def centroid(stamp):
"""
Calcula el centro de la estrella viendo un centro de masasx
con el flujo.
Parameters
----------
stamp : (N,)array_like
Arreglo en 2-D, representa una seccion de imagen que
engloba a una estrella.
Returns
-------
cx : float
Coordenada x del centro de la estrella.
cy : float
Coordenada y del centro de la estrella.
"""
# Se crean vectores con los indices x e y de la estampilla.
x_vect = sp.arange(0, sp.shape(stamp)[1])
y_vect = sp.arange(0, sp.shape(stamp)[0])
# Se estima un centro de la estrella.
cx = sp.median(x_vect)
cy = sp.median(y_vect)
# Se calcula la coordenada x del centro de la estrella.
sum_x = sp.nansum(x_vect * stamp[cy, :])
cx = sum_x / sp.nansum(stamp[cy, :])
# Se calcula la coordenada y del centro de la estrella.
sum_y = sp.nansum(y_vect * stamp[:, cx])
cy = sum_y / sp.nansum(stamp[:, cx])
return cx, cy
def fitdata(basedir, configfile, optintputs):
dirio = ("ACF", "Fitted")
inputdir = os.path.join(basedir, dirio[0])
outputdir = os.path.join(basedir, dirio[1])
dirlist = glob.glob(os.path.join(inputdir, "*lags.h5"))
dirlistsig = glob.glob(os.path.join(inputdir, "*sigs.h5"))
Ionoin = IonoContainer.readh5(dirlist[0])
Ionoinsig = IonoContainer.readh5(dirlistsig[0])
fitterone = Fitterionoconainer(Ionoin, Ionoinsig, configfile)
(fitteddata, fittederror) = fitterone.fitdata(
ISRSfitfunction, startvalfunc, exinputs=[fitterone.simparams["startfile"]]
)
if fitterone.simparams["Pulsetype"].lower() == "barker":
paramlist = fitteddata
species = fitterone.simparams["species"]
paranamsf = ["Ne"]
else:
(Nloc, Ntimes, nparams) = fitteddata.shape
fittederronly = fittederror[:, :, range(nparams), range(nparams)]
paramnames = []
species = fitterone.simparams["species"]
Nions = len(species) - 1
Nis = fitteddata[:, :, 0 : Nions * 2 : 2]
Tis = fitteddata[:, :, 1 : Nions * 2 : 2]
Nisum = sp.nansum(Nis, axis=2)[:, :, sp.newaxis]
Tisum = sp.nansum(Nis * Tis, axis=2)[:, :, sp.newaxis]
Ti = Tisum / Nisum
nNis = fittederronly[:, :, 0 : Nions * 2 : 2]
nTis = fittederronly[:, :, 1 : Nions * 2 : 2]
nNisum = sp.sqrt(sp.nansum(Nis * nNis ** 2, axis=2))[:, :, sp.newaxis] / Nisum
nTisum = sp.sqrt(sp.nansum(Nis * nTis ** 2, axis=2))[:, :, sp.newaxis]
nTi = nTisum / Nisum
paramlist = sp.concatenate((fitteddata, Nisum, Ti, fittederronly, nNisum, nTi), axis=2)
for isp in species[:-1]:
paramnames.append("Ni_" + isp)
paramnames.append("Ti_" + isp)
paramnames = paramnames + ["Ne", "Te", "Vi", "Nepow", "Ni", "Ti"]
paramnamese = ["n" + ip for ip in paramnames]
paranamsf = sp.array(paramnames + paramnamese)
Ionoout = IonoContainer(
Ionoin.Sphere_Coords,
paramlist,
Ionoin.Time_Vector,
ver=1,
coordvecs=Ionoin.Coord_Vecs,
paramnames=paranamsf,
species=species,
)
outfile = os.path.join(outputdir, "fitteddata.h5")
Ionoout.saveh5(outfile)
def nandot(x1, x2):
if len(x1.shape) == 1 and len(x2.shape) == 2:
x1T = SP.tile(x1, [x2.shape[1], 1]).transpose()
return SP.nansum(SP.multiply(x1T, x2), axis=0)
elif len(x2.shape) == 1 and len(x1.shape) == 2:
x2T = SP.tile(x2, [x1.shape[0], 1])
return SP.nansum(SP.multiply(x1, x2T), axis=1)
elif len(x1.shape) == 1 and len(x2.shape) == 1:
return SP.nansum(SP.multiply(x1, x2))
return None
def calc_MI_fore_only(self):
"""
Calculate the mutual information; now response variability comes from
responses to background; information calculated for foreground
"""
ds = 1. / self.num_fore_signals
dr = self.entropy_pdf_dy
pdf_r = ds * sp.sum(self.pdf_r_s, axis=0)
noise_H = -dr * ds * sp.nansum(
sp.log(self.pdf_r_s) / sp.log(2) * self.pdf_r_s, axis=(0, 1))
response_H = -dr * sp.nansum(sp.log(pdf_r + 1e-9) / sp.log(2) * pdf_r,
axis=0)
self.entropy = response_H - noise_H
def vi_metric(confmx):
"""computes Marina Meila's variation of information metric between two clusterings of the same data"""
# init
rval = {'MI': None, 'VI': None, 'Px': None, 'Py': None, 'Pxy': None, 'Hx': None, 'Hy': None}
nx, ny = confmx.shape
Px = sp.zeros(nx)
Py = sp.zeros(ny)
# compute
tot = sp.nansum(confmx)
for i in xrange(nx):
Px[i] = confmx[i, :].sum() / tot
for j in xrange(ny):
Py[j] = confmx[:, j].sum() / tot
Pxy = confmx / tot
Hx = ModMetricMeila.entropy(Px)
Hy = ModMetricMeila.entropy(Py)
MI = ModMetricMeila.mutual_information(Px, Py, Pxy)
# return
rval['VI'] = Hx + Hy - 2 * MI
rval['MI'] = MI
rval['Pxy'] = Pxy
rval['Px'] = Px
rval['Py'] = Py
rval['Hx'] = Hx
rval['Hy'] = Hy
return rval
def movnanmean(x, window_size, axis=0, accumulate=False):
r'''
Calculate the moving average for a given window size, without NaN
Parameters
----------
x : 1d numpy array
.
window_size : int
.
axis : int
.
Returns
-------
Obs:
----
Slower and higher memory consumption but can ignore NaN values in the
window
'''
if x.ndim == 1:
y = rolling_window(x, window_size)
if accumulate:
z = scipy.nansum(y, axis)
else:
z = scipy.stats.stats.nanmean(y, axis)
return z
def movnanmean(x, window_size, axis=0, accumulate=False):
r'''
Calculate the moving average for a given window size, without NaN
Parameters
----------
x : 1d numpy array
.
window_size : int
.
axis : int
.
Returns
-------
Obs:
----
Slower and higher memory consumption but can ignore NaN values in the
window
'''
if x.ndim == 1:
y = rolling_window(x, window_size)
if accumulate:
z = scipy.nansum(y, axis)
else:
z = scipy.stats.stats.nanmean(y, axis)
return z
def rl_standard(raw_image, psf, niter):
""" Standerd lucy-richardson convolution
arXiv 2002 Lauer
"""
psf /= psf.sum()
psf_inverse = psf[::-1]
lucy = np.ones( raw_image.shape ) * raw_image.mean()
for i in xrange( niter ):
estimate = convolve(lucy, psf, mode='mirror')
estimate[ np.isnan(estimate) ] = 0
correction = convolve(raw_image/estimate, psf_inverse, mode='mirror')
correction[ np.isnan(correction) ] = 0
print 'Correction:',correction.mean()
lucy *= correction
print 'Means:', raw_image.mean(), lucy.mean()
chisq = scipy.nansum((lucy - raw_image)**2 / (lucy)) / (raw_image.size-1)
print chisq
return lucy
def veldist_1d_rolr(plotfilename,phi=_DEFAULTPHI,R=_DEFAULTR,
ngrid=201,saveDir='../bar/1dvar/'):
"""
NAME:
veldist_1d_rolr
PURPOSE:
make a plot showing the influence of the bar R_OLR
INPUT:
plotfilename - filename for figure
phi - Galactocentric azimuth
R - Galactocentric radius
ngrid - number of grid-points to calculate the los velocity distribution
on
saveDir - save pickles here
OUTPUT:
Figure in plotfilename
HISTORY:
2010-09-11 - Written - Bovy (NYU)
"""
rolrs= [0.85,0.9,0.95]
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
vlosds= []
basesavefilename= os.path.join(saveDir,'rolr_')
for rolr in rolrs:
thissavefilename= basesavefilename+'%.3f.sav' % rolr
if os.path.exists(thissavefilename):
print "Restoring los-velocity distribution at R_OLR %.2f" % rolr
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating los-velocity distribution at R_OLR %.2f" % rolr
potparams= (rolr,0.01,25.*_degtorad,.8,None)
vlosd= predictVlos(vloslinspace,
l=phi,
d=R,
distCoord='GCGC',
pot='bar',beta=0.,
potparams=potparams)
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
savefile.close()
vlosds.append(vlosd)
#Plot
plot.bovy_print()
plot.bovy_plot(vloss,vlosds[1],'k-',zorder=3,
xrange=[vloslinspace[0],vloslinspace[1]],
yrange=[0.,sc.amax(sc.array(vlosds).flatten())*1.1],
xlabel=r'$v_{\mathrm{los}} / v_0$')
plot.bovy_plot(vloss,vlosds[0],ls='-',color='0.75',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[2],ls='-',color='0.5',
overplot=True,zorder=2,lw=1.5)
plot.bovy_text(r'$\mathrm{bar}\ R_{\mathrm{OLR}}$',title=True)
plot.bovy_text(0.36,.75,r'$R_{\mathrm{OLR}} = 0.95\ R_0$'+'\n'+r'$R_{\mathrm{OLR}} = 0.90\ R_0$'+ '\n'+r'$R_{\mathrm{OLR}} = 0.85\ R_0$')
plot.bovy_end_print(plotfilename)
def replaceNansByMeans(self):
"""Replace all not-a-number entries in the dataset by the means of the
corresponding column."""
for d in self.data.itervalues():
means = scipy.nansum(d[:self.getLength()], axis=0) / self.getLength()
for i in xrange(self.getLength()):
for j in xrange(d.dim):
if not scipy.isfinite(d[i, j]):
d[i, j] = means[j]
def replaceNansByMeans(self):
"""Replace all not-a-number entries in the dataset by the means of the
corresponding column."""
for d in self.data.itervalues():
means = scipy.nansum(d[:self.getLength()], axis=0) / self.getLength()
for i in xrange(self.getLength()):
for j in xrange(ds.dim):
if not scipy.isfinite(d[i, j]):
d[i, j] = means[j]
def calc_MI(self):
"""
Calculate the mutual information between signal and response.
"""
cond_H = -sp.nansum(self.pdf_r_s * sp.log(self.pdf_r_s),
axis=0) * self.entropy_pdf_dy
noise_H = (1 + sp.log(2 * sp.pi *
(self.NL_scale * self.meas_noise)**2)) / 2
self.entropy = (cond_H - noise_H) / sp.log(2)
def average_out_degree_fraction(cover, weights=None):
'''
Out Degree Fraction (ODF) of a node in a cluster is the ratio between its number of external (boundary) edges
and its internal edges. Average ODF returns the average fraction for the cluster.
'''
rv = []
odf = out_degree_fraction(cover, weights)
for i in range(len(cover)):
ratios = odf[i]
rv += [ nansum(ratios)/cover.subgraph(i).vcount() ]
return rv
def mutual_information(x, y, xy):
"""compute mutual information between the associated random variables"""
# init
MI = sp.zeros(x.size, y.size)
for i in xrange(x.size):
for j in xrange(y.size):
MI[i, j] = xy[i, j] * sp.log(xy[i, j] / (x[i] * y[j]))
# return
return sp.nansum(MI)
def mutual_information(x, y, xy):
"""compute mutual information between the associated random variables"""
# init
MI = sp.zeros(x.size, y.size)
for i in xrange(x.size):
for j in xrange(y.size):
MI[i, j] = xy[i, j] * sp.log(xy[i, j] / (x[i] * y[j]))
# return
return sp.nansum(MI)
def kullbackLeibler(p, q, dx=1, nan=False):
"""
NAME:
kullbackLeibler
PURPOSE:
Calculate the Kullback-Leibler divergence D(p||q)
INPUT:
p - probability density at points i
q - another probability density at points i
dx - distance between points i (can be an array)
nan - ignore nans
OUTPUT:
D(p||q)
HISTORY:
2010-05-09 - Written - Bovy (NYU)
"""
if nan:
return sc.nansum(p * dx * sc.log(p / q))
else:
return sc.sum(p * dx * sc.log(p / q))
def vi_metric(confmx):
"""computes Marina Meila's variation of information metric between two clusterings of the same data"""
# init
rval = {
'MI': None,
'VI': None,
'Px': None,
'Py': None,
'Pxy': None,
'Hx': None,
'Hy': None
}
nx, ny = confmx.shape
Px = sp.zeros(nx)
Py = sp.zeros(ny)
# compute
tot = sp.nansum(confmx)
for i in xrange(nx):
Px[i] = confmx[i, :].sum() / tot
for j in xrange(ny):
Py[j] = confmx[:, j].sum() / tot
Pxy = confmx / tot
Hx = ModMetricMeila.entropy(Px)
Hy = ModMetricMeila.entropy(Py)
MI = ModMetricMeila.mutual_information(Px, Py, Pxy)
# return
rval['VI'] = Hx + Hy - 2 * MI
rval['MI'] = MI
rval['Pxy'] = Pxy
rval['Px'] = Px
rval['Py'] = Py
rval['Hx'] = Hx
rval['Hy'] = Hy
return rval
def entropy(x):
"""compute entropy of a discrete random variable"""
return -sp.nansum(x * sp.log(x))
def invertRSTO(RSTO,Iono,alpha_list=1e-2,invtype='tik',rbounds=[100,200],Nlin=0):
""" This will run the inversion program given an ionocontainer, an alpha and """
nlout,ntout,nl=Iono.Param_List.shape
if Nlin !=0:
nl=Nlin
nlin=len(RSTO.Cart_Coords_In)
time_out=RSTO.Time_Out
time_in=RSTO.Time_In
overlaps = RSTO.overlaps
xin,yin,zin=RSTO.Cart_Coords_In.transpose()
z_u=sp.unique(zin)
rplane=sp.sqrt(xin**2+yin**2)*sp.sign(xin)
r_u=sp.unique(rplane)
n_z=z_u.size
n_r=r_u.size
dims= [n_r,n_z]
rin,azin,elin=RSTO.Sphere_Coords_In.transpose()
anglist=RSTO.simparams['angles']
ang_vec=sp.array([[i[0],i[1]] for i in anglist])
# trim out cruft
zmin,zmax=[150,500]
rpmin,rpmax=rbounds#[-50,100]#[100,200]
altlog= sp.logical_and(zin>zmin,zin<zmax)
rplog=sp.logical_and(rplane>rpmin,rplane<rpmax)
allrng= RSTO.simparams['Rangegatesfinal']
dR=allrng[1]-allrng[0]
nldir=sp.ceil(int(nl)/2.)
posang_log1= sp.logical_and(ang_vec[:,0]<=180.,ang_vec[:,0]>=0)
negang_log1 = sp.logical_or(ang_vec[:,0]>180.,ang_vec[:,0]<0)
azin_pos = sp.logical_and(azin<=180.,azin>=0)
azin_neg = sp.logical_or(azin>180.,azin<0)
minangpos=0
minangneg=0
if sp.any(posang_log1):
minangpos=ang_vec[posang_log1,1].min()
if sp.any(negang_log1):
minangneg=ang_vec[negang_log1,1].min()
rngbounds=[allrng[0]-nldir*dR,allrng[-1]+nldir*dR]
rng_log=sp.logical_and(rin>rngbounds[0],rin<rngbounds[1])
elbounds_pos=sp.logical_and(azin_pos,elin>minangpos)
elbounds_neg=sp.logical_and(azin_neg,elin>minangneg)
elbounds=sp.logical_or(elbounds_pos,elbounds_neg)
keeplog=sp.logical_and(sp.logical_and(rng_log,elbounds),sp.logical_and(altlog,rplog))
keeplist=sp.where(keeplog)[0]
nlin_red=len(keeplist)
# set up derivative matrix
dx,dy=diffmat(dims)
dx_red=dx[keeplist][:,keeplist]
dy_red=dy[keeplist][:,keeplist]
# need the sparse vstack to make srue things stay sparse
D=sp.sparse.vstack((dx_red,dy_red))
# New parameter matrix
new_params=sp.zeros((nlin,len(time_out),nl),dtype=Iono.Param_List.dtype)
if isinstance(alpha_list,numbers.Number):
alpha_list=[alpha_list]*nl
ave_datadif=sp.zeros((len(time_out),nl))
ave_data_const = sp.zeros_like(ave_datadif)
q=1e10
for itimen, itime in enumerate(time_out):
print('Making Outtime {0:d} of {1:d}'.format(itimen+1,len(time_out)))
#allovers=overlaps[itimen]
#curintimes=[i[0] for i in allovers]
#for it_in_n,it in enumerate(curintimes):
#print('\t Making Intime {0:d} of {1:d}'.format(it_in_n+1,len(curintimes)))
#A=RSTO.RSTMat[itimen*nlout:(itimen+1)*nlout,it*nlin:(it+1)*nlin]
A=RSTO.RSTMat[itimen*nlout:(itimen+1)*nlout,itimen*nlin:(itimen+1)*nlin]
Acvx=cvx.Constant(A[:,keeplist])
for ip in range(nl):
alpha=alpha_list[ip]*2
print('\t\t Making Lag {0:d} of {1:d}'.format(ip+1,nl))
datain=Iono.Param_List[:,itimen,ip]
xr=cvx.Variable(nlin_red)
xi=cvx.Variable(nlin_red)
if invtype.lower()=='tik':
constr=alpha*cvx.norm(xr,2)
consti=alpha*cvx.norm(xi,2)
elif invtype.lower()=='tikd':
constr=alpha*cvx.norm(D*xr,2)
consti=alpha*cvx.norm(D*xi,2)
elif invtype.lower()=='tv':
constr=alpha*cvx.norm(D*xr,1)
consti=alpha*cvx.norm(D*xi,1)
br=datain.real/q
bi=datain.imag/q
if ip==0:
objective=cvx.Minimize(cvx.norm(Acvx*xr-br,2)+constr)
constraints= [xr>=0]
prob=cvx.Problem(objective)
result=prob.solve(verbose=True,solver=cvx.SCS,use_indirect=True,max_iters=4000)
# new_params[keeplog,it,ip]=xr.value.flatten()
xcomp=sp.array(xr.value).flatten()*q
else:
objective=cvx.Minimize(cvx.norm(Acvx*xr-br,2)+constr)
prob=cvx.Problem(objective)
result=prob.solve(verbose=True,solver=cvx.SCS,use_indirect=True,max_iters=4000)
objective=cvx.Minimize(cvx.norm(Acvx*xi-bi,2)+consti)
prob=cvx.Problem(objective)
result=prob.solve(verbose=True,solver=cvx.SCS,use_indirect=True,max_iters=4000)
xcomp=sp.array(xr.value + 1j*xi.value).flatten()*q
# new_params[keeplog,it,ip]=xcomp
new_params[keeplog,itimen,ip]=xcomp
ave_datadif[itimen,ip]=sp.sqrt(sp.nansum(sp.absolute(A[:,keeplist].dot(xcomp)-datain)**2))
if invtype.lower()=='tik':
sumconst=sp.sqrt(sp.nansum(sp.power(sp.absolute(xcomp),2)))
elif invtype.lower()=='tikd':
dx=D.dot(xcomp)
sumconst=sp.sqrt(sp.nansum(sp.power(sp.absolute(dx),2)))
elif invtype.lower()=='tv':
dx=D.dot(xcomp)
sumconst=sp.nansum(sp.absolute(dx))
ave_data_const[itimen,ip]=sumconst
# set up nans
new_params[sp.logical_not(keeplog),itimen]=sp.nan
datadif=sp.nanmean(ave_datadif,axis=0)
constval=sp.nanmean(ave_data_const,axis=0)
ionoout=IonoContainer(coordlist=RSTO.Cart_Coords_In,paramlist=new_params,times = time_out,sensor_loc = sp.zeros(3),ver =0,coordvecs =
['x','y','z'],paramnames=Iono.Param_Names[:Nlin])
return (ionoout,datadif,constval)
def veldist_1d_Rphi(plotfilename,nx=100,ny=20,dx=_XWIDTH/20.,dy=_YWIDTH/20.,
ngrid=201,rrange=[0.7,1.3],
phirange=[-m.pi/2.,m.pi/2.],
saveDir='../bar/1dLarge/',normalize=True,
row=None):
"""
NAME:
veldist_1d_Rphi
PURPOSE:
plot how the los-velocity distribution changes as a function of
R and phi
INPUT:
nx - number of plots in the x-direction
ny - number of plots in the y direction
dx - x-spacing
dy - y-spacing
ngrid - number of gridpoints to evaluate the density on
rrange - range of Galactocentric radii to consider
phirange - range of Galactic azimuths to consider
saveDir - directory to save the pickles in
normalize - if True (default), normalize the los-vd to integrate to one
row - if set to a row number, calculate the los-velocity distributions
for this row only, and do not plot anything (just save for later)
OUTPUT:
plot!
HISTORY:
2010-04-21 - Written - Bovy (NYU)
"""
if row == None:
rowStart= 0
rowEnd= nx
calcOnly= False
else:
rowStart= row
rowEnd= rowStart+1
calcOnly= True
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
picklebasename= '1d_%i_%i_%i_%.1f_%.1f_%.1f_%.1f' % (nx,ny,ngrid,rrange[0],rrange[1],phirange[0],phirange[1])
if not os.path.exists(saveDir):
os.mkdir(saveDir)
left, bottom = 0.1, 0.1
width= (nx*_XWIDTH+(nx-1)*dx)/(1.-2.*left)
height= (ny*_YWIDTH+(ny-1)*dy)/(1.-2.*bottom)
if not calcOnly:
plot.bovy_print(fig_width=width,fig_height=height,
xtick_major_size=2.,ytick_major_size=2.,
xtick_minor_size=0.,ytick_minor_size=0.)
fig= pyplot.figure()
#Make theta-R axes
fudge= 8.0
thisax= fig.add_axes([left-_XWIDTH/width/fudge,
bottom-_XWIDTH/height/fudge,
1.+2*_XWIDTH/width/fudge-2*left,
1.+2*_XWIDTH/height/fudge-2*bottom])
xrange= sc.array(phirange)*_radtodeg
yrange=rrange
thisax.xaxis.set_label_text(r'$\mathrm{Galactocentric\ azimuth}\ [\mathrm{deg}]$')
thisax.set_xlim(-90.01,90.01)
thisax.yaxis.set_label_text(r'$\mathrm{Galactocentric\ radius}\ / R_0$')
thisax.set_ylim(yrange[0],yrange[1])
thisax.xaxis.set_major_locator(ticker.MultipleLocator(10.))
for ii in range(rowStart,rowEnd):
for jj in range(ny):
if not calcOnly:
thisax= fig.add_axes([left+ii*(_XWIDTH+dx)/width,
bottom+jj*(_YWIDTH+dy)/height,
_XWIDTH/width,_YWIDTH/height])
thisR= (rrange[0]+(rrange[1]-rrange[0])/
(ny*_YWIDTH+(ny-1)*dy)*(jj*(_YWIDTH+dy)+_YWIDTH/2.))
thisphi= (phirange[0]+(phirange[1]-phirange[0])/
(nx*_XWIDTH+(nx-1)*dx)*(ii*(_XWIDTH+dx)+_XWIDTH/2.))
thissavefilename= os.path.join(saveDir,picklebasename+'_%i_%i.sav' %(ii,jj))
if os.path.exists(thissavefilename):
print "Restoring los-velocity distribution at %.1f, %.1f ..." %(thisR,thisphi)
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
axivlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating los-velocity distribution at %.1f, %.1f ..." %(thisR,thisphi)
vlosd= predictVlos(vloslinspace,
l=thisphi,
d=thisR,
distCoord='GCGC',
pot='bar',beta=0.,
potparams=(0.9,0.01,25.*_degtorad,.8,None))
axivlosd= predictVlos(vloslinspace,
l=thisphi,
d=thisR,
distCoord='GCGC',
pot='bar',beta=0.,t=-0.00001,
potparams=(0.9,0.0,25.*_degtorad,.8,None))
if normalize:
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
axivlosd= axivlosd/(sc.nansum(axivlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
pickle.dump(axivlosd,savefile)
savefile.close()
if calcOnly:
continue
fig.sca(thisax)
plot.bovy_plot(vloss,vlosd,'k',
overplot=True,zorder=3)
plot.bovy_plot(vloss,axivlosd,ls='-',color='0.5',
overplot=True,zorder=2)
thisax.set_xlim(vloslinspace[0],vloslinspace[1])
thisax.set_ylim(0.,sc.amax(sc.concatenate((axivlosd,vlosd)))*1.1)
thisax.xaxis.set_ticklabels('')
thisax.yaxis.set_ticklabels('')
if not calcOnly:
plot.bovy_end_print(plotfilename)
def fit_5_peaks_cest(scn_to_analyse, fitrounds = 1):
scn = sarpy.Scan(scn_to_analyse)
pdata_num = 0
x_size = scn.pdata[pdata_num].data.shape[0]
y_size = scn.pdata[pdata_num].data.shape[1]
try:
roi = scn.adata['roi'].data
except KeyError:
roi = scn.pdata[0].data[:,:,0]*0+1
# Get the bbox so that the whole image isn't fit
try:
bbox = scn.adata['bbox'].data
except KeyError:
bbox = numpy.array([0,x_size-1,0,y_size-1])
datashape = roi.shape
roi_reshaped = numpy.reshape(roi,[roi.shape[0],roi.shape[1],1])
cestscan_roi = scn.pdata[0].data * roi_reshaped
# Fit multiple peaks, need some empty arrays
offst = numpy.empty_like(roi) + numpy.nan
pk1_amp = numpy.empty_like(roi) + numpy.nan
pk1_pos = numpy.empty_like(roi) + numpy.nan
pk1_width = numpy.empty_like(roi) + numpy.nan
pk2_amp = numpy.empty_like(roi) + numpy.nan
pk2_pos = numpy.empty_like(roi) + numpy.nan
pk2_width = numpy.empty_like(roi) + numpy.nan
pk3_amp = numpy.empty_like(roi) + numpy.nan
pk3_pos = numpy.empty_like(roi) + numpy.nan
pk3_width = numpy.empty_like(roi) + numpy.nan
pk4_amp = numpy.empty_like(roi) + numpy.nan
pk4_pos = numpy.empty_like(roi) + numpy.nan
pk4_width = numpy.empty_like(roi) + numpy.nan
water_amp = numpy.empty_like(roi) + numpy.nan
water_pos = numpy.empty_like(roi) + numpy.nan
water_width = numpy.empty_like(roi) + numpy.nan
fit_quality = numpy.empty_like(roi) + numpy.nan
fit_params_arr = numpy.empty_like(roi, dtype=object)
fit_params_arr[:] = [numpy.nan]
ppm_corrected_arr = numpy.empty_like(roi, dtype=object)
# Defining parameters
freq_list = scn.method.CEST_FreqListPPM
ppm_limit_min = -50
ppm_limit_max = 50
exclude_ppm = 200
normalize_to_ppm = 66.6
possibleNormalizations = [i for i, x in enumerate(freq_list) if numpy.abs(x - normalize_to_ppm) <1E-4]
normalizeTo = possibleNormalizations[-1]
# Get only the frequencies within the ppm_limit
ppm_filtered = [f for f in freq_list if ppm_limit_max > f > ppm_limit_min]
# Exclude the dummy frequencies at the beginning (66.6 ppm)
ppm_filtered = sorted([n for n in ppm_filtered if n!= exclude_ppm])
# Get the index of the good frequencies relative to the original list
ppm_filtered_ind = [freq_list.index(c) for c in ppm_filtered]
# get the freqs that'll be used for water fit
water_fit_freqs = [f for f in ppm_filtered if (numpy.abs(f)< 3.)]
water_fit_freqs_ind = sorted([ppm_filtered.index(c) for c in water_fit_freqs])
# Create some empty arrays
water_shifts = numpy.empty_like(roi) + numpy.nan
new_shifted = numpy.empty(shape=(water_shifts.shape[0], water_shifts.shape[0], len(ppm_filtered))) + numpy.nan
# Create temporary structs to store paramArrays
tempstruct = numpy.zeros((1), dtype=[('offset', 'float64'),
('A1', 'float64'),('w1', 'float64'),('p1', 'float64'),
('A2', 'float64'),('w2', 'float64'),('p2', 'float64'),
('A3', 'float64'),('w3', 'float64'),('p3', 'float64'),
('A4', 'float64'),('w4', 'float64'),('p4', 'float64'),
('water_A', 'float64'),('water_w', 'float64'),('water_p', 'float64')])
newstruct = numpy.zeros(roi.shape, dtype=[('offset', 'float64'),
('A1', 'float64'),('w1', 'float64'),('p1', 'float64'),
('A2', 'float64'),('w2', 'float64'),('p2', 'float64'),
('A3', 'float64'),('w3', 'float64'),('p3', 'float64'),
('A4', 'float64'),('w4', 'float64'),('p4', 'float64'),
('water_A', 'float64'),('water_w', 'float64'),('water_p', 'float64')])
# Nan the array so there are no zeroes anywhere
newstruct[:] = numpy.nan
#tempstruct[:] = numpy.nan
# Fit count, this counts the number of rounds the data has been fit
fitcount = 0
while fitcount < fitrounds:
for xval in range(bbox[0],bbox[1]):
for yval in range(bbox[2],bbox[3]):
# Get the data and normalize it to index of normalize_to_ppm
tmp = cestscan_roi[xval,yval][ppm_filtered_ind] / scn.pdata[0].data[xval,yval,normalizeTo]
# Check to make sure I'm inside the ROI
if numpy.isfinite(numpy.sum(tmp)):
# First do the water fit and shift the data so water is at 0
shiftParams = fit_water_peak(tmp[water_fit_freqs_ind],water_fit_freqs,allParams=True)
shift = shiftParams[3]
water_shifts[xval,yval] = shift
# Interpolation happens here
if numpy.isfinite(shift):
s_shifted_back = scipy.interp(ppm_filtered, ppm_filtered+shift/2, tmp)
new_shifted[xval,yval,:] = s_shifted_back
else:
print(shift)
pass
testParams = get_neighbours_starting(fit_params_arr,xval,yval)
testParams = h_convertBetweenStructArrays(testParams,toType = 'array')
fit_params,cov,infodict,mesg,ier = scipy.optimize.leastsq(
h_residual_Zspectrum_N,
testParams,
args=(new_shifted[xval,yval], ppm_filtered),
full_output = True,
maxfev = 900,
ftol =1E-9)
# Specify paramsets for peaks:
#TOFIX: why is the offset applied to each peak
#pk1 = [fit_params[0]]+list(fit_params[1:4])
#pk2 = [fit_params[0]]+list(fit_params[4:7])
#pk3 = [fit_params[0]]+list(fit_params[7:10])
#pk4 = [fit_params[0]]+list(fit_params[10:13])
#waterpk = [fit_params[0]]+list(fit_params[13:16])
offst[xval,yval] = fit_params[0]
pk1_amp[xval,yval] = fit_params[1]
pk1_width[xval,yval] = fit_params[2]
pk1_pos[xval,yval] = fit_params[3]
pk2_amp[xval,yval] = fit_params[4]
pk2_width[xval,yval] = fit_params[5]
pk2_pos[xval,yval] = fit_params[6]
pk3_amp[xval,yval] = fit_params[7]
pk3_width[xval,yval] = fit_params[8]
pk3_pos[xval,yval] = fit_params[9]
pk4_amp[xval,yval] = fit_params[10]
pk4_width[xval,yval] = fit_params[11]
pk4_pos[xval,yval] = fit_params[12]
water_amp[xval,yval] = fit_params[13]
water_width[xval,yval] = fit_params[14]
water_pos[xval,yval] = fit_params[15]
fit_quality[xval,yval] = scipy.nansum(numpy.abs(new_shifted - h_zspectrum_N(fit_params,ppm_filtered-shift)))
fit_params_arr[xval,yval] = fit_params
ppm_corrected_arr[xval,yval] = ppm_filtered
fitcount+=1 # increment fitcounter
# Save the data as a structured array
newstruct['offset'] = offst
newstruct['A1'] = pk1_amp
newstruct['w1'] = pk1_width
newstruct['p1'] = pk1_pos
newstruct['A2'] = pk2_amp
newstruct['w2'] = pk2_width
newstruct['p2'] = pk2_pos
newstruct['A3'] = pk3_amp
newstruct['w3'] = pk3_width
newstruct['p3'] = pk3_pos
newstruct['A4'] = pk4_amp
newstruct['w4'] = pk4_width
newstruct['p4'] = pk4_pos
newstruct['water_A'] = water_amp
newstruct['water_w'] = water_width
newstruct['water_p'] = water_pos
return {'':newstruct,'fit_quality':fit_quality}
def parametersweep(basedir,configfile,acfdir='ACF',invtype='tik'):
"""
This function will run the inversion numerious times with different constraint
parameters. This will create a directory called cost and place.
Input
basedir - The directory that holds all of the data for the simulator.
configfile - The ini file for the simulation.
acfdir - The directory within basedir that hold the acfs to be inverted.
invtype - The inversion method that will be tested. Can be tik, tikd, and tv.
"""
alpha_sweep=sp.logspace(-3.5,sp.log10(7),25)
costdir = os.path.join(basedir,'Cost')
ionoinfname=os.path.join(basedir,acfdir,'00lags.h5')
ionoin=IonoContainer.readh5(ionoinfname)
dirio = ('Spectrums','Mat','ACFMat')
inputdir = os.path.join(basedir,dirio[0])
dirlist = glob.glob(os.path.join(inputdir,'*.h5'))
(listorder,timevector,filenumbering,timebeg,time_s) = IonoContainer.gettimes(dirlist)
Ionolist = [dirlist[ikey] for ikey in listorder]
RSTO = RadarSpaceTimeOperator(Ionolist,configfile,timevector,mattype='Sim')
npts=RSTO.simparams['numpoints']
ionospec=makeionocombined(dirlist)
if npts==ionospec.Param_List.shape[-1]:
tau,acfin=spect2acf(ionospec.Param_Names,ionospec.Param_List)
nloc,ntimes=acfin.shape[:2]
ambmat=RSTO.simparams['amb_dict']['WttMatrix']
np=ambmat.shape[0]
acfin_amb=sp.zeros((nloc,ntimes,np),dtype=acfin.dtype)
# get the original acf
ambmat=RSTO.simparams['amb_dict']['WttMatrix']
np=ambmat.shape[0]
for iloc,locarr in enumerate(acfin):
for itime,acfarr in enumerate(locarr):
acfin_amb[iloc,itime]=sp.dot(ambmat,acfarr)
acfin_amb=acfin_amb[:,0]
else:
acfin_amb=ionospec.Param_List[:,0]
if not os.path.isdir(costdir):
os.mkdir(costdir)
# pickle file stuff
pname=os.path.join(costdir,'cost{0}-{1}.pickle'.format(acfdir,invtype))
alpha_list=[]
errorlist=[]
errorlaglist=[]
datadiflist=[]
constlist=[]
if 'perryplane' in basedir.lower() or 'SimpData':
rbounds=[-500,500]
else:
rbounds=[0,500]
alpha_list_new=alpha_sweep.tolist()
for i in alpha_list:
if i in alpha_list_new:
alpha_list_new.remove(i)
for i in alpha_list_new:
ionoout,datadif,constdif=invertRSTO(RSTO,ionoin,alpha_list=i,invtype=invtype,rbounds=rbounds,Nlin=1)
datadiflist.append(datadif)
constlist.append(constdif)
acfout=ionoout.Param_List[:,0]
alpha_list.append(i)
outdata=sp.power(sp.absolute(acfout-acfin_amb),2)
aveerror=sp.sqrt(sp.nanmean(outdata,axis=0))
errorlaglist.append(aveerror)
errorlist.append(sp.nansum(aveerror))
pickleFile = open(pname, 'wb')
pickle.dump([alpha_list,errorlist,datadiflist,constlist,errorlaglist],pickleFile)
pickleFile.close()
mkalphalist(pname)
alphaarr=sp.array(alpha_list)
errorarr=sp.array(errorlist)
errorlagarr=sp.array(errorlaglist)
datadif=sp.array(datadiflist)
constdif=sp.array(constlist)
fig,axlist,axmain=plotalphaerror(alphaarr,errorarr,errorlagarr)
fig.savefig(os.path.join(costdir,'cost{0}-{1}.png'.format(acfdir,invtype)))
fig,axlist=plotLcurve(alphaarr,datadif,constdif)
fig.savefig(os.path.join(costdir,'lcurve{0}-{1}.png'.format(acfdir,invtype)))
def veldist_1d_slope(plotfilename,phi=_DEFAULTPHI,R=_DEFAULTR,
ngrid=201,saveDir='../bar/1dvar/'):
"""
NAME:
veldist_1d_slope
PURPOSE:
make a plot showing the influence of the shape of the rotation curve
INPUT:
plotfilename - filename for figure
phi - Galactocentric azimuth
R - Galactocentric radius
ngrid - number of grid-points to calculate the los velocity distribution
on
saveDir - save pickles here
OUTPUT:
Figure in plotfilename
HISTORY:
2010-05-15 - Written - Bovy (NYU)
"""
slopes= [-0.2,-0.1,0.,0.1,0.2]
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
vlosds= []
basesavefilename= os.path.join(saveDir,'slope_')
for slope in slopes:
thissavefilename= basesavefilename+'%.1f.sav' % slope
if os.path.exists(thissavefilename):
print "Restoring los-velocity distribution at slope %.1f" % slope
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating los-velocity distribution at slope %.1f" % slope
potparams= (0.9,0.01,25.*_degtorad,.8,None)
vlosd= predictVlos(vloslinspace,
l=phi,
d=R,
distCoord='GCGC',
pot='bar',beta=slope,
potparams=potparams)
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
savefile.close()
vlosds.append(vlosd)
#Plot
plot.bovy_print()
plot.bovy_plot(vloss,vlosds[2],'k-',zorder=3,
xrange=[vloslinspace[0],vloslinspace[1]],
yrange=[0.,sc.nanmax(sc.array(vlosds).flatten())*1.1],
xlabel=r'$v_{\mathrm{los}} / v_0$')
plot.bovy_plot(vloss,vlosds[0],ls='-',color='0.75',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[1],ls='-',color='0.60',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[3],ls='-',color='0.45',
overplot=True,zorder=2,lw=1.5)
plot.bovy_plot(vloss,vlosds[4],ls='-',color='0.3',
overplot=True,zorder=2,lw=1.5)
plot.bovy_text(r'$\mathrm{shape\ of\ the\ rotation\ curve}$',title=True)
plot.bovy_text(0.5,.5,r'$\beta = -0.2$'+'\n'+r'$\beta = -0.1$'+ '\n'+
r'$\beta = \phantom{-}0.0$'+'\n'+
r'$\beta= \phantom{-}0.1$'+'\n'+
r'$\beta= \phantom{-}0.2$')
plot.bovy_end_print(plotfilename)
def extract(data, varimg, fitwidth=10., extractwidth=1.5, thresh=5.):
"""
extract(data,varimg,width=WIDTH,nsig=NSIG,noise=NOISE)
From an input 2d array, find and extract spectral traces.
Inputs:
data - 2d science spectrum
varimg - 2d variance spectrum
fitwidth - width to fit profile to in pixels
extractwidth - width to extract (in sigma)
thresh - signal/noise threshold for extraction
Outputs:
a list containing the [profile, extracted spectrum, a smoothed
spectrum, the extracted variance spectrum] for each extracted
trace
"""
WIDTH = fitwidth
NSIG = extractwidth
NOISE = thresh
FILTSIZE = 7
data = data.copy()
spectra = []
# Replace nan with zero
data[scipy.isnan(data)] = 0.
varimg[scipy.isnan(varimg)] = 0.
data[scipy.isinf(data)] = 0.
varimg[scipy.isinf(varimg)] = 0.
# Create model of real flux. We ignore the slit ends, which may have
# artifacts from the resampling.
slit = data[:, 8:-8].astype(scipy.float32)
var = varimg[:, 8:-8]
# OK...so negative-variance also isn't good; set these pixels to zero
var[var < 0] = 0
# Create noise models
sigmaimg = slit / scipy.sqrt(var)
highpix = scipy.where(sigmaimg > 1.5, sigmaimg, 0.)
source_columns = highpix.sum(axis=0)
# MASKING DISABLED (this would take only columns with lotsa flux...)
# mask = scipy.where(source_columns>4.,1.,scipy.nan)
mask = source_columns * 0.
# Condition 1, dealing with bad pixels
if (var == 0).any():
cond = var == 0
var[cond] = scipy.nan
slit[cond] = scipy.nan
mask = scipy.where(cond, 0, 1)
flux = scipy.nansum(slit / var, axis=1) / scipy.nansum(1. / var,
axis=1)
noise = scipy.sqrt(scipy.nansum(var, axis=1)) / mask.sum(axis=1)
# Condition 2, no masking
elif scipy.nansum(mask) == 0:
flux = (slit / var).sum(axis=1) / (1. / var).sum(axis=1)
noise = scipy.sqrt(var.sum(axis=1)) / mask.size
# Condition 3, masking
else:
fluxmodel = slit * mask
noisemodel = var * mask
noise = scipy.sqrt(scipy.nansum(noisemodel,
axis=1)) / scipy.nansum(mask)
flux = stats.stats.nanmean(fluxmodel, axis=1)
# A smooth S/N estimate for the slit
# sig2noise = ndimage.gaussian_filter1d(flux,1)/noise
row = scipy.arange(flux.size)
model = flux.copy()
nspec = 10 # Maximum number of attempts
while nspec:
nspec -= 1
# Fit a gaussian around the peak of the S/N model
start = model.argmax() - WIDTH
end = model.argmax() + WIDTH + 1
if start < 0:
start = 0.
if end > model.size:
end = model.size
fitarr = model[start:end]
p = scipy.zeros(4)
p[1] = fitarr.max()
p[2] = fitarr.argmax()
p[3] = 2.
fit, val = special_functions.ngaussfit(fitarr, p)
chi2 = val / (fitarr.size - 3)
fit[2] += start
# If the centroid doesn't lie on the slit, get use the edge pix
midcol = fit[2].round()
if midcol >= flux.size:
midcol = flux.size - 1
elif midcol < 0:
midcol = 0
# Require a reasonable S/N and width
if fit[3] > fitarr.size / 2. or fit[3] < 0.85:
break
elif fit[0] > 0 and fit[1] < NOISE * noise[midcol]:
break
elif fit[0] < 0 and fit[1] - fit[0] < NOISE * noise[midcol]:
break
else:
fit[1] += fit[0]
fit[0] = 0.
# Subtract away a model of the source
source = special_functions.ngauss(row, fit)
model -= scipy.where(source > noise, source, 0.)
# Skip Slits off the edge
if fit[2] < 0 or fit[2] >= flux.size:
continue
# Skip residuals!
if fit[1] < scipy.sqrt(flux[fit[2]]):
continue
fit[1] = 1.
weight = special_functions.ngauss(row, fit)
cond = (row > fit[2] - fit[3] * NSIG) & (row <
fit[2] + fit[3] * NSIG)
weight = scipy.where(cond, weight, 0)
weight /= weight.sum()
spec = weight * data.T
spec = spec.sum(axis=1)
varspec = weight * varimg.T
varspec = varspec.sum(axis=1)
spec[varspec == 0] = 0.
smooth = signal.wiener(spec, FILTSIZE, varspec)
smooth[scipy.isnan(smooth)] = 0.
spectra.append([fit, spec, smooth, varspec])
return spectra
'''
end
'''
stitchLower = sp.searchsorted(wavelength, 5570, side="left")
stitchUpper = sp.searchsorted(wavelength, 5590, side="right")
flux[stitchLower:stitchUpper] = sp.nan
flux[flux < 0] = sp.nan
smoothFlux = convolve(flux, Box1DKernel(width))[5 * width:-5 * width]
flux = flux[5 * width:-5 * width]
wavelength = wavelength[5 * width:-5 * width]
totalCounts = sp.nansum(flux)
#spike = sp.median(sp.diff(flux[::10]))
plt.plot(wavelength, smoothFlux)
'''
start
'''
#testing = sp.diff(flux[::10])
#testing2 = (testing==testing and abs(testing)>10)
# counts = [abs(testing)]
#to do: look into 'spikeness'
'''
end
'''
def bovy_dens2d(X, **kwargs):
"""
NAME:
bovy_dens2d
PURPOSE:
plot a 2d density with optional contours
INPUT:
first argument is the density
matplotlib.pyplot.imshow keywords (see http://matplotlib.sourceforge.net/api/axes_api.html#matplotlib.axes.Axes.imshow)
xlabel - (raw string!) x-axis label, LaTeX math mode, no $s needed
ylabel - (raw string!) y-axis label, LaTeX math mode, no $s needed
xrange
yrange
noaxes - don't plot any axes
overplot - if True, overplot
colorbar - if True, add colorbar
shrink= colorbar argument: shrink the colorbar by the factor (optional)
Contours:
contours - if True, draw contours (10 by default)
levels - contour-levels
cntrmass - if True, the density is a probability and the levels
are probability masses contained within the contour
cntrcolors - colors for contours (single color or array)
cntrlabel - label the contours
cntrlw, cntrls - linewidths and linestyles for contour
cntrlabelsize, cntrlabelcolors,cntrinline - contour arguments
onedhists - if True, make one-d histograms on the sides
onedhistcolor - histogram color
retAxes= return all Axes instances
OUTPUT:
HISTORY:
2010-03-09 - Written - Bovy (NYU)
"""
if kwargs.has_key('overplot'):
overplot = kwargs['overplot']
kwargs.pop('overplot')
else:
overplot = False
if not overplot:
pyplot.figure()
if kwargs.has_key('xlabel'):
xlabel = kwargs['xlabel']
kwargs.pop('xlabel')
else:
xlabel = None
if kwargs.has_key('ylabel'):
ylabel = kwargs['ylabel']
kwargs.pop('ylabel')
else:
ylabel = None
if kwargs.has_key('zlabel'):
zlabel = kwargs['zlabel']
kwargs.pop('zlabel')
else:
zlabel = None
if kwargs.has_key('extent'):
extent = kwargs['extent']
kwargs.pop('extent')
else:
if kwargs.has_key('xrange'):
xlimits = list(kwargs['xrange'])
kwargs.pop('xrange')
else:
xlimits = [0, X.shape[0]]
if kwargs.has_key('yrange'):
ylimits = list(kwargs['yrange'])
kwargs.pop('yrange')
else:
ylimits = [0, X.shape[1]]
extent = xlimits + ylimits
if not kwargs.has_key('aspect'):
kwargs['aspect'] = (xlimits[1] - xlimits[0]) / float(ylimits[1] -
ylimits[0])
if kwargs.has_key('noaxes'):
noaxes = kwargs['noaxes']
kwargs.pop('noaxes')
else:
noaxes = False
if (kwargs.has_key('contours') and kwargs['contours']) or \
kwargs.has_key('levels') or \
(kwargs.has_key('cntrmass') and kwargs['cntrmass']):
contours = True
else:
contours = False
if kwargs.has_key('contours'): kwargs.pop('contours')
if kwargs.has_key('levels'):
levels = kwargs['levels']
kwargs.pop('levels')
elif contours:
if kwargs.has_key('cntrmass') and kwargs['cntrmass']:
levels = sc.linspace(0., 1., _DEFAULTNCNTR)
elif True in sc.isnan(sc.array(X)):
levels = sc.linspace(sc.nanmin(X), sc.nanmax(X), _DEFAULTNCNTR)
else:
levels = sc.linspace(sc.amin(X), sc.amax(X), _DEFAULTNCNTR)
if kwargs.has_key('cntrmass') and kwargs['cntrmass']:
cntrmass = True
kwargs.pop('cntrmass')
else:
cntrmass = False
if kwargs.has_key('cntrmass'): kwargs.pop('cntrmass')
if kwargs.has_key('cntrcolors'):
cntrcolors = kwargs['cntrcolors']
kwargs.pop('cntrcolors')
elif contours:
cntrcolors = 'k'
if kwargs.has_key('cntrlabel') and kwargs['cntrlabel']:
cntrlabel = True
kwargs.pop('cntrlabel')
else:
cntrlabel = False
if kwargs.has_key('cntrlabel'): kwargs.pop('cntrlabel')
if kwargs.has_key('cntrlw'):
cntrlw = kwargs['cntrlw']
kwargs.pop('cntrlw')
elif contours:
cntrlw = None
if kwargs.has_key('cntrls'):
cntrls = kwargs['cntrls']
kwargs.pop('cntrls')
elif contours:
cntrls = None
if kwargs.has_key('cntrlabelsize'):
cntrlabelsize = kwargs['cntrlabelsize']
kwargs.pop('cntrlabelsize')
elif contours:
cntrlabelsize = None
if kwargs.has_key('cntrlabelcolors'):
cntrlabelcolors = kwargs['cntrlabelcolors']
kwargs.pop('cntrlabelcolors')
elif contours:
cntrlabelcolors = None
if kwargs.has_key('cntrinline'):
cntrinline = kwargs['cntrinline']
kwargs.pop('cntrinline')
elif contours:
cntrinline = None
if kwargs.has_key('retCumImage'):
retCumImage = kwargs['retCumImage']
kwargs.pop('retCumImage')
else:
retCumImage = False
if kwargs.has_key('colorbar'):
cb = kwargs['colorbar']
kwargs.pop('colorbar')
else:
cb = False
if kwargs.has_key('shrink'):
shrink = kwargs['shrink']
kwargs.pop('shrink')
else:
shrink = None
if kwargs.has_key('onedhists'):
onedhists = kwargs['onedhists']
kwargs.pop('onedhists')
else:
onedhists = False
if kwargs.has_key('onedhistcolor'):
onedhistcolor = kwargs['onedhistcolor']
kwargs.pop('onedhistcolor')
else:
onedhistcolor = 'k'
if kwargs.has_key('retAxes'):
retAxes = kwargs['retAxes']
kwargs.pop('retAxes')
else:
retAxes = False
if onedhists:
if overplot: fig = pyplot.gcf()
else: fig = pyplot.figure()
nullfmt = NullFormatter() # no labels
# definitions for the axes
left, width = 0.1, 0.65
bottom, height = 0.1, 0.65
bottom_h = left_h = left + width
rect_scatter = [left, bottom, width, height]
rect_histx = [left, bottom_h, width, 0.2]
rect_histy = [left_h, bottom, 0.2, height]
axScatter = pyplot.axes(rect_scatter)
axHistx = pyplot.axes(rect_histx)
axHisty = pyplot.axes(rect_histy)
# no labels
axHistx.xaxis.set_major_formatter(nullfmt)
axHistx.yaxis.set_major_formatter(nullfmt)
axHisty.xaxis.set_major_formatter(nullfmt)
axHisty.yaxis.set_major_formatter(nullfmt)
fig.sca(axScatter)
ax = pyplot.gca()
ax.set_autoscale_on(False)
out = pyplot.imshow(X, extent=extent, **kwargs)
pyplot.axis(extent)
_add_axislabels(xlabel, ylabel)
_add_ticks()
#Add colorbar
if cb:
if shrink is None:
if kwargs.has_key('aspect'):
shrink = sc.amin([float(kwargs['aspect']) * 0.87, 1.])
else:
shrink = 0.87
CB1 = pyplot.colorbar(out, shrink=shrink)
if not zlabel is None:
if zlabel[0] != '$':
thiszlabel = r'$' + zlabel + '$'
else:
thiszlabel = zlabel
CB1.set_label(zlabel)
if contours or retCumImage:
if kwargs.has_key('aspect'):
aspect = kwargs['aspect']
else:
aspect = None
if kwargs.has_key('origin'):
origin = kwargs['origin']
else:
origin = None
if cntrmass:
#Sum from the top down!
X[sc.isnan(X)] = 0.
sortindx = sc.argsort(X.flatten())[::-1]
cumul = sc.cumsum(sc.sort(X.flatten())[::-1]) / sc.sum(X.flatten())
cntrThis = sc.zeros(sc.prod(X.shape))
cntrThis[sortindx] = cumul
cntrThis = sc.reshape(cntrThis, X.shape)
else:
cntrThis = X
if contours:
cont = pyplot.contour(cntrThis,
levels,
colors=cntrcolors,
linewidths=cntrlw,
extent=extent,
aspect=aspect,
linestyles=cntrls,
origin=origin)
if cntrlabel:
pyplot.clabel(cont,
fontsize=cntrlabelsize,
colors=cntrlabelcolors,
inline=cntrinline)
if noaxes:
ax.set_axis_off()
#Add onedhists
if not onedhists:
if retCumImage:
return cntrThis
elif retAxes:
return pyplot.gca()
else:
return out
histx = sc.nansum(X.T, axis=1) * m.fabs(ylimits[1] - ylimits[0]) / X.shape[
1] #nansum bc nan is *no dens value*
histy = sc.nansum(X.T,
axis=0) * m.fabs(xlimits[1] - xlimits[0]) / X.shape[0]
histx[sc.isnan(histx)] = 0.
histy[sc.isnan(histy)] = 0.
dx = (extent[1] - extent[0]) / float(len(histx))
axHistx.plot(sc.linspace(extent[0] + dx, extent[1] - dx, len(histx)),
histx,
drawstyle='steps-mid',
color=onedhistcolor)
dy = (extent[3] - extent[2]) / float(len(histy))
axHisty.plot(histy,
sc.linspace(extent[2] + dy, extent[3] - dy, len(histy)),
drawstyle='steps-mid',
color=onedhistcolor)
axHistx.set_xlim(axScatter.get_xlim())
axHisty.set_ylim(axScatter.get_ylim())
axHistx.set_ylim(0, 1.2 * sc.amax(histx))
axHisty.set_xlim(0, 1.2 * sc.amax(histy))
if retCumImage:
return cntrThis
elif retAxes:
return (axScatter, axHistx, axHisty)
else:
return out
def veldist_1d_apogee(plotfilename,l=250./180.*m.pi,d=0.25,
ngrid=201,saveDir='../bar/apogee/'):
"""
NAME:
veldist_1d_apogee
PURPOSE:
make a plot showing a 1d velocity distribution in an apogee los
INPUT:
plotfilename - filename for figure
l - Galactic longitude
d - distance from the Sun
ngrid - number of grid-points to calculate the los velocity distribution
on
saveDir - save pickles here
OUTPUT:
Figure in plotfilename
HISTORY:
2010-05-28 - Written - Bovy (NYU)
"""
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
basesavefilename= os.path.join(saveDir,'apogee_')
thissavefilename= basesavefilename+'%.2f_%.2f.sav' % (d,l)
if os.path.exists(thissavefilename):
print "Restoring apogee los-velocity distribution at d,l = %.2f,%.2f" % (d,l)
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
axivlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating apogee los-velocity distribution at d,l = %.2f,%.2f" % (d,l)
potparams= (0.9,0.01,25.*_degtorad,.8,None)
vlosd= predictVlos(vloslinspace,
l=l,
d=d,
distCoord='sun',
pot='bar',beta=0.,
potparams=potparams)
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
potparams= (0.9,0.00,25.*_degtorad,.8,None)
axivlosd= predictVlos(vloslinspace,
l=l,
d=d,
t=0.01,
distCoord='sun',
pot='bar',beta=0.,
potparams=potparams)
axivlosd= axivlosd/(sc.nansum(axivlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
pickle.dump(axivlosd,savefile)
savefile.close()
#Plot
plot.bovy_print()
plot.bovy_plot(vloss,vlosd,'k',
xlabel=r'$v_{\mathrm{los}} / v_0$',zorder=3)
plot.bovy_plot(vloss,axivlosd,ls='-',color='0.5',
overplot=True,zorder=2)
thisax= pyplot.gca()
thisax.set_xlim(vloslinspace[0],vloslinspace[1])
thisax.set_ylim(0.,sc.amax(sc.concatenate((axivlosd,vlosd)))*1.1)
plot.bovy_text(r'$d = %.2f R_0$' % d + '\n'+r'$l = %.0f^\circ$' %(l/m.pi*180.),
top_right=True)
plot.bovy_end_print(plotfilename)
def veldist_1d_convolve(plotfilename,phi=_DEFAULTPHI,R=_DEFAULTR,
ngrid=201,saveDir='../bar/1dvar/'):
"""
NAME:
veldist_1d_convolve
PURPOSE:
make a plot showing the influence of the distance uncertainties
INPUT:
plotfilename - filename for figure
phi - Galactocentric azimuth
R - Galactocentric radius
ngrid - number of grid-points to calculate the los velocity distribution
on
saveDir - save pickles here
OUTPUT:
Figure in plotfilename
HISTORY:
2010-05-15 - Written - Bovy (NYU)
"""
convolves= [0.,0.2,0.3]
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
vlosds= []
basesavefilename= os.path.join(saveDir,'convolve_')
for distsig in convolves:
thissavefilename= basesavefilename+'%.1f.sav' % distsig
if os.path.exists(thissavefilename):
print "Restoring los-velocity distribution at distance uncertainties %.1f" % distsig
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating los-velocity distribution at distance uncertainties %.1f" % distsig
potparams= (0.9,0.01,25.*_degtorad,.8,None)
if distsig == 0.:
vlosd= predictVlos(vloslinspace,
l=phi,
d=R,
distCoord='GCGC',
pot='bar',beta=0.,
potparams=potparams)
else:
vlosd= predictVlosConvolve(vloslinspace,
l=phi,
d=R,
distCoord='GCGC',
pot='bar',beta=0.,
potparams=potparams,
convolve=distsig)
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
savefile.close()
vlosds.append(vlosd)
#Plot
plot.bovy_print()
plot.bovy_plot(vloss,vlosds[0],'k-',zorder=3,
xrange=[vloslinspace[0],vloslinspace[1]],
yrange=[0.,sc.nanmax(sc.array(vlosds).flatten())*1.1],
xlabel=r'$v_{\mathrm{los}} / v_0$')
plot.bovy_plot(vloss,vlosds[1],ls='-',color='0.75',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[2],ls='-',color='0.6',
overplot=True,zorder=2,lw=2.)
#plot.bovy_plot(vloss,vlosds[3],ls='-',color='0.45',
# overplot=True,zorder=2,lw=2.)
plot.bovy_text(r'$\mathrm{distance\ uncertainties}$',title=True)
plot.bovy_text(0.5,.65,r'$\sigma_d = 0$'+'\n'+r'$\sigma_d = 20 \%$'+'\n'+r'$\sigma_d = 30 \%$')
plot.bovy_end_print(plotfilename)
def entropy(x):
"""compute entropy of a discrete random variable"""
return -sp.nansum(x * sp.log(x))
def veldist_1d_df(plotfilename,phi=_DEFAULTPHI,R=_DEFAULTR,
ngrid=201,saveDir='../bar/1dvar/'):
"""
NAME:
veldist_1d_df
PURPOSE:
make a plot showing the influence of the DF
INPUT:
plotfilename - filename for figure
phi - Galactocentric azimuth
R - Galactocentric radius
ngrid - number of grid-points to calculate the los velocity distribution
on
saveDir - save pickles here
OUTPUT:
Figure in plotfilename
HISTORY:
2010-05-15 - Written - Bovy (NYU)
"""
dftypes= ['dehnen','dehnen','dehnen','dehnen','shu']
scalelengths= [1./3.,1./3.,1./4.,4./10.,1./3]
sigscales= [1.,2./3.,3./4.,12./10.,1.]
vloslinspace= (-.9,.9,ngrid)
vloss= sc.linspace(*vloslinspace)
vlosds= []
basesavefilename= os.path.join(saveDir,'df_')
ndfs= len(dftypes)
for ii in range(ndfs):
thissavefilename= basesavefilename+dftypes[ii]+'_%.3f_%.3f.sav' % (scalelengths[ii],sigscales[ii])
if os.path.exists(thissavefilename):
print "Restoring los-velocity distribution at df: "+dftypes[ii]+' %.3f and %.3f' % (scalelengths[ii],sigscales[ii])
savefile= open(thissavefilename,'r')
vlosd= pickle.load(savefile)
savefile.close()
else:
print "Calculating los-velocity distribution at df: "+dftypes[ii]+' %.3f and %.3f' % (scalelengths[ii],sigscales[ii])
potparams= (0.9,0.01,25.*_degtorad,.8,None)
dftype= dftypes[ii]
dfparams= (scalelengths[ii],sigscales[ii],0.2)
vlosd= predictVlos(vloslinspace,
l=phi,
d=R,
distCoord='GCGC',
pot='bar',beta=0.,
potparams=potparams,
dftype=dftype,dfparams=dfparams)
vlosd= vlosd/(sc.nansum(vlosd)*(vloss[1]-vloss[0]))
savefile= open(thissavefilename,'w')
pickle.dump(vlosd,savefile)
savefile.close()
vlosds.append(vlosd)
#Plot
plot.bovy_print()
plot.bovy_plot(vloss,vlosds[0],'k-',zorder=3,
xrange=[vloslinspace[0],vloslinspace[1]],
yrange=[0.,sc.amax(sc.array(vlosds).flatten())*1.1],
xlabel=r'$v_{\mathrm{los}} / v_0$')
plot.bovy_plot(vloss,vlosds[1],ls='-',color='0.75',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[2],ls='-',color='0.60',
overplot=True,zorder=2,lw=2.)
plot.bovy_plot(vloss,vlosds[3],ls='-',color='0.45',
overplot=True,zorder=2,lw=1.5)
plot.bovy_plot(vloss,vlosds[4],ls='-',color='0.3',
overplot=True,zorder=2,lw=1.5)
plot.bovy_text(r'$\mathrm{distribution\ function}$',title=True)
plot.bovy_text(0.53,.3,r'$R_s = 0.25 R_0$'+'\n'
+r'$R_{\sigma} = 2 R_s$'+'\n'
+r'$\mathrm{fiducial}$'+'\n'
+r'$\mathrm{Shu\ DF}$'+'\n'
+r'$R_s = 0.4 R_0$',size=10.)
plot.bovy_end_print(plotfilename)
def fit_px_cest(scn_to_analyse, xval, yval, fitrounds = 1):
scn = sarpy.Scan(scn_to_analyse)
pdata_num = 0
# Defining parameters
freq_list = scn.method.CEST_FreqListPPM
ppm_limit_min = -50
ppm_limit_max = 50
exclude_ppm = 200
normalize_to_ppm = 66.6
possibleNormalizations = [i for i, x in enumerate(freq_list) if numpy.abs(x - normalize_to_ppm) <1E-4]
normalizeTo = possibleNormalizations[-1]
# Get only the frequencies within the ppm_limit
ppm_filtered = [f for f in freq_list if ppm_limit_max > f > ppm_limit_min]
# Exclude the dummy frequencies at the beginning (66.6 ppm)
ppm_filtered = sorted([n for n in ppm_filtered if n!= exclude_ppm])
# Get the index of the good frequencies relative to the original list
ppm_filtered_ind = [freq_list.index(c) for c in ppm_filtered]
# get the freqs that'll be used for water fit
water_fit_freqs = [f for f in ppm_filtered if (numpy.abs(f)< 3.)]
water_fit_freqs_ind = sorted([ppm_filtered.index(c) for c in water_fit_freqs])
# Create some empty arrays
water_shifts = numpy.zeros(shape=(1)) + numpy.nan
new_shifted = numpy.zeros(shape=(1)) + numpy.nan
newstruct = numpy.zeros((1), dtype=[('offset', 'float64'),
('A1', 'float64'),('w1', 'float64'),('p1', 'float64'),
('A2', 'float64'),('w2', 'float64'),('p2', 'float64'),
('A3', 'float64'),('w3', 'float64'),('p3', 'float64'),
('A4', 'float64'),('w4', 'float64'),('p4', 'float64'),
('water_A', 'float64'),('water_w', 'float64'),('water_p', 'float64')])
# Fit count, this counts the number of rounds the data has been fit
fitcount = 0
while fitcount < fitrounds:
# Get the data and normalize it to index of normalize_to_ppm
tmp = scn.pdata[0].data[xval,yval,:][ppm_filtered_ind] / scn.pdata[0].data[xval,yval,normalizeTo]
# First do the water fit and shift the data so water is at 0
shiftParams = fit_water_peak(tmp[water_fit_freqs_ind],water_fit_freqs,allParams=True)
shift = shiftParams[3]
# Interpolating the Y-data so that it gets shifted to the acquired offsets!
if numpy.isfinite(shift):
s_shifted_back = scipy.interp(ppm_filtered, ppm_filtered+shift/2, tmp)
new_shifted = s_shifted_back
else:
print(shift)
pass
if fitcount>0: # Use parameters from last fit
testParams = h_convertBetweenStructArrays(newstruct,toType='array')
else: # Get initial starting parameters
testParams = get_neighbours_starting()
testParams = h_convertBetweenStructArrays(testParams,toType = 'array')
fit_params,cov,infodict,mesg,ier = scipy.optimize.leastsq(
h_residual_Zspectrum_N,
testParams,
args=(new_shifted, ppm_filtered),
full_output = True,
maxfev = 900,
ftol =1E-9)
newstruct['offset'] = fit_params[0]
newstruct['A1'] = fit_params[1]
newstruct['w1'] = fit_params[2]
newstruct['p1'] = fit_params[3]
newstruct['A2'] = fit_params[4]
newstruct['w2'] = fit_params[5]
newstruct['p2'] = fit_params[6]
newstruct['A3'] = fit_params[7]
newstruct['w3'] = fit_params[8]
newstruct['p3'] = fit_params[9]
newstruct['A4'] = fit_params[10]
newstruct['w4'] = fit_params[11]
newstruct['p4'] = fit_params[12]
newstruct['water_A'] = fit_params[13]
newstruct['water_w'] = fit_params[14]
newstruct['water_p'] = fit_params[15]
fitcount+=1
freqs = numpy.arange(-10,10,0.1)
fit_quality = scipy.nansum(numpy.abs(new_shifted - h_zspectrum_N(fit_params,ppm_filtered)))
return {'fit_params':newstruct,
'data': [ppm_filtered, new_shifted],
'fitdata': [freqs, h_zspectrum_N(newstruct, freqs)],
'fit_quality': fit_quality}
def calculate_avg(): #DONE global data_avg global data_std global nb_rows global nb_cols #calculate raw average #--------------------- data_avg = np.zeros((nb_rows,nb_cols)) if len(args.xvgfilenames) > 1: data_std = np.zeros((nb_rows,nb_cols-1)) data_avg[:,0] = first_col for col_index in range(1, nb_cols): col_name = columns_names[col_index-1] #initialise average with first file filename = args.xvgfilenames[0] tmp_col_nb = files_columns[filename]["leg2col"][col_name] tmp_col_avg = files_columns[filename]["data"][:,tmp_col_nb:tmp_col_nb+1] * files_columns[filename]["weight"] * len(args.xvgfilenames) / float(weight_sum) #add columns of following files for f_index in range(1,len(args.xvgfilenames)): filename = args.xvgfilenames[f_index] tmp_col_nb = files_columns[filename]["leg2col"][col_name] tmp_col_avg = np.concatenate([tmp_col_avg,files_columns[filename]["data"][:,tmp_col_nb:tmp_col_nb+1] * files_columns[filename]["weight"] * len(args.xvgfilenames) / float(weight_sum)], axis = 1) if len(args.xvgfilenames) > 1: #calculate weighted average taking into account "nan" #---------------------------------------------------- data_avg[:,col_index] = scipy.stats.nanmean(tmp_col_avg, axis = 1) #calculate unbiased weighted std dev taking into account "nan" #------------------------------------------------------------- #initialise average with first file filename = args.xvgfilenames[0] tmp_col_nb = files_columns[filename]["leg2col"][col_name] tmp_col_std = files_columns[filename]["weight"] * (files_columns[filename]["data"][:,tmp_col_nb:tmp_col_nb+1] - data_avg[:,col_index:col_index+1])**2 tmp_weigh2_sum = files_columns[filename]["weight"]**2 #add columns of following files for f_index in range(1,len(args.xvgfilenames)): filename = args.xvgfilenames[f_index] tmp_col_nb = files_columns[filename]["leg2col"][col_name] tmp_col_std = np.concatenate([tmp_col_std, files_columns[filename]["weight"] * (files_columns[filename]["data"][:,tmp_col_nb:tmp_col_nb+1] - data_avg[:,col_index:col_index+1])**2], axis = 1) tmp_weigh2_sum += files_columns[filename]["weight"]**2 #calculate unbiased standard deviation as defined on wikipedia: https://en.wikipedia.org/wiki/Weighted_variance#Weighted_sample_variance tmp_col_std = np.sqrt(weight_sum / float(weight_sum**2 - tmp_weigh2_sum) * scipy.nansum(tmp_col_std, axis = 1)) data_std[:,col_index-1] = tmp_col_std else: data_avg[:,col_index] = tmp_col_avg[:,0] #update by smoothing #------------------- if args.nb_smoothing > 1: nb_rows = nb_rows - args.nb_smoothing + 1 tmp_data_avg_smoothed = np.zeros((nb_rows,nb_cols)) tmp_data_std_smoothed = np.zeros((nb_rows,nb_cols-1)) tmp_data_avg_smoothed[:,0] = np.transpose(rolling_avg(np.transpose(data_avg[:,0]))[0]) for col_index in range(1, nb_cols): tmp_avg, tmp_std = rolling_avg(np.transpose(data_avg[:,col_index])) tmp_data_avg_smoothed[:,col_index] = np.transpose(tmp_avg) #if one file the std correspond to the fluctuation around the smooth value if len(args.xvgfilenames) == 1: tmp_data_std_smoothed[:,col_index-1] = np.transpose(tmp_std) #if several files the std correspond to the smoothing of the std obtained when calculating the files average else: tmp_data_std_smoothed[:,col_index-1] = np.transpose(rolling_avg(np.transpose(data_std[:,col_index-1]))) data_avg = tmp_data_avg_smoothed data_std = tmp_data_std_smoothed #update by skipping #------------------ if args.nb_skipping > 1 : rows_to_keep = [r for r in range(0,nb_rows) if r%args.nb_skipping ==0] nb_rows = len(rows_to_keep) data_avg = data_avg[rows_to_keep,:] if len(args.xvgfilenames) > 1: data_std = data_std[rows_to_keep,:] #replace nan values if necessary #------------------------------- if args.nan2num != "no": data_avg[np.isnan(data_avg)] = args.nan2num if len(args.xvgfilenames) > 1: data_std[np.isnan(data_std)] = args.nan2num return
def lowerBound(x1, x2, w1, w2, y, tau):
xw = SP.outer(x1, w1)
return SP.nansum(tau * (y**2 + SP.outer(x2, w2) - 2 * xw * y))
def apogee_figures(
plotfilename,
savefilename=None,
bar_angle=25.0,
dt=None,
l=None,
rolr=None,
bar_strength=None,
slope=None,
vlosgrid=201,
dgrid=101,
conditional=False,
dmax=10.0 / 8.0,
):
"""
NAME:
apogee_figures
PURPOSE:
make a vlos-d plot for APOGEE
INPUT:
plotfilename - name of the file the figure will be saved to
savefilename - name of the file the velocity distributions will
be saved to
bar_angle= angle between the GC-Sun lin and the bar major axis
dt= - time to integrate for (in bar-periods)
l= - Galactic longitude
rolr= radius of outer lindblad radius
bar_strength= strength of the bar
slop= slope of the rotation curve (power-law index)
conditional= if True, normalize each velocity distribution independently
OUTPUT:
saves velocity distributions to pickle save file and produces plot
HISTORY:
2011-03-19 - Written - Bovy (NYU)
"""
# Grid
vlosgrid = _VLOSGRID
dgrid = _DGRID
vloslinspace = (-0.9, 0.9, vlosgrid)
vloss = sc.linspace(*vloslinspace)
dlinspace = (0.0001, dmax, dgrid)
ds = sc.linspace(*dlinspace)
# Set up parameters
potparams = (rolr, bar_strength, bar_angle * _degtorad, 0.8, None)
if os.path.exists(savefilename):
savefile = open(savefilename, "rb")
vlosds = pickle.load(savefile)
dd = pickle.load(savefile)
savefile.close()
else:
vlosds = []
dd = 0
while dd < dgrid:
print "Working on %i / %i ..." % (dd + 1, dgrid)
# Calculate vlos for this distance
if dt is None:
vlosd = predictVlos(
vloslinspace, l=(l * _degtorad), d=ds[dd], distCoord="Sun", pot="bar", beta=slope, potparams=potparams
)
else:
vlosd = predictVlos(
vloslinspace,
l=(l * _degtorad),
d=ds[dd],
distCoord="Sun",
pot="bar",
beta=slope,
potparams=potparams,
t=dt,
)
vlosds.append(vlosd)
dd += 1
# Save
savefile = open(savefilename, "wb")
pickle.dump(vlosds, savefile)
pickle.dump(dd, savefile)
savefile.close()
# Plot
if conditional:
newvlosds = []
for vlosd in vlosds:
newvlosds.append(vlosd / (sc.nansum(vlosd) * (vloss[1] - vloss[0])))
vlosds = newvlosds
bovy_plot.bovy_print()
bovy_plot.bovy_dens2d(
sc.array(vlosds).T,
origin="lower",
cmap="gist_yarg",
aspect=0.66,
xlabel=r"$d\ /\ R_0$",
ylabel=r"$(v_{\mathrm{los}} - \vec{v}_c \cdot \vec{d})\ /\ v_0$",
yrange=sc.array([vloslinspace[0], vloslinspace[1]]),
xrange=sc.array([dlinspace[0], dlinspace[1]]),
contours=True,
cntrmass=True,
cntrcolors=["w", "w", "w", "w", "w", "k", "k", "k", "k", "k"],
)
if bar_strength == 0.0:
bovy_plot.bovy_text(r"$l = %i^\circ$" % int(l), top_right=True)
else:
bovy_plot.bovy_text(
r"$l = %i^\circ$" % int(l)
+ "\n"
+ r"$R_{\mathrm{OLR}} = %3.1f$" % rolr
+ "\n"
+ r"$\alpha = %5.3f$" % bar_strength
+ "\n"
+ r"$\phi_{\mathrm{bar}} = %i^\circ$" % int(bar_angle),
top_right=True,
)
bovy_plot.bovy_end_print(plotfilename)
def processdata(self):
""" This will perform the the data processing and create the ACF estimates
for both the data and noise.
Inputs:
timevec - A numpy array of times in seconds where the integration will begin.
inttime - The integration time in seconds.
lagfunc - A function that will make the desired lag products.
Outputs:
DataLags: A dictionary with keys 'Power' 'ACF','RG','Pulses' that holds
the numpy arrays of the data.
NoiseLags: A dictionary with keys 'Power' 'ACF','RG','Pulses' that holds
the numpy arrays of the data.
"""
timevec = self.simparams['Timevec'] + self.timeoffset
inttime = self.simparams['Tint']
# Get array sizes
NNs = int(self.simparams['NNs'])
range_gates = self.simparams['Rangegates']
N_rg = len(range_gates) # take the size
pulse = self.simparams['Pulse']
Pulselen = len(pulse)
N_samps = N_rg + Pulselen - 1
simdtype = self.simparams['dtype']
Ntime = len(timevec)
if 'outangles' in self.simparams.keys():
Nbeams = len(self.simparams['outangles'])
inttime = inttime
else:
Nbeams = len(self.simparams['angles'])
# Choose type of processing
if self.simparams['Pulsetype'].lower() == 'barker':
lagfunc = BarkerLag
Nlag = 1
else:
lagfunc = CenteredLagProduct
Nlag = Pulselen
# initialize output arrays
outdata = sp.zeros((Ntime, Nbeams, N_rg, Nlag), dtype=simdtype)
outaddednoise = sp.zeros((Ntime, Nbeams, N_rg, Nlag), dtype=simdtype)
outnoise = sp.zeros((Ntime, Nbeams, NNs - Pulselen + 1, Nlag),
dtype=simdtype)
pulses = sp.zeros((Ntime, Nbeams))
pulsesN = sp.zeros((Ntime, Nbeams))
timemat = sp.zeros((Ntime, 2))
Ksysvec = self.sensdict['Ksys']
# set up arrays that hold the location of pulses that are to be processed together
infoname = self.datadir / 'INFO.h5'
# Just going to assume that the info file is in the directory
infodict = h52dict(str(infoname))
flist = infodict['Files']
file_list = [str(self.datadir / i) for i in flist]
pulsen_list = infodict['Pulses']
beamn_list = infodict['Beams']
time_list = infodict['Time']
file_loclist = [
ifn * sp.ones(len(ifl)) for ifn, ifl in enumerate(beamn_list)
]
if 'NoiseTime' in infodict.keys():
sridata = True
tnoiselist = infodict['NoiseTime']
nfile_loclist = [
ifn * sp.ones(len(ifl)) for ifn, ifl in enumerate(tnoiselist)
]
else:
sridata = False
pulsen = sp.hstack(pulsen_list).astype(int) # pulse number
beamn = sp.hstack(beamn_list).astype(int) # beam numbers
ptimevec = sp.hstack(time_list).astype(float) # time of each pulse
file_loc = sp.hstack(file_loclist).astype(int) # location in the file
if sridata:
ntimevec = sp.vstack(tnoiselist).astype(float)
nfile_loc = sp.hstack(nfile_loclist).astype(int)
outnoise = sp.zeros((Ntime, Nbeams, NNs - Pulselen + 1, Nlag),
dtype=simdtype)
# run the time loop
print("Forming ACF estimates")
# For each time go through and read only the necisary files
for itn, it in enumerate(timevec):
update_progress(
float(itn) / Ntime, "Time {0:d} of {1:d}".format(itn, Ntime))
# do the book keeping to determine locations of data within the files
cur_tlim = (it, it + inttime)
curcases = sp.logical_and(ptimevec >= cur_tlim[0],
ptimevec < cur_tlim[1])
# SRI data Hack
if sridata:
curcases_n = sp.logical_and(ntimevec[:, 0] >= cur_tlim[0],
ntimevec[:, 0] < cur_tlim[1])
curfileloc_n = nfile_loc[curcases_n]
curfiles_n = set(curfileloc_n)
if not sp.any(curcases):
update_progress(
float(itn) / Ntime,
"No pulses for time {0:d} of {1:d}, lagdata adjusted accordinly"
.format(itn, Ntime))
outdata = outdata[:itn]
outnoise = outnoise[:itn]
pulses = pulses[:itn]
pulsesN = pulsesN[:itn]
timemat = timemat[:itn]
continue
pulseset = set(pulsen[curcases])
poslist = [sp.where(pulsen == item)[0] for item in pulseset]
pos_all = sp.hstack(poslist)
try:
pos_all = sp.hstack(poslist)
curfileloc = file_loc[pos_all]
except:
pdb.set_trace()
# Find the needed files and beam numbers
curfiles = set(curfileloc)
beamlocs = beamn[pos_all]
timemat[itn, 0] = ptimevec[pos_all].min()
timemat[itn, 1] = ptimevec[pos_all].max()
# cur data pulls out all data from all of the beams and posisions
curdata = sp.zeros((len(pos_all), N_samps), dtype=simdtype)
curaddednoise = sp.zeros((len(pos_all), N_samps), dtype=simdtype)
curnoise = sp.zeros((len(pos_all), NNs), dtype=simdtype)
# Open files and get required data
# XXX come up with way to get open up new files not have to reread in data that is already in memory
for ifn in curfiles:
curfileit = [
sp.where(pulsen_list[ifn] == item)[0] for item in pulseset
]
curfileitvec = sp.hstack(curfileit)
ifile = file_list[ifn]
curh5data = h52dict(ifile)
file_arlocs = sp.where(curfileloc == ifn)[0]
curdata[file_arlocs] = curh5data['RawData'][curfileitvec]
curaddednoise[file_arlocs] = curh5data['AddedNoise'].astype(
simdtype)[curfileitvec]
# Read in noise data when you have don't have ACFs
if not sridata:
curnoise[file_arlocs] = curh5data['NoiseData'].astype(
simdtype)[curfileitvec]
#SRI data
if sridata:
curnoise = sp.zeros(
(len(curfileloc_n), Nbeams, NNs - Pulselen + 1, Pulselen),
dtype=simdtype)
for ifn in curfiles_n:
curfileit_n = sp.where(
sp.logical_and(tnoiselist[ifn][:, 0] >= cur_tlim[0],
tnoiselist[ifn][:, 0] < cur_tlim[1]))[0]
ifile = file_list[ifn]
curh5data_n = h52dict(ifile)
file_arlocs = sp.where(curfileloc_n == ifn)[0]
curnoise[file_arlocs] = curh5data_n['NoiseDataACF'][
curfileit_n]
# differentiate between phased arrays and dish antennas
if self.sensdict['Name'].lower() in ['risr', 'pfisr', 'risr-n']:
# After data is read in form lags for each beam
for ibeam in range(Nbeams):
update_progress(
float(itn) / Ntime + float(ibeam) / Ntime / Nbeams,
"Beam {0:d} of {1:d}".format(ibeam, Nbeams))
beamlocstmp = sp.where(beamlocs == ibeam)[0]
pulses[itn, ibeam] = len(beamlocstmp)
outdata[itn,
ibeam] = lagfunc(curdata[beamlocstmp].copy(),
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
if sridata:
pulsesN[itn, ibeam] = len(curnoise)
outnoise[itn, ibeam] = sp.nansum(curnoise[:, ibeam],
axis=0)
else:
pulsesN[itn, ibeam] = len(beamlocstmp)
outnoise[itn, ibeam] = lagfunc(
curnoise[beamlocstmp].copy(),
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
outaddednoise[itn, ibeam] = lagfunc(
curaddednoise[beamlocstmp].copy(),
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
else:
for ibeam, ibeamlist in enumerate(self.simparams['outangles']):
update_progress(
float(itn) / Ntime + float(ibeam) / Ntime / Nbeams,
"Beam {0:d} of {1:d}".format(ibeam, Nbeams))
beamlocstmp = sp.where(sp.in1d(beamlocs, ibeamlist))[0]
curbeams = beamlocs[beamlocstmp]
ksysmat = Ksysvec[curbeams]
ksysmean = Ksysvec[ibeamlist[0]]
inputdata = curdata[beamlocstmp].copy()
noisedata = curnoise[beamlocstmp].copy()
noisedataadd = curaddednoise[beamlocstmp].copy()
ksysmult = ksysmean / sp.tile(ksysmat[:, sp.newaxis],
(1, inputdata.shape[1]))
ksysmultn = ksysmean / sp.tile(ksysmat[:, sp.newaxis],
(1, noisedata.shape[1]))
ksysmultna = ksysmean / sp.tile(ksysmat[:, sp.newaxis],
(1, noisedataadd.shape[1]))
pulses[itn, ibeam] = len(beamlocstmp)
pulsesN[itn, ibeam] = len(beamlocstmp)
outdata[itn,
ibeam] = lagfunc(inputdata * ksysmult,
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
outnoise[itn, ibeam] = lagfunc(
noisedata * ksysmultn,
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
outaddednoise[itn, ibeam] = lagfunc(
noisedataadd * ksysmultna,
numtype=self.simparams['dtype'],
pulse=pulse,
lagtype=self.simparams['lagtype'])
# Create output dictionaries and output data
DataLags = {
'ACF': outdata,
'Pow': outdata[:, :, :, 0].real,
'Pulses': pulses,
'Time': timemat,
'AddedNoiseACF': outaddednoise
}
NoiseLags = {
'ACF': outnoise,
'Pow': outnoise[:, :, :, 0].real,
'Pulses': pulsesN,
'Time': timemat
}
return (DataLags, NoiseLags)
def bovy_dens2d(X,**kwargs):
"""
NAME:
bovy_dens2d
PURPOSE:
plot a 2d density with optional contours
INPUT:
first argument is the density
matplotlib.pyplot.imshow keywords (see http://matplotlib.sourceforge.net/api/axes_api.html#matplotlib.axes.Axes.imshow)
xlabel - (raw string!) x-axis label, LaTeX math mode, no $s needed
ylabel - (raw string!) y-axis label, LaTeX math mode, no $s needed
xrange
yrange
noaxes - don't plot any axes
overplot - if True, overplot
colorbar - if True, add colorbar
shrink= colorbar argument: shrink the colorbar by the factor (optional)
conditional - normalize each column separately (for probability densities, i.e., cntrmass=True)
Contours:
justcontours - if True, only draw contours
contours - if True, draw contours (10 by default)
levels - contour-levels
cntrmass - if True, the density is a probability and the levels are probability masses contained within the contour
cntrcolors - colors for contours (single color or array)
cntrlabel - label the contours
cntrlw, cntrls - linewidths and linestyles for contour
cntrlabelsize, cntrlabelcolors,cntrinline - contour arguments
cntrSmooth - use ndimage.gaussian_filter to smooth before contouring
onedhists - if True, make one-d histograms on the sides
onedhistcolor - histogram color
retAxes= return all Axes instances
retCont= return the contour instance
OUTPUT:
plot to output device, Axes instances depending on input
HISTORY:
2010-03-09 - Written - Bovy (NYU)
"""
overplot= kwargs.pop('overplot',False)
if not overplot:
pyplot.figure()
xlabel= kwargs.pop('xlabel',None)
ylabel= kwargs.pop('ylabel',None)
zlabel= kwargs.pop('zlabel',None)
if 'extent' in kwargs:
extent= kwargs.pop('extent')
else:
xlimits= kwargs.pop('xrange',[0,X.shape[1]])
ylimits= kwargs.pop('yrange',[0,X.shape[0]])
extent= xlimits+ylimits
if not 'aspect' in kwargs:
kwargs['aspect']= (xlimits[1]-xlimits[0])/float(ylimits[1]-ylimits[0])
noaxes= kwargs.pop('noaxes',False)
justcontours= kwargs.pop('justcontours',False)
if ('contours' in kwargs and kwargs['contours']) or \
'levels' in kwargs or justcontours or \
('cntrmass' in kwargs and kwargs['cntrmass']):
contours= True
else:
contours= False
kwargs.pop('contours',None)
if 'levels' in kwargs:
levels= kwargs['levels']
kwargs.pop('levels')
elif contours:
if 'cntrmass' in kwargs and kwargs['cntrmass']:
levels= sc.linspace(0.,1.,_DEFAULTNCNTR)
elif True in sc.isnan(sc.array(X)):
levels= sc.linspace(sc.nanmin(X),sc.nanmax(X),_DEFAULTNCNTR)
else:
levels= sc.linspace(sc.amin(X),sc.amax(X),_DEFAULTNCNTR)
cntrmass= kwargs.pop('cntrmass',False)
conditional= kwargs.pop('conditional',False)
cntrcolors= kwargs.pop('cntrcolors','k')
cntrlabel= kwargs.pop('cntrlabel',False)
cntrlw= kwargs.pop('cntrlw',None)
cntrls= kwargs.pop('cntrls',None)
cntrSmooth= kwargs.pop('cntrSmooth',None)
cntrlabelsize= kwargs.pop('cntrlabelsize',None)
cntrlabelcolors= kwargs.pop('cntrlabelcolors',None)
cntrinline= kwargs.pop('cntrinline',None)
retCumImage= kwargs.pop('retCumImage',False)
cb= kwargs.pop('colorbar',False)
shrink= kwargs.pop('shrink',None)
onedhists= kwargs.pop('onedhists',False)
onedhistcolor= kwargs.pop('onedhistcolor','k')
retAxes= kwargs.pop('retAxes',False)
retCont= kwargs.pop('retCont',False)
if onedhists:
if overplot: fig= pyplot.gcf()
else: fig= pyplot.figure()
nullfmt = NullFormatter() # no labels
# definitions for the axes
left, width = 0.1, 0.65
bottom, height = 0.1, 0.65
bottom_h = left_h = left+width
rect_scatter = [left, bottom, width, height]
rect_histx = [left, bottom_h, width, 0.2]
rect_histy = [left_h, bottom, 0.2, height]
axScatter = pyplot.axes(rect_scatter)
axHistx = pyplot.axes(rect_histx)
axHisty = pyplot.axes(rect_histy)
# no labels
axHistx.xaxis.set_major_formatter(nullfmt)
axHistx.yaxis.set_major_formatter(nullfmt)
axHisty.xaxis.set_major_formatter(nullfmt)
axHisty.yaxis.set_major_formatter(nullfmt)
fig.sca(axScatter)
ax=pyplot.gca()
ax.set_autoscale_on(False)
if conditional:
plotthis= X/sc.tile(sc.sum(X,axis=0),(X.shape[1],1))
else:
plotthis= X
if not justcontours:
out= pyplot.imshow(plotthis,extent=extent,**kwargs)
if not overplot:
pyplot.axis(extent)
_add_axislabels(xlabel,ylabel)
_add_ticks()
#Add colorbar
if cb and not justcontours:
if shrink is None:
shrink= sc.amin([float(kwargs.pop('aspect',1.))*0.87,1.])
CB1= pyplot.colorbar(out,shrink=shrink)
if not zlabel is None:
if zlabel[0] != '$':
thiszlabel=r'$'+zlabel+'$'
else:
thiszlabel=zlabel
CB1.set_label(thiszlabel)
if contours or retCumImage:
aspect= kwargs.get('aspect',None)
origin= kwargs.get('origin',None)
if cntrmass:
#Sum from the top down!
plotthis[sc.isnan(plotthis)]= 0.
sortindx= sc.argsort(plotthis.flatten())[::-1]
cumul= sc.cumsum(sc.sort(plotthis.flatten())[::-1])/sc.sum(plotthis.flatten())
cntrThis= sc.zeros(sc.prod(plotthis.shape))
cntrThis[sortindx]= cumul
cntrThis= sc.reshape(cntrThis,plotthis.shape)
else:
cntrThis= plotthis
if contours:
if not cntrSmooth is None:
cntrThis= ndimage.gaussian_filter(cntrThis,cntrSmooth,
mode='nearest')
cont= pyplot.contour(cntrThis,levels,colors=cntrcolors,
linewidths=cntrlw,extent=extent,aspect=aspect,
linestyles=cntrls,origin=origin)
if cntrlabel:
pyplot.clabel(cont,fontsize=cntrlabelsize,
colors=cntrlabelcolors,
inline=cntrinline)
if noaxes:
ax.set_axis_off()
#Add onedhists
if not onedhists:
if retCumImage:
return cntrThis
elif retAxes:
return pyplot.gca()
elif retCont:
return cont
elif justcontours:
return cntrThis
else:
return out
histx= sc.nansum(X.T,axis=1)*m.fabs(ylimits[1]-ylimits[0])/X.shape[1] #nansum bc nan is *no dens value*
histy= sc.nansum(X.T,axis=0)*m.fabs(xlimits[1]-xlimits[0])/X.shape[0]
histx[sc.isnan(histx)]= 0.
histy[sc.isnan(histy)]= 0.
dx= (extent[1]-extent[0])/float(len(histx))
axHistx.plot(sc.linspace(extent[0]+dx,extent[1]-dx,len(histx)),histx,
drawstyle='steps-mid',color=onedhistcolor)
dy= (extent[3]-extent[2])/float(len(histy))
axHisty.plot(histy,sc.linspace(extent[2]+dy,extent[3]-dy,len(histy)),
drawstyle='steps-mid',color=onedhistcolor)
axHistx.set_xlim( axScatter.get_xlim() )
axHisty.set_ylim( axScatter.get_ylim() )
axHistx.set_ylim( 0, 1.2*sc.amax(histx))
axHisty.set_xlim( 0, 1.2*sc.amax(histy))
if retCumImage:
return cntrThis
elif retAxes:
return (axScatter,axHistx,axHisty)
elif justcontours:
return cntrThis
else:
return out
def bovy_dens2d(X,**kwargs):
"""
NAME:
bovy_dens2d
PURPOSE:
plot a 2d density with optional contours
INPUT:
first argument is the density
matplotlib.pyplot.imshow keywords (see http://matplotlib.sourceforge.net/api/axes_api.html#matplotlib.axes.Axes.imshow)
xlabel - (raw string!) x-axis label, LaTeX math mode, no $s needed
ylabel - (raw string!) y-axis label, LaTeX math mode, no $s needed
xrange
yrange
noaxes - don't plot any axes
overplot - if True, overplot
colorbar - if True, add colorbar
shrink= colorbar argument: shrink the colorbar by the factor (optional)
Contours:
contours - if True, draw contours (10 by default)
levels - contour-levels
cntrmass - if True, the density is a probability and the levels
are probability masses contained within the contour
cntrcolors - colors for contours (single color or array)
cntrlabel - label the contours
cntrlw, cntrls - linewidths and linestyles for contour
cntrlabelsize, cntrlabelcolors,cntrinline - contour arguments
onedhists - if True, make one-d histograms on the sides
onedhistcolor - histogram color
retAxes= return all Axes instances
OUTPUT:
HISTORY:
2010-03-09 - Written - Bovy (NYU)
"""
if kwargs.has_key('overplot'):
overplot= kwargs['overplot']
kwargs.pop('overplot')
else:
overplot= False
if not overplot:
pyplot.figure()
if kwargs.has_key('xlabel'):
xlabel= kwargs['xlabel']
kwargs.pop('xlabel')
else:
xlabel=None
if kwargs.has_key('ylabel'):
ylabel= kwargs['ylabel']
kwargs.pop('ylabel')
else:
ylabel=None
if kwargs.has_key('zlabel'):
zlabel= kwargs['zlabel']
kwargs.pop('zlabel')
else:
zlabel=None
if kwargs.has_key('extent'):
extent= kwargs['extent']
kwargs.pop('extent')
else:
if kwargs.has_key('xrange'):
xlimits=list(kwargs['xrange'])
kwargs.pop('xrange')
else:
xlimits=[0,X.shape[0]]
if kwargs.has_key('yrange'):
ylimits=list(kwargs['yrange'])
kwargs.pop('yrange')
else:
ylimits=[0,X.shape[1]]
extent= xlimits+ylimits
if not kwargs.has_key('aspect'):
kwargs['aspect']= (xlimits[1]-xlimits[0])/float(ylimits[1]-ylimits[0])
if kwargs.has_key('noaxes'):
noaxes= kwargs['noaxes']
kwargs.pop('noaxes')
else:
noaxes= False
if (kwargs.has_key('contours') and kwargs['contours']) or \
kwargs.has_key('levels') or \
(kwargs.has_key('cntrmass') and kwargs['cntrmass']):
contours= True
else:
contours= False
if kwargs.has_key('contours'): kwargs.pop('contours')
if kwargs.has_key('levels'):
levels= kwargs['levels']
kwargs.pop('levels')
elif contours:
if kwargs.has_key('cntrmass') and kwargs['cntrmass']:
levels= sc.linspace(0.,1.,_DEFAULTNCNTR)
elif True in sc.isnan(sc.array(X)):
levels= sc.linspace(sc.nanmin(X),sc.nanmax(X),_DEFAULTNCNTR)
else:
levels= sc.linspace(sc.amin(X),sc.amax(X),_DEFAULTNCNTR)
if kwargs.has_key('cntrmass') and kwargs['cntrmass']:
cntrmass= True
kwargs.pop('cntrmass')
else:
cntrmass= False
if kwargs.has_key('cntrmass'): kwargs.pop('cntrmass')
if kwargs.has_key('cntrcolors'):
cntrcolors= kwargs['cntrcolors']
kwargs.pop('cntrcolors')
elif contours:
cntrcolors='k'
if kwargs.has_key('cntrlabel') and kwargs['cntrlabel']:
cntrlabel= True
kwargs.pop('cntrlabel')
else:
cntrlabel= False
if kwargs.has_key('cntrlabel'): kwargs.pop('cntrlabel')
if kwargs.has_key('cntrlw'):
cntrlw= kwargs['cntrlw']
kwargs.pop('cntrlw')
elif contours:
cntrlw= None
if kwargs.has_key('cntrls'):
cntrls= kwargs['cntrls']
kwargs.pop('cntrls')
elif contours:
cntrls= None
if kwargs.has_key('cntrlabelsize'):
cntrlabelsize= kwargs['cntrlabelsize']
kwargs.pop('cntrlabelsize')
elif contours:
cntrlabelsize= None
if kwargs.has_key('cntrlabelcolors'):
cntrlabelcolors= kwargs['cntrlabelcolors']
kwargs.pop('cntrlabelcolors')
elif contours:
cntrlabelcolors= None
if kwargs.has_key('cntrinline'):
cntrinline= kwargs['cntrinline']
kwargs.pop('cntrinline')
elif contours:
cntrinline= None
if kwargs.has_key('retCumImage'):
retCumImage= kwargs['retCumImage']
kwargs.pop('retCumImage')
else:
retCumImage= False
if kwargs.has_key('colorbar'):
cb= kwargs['colorbar']
kwargs.pop('colorbar')
else:
cb= False
if kwargs.has_key('shrink'):
shrink= kwargs['shrink']
kwargs.pop('shrink')
else:
shrink= None
if kwargs.has_key('onedhists'):
onedhists= kwargs['onedhists']
kwargs.pop('onedhists')
else:
onedhists= False
if kwargs.has_key('onedhistcolor'):
onedhistcolor= kwargs['onedhistcolor']
kwargs.pop('onedhistcolor')
else:
onedhistcolor= 'k'
if kwargs.has_key('retAxes'):
retAxes= kwargs['retAxes']
kwargs.pop('retAxes')
else:
retAxes= False
if onedhists:
if overplot: fig= pyplot.gcf()
else: fig= pyplot.figure()
nullfmt = NullFormatter() # no labels
# definitions for the axes
left, width = 0.1, 0.65
bottom, height = 0.1, 0.65
bottom_h = left_h = left+width
rect_scatter = [left, bottom, width, height]
rect_histx = [left, bottom_h, width, 0.2]
rect_histy = [left_h, bottom, 0.2, height]
axScatter = pyplot.axes(rect_scatter)
axHistx = pyplot.axes(rect_histx)
axHisty = pyplot.axes(rect_histy)
# no labels
axHistx.xaxis.set_major_formatter(nullfmt)
axHistx.yaxis.set_major_formatter(nullfmt)
axHisty.xaxis.set_major_formatter(nullfmt)
axHisty.yaxis.set_major_formatter(nullfmt)
fig.sca(axScatter)
ax=pyplot.gca()
ax.set_autoscale_on(False)
out= pyplot.imshow(X,extent=extent,**kwargs)
pyplot.axis(extent)
_add_axislabels(xlabel,ylabel)
_add_ticks()
#Add colorbar
if cb:
if shrink is None:
if kwargs.has_key('aspect'):
shrink= sc.amin([float(kwargs['aspect'])*0.87,1.])
else:
shrink= 0.87
CB1= pyplot.colorbar(out,shrink=shrink)
if not zlabel is None:
if zlabel[0] != '$':
thiszlabel=r'$'+zlabel+'$'
else:
thiszlabel=zlabel
CB1.set_label(zlabel)
if contours or retCumImage:
if kwargs.has_key('aspect'):
aspect= kwargs['aspect']
else:
aspect= None
if kwargs.has_key('origin'):
origin= kwargs['origin']
else:
origin= None
if cntrmass:
#Sum from the top down!
X[sc.isnan(X)]= 0.
sortindx= sc.argsort(X.flatten())[::-1]
cumul= sc.cumsum(sc.sort(X.flatten())[::-1])/sc.sum(X.flatten())
cntrThis= sc.zeros(sc.prod(X.shape))
cntrThis[sortindx]= cumul
cntrThis= sc.reshape(cntrThis,X.shape)
else:
cntrThis= X
if contours:
cont= pyplot.contour(cntrThis,levels,colors=cntrcolors,
linewidths=cntrlw,extent=extent,aspect=aspect,
linestyles=cntrls,origin=origin)
if cntrlabel:
pyplot.clabel(cont,fontsize=cntrlabelsize,
colors=cntrlabelcolors,
inline=cntrinline)
if noaxes:
ax.set_axis_off()
#Add onedhists
if not onedhists:
if retCumImage:
return cntrThis
elif retAxes:
return pyplot.gca()
else:
return out
histx= sc.nansum(X.T,axis=1)*m.fabs(ylimits[1]-ylimits[0])/X.shape[1] #nansum bc nan is *no dens value*
histy= sc.nansum(X.T,axis=0)*m.fabs(xlimits[1]-xlimits[0])/X.shape[0]
histx[sc.isnan(histx)]= 0.
histy[sc.isnan(histy)]= 0.
dx= (extent[1]-extent[0])/float(len(histx))
axHistx.plot(sc.linspace(extent[0]+dx,extent[1]-dx,len(histx)),histx,
drawstyle='steps-mid',color=onedhistcolor)
dy= (extent[3]-extent[2])/float(len(histy))
axHisty.plot(histy,sc.linspace(extent[2]+dy,extent[3]-dy,len(histy)),
drawstyle='steps-mid',color=onedhistcolor)
axHistx.set_xlim( axScatter.get_xlim() )
axHisty.set_ylim( axScatter.get_ylim() )
axHistx.set_ylim( 0, 1.2*sc.amax(histx))
axHisty.set_xlim( 0, 1.2*sc.amax(histy))
if retCumImage:
return cntrThis
elif retAxes:
return (axScatter,axHistx,axHisty)
else:
return out
def bovy_dens2d(X, **kwargs):
"""
NAME:
bovy_dens2d
PURPOSE:
plot a 2d density with optional contours
INPUT:
first argument is the density
matplotlib.pyplot.imshow keywords (see http://matplotlib.sourceforge.net/api/axes_api.html#matplotlib.axes.Axes.imshow)
xlabel - (raw string!) x-axis label, LaTeX math mode, no $s needed
ylabel - (raw string!) y-axis label, LaTeX math mode, no $s needed
xrange
yrange
noaxes - don't plot any axes
overplot - if True, overplot
colorbar - if True, add colorbar
shrink= colorbar argument: shrink the colorbar by the factor (optional)
conditional - normalize each column separately (for probability densities, i.e., cntrmass=True)
gcf=True does not start a new figure (does change the ranges and labels)
Contours:
justcontours - if True, only draw contours
contours - if True, draw contours (10 by default)
levels - contour-levels
cntrmass - if True, the density is a probability and the levels are probability masses contained within the contour
cntrcolors - colors for contours (single color or array)
cntrlabel - label the contours
cntrlw, cntrls - linewidths and linestyles for contour
cntrlabelsize, cntrlabelcolors,cntrinline - contour arguments
cntrSmooth - use ndimage.gaussian_filter to smooth before contouring
onedhists - if True, make one-d histograms on the sides
onedhistcolor - histogram color
retAxes= return all Axes instances
retCont= return the contour instance
OUTPUT:
plot to output device, Axes instances depending on input
HISTORY:
2010-03-09 - Written - Bovy (NYU)
"""
overplot = kwargs.pop('overplot', False)
gcf = kwargs.pop('gcf', False)
if not overplot and not gcf:
pyplot.figure()
xlabel = kwargs.pop('xlabel', None)
ylabel = kwargs.pop('ylabel', None)
zlabel = kwargs.pop('zlabel', None)
if 'extent' in kwargs:
extent = kwargs.pop('extent')
else:
xlimits = kwargs.pop('xrange', [0, X.shape[1]])
ylimits = kwargs.pop('yrange', [0, X.shape[0]])
extent = xlimits + ylimits
if not 'aspect' in kwargs:
kwargs['aspect'] = (xlimits[1] - xlimits[0]) / float(ylimits[1] -
ylimits[0])
noaxes = kwargs.pop('noaxes', False)
justcontours = kwargs.pop('justcontours', False)
if ('contours' in kwargs and kwargs['contours']) or \
'levels' in kwargs or justcontours or \
('cntrmass' in kwargs and kwargs['cntrmass']):
contours = True
else:
contours = False
kwargs.pop('contours', None)
if 'levels' in kwargs:
levels = kwargs['levels']
kwargs.pop('levels')
elif contours:
if 'cntrmass' in kwargs and kwargs['cntrmass']:
levels = sc.linspace(0., 1., _DEFAULTNCNTR)
elif True in sc.isnan(sc.array(X)):
levels = sc.linspace(sc.nanmin(X), sc.nanmax(X), _DEFAULTNCNTR)
else:
levels = sc.linspace(sc.amin(X), sc.amax(X), _DEFAULTNCNTR)
cntrmass = kwargs.pop('cntrmass', False)
conditional = kwargs.pop('conditional', False)
cntrcolors = kwargs.pop('cntrcolors', 'k')
cntrlabel = kwargs.pop('cntrlabel', False)
cntrlw = kwargs.pop('cntrlw', None)
cntrls = kwargs.pop('cntrls', None)
cntrSmooth = kwargs.pop('cntrSmooth', None)
cntrlabelsize = kwargs.pop('cntrlabelsize', None)
cntrlabelcolors = kwargs.pop('cntrlabelcolors', None)
cntrinline = kwargs.pop('cntrinline', None)
retCumImage = kwargs.pop('retCumImage', False)
cb = kwargs.pop('colorbar', False)
shrink = kwargs.pop('shrink', None)
onedhists = kwargs.pop('onedhists', False)
onedhistcolor = kwargs.pop('onedhistcolor', 'k')
retAxes = kwargs.pop('retAxes', False)
retCont = kwargs.pop('retCont', False)
if onedhists:
if overplot or gcf: fig = pyplot.gcf()
else: fig = pyplot.figure()
nullfmt = NullFormatter() # no labels
# definitions for the axes
left, width = 0.1, 0.65
bottom, height = 0.1, 0.65
bottom_h = left_h = left + width
rect_scatter = [left, bottom, width, height]
rect_histx = [left, bottom_h, width, 0.2]
rect_histy = [left_h, bottom, 0.2, height]
axScatter = pyplot.axes(rect_scatter)
axHistx = pyplot.axes(rect_histx)
axHisty = pyplot.axes(rect_histy)
# no labels
axHistx.xaxis.set_major_formatter(nullfmt)
axHistx.yaxis.set_major_formatter(nullfmt)
axHisty.xaxis.set_major_formatter(nullfmt)
axHisty.yaxis.set_major_formatter(nullfmt)
fig.sca(axScatter)
ax = pyplot.gca()
ax.set_autoscale_on(False)
if conditional:
plotthis = X / sc.tile(sc.sum(X, axis=0), (X.shape[1], 1))
else:
plotthis = X
if not justcontours:
out = pyplot.imshow(plotthis, extent=extent, **kwargs)
if not overplot:
pyplot.axis(extent)
_add_axislabels(xlabel, ylabel)
_add_ticks()
#Add colorbar
if cb and not justcontours:
if shrink is None:
shrink = sc.amin([float(kwargs.pop('aspect', 1.)) * 0.87, 1.])
CB1 = pyplot.colorbar(out, shrink=shrink)
if not zlabel is None:
if zlabel[0] != '$':
thiszlabel = r'$' + zlabel + '$'
else:
thiszlabel = zlabel
CB1.set_label(thiszlabel)
if contours or retCumImage:
aspect = kwargs.get('aspect', None)
origin = kwargs.get('origin', None)
if cntrmass:
#Sum from the top down!
plotthis[sc.isnan(plotthis)] = 0.
sortindx = sc.argsort(plotthis.flatten())[::-1]
cumul = sc.cumsum(sc.sort(plotthis.flatten())[::-1]) / sc.sum(
plotthis.flatten())
cntrThis = sc.zeros(sc.prod(plotthis.shape))
cntrThis[sortindx] = cumul
cntrThis = sc.reshape(cntrThis, plotthis.shape)
else:
cntrThis = plotthis
if contours:
if not cntrSmooth is None:
cntrThis = ndimage.gaussian_filter(cntrThis,
cntrSmooth,
mode='nearest')
cont = pyplot.contour(cntrThis,
levels,
colors=cntrcolors,
linewidths=cntrlw,
extent=extent,
aspect=aspect,
linestyles=cntrls,
origin=origin)
if cntrlabel:
pyplot.clabel(cont,
fontsize=cntrlabelsize,
colors=cntrlabelcolors,
inline=cntrinline)
if noaxes:
ax.set_axis_off()
#Add onedhists
if not onedhists:
if retCumImage:
return cntrThis
elif retAxes:
return pyplot.gca()
elif retCont:
return cont
elif justcontours:
return cntrThis
else:
return out
histx = sc.nansum(X.T, axis=1) * m.fabs(ylimits[1] - ylimits[0]) / X.shape[
1] #nansum bc nan is *no dens value*
histy = sc.nansum(X.T,
axis=0) * m.fabs(xlimits[1] - xlimits[0]) / X.shape[0]
histx[sc.isnan(histx)] = 0.
histy[sc.isnan(histy)] = 0.
dx = (extent[1] - extent[0]) / float(len(histx))
axHistx.plot(sc.linspace(extent[0] + dx, extent[1] - dx, len(histx)),
histx,
drawstyle='steps-mid',
color=onedhistcolor)
dy = (extent[3] - extent[2]) / float(len(histy))
axHisty.plot(histy,
sc.linspace(extent[2] + dy, extent[3] - dy, len(histy)),
drawstyle='steps-mid',
color=onedhistcolor)
axHistx.set_xlim(axScatter.get_xlim())
axHisty.set_ylim(axScatter.get_ylim())
axHistx.set_ylim(0, 1.2 * sc.amax(histx))
axHisty.set_xlim(0, 1.2 * sc.amax(histy))
if retCumImage:
return cntrThis
elif retAxes:
return (axScatter, axHistx, axHisty)
elif justcontours:
return cntrThis
else:
return out
def processdata(self):
""" This will perform the the data processing and create the ACF estimates
for both the data and noise.
Inputs:
timevec - A numpy array of times in seconds where the integration will begin.
inttime - The integration time in seconds.
lagfunc - A function that will make the desired lag products.
Outputs:
DataLags: A dictionary with keys 'Power' 'ACF','RG','Pulses' that holds
the numpy arrays of the data.
NoiseLags: A dictionary with keys 'Power' 'ACF','RG','Pulses' that holds
the numpy arrays of the data.
"""
timevec = self.simparams['Timevec'] +self.timeoffset
inttime = self.simparams['Tint']
# Get array sizes
NNs = int(self.simparams['NNs'])
range_gates = self.simparams['Rangegates']
N_rg = len(range_gates)# take the size
pulse = self.simparams['Pulse']
Pulselen = len(pulse)
N_samps = N_rg +Pulselen-1
simdtype = self.simparams['dtype']
Ntime=len(timevec)
if 'outangles' in self.simparams.keys():
Nbeams = len(self.simparams['outangles'])
inttime = inttime
else:
Nbeams = len(self.simparams['angles'])
# Choose type of processing
if self.simparams['Pulsetype'].lower() == 'barker':
lagfunc=BarkerLag
Nlag=1
else:
lagfunc=CenteredLagProduct
Nlag=Pulselen
# initialize output arrays
outdata = sp.zeros((Ntime,Nbeams,N_rg,Nlag),dtype=simdtype)
outaddednoise = sp.zeros((Ntime,Nbeams,N_rg,Nlag),dtype=simdtype)
outnoise = sp.zeros((Ntime,Nbeams,NNs-Pulselen+1,Nlag),dtype=simdtype)
pulses = sp.zeros((Ntime,Nbeams))
pulsesN = sp.zeros((Ntime,Nbeams))
timemat = sp.zeros((Ntime,2))
Ksysvec = self.sensdict['Ksys']
# set up arrays that hold the location of pulses that are to be processed together
infoname = self.datadir / 'INFO.h5'
# Just going to assume that the info file is in the directory
infodict =h52dict(str(infoname))
flist = infodict['Files']
file_list = [str(self.datadir/i) for i in flist]
pulsen_list = infodict['Pulses']
beamn_list = infodict['Beams']
time_list = infodict['Time']
file_loclist = [ifn*sp.ones(len(ifl)) for ifn,ifl in enumerate(beamn_list)]
if 'NoiseTime'in infodict.keys():
sridata = True
tnoiselist=infodict['NoiseTime']
nfile_loclist=[ifn*sp.ones(len(ifl)) for ifn,ifl in enumerate(tnoiselist)]
else:
sridata=False
pulsen = sp.hstack(pulsen_list).astype(int)# pulse number
beamn = sp.hstack(beamn_list).astype(int)# beam numbers
ptimevec = sp.hstack(time_list).astype(float)# time of each pulse
file_loc = sp.hstack(file_loclist).astype(int)# location in the file
if sridata:
ntimevec = sp.vstack(tnoiselist).astype(float)
nfile_loc = sp.hstack(nfile_loclist).astype(int)
outnoise = sp.zeros((Ntime,Nbeams,NNs-Pulselen+1,Nlag),dtype=simdtype)
# run the time loop
print("Forming ACF estimates")
# For each time go through and read only the necisary files
for itn,it in enumerate(timevec):
print("\tTime {0:d} of {1:d}".format(itn,Ntime))
# do the book keeping to determine locations of data within the files
cur_tlim = (it,it+inttime)
curcases = sp.logical_and(ptimevec>=cur_tlim[0],ptimevec<cur_tlim[1])
# SRI data Hack
if sridata:
curcases_n=sp.logical_and(ntimevec[:,0]>=cur_tlim[0],ntimevec[:,0]<cur_tlim[1])
curfileloc_n = nfile_loc[curcases_n]
curfiles_n = set(curfileloc_n)
if not sp.any(curcases):
print("\tNo pulses for time {0:d} of {1:d}, lagdata adjusted accordinly".format(itn,Ntime))
outdata = outdata[:itn]
outnoise = outnoise[:itn]
pulses=pulses[:itn]
pulsesN=pulsesN[:itn]
timemat=timemat[:itn]
continue
pulseset = set(pulsen[curcases])
poslist = [sp.where(pulsen==item)[0] for item in pulseset ]
pos_all = sp.hstack(poslist)
try:
pos_all = sp.hstack(poslist)
curfileloc = file_loc[pos_all]
except:
pdb.set_trace()
# Find the needed files and beam numbers
curfiles = set(curfileloc)
beamlocs = beamn[pos_all]
timemat[itn,0] = ptimevec[pos_all].min()
timemat[itn,1]=ptimevec[pos_all].max()
# cur data pulls out all data from all of the beams and posisions
curdata = sp.zeros((len(pos_all),N_samps),dtype = simdtype)
curaddednoise = sp.zeros((len(pos_all),N_samps),dtype = simdtype)
curnoise = sp.zeros((len(pos_all),NNs),dtype = simdtype)
# Open files and get required data
# XXX come up with way to get open up new files not have to reread in data that is already in memory
for ifn in curfiles:
curfileit = [sp.where(pulsen_list[ifn]==item)[0] for item in pulseset ]
curfileitvec = sp.hstack(curfileit)
ifile = file_list[ifn]
curh5data = h52dict(ifile)
file_arlocs = sp.where(curfileloc==ifn)[0]
curdata[file_arlocs] = curh5data['RawData'][curfileitvec]
curaddednoise[file_arlocs] = curh5data['AddedNoise'].astype(simdtype)[curfileitvec]
# Read in noise data when you have don't have ACFs
if not sridata:
curnoise[file_arlocs] = curh5data['NoiseData'].astype(simdtype)[curfileitvec]
#SRI data
if sridata:
curnoise = sp.zeros((len(curfileloc_n),Nbeams,NNs-Pulselen+1,Pulselen),dtype = simdtype)
for ifn in curfiles_n:
curfileit_n = sp.where(sp.logical_and(tnoiselist[ifn][:,0]>=cur_tlim[0],tnoiselist[ifn][:,0]<cur_tlim[1]))[0]
ifile=file_list[ifn]
curh5data_n = h52dict(ifile)
file_arlocs = sp.where(curfileloc_n==ifn)[0]
curnoise[file_arlocs] = curh5data_n['NoiseDataACF'][curfileit_n]
# differentiate between phased arrays and dish antennas
if self.sensdict['Name'].lower() in ['risr','pfisr','risr-n']:
# After data is read in form lags for each beam
for ibeam in range(Nbeams):
print("\t\tBeam {0:d} of {0:d}".format(ibeam,Nbeams))
beamlocstmp = sp.where(beamlocs==ibeam)[0]
pulses[itn,ibeam] = len(beamlocstmp)
outdata[itn,ibeam] = lagfunc(curdata[beamlocstmp].copy(),
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
if sridata:
pulsesN[itn,ibeam] = len(curnoise)
outnoise[itn,ibeam] = sp.nansum(curnoise[:,ibeam],axis=0)
else:
pulsesN[itn,ibeam] = len(beamlocstmp)
outnoise[itn,ibeam] = lagfunc(curnoise[beamlocstmp].copy(),
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
outaddednoise[itn,ibeam] = lagfunc(curaddednoise[beamlocstmp].copy(),
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
else:
for ibeam,ibeamlist in enumerate(self.simparams['outangles']):
print("\t\tBeam {0:d} of {1:d}".format(ibeam,Nbeams))
beamlocstmp = sp.where(sp.in1d(beamlocs,ibeamlist))[0]
curbeams = beamlocs[beamlocstmp]
ksysmat = Ksysvec[curbeams]
ksysmean = Ksysvec[ibeamlist[0]]
inputdata = curdata[beamlocstmp].copy()
noisedata = curnoise[beamlocstmp].copy()
noisedataadd=curaddednoise[beamlocstmp].copy()
ksysmult = ksysmean/sp.tile(ksysmat[:,sp.newaxis],(1,inputdata.shape[1]))
ksysmultn = ksysmean/sp.tile(ksysmat[:,sp.newaxis],(1,noisedata.shape[1]))
ksysmultna = ksysmean/sp.tile(ksysmat[:,sp.newaxis],(1,noisedataadd.shape[1]))
pulses[itn,ibeam] = len(beamlocstmp)
pulsesN[itn,ibeam] = len(beamlocstmp)
outdata[itn,ibeam] = lagfunc(inputdata *ksysmult,
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
outnoise[itn,ibeam] = lagfunc(noisedata*ksysmultn,
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
outaddednoise[itn,ibeam] = lagfunc(noisedataadd*ksysmultna,
numtype=self.simparams['dtype'], pulse=pulse,lagtype=self.simparams['lagtype'])
# Create output dictionaries and output data
DataLags = {'ACF':outdata,'Pow':outdata[:,:,:,0].real,'Pulses':pulses,
'Time':timemat,'AddedNoiseACF':outaddednoise}
NoiseLags = {'ACF':outnoise,'Pow':outnoise[:,:,:,0].real,'Pulses':pulsesN,'Time':timemat}
return(DataLags,NoiseLags)
