コード例 #1
0
ファイル: distrib.py プロジェクト: astrofanlee/project_TL
def expy(d):
    colors = ['b','g','r','c','m','y','k','b--','g--','r--','c--','m--','y--']
    multi = 2.**N.arange(2,3.1,1.)
    #multi = [77.]
    for i in range(len(multi)):
        dinflate = N.exp((d)*multi[i])-1.
        k,p = power.pk(dinflate)

        var = N.var((d)*multi[i])
        lognocor = ((N.exp(var)-1)*N.exp(var)/var)
        lognovar = (N.exp(var)-1)*N.exp(var)
        print 1+2*var,'lognocor:',lognocor
        #varlog = N.var(N.log(dinflate+1.).flatten())
        k,plog = power.pk(N.log(dinflate+1))
        print p[0]/plog[0], p[-1]/plog[-1]

        #M.subplot(121)
        M.loglog(k,p/plog/lognocor,colors[i])
        #M.subplot(122)

        #M.loglog(k,plog,colors[i])
        #M.loglog([k[0],k[-1]],[lognovar,lognovar],colors[i])
        #M.loglog(k,1./plog**mul,colors[i])
        

    
    #preal = M.load('mill/s63/pm.pnl.dat')
    #plogreal = M.load('mill/s63/plogm.pnl.dat')    
    #M.loglog(preal[:,0],preal[:,1]/plogreal[:,1],'b')

    #M.xlabel(r'$k\ [\rm{Mpc}/h]$',fontsize=20)
    #M.ylabel(r'$P_\delta(k)/P_{\log (1+\delta)}(k)$',fontsize=20)

    M.show()
コード例 #2
0
ファイル: distrib.py プロジェクト: astrofanlee/project_TL
def logskew(d,floors = [],col='',divvypk=[]):
    maxd = max(d.flatten())
    if len(floors) == 0:
        floors = 1./maxd * 2.**N.arange(-5,5.01,1.)
    print floors

    for fl in floors:
        dcopy = 1.*d
        wltf = N.where(dcopy < fl)
        dcopy[wltf] = 0.*dcopy[wltf] + fl

        logrho = N.log(dcopy)
        var  = N.var(decreaseres(logrho,f=16).flatten())
        #skew = SS.skew(logrho.flatten())
        #print fl,'log:',var,'lin:',N.var(dcopy.flatten())
        print fl,'log:',var#,SS.skew(dcopy.flatten())

        k,pk = power.pk(logrho)

        if (len(divvypk) > 0):
            M.loglog(k,pk/divvypk/var,col)

    if (len(divvypk) == 0):
        return pk,pk/var
    else:
        return
コード例 #3
0
ファイル: distrib.py プロジェクト: astrofanlee/project_TL
def gaussy(d):
    colors = ['b','g','r','c','m','y','b--','g--','r--','c--','m--','y--']
    multi = 2.**N.arange(0,4.1,1)

    M.clf()

    for i in range(len(multi)):
        dinflate = (d-1.)*multi[i]
        k,p = power.pk(dinflate)
        w0 = N.where(dinflate <=-0.9999)
        dinflate[w0] = dinflate[w0]*0. -0.9999
        k,plog = power.pk(N.log(dinflate+1.))
        print p[0]/plog[0], p[-1]/plog[-1]

        M.loglog(k,p/plog,colors[i])

    M.show()
コード例 #4
0
ファイル: Fisher.py プロジェクト: ARepp/Fisher
cdNu2 = CIC.getDemNu(mapNu2)
cdNu2 = N.double(cdNu2)
den2 = N.sum(cdNu2)/2000.**3
npix = N.size(cdNu2.flat)
cdNu2 = cdNu2/((N.sum(cdNu2))/npix) #turn into a density field

print N.var(cdNu1)
print N.var(cdNu2)
print N.var(N.log(cdNu1))
print N.var(N.log(cdNu2))

"""
Calculate Power spectrum
"""
print 'Power spectrum min mass'
Pow.pk(cdNu1, boxsize=2000., filename='PkNu17z0.txt')
out = N.loadtxt(open('./Output/PkNu17z0.txt'))
kmin = out[:,0]
Pkmin = out[:,1]
print 'Log power spectrum min mass'
Pow.pk(N.log(cdNu1), boxsize=2000., filename='PklogNu17z0.txt') 
out = N.loadtxt(open('./Output/PklogNu17z0.txt'))
klogmin = out[:,0]
Pklogmin = out[:,1]

print 'Power spectrum max mass'
Pow.pk(cdNu2, boxsize=2000., filename='PkNu30z0.txt')
out = N.loadtxt(open('./Output/PkNu30z0.txt'))
kmax = out[:,0]
Pkmax = out[:,1]
print 'Log power spectrum max mass'