Difference between std and t distributions - r

I have a question regarding the definitions std and t of the student-t distribution in R. std comes with the rugarch package, while t is from the stats package. When plotting
qqplot(qstd(c(1:1000)/1001, nu=5),qt(c(1:1000)/1001,df=5))
abline(0,1)
it is clear to see that the two definitions are different. Can anyone tell me why there is this difference and which one of the functions gives the correct values?

If you open up the qstd function (which is actually from fGarch), you'll see that it's modifying stats::qt:
> qstd
function (p, mean = 0, sd = 1, nu = 5)
{
s = sqrt(nu/(nu - 2))
result = qt(p = p, df = nu) * sd/s + mean
result
}
<environment: namespace:fGarch>
So, what it's giving you is a "non-standardized Student's t-distribution" as opposed to the standardized distribution available from stats. If s=1 and as degrees of freedom goes to infinity, they will produce the same result.

Related

Estimating PDF with monotonically declining density at tails

tldr: I am numerically estimating a PDF from simulated data and I need the density to monotonically decrease outside of the 'main' density region (as x-> infinity). What I have yields a close to zero density, but which does not monotonically decrease.
Detailed Problem
I am estimating a simulated maximum likelihood model, which requires me to numerically evaluate the probability distribution function of some random variable (the probability of which cannot be analytically derived) at some (observed) value x. The goal is to maximize the log-likelihood of these densities, which requires them to not have spurious local maxima.
Since I do not have an analytic likelihood function I numerically simulate the random variable by drawing the random component from some known distribution function, and apply some non-linear transformation to it. I save the results of this simulation in a dataset named simulated_stats.
I then use density() to approximate the PDF and approxfun() to evaluate the PDF at x:
#some example simulation
Simulated_stats_ <- runif(n=500, 10,15)+ rnorm(n=500,mean = 15,sd = 3)
#approximation for x
approxfun(density(simulated_stats))(x)
This works well within the range of simulated simulated_stats, see image:
Example PDF. The problem is I need to be able to evaluate the PDF far from the range of simulated data.
So in the image above, I would need to evaluate the PDF at, say, x=50:
approxfun(density(simulated_stats))(50)
> [1] NA
So instead I use the from and to arguments in the density function, which correctly approximate near 0 tails, such
approxfun(
density(Simulated_stats, from = 0, to = max(Simulated_stats)*10)
)(50)
[1] 1.924343e-18
Which is great, under one condition - I need the density to go to zero the further out from the range x is. That is, if I evaluated at x=51 the result must be strictly smaller. (Otherwise, my estimator may find local maxima far from the 'true' region, since the likelihood function is not monotonic very far from the 'main' density mass, i.e. the extrapolated region).
To test this I evaluated the approximated PDF at fixed intervals, took logs, and plotted. The result is discouraging: far from the main density mass the probability 'jumps' up and down. Always very close to zero, but NOT monotonically decreasing.
a <- sapply(X = seq(from = 0, to = 100, by = 0.5), FUN = function(x){approxfun(
density(Simulated_stats_,from = 0, to = max(Simulated_stats_)*10)
)(x)})
aa <- cbind( seq(from = 0, to = 100, by = 0.5), a)
plot(aa[,1],log(aa[,2]))
Result:
Non-monotonic log density far from density mass
My question
Does this happen because of the kernel estimation in density() or is it inaccuracies in approxfun()? (or something else?)
What alternative methods can I use that will deliver a monotonically declining PDF far from the simulated density mass?
Or - how can I manually change the approximated PDF to monotonically decline the further I am from the density mass? I would happily stick some linear trend that goes to zero...
Thanks!
One possibility is to estimate the CDF using a beta regression model; numerical estimate of the derivative of this model could then be used to estimate the pdf at any point. Here's an example of what I was thinking. I'm not sure if it helps you at all.
Import libraries
library(mgcv)
library(data.table)
library(ggplot2)
Generate your data
set.seed(123)
Simulated_stats_ <- runif(n=5000, 10,15)+ rnorm(n=500,mean = 15,sd = 3)
Function to estimate CDF using gam beta regression model
get_mod <- function(ss,p = seq(0.02, 0.98, 0.02)) {
qp = quantile(ss, probs=p)
betamod = mgcv::gam(p~s(qp, bs="cs"), family=mgcv::betar())
return(betamod)
}
betamod <- get_mod(Simulated_stats_)
Very basic estimate of PDF at val given model that estimates CDF
est_pdf <- function(val, betamod, tol=0.001) {
xvals = c(val,val+tol)
yvals = predict(betamod,newdata=data.frame(qp = xvals), type="response")
as.numeric((yvals[1] - yvals[2])/(xvals[1] - xvals[2]))
}
Lets check if monotonically increasing below min of Simulated_stats
test_x = seq(0,min(Simulated_stats_), length.out=1000)
pdf = sapply(test_x, est_pdf, betamod=betamod)
all(pdf == cummax(pdf))
[1] TRUE
Lets check if monotonically decreasing above max of Simulated_stats
test_x = seq(max(Simulated_stats_), 60, length.out=1000)
pdf = sapply(test_x, est_pdf, betamod=betamod)
all(pdf == cummin(pdf))
[1] TRUE
Additional thoughts 3/5/22
As discussed in comments, using the betamod to predict might slow down the estimator. While this could be resolved to a great extent by writing your own predict function directly, there is another possible shortcut.
Generate estimates from the betamod over the range of X, including the extremes
k <- sapply(seq(0,max(Simulated_stats_)*10, length.out=5000), est_pdf, betamod=betamod)
Use the approach above that you were initially using, i.e. a linear interpolation across the density, but rather than doing this over the density outcome, instead do over k (i.e. over the above estimates from the beta model)
lin_int = approxfun(x=seq(0,max(Simulated_stats_)*10, length.out=5000),y=k)
You can use the lin_int() function for prediction in the estimator, and it will be lighting fast. Note that it produces virtually the same value for a given x
c(est_pdf(38,betamod), lin_int(38))
[1] 0.001245894 0.001245968
and it is very fast
microbenchmark::microbenchmark(
list = alist("betamod" = est_pdf(38, betamod),"lin_int" = lint(38)),times=100
)
Unit: microseconds
expr min lq mean median uq max neval
betamod 1157.0 1170.20 1223.304 1188.25 1211.05 2799.8 100
lin_int 1.7 2.25 3.503 4.35 4.50 10.5 100
Finally, lets check the same plot you did before, but using lin_int() instead of approxfun(density(....))
a <- sapply(X = seq(from = 0, to = 100, by = 0.5), lin_int)
aa <- cbind( seq(from = 0, to = 100, by = 0.5), a)
plot(aa[,1],log(aa[,2]))

Hydenet r package: setnode() simulates wrong standard deviation for normal distribution

In the r package hydenet I'm unable to simulate the standard deviations I inputted earlier using setnode(). hydenet exports to jags for simulations.
I load in libraries here and make a simple graph showing that node_a affects node_b
library(rjags)
library(HydeNet)
dag = HydeNetwork(~node_a
+ node_b | node_a)
I give both nodes a standard deviation (node a is set to 100, node b is set to 0.25)
dag = setNode(dag, node_a, nodeType = "dnorm", mean = 10, sd = 100) #.1
dag = setNode(dag, node_b, nodeType = "dnorm", mean = "15 + 0.2*node_a", sd = 0.25)
I compile to Jags and simulate a data frame of 100000 below.
comp_dag = compileJagsModel(dag)
sim = HydeSim(comp_dag, variable.names = c("node_a", "node_b"), n.iter = 100000)
yet for some reason when I check the standard deviations for the nodes on the simulated data, the standard deviations are wrong. For some reason, simulated_sd=sqrt(1/input_sd). I also don't know why it follows this equation.
sd(sim$node_a)
#0.1000575
sd(sim$node_b)
#1.992311
when hydenet is fed the simulated data it estimates close to the original input of standard deviation, so weirdly that seems to work. This is unfortunate because I need to use both of these equations. Thus, it prevents me from just reversing the equation I derived before.
sim_dag = HydeNetwork(~node_a
+ node_b | node_a, data = sim)
writeNetworkModel(sim_dag, pretty = T)
# model{
# node_a ~ dnorm(9.99955, 100.00706)
# node_b ~ dnorm(15.53815 + 0.1468 * node_a, 0.25169)
# }
I figured it out, though I thought I'd leave my post up for anyone else who's confused. JAGs takes mean and precision not mean and standard deviations. Precision is 1/variance which also explains the equation I got between the input and output standard deviations.
Back calculating based on the equation I wrote (simulated_sd = 1/sqrt(input_sd)) will work if you're simulating things from JAGS in R.

Using mle2 function

I would like to find the MLE for parameters epsilon and mu in such a model:
$$X \sim \frac{1}{mu1}e^{-x/mu1}+\frac{1}{mu2}e^[-x/mu2}$$
library(Renext)
library(bbmle)
epsilon = 0.01
#the real model
X <- rmixexp2(n = 20, prob1 = epsilon, rate1 = 1/mu1, rate2 = 1/mu2)
LL <- function(mu1,mu2, eps){
R = (1-eps)*dexp(X,rate=1/mu1,log=TRUE)+eps*dexp(X,rate=1/mu2,log=TRUE)
-sum(R)
}
fit_norm <- mle2(LL, start = list(eps = 0,mu1=1, mu2 = 1), lower = c(-Inf, 0),
upper = c(Inf, Inf), method = 'L-BFGS-B')
summary(fit_norm)
But I get the error
> fn = function (p) ':method 'L-BFGS-B' requires finite values of fn"
There are a bunch of issues here. The primary one is that your likelihood expression is wrong (you can't log the components separately and then add them, you have to add the components and then take the log). Your bounds are also funny: the mixture probability should be [0,1] and the means should be [0, Inf].
The other problem you have is that with the current simulation design (n=20, prob=0.01), you have a high probability of getting no points in the first mixture component (the probability of a point being in the second component is 1-0.01=0.99, so the probability that all of the points are in the second component is 0.99^20 = 82%). In this case the MLE will be degenerate (i.e., you're trying to fit a two-component mixture to a data set that essentially only has one component); in this case any of these solutions will give equivalent likelihoods:
prob=0, mu2=mean of the data, mu1=anything
prob=1, mu1=mean of the data, mu2=anything
mu1=mu2=mean of the data, prob=anything
With all these solutions, where you end up will depend very sensitively on starting conditions and optimization algorithm.
For this problem I would encourage you to use the built-in dmixexp2 function from the Renext package (which correctly implements the log-likelihood as log(p*Prob(X|exp1) + (1-p)*Prob(X|exp2))) and the formula interface to mle2:
fit_norm <- mle2(X ~ dmixexp2(rate1=1/mu1,rate2=1/mu2,prob1=eps),
data=list(X=X),
start = list(mu1=1, mu2 = 2, eps=0.4),
lower = c(mu1=0, mu2=0, eps=0),
upper = c(mu1=Inf, mu2=Inf, eps=1),
method = 'L-BFGS-B')
This gives me estimates of mu1=1.58, mu2=2.702, eps=0. mean(X) in my case equals the value of mu2, so this is the first case in the bulleted list above. You also get a warning:
some parameters are on the boundary: variance-covariance calculations based on Hessian may be unreliable
There are also a variety of more specialized algorithms for fitting mixture models (especially those based on the expectation-maximization algorithm); you can look for packages on CRAN (flexmix is one of them).
This problem is small enough that you can visualize the whole log-likelihood surface by brute force (code below): the colours represent deviations from the minimum negative log-likelihood (the colour gradient is log-scaled, so there's a small offset to avoid log(0)). Dark blue represents parameters that are the best fit to the data, yellow are the worst.
dd <- expand.grid(mu1=seq(0.1,4,length=51),
mu2=seq(0.1,4,length=51),
eps=seq(0,1,length=9),
nll=NA)
for (i in 1:nrow(dd)) {
dd$nll[i] <- with(dd[i,],
-sum(dmixexp2(X,rate1=1/mu1,
rate2=1/mu2,
prob1=eps,
log=TRUE)))
}
library(ggplot2)
ggplot(dd,aes(mu1,mu2,fill=nll-min(nll)+1e-4)) +
facet_wrap(~eps, labeller=label_both) +
geom_raster() +
scale_fill_viridis_c(trans="log10") +
scale_x_continuous(expand=c(0,0)) +
scale_y_continuous(expand=c(0,0)) +
theme(panel.spacing=grid::unit(0.1,"lines"))
ggsave("fit_norm.png", type="cairo-png")

How does the pnorm aspect of work with z scores & x-values?

My professor assigned us some homework questions regarding normal distributions. We are using R studio to calculate our values instead of the z-tables.
One question asks about something about meteors where the mean (μ) = 4.35, standard deviation (σ) = 0.59 and we are looking for the probability of x>5.
I already figured out the answer with 1-pnorm((5-4.35)/0.59) ~ 0.135.
However, I am currently having some difficulty trying to understand what pnorm calculates.
Originally, I just assumed that z scores were the only arguments needed. So I proceeded to use pnorm(z-score) for most of the normal curvature problems.
The help page for pnorm accessed through ?pnorm() indicates that the usage is:
pnorm(q, mean = 0, sd = 1, lower.tail = TRUE, log.p = FALSE).
My professor also says that I am ignoring the mean and sd by just using pnorm(z-score). I feel like it is just easier to type in one value instead of the whole set of arguments. So I experimented and found that
1-pnorm((5-4.35)/0.59) = 1-pnorm(5,4.35,0.59)
So it looks like pnorm(z-score) = pnorm (x,μ,σ).
Is there a reason that using the z-score allows to skip the mean and
standard deviation in the pnorm function?
I have also noticed that trying to add μ,σ arguments with the z-score gives the wrong answer (ex: pnorm(z-score,μ,σ).
> 1-pnorm((5-4.35)/0.59)
[1] 0.1352972
> pnorm(5,4.35,0.59)
[1] 0.8647028
> 1-pnorm(5,4.35,0.59)
[1] 0.1352972
> 1-pnorm((5-4.35)/0.59,4.35,0.59)
[1] 1
That is because a z-score is standard normally distributed, meaning it has μ = 0 and σ = 1, which, as you found out, are the default parameters for pnorm().
The z-score is just the transformation of any normally distributed value to a standard normally distributed one.
So when you output the probability of the z-score for x = 5 you indeed get the same value than asking for the probability of x > 5 in a normal distribution with μ = 4.35 and σ = 0.59.
But when you add μ = 4.35 and σ = 0.59 to your z-score inside pnorm() you get it all wrong, because you're looking for a standard normally distributed value in a different distribution.
pnorm() (to answer your first question) calculates the cumulative density function, which shows you P(X < x) (the probability that a random variable takes a value equal or less than x). That's why you do 1 - pnorm(..) to find out P(X > x).

R: Robust fitting of data points to a Gaussian function

I need to do some robust data-fitting operation.
I have bunch of (x,y) data, that I want to fit to a Gaussian (aka normal) function.
The point is, I want to remove the ouliers. As one can see on the sample plot below, there is another distribution of data thats pollutting my data on the right, and I don't want to take it into account to do the fitting (i.e. to find \sigma, \mu and the overall scale parameter).
R seems to be the right tool for the job, I found some packages (robust, robustbase, MASS for example) that are related to robust fitting.
However, they assume the user already has a strong knowledge of R, which is not my case, and the documentation is only provided as a sort of reference manual, no tutorial or equivalent. My statistical background is rather low, I attempted to read reference material on fitting with R, but it didn't really help (and I'm not even sure thats the right way to go).
But I have the feeling that this is actually a quite simple operation.
I have checked this related question (and the linked ones), however they take as input a single vector of values, and I have a vector of pairs, so I don't see how to transpose.
Any help on how to do this would be appreciated.
Fitting a Gaussian curve to the data, the principle is to minimise the sum of squares difference between the fitted curve and the data, so we define f our objective function and run optim on it:
fitG =
function(x,y,mu,sig,scale){
f = function(p){
d = p[3]*dnorm(x,mean=p[1],sd=p[2])
sum((d-y)^2)
}
optim(c(mu,sig,scale),f)
}
Now, extend this to two Gaussians:
fit2G <- function(x,y,mu1,sig1,scale1,mu2,sig2,scale2,...){
f = function(p){
d = p[3]*dnorm(x,mean=p[1],sd=p[2]) + p[6]*dnorm(x,mean=p[4],sd=p[5])
sum((d-y)^2)
}
optim(c(mu1,sig1,scale1,mu2,sig2,scale2),f,...)
}
Fit with initial params from the first fit, and an eyeballed guess of the second peak. Need to increase the max iterations:
> fit2P = fit2G(data$V3,data$V6,6,.6,.02,8.3,0.10,.002,control=list(maxit=10000))
Warning messages:
1: In dnorm(x, mean = p[1], sd = p[2]) : NaNs produced
2: In dnorm(x, mean = p[4], sd = p[5]) : NaNs produced
3: In dnorm(x, mean = p[4], sd = p[5]) : NaNs produced
> fit2P
$par
[1] 6.035610393 0.653149616 0.023744876 8.317215066 0.107767881 0.002055287
What does this all look like?
> plot(data$V3,data$V6)
> p = fit2P$par
> lines(data$V3,p[3]*dnorm(data$V3,p[1],p[2]))
> lines(data$V3,p[6]*dnorm(data$V3,p[4],p[5]),col=2)
However I would be wary about statistical inference about your function parameters...
The warning messages produced are probably due to the sd parameter going negative. You can fix this and also get a quicker convergence by using L-BFGS-B and setting a lower bound:
> fit2P = fit2G(data$V3,data$V6,6,.6,.02,8.3,0.10,.002,control=list(maxit=10000),method="L-BFGS-B",lower=c(0,0,0,0,0,0))
> fit2P
$par
[1] 6.03564202 0.65302676 0.02374196 8.31424025 0.11117534 0.00208724
As pointed out, sensitivity to initial values is always a problem with curve fitting things like this.
Fitting a Gaussian:
# your data
set.seed(0)
data <- c(rnorm(100,0,1), 10, 11)
# find & remove outliers
outliers <- boxplot(data)$out
data <- setdiff(data, outliers)
# fitting a Gaussian
mu <- mean(data)
sigma <- sd(data)
# testing the fit, check the p-value
reference.data <- rnorm(length(data), mu, sigma)
ks.test(reference.data, data)

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