bayes.py 文件源码

python
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项目:nmmn 作者: rsnemmen 项目源码 文件源码
def allplot(xb,yb,bins=30,fig=1,xlabel='x',ylabel='y'):
    """
Input:
X,Y : objects referring to the variables produced by PyMC that you want
to analyze. Example: X=M.theta, Y=M.slope.

Inherited from Tommy LE BLANC's code at astroplotlib|STSCI.
    """
    #X,Y=xb.trace(),yb.trace()
    X,Y=xb,yb

    #pylab.rcParams.update({'font.size': fontsize})
    fig=pylab.figure(fig)
    pylab.clf()

    gs = pylab.GridSpec(2, 2, width_ratios=[3,1], height_ratios=[1,3], wspace=0.07, hspace=0.07)
    scat=pylab.subplot(gs[2])
    histx=pylab.subplot(gs[0], sharex=scat)
    histy=pylab.subplot(gs[3], sharey=scat)
    #scat=fig.add_subplot(2,2,3)
    #histx=fig.add_subplot(2,2,1, sharex=scat)
    #histy=fig.add_subplot(2,2,4, sharey=scat)

    # Scatter plot
    scat.plot(X, Y,linestyle='none', marker='o', color='green', mec='green',alpha=.2, zorder=-99)

    gkde = scipy.stats.gaussian_kde([X, Y])
    x,y = numpy.mgrid[X.min():X.max():(X.max()-X.min())/25.,Y.min():Y.max():(Y.max()-Y.min())/25.]
    z = numpy.array(gkde.evaluate([x.flatten(), y.flatten()])).reshape(x.shape)
    scat.contour(x, y, z, linewidths=2)
    scat.set_xlabel(xlabel)
    scat.set_ylabel(ylabel)

    # X-axis histogram
    histx.hist(X, bins, histtype='stepfilled')
    pylab.setp(histx.get_xticklabels(), visible=False)  # no X label
    #histx.xaxis.set_major_formatter(pylab.NullFormatter()) # no X label

    # Y-axis histogram
    histy.hist(Y, bins, histtype='stepfilled', orientation='horizontal')
    pylab.setp(histy.get_yticklabels(), visible=False)  # no Y label
    #histy.yaxis.set_major_formatter(pylab.NullFormatter()) # no Y label

    #pylab.minorticks_on()
    #pylab.subplots_adjust(hspace=0.1)
    #pylab.subplots_adjust(wspace=0.1)
    pylab.draw()
    pylab.show()
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