ANGSD: Analysis of next generation Sequencing Data

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This method will estimate the site frequency spectrum, the method is described in [[Nielsen2012]].
Latest version can now do bootstrapping. Folding should now be done in realSFS and not in the saf file generation.


This is a 2 step procedure first generate a ".saf" file, followed by an optimization of the .saf file which will estimate the Site frequency spectrum.
=Quick Start=
The process of estimating the SFS and multidimensional has improved a lot in the newer versions.


For the optimization we have implemented 2 different approaches both found in the misc subdir of the root subdir.This is shown in the diagram below.
Assuming you have a bam/cram file list in the file 'file.list' and you have your ancestral state in ancestral.fasta, then the process is:


<pre>
<pre>
NB the ancestral state needs to be supplied for the full SFS, but you can use the -fold 1 to estimate the folded SFS and then use the reference as ancestral.
#no filtering
./angsd -gl 1 -anc ancestral -dosaf 1
#or alot of filtering
./angsd -gl 1 -anc ancestral -dosaf 1 -baq 1 -C 50 -minMapQ 30 -minQ 20


The information on this page relates to versions 0.570 or higher.
#this will generate 3 files
1) angsdput.saf.idx 2) angsdput.saf.pos.gz 3) angsdput.saf.gz
#these are binary files that are formally defined in https://github.com/ANGSD/angsd/blob/newsaf/doc/formats.pdf
 
#To find the global SFS based on the run from above simply do
./realSFS angsdput.saf.idx
##or only use chromosome 22
./realSFS angsdput.saf.idx -r 22
 
## or specific regions
./realSFS angsdput.saf.idx -r 22:100000-150000000
 
##or limit to a fixed number of sites
./realSFS angsdput.saf.idx -r 17 -nSites 10000000
 
##or you can find the 2dim sf by
./realSFS ceu.saf.idx yri.saf.idx
##NB the program will find the intersect internally. No need for multiple runs with angsd main program.
 
##or you can find the 3dim sf by
./realSFS ceu.saf.idx yri.saf.idx MEX.saf.idx
</pre>
 
=SFS=
This method will estimate the site frequency spectrum, the method is described in [[Nielsen2012]]. The theory behind the model is briefly described [[realSFSmethod|here]]
 
This is a 2 step procedure first generate a ".saf" file (site allele frequency likelihood), followed by an optimization of the .saf file which will estimate the Site frequency spectrum (SFS).
 
For the optimization we have implemented 2 different approaches both found in the misc folder. The diagram below shows the how the method goes from raw bam files to the SFS.  
 
You can also estimate a [[2d SFS Estimation| 2dsfs]] or even higher if you want to.
<pre>
* NB the ancestral state needs to be supplied for the full SFS, but you can use the -fold 1 to estimate the folded SFS and then use the reference as ancestral.
* NB the output from the -doSaf 2 are not sample allele frequency likelihoods but sample alle posteriors.
And applying the realSFS to this output is therefore NOT the ML estimate of the SFS as described in the Nielsen 2012 paper,
but the 'Incorporating deviations from Hardy-Weinberg Equilibrium (HWE)' section of that paper.


In earlier version -doSaf was called -realSFS
</pre>
</pre>
<classdiagram type="dir:LR">
 
[sequence data{bg:orange}]->GL[genotype likelihoods|SAMtools;GATK;SOAPsnp;Kim et.al]
{{#mermaid:graph LR;
[genotype likelihoods|SAMtools;GATK;SOAPsnp;Kim et.al]->doSaf[.saf file{bg:blue}]
    A[sequence data] --> B[genotype likelihoods<br/>- SAMtools<br/>- GATK<br/>- SOAPsnp<br/>- Kim et.al]
[.saf file{bg:blue}]->optimize('emOptim2')[.saf.ml file{bg:red}]
    B -->|doSaf| C[.saf file]
</classdiagram>
    C -->|optimize realSFS| D[.saf.ml file]
 
    class A sequenceData;
    class B genotypeLikelihoods;
    class C safFile;
    class D safMlFile;
 
    classDef sequenceData fill:#FFA500;
    classDef genotypeLikelihoods fill:#FFFFFF;
    classDef safFile fill:#009FFF;
    classDef safMlFile fill:#FF0000;
}}
 


=Brief Overview=
=Brief Overview=
<pre>
<pre>
./angsd -doSaf
./angsd -dosaf
-> angsd version: 0.569 build(Dec 17 2013 12:40:00)
-> angsd version: 0.935-44-g02a07fc-dirty (htslib: 1.12-1-g9672589) build(Jul  8 2021 08:04:55)
-> ./angsd -dosaf
-> Analysis helpbox/synopsis information:
-> Analysis helpbox/synopsis information:
-> Wed Aug 18 11:09:03 2021
-> doMcall=0
--------------
--------------
angsd_realSFS.cpp:
abcSaf.cpp:
-doSaf 0
-doSaf 0
1: perform multisample GL estimation
1: perform multisample GL estimation
2: use an inbreeding version
2: use an inbreeding version
3: calculate genotype probabilities
3: calculate genotype probabilities (use -doPost 3 instead)
4: Assume genotype posteriors as input (still beta)  
4: Assume genotype posteriors as input (still beta)  
-doThetas 0 (calculate thetas)
-underFlowProtect 0
-underFlowProtect 0
-fold 0 (deprecated)
-anc (null) (ancestral fasta)
-anc (null) (ancestral fasta)
-noTrans 0 (remove transitions)
-noTrans 0 (remove transitions)
-pest (null) (prior SFS)
-pest (null) (prior SFS)
-isHap 0 (is haploid beta!)
-doPost 0 (doPost 3,used for accesing saf based variables)
NB:
  If -pest is supplied in addition to -doSaf then the output will then be posterior probability of the sample allelefrequency for each site
</pre>


<pre>
misc/realSFS
./realSFS afile.saf.idx [-start FNAME -P nThreads -tole tole -maxIter  -nSites ]
</pre>
</pre>
For information and parameters concerning the realSFS subprogram go here: [[realSFS]]


=Options=
=Options=
;-doSaf 1: an saf file will be generated.
;-doSaf 1: Calculate the Site allele frequency likelihood based on individual genotype likelihoods assuming HWE


;-doSaf 2:(version above 0.503) Taking into account perIndividual inbreeding coefficients. This is the work of Filipe G. Vieira
;-doSaf 2:(version above 0.503) Calculate per site posterior probabilities of the  site allele frequencies based on individual genotype likelihoods while taking into account individual inbreeding coefficients. This is implemented by Filipe G. Vieira.  You need to supply a file containing all the inbreeding coefficients. -indF. Consider if you want to either get the MAP estimate by using all sites, or get the standardized values by conditioning on the called snpsites. See bottom of this page for examples.


;-doSaf 3: Calculate genotype probabilities  
;-doSaf 3: Calculate the genotype posterior probabilities for all samples forall sites, using an estimate of the sfs (sample allele frequency distribution). This needs a prior distribution of the SFS (which can be obtained from -doSaf 1/realSFS).
 
;-doSaf 4: Assume genotype probs as intput (beta)
 
For the inbreeding version you need to supply a file containing all the inbreeding coefficients. -indF


;-doSaf 4: Calculate the posterior probabilities of the sample allele frequency distribution for each site based on genotype probabilities. The genotype probabilities should be provided by the using using the -beagle options. Often the genotype probabilities will be obtained by haplotype imputation.


;-underFlowProtect [INT]  
;-underFlowProtect [INT]  
a very basic underflowprotection
0: (default) no underflow protection. 1: use underflow protection. For large data sets (large number of individuals) underflow projection is needed.
 


=Output file=
The output file from the ''-doSaf'' is described in detail in angsd/doc/formats.pdf. These binary annoying files can be printed with
<pre>
realSFS print myfile.saf.idx
#or
realSFS print mayflies.saf.idx -r chr1:10000-20000
</pre>
==Example==
==Example==
A full example is shown below, here we use GATK genotype likelihoods and hg19.fa as the ancestral. The [[emOptim2]] can be found in the misc subfolder.
A full example is shown below where we use the test data that can be found on the [[quick start]] page. In this example we use GATK genotype likelihoods.


first generate .saf file  with 4 threads
<pre>
./angsd -bam bam.filelist -doSaf 1 -out small -anc  chimpHg19.fa -GL 2 -P 4
</pre>
We always recommend that you filter out the bad qscore bases and meaningless mapQ reads. eg '''-minMapQ 1 -minQ 20'''. So the above analysis with these filters can be written as:
<pre>
<pre>
#first generate .saf file
./angsd -bam bam.filelist -doSaf 1 -out small -anc chimpHg19.fa -GL 2 -P 4 -minMapQ 1 -minQ 20
./angsd -bam smallBam.filelist -doSaf 1 -out small -anc hg19.fa -GL 2 [options]
#now try the EM optimization with 4 threads
./emOptim2 small.saf 20 -maxIter 100 -P 4 >small.saf.em.ml
</pre>
</pre>
We always recommend that you filter out the bad qscore bases and meaningless mapQ reads. eg '''-minMapQ 1 -minQ 20'''.
Obtain a maximum likelihood estimate of the SFS using EM algorithm
<pre>
<pre>
If you have say 10 diploid samples, then you should do -nChr 20
misc/realSFS small.saf.idx -maxIter 100 -P 4 >small.sfs
if you have say 12 diploid samples, then you should do -nChr 24.
</pre>
</pre>


=Interpretation of output file=
[[File:SfsSmall.png|thumb]]
 
The outpiles are then called small.em.ml. This will be the SFS in logscale.
This is to be interpreted as:
 
column1 := probabilty of sampling zero derived alleles
 
column2 := probabilty of sampling one derived allele
 
column3 := probabilty of sampling two derived allele
 
column4 := probabilty of sampling three derived allele


etc
A plot of this figure are seen on the right. The jaggedness is due to the very low number of sites in this small dataset.


=Interpretation of the output file=
Each row is a region of the genome (see below).
Each row is the expected values of the SFS.
==NB==
==NB==
The generation of the .saf file is done on a persite basis, whereas the optimization requires information for a region of the genome. The optimization will therefore use large amounts of memory.
The generation of the .saf file contains a saf for each site, whereas the optimization requires information for a region of the genome. The optimization will therefore use large amounts of memory.
The program defaults to 50megabase regions, and will loop over the genome using 50 megebase chunks. You can increase this adding -nSites 500000000. Which will then use 500megabase regions.


=Folded spectra=
=Folded spectra=
<pre>
If you don't have the ancestral state, you can instead estimate the folded SFS. This is done by supplying the -anc with the reference genome and applying -fold 1 to realSFS.
Below is for version 0.556 and above
 
</pre>
If you don't have the ancestral state, you can instead estimate the folded SFS. This is done by supplying the -anc with the reference and also supply -fold 1.
Then you should remember to change the second parameter to the emOptim2 function as the number of individuals instead of the number of chromosomes.


The above example would then be
The above example would then be
Line 100: Line 152:
<pre>
<pre>
#first generate .saf file
#first generate .saf file
./angsd -bam smallBam.filelist -doSaf 1 -out small -anc  hg19.fa -GL 2 -fold 1 [options]
./angsd -bam bam.filelist -doSaf 1 -out smallFolded -anc  chimpHg19.fa -GL 2
#now try the EM optimization with 4 threads
#now try the EM optimization with 4 threads
./emOptim2 small.saf 10 -maxIter 100 -P 4 >small.saf.em.ml
misc/realSFS smallFolded.saf.idx -maxIter 100 -P 4 >smallFolded.sfs
#in R
sfs<-scan("smallFolded.sfs")
barplot(sfs[-1])
</pre>
</pre>
[[File:SmallFolded.png|thumb]]
=Posterior of the per-site distributions of the sample allele frequency=
If you supply a prior for the SFS (which can be obtained from the -doSaf/realSFS analysis), the output of the .saf file will no longer be  site allele frequency likelihoods but instead will be the log posterior probability of the sample allele frequency for each site in logspace.
=Format specification of binary .saf* files=
This can be found in the angsd/doc/formats.pdf
* If the -fold 1 has been set, then the dimension is no longer 2*nInd+1 but nInd+1 (this is deprecated)
* If the -pest parameter has been supplied the output is no longer likelihoods but log posterior site allele frequencies


=Posterior per-site distributions of the sample allele frequency=
=Bootstrapping=
This is assuming version 0.556 or higher.
We have recently added the possibility to bootstrap the SFS. Which can be very usefull for getting confidence intervals of the estimated SFS.
If you supply a prior for the -doSaf analysis, the output of the .saf file will no longer be loglikeratios of the different categories but log posteriors of the different categories.


=Format specification of binary .saf file=
This is done by:
The information in this section is only usefull for people who wants to work with the "multisample GL"/"sample allele frequencies" for the individual sites.


Assuming 'n' individuals we have (2n+1) categories for each site, each value is encoded as ctype double which on 'all known' platforms occupies 8 bytes. The (2n+1) values are log scaled like ratios, which means that the most likely category will have a value of 0.
<pre>
realSFS pop.saf.idx -bootstrap 100 -P number_of_cores
</pre>
The program will then get you 100 estimates of SFS, based on data that has been subsampled with replacement.
 
=How to plot=
Assuming the we have obtained a single global sfs(only one line in the output) from '''realSFS''' program, and this is located in '''file.saf.sfs''', then we can plot the results simply like:
<pre>
sfs<-(scan("small.sfs")) #read in the log sfs
barplot(sfs[-c(1,length(sfs))]) #plot variable sites
</pre>
[[File:SfsSmall.png|thumb]]
We can make it more fancy like below:


The information for the first site is the first (2n+1)sizeof(double) bytes. The information for the next site is the next (2n+1) bytes etc. The positions are given by the ascii file called '.saf.pos'
<pre>
#function to normalize
norm <- function(x) x/sum(x)
#read data
sfs <- (scan("small.sfs"))
#the variability as percentile
pvar<- (1-sfs[1]-sfs[length(sfs)])*100
#the variable categories of the sfs
sfs<-norm(sfs[-c(1,length(sfs))])
barplot(sfs,legend=paste("Variability:= ",round(pvar,3),"%"),xlab="Chromosomes",
names=1:length(sfs),ylab="Proportions",main="mySFS plot",col='blue')
</pre>
[[File:SfsSmallFine.png|thumb]]


If your output from '''realSFS''' contains more than one line, it is because you have estimated multiple local SFS's. Then you can't use the above commands directly but should first pick a specific row.


<pre>
<pre>
#sample code to read .saf in c/c++ assuming 10 individuals
sfs<-(as.numeric(read.table("multiple.sfs")[1,])) #first region.
FILE *fp = fopen("mySFS.saf","rb");
#do the above
int nInd = 10;
sfs<-(as.numeric(read.table("multiple.sfs")[2,])) #second region.
double persite[2*nInd+1];
fread(persite,sizeof(double)*(2*nInd+1),1,fp);
for(int i=0;i<2*nind+1;i++)
  fprintf(stderr,"cat: %d = %f\n",i,persite[i]);
</pre>
</pre>


* If the -fold 1 has been set, then the dimension is no longer 2*nInd+1 but nInd+1
=Which genotype likelihood model should I choose ?=
* If the -pest parameter has been supplied the output is no longer like ratios to the most likely but log posts of the different categories.
It depends on the data. As shown on this example [[Glcomparison]], there was a huge difference between '''-GL 1''' and '''-GL 2''' for older 1000genomes BAM files, but little difference for newer bam files.
=Theory=
=Validation=
The validation is based on the pre 0.900 version
==-doSaf 1==
<pre>
<pre>
We will try to elaborate on the theory behind the methods. Below is only a preliminary version of the theory.
cd misc;
./supersim -outfiles test -npop 1 -nind 12 -pvar 0.9 -nsites 50000
echo testchr1 100000 >test.fai
../angsd -fai test.fai -glf test.glf.gz -nind 12 -doSaf 1 -issim 1
./realSFS angsdput.saf 24 2>/dev/null >res
cat res
31465.429798 4938.453115 2568.586388 1661.227445 1168.891114 975.302535 794.727537 632.691896 648.223566 546.293853 487.936192 417.178505 396.200026 409.813797 308.434836 371.699254 245.585920 322.293532 282.980046 292.584975 212.845183 196.682483 221.802128 236.221205 197.914673
</pre>
</pre>
This method is described in [[Nielsen2012]].
==SFS definition==
For 'n' diploid samples, the site frequency spectrum '''(SFS)''' is the (2n+1) vector containing the proportion of site carrying 'k'-mutations. This means that the first element in the SFS is the proportion of sites where we don't observe any mutations, The second value is the proportion of sites where we observe 1 mutations. The last value is the proportion of sites we only observe mutations. It follows that the first and last column are the invariable categories and assuming that the SFS contains relative frequencies the variability in the sample can be estimated by:


<math>pvar=1-sfs_0-sfs_{2n}=\sum_{i=1}^{2n-1}sfs_i</math>
==-doSaf 2==
<pre>
ngsSim=../ngsSim/ngsSim
angsd=./angsd
realSFS=./misc/realSFS
 
$ngsSim  -npop 1 -nind 24 -nsites 1000000 -depth 4 -F 0.0 -outfiles testF0.0
$ngsSim  -npop 1 -nind 24 -nsites 1000000 -depth 4 -F 0.9 -outfiles testF0.9
 
for i in `seq 24`;do echo 0.9;done >indF
echo testchr1 250000000 >test.fai
$angsd -fai test.fai -issim 1 -glf testF0.0.glf.gz -nind 24 -out noF -dosaf 1
$angsd -fai test.fai -issim 1 -glf testF0.9.glf.gz -nind 24 -out withF -dosaf 2 -domajorminor 1 -domaf 1 -indF indF
$angsd -fai test.fai -issim 1 -glf testF0.9.glf.gz -nind 24 -out withFsnp -dosaf 2 -domajorminor 1 -domaf 1 -indF indF -snp_pval 1e-4
 
$realSFS noF.saf 48 >noF.sfs
$realSFS withF.saf 48 >withF.sfs
 
 
 
#in R
trueNoF<-scan("testF0.0.frq")
trueWithF<-scan("testF0.9.frq")
pdf("sfsFcomparison.pdf",width=14)
par(mfrow=c(1,2),width=14)
barplot(trueNoF[-1],main='true sfs F=0.0')
barplot(trueWithF[-1],main='true sfs F=0.9')
 
estWithF<-scan("withF.sfs")
estNoF<-scan("noF.sfs")


==Sample allele frequency/Multisample GL==
By supplying the -doSaf 1, flag to angsd. Angsd will calculate the likelihood of the sample allele frequency for each site and dump these into the .saf file. The likelihood of the sample allele frequency are in this context the likelihood of sampling k-derived alleles. This is estimated on the basis of the 10 possible genotype likelihoods for all individuals by summing over all combinations. This is done using the recursive algorithm described in [[Nielsen2012]]. This we write as <math>p(X^s\mid j)</math> meaning the likelihood of sampling j derived alleles for site s. And we calculate the folded as


<math>
barplot(rbind(trueNoF,estNoF)[,-1],main="true vs est SFS F=0 (ML) (all sites)",be=T,col=1:2)
p_{fold}(x^s\mid j) =p(x^s\mid j) + p(x^s\mid 2n- j),\qquad j\in\{0,1,3,\ldots,n-1\},
barplot(rbind(trueWithF,estWithF)[,-1],main='true vs est sfs=0.9 (MAP) (all sites)',be=T,col=1:2)
</math>


<math>
readBjoint <- function(file=NULL,nind=10,nsites=10){
p_{fold}(x^s\mid j) =2p(x^s\mid j) ,\qquad j=n
  ff <- gzfile(file,"rb")
</math>
  m<-matrix(readBin(ff,double(),(2*nind+1)*nsites),ncol=(2*nind+1),byrow=TRUE)
  close(ff)
  return(m)
}


==Likelihood of the SFS==
The likelihood of the sfs is then given as:


<math>
m <- exp(readBjoint("withF.saf",nind=24,5e6))
p(X|\theta) = \prod_{s=0}^S\sum_{i=0}^{2n} p(X^s\mid i )\theta_i
barplot(rbind(trueWithF,colMeans(m))[,-1],main='true vs est sfs F=0.9 (colmean of site pp) (all sites)',be=T,col=1:2)
</math>
m <- exp(readBjoint("withFsnp.saf",nind=24,5e6))
m <- colMeans(m)*nrow(m)
##m contains SFS for absolute frequencies
m[1] <-1e6-sum(m[-1])
##m now contains a corrected estimate containing the zero category
barplot(rbind(trueWithF,norm(m))[,-1],main='true vs est sfs F=0.9 (colmean of site pp) (called snp sites)',be=T,col=1:2)
 
dev.off()
 
 
</pre>
See results from above here:http://www.popgen.dk/angsd/sfsFcomparison.pdf


Here <math>\theta</math> is our sfs. In the case of the folded sfs, we use n instead of 2n in the summation. We can find the MLE of the SFS by using either an BFGS approach that uses derivatives or by using en EM algorithm. Both is implemented in the emOptim2 program.
=safv3 comparison=
Between 0.800 and 0.900 i decided to move to a better format than the raw sad files. This new format takes up half the storage and allows for easy random access and generalizes to unto 5dimensional sfs. A comparison can be found here: [[safv3]]
=Using NGStools=
See [[realSFS]] for how to convert the new safformat to the old safformat if you use NGStools.

Latest revision as of 15:22, 8 December 2023

Latest version can now do bootstrapping. Folding should now be done in realSFS and not in the saf file generation.

Quick Start

The process of estimating the SFS and multidimensional has improved a lot in the newer versions.

Assuming you have a bam/cram file list in the file 'file.list' and you have your ancestral state in ancestral.fasta, then the process is:

#no filtering
./angsd -gl 1 -anc ancestral -dosaf 1
#or alot of filtering
./angsd -gl 1 -anc ancestral -dosaf 1 -baq 1 -C 50 -minMapQ 30 -minQ 20

#this will generate 3 files
1) angsdput.saf.idx 2) angsdput.saf.pos.gz 3) angsdput.saf.gz
#these are binary files that are formally defined in https://github.com/ANGSD/angsd/blob/newsaf/doc/formats.pdf

#To find the global SFS based on the run from above simply do
./realSFS angsdput.saf.idx
##or only use chromosome 22
./realSFS angsdput.saf.idx -r 22

## or specific regions
./realSFS angsdput.saf.idx -r 22:100000-150000000

##or limit to a fixed number of sites
./realSFS angsdput.saf.idx -r 17 -nSites 10000000

##or you can find the 2dim sf by
./realSFS ceu.saf.idx yri.saf.idx
##NB the program will find the intersect internally. No need for multiple runs with angsd main program.

##or you can find the 3dim sf by
./realSFS ceu.saf.idx yri.saf.idx MEX.saf.idx

SFS

This method will estimate the site frequency spectrum, the method is described in Nielsen2012. The theory behind the model is briefly described here

This is a 2 step procedure first generate a ".saf" file (site allele frequency likelihood), followed by an optimization of the .saf file which will estimate the Site frequency spectrum (SFS).

For the optimization we have implemented 2 different approaches both found in the misc folder. The diagram below shows the how the method goes from raw bam files to the SFS.

You can also estimate a 2dsfs or even higher if you want to.

* NB the ancestral state needs to be supplied for the full SFS, but you can use the -fold 1 to estimate the folded SFS and then use the reference as ancestral.
* NB the output from the -doSaf 2 are not sample allele frequency likelihoods but sample alle posteriors.
And applying the realSFS to this output is therefore NOT the ML estimate of the SFS as described in the Nielsen 2012 paper,
but the 'Incorporating deviations from Hardy-Weinberg Equilibrium (HWE)' section of that paper.


Brief Overview

./angsd -dosaf
	-> angsd version: 0.935-44-g02a07fc-dirty (htslib: 1.12-1-g9672589) build(Jul  8 2021 08:04:55)
	-> ./angsd -dosaf 
	-> Analysis helpbox/synopsis information:
	-> Wed Aug 18 11:09:03 2021
	-> doMcall=0
--------------
abcSaf.cpp:
	-doSaf		0
	1: perform multisample GL estimation
	2: use an inbreeding version
	3: calculate genotype probabilities (use -doPost 3 instead)
	4: Assume genotype posteriors as input (still beta) 
	-underFlowProtect	0
	-anc			(null) (ancestral fasta)
	-noTrans		0 (remove transitions)
	-pest			(null) (prior SFS)
	-isHap			0 (is haploid beta!)
	-doPost			0 (doPost 3,used for accesing saf based variables)
NB:
	  If -pest is supplied in addition to -doSaf then the output will then be posterior probability of the sample allelefrequency for each site
misc/realSFS
./realSFS afile.saf.idx [-start FNAME -P nThreads -tole tole -maxIter  -nSites ]

For information and parameters concerning the realSFS subprogram go here: realSFS

Options

-doSaf 1
Calculate the Site allele frequency likelihood based on individual genotype likelihoods assuming HWE
-doSaf 2
(version above 0.503) Calculate per site posterior probabilities of the site allele frequencies based on individual genotype likelihoods while taking into account individual inbreeding coefficients. This is implemented by Filipe G. Vieira. You need to supply a file containing all the inbreeding coefficients. -indF. Consider if you want to either get the MAP estimate by using all sites, or get the standardized values by conditioning on the called snpsites. See bottom of this page for examples.
-doSaf 3
Calculate the genotype posterior probabilities for all samples forall sites, using an estimate of the sfs (sample allele frequency distribution). This needs a prior distribution of the SFS (which can be obtained from -doSaf 1/realSFS).
-doSaf 4
Calculate the posterior probabilities of the sample allele frequency distribution for each site based on genotype probabilities. The genotype probabilities should be provided by the using using the -beagle options. Often the genotype probabilities will be obtained by haplotype imputation.
-underFlowProtect [INT]

0: (default) no underflow protection. 1: use underflow protection. For large data sets (large number of individuals) underflow projection is needed.

Output file

The output file from the -doSaf is described in detail in angsd/doc/formats.pdf. These binary annoying files can be printed with

realSFS print myfile.saf.idx
#or
realSFS print mayflies.saf.idx -r chr1:10000-20000

Example

A full example is shown below where we use the test data that can be found on the quick start page. In this example we use GATK genotype likelihoods.

first generate .saf file with 4 threads

./angsd -bam bam.filelist -doSaf 1 -out small -anc  chimpHg19.fa -GL 2 -P 4

We always recommend that you filter out the bad qscore bases and meaningless mapQ reads. eg -minMapQ 1 -minQ 20. So the above analysis with these filters can be written as:

./angsd -bam bam.filelist -doSaf 1 -out small -anc chimpHg19.fa -GL 2 -P 4 -minMapQ 1 -minQ 20

Obtain a maximum likelihood estimate of the SFS using EM algorithm

misc/realSFS small.saf.idx -maxIter 100 -P 4 >small.sfs

A plot of this figure are seen on the right. The jaggedness is due to the very low number of sites in this small dataset.

Interpretation of the output file

Each row is a region of the genome (see below). Each row is the expected values of the SFS.

NB

The generation of the .saf file contains a saf for each site, whereas the optimization requires information for a region of the genome. The optimization will therefore use large amounts of memory.

Folded spectra

If you don't have the ancestral state, you can instead estimate the folded SFS. This is done by supplying the -anc with the reference genome and applying -fold 1 to realSFS.


The above example would then be

#first generate .saf file
./angsd -bam bam.filelist -doSaf 1 -out smallFolded -anc  chimpHg19.fa -GL 2
#now try the EM optimization with 4 threads
misc/realSFS smallFolded.saf.idx -maxIter 100 -P 4 >smallFolded.sfs
#in R
sfs<-scan("smallFolded.sfs")
barplot(sfs[-1])

Posterior of the per-site distributions of the sample allele frequency

If you supply a prior for the SFS (which can be obtained from the -doSaf/realSFS analysis), the output of the .saf file will no longer be site allele frequency likelihoods but instead will be the log posterior probability of the sample allele frequency for each site in logspace.

Format specification of binary .saf* files

This can be found in the angsd/doc/formats.pdf

  • If the -fold 1 has been set, then the dimension is no longer 2*nInd+1 but nInd+1 (this is deprecated)
  • If the -pest parameter has been supplied the output is no longer likelihoods but log posterior site allele frequencies

Bootstrapping

We have recently added the possibility to bootstrap the SFS. Which can be very usefull for getting confidence intervals of the estimated SFS.

This is done by:

realSFS pop.saf.idx -bootstrap 100 -P number_of_cores

The program will then get you 100 estimates of SFS, based on data that has been subsampled with replacement.

How to plot

Assuming the we have obtained a single global sfs(only one line in the output) from realSFS program, and this is located in file.saf.sfs, then we can plot the results simply like:

sfs<-(scan("small.sfs")) #read in the log sfs
barplot(sfs[-c(1,length(sfs))]) #plot variable sites 

We can make it more fancy like below:

#function to normalize
norm <- function(x) x/sum(x)
#read data
sfs <- (scan("small.sfs"))
#the variability as percentile
pvar<- (1-sfs[1]-sfs[length(sfs)])*100
#the variable categories of the sfs
sfs<-norm(sfs[-c(1,length(sfs))]) 
barplot(sfs,legend=paste("Variability:= ",round(pvar,3),"%"),xlab="Chromosomes",
names=1:length(sfs),ylab="Proportions",main="mySFS plot",col='blue')

If your output from realSFS contains more than one line, it is because you have estimated multiple local SFS's. Then you can't use the above commands directly but should first pick a specific row.

sfs<-(as.numeric(read.table("multiple.sfs")[1,])) #first region.
#do the above
sfs<-(as.numeric(read.table("multiple.sfs")[2,])) #second region.

Which genotype likelihood model should I choose ?

It depends on the data. As shown on this example Glcomparison, there was a huge difference between -GL 1 and -GL 2 for older 1000genomes BAM files, but little difference for newer bam files.

Validation

The validation is based on the pre 0.900 version

-doSaf 1

cd misc;
./supersim -outfiles test -npop 1 -nind 12 -pvar 0.9 -nsites 50000
echo testchr1 100000 >test.fai
../angsd -fai test.fai -glf test.glf.gz -nind 12 -doSaf 1 -issim 1
./realSFS angsdput.saf 24 2>/dev/null >res
cat res
31465.429798 4938.453115 2568.586388 1661.227445 1168.891114 975.302535 794.727537 632.691896 648.223566 546.293853 487.936192 417.178505 396.200026 409.813797 308.434836 371.699254 245.585920 322.293532 282.980046 292.584975 212.845183 196.682483 221.802128 236.221205 197.914673

-doSaf 2

ngsSim=../ngsSim/ngsSim
angsd=./angsd
realSFS=./misc/realSFS

$ngsSim  -npop 1 -nind 24 -nsites 1000000 -depth 4 -F 0.0 -outfiles testF0.0
$ngsSim  -npop 1 -nind 24 -nsites 1000000 -depth 4 -F 0.9 -outfiles testF0.9

for i in `seq 24`;do echo 0.9;done >indF
echo testchr1 250000000 >test.fai
$angsd -fai test.fai -issim 1 -glf testF0.0.glf.gz -nind 24 -out noF -dosaf 1
$angsd -fai test.fai -issim 1 -glf testF0.9.glf.gz -nind 24 -out withF -dosaf 2 -domajorminor 1 -domaf 1 -indF indF
$angsd -fai test.fai -issim 1 -glf testF0.9.glf.gz -nind 24 -out withFsnp -dosaf 2 -domajorminor 1 -domaf 1 -indF indF -snp_pval 1e-4

$realSFS noF.saf 48 >noF.sfs
$realSFS withF.saf 48 >withF.sfs



#in R
trueNoF<-scan("testF0.0.frq")
trueWithF<-scan("testF0.9.frq")
pdf("sfsFcomparison.pdf",width=14)
par(mfrow=c(1,2),width=14)
barplot(trueNoF[-1],main='true sfs F=0.0')
barplot(trueWithF[-1],main='true sfs F=0.9')

estWithF<-scan("withF.sfs")
estNoF<-scan("noF.sfs")


barplot(rbind(trueNoF,estNoF)[,-1],main="true vs est SFS F=0 (ML) (all sites)",be=T,col=1:2)
barplot(rbind(trueWithF,estWithF)[,-1],main='true vs est sfs=0.9 (MAP) (all sites)',be=T,col=1:2)

readBjoint <- function(file=NULL,nind=10,nsites=10){
  ff <- gzfile(file,"rb")
  m<-matrix(readBin(ff,double(),(2*nind+1)*nsites),ncol=(2*nind+1),byrow=TRUE)
  close(ff)
  return(m)
}


m <- exp(readBjoint("withF.saf",nind=24,5e6))
barplot(rbind(trueWithF,colMeans(m))[,-1],main='true vs est sfs F=0.9 (colmean of site pp) (all sites)',be=T,col=1:2)
m <- exp(readBjoint("withFsnp.saf",nind=24,5e6))
m <- colMeans(m)*nrow(m)
##m contains SFS for absolute frequencies
m[1] <-1e6-sum(m[-1])
##m now contains a corrected estimate containing the zero category
barplot(rbind(trueWithF,norm(m))[,-1],main='true vs est sfs F=0.9 (colmean of site pp) (called snp sites)',be=T,col=1:2)

dev.off()


See results from above here:http://www.popgen.dk/angsd/sfsFcomparison.pdf

safv3 comparison

Between 0.800 and 0.900 i decided to move to a better format than the raw sad files. This new format takes up half the storage and allows for easy random access and generalizes to unto 5dimensional sfs. A comparison can be found here: safv3

Using NGStools

See realSFS for how to convert the new safformat to the old safformat if you use NGStools.