def simple_previous_snap_read(Nsnap, use_multi='n'):
	if (int(Nsnap) < 10):
		Nsnapstring = '00'+str(Nsnap)
	elif (int(Nsnap) < 100):
		Nsnapstring = '0'+str(Nsnap)
	else:
		Nsnapstring = str(Nsnap)

	the_snapdir = './hdf5/'
	the_prefix ='snapshot'
	if (use_multi == 'y'):
		the_snapdir = './snapdir_'+Nsnapstring+'/'
	the_suffix = '.hdf5'
	
	print 'reading particle type 0 (gas?)' 
	G = readsnap(the_snapdir, Nsnapstring, 0, snapshot_name=the_prefix, extension=the_suffix)
	if (len(G['p'][:,0]) < 1 ):
		print 'no previous snapshot detected! ',Nsnap
		sys.exit()
	x = G['p'][:,0]
	y = G['p'][:,1]
	z = G['p'][:,2]
	ID = G['id']
	a = G['header'][2]
	Ttbl = (np.array([ID, x, y, z])).T
	return Ttbl, a
Beispiel #2
0
    def importParticleData(self, ptype):
        """
	Reads data in from whatever format you'd like.
	Input:
	    ptype - The numerical index of the particle type you want
	Output:
	    res - A dictionary that contains information for a *single* pointcloud!
	"""
        #we have a function of exactly this format, how convenient (/sarcasm)!
        return readsnap(self.snapdir, self.snapnum, ptype)
Beispiel #3
0
    def importParticleData(self,ptype):
	"""
	Reads data in from whatever format you'd like.
	Input:
	    ptype - The numerical index of the particle type you want
	Output:
	    res - A dictionary that contains information for a *single* pointcloud!
	"""
	#we have a function of exactly this format, how convenient (/sarcasm)!
	return readsnap(self.snapdir,self.snapnum,ptype)
Beispiel #4
0
def loop_rdf_wr(sdir, snum, num_bins, box_size=[1, 1, 1]):
    """This computes the radial distribution function(g(r)) and radial velocities
    between grains of size bin i and those of size bin j, at separations given by
    vector 'radii'. The results are stored as 3 dimensional matrices; 
    the first two axes are just spanning the possible i-j pairs, so it will be 
    lower triangular; the third direction runs over the separations at which g 
    and wr are computed"""
    Pd = readsnap(sdir, snum, 3)
    xd = Pd['p'][:, 0]
    yd = Pd['p'][:, 1]
    zd = Pd['p'][:, 2]
    vxd = Pd['v'][:, 0]
    vyd = Pd['v'][:, 1]
    vzd = Pd['v'][:, 2]

    # Shells
    # to be modified such that these numbers are not hard coded, but passed on
    # as a variable or something..
    radii = np.array([0.0025, 0.005, 0.01, 0.025, 0.05])
    dr = np.array([0.0025, 0.0025, 0.0075, 0.0225, 0.0275])
    num_radii = radii.size

    # Construct the dust size bins and the vectors with their indices, ok_ds
    # The size bins are equally spaced in log-space
    # ok_ds is a list of vectors, each vector containing the indices of dust
    # particles in a certain size bin
    e_min = np.amin(Pd['R_d'])
    e_max = np.amax(Pd['R_d'])
    size_bins = np.linspace(np.log10(e_min * 0.99),
                            np.log10(e_max * 1.01),
                            num=num_bins + 1,
                            endpoint=True)
    ok_ds = []
    for i in np.arange(num_bins):
        dummy, = np.where((np.log10(Pd['R_d']) >= size_bins[i])
                          & (np.log10(Pd['R_d']) < size_bins[i + 1]))
        ok_ds.append(dummy)

    g_list = np.zeros((num_bins, num_bins, num_radii))
    wr_list = np.zeros((num_bins, num_bins, num_radii))
    for i in np.arange(num_bins):
        for j in np.arange(i + 1):
            print('Computing bins', i, j)
            # This is the call to the main routine to compute g(r) and wr(r)
            # between dust species i and dust species j
            g,wr = compute_rdf_wr(xd[ok_ds[i]],yd[ok_ds[i]],zd[ok_ds[i]],\
                                  xd[ok_ds[j]],yd[ok_ds[j]],zd[ok_ds[j]],\
                                  vxd[ok_ds[i]],vyd[ok_ds[i]],vzd[ok_ds[i]],\
                                  vxd[ok_ds[j]],vyd[ok_ds[j]],vzd[ok_ds[j]],\
                                  box_size, radii, dr, 0.1, Nt=10)
            g_list[i, j, :] = g
            wr_list[i, j, :] = wr
    return (g_list, wr_list, radii)
Beispiel #5
0
def readsnapToDF(snapdir, snapnum, parttype):
    res = readsnap(snapdir, snapnum, parttype, cosmological='m12i' in snapdir)

    ids = res.pop('id')

    vels = res.pop('v')
    coords = res.pop('p')

    res['xs'], res['vxs'] = coords[:, 0], vels[:, 0]
    res['ys'], res['vys'] = coords[:, 1], vels[:, 1]
    res['zs'], res['vzs'] = coords[:, 2], vels[:, 2]

    metallicity = res.pop('z')
    for i, zarray in enumerate(metallicity.T):
        res['met%d' % i] = zarray

    snap_df = pd.DataFrame(res, index=ids)
    return snap_df
def match_particles(PID_list, Nsnap, use_multi='n'):

	if (int(Nsnap) < 10):
		Nsnapstring = '00'+str(Nsnap)
	elif (int(Nsnap) < 100):
		Nsnapstring = '0'+str(Nsnap)
	else:
		Nsnapstring = str(Nsnap)

	the_snapdir = './hdf5/'
	the_prefix ='snapshot'
	if (use_multi == 'y'):
		the_snapdir = './snapdir_'+Nsnapstring+'/'
	the_suffix = '.hdf5'
	
	print 'reading particle type 0 (gas?)' 
	G = readsnap(the_snapdir, Nsnapstring, 0, snapshot_name=the_prefix, extension=the_suffix)
	here =  np.in1d(G['id'], PID_list)
	
	PID = G['id'][here]
	
	x = G['p'][:,0][here]
	y = G['p'][:,1][here]
	z = G['p'][:,2][here]

	vx = G['v'][:,0][here]
	vy = G['v'][:,1][here]
	vz = G['v'][:,2][here]
	h = G['header'][12]
	PhysTemp, PhysRho = convertTemp(G['u'][here], G['ne'][here], G['rho'][here], h)
	Metallicity = G['z'][:,0][here]
	a =  G['header'][2]
	boxsize = G['header'][9]
	tbl = []
	base = [PID, x,y,z, vx,vy,vz, PhysTemp, PhysRho, Metallicity]
	for part in base:
		tbl.append(part)
	tbl = np.array(tbl)
	Ttbl = tbl.T
	return (Ttbl, a, boxsize)
Beispiel #7
0
        print "<nameout> == snapshot_184.hdf5"
        print "<nchunks> == 8"
        sys.exit(1337)
    namein0 = sys.argv[1]
    nameout = sys.argv[2]
    nchunks = sys.argv[3]

    fname_in = "%s/%s" % (dirpath, namein0)
    fname_out = "%s/%s" % (dirpath, nameout)

    print "Reading from input file"
    import readsnap as reads
    # For reading the properties
    # Gas
    print "Reading gas data"
    P0 = reads.readsnap(dirpath, nchunks, 0, cosmological=1, loud=1)
    # dark matter particles(high res.)
    print "Reading Dark Matter data: (only high res. particles)"
    P1 = reads.readsnap(dirpath, nchunks, 1, cosmological=1, loud=1)
    print "Reading Dark Matter data: (low res. particles: PartType2)"
    P2 = reads.readsnap(dirpath, nchunks, 2, cosmological=1, loud=1)
    print "Reading Dark Matter data: (low res. particles: PartType3)"
    P3 = reads.readsnap(dirpath, nchunks, 3, cosmological=1, loud=1)
    # Stellar particles
    print "Reading data for Stellar Particles"
    P4 = reads.readsnap(dirpath, nchunks, 4, cosmological=1, loud=1)

    # This is just for making a copy of the header
    file = h5py.File(fname_in, 'r')

    #fnew = h5py.File(fname_base+'.'+fname_ext, "w")
Beispiel #8
0
import h5py
import numpy as np
import readsnap as reads

halo_list = ['/gdata/rouge/agraus/Alternative_physics_runs/SIDM_runs/h11707/','/gdata/rouge/agraus/Alternative_physics_runs/WDM_runs/h11707/']

for halo_number in halo_list:
    dirname = halo_number
    snap_start = 'snapshot_184'
    #For reading the properties
    P0=reads.readsnap(dirname,7,0,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)
    P1=reads.readsnap(dirname,7,1,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)
    P2=reads.readsnap(dirname,7,2,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)
    P3=reads.readsnap(dirname,7,3,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)
    P5=reads.readsnap(dirname,7,5,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)
    P4=reads.readsnap(dirname,7,4,cosmological=1,loud=1,snapshot_name=snap_start,h0=1.0)

    #This is just for making a copy of the header
    print dirname+snap_start+'.0.hdf5'
    print 'whatever'
    file = h5py.File(dirname+snap_start+'.0.hdf5', 'r')
    stars=file['PartType4']
    coord = stars['Coordinates']
    Masses = stars['Masses']
    Metallicity = stars['Metallicity']
    ParticleIDs = stars['ParticleIDs']
    SFT = stars['StellarFormationTime']
    Vel = stars['Velocities']

    fnew = h5py.File(dirname+snap_start+'_for_rock.'+'hdf5', "w")
    #Creating the header
Beispiel #9
0
import os, sys
from readsnap import readsnap
import np_tools
import numpy as np

global colormapMin,colormapMax

########################################################################
# Load the Data from the Data Files
########################################################################

# Load the snapshot data. datasetBase and snapshotNumber are defined in the config file!
res = readsnap(datasetBase, snapshotNumber, 0)

# Calculate what the radius and weight should be when shown, as an approximation to what it really is.
radius = np.power(((res['m'] / res['rho'])/(2 * np.pi) ),(1.0/3.0))
weight = 2 * radius * res['rho']

########################################################################
# Orient the Camera
########################################################################

if orientOnCoM:
    cameraPosition, pivotPoint, cameraOrientation = np_tools.setCenterOfMassView( res['p'], res['m'], 4. )

########################################################################
# Put the Data in a Firefly-Recognizable Format
########################################################################

# Make a loader to keep the dataset around
numpy_loader = NumpyLoader()
Beispiel #10
0
#dirname = './halo796_Y13/snapdir_184/'
#dirname = './halo897_Y13/snapdir_184/'
#dirname = './halo897_Y13_stampede/'
#dirname = './halo848_Y13/snapdir_184/'
#dirname = './halo11707_Y13/snapdir_184/'
#dirname = './halo1016_Y13/snapdir_184/'
#dirname = './halo12596_Y13/snapdir_184/'
#dirname = './halo20910_Y13/snapdir_184/'
#dirname = './halo32503_Y13/snapdir_184/'
#dirname = './halo20192_Y13/snapdir_184/'
#dirname = './halo897_Y13/snapdir_184/'
dirname = './snapdir_184/'
import readsnap as reads
# For reading the properties
# Gas
P0=reads.readsnap(dirname,7,0,cosmological=1,loud=1)
# dark matter particles(high res.)
P1=reads.readsnap(dirname,7,1,cosmological=1,loud=1)
# dark matter particles(low res.)
P2=reads.readsnap(dirname,7,2,cosmological=1,loud=1)
P3=reads.readsnap(dirname,7,3,cosmological=1,loud=1)
P5=reads.readsnap(dirname,7,5,cosmological=1,loud=1)
# Stellar particles
P4=reads.readsnap(dirname,7,4,cosmological=1,loud=1)

# This is just for making a copy of the header
file = h5py.File(dirname+'snapshot_184.0.hdf5', 'r')
#stars=file['PartType4']
#coord = stars['Coordinates']
#Masses = stars['Masses']
#Metallicity = stars['Metallicity']
Beispiel #11
0
    theN = Ns[count]
    print 'reading particle type 4 for ', theN
    if (theN < 10):
        Nsnapstring = '00' + str(theN)
    elif (theN < 100):
        Nsnapstring = '0' + str(theN)
    else:
        Nsnapstring = str(theN)
    the_snapdir = './hdf5/'
    if (multifile):
        the_snapdir = './snapdir_' + Nsnapstring + '/'
    the_prefix = 'snapshot'
    the_suffix = '.hdf5'
    S = readsnap(the_snapdir,
                 Nsnapstring,
                 4,
                 snapshot_name=the_prefix,
                 extension=the_suffix)
    thetime = S['header'][2]
    redshift = S['header'][3]
    boxsize = S['header'][9]
    omega_matter = S['header'][10]
    omega_L = S['header'][11]
    h = S['header'][12]
    AHF_haloX = x[count]
    AHF_haloY = y[count]
    AHF_haloZ = z[count]
    AHF_Rvir = Rvir[count]
    AHF_a = 1.0 / (1.0 + Zs[count])

    if (adaptive_Rstar):
while (count < TheLen and not fake):
	theN = Ns[count]
	print 'reading particle type 4 for ',theN
	if (theN < 10):
		Nsnapstring = '00'+str(theN)
	elif (theN < 100):
		Nsnapstring = '0'+str(theN)
	else:
		Nsnapstring = str(theN)
	the_snapdir = './hdf5/'
	if (multifile):
		the_snapdir = './snapdir_'+Nsnapstring+'/'
	the_prefix ='snapshot'
	the_suffix = '.hdf5'
	S = readsnap(the_snapdir, Nsnapstring, 4, snapshot_name=the_prefix, extension=the_suffix)
	thetime = S['header'][2]
	redshift = S['header'][3]
	boxsize = S['header'][9]
	omega_matter = S['header'][10]
	omega_L = S['header'][11]
	h = S['header'][12]
	AHF_haloX = x[count]
	AHF_haloY = y[count] 
	AHF_haloZ = z[count]
	AHF_Rvir = Rvir[count]
	AHF_a = 1.0 / (1.0 + Zs[count])
	
	
	if (adaptive_Rstar):
		Rstars = Inner_SF_thresh*Rvir[count]
Beispiel #13
0
    Nsnapstring = str(Nsnap)

the_snapdir = './hdf5/'
the_prefix = 'snapshot'
if (multifile == 'y'):
    the_snapdir = './snapdir_' + Nsnapstring + '/'
the_suffix = '.hdf5'

#get the first 20 DM particles and see where they came from
the_ptype = 1
gthe_ptype = 0
sthe_ptype = 4

S = readsnap(the_snapdir,
             Nsnapstring,
             the_ptype,
             snapshot_name=the_prefix,
             extension=the_suffix)
gS = readsnap(the_snapdir,
              Nsnapstring,
              gthe_ptype,
              snapshot_name=the_prefix,
              extension=the_suffix)
sS = readsnap(the_snapdir,
              Nsnapstring,
              sthe_ptype,
              snapshot_name=the_prefix,
              extension=the_suffix)

PID_list = S['id'][:]
DMpos = S['p'][:, :]
Beispiel #14
0
        print "<nchunks> == 8"
        sys.exit(1337)
    dirpath=sys.argv[1]
    namein0=sys.argv[2]
    nameout=sys.argv[3]
    nchunks=sys.argv[4]
    
    fname_in = "%s/%s"%(dirpath,namein0)
    fname_out = "%s/%s"%(dirpath,nameout)
    
    print "Reading from input file"
    import readsnap as reads
    # For reading the properties
    # Gas
    print "Reading gas data"
    P0=reads.readsnap(dirpath,nchunks,0,cosmological=0,loud=1,snapshot_name='snapshot_184')
    # dark matter particles(high res.)
    print "Reading Dark Matter data: (only high res. particles)"
    P1=reads.readsnap(dirpath,nchunks,1,cosmological=0,loud=1,snapshot_name='snapshot_184')
    print "Reading Dark Matter data: (low res. particles: PartType2)"
    P2=reads.readsnap(dirpath,nchunks,2,cosmological=0,loud=1,snapshot_name='snapshot_184')
    print "Reading Dark Matter data: (low res. particles: PartType3)"
    P3=reads.readsnap(dirpath,nchunks,3,cosmological=0,loud=1,snapshot_name='snapshot_184')
    # Stellar particles
    print "Reading data for Stellar Particles"
    P4=reads.readsnap(dirpath,nchunks,4,cosmological=0,loud=1,snapshot_name='snapshot_184')

    # This is just for making a copy of the header
    print 'copying header from: '+str(fname_in) 
    file_copy = h5py.File(fname_in+'0.hdf5', 'r')
Beispiel #15
0
	Nsnapstring = '00'+str(sys.argv[1])
elif (int(sys.argv[1]) < 100):
	Nsnapstring = '0'+str(sys.argv[1])
else:
	Nsnapstring = str(sys.argv[1])
Nsnap = int(sys.argv[1])

the_snapdir = './hdf5/'
if (multifile):
	the_snapdir = './snapdir_'+Nsnapstring+'/'
the_prefix ='snapshot'
the_suffix = '.hdf5'

#read the snapshot
print 'reading particle type 0 (gas?)' 
G = readsnap(the_snapdir, Nsnapstring, 0, snapshot_name=the_prefix, extension=the_suffix)

print 'reading particle type 4'
S = readsnap(the_snapdir, Nsnapstring, 4, snapshot_name=the_prefix, extension=the_suffix)

if (readDM):
	print 'reading particle type 5 (black holes? I hope not)'
	P5 = readsnap(the_snapdir, Nsnapstring, 5, snapshot_name=the_prefix, extension=the_suffix,skip_bh=1)

	print 'reading particle type 1 (fine DM?)'
	DM = readsnap(the_snapdir, Nsnapstring, 1, snapshot_name=the_prefix, extension=the_suffix)

	print 'reading particle type 2'
	P2 = readsnap(the_snapdir, Nsnapstring, 2, snapshot_name=the_prefix, extension=the_suffix)

	print 'reading particle type 3'
Beispiel #16
0
    Nsnapstring = '0' + str(sys.argv[1])
else:
    Nsnapstring = str(sys.argv[1])
Nsnap = int(sys.argv[1])

the_snapdir = './hdf5/'
if (multifile):
    the_snapdir = './snapdir_' + Nsnapstring + '/'
the_prefix = 'snapshot'
the_suffix = '.hdf5'

#read the snapshot
print 'reading particle type 0 (gas?)'
G = readsnap(the_snapdir,
             Nsnapstring,
             0,
             snapshot_name=the_prefix,
             extension=the_suffix)

a = G['header'][2]
z = 1.0 / a - 1.0
redshift = G['header'][3]
boxsize = G['header'][9]
omega_matter = G['header'][10]
omega_L = G['header'][11]
h = G['header'][12]
redshiftstring = "{0:.3f}".format(redshift)
Hubble = hubble_param(a, omega_matter, h)
PhysTemp, PhysRho = SF.convertTemp(G['u'], G['ne'], G['rho'], h)

halostats = SF.find_halo_now(halo_to_do, a, therod=use_fixed_halos)
Beispiel #17
0
snum_max = snum_min
zmin = 0.510
zmax = 0.525
dt = 0.025
# don't forget to adjust colorbar min/max scale below
vmin = -0.5
vmax = 0.5

x_subtract = 0
y_subtract = 0
z_subtract = 0

xg, yg = np.mgrid[0:1:512j, 0:1:512j]
for snum in np.arange(snum_min, snum_max + 1):
    print(snum)
    H = readsnap(sdir, snum, 0, header_only=1)
    time = H['time']
    print('time', time)
    P = readsnap(sdir, snum, 0)
    Pd = readsnap(sdir, snum, 3)
    x = P['p'][:, 0]
    y = P['p'][:, 1]
    z = P['p'][:, 2]
    vx = P['v'][:, 0]
    vy = P['v'][:, 1]
    vz = P['v'][:, 2]
    rho = P['rho']

    xd = Pd['p'][:, 0]
    yd = Pd['p'][:, 1]
    zd = Pd['p'][:, 2]
def snapdata(path, snap):
    data = rs.readsnap(path, snap, 0)
    dataBH = rs.readsnap(path, snap, 5, skip_bh=1)
    dataSTAR = rs.readsnap(path, snap, 4)

    return data, dataBH, dataSTAR