コード例 #1
0
                              R2=R2,
                              pmesh=True,
                              abund=abund,
                              doexp=doexp,
                              mexp=mexp,
                              cc=cc,
                              stellar=stellar)[1]
    datap = pm.paint(hdictf['position'][:num], hdictf['mass'][:num])
    datapR = ft.smooth(datap, Rsm, 'fingauss')

    predicts.append(predictR[...].copy())
    datas.append(datapR[...].copy())

    for i, sg in enumerate(sgs):
        hmass, hpos = dg.scatter_catalog(hdictf['mass'],
                                         hdictf['position'],
                                         sg,
                                         seed=i)
        datasg = pm.paint(hpos[:num], hmass[:num])
        datasgR = ft.smooth(datasg, Rsm, 'fingauss')
        datasgs[i].append(datasgR[...].copy())

#####Setup
#bins = np.linspace(-3, 3, 300)
func = dg.normal
colors = ['r', 'b', 'g', 'y', 'm', 'orange', 'brown', 'k']

if doexp:
    mms = [10**8, 10**8.5, 10**9, 10**9.2, 10**9.8, 10**10][::-1]

elif stellar:
    mms = [1e6, 1e7, 1e8, 1e9, 1e10][::-1]
コード例 #2
0
ファイル: nettools.py プロジェクト: modichirag/cosmo4dv2
def gridhalos(pm,
              dpath=None,
              pos=None,
              mass=None,
              R1=None,
              R2=None,
              rank=None,
              abund=True,
              sigma=None,
              seed=123,
              pmesh=True,
              z=0,
              doexp=False,
              mexp=None,
              cc=None,
              stellar=False,
              verbose=True):
    '''Read halo file or pos/mas arrays and grid and smooth them after scattering or matching abundance or both
    The path should have folder FOF in it. 
    '''
    #Matter
    bs, nc = pm.BoxSize[0], pm.Nmesh[0]

    #Halos
    if dpath is not None:
        from nbodykit.lab import CurrentMPIComm
        CurrentMPIComm.set(
            pm.comm
        )  #WORKAROUND because BigFileCatalog ignores comm o/w. Should not need after nbodykit v0.3.4
        fofcat = BigFileCatalog(dpath + 'FOF', header='Header', comm=pm.comm)

        halopos = fofcat['PeakPosition'].compute()[1:]
        halomass = (fofcat['Mass'].compute() * 10**10)[1:]
        try:
            hvel = fofcat['CMVelocity'].compute()[1:]
        except Exception as e:
            print(e)
            print('Cannot read velocity')
            hvel = None

        if verbose: print('BigFileCatalog read')
    elif pos is not None:
        halopos = pos
        if mass is not None:
            halomass = mass
        else:
            print(
                'No halo masses given, so mass=1. Scatter and abundance not valid'
            )
            halomass = np.ones(halopos.shape[0])
            sigma = None
            abund = False
    else:
        print('Need either path of Bigfile, or catalogs')
        return None

    if abund:
        if verbose: print('Match abundance')
        halomass = mf.icdf_sampling(hmass=halomass, bs=bs, z=z)

    if stellar:
        halomass = mf.stellar_mass(halomass)

    if sigma is not None:
        print('Scatter catalog with sigma = %0.2f' % sigma)
        halomass, halopos = dg.scatter_catalog(halomass, halopos, sigma, seed)

    if doexp:
        if verbose:
            print('Doing doexp with mexp = %0.2f, cc=%0.2f' % (mexp, cc))
        halomass = mf.fmexp(halomass, mexp, cc)
    #print('In gridhalos')
    #print(rank, halomass.size)
    #print(dpath)
    if rank is not None:
        if rank > halomass.size:
            print('\nCatalog not big enough to be able to match abundance')
            print('\nDesired rank = %d, catalog size = %d' %
                  (rank, halomass.size))
            return None
        else:
            halopos = halopos[:rank + 1]
            halomass = halomass[:rank + 1]
            hvel = hvel[:rank + 1]

    halos = {'position': halopos, 'mass': halomass, 'velocity': hvel}
    if pmesh:
        halomesh = pm.paint(halopos, mass=halomass)
        hposmesh = pm.paint(halopos)
        meshdict = {'hposmesh': hposmesh.value, 'halomesh': halomesh.value}

        dkh = halomesh.r2c()

        if R1 is not None:
            hmR1mesh = ft.smooth(dkh, R1, 'fingauss')
            meshdict['hmR1mesh'] = hmR1mesh.value
        if R2 is not None:
            hmR2mesh = ft.smooth(dkh, R2, 'fingauss')
            meshdict['hmR2mesh'] = hmR2mesh.value
    else:
        meshdict = None
    return meshdict, halos
コード例 #3
0
                         predictR.value,
                         M0=M0,
                         binfit=bins,
                         c='k',
                         axin=ax,
                         func=func,
                         mbin=mbinsm,
                         retfit=True,
                         lsf='--')[0]

    fits = []
    sgs = [0.2]
    for i, sg in enumerate(sgs):

        hmass, hpos = dg.scatter_catalog(hdictf['mass'],
                                         hdictf['position'],
                                         sigma=sg)
        datasg = pm.paint(hpos[:num], hmass[:num])
        datasgR = ft.smooth(datasg, 3, 'fingauss')
        fitt = dg.plot_noise(datasgR.value,
                             predictR.value,
                             M0=M0,
                             binfit=bins,
                             c='k',
                             axin=ax,
                             func=func,
                             mbin=mbinsm,
                             retfit=True)[0]
        fits.append(fitt)

    for i in range(3):
コード例 #4
0
                         predictR.value,
                         M0=M0,
                         binfit=bins,
                         c='k',
                         axin=ax,
                         func=func,
                         mbin=mbinsm,
                         retfit=True,
                         lsf='--')[0]

    fits = []
    sgs = [0.1, 0.15, 0.20]
    for i, sg in enumerate(sgs):

        hmass, hpos, hvel = dg.scatter_catalog(hdictf['mass'],
                                               hdictf['position'],
                                               sg,
                                               hvel=hdictf['velocity'])
        if rsd:
            datasg = pm.paint(
                hpos[:num] +
                (np.array([0, 0, 1]).reshape(-1, 1) * hvel[:num][:, 2]).T,
                mass=hmass[:num])
        else:
            datasg = pm.paint(hpos[:num], mass=hmass[:num])
        datasgR = ft.smooth(datasg, Rsm, 'fingauss')
        fitt = dg.plot_noise(datasgR.value,
                             predictR.value,
                             M0=M0,
                             binfit=bins,
                             c=colors[i],
                             axin=ax,
コード例 #5
0
ファイル: noise_files.py プロジェクト: modichirag/cosmo4dv2
#    bins = np.zeros((mbinsm.size, 1000 ))
#    for i in range(0, bins.shape[0]):
#        bins[i] = np.linspace(-3*mbinsm[i]/M0, 2*mbinsm[i]/M0, bins.shape[1])
#
    print('mbinsm -- ', mbinsm)

    ####
    fig, ax = plt.subplots(3, 3, figsize = (14, 12))
    fit0 = dg.plot_noise(datapR.value, predictR.value, M0=M0, binfit=bins, c='k', axin=ax, func=func, mbin=mbinsm, retfit=True, lsf='--')[0]
    
    fits = []
    sgs = [0.1, 0.15, 0.20]
    for i, sg in enumerate(sgs):
        
        if truemass:
            hmass, hpos, hmasstrue = dg.scatter_catalog(hdictf['mass'], hdictf['position'], sg, truemass=True)        
            datasg = pm.paint(hpos[:num], mass = hmasstrue[:num])
            datasgR = ft.smooth(datasg, Rsm, 'fingauss')
        else:
            hmass, hpos = dg.scatter_catalog(hdictf['mass'], hdictf['position'], sg)        
            datasg = pm.paint(hpos[:num], mass = hmass[:num])
            datasgR = ft.smooth(datasg, Rsm, 'fingauss')
        fitt = dg.plot_noise(datasgR.value, predictR.value, M0=M0, binfit=bins, c=colors[i], axin=ax, func=func, mbin=mbinsm, retfit=True)[0]
        fits.append(fitt)

    ff = mtpath + 'noisehist_M%02d_na.png'%(10*np.log10(M0))
    if truemass: ff = ff[:-4] + 'trueM.png'
    if Rsm !=3 : ff = ff[:-4] + '_R%d.png'%Rsm
    fig.savefig(ff)

    tosave = []