection of y onto the range of X in fit , the projection onto the orthogonal complement in res and the coefficient vector for the projection in b , that is, b is essentially the result of the MATLAB ‘backslash’ operator.
It is not assumed that X has full column rank. Redundancies will be discovered and removed as they are found.
This alternative is the older, low-level way to perform least squares calculations. Although still useful in some contexts, it would now generally be replaced by the statistical models features, as will be discussed in Statistical models in R.
5.8 Forming partitioned matrices, cbind() and rbind() ¶
As we have already seen informally, matrices can be built up from other vectors and matrices by the functions cbind() and rbind() . Roughly cbind() forms matrices by binding together matrices horizontally, or column-wise, and rbind() vertically, or row-wise.
In the assignment
> X arg_1, arg_2, arg_3, . )the arguments to cbind() must be either vectors of any length, or matrices with the same column size, that is the same number of rows. The result is a matrix with the concatenated arguments arg_1 , arg_2 , … forming the columns.
If some of the arguments to cbind() are vectors they may be shorter than the column size of any matrices present, in which case they are cyclically extended to match the matrix column size (or the length of the longest vector if no matrices are given).
The function rbind() does the corresponding operation for rows. In this case any vector argument, possibly cyclically extended, are of course taken as row vectors.
Suppose X1 and X2 have the same number of rows. To combine these by columns into a matrix X , together with an initial column of 1 s we can use
The result of rbind() or cbind() always has matrix status. Hence cbind(x) and rbind(x) are possibly the simplest ways explicitly to allow the vector x to be treated as a column or row matrix respectively.
5.9 The concatenation function, c() , with arrays ¶
It should be noted that whereas cbind() and rbind() are concatenation functions that respect dim attributes, the basic c() function does not, but rather clears numeric objects of all dim and dimnames attributes. This is occasionally useful in its own right.
The official way to coerce an array back to a simple vector object is to use as.vector()
However a similar result can be achieved by using c() with just one argument, simply for this side-effect:
There are slight differences between the two, but ultimately the choice between them is largely a matter of style (with the former being preferable).
5.10 Frequency tables from factors ¶
Recall that a factor defines a partition into groups. Similarly a pair of factors defines a two way cross classification, and so on. The function table() allows frequency tables to be calculated from equal length factors. If there are k factor arguments, the result is a k-way array of frequencies.
Suppose, for example, that statef is a factor giving the state code for each entry in a data vector. The assignment
> statefrgives in statefr a table of frequencies of each state in the sample. The frequencies are ordered and labelled by the levels attribute of the factor. This simple case is equivalent to, but more convenient than,
> statefrFurther suppose that incomef is a factor giving a suitably defined “income class” for each entry in the data vector, for example with the cut() function:
> factor(cut(incomes, breaks = 35+10*(0:7))) -> incomefThen to calculate a two-way table of frequencies:
> table(incomef,statef) statef incomef act nsw nt qld sa tas vic wa (35,45] 1 1 0 1 0 0 1 0 (45,55] 1 1 1 1 2 0 1 3 (55,65] 0 3 1 3 2 2 2 1 (65,75] 0 1 0 0 0 0 1 0Extension to higher-way frequency tables is immediate.
6 Lists and data frames ¶
An R list is an object consisting of an ordered collection of objects known as its components.
There is no particular need for the components to be of the same mode or type, and, for example, a list could consist of a numeric vector, a logical value, a matrix, a complex vector, a character array, a function, and so on. Here is a simple example of how to make a list:
Components are always numbered and may always be referred to as such. Thus if Lst is the name of a list with four components, these may be individually referred to as Lst[[1]] , Lst[[2]] , Lst[[3]] and Lst[[4]] . If, further, Lst[[4]] is a vector subscripted array then Lst[[4]][1] is its first entry.
If Lst is a list, then the function length(Lst) gives the number of (top level) components it has.
Components of lists may also be named, and in this case the component may be referred to either by giving the component name as a character string in place of the number in double square brackets, or, more conveniently, by giving an expression of the form
> name$component_name
for the same thing.
This is a very useful convention as it makes it easier to get the right component if you forget the number.
So in the simple example given above:
Lst$name is the same as Lst[[1]] and is the string "Fred" ,
Lst$wife is the same as Lst[[2]] and is the string "Mary" ,
Lst$child.ages[1] is the same as Lst[[4]][1] and is the number 4 .
Additionally, one can also use the names of the list components in double square brackets, i.e., Lst[["name"]] is the same as Lst$name . This is especially useful, when the name of the component to be extracted is stored in another variable as in
It is very important to distinguish Lst[[1]] from Lst[1] . ‘ [[ … ]] ’ is the operator used to select a single element, whereas ‘ [ … ] ’ is a general subscripting operator. Thus the former is the first object in the list Lst , and if it is a named list the name is not included. The latter is a sublist of the list Lst consisting of the first entry only. If it is a named list, the names are transferred to the sublist.
The names of components may be abbreviated down to the minimum number of letters needed to identify them uniquely. Thus Lst$coefficients may be minimally specified as Lst$coe and Lst$covariance as Lst$cov .
The vector of names is in fact simply an attribute of the list like any other and may be handled as such. Other structures besides lists may, of course, similarly be given a names attribute also.
New lists may be formed from existing objects by the function list() . An assignment of the form
> Lst name_1=object_1, . , name_m=object_m)
sets up a list Lst of m components using object_1 , …, object_m for the components and giving them names as specified by the argument names, (which can be freely chosen). If these names are omitted, the components are numbered only. The components used to form the list are copied when forming the new list and the originals are not affected.
Lists, like any subscripted object, can be extended by specifying additional components. For example
> Lst[5]6.2.1 Concatenating lists ¶
When the concatenation function c() is given list arguments, the result is an object of mode list also, whose components are those of the argument lists joined together in sequence.
> list.ABCRecall that with vector objects as arguments the concatenation function similarly joined together all arguments into a single vector structure. In this case all other attributes, such as dim attributes, are discarded.
6.3 Data frames ¶
A data frame is a list with class "data.frame" . There are restrictions on lists that may be made into data frames, namely
A data frame may for many purposes be regarded as a matrix with columns possibly of differing modes and attributes. It may be displayed in matrix form, and its rows and columns extracted using matrix indexing conventions.
Objects satisfying the restrictions placed on the columns (components) of a data frame may be used to form one using the function data.frame :
> accountantsA list whose components conform to the restrictions of a data frame may be coerced into a data frame using the function as.data.frame()
The simplest way to construct a data frame from scratch is to use the read.table() function to read an entire data frame from an external file. This is discussed further in Reading data from files.
6.3.2 attach() and detach() ¶
The $ notation, such as accountants$home , for list components is not always very convenient. A useful facility would be somehow to make the components of a list or data frame temporarily visible as variables under their component name, without the need to quote the list name explicitly each time.
The attach() function takes a ‘database’ such as a list or data frame as its argument. Thus suppose lentils is a data frame with three variables lentils$u , lentils$v , lentils$w . The attach
> attach(lentils)places the data frame in the search path at position 2 , and provided there are no variables u , v or w in position 1 , u , v and w are available as variables from the data frame in their own right. At this point an assignment such as
does not replace the component u of the data frame, but rather masks it with another variable u in the workspace at position 1 on the search path. To make a permanent change to the data frame itself, the simplest way is to resort once again to the $ notation:
> lentils$uHowever the new value of component u is not visible until the data frame is detached and attached again.
To detach a data frame, use the function
> detach()More precisely, this statement detaches from the search path the entity currently at position 2 . Thus in the present context the variables u , v and w would be no longer visible, except under the list notation as lentils$u and so on. Entities at positions greater than 2 on the search path can be detached by giving their number to detach , but it is much safer to always use a name, for example by detach(lentils) or detach("lentils")
Note: In R lists and data frames can only be attached at position 2 or above, and what is attached is a copy of the original object. You can alter the attached values via assign , but the original list or data frame is unchanged.
6.3.3 Working with data frames ¶
A useful convention that allows you to work with many different problems comfortably together in the same workspace is
In this way it is quite simple to work with many problems in the same directory, all of which have variables named x , y and z , for example.
attach() is a generic function that allows not only directories and data frames to be attached to the search path, but other classes of object as well. In particular any object of mode "list" may be attached in the same way:
> attach(any.old.list)
Anything that has been attached can be detached by detach , by position number or, preferably, by name.
The function search shows the current search path and so is a very useful way to keep track of which data frames and lists (and packages) have been attached and detached. Initially it gives
> search() [1] ".GlobalEnv" "Autoloads" "package:base"
where .GlobalEnv is the workspace. 18
After lentils is attached we have
> search() [1] ".GlobalEnv" "lentils" "Autoloads" "package:base" > ls(2) [1] "u" "v" "w"
and as we see ls (or objects ) can be used to examine the contents of any position on the search path.
Finally, we detach the data frame and confirm it has been removed from the search path.
> detach("lentils") > search() [1] ".GlobalEnv" "Autoloads" "package:base"
Large data objects will usually be read as values from external files rather than entered during an R session at the keyboard. R input facilities are simple and their requirements are fairly strict and even rather inflexible. There is a clear presumption by the designers of R that you will be able to modify your input files using other tools, such as file editors or Perl 19 to fit in with the requirements of R. Generally this is very simple.
If variables are to be held mainly in data frames, as we strongly suggest they should be, an entire data frame can be read directly with the read.table() function. There is also a more primitive input function, scan() , that can be called directly.
For more details on importing data into R and also exporting data, see the R Data Import/Export manual.
To read an entire data frame directly, the external file will normally have a special form.
If the file has one fewer item in its first line than in its second, this arrangement is presumed to be in force. So the first few lines of a file to be read as a data frame might look as follows.
Input file form with names and row labels: Price Floor Area Rooms Age Cent.heat 01 52.00 111.0 830 5 6.2 no 02 54.75 128.0 710 5 7.5 no 03 57.50 101.0 1000 5 4.2 no 04 57.50 131.0 690 6 8.8 no 05 59.75 93.0 900 5 1.9 yes .
By default numeric items (except row labels) are read as numeric variables and non-numeric variables, such as Cent.heat in the example, as character variables. This can be changed if necessary.
The function read.table() can then be used to read the data frame directly
> HousePriceOften you will want to omit including the row labels directly and use the default labels. In this case the file may omit the row label column as in the following.
Input file form without row labels: Price Floor Area Rooms Age Cent.heat 52.00 111.0 830 5 6.2 no 54.75 128.0 710 5 7.5 no 57.50 101.0 1000 5 4.2 no 57.50 131.0 690 6 8.8 no 59.75 93.0 900 5 1.9 yes .
The data frame may then be read as
> HousePricewhere the header=TRUE option specifies that the first line is a line of headings, and hence, by implication from the form of the file, that no explicit row labels are given.
7.2 The scan() function ¶
Suppose the data vectors are of equal length and are to be read in parallel. Further suppose that there are three vectors, the first of mode character and the remaining two of mode numeric, and the file is input.dat . The first step is to use scan() to read in the three vectors as a list, as follows
The second argument is a dummy list structure that establishes the mode of the three vectors to be read. The result, held in inp , is a list whose components are the three vectors read in. To separate the data items into three separate vectors, use assignments like
> labelMore conveniently, the dummy list can have named components, in which case the names can be used to access the vectors read in. For example
If you wish to access the variables separately they may either be re-assigned to variables in the working frame:
> labelor the list may be attached at position 2 of the search path (see Attaching arbitrary lists).
If the second argument is a single value and not a list, a single vector is read in, all components of which must be of the same mode as the dummy value.
There are more elaborate input facilities available and these are detailed in the manuals.
7.3 Accessing builtin datasets ¶
Around 100 datasets are supplied with R (in package datasets), and others are available in packages (including the recommended packages supplied with R). To see the list of datasets currently available use
data()All the datasets supplied with R are available directly by name. However, many packages still use the obsolete convention in which data was also used to load datasets into R, for example
data(infert)and this can still be used with the standard packages (as in this example). In most cases this will load an R object of the same name. However, in a few cases it loads several objects, so see the on-line help for the object to see what to expect.
7.3.1 Loading data from other R packages ¶
To access data from a particular package, use the package argument, for example
data(package="rpart") data(Puromycin, package="datasets")If a package has been attached by library , its datasets are automatically included in the search.
User-contributed packages can be a rich source of datasets.
7.4 Editing data ¶
When invoked on a data frame or matrix, edit brings up a separate spreadsheet-like environment for editing. This is useful for making small changes once a data set has been read. The command
> xnewwill allow you to edit your data set xold , and on completion the changed object is assigned to xnew . If you want to alter the original dataset xold , the simplest way is to use fix(xold) , which is equivalent to xold
> xnewto enter new data via the spreadsheet interface.
8 Probability distributions ¶
One convenient use of R is to provide a comprehensive set of statistical tables. Functions are provided to evaluate the cumulative distribution function P(X q, the smallest x such that P(X q), and to simulate from the distribution.
Distribution | R name | additional arguments |
---|---|---|
beta | beta | shape1, shape2, ncp |
binomial | binom | size, prob |
Cauchy | cauchy | location, scale |
chi-squared | chisq | df, ncp |
exponential | exp | rate |
F | f | df1, df2, ncp |
gamma | gamma | shape, scale |
geometric | geom | prob |
hypergeometric | hyper | m, n, k |
log-normal | lnorm | meanlog, sdlog |
logistic | logis | location, scale |
negative binomial | nbinom | size, prob |
normal | norm | mean, sd |
Poisson | pois | lambda |
signed rank | signrank | n |
Student’s t | t | df, ncp |
uniform | unif | min, max |
Weibull | weibull | shape, scale |
Wilcoxon | wilcox | m, n |
Prefix the name given here by ‘ d ’ for the density, ‘ p ’ for the CDF, ‘ q ’ for the quantile function and ‘ r ’ for simulation (random deviates). The first argument is x for d xxx , q for p xxx , p for q xxx and n for r xxx (except for rhyper , rsignrank and rwilcox , for which it is nn ). In not quite all cases is the non-centrality parameter ncp currently available: see the on-line help for details.
The p xxx and q xxx functions all have logical arguments lower.tail and log.p and the d xxx ones have log . This allows, e.g., getting the cumulative (or “integrated”) hazard function, H(t) = - log(1 - F(t)), by
- pxxx(t, . lower.tail = FALSE, log.p = TRUE)
or more accurate log-likelihoods (by d xxx (. log = TRUE) ), directly.
In addition there are functions ptukey and qtukey for the distribution of the studentized range of samples from a normal distribution, and dmultinom and rmultinom for the multinomial distribution. Further distributions are available in contributed packages, notably SuppDists.
Here are some examples
> ## 2-tailed p-value for t distribution > 2*pt(-2.43, df = 13) > ## upper 1% point for an F(2, 7) distribution > qf(0.01, 2, 7, lower.tail = FALSE)
See the on-line help on RNG for how random-number generation is done in R.
Given a (univariate) set of data we can examine its distribution in a large number of ways. The simplest is to examine the numbers. Two slightly different summaries are given by summary and fivenum and a display of the numbers by stem (a “stem and leaf” plot).
> attach(faithful) > summary(eruptions) Min. 1st Qu. Median Mean 3rd Qu. Max. 1.600 2.163 4.000 3.488 4.454 5.100 > fivenum(eruptions) [1] 1.6000 2.1585 4.0000 4.4585 5.1000 > stem(eruptions) The decimal point is 1 digit(s) to the left of the | 16 | 070355555588 18 | 000022233333335577777777888822335777888 20 | 00002223378800035778 22 | 0002335578023578 24 | 00228 26 | 23 28 | 080 30 | 7 32 | 2337 34 | 250077 36 | 0000823577 38 | 2333335582225577 40 | 0000003357788888002233555577778 42 | 03335555778800233333555577778 44 | 02222335557780000000023333357778888 46 | 0000233357700000023578 48 | 00000022335800333 50 | 0370
A stem-and-leaf plot is like a histogram, and R has a function hist to plot histograms.
> hist(eruptions) ## make the bins smaller, make a plot of density > hist(eruptions, seq(1.6, 5.2, 0.2), prob=TRUE) > lines(density(eruptions, bw=0.1)) > rug(eruptions) # show the actual data points
More elegant density plots can be made by density , and we added a line produced by density in this example. The bandwidth bw was chosen by trial-and-error as the default gives too much smoothing (it usually does for “interesting” densities). (Better automated methods of bandwidth choice are available, and in this example bw = "SJ" gives a good result.)
We can plot the empirical cumulative distribution function by using the function ecdf .
> plot(ecdf(eruptions), do.points=FALSE, verticals=TRUE)
This distribution is obviously far from any standard distribution. How about the right-hand mode, say eruptions of longer than 3 minutes? Let us fit a normal distribution and overlay the fitted CDF.
> long 3] > plot(ecdf(long), do.points=FALSE, verticals=TRUE) > x lines(x, pnorm(x, mean=mean(long), sd=sqrt(var(long))), lty=3)
Quantile-quantile (Q-Q) plots can help us examine this more carefully.
par(pty="s") # arrange for a square figure region qqnorm(long); qqline(long)
which shows a reasonable fit but a shorter right tail than one would expect from a normal distribution. Let us compare this with some simulated data from a t distribution
which will usually (if it is a random sample) show longer tails than expected for a normal. We can make a Q-Q plot against the generating distribution by
qqplot(qt(ppoints(250), df = 5), x, xlab = "Q-Q plot for t dsn") qqline(x)
Finally, we might want a more formal test of agreement with normality (or not). R provides the Shapiro-Wilk test
> shapiro.test(long) Shapiro-Wilk normality test data: long W = 0.9793, p-value = 0.01052
and the Kolmogorov-Smirnov test
> ks.test(long, "pnorm", mean = mean(long), sd = sqrt(var(long))) One-sample Kolmogorov-Smirnov test data: long D = 0.0661, p-value = 0.4284 alternative hypothesis: two.sided
(Note that the distribution theory is not valid here as we have estimated the parameters of the normal distribution from the same sample.)
So far we have compared a single sample to a normal distribution. A much more common operation is to compare aspects of two samples. Note that in R, all “classical” tests including the ones used below are in package stats which is normally loaded.
Consider the following sets of data on the latent heat of the fusion of ice (cal/gm) from Rice (1995, p.490)
Method A: 79.98 80.04 80.02 80.04 80.03 80.03 80.04 79.97 80.05 80.03 80.02 80.00 80.02 Method B: 80.02 79.94 79.98 79.97 79.97 80.03 79.95 79.97
Boxplots provide a simple graphical comparison of the two samples.
which indicates that the first group tends to give higher results than the second.
To test for the equality of the means of the two examples, we can use an unpaired t-test by
> t.test(A, B) Welch Two Sample t-test data: A and B t = 3.2499, df = 12.027, p-value = 0.00694 alternative hypothesis: true difference in means is not equal to 0 95 percent confidence interval: 0.01385526 0.07018320 sample estimates: mean of x mean of y 80.02077 79.97875
which does indicate a significant difference, assuming normality. By default the R function does not assume equality of variances in the two samples. We can use the F test to test for equality in the variances, provided that the two samples are from normal populations.
> var.test(A, B) F test to compare two variances data: A and B F = 0.5837, num df = 12, denom df = 7, p-value = 0.3938 alternative hypothesis: true ratio of variances is not equal to 1 95 percent confidence interval: 0.1251097 2.1052687 sample estimates: ratio of variances 0.5837405
which shows no evidence of a significant difference, and so we can use the classical t-test that assumes equality of the variances.
> t.test(A, B, var.equal=TRUE) Two Sample t-test data: A and B t = 3.4722, df = 19, p-value = 0.002551 alternative hypothesis: true difference in means is not equal to 0 95 percent confidence interval: 0.01669058 0.06734788 sample estimates: mean of x mean of y 80.02077 79.97875
All these tests assume normality of the two samples. The two-sample Wilcoxon (or Mann-Whitney) test only assumes a common continuous distribution under the null hypothesis.
> wilcox.test(A, B) Wilcoxon rank sum test with continuity correction data: A and B W = 89, p-value = 0.007497 alternative hypothesis: true location shift is not equal to 0 Warning message: Cannot compute exact p-value with ties in: wilcox.test(A, B)
Note the warning: there are several ties in each sample, which suggests strongly that these data are from a discrete distribution (probably due to rounding).
There are several ways to compare graphically the two samples. We have already seen a pair of boxplots. The following
> plot(ecdf(A), do.points=FALSE, verticals=TRUE, xlim=range(A, B)) > plot(ecdf(B), do.points=FALSE, verticals=TRUE, add=TRUE)
will show the two empirical CDFs, and qqplot will perform a Q-Q plot of the two samples. The Kolmogorov-Smirnov test is of the maximal vertical distance between the two ecdf s, assuming a common continuous distribution:
> ks.test(A, B) Two-sample Kolmogorov-Smirnov test data: A and B D = 0.5962, p-value = 0.05919 alternative hypothesis: two-sided Warning message: cannot compute correct p-values with ties in: ks.test(A, B)