""" oct 2009 - multiple output files Dear Matthias, Yes, you can define number of outputs dynamically in Galaxy. For doing this, you'll have to declare one output dataset in your xml and pass its ID ($out_file.id) to your python script. Also, set force_history_refresh="True" in your tool tag in xml, like this: In your script, if your outputs are named in the following format, primary_associatedWithDatasetID_designation_visibility_extension (_DBKEY), all your datasets will show up in the history pane. associatedWithDatasetID is the $out_file.ID passed from xml, designation will be a unique identifier for each output (set in your script), visibility can be set to visible if you want the dataset visible in your history, or notvisible otherwise extension is the required format for your dataset (bed, tabular, fasta etc) DBKEY is optional, and can be set if required (e.g. hg18, mm9 etc) One of our tools "MAF to Interval converter" (tools/maf/ maf_to_interval.xml) already uses this feature. You can use it as a reference. qq.chisq Quantile-quantile plot for chi-squared tests Description This function plots ranked observed chi-squared test statistics against the corresponding expected order statistics. It also estimates an inflation (or deflation) factor, lambda, by the ratio of the trimmed means of observed and expected values. This is useful for inspecting the results of whole-genome association studies for overdispersion due to population substructure and other sources of bias or confounding. Usage qq.chisq(x, df=1, x.max, main="QQ plot", sub=paste("Expected distribution: chi-squared (",df," df)", sep=""), xlab="Expected", ylab="Observed", conc=c(0.025, 0.975), overdisp=FALSE, trim=0.5, slope.one=FALSE, slope.lambda=FALSE, thin=c(0.25,50), oor.pch=24, col.shade="gray", ...) Arguments x A vector of observed chi-squared test values df The degreees of freedom for the tests x.max If present, truncate the observed value (Y) axis here main The main heading sub The subheading xlab x-axis label (default "Expected") ylab y-axis label (default "Observed") conc Lower and upper probability bounds for concentration band for the plot. Set this to NA to suppress this overdisp If TRUE, an overdispersion factor, lambda, will be estimated and used in calculating concentration band trim Quantile point for trimmed mean calculations for estimation of lambda. Default is to trim at the median slope.one Is a line of slope one to be superimpsed? slope.lambda Is a line of slope lambda to be superimposed? thin A pair of numbers indicating how points will be thinned before plotting (see Details). If NA, no thinning will be carried out oor.pch Observed values greater than x.max are plotted at x.max. This argument sets the plotting symbol to be used for out-of-range observations col.shade The colour with which the concentration band will be filled ... Further graphical parameter settings to be passed to points() Details To reduce plotting time and the size of plot files, the smallest observed and expected points are thinned so that only a reduced number of (approximately equally spaced) points are plotted. The precise behaviour is controlled by the parameter thin, whose value should be a pair of numbers. The first number must lie between 0 and 1 and sets the proportion of the X axis over which thinning is to be applied. The second number should be an integer and sets the maximum number of points to be plotted in this section. The "concentration band" for the plot is shown in grey. This region is defined by upper and lower probability bounds for each order statistic. The default is to use the 2.5 Note that this is not a simultaneous confidence region; the probability that the plot will stray outside the band at some point exceeds 95 When required, he dispersion factor is estimated by the ratio of the observed trimmed mean to its expected value under the chi-squared assumption. Value The function returns the number of tests, the number of values omitted from the plot (greater than x.max), and the estimated dispersion factor, lambda. Note All tests must have the same number of degrees of freedom. If this is not the case, I suggest transforming to p-values and then plotting -2log(p) as chi-squared on 2 df. Author(s) David Clayton hdavid.clayton@cimr.cam.ac.uki References Devlin, B. and Roeder, K. (1999) Genomic control for association studies. Biometrics, 55:997-1004 """ import sys, random, math, copy,os, subprocess, tempfile from rgutils import RRun, rexe rqq = """ # modified by ross lazarus for the rgenetics project may 2000 # makes a pdf for galaxy from an x vector of chisquare values # from snpMatrix # http://www.bioconductor.org/packages/bioc/html/snpMatrix.html qq.chisq <- function(x, df=1, x.max, main="QQ plot", sub=paste("Expected distribution: chi-squared (",df," df)", sep=""), xlab="Expected", ylab="Observed", conc=c(0.025, 0.975), overdisp=FALSE, trim=0.5, slope.one=T, slope.lambda=FALSE, thin=c(0.5,200), oor.pch=24, col.shade="gray", ofname="qqchi.pdf", h=6,w=6,printpdf=F,...) { # Function to shade concentration band shade <- function(x1, y1, x2, y2, color=col.shade) { n <- length(x2) polygon(c(x1, x2[n:1]), c(y1, y2[n:1]), border=NA, col=color) } # Sort values and see how many out of range obsvd <- sort(x, na.last=NA) N <- length(obsvd) if (missing(x.max)) { Np <- N } else { Np <- sum(obsvd<=x.max) } if(Np==0) stop("Nothing to plot") # Expected values if (df==2) { expctd <- 2*cumsum(1/(N:1)) } else { expctd <- qchisq(p=(1:N)/(N+1), df=df) } # Concentration bands if (!is.null(conc)) { if(conc[1]>0) { e.low <- qchisq(p=qbeta(conc[1], 1:N, N:1), df=df) } else { e.low <- rep(0, N) } if (conc[2]<1) { e.high <- qchisq(p=qbeta(conc[2], 1:N, N:1), df=df) } else { e.high <- 1.1*rep(max(x),N) } } # Plot outline if (Np < N) top <- x.max else top <- obsvd[N] right <- expctd[N] if (printpdf) {pdf(ofname,h,w)} plot(c(0, right), c(0, top), type="n", xlab=xlab, ylab=ylab, main=main, sub=sub) # Thinning if (is.na(thin[1])) { show <- 1:Np } else if (length(thin)!=2 || thin[1]<0 || thin[1]>1 || thin[2]<1) { warning("invalid thin parameter; no thinning carried out") show <- 1:Np } else { space <- right*thin[1]/floor(thin[2]) iat <- round((N+1)*pchisq(q=(1:floor(thin[2]))*space, df=df)) if (max(iat)>thin[2]) show <- unique(c(iat, (1+max(iat)):Np)) else show <- 1:Np } Nu <- floor(trim*N) if (Nu>0) lambda <- mean(obsvd[1:Nu])/mean(expctd[1:Nu]) if (!is.null(conc)) { if (Np0) { key <- c(key, line.types[2]) txt <- c(txt, paste("y = ", format(lambda, digits=4), "x", sep="")) if (!is.null(conc)) { if (Np maxveclen: # now have half a million markers eg - too many to plot all for a pdf - sample to get 10k or so points # oversample part of the distribution always = min(1000,nrows/20) # oversample smaller of lowest few hundred items or 5% skip = int(nrows/float(maxveclen)) # take 1 in skip to get about maxveclen points if skip <= 1: skip = 2 samplei = [i for i in range(nrows) if (i < always) or (i % skip == 0)] # always oversample first sorted (here lowest) values yvec = [dat[i] for i in samplei] # always get first and last xvec = [unifx[i] for i in samplei] # and sample xvec same way maint='QQ %s (random %d of %d)' % (title,len(yvec),nrows) else: yvec = [x for x in dat] maint='QQ %s (n=%d)' % (title,nrows) xvec = unifx if logscale: maint = 'Log%s' % maint mx = [0,math.log10(nrows)] # if 1000, becomes 3 for the null line ylab = '-log10(%s) Quantiles' % title xlab = '-log10(Uniform 0-1) Quantiles' yvec = [-math.log10(x) for x in yvec if x > 0.0] else: mx = [0,1] ylab = '%s Quantiles' % title xlab = 'Uniform 0-1 Quantiles' xv = ['%f' % x for x in xvec] R.append('xvec = c(%s)' % ','.join(xv)) yv = ['%f' % x for x in yvec] R.append('yvec = c(%s)' % ','.join(yv)) R.append('mx = c(0,%f)' % (math.log10(fn))) R.append('pdf("%s",h=%d,w=%d)' % (fname,h,w)) R.append("par(lab=c(10,10,10))") R.append('qqplot(xvec,yvec,xlab="%s",ylab="%s",main="%s",sub="%s",pch=19,col="%s",cex=0.8)' % (xlab,ylab,maint,title,colour)) R.append('points(mx,mx,type="l")') R.append('grid(col="lightgray",lty="dotted")') R.append('dev.off()') RRun(rcmd=R,title='makeQQplot',outdir=outdir) def main(): u = """ """ u = """ rgQQ.py "$input1" "$name" $sample "$cols" $allqq $height $width $logtrans $allqq.id $__new_file_path__ """ print >> sys.stdout,'## rgQQ.py. cl=',sys.argv npar = 11 if len(sys.argv) < npar: print >> sys.stdout, '## error - too few command line parameters - wanting %d' % npar print >> sys.stdout, u sys.exit(1) in_fname = sys.argv[1] name = sys.argv[2] sample = float(sys.argv[3]) head = None columns = [int(x) for x in sys.argv[4].strip().split(',')] # work with python columns! allout = sys.argv[5] height = int(sys.argv[6]) width = int(sys.argv[7]) logscale = (sys.argv[8].lower() == 'true') outid = sys.argv[9] # this is used to allow multiple output files outdir = sys.argv[10] nan_row = False rows = [] for i, line in enumerate( file( sys.argv[1] ) ): # Skip comments if line.startswith( '#' ) or ( i == 0 ): if i == 0: head = line.strip().split("\t") continue if len(line.strip()) == 0: continue # Extract values and convert to floats fields = line.strip().split( "\t" ) row = [] nan_row = False for column in columns: if len( fields ) <= column: return fail( "No column %d on line %d: %s" % ( column, i, fields ) ) val = fields[column] if val.lower() == "na": nan_row = True else: try: row.append( float( fields[column] ) ) except ValueError: return fail( "Value '%s' in column %d on line %d is not numeric" % ( fields[column], column+1, i ) ) if not nan_row: rows.append( row ) if i > 1: i = i-1 # remove header row from count if head == None: head = ['Col%d' % (x+1) for x in columns] R = [] for c,column in enumerate(columns): # we appended each column in turn outname = allout if c > 0: # after first time outname = 'primary_%s_col%s_visible_pdf' % (outid,column) outname = os.path.join(outdir,outname) dat = [] nrows = len(rows) # sometimes lots of NA's!! for arow in rows: dat.append(arow[c]) # remember, we appended each col in turn! cname = head[column] makeQQ(dat=dat,sample=sample,fname=outname,title='%s_%s' % (name,cname), xvar=cname,h=height,w=width,logscale=logscale,outdir=outdir) if __name__ == "__main__": main()