2020-09-18 11:56:30 +00:00
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# tocID <- "FND-STA-Probability_distribution.R"
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#
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# ---------------------------------------------------------------------------- #
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# PATIENCE ... #
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# Do not yet work wih this code. Updates in progress. Thank you. #
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# boris.steipe@utoronto.ca #
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# ---------------------------------------------------------------------------- #
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2017-10-12 19:11:38 +00:00
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#
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# Purpose: A Bioinformatics Course:
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# R code accompanying the FND-STA-Probability_distribution unit.
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#
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2019-01-08 07:11:25 +00:00
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# Version: 1.3
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2017-10-12 19:11:38 +00:00
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#
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2019-01-07 06:17:23 +00:00
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# Date: 2017 10 - 2019 01
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2017-10-12 19:11:38 +00:00
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# Author: Boris Steipe (boris.steipe@utoronto.ca)
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#
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# Versions:
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2019-01-08 07:11:25 +00:00
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# 1.3 Change from require() to requireNamespace(),
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# use <package>::<function>() idiom throughout,
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2019-01-07 06:17:23 +00:00
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# 1.2 Update set.seed() usage
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2017-11-02 03:29:18 +00:00
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# 1.1 Corrected empirical p-value
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2017-10-12 19:11:38 +00:00
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# 1.0 First code live version
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#
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# TODO:
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# Add tasks
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#
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# == DO NOT SIMPLY source() THIS FILE! =======================================
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#
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# If there are portions you don't understand, use R's help system, Google for an
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# answer, or ask your instructor. Don't continue if you don't understand what's
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# going on. That's not how it works ...
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#
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# ==============================================================================
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2017-10-12 19:14:46 +00:00
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2017-10-29 03:05:53 +00:00
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2017-10-12 19:11:38 +00:00
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#TOC> ==========================================================================
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2020-09-18 11:56:30 +00:00
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#TOC>
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2019-01-08 07:11:25 +00:00
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#TOC> Section Title Line
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#TOC> -----------------------------------------------------------------------------
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#TOC> 1 Introduction 52
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#TOC> 2 Three fundamental distributions 115
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#TOC> 2.1 The Poisson Distribution 118
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#TOC> 2.2 The uniform distribution 172
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#TOC> 2.3 The Normal Distribution 192
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#TOC> 3 quantile-quantile comparison 233
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#TOC> 3.1 qqnorm() 243
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#TOC> 3.2 qqplot() 309
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#TOC> 4 Quantifying the difference 326
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#TOC> 4.1 Chi2 test for discrete distributions 361
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#TOC> 4.2 Kullback-Leibler divergence 452
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#TOC> 4.2.1 An example from tossing dice 463
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#TOC> 4.2.2 An example from lognormal distributions 586
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#TOC> 4.3 Kolmogorov-Smirnov test for continuous distributions 629
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#TOC>
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2017-10-12 19:11:38 +00:00
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#TOC> ==========================================================================
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2017-10-12 19:14:46 +00:00
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# = 1 Introduction ========================================================
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# The space of possible outcomes of events is called a probability distribution
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# and the properties of probability distributions are crucial to our work. Many
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# distributions like the (discrete) Poisson, or the (continuous) Normal
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# distribution have been characterized in great detail, their behaviour is well
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# understood, and they are useful for countless applications - but we also need
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# to able to work with ad hoc distributions that have never been seen before.
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# Let's get a few facts about probability distributions out of the way:
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# The "support" of a probability distribution is the range of outcomes that have
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# a non-zero probability. The "domain" of a probability distribution is the
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# range of probabilities that the distribution can take over its support. Think
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# of this as the ranges on the x- and y-axis respectively. Thus the distribution
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# can be written as p = f(x).
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# The integral over a probability distribution is always 1. This means: the
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# distribution reflects the situation that an event does occur, any event, but
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# there is not "no event".
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2017-10-12 19:14:46 +00:00
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# R's inbuilt probability functions always come in four flavours:
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# d... for "density": this is the probability density function (p.d.f.),
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# the value of f(x) at x.
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# p... for "probability": this is the cumulative distribution function
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# (c.d.f.). It is 0 at the left edge of the support, and 1 at
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# the right edge.
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# q... for "quantile": The quantile function returns the x value at which p...
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# takes a requested value.
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# r... for "random": produces random numbers that are distributed according
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# to the p.d.f.
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# To illustrate with the "Normal Distribution" (Gaussian distribution):
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# 1000 normally distributed values with default parameters: mean 0, sd 1.
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r <- rnorm(1000)
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# pastel green: histogram of 1000 random samples
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hist(r,
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freq = FALSE,
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breaks = 30,
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xlim = c(-4, 4),
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ylim = c(0, 1),
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main = "Normal Distribution",
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xlab = "x",
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ylab = "f(x)",
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col = "#E6FFF6")
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# 100 equally spaced point along x
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x <- seq(-4, 4, length.out = 100)
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# black: c. d. f. along x. Note that this asymptotically reaches 1
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points(x, pnorm(x), type = "l")
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# dark red: p. d. f. along x
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points(x, dnorm(x), type = "l", lwd = 2, col="firebrick")
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# purple: 1% and 99% quantiles
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abline(v = qnorm(c(0.01, 0.99)), lwd = 0.5, col = "#CCAAFF")
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# Study this plot well and familiarize yourself with the terms.
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# = 2 Three fundamental distributions =====================================
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# == 2.1 The Poisson Distribution ==========================================
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# The Poisson distribution is a discrete probability distribution that
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# characterizes how many events we expect among a given number of observations
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# if the mean probability of an event is known. Assume we know that there are
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# 256 transcription factors among the 6091 protein-coding genes of yeast, then
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# the probability of picking a transcription factor at random from all ORFs is
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# 256/6091 ~= 4.2%. How many do we expect if we look e.g. at 250 differentially
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# expressed genes? This means the mean number of transcription factors we would
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# expect in that sample of differentially expressed genes is (250 * 256)/6091.
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dpois(0, (250 * 256) / 6091) # Probability of seeing no TFs
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dpois(1, (250 * 256) / 6091) # Probability of seing one ...
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dpois(2, (250 * 256) / 6091) # Probability of seing two ...
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dpois(3:10, (250 * 256) / 6091) # Probability of seing from three to ten ...
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sum(dpois(0:4, (250 * 256) / 6091)) # Probability of seeing four or less ...
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# Lets plot this
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N <- 25
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x <- dpois(0:N, (250 * 256) / 6091)
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names(x) <- as.character(0:N)
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midPoints <- barplot(x, col = "#E6FFF6",
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axes = TRUE,
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ylim = c(0, 0.15),
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xlab = "# of TF in set",
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ylab = "p")
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# Confirm that our understanding of dpois() is correct, by simulating actual
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# trials:
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N <- 1000
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genes <- numeric(6091) # All genes are 0
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genes[1:256] <- 1 # TFs are 1
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x <- numeric(N) # initialize vector
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set.seed(112358)
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for (i in 1:N) {
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x[i] <- sum(sample(genes, 250)) # sum of TFs in our sample in this trial
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}
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2019-01-07 06:17:23 +00:00
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set.seed(NULL)
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(t <- table(x)/N)
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# Add these values to the plot
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y <- numeric(26) # initialize vector with 26 slots
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y[as.numeric(names(t)) + 1] <- t # put the tabled values there (index + 1)
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points(midPoints, y, pch = 21, cex = 0.7, bg = "firebrick")
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legend("topright",
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legend = c("poisson distribution", "samples"),
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pch = c(22, 21),
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pt.bg = c("#E6FFF6", "firebrick"),
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bty = "n")
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# == 2.2 The uniform distribution ==========================================
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# The uniform distribution has the same probability over its entire support. R's
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# runif() function takes the desired number, the min and the max as arguments.
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# Let's plot a histogram of a million values between -1 and 1 to demonstrate.
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hist(runif(1e6, -1, 1), breaks = 20, col = "#FFE6F6")
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abline(h = 1e6/20, col="firebrick")
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# One of the important uses of the uniform distribution is to write conditional
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# expressions that are TRUE with a given probability. For example, to get TRUE
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# values with a probability of 1/3, we pick a random number between 0 and 1, and
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# ask whether the number is smaller than 1/3. Example:
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runif(10) < 1/3
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#confirm with a million trials
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sum(runif(1e6) < 1/3)/1e6 # should be close to 0.33333...
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# == 2.3 The Normal Distribution ===========================================
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# The king of probability distributions. Why? That's because of the Central
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# Limit Theorem (CLT) that essentially says that a process that is subject to
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# small fluctuations will tend to normally distributed outcomes ... and in
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# biology literally everything is subject to small fluctuations.
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# Lets simulate: Lets create a vector of 12345 numbers, choose samples of size
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# 77 from that vector and calculate the mean. We do that 9999 times. I am just
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# using odd numbers so it is clear in the code which number represents what.
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x <- runif(12345)
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v <- numeric(9999)
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 77))
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}
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hist(v, breaks = 20, col = "#F8DDFF")
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# Let's try this again, this time sampling from an exponential distribution ...
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x <- rexp(12345)
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v <- numeric(9999)
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 77))
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}
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hist(v, breaks = 20, col = "#F8DDFF")
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# ... or from a t-distribution ...
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x <- rt(12345, df = 3)
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v <- numeric(9999)
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 77))
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}
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hist(v, breaks = 20, col = "#F8DDFF")
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# The outcomes all give normal distributions, regardless what the details of our
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# original distribution were!
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# = 3 quantile-quantile comparison ========================================
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# Once we have observed a distribution of outcomes, the next task is often to
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# quantify whether the values correspond to a known distribution. This can be
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# done with quantile-quantile plots that plot the quantile values of one
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# distribution against those of the other. Identically distributed quantiles lie
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# on a straight line.
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# == 3.1 qqnorm() ==========================================================
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# The functions qqnorm() and qqline() perform this
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# comparison with the normal distribution.
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2019-01-07 06:17:23 +00:00
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set.seed(112358)
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x <- rnorm(100, mean=0, sd=1) # 100 normally distributed values
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set.seed(NULL)
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qqnorm(x)
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qqline(x, col = "seagreen")
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# Our variables in x appear normally distribute - which is not surprising since
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# we produced them with rnorm(). What about the kind of sampling we did above?
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# Let's test whether samples from an exponential distribution are normally
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# distributed (previously we just visually inspected the histogram.)
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# Create a vector of sample means from the exponential distribution; use
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# only a few samples for the mean
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x <- rexp(12345)
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v <- numeric(999)
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set.seed(112358)
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 12))
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}
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set.seed(NULL)
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qqnorm(v)
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qqline(v, col = "turquoise") # normal
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#try with more samples
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 77))
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}
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qqnorm(v)
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qqline(v, col = "steelblue") # normal
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#try with many samples
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for (i in 1:length(v)) {
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v[i] <- mean(sample(x, 374))
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}
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qqnorm(v)
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qqline(v, col = "plum") # normal
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# Exactly as the CLT predicts, the more often we sample - we tried
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# 12, 77, and 374 samples - the more "normal" the distribution looks.
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# What does a distribution look like that is NOT normal?
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# Let's try simulating an "Extreme value distribution". This type of
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# distribution appears if we choose the max() of a sample
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set.seed(112358)
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rEVD <- numeric(9999)
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for (i in seq_along(rEVD)) {
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rEVD[i] <- max(rnorm(100))
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}
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set.seed(NULL)
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hist(rEVD, breaks = 20, col = "orchid")
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# Note the long tail on the right!
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qqnorm(rEVD)
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qqline(rEVD, col = "orchid") # Definitely not "normal"!
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# == 3.2 qqplot() ==========================================================
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# qqplot() works like qqnorm(), except that we compare two arbitrary
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# distribtutions, rather than one distribution against the normal distribution
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# as we did before. Sample against sample.
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x <- seq(0, 4, length.out = 100)
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dl <- dlnorm(x) # log-normal distribution
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dg <- dgamma(x, shape=1.5) # gamma distribution
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plot(dl, type="l")
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points(dg, type="l", col = "maroon")
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qqplot(dl, dg) # clearly not equal
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# = 4 Quantifying the difference ==========================================
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# Quantile-quantile plots give us a visual estimate, but how do we quantify the
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# difference between distributions? Let's compare two types of extreme-value
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|
# distributions, a lognormal distribution with the same distribution that is
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# slightly shifted, and three gamma distributions with three different shape
|
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# parameters. Let's define and visualize the distributions first, to see what
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# we are comparing.
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x <- seq(0, 4, length.out = 100)
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set.seed(112358)
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dl1 <- dlnorm(x) # log-normal distribution
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dl2 <- dlnorm(x - 0.25) # log-normal distribution, shifted right (a bit)
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dg1.2 <- dgamma(x, shape=1.2) # three gamma distributions with...
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dg1.5 <- dgamma(x, shape=1.5) # ...wider, and wider...
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dg1.9 <- dgamma(x, shape=1.9) # ...peak
|
2019-01-07 06:17:23 +00:00
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set.seed(NULL)
|
2017-10-12 19:11:38 +00:00
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myCols <- c("black", "grey", "maroon", "turquoise", "steelblue")
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plot(dl1, type="l", lwd=2) # visualize the distributions
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points(dl2, type="l", col = myCols[2])
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points(dg1.2, type="l", col = myCols[3])
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points(dg1.5, type="l", col = myCols[4])
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points(dg1.9, type="l", col = myCols[5])
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legend("topright",
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legend = c("dl1", "dl2", "dg1.2", "dg1.5", "dg1.9"),
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lty = 1,
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lwd = c(2, 1, 1, 1, 1),
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col = myCols,
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bty = "n")
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|
# == 4.1 Chi2 test for discrete distributions ==============================
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# The chi2 test can be used to compare discrete distributions - even though
|
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# it is not ideal for this purpose.
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# (https://stats.stackexchange.com/questions/113692/test-identicality-of-discrete-distributions)
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#
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# Let's draw 100 random variables according to our target distributions
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N <- 100
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set.seed(112358)
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rL1 <- rlnorm(N) # log-normal distribution
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rL2 <- rlnorm(N, meanlog = 0.25) # log-normal distribution, shifted right
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rG1.2 <- rgamma(N, shape=1.2) # three gamma distributions with...
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rG1.5 <- rgamma(N, shape=1.5) # ...wider, and wider...
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rG1.9 <- rgamma(N, shape=1.9) # ...peak
|
2019-01-07 06:17:23 +00:00
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|
set.seed(NULL)
|
2017-10-12 19:11:38 +00:00
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maxX <- max(c(rL1, rL2, rG1.2, rG1.5, rG1.9))
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myBreaks <- seq(0, 5, length.out = 10) # 9 intervals from 0 to 5...
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myBreaks <- c(myBreaks, maxX) # ... and one that contains the outliers
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|
# It's easy to plot a histogram of one set of random deviates...
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|
hist(rG1.5, breaks = myBreaks, col = myCols[4])
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|
# ... but basic R has no inbuilt function to stack histogram bars side-by-side.
|
2017-10-29 03:05:53 +00:00
|
|
|
# We use the multhist() function in the plotrix package: check out the
|
|
|
|
# package information - plotrix has _many_ useful utilities to enhance
|
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|
|
# plots or produce informative visualizations.
|
2017-10-12 19:11:38 +00:00
|
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|
|
2019-01-08 07:11:25 +00:00
|
|
|
if (! requireNamespace("plotrix", quietly = TRUE)) {
|
2017-10-12 19:11:38 +00:00
|
|
|
install.packages("plotrix")
|
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|
|
}
|
2017-10-29 03:05:53 +00:00
|
|
|
# Package information:
|
|
|
|
# library(help = plotrix) # basic information
|
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|
|
# browseVignettes("plotrix") # available vignettes
|
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|
|
# data(package = "plotrix") # available datasets
|
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|
2017-10-12 19:11:38 +00:00
|
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|
|
2019-01-08 07:11:25 +00:00
|
|
|
h <- plotrix::multhist(list(rL1, rL2, rG1.2, rG1.5, rG1.9 ),
|
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|
breaks = myBreaks,
|
|
|
|
col = myCols)
|
2017-10-12 19:11:38 +00:00
|
|
|
legend("topright",
|
|
|
|
legend = c("rL1", "rL2", "rG1.2", "rG1.5", "rG1.9"),
|
|
|
|
pch=15,
|
|
|
|
col = myCols,
|
|
|
|
bty="n")
|
|
|
|
|
|
|
|
# We have assigned the output of multihist to the variable h, which now
|
|
|
|
# contains the densities, midpoints, breaks etc. of the histogram ...
|
|
|
|
# as well as the matrix of counts:
|
|
|
|
h[[2]]
|
|
|
|
|
|
|
|
# But using hist() or multhist() for binning is a bit of a hack - even though
|
|
|
|
# it works, of course. The "real" R function to bin data is cut(). cut()
|
|
|
|
# sorts the values of a vector into bins, and returns the bin-labels as
|
|
|
|
# integers.
|
|
|
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|
|
x <- cut(rL1, breaks = myBreaks, labels = FALSE)
|
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|
|
table(x)
|
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|
|
countsL1 <- table(cut(rL1 , breaks = myBreaks, labels = FALSE))
|
|
|
|
countsL2 <- table(cut(rL2 , breaks = myBreaks, labels = FALSE))
|
|
|
|
countsG1.2 <- table(cut(rG1.2, breaks = myBreaks, labels = FALSE))
|
|
|
|
countsG1.5 <- table(cut(rG1.5, breaks = myBreaks, labels = FALSE))
|
|
|
|
countsG1.9 <- table(cut(rG1.9, breaks = myBreaks, labels = FALSE))
|
|
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|
|
chisq.test(countsL1, countsL2)
|
|
|
|
|
|
|
|
# Note that this use of the chi2 test does not have very much power, since it
|
|
|
|
# does not assume the values for the bins are ordered, but takes them to
|
|
|
|
# be independent. Also, chisq.test() complains about the Chi-squared
|
|
|
|
# approximation to be possibly incorrect because some of the counts are small.
|
|
|
|
# In this case, rather than rely on the in-built chi-square table, we can do
|
|
|
|
# an explicit simulation to estimate the p-value for the null hypothesis.
|
|
|
|
#
|
|
|
|
chisq.test(countsL1, countsL2, simulate.p.value = TRUE, B = 10000)
|
|
|
|
|
|
|
|
# Note that the probability that the samples came from the same distribution is
|
|
|
|
# quite high. We don't seem to be able to distinguish l1 and l2 with the chi2
|
|
|
|
# test.
|
|
|
|
|
|
|
|
# Let's calculate this for the other distribution too:
|
|
|
|
|
|
|
|
chisq.test(countsL1, countsG1.2, simulate.p.value = TRUE, B = 10000)
|
|
|
|
chisq.test(countsL1, countsG1.5, simulate.p.value = TRUE, B = 10000)
|
|
|
|
chisq.test(countsL1, countsG1.9, simulate.p.value = TRUE, B = 10000)
|
|
|
|
|
|
|
|
# As a result, we would conclude that none of these distributions are
|
|
|
|
# significantly different.
|
|
|
|
|
|
|
|
# == 4.2 Kullback-Leibler divergence =======================================
|
|
|
|
|
|
|
|
# For discrete probability distributions, there is a much better statistic, the
|
|
|
|
# Kullback-Leibler divergence (or relative entropy). It is based in information
|
2017-10-29 03:05:53 +00:00
|
|
|
# theory, and evaluates how different the matched pairs of outcome categories
|
2017-10-12 19:11:38 +00:00
|
|
|
# are. Its inputs are the probability mass functions (p.m.f.) of the two
|
|
|
|
# functions to be compared. A probability mass function is the probability of
|
|
|
|
# every outcome the process can have. Kullback-Leibler divergence therefore can
|
|
|
|
# be applied to discrete distributions. But we need to talk a bit about
|
|
|
|
# converting counts to p.m.f.'s.
|
|
|
|
|
2020-09-18 11:56:30 +00:00
|
|
|
# === 4.2.1 An example from tossing dice
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
# The p.m.f of an honest die is (1:1/6, 2:1/6, 3:1/6, 4:1/6, 5:1/6, 6:1/6). But
|
|
|
|
# there is an issue when we convert sampled counts to frequencies, and estimate
|
|
|
|
# probabilities with these frequencies. The problem is: by chance we might not
|
|
|
|
# have observed a particular outcome! Consider this example:
|
|
|
|
|
|
|
|
set.seed(47)
|
|
|
|
N <- 20
|
|
|
|
(counts <- table(sample(1:6, N, replace = TRUE)))
|
2019-01-07 06:17:23 +00:00
|
|
|
set.seed(NULL)
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
# We have not observed a "2"!
|
|
|
|
#
|
|
|
|
# Now, if we convert the counts to frequencies, and assume these to be
|
|
|
|
# probabilities, we get an observed p.m.f:
|
|
|
|
pmf <- numeric(6)
|
|
|
|
for (i in seq_along(counts)) {
|
|
|
|
outcome <- as.integer(names(counts)[i])
|
|
|
|
pmf[outcome] <- counts[i]/N
|
|
|
|
}
|
|
|
|
names(pmf) <- 1:6
|
|
|
|
pmf
|
|
|
|
|
|
|
|
# This means we assign a probability of 0 to the outcome "2" - because we
|
|
|
|
# haven't observed it. But how do we compare it then? What does it mean when we
|
|
|
|
# should have 1/6 of "2"s but we have none whatsoever? Taken at face value it
|
|
|
|
# means we are comparing apples to oranges - essentially a five-faced die with a
|
|
|
|
# six-faced die - and therefore divergence is infinitely large. Obviously, that
|
|
|
|
# was just a problem caused by our limited sampling, but the question remains:
|
|
|
|
# how do we account for missing data? There are several solutions, for example,
|
|
|
|
# for ordered data one could substitute the average values of the two bracketing
|
|
|
|
# outcomes. But a simple and quite robust solution is to add "pseudocounts".
|
|
|
|
# This is called adding a Laplace prior, or a Jeffreys prior: in our case,
|
2017-11-21 00:00:23 +00:00
|
|
|
# simply add 0.5 to every category.
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
# pmf of an honest die
|
|
|
|
pmfHD <- rep(1/6, 6)
|
|
|
|
names(pmfHD) <- 1:6
|
|
|
|
pmfHD
|
|
|
|
|
|
|
|
# pmf, estimated from our sampled counts with and without pseudocounts
|
|
|
|
|
|
|
|
pmfPC <- numeric(6) + 0.5
|
|
|
|
for (i in seq_along(counts)) {
|
|
|
|
outcome <- as.integer(names(counts)[i])
|
|
|
|
pmfPC[outcome] <- counts[i] + pmfPC[outcome]
|
|
|
|
}
|
|
|
|
pmfPC <- pmfPC / sum(pmfPC)
|
|
|
|
names(pmfPC) <- 1:6
|
|
|
|
pmf # before
|
|
|
|
pmfPC # after
|
|
|
|
|
|
|
|
# The definition of a function that takes samples and returns a pmf
|
|
|
|
# with pseudocounts is straightforward, but requires a bit of juggling
|
|
|
|
# the observed values into the right slots. Here's what this can look like:
|
|
|
|
|
|
|
|
pmfPC <- function(cts, nam) {
|
|
|
|
# Convert counts to a p.m.f, adding a pseudocount of 0.5 to all categories
|
|
|
|
# of outcomes (Jeffreys prior).
|
|
|
|
# Parameters:
|
|
|
|
# cts num raw counts
|
|
|
|
# nam names of the categories, converted to char
|
|
|
|
# Value a probability mass function
|
|
|
|
|
|
|
|
nam <- as.character(nam)
|
|
|
|
if (!all(names(cts) %in% nam)) {
|
|
|
|
stop("PANIC: names in \"cts\" do not match \"nam\"!")
|
|
|
|
}
|
|
|
|
pmf <- numeric(length(nam))
|
|
|
|
names(pmf) <- nam
|
|
|
|
pmf[names(cts)] <- cts[names(cts)]
|
|
|
|
pmf <- pmf + 0.5 # add pseudocounts
|
|
|
|
return(pmf/sum(pmf))
|
|
|
|
}
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
# The definition of the Kullback-Leibler divergence itself is quite simple
|
|
|
|
# actually: for two distributions, p and q it is sum(p * log( p / q))
|
|
|
|
|
|
|
|
KLdiv <- function(p, q) {
|
|
|
|
# p and q are two pmfs of discrete probability distributions
|
|
|
|
# with the same outcomes, which are nowhere 0.
|
|
|
|
# Value: Kullback-Leibler divergence sum(p * log( p / q))).
|
|
|
|
|
|
|
|
if (length(p) != length(q)) {
|
|
|
|
stop("PANIC: input vector lengths differ!")
|
|
|
|
}
|
|
|
|
if (any(c((p == 0), (q == 0)))) {
|
|
|
|
stop("PANIC: 0's found in input vectors!")
|
|
|
|
}
|
|
|
|
|
|
|
|
return(sum(p * log( p / q )))
|
|
|
|
}
|
|
|
|
|
|
|
|
# Now we can calculate KL-divergences for our six-faced die example:
|
|
|
|
|
|
|
|
KLdiv(rep(1/6, 6), pmfPC(counts, 1:6)) # p.m.f. of an honest die vs. our
|
|
|
|
# actual counts
|
|
|
|
|
|
|
|
# Is that a lot? Let's look at the distribution of KL-divergences in our
|
|
|
|
# six-sided die scenario: p.m.f. of 20 samples each versus the theoretical
|
|
|
|
# p.m.f.
|
|
|
|
|
|
|
|
N <- 1000
|
|
|
|
nSample <- 20
|
|
|
|
divs <- numeric(N)
|
|
|
|
for (i in 1:N) {
|
|
|
|
x <- table(sample(1:6, nSample, replace = TRUE))
|
|
|
|
divs[i] <- KLdiv(rep(1/6, 6), pmfPC(x, 1:6))
|
|
|
|
}
|
|
|
|
|
|
|
|
hist(divs,
|
|
|
|
col = "whitesmoke",
|
|
|
|
xlab = "Kullback-Leibler divergence",
|
|
|
|
main = sprintf("%d samples of honest die", nSample))
|
|
|
|
abline(v = KLdiv(rep(1/6, 6), pmfPC(counts, 1:6)), col="firebrick")
|
|
|
|
|
|
|
|
# We see that our example sample (KL-divergence marked with the red line) is
|
|
|
|
# somewhat but not drastically atypical.
|
|
|
|
|
|
|
|
|
2020-09-18 11:56:30 +00:00
|
|
|
# === 4.2.2 An example from lognormal distributions
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
# We had compared a set of lognormal and gamma distributions above, now we
|
|
|
|
# can use KL-divergence to quantify their similarity:
|
|
|
|
|
|
|
|
pmfL1 <- pmfPC(countsL1, nam = 1:10)
|
|
|
|
pmfL2 <- pmfPC(countsL2, nam = 1:10)
|
|
|
|
KLdiv(pmfL1, pmfL2) # 0.1087
|
|
|
|
|
|
|
|
# To evaluate what this number means, we can run a simple simulation: we create
|
|
|
|
# random samples according to the rL1 distribution, calculate the Kullback
|
|
|
|
# Leibler divergence with countsL1, and compare the distribution we get with the
|
|
|
|
# value we observed as the difference with discL2. Essentially, this tells us
|
2018-10-31 01:27:42 +00:00
|
|
|
# the probability that countsL2 is actually a sample from the L1 function.
|
|
|
|
# Here we go:
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
N <- 1000
|
|
|
|
divs <- numeric(N)
|
|
|
|
|
|
|
|
set.seed(31416)
|
|
|
|
for (i in 1:N) {
|
|
|
|
x <- rlnorm(100) # get random samples from our reference distributions
|
|
|
|
y <- table(cut(x, breaks = myBreaks, labels = FALSE)) # tabulate counts
|
|
|
|
q <- pmfPC(y, nam = 1:10) # convert to p.m.f. with pseudocounts
|
|
|
|
divs[i] <- KLdiv(pmfL1, q) # calculate Kullback-Leibler divergence
|
|
|
|
}
|
2019-01-07 06:17:23 +00:00
|
|
|
set.seed(NULL)
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
hist(divs,
|
|
|
|
col = "thistle",
|
|
|
|
xlab = "Kullback-Leibler divergence",
|
|
|
|
main = sprintf("Samples from shifted lnorm()"))
|
|
|
|
abline(v = KLdiv(pmfL1, pmfL2), col="firebrick")
|
|
|
|
|
|
|
|
# How many KL-divergences were less than the difference we observed?
|
2019-01-07 06:17:23 +00:00
|
|
|
sum(divs < KLdiv(pmfL1, pmfL2)) # 933
|
2017-10-12 19:11:38 +00:00
|
|
|
|
2017-11-02 03:29:18 +00:00
|
|
|
# Therefore the empirical p-value that the samples came from the same
|
|
|
|
# distribution is only 100 * ((N - 933) + 1) / (N + 1) (%) ... 6.8%. You see
|
|
|
|
# that this gives a much more powerful statistical approach than the chi2 test
|
|
|
|
# we used above.
|
2017-10-12 19:11:38 +00:00
|
|
|
|
|
|
|
|
|
|
|
# == 4.3 Kolmogorov-Smirnov test for continuous distributions ==============
|
|
|
|
|
|
|
|
# The Kolmogorov-Smirnov (KS) test is meant for continuous distributions, i.e.
|
|
|
|
# the probability it calculates assumes that the function values are all
|
|
|
|
# different. In the case of random samples, that is a reasonable assumption. KS
|
|
|
|
# is a two-sample goodness of fit test, i.e. it has a null-hypothesis that the
|
|
|
|
# samples were taken from the same (unknown) distribution, and then asks whether
|
|
|
|
# this is likely, given the actual values. It is sensitive both to differences
|
|
|
|
# in location (position of the mean), and differences in shape. R has the
|
|
|
|
# ks.test() function to calculate it.
|
|
|
|
|
|
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ks.test(dl1, dl2) # vs. shifted log-normal.
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ks.test(dl1, dg1.2) # vs. the three gamma distributions
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ks.test(dl1, dg1.5)
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ks.test(dl1, dg1.9)
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ks.test(dg1.5, dg1.9) # the two last gammas against each other
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2017-11-02 03:29:18 +00:00
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# (The warnings about the presence of ties comes from the 0's in our function
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2017-10-12 19:11:38 +00:00
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# values). The p-value that these distributions are samples of the same
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# probability distribution gets progressively smaller.
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# [END]
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