def getimage(data, poss, temp, mass, hsml, num, norm, cmap):
print('There are', poss.shape[0], 'gas particles in the region')
# Set up particle objects
P1 = sph.Particles(poss, mass=temp * mass, hsml=hsml)
P2 = sph.Particles(poss, mass=mass, hsml=hsml)
# Initialise the scene
S1 = sph.Scene(P1)
S2 = sph.Scene(P2)
i = data[num]
i['xsize'] = 3840
i['ysize'] = 2160
i['roll'] = 0
S1.update_camera(**i)
S2.update_camera(**i)
R1 = sph.Render(S1)
R2 = sph.Render(S2)
R1.set_logscale()
R2.set_logscale()
img1 = R1.get_image()
img2 = R2.get_image()
img = img1 - img2
vmax = 7.5
vmin = 3.5
print("gas temperature", np.min(img), np.max(img))
# Convert images to rgb arrays
rgb = cmap(norm(img))
return rgb, R1.get_extent()
def getimage(data, poss, mass, hsml, num, max_pixel, cmap, Type="gas"):
print('There are', poss.shape[0], 'gas particles in the region')
# Set up particle objects
P = sph.Particles(poss, mass=mass, hsml=hsml)
print(np.min(mass))
# Initialise the scene
S = sph.Scene(P)
i = data[num]
i['xsize'] = 5000
i['ysize'] = 5000
i['roll'] = 0
S.update_camera(**i)
R = sph.Render(S)
R.set_logscale()
img = R.get_image()
if Type == "gas":
vmax =11
vmin = 6
print("gas", np.max(img))
# Convert images to rgb arrays
rgb = cmap(get_normalised_image(img, vmin=vmin, vmax=vmax))
else:
vmax = 21.6
vmin = 15.0
print("star", np.min(img[img != 0]), np.max(img))
rgb = img
return rgb, R.get_extent()
def getimage_stars(data, poss, mass, hsml, num, max_pixel, cmap, Type="gas"):
print('There are', poss.shape[0], 'gas particles in the region')
# Set up particle objects
P = sph.Particles(poss, mass=mass, hsml=hsml)
print(np.min(mass))
# Initialise the scene
S = sph.Scene(P)
i = data[num]
i['xsize'] = 3840
i['ysize'] = 2160
i['roll'] = 0
S.update_camera(**i)
R = sph.Render(S)
R.set_logscale()
img = R.get_image()
img = ndimage.gaussian_filter(img, sigma=(3, 3), order=0)
if Type == "gas":
vmax = 11
vmin = 6
print("gas", np.max(img))
else:
vmax = 13
vmin = 7.5
print("star", np.max(img))
# Convert images to rgb arrays
rgb = cmap(get_normalised_image(img, vmin=vmin, vmax=vmax))
return rgb, R.get_extent()
def getimage(data, poss, hsml, num, boxsize):
print('There are', poss.shape[0], 'dark matter particles in the region')
# Set up particle objects
P = sph.Particles(poss, mass=np.ones(poss.shape[0]), hsml=hsml)
# Initialise the scene
S = sph.Scene(P)
i = data[num]
i['xsize'] = int(boxsize / hsml.max())
i['ysize'] = int(boxsize / hsml.max())
i['roll'] = 0
S.update_camera(**i)
R = sph.Render(S)
R.set_logscale()
img = R.get_image()
vmax = 7
vmin = 1
# Get colormaps
cmap = cmaps.twilight()
print(img.max())
# Convert images to rgb arrays
rgb = cmap(get_normalised_image(img, vmin=vmin, vmax=vmax))
return rgb, R.get_extent()
def myplot(x, y, nb=32, xsize=500, ysize=500): xmin = np.min(x) xmax = np.max(x) ymin = np.min(y) ymax = np.max(y) print xmin, xmax, ymin, ymax x0 = (xmin+xmax)/2. y0 = (ymin+ymax)/2. pos = np.zeros([3, len(x)]) pos[0,:] = x pos[1,:] = y w = np.ones(len(x)) P = sph.Particles(pos, w, nb=nb) S = sph.Scene(P) S.update_camera(r='infinity', x=x0, y=y0, z=0, xsize=xsize, ysize=ysize) R = sph.Render(S) R.set_logscale() img = R.get_image() extent = R.get_extent() for i, j in zip(xrange(4), [x0,x0,y0,y0]): extent[i] += j #print extent return img, extent
def myplot(x, y, nb=32, xsize=500, ysize=500):
"""This function reads in a set of data and smooths it using
nearest neighbors summing. It then outputs the smoothed data
with a measure of its extent. This output is then inputed to
Axes.imshow.
:param: x,y two columns of data such as particle positions
:param: nb smoothing size.
"""
xmin = np.min(x)
xmax = np.max(x)
ymin = np.min(y)
ymax = np.max(y)
x0 = (xmin + xmax) / 2.
y0 = (ymin + ymax) / 2.
pos = np.zeros([3, len(x)])
pos[0, :] = x
pos[1, :] = y
w = np.ones(len(x))
P = sph.Particles(pos, w, nb=nb)
S = sph.Scene(P)
S.update_camera(r='infinity', x=x0, y=y0, z=0, xsize=xsize, ysize=ysize)
R = sph.Render(S)
R.set_logscale()
img = R.get_image()
extent = R.get_extent()
for i, j in zip(xrange(4), [x0, x0, y0, y0]):
extent[i] += j
print extent, x0, y0
return img, extent
def plot_dist(fig, ax,P,coods,cmap,
vmin=1e-4,vmax=None,extent=300,
p=0,t=0,roll=0):
C = sph.Camera(x=coods[0], y=coods[1], z=coods[2],
r='infinity', zoom=1,
t=t, p=p, roll=roll,
extent=[-extent,extent,-extent,extent],
xsize=512, ysize=512)
S = sph.Scene(P, Camera=C)
R = sph.Render(S)
#R.set_logscale()
img = R.get_image()
# img = img / img.mean()
if vmax is None:
vmax = img.max()
if vmin > vmax:
print("vmin larger than vmax! Setting lower")
vmin = img.max() / 10
print("vmin,vmax:",vmin,vmax)
cNorm = colors.LogNorm(vmin=vmin,vmax=vmax)
sm = cm.ScalarMappable(norm=cNorm, cmap=cmap)
ax.imshow(img, extent=[-extent,extent,-extent,extent],
cmap=cmap, norm=cNorm)
return sm,img
def plot_sph(x: pd.Series,
y: pd.Series,
w: pd.Series,
nb=32,
xsize=1000,
ysize=1000):
x_min = np.min(x)
x_max = np.max(x)
y_min = np.min(y)
y_max = np.max(y)
x0 = np.average((x_min, x_max))
y0 = np.average((y_min, y_max))
pos = np.zeros([len(df), 3])
pos[:, 0] = x
pos[:, 1] = y
w = w.to_numpy() * 100
particles = sph.Particles(pos, mass=w, nb=nb)
scene = sph.Scene(particles)
scene.update_camera(r="infinity",
x=x0,
y=y0,
z=0,
xsize=xsize,
ysize=ysize)
render = sph.Render(scene)
render.set_logscale()
img = render.get_image()
extent = render.get_extent()
for i, j in zip(range(4), [x0, x0, y0, y0]):
extent[i] += j
return img, extent
def plot_ledlow_contours(t, world2pixel, ngb=12, xsize=500, ysize=500):
""" Smooth galaxy positions of Ledlow+ (2005) to get contour lines
@param t : astropy.table.Table holding Ledlow data
@param world2pixel : aplpy.FITSFigure world2pixel function to map
RA,dec coordinates to Chandra mosaic pixels
@param ngb : number of neighbours to smooth over
@param xsize, ysize: size of the image (resolution?)
@return : img, extent """
ra = 15 * astropy.coordinates.Angle(t['RAJ2000'].filled(numpy.nan),
unit=u.degree)
dec = astropy.coordinates.Angle(t['DEJ2000'].filled(numpy.nan),
unit=u.degree)
ra, dec = world2pixel(ra,
dec) # convert ra, dec to xray mosaic pixel values
# Perform kernel density estimate
# https://docs.scipy.org/doc/scipy-0.18.1/reference/generated/scipy.stats.gaussian_kde.html
# X, Y = numpy.mgrid[xmax:xmin:300j, ymin:ymax:3000j]
# positions = numpy.vstack([X.ravel(), Y.ravel()])
# values = numpy.vstack([ra, dec])
# kernel = kde.gaussian_kde(values)
# Z = numpy.reshape(kernel(positions).T, X.shape)
# Z /= ((41.1-40.6)*60*(20.025-19.50)*60)
# pyplot.imshow(numpy.rot90(Z), cmap=pyplot.cm.gist_earth_r,
# extent=[xmax, xmin, ymin, ymax])
# cset = pyplot.contour(X, Y, Z, colors="w",
# levels=numpy.array([1,2,3,5,8,10])*Z.max()/10)
# pyplot.clabel(cset, inline=1, fontsize=10)
# https://stackoverflow.com/questions/2369492
xmin, xmax = ra.min(), ra.max()
ymin, ymax = dec.min(), dec.max()
x0 = (xmin + xmax) / 2.
y0 = (ymin + ymax) / 2.
pos = numpy.zeros([3, len(ra)])
pos[0, :] = ra
pos[1, :] = dec
w = numpy.ones(len(ra))
P = sphviewer.Particles(pos, w, nb=ngb)
S = sphviewer.Scene(P)
S.update_camera(r="infinity", x=x0, y=y0, z=0, xsize=xsize, ysize=ysize)
R = sphviewer.Render(S)
img = R.get_image()
extent = R.get_extent()
for i, j in zip(xrange(4), [x0, x0, y0, y0]):
extent[i] += j
img = 10 * img / numpy.max(img)
return img, extent
def getimage(data, poss, hsml, num, z, cmap):
print('There are', poss.shape[0], 'dark matter particles in the region')
# Set up particle objects
P = sph.Particles(poss, mass=np.ones(poss.shape[0]), hsml=hsml)
# Initialise the scene
S = sph.Scene(P)
i = data[num]
i['xsize'] = 3840
i['ysize'] = 2160
i['roll'] = 0
S.update_camera(**i)
print("Scene")
R = sph.Render(S)
print("Render")
R.set_logscale()
print("Logscale")
img = R.get_image()
print("Image")
print(img.max(),
np.percentile(img, 99.99),
np.percentile(img, 95),
np.percentile(img, 90),
np.percentile(img, 67.5),
np.percentile(img, 50))
vmax = 6.9
vmin = 0.1
# # Get colormaps
# cmap2 = cmr.torch_r(np.linspace(0, 1, 128))
# cmap3 = cmr.swamp(np.linspace(0, 1, 128))
#
# # combine them and build a new colormap
# colors = np.vstack((cmap2, cmap3))
# cmap = mcolors.LinearSegmentedColormap.from_list('colormap', colors)
hex_list = ["#000000", "#590925", "#6c1c55", "#7e2e84", "#ba4051",
"#f6511d", "#ffb400", "#f7ec59", "#fbf6ac", "#ffffff"]
#cmap = get_continuous_cmap(hex_list, float_list=None)
img = ndimage.gaussian_filter(img, sigma=(3, 3), order=0)
# Convert images to rgb arrays
rgb = cmap(get_normalised_image(img, vmin=vmin, vmax=vmax))
return rgb, R.get_extent()
def __init__(self,
pos,
mass=None,
hsml=None,
nb=None,
logscale=True,
plot=True,
min_hsml=None,
max_hsml=None,
**kwargs):
if (mass is None):
mass = np.ones(len(pos[0, :]))
if (nb == None):
self._P = sph.Particles(pos, mass, hsml)
else:
self._P = sph.Particles(pos, mass, hsml, nb)
if ((min_hsml is not None) or (max_hsml is not None)):
hsml = self.get_hsml()
if (min_hsml is not None):
min_hsml = min_hsml
else:
min_hsml = np.min(hsml)
if (max_hsml is not None):
max_hsml = max_hsml
else:
max_hsml = np.max(hsml)
hsml = np.clip(hsml, min_hsml, max_hsml)
print 'Limiting smoothing lenght to the range [%.3f,%.3f]' % (
min_hsml, max_hsml)
self._P.set_hsml(hsml)
self._S = sph.Scene(self._P)
self._S.update_camera(**kwargs)
self._R = sph.Render(self._S)
if (logscale):
self._R.set_logscale()
self._img = self._R.get_image()
self._extent = self._R.get_extent()
if (plot):
self.imshow(aspect='auto')
return
else:
return
def single_sphere(reg, snap, soft, num, part_type, cmap, vlims, runall=True):
if runall:
# Define path
path = '/cosma/home/dp004/dc-rope1/FLARES/FLARES-1/G-EAGLE_' + reg + '/data'
poss, masses, smls = get_particle_data(path, snap, part_type=part_type, soft=soft)
# Get the spheres centre
centre, radius, mindist = spherical_region(path, snap)
# Cutout particles
poss, masses, smls = cutout_particles(poss, masses, smls, centre, radius)
print('There are %i particles (type %s) in the region'%(len(masses),part_type))
# Set up particle objects
P = sph.Particles(poss, mass=masses, hsml=smls)
# Initialise the scene
S = sph.Scene(P)
targets = [[0,0,0]]#,0,0,0,0,0,0]
# Define the box size
lbox = (15 / 0.677) * 2
# Define anchors dict for camera parameters
anchors = {}
anchors['sim_times'] = [0.0, 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
anchors['id_frames'] = [0, 90, 180, 270, 360, 450, 540, 630, 720]
anchors['id_targets'] = [0, 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
anchors['r'] = [lbox * 3 / 4, 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
anchors['t'] = [0, 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
anchors['p'] = [0, 'pass', 'pass', 'pass', 'pass', 'pass', 'pass', 'pass', 360]
anchors['zoom'] = [1., 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
anchors['extent'] = [10, 'same', 'same', 'same', 'same', 'same', 'same', 'same', 'same']
# Define the camera trajectory
data = camera_tools.get_camera_trajectory(targets, anchors)
for N in np.arange(num*N_block,(num*N_block)+N_block):
print("N:",N,'| p:',data[N]['p'])
# Get images
if runall:
img, extent = getimage(snap, N, data, part_type=part_type, overwrite=True, P=P, S=S)
else:
img, extent = getimage(snap, N, data, part_type=part_type, overwrite=False)
rgb = apply_cmap(img,cmap,vlims)
fig = plt.figure(figsize=(16,9), frameon=False)
ax = fig.add_subplot(111)
# set extent to 16:9 ratio
ax.set_xlim(extent[0] * 16/9, extent[1] * 16/9)
ax.imshow(rgb, origin='lower', aspect='equal', extent=extent)
ax.tick_params(axis='both', left=False, top=False, right=False,
bottom=False, labelleft=False, labeltop=False,
labelright=False, labelbottom=False)
ax.set_facecolor(cmap(0.0)) # (0.95588623, 0.91961077, 0.95812116))
fname = 'plots/spheres/All/all_parts_animation_reg%s_snap%s_ptype%s_angle%05d.png'%(reg,snap,part_type,N)
print("Saving:",fname)
fig.savefig(fname, dpi=300, bbox_inches='tight')
plt.close(fig)
def plot_parent(i, P, n, res, centre, z_centre):
print("i:", i)
sys.stdout.flush()
cmap = cmaps.twilight()
f = modified_sigmoid(i / n, 3)
L, l = 3300 / 2, 50
dl = L * (1 - f) + l * f
R = 16. / 9
offset = 100
dx = dl * R
dy = dl
ext_x = 3200 / 2
ext_y = 3200 / 2
if ext_x > dx: ext_x = dx
if ext_y > dy: ext_y = dy
C = sph.Camera(r='infinity',
t=0,
p=0,
roll=0,
xsize=res,
ysize=res,
x=centre,
y=centre,
z=z_centre,
extent=[-ext_x, ext_x, -ext_y, ext_y])
S = sph.Scene(P, C)
R = sph.Render(S)
extent = R.get_extent()
img = np.log10(R.get_image())
print(img.max(), img.min())
fig = plt.figure(figsize=(16, 9))
ax = fig.add_axes([0, 0, 1, 1])
# ax.imshow(img, cmap=cmap, vmin=-0.05, vmax=1.2, extent=extent,aspect='equal')
ax.imshow(img,
cmap=cmap,
vmin=--1,
vmax=2.4,
extent=extent,
aspect='equal')
del (img)
del (C)
ax.set_facecolor(cmap(0.0))
ax.set_xlim(-dx, dx)
ax.set_ylim(-dy, dy)
ax.hlines(0.9, 0.092, 0.192, transform=ax.transAxes, color='red', lw=2)
ax.text(0.1,
0.94,
'$%i \; \mathrm{cMpc}$' % (dx * 0.2),
transform=ax.transAxes,
size=12,
color='black')
rect = patches.Rectangle((0.09, 0.92),
0.105,
0.065,
linewidth=1,
edgecolor='none',
facecolor='white',
alpha=0.5,
transform=ax.transAxes)
ax.add_patch(rect)
ax.get_xaxis().set_visible(False)
ax.get_yaxis().set_visible(False)
# plt.show()
fname = 'plots/parent_zoom/parent_zoom_%03d.png' % i
# plt.gca().set_axis_off()
# plt.subplots_adjust(top = 1, bottom = 0, right = 1, left = 0,
# hspace = 0, wspace = 0)
# plt.margins(0,0)
print(fname)
fig.savefig(fname, dpi=150) #, bbox_inches='tight', pad_inches = 0)
plt.close(fig)
cmap = 'gnuplot'
axlab = r'$\log\Sigma_{X,\mathrm{0.5-2keV}}$ [$\mathrm{erg}$ $\mathrm{s}^{-1}$ $\mathrm{pc}^{-2}]$'
elif prop == 'stars':
cmap = 'bone'
axlab = r'$\log\Sigma_*$ [$M_{\odot}$ $\mathrm{pc}^{-2}]$'
elif prop == 'temperature':
cmap = 'seismic'
axlab = r'$\langle\log(T)\rangle$ $[\mathrm{K}]$'
else:
raise IOError(
'Plot options are "gasmass", "stars", "temperature" or "xrays"')
if not mean_mass_weighted:
Particles = sphviewer.Particles(pos, quantity, hsml=smoothing_length)
Scene = sphviewer.Scene(Particles)
phi_list = np.arange(0., 359., 1)
for p, phi in tqdm(enumerate(phi_list)):
Scene.update_camera(x=0.,
y=0.,
z=0.,
r='infinity',
t=45.,
p=phi,
extent=[-ext, ext, -ext, ext],
xsize=res,
ysize=res)
Render = sphviewer.Render(Scene)
Render.set_logscale()
for ax, t, p, c1, c2 in zip([ax1, ax2, ax3], [0, 0, 90], [0, 90, 90],
[0, 2, 2], [1, 1, 0]):
C = sph.Camera(r='infinity',
t=t,
p=p,
roll=0,
xsize=ext,
ysize=ext,
x=c[0],
y=c[1],
z=c[2],
extent=[-dl, dl, -dl, dl])
S = sph.Scene(P, C)
R = sph.Render(S)
img = np.log10(R.get_image())
extent = R.get_extent()
ax.imshow(img, cmap=cmaps.twilight())
ax1.text(0.1,0.9,'$\mathrm{log_{10}}(M_{\star} \,/\, \mathrm{M_{\odot}}) = %.2f$'%\
np.log10(mstar["%02d"%region][tag][_idx] * 1e10),
transform=ax1.transAxes)
for ax in [ax1, ax2, ax3]:
ax.xaxis.set_major_formatter(
FuncFormatter(lambda x, pos: (x / convers) * 1e3))
ax.yaxis.set_major_formatter(
FuncFormatter(lambda x, pos: (x / convers) * 1e3))
def __init__(self, gn, prop,
sim='L0100N1504',
run='REFERENCE',
snapnum=28,
halotype='all'):
self.groupnumber = gn
self.property = prop
tag = snapdict[str(snapnum)][0]
try:
data = h5.File(
'/data5/arijdav1/saved_regions/' + sim + '_' + run + '/' + tag + '/' + halotype + '/group' + str(
gn) + '.hdf5', 'r')
except IOError:
print 'Invalid group number for this box.'
exit()
if prop == 'stars':
pos = np.array(data['Stars/Coordinates']).T
smoothing_length = np.array(data['Stars/SmoothingLength'])
quantity = np.array(data['Stars/Mass']) * 1e10
else:
pos = np.array(data['Gas/Coordinates']).T
smoothing_length = np.array(data['Gas/SmoothingLength'])
if prop == 'gas':
quantity = np.array(data['Gas/Mass']) * 1e10
elif prop == 'hotgas':
quantity = np.array(data['Gas/Mass']) * 1e10
temp = np.array(data['Gas/Temperature'])
mask = np.where(temp > np.power(10., 5.5))[0]
column_pos = column_pos[mask]
smoothing_length = smoothing_length[mask]
quantity = quantity[mask]
elif prop == 'xrays':
quantity = np.array(
data['Gas/Xray_luminosity']) / 1e30 # make the numbers smaller so sphviewer can deal with them
else:
raise IOError('Plot options are "gas", "hotgas", "stars" or "xrays"')
N = len(quantity)
pos *= 1e3 # convert to kpc
smoothing_length *= 1e3
if prop == 'gas':
self.cmap = 'hot'
self.axlab = r'$\log\Sigma_g$ [$M_{\odot}$ $\mathrm{pc}^{-2}]$'
elif prop == 'hotgas':
self.cmap = 'hot'
self.axlab = r'$\log\Sigma_{\mathrm{g,hot}}$ [$M_{\odot}$ $\mathrm{pc}^{-2}]$'
elif prop == 'xrays':
self.cmap = 'gnuplot'
self.axlab = r'$\log\Sigma_{X,\mathrm{0.5-2keV}}$ [$\mathrm{erg}$ $\mathrm{s}^{-1}$ $\mathrm{pc}^{-2}]$'
elif prop == 'stars':
self.cmap = 'bone'
self.axlab = r'$\log\Sigma_*$ [$M_{\odot}$ $\mathrm{pc}^{-2}]$'
else:
raise IOError('Plot options are "gas", "hotgas", "stars" or "xrays"')
Particles = sphviewer.Particles(pos, quantity, hsml=smoothing_length)
self.Scene = sphviewer.Scene(Particles)
def select(self,centre,region_size): # Region size in Mpc
print 'Loading region...'
code_centre = centre * self.h/(self.a_0*1e3) # convert to h-less comoving code units
region_size *= self.h/self.a_0
# Point read_eagle to the data
snapfile = self.sim_path + 'snapshot_' + self.tag + '/snap_' + self.tag + '.0.hdf5'
# Open snapshot
snap = read.EagleSnapshot(snapfile)
# Select region of interest
snap.select_region(code_centre[0]-region_size/2.,
code_centre[0]+region_size/2.,
code_centre[1]-region_size/2.,
code_centre[1]+region_size/2.,
code_centre[2]-region_size/2.,
code_centre[2]+region_size/2.)
if self.property == 'stars':
pos = snap.read_dataset(4,'Coordinates') * self.a_0/self.h
smoothing_length = snap.read_dataset(4, 'SmoothingLength') * self.a_0 / self.h
quantity = snap.read_dataset(4, 'Mass') / self.h * 1e10
else:
pos = snap.read_dataset(0, 'Coordinates') * self.a_0 / self.h
smoothing_length = snap.read_dataset(0, 'SmoothingLength') * self.a_0 / self.h
if self.property == 'gas':
quantity = snap.read_dataset(0, 'Mass') / self.h / 1e10
elif self.property == 'xrays':
pids = snap.read_dataset(0, 'ParticleIDs')
quantity = self.xrays[np.searchsorted(self.xray_pids,pids)]
else:
raise IOError('Plot options are "gas","stars" or "xrays"')
print 'Wrapping box...'
region_size /= self.h/self.a_0
centre_mpc = centre /1e3
pos = ne.evaluate("pos-centre_mpc")
pos[pos[:,0]<(-1.*self.boxsize/2.),0] += self.boxsize
pos[pos[:,1]<(-1.*self.boxsize/2.),1] += self.boxsize
pos[pos[:,2]<(-1.*self.boxsize/2.),2] += self.boxsize
pos[pos[:,0]>self.boxsize/2.,0] -= self.boxsize
pos[pos[:,1]>self.boxsize/2.,1] -= self.boxsize
pos[pos[:,2]>self.boxsize/2.,2] -= self.boxsize
pos = ne.evaluate("pos+centre_mpc")
pos = pos.T
N = len(quantity)
pos *= 1e3 # convert to kpc
smoothing_length *= 1e3
print 'Creating scene...'
Particles = sphviewer.Particles(pos, quantity, hsml=smoothing_length)
self.Scene = sphviewer.Scene(Particles)
def __init__(self, prop,
sim='L0100N1504',
run='REFERENCE',
snapnum=28):
print 'Initialising box for imaging...'
tag = snapdict[str(snapnum)][0]
sim_path = '/data5/simulations/EAGLE/' + sim + '/' + run + '/data/'
# Get volume information
boxsize = E.readAttribute('SNAP', sim_path, tag, "/Header/BoxSize")
h = E.readAttribute('SNAP', sim_path, tag, "/Header/HubbleParam")
a_0 = E.readAttribute('SNAP', sim_path, tag, "/Header/ExpansionFactor")
# Point read_eagle to the data
snapfile = sim_path + 'snapshot_' + tag + '/snap_' + tag + '.0.hdf5'
comm = MPI.COMM_WORLD
comm_rank = comm.Get_rank()
comm_size = comm.Get_size()
# Open snapshot
snap = read.EagleSnapshot(snapfile)
# Select region of interest
snap.select_region(0.,boxsize,0.,boxsize,0.,boxsize)
# Split selection between processors
# This assigns an equal number of hash cells to each processor.
snap.split_selection(comm_rank,comm_size)
if prop == 'stars':
#pos = load_array('Coordinates', 4, sim=sim, run=run, tag=tag).T
#smoothing_length = load_array('SmoothingLength', 4, sim=sim, run=run, tag=tag)
#quantity = load_array('Mass', 4, sim=sim, run=run, tag=tag) * 1e10
pos = snap.read_dataset(4,'Coordinates') * a_0/h
pos = pos.T
smoothing_length = snap.read_dataset(4, 'SmoothingLength') * a_0 / h
quantity = snap.read_dataset(4, 'Mass') / h * 1e10
else:
#pos = load_array('Coordinates', 0, sim=sim, run=run, tag=tag).T
#smoothing_length = load_array('SmoothingLength', 0, sim=sim, run=run, tag=tag)
pos = snap.read_dataset(0, 'Coordinates') * a_0 / h
print pos
pos = pos.T
smoothing_length = snap.read_dataset(0, 'SmoothingLength') * a_0 / h
if prop == 'gas':
quantity = snap.read_dataset(0, 'Mass') / h / 1e10
print quantity
elif prop == 'xrays':
pids = snap.read_dataset(0, 'ParticleIDs')
print 'Matching x-rays to particles'
xray_data = h5.File('/data6/arijdav1/Lx_matching/'+sim+'_'+run+'/'+tag+'.hdf5','r')
xrays = np.array(xray_data['Xray_luminosity']) / 1e30
xray_pids = np.array(xray_data['ParticleIDs'])
#match_sort = np.argsort(xray_pids)
#xrays = xrays[match_sort]
#xray_pids = xray_pids[match_sort]
quantity = xrays[np.searchsorted(xray_pids,pids)]
else:
raise IOError('Plot options are "gas","stars" or "xrays"')
N = len(quantity)
pos *= 1e3 # convert to kpc
smoothing_length *= 1e3
print N
Particles = sphviewer.Particles(pos, quantity, hsml=smoothing_length)
print Particles.get_pos()
print Particles.get_mass()
print Particles.get_hsml()
self.Scene = sphviewer.Scene(Particles)
self.sim = sim
self.run = run
self.tag = tag
self.property = prop
self.boxsize = boxsize / h
print("mass weighted temp:",
np.sum((_temp * _mass)[mask]) / np.sum(_mass[mask]))
extent = 15
img = [None, None]
for i, _weight in enumerate([_temp, _temp * (_mass / 1.99e38)]):
Pd = sph.Particles(_coods, _weight) # halog_dust[mask] * 1e10)
C = sph.Camera(x=0,
y=0,
z=0,
r='infinity',
zoom=1,
extent=[-extent, extent, -extent, extent],
xsize=512,
ysize=512)
S = sph.Scene(Pd, Camera=C)
R = sph.Render(S)
# R.set_logscale()
img[i] = R.get_image()
#if vmax is None:
# vmax = img.max()
#
#if vmin > vmax:
# print("vmin larger than vmax! Setting lower")
# vmin = img.max() / 10
#print("vmin,vmax:",vmin,vmax)
#cNorm = colors.LogNorm(vmin=vmin,vmax=vmax)
#sm = cm.ScalarMappable(norm=cNorm, cmap=cmap)
def select(self, centre, region_size): # Region size in Mpc
if not self.quiet:
print 'Loading region...'
code_centre = centre * self.h / (
self.a_0 * 1e3) # convert to h-less comoving code units
code_region_size = region_size * self.h / self.a_0
centre_mpc = centre / 1e3
# Point read_eagle to the data
snapfile = self.sim_path + 'snapshot_' + self.tag + '/snap_' + self.tag + '.0.hdf5'
# Open snapshot
snap = read.EagleSnapshot(snapfile)
# Select region of interest
snap.select_region(code_centre[0] - code_region_size / 2.,
code_centre[0] + code_region_size / 2.,
code_centre[1] - code_region_size / 2.,
code_centre[1] + code_region_size / 2.,
code_centre[2] - code_region_size / 2.,
code_centre[2] + code_region_size / 2.)
if self.property == 'stars':
pos = snap.read_dataset(4, 'Coordinates') * self.a_0 / self.h
smoothing_length = snap.read_dataset(
4, 'SmoothingLength') * self.a_0 / self.h
quantity = snap.read_dataset(4, 'Mass') / self.h * 1e10
else:
pos = snap.read_dataset(0, 'Coordinates') * self.a_0 / self.h
smoothing_length = snap.read_dataset(
0, 'SmoothingLength') * self.a_0 / self.h
if self.property == 'gas':
quantity = snap.read_dataset(0, 'Mass') / self.h / 1e10
elif self.property == 'xrays':
pids = snap.read_dataset(0, 'ParticleIDs')
quantity = self.xrays[np.searchsorted(self.xray_pids, pids)]
elif self.property == 'entropy':
m_H_cgs = 1.6737e-24
weight = snap.read_dataset(0, 'Mass') / self.h / 1e10
temp = snap.read_dataset(0, 'Temperature')
abunds = np.zeros((len(temp), 11))
abunds[:, 0] = snap.read_dataset(
0, "SmoothedElementAbundance/Hydrogen")
abunds[:, 1] = snap.read_dataset(
0, "SmoothedElementAbundance/Helium")
abunds[:, 2] = snap.read_dataset(
0, "SmoothedElementAbundance/Carbon")
abunds[:, 3] = snap.read_dataset(
0, "SmoothedElementAbundance/Nitrogen")
abunds[:, 4] = snap.read_dataset(
0, "SmoothedElementAbundance/Oxygen")
abunds[:,
5] = snap.read_dataset(0,
"SmoothedElementAbundance/Neon")
abunds[:, 6] = snap.read_dataset(
0, "SmoothedElementAbundance/Magnesium")
abunds[:, 7] = snap.read_dataset(
0, "SmoothedElementAbundance/Silicon")
abunds[:, 8] = abunds[:, 7] * 0.6054160
abunds[:, 9] = abunds[:, 7] * 0.0941736
abunds[:, 10] = snap.read_dataset(
0, "SmoothedElementAbundance/Iron")
atomic_numbers = np.array(
[1., 2., 6., 7., 8., 10., 12., 14., 16., 20., 26.])
Xe = np.ones(len(abunds[:, 0]))
num_ratios = np.zeros(np.shape(abunds))
for col in range(len(abunds[0, :])):
num_ratios[:, col] = abunds[:, col] / abunds[:, 0]
for element in range(len(abunds[0, :]) - 1):
Xe += num_ratios[:,
element + 1] * atomic_numbers[element + 1]
density = snap.read_dataset(0, 'Density')
n_H = density * abunds[:, 0] / m_H_cgs # convert into nH cm^-3
n_e = n_H * Xe # electron density in cm^-3
quantity = temp / np.power(n_e, 2. / 3.)
else:
raise IOError(
'Plot options are "gas","ion", stars" or "xrays"')
if not self.quiet:
print 'Wrapping box...'
pos = ne.evaluate("pos-centre_mpc")
pos[pos[:, 0] < (-1. * self.boxsize / 2.), 0] += self.boxsize
pos[pos[:, 1] < (-1. * self.boxsize / 2.), 1] += self.boxsize
pos[pos[:, 2] < (-1. * self.boxsize / 2.), 2] += self.boxsize
pos[pos[:, 0] > self.boxsize / 2., 0] -= self.boxsize
pos[pos[:, 1] > self.boxsize / 2., 1] -= self.boxsize
pos[pos[:, 2] > self.boxsize / 2., 2] -= self.boxsize
pos = ne.evaluate("pos+centre_mpc")
# read_eagle loads in more than we actually asked for above. We need to mask to the region size again!
posmask = np.where(
(np.absolute(pos[:, 0] - centre_mpc[0]) < region_size / 2.)
& (np.absolute(pos[:, 1] - centre_mpc[1]) < region_size / 2.)
& (np.absolute(pos[:, 2] - centre_mpc[2]) < region_size / 2.))[0]
pos = pos[posmask, :]
smoothing_length = smoothing_length[posmask]
quantity = quantity[posmask]
N = len(quantity)
pos *= 1e3 # convert to kpc
smoothing_length *= 1e3
if not self.quiet:
print 'Creating scene...'
if self.property in [
'entropy',
]:
weight = weight[posmask]
Particles = sphviewer.Particles(pos, weight, hsml=smoothing_length)
self.weightScene = sphviewer.Scene(Particles)
Particles = sphviewer.Particles(pos,
quantity * weight,
hsml=smoothing_length)
self.propScene = sphviewer.Scene(Particles)
else:
if pos.size == 0:
self.Scene = None
else:
Particles = sphviewer.Particles(pos,
quantity,
hsml=smoothing_length)
self.Scene = sphviewer.Scene(Particles)
vmin=3
vmax=7
# ----escala de colores que te guste (http://matplotlib.org/examples/color/colormaps_reference.html)---
cmap='jet'
<<<<<<< HEAD
nb1 = 10
#nb1 = 100
=======
#nb1 = 5
nb1 = 100
>>>>>>> b29321f0c229ffcfec5b2b43354097e24d056487
particles=sph.Particles(pos[:3,corte],mstr[corte]*1e10,nb=nb1)
escena=sph.Scene(particles)
escena.update_camera(r='infinity',x=0,y=0,z=0,extent=[-rl,rl,-rl,rl])
rend=sph.Render(escena)
extent=escena.get_extent()
rend.set_logscale()
ax[0,0].imshow(rend.get_image(),extent=extent,origin='lower',cmap=cmap, vmin=vmin, vmax= vmax)
ax[0,0].set_xlim(-5,5)
ax[0,0].set_ylim(-5,5)
ax[0,0].set_xticks([])
ax[0,0].set_yticks([])
ax[0,0].set_yticklabels([])
ax[0,0].set_xticklabels([])
# ax[0,0].set_ylabel('$y\:[kpc]$', fontsize=40)
# ax[0,0].minorticks_on()
# ax[0,0].tick_params( labelsize=40)
def __init__(self,
pos,
mass=None,
hsml=None,
nb=None,
logscale=True,
plot=True,
min_hsml=None,
max_hsml=None,
**kwargs):
"""
Quickview is a simple wrapper of the sphviewer API.
This utility stores the particles, defines the Scene and the Camera, and produces the rendering of the Scene in one step, thus making the process of producing images of SPH particles easy and quick.
The arguments of the functions are:
- pos = SPH particle positions. Array of shape [N,3], where N in the
number of particles and pos[:,0] = x; pos[:,1] = y; pos[:,2] = z.
- mass (optional): is the mass of the SPH particles. If present,
it must be an array of size N. If absent, a constant value,
mass = 1, will be assumed for all particles.
- hsml (optional): this is an array containing the smoothing lenghts
of the SPH particles. The absence of the array will trigger the
calculation of the smoothing lenghts.
- nb (optional): number of neighbours to be used for the calculation
of the SPH smoothing lengths. If absent, the default value nb=32 will
be used. This arguement is ignored if the array hsml is provided.
- logscale (optional): If True, the output image becomes
out_log = log10(1.0+output)
- plot (optional): If true, QuickView will plot the resulting image in
the current active figure.
- min_hsml / max_hsml: Physical values of the minimum / maximum
smoothing lengths. Only used when defined.
**kwargs
These include the parameters of the Camera:
"""
if (mass is None):
mass = np.ones(len(pos))
if (nb == None):
self._P = sph.Particles(pos, mass, hsml)
else:
self._P = sph.Particles(pos, mass, hsml, nb)
if ((min_hsml is not None) or (max_hsml is not None)):
hsml = self.get_hsml()
if (min_hsml is not None):
min_hsml = min_hsml
else:
min_hsml = np.min(hsml)
if (max_hsml is not None):
max_hsml = max_hsml
else:
max_hsml = np.max(hsml)
hsml = np.clip(hsml, min_hsml, max_hsml)
print('Limiting smoothing length to the range '
'[%.3f,%.3f]' % (min_hsml, max_hsml))
self._P.set_hsml(hsml)
self._S = sph.Scene(self._P)
self._S.update_camera(**kwargs)
self._R = sph.Render(self._S)
if (logscale):
self._R.set_logscale()
self._img = self._R.get_image()
self._extent = self._R.get_extent()
if (plot):
self.imshow(aspect='auto')
return
else:
return
smoothing_length *= 1e3
if prop == 'gasmass':
cmap = 'hot'
axlab = r'$\log\Sigma_g$ [$M_{\odot}$ $\mathrm{kpc}^{-2}]$'
elif prop == 'xrays':
cmap = 'gnuplot'
axlab = r'$\log\Sigma_{X,\mathrm{0.5-2keV}}$ [$\mathrm{erg}$ $\mathrm{s}^{-1}$ $\mathrm{kpc}^{-2}]$'
elif prop == 'stars':
cmap = 'bone'
axlab = r'$\log\Sigma_*$ [$M_{\odot}$ $\mathrm{kpc}^{-2}]$'
else:
raise IOError('Plot options are "gasmass", "stars", "temperature" or "xrays"')
Particles = sphviewer.Particles(pos,quantity,hsml=smoothing_length)
Scene = sphviewer.Scene(Particles)
Scene.update_camera(x=0.,y=0.,z=0.,r='infinity',t=90.,extent=[-ext,ext,-ext,ext],xsize=res,ysize=res)
Render = sphviewer.Render(Scene)
#Render.set_logscale()
img = Render.get_image()
sdensity_img = img/px_size**2
'''
# For quickly viewing the individual images
extent = Render.get_extent()
plt.figure()
plt.imshow(sdensity_img,cmap='hot',extent=extent, origin='lower')
plt.show()
'''
extent=[-dx, dx, -dx, dx],
t=t,
p=p,
roll=0,
xsize=4000,
ysize=2250)
# Gas density
P = sph.Particles(norm_coods[coods_mask],
pmass[coods_mask] / pmass[coods_mask].min())
# hsml = hsml * 10)# * 2)
hsml = P.get_hsml()
## Create scene and render
S = sph.Scene(P, Camera=C)
R = sph.Render(S)
## Get image and plot
# R.set_logscale()
img = R.get_image()
print(img.min(), img.max())
cmap = sph_cmaps.desert() # plt.get_cmap('twilight')
img = cmap(vis_util.get_normalized_image(img, vmin=0, vmax=7))
fig, ax = vis_util.plot_img(img, R.get_extent())
# plt.show()
fig.savefig('test_out/gas_time_%s.png' % (tag_idx),
bbox_inches='tight',
pad_inches=0)
def getimage(path, snap, soft, num, centre, data, part_type):
# Get plot data
if part_type == 0:
poss_gas, masses_gas, smls_gas = get_sphere_data(path,
snap,
part_type=0,
soft=None)
elif part_type == 1:
poss_gas, masses_gas, smls_gas = get_sphere_data(path,
snap,
part_type=1,
soft=soft)
else:
return -1
# Centre particles
poss_gas -= centre
# Remove boundary particles
rgas = np.linalg.norm(poss_gas, axis=1)
okinds_gas = rgas < 14 / 0.677
poss_gas = poss_gas[okinds_gas, :]
masses_gas = masses_gas[okinds_gas]
smls_gas = smls_gas[okinds_gas]
if part_type == 0:
print('There are', len(masses_gas), 'gas particles in the region')
elif part_type == 1:
print('There are', len(masses_gas),
'dark matter particles in the region')
# Set up particle objects
P_gas = sph.Particles(poss_gas, mass=masses_gas, hsml=smls_gas)
# Initialise the scene
S_gas = sph.Scene(P_gas)
i = data[num]
i['xsize'] = 5000
i['ysize'] = 5000
i['roll'] = 0
S_gas.update_camera(**i)
R_gas = sph.Render(S_gas)
R_gas.set_logscale()
img_gas = R_gas.get_image()
if part_type == 0:
np.save(
'animationdata/gas_animationdata_reg' + reg + '_snap' + snap +
'_angle%05d.npy' % num, img_gas)
if part_type == 1:
np.save(
'animationdata/dm_animationdata_reg' + reg + '_snap' + snap +
'_angle%05d.npy' % num, img_gas)
# fig = plt.figure()
# ax = fig.add_subplot(111)
#
# ax.hist(get_normalised_image(img_gas).ravel(), bins=256, range=(0.0, 1.0), fc='k', ec='k')
#
# if part_type == 0:
# fig.savefig('plots/spheres/All/histDM_animation_reg' + reg + '_snap' + snap + '_angle%05d.png'%num,
# bbox_inches='tight')
# if part_type == 1:
# fig.savefig('plots/spheres/All/histgas_animation_reg' + reg + '_snap' + snap + '_angle%05d.png'%num,
# bbox_inches='tight')
# plt.close(fig)
vmax_gas = img_gas.max()
vmin_gas = vmax_gas * 0.5
# Get colormaps
if part_type == 0:
cmap_gas = cmaps.twilight()
elif part_type == 1:
cmap_gas = ml.cm.Greys_r
# Convert images to rgb arrays
rgb_gas = cmap_gas(get_normalised_image(img_gas, vmin=vmin_gas))
return rgb_gas, R_gas.get_extent()
for i in range(0, N_StePS):
if StePS_coordinates[i, 2] > -alpha and StePS_coordinates[
i,
2] < alpha and plot_R_limit > np.sqrt(StePS_coordinates[i, 0]**2 +
StePS_coordinates[i, 1]**2 +
StePS_coordinates[i, 2]**2):
StePS_slice[j, 0] = StePS_coordinates[i, 0]
StePS_slice[j, 1] = StePS_coordinates[i, 1]
StePS_slice[j, 2] = StePS_coordinates[i, 2]
StePS_slice[j, 3] = StePS_coordinates[i, 3]
j += 1
end = time.time()
print("..done in %fs. \n\n" % (end - start))
cmap = 'inferno'
extent = [-R_plot, R_plot, -R_plot, R_plot]
Particles = sph.Particles(StePS_slice[:, 0:3].T, StePS_slice[:, 3].T)
Scene = sph.Scene(Particles)
Scene.update_camera(r='infinity', extent=extent)
Render = sph.Render(Scene)
Render.set_logscale()
img = Render.get_image()
fig = plt.figure(1, figsize=(6, 6))
ax1 = fig.add_subplot(111)
ax1.imshow(img, extent=extent, origin='lower', cmap=cmap)
ax1.set_xlabel('x[Mpc]', size=10)
ax1.set_ylabel('y[Mpc]', size=10)
plt.title(title)
plt.show()
anchors['zoom'] = [1., 'same', 'same', 'same', 'same', 'same', 'same']
anchors['extent'] = [10, 'pass', 'pass', 'pass', 'pass', 'pass', 30]
data = get_camera_trajectory(targets, anchors)
n1 = 10000
cube1 = np.random.rand(3, n1)
cube1[1, :] -= 6
cube2 = np.random.rand(3, n1)
cube2[1, :] += 1
cubes = np.concatenate((cube1, cube2), axis=1)
mass = np.ones(n1+n1)
P = sph.Particles(cubes, mass)
S = sph.Scene(P)
h = 0
for i in data:
i['xsize'] = 200
i['ysize'] = 200
i['roll'] = 0
S = sph.Scene(P)
S.update_camera(**i)
print(S.Camera.get_params())
R = sph.Render(S)
img = R.get_image()
R.set_logscale()
plt.imsave('test/image_'+str('%d.png' % h), img,
vmin=0, vmax=6, cmap='cubehelix')
h += 1
def select(self, centre, region_size): # Region size in Mpc
if not self.quiet:
print 'Loading region...'
code_centre = centre * self.h / (
self.a_0 * 1e3) # convert to h-less comoving code units
code_region_size = region_size * self.h / self.a_0
centre_mpc = centre / 1e3
# Point read_eagle to the data
snapfile = self.sim_path + 'snapshot_' + self.tag + '/snap_' + self.tag + '.0.hdf5'
# Open snapshot
snap = read.EagleSnapshot(snapfile)
# Select region of interest
snap.select_region(code_centre[0] - code_region_size / 2.,
code_centre[0] + code_region_size / 2.,
code_centre[1] - code_region_size / 2.,
code_centre[1] + code_region_size / 2.,
code_centre[2] - code_region_size / 2.,
code_centre[2] + code_region_size / 2.)
if self.property == 'stars':
pos = snap.read_dataset(4, 'Coordinates') * self.a_0 / self.h
smoothing_length = snap.read_dataset(
4, 'SmoothingLength') * self.a_0 / self.h
quantity = snap.read_dataset(4, 'Mass') / self.h * 1e10
else:
pos = snap.read_dataset(0, 'Coordinates') * self.a_0 / self.h
smoothing_length = snap.read_dataset(
0, 'SmoothingLength') * self.a_0 / self.h
if self.property == 'gas':
quantity = snap.read_dataset(0, 'Mass') / self.h / 1e10
elif self.property == 'ion': # do this in CGS units
self.masses_u_dict = {
'Hydrogen': 1.00794,
'Carbon': 12.0107,
'Oxygen': 15.9994
}
p_mass = snap.read_dataset(
0, 'Mass') / self.h * C.unit_mass_cgs # in g
p_density = snap.read_dataset(
0, "Density"
) * self.h**2 / self.a_0**3 * C.unit_density_cgs # in g cm^-3
p_temp = snap.read_dataset(0, "Temperature")
el_mass_abund = snap.read_dataset(
0, 'SmoothedElementAbundance/' + self.element)
H_abund = snap.read_dataset(
0, 'SmoothedElementAbundance/Hydrogen')
p_nH = p_density * H_abund / C.m_H_cgs
ion_fraction = ionbal.find_ionbal(self.z, self.ion,
np.log10(p_nH),
np.log10(p_temp))
mass_in_ion = p_mass * el_mass_abund * ion_fraction
quantity = mass_in_ion / 1e40
elif self.property == 'xrays':
pids = snap.read_dataset(0, 'ParticleIDs')
quantity = self.xrays[np.searchsorted(self.xray_pids, pids)]
else:
raise IOError(
'Plot options are "gas","ion", stars" or "xrays"')
# read_eagle loads in more than we actually asked for above. We need to mask to the region size again!
posmask = np.where(
(np.absolute(pos[:, 0] - centre_mpc[0]) < region_size / 2.)
& (np.absolute(pos[:, 1] - centre_mpc[1]) < region_size / 2.)
& (np.absolute(pos[:, 2] - centre_mpc[2]) < region_size / 2.))[0]
pos = pos[posmask, :]
smoothing_length = smoothing_length[posmask]
quantity = quantity[posmask]
if self.property == 'ion':
mass_in_ion = mass_in_ion[posmask]
if not self.quiet:
print 'Wrapping box...'
pos = ne.evaluate("pos-centre_mpc")
pos[pos[:, 0] < (-1. * self.boxsize / 2.), 0] += self.boxsize
pos[pos[:, 1] < (-1. * self.boxsize / 2.), 1] += self.boxsize
pos[pos[:, 2] < (-1. * self.boxsize / 2.), 2] += self.boxsize
pos[pos[:, 0] > self.boxsize / 2., 0] -= self.boxsize
pos[pos[:, 1] > self.boxsize / 2., 1] -= self.boxsize
pos[pos[:, 2] > self.boxsize / 2., 2] -= self.boxsize
pos = ne.evaluate("pos+centre_mpc")
N = len(quantity)
pos *= 1e3 # convert to kpc
smoothing_length *= 1e3
if not self.quiet:
print 'Creating scene...'
Particles = sphviewer.Particles(pos, quantity, hsml=smoothing_length)
self.Scene = sphviewer.Scene(Particles)
if self.property == 'ion':
self.ion_positions = pos / 1e3
self.ion_hsml = smoothing_length / 1e3
self.ion_quantity = mass_in_ion / (
C.m_sol_cgs * self.masses_u_dict[self.element])
self.ion_centre = centre / 1e3
