def energy(self, x):
r"""
Calculates the energy of a pattern ``x`` according to the
Hopfield network.
The energy of a pattern ``x`` computes as:
.. math:: E(x) = -\frac{1}{2} x^T \cdot [J - \text{diag}(J)] \cdot x + \theta\cdot x
Parameters
----------
X : numpy array
(M, N)-dim array of binary input patterns of length N,
where N is the number of nodes in the network
Returns
-------
energy : float
Energy of input pattern according to Hopfield network.
"""
X = np.atleast_2d(x)
energies = []
for x in X:
energies.append(-.5 * np.dot(x, np.dot(self._J - np.diag(self._J.diagonal()), x)) + np.dot(self._theta, x))
if len(energies) == 1:
return np.array(energies[0], dtype = np.double)
else:
return np.array(energies, dtype = np.double)
def policy_backward(eph, epdlogp):
""" backward pass. (eph is array of intermediate hidden states) """
dW2 = np.dot(eph.T, epdlogp).ravel()
dh = np.outer(epdlogp, model['W2'])
dh[eph <= 0] = 0 # backpro prelu
dW1 = np.dot(dh.T, epx)
return {'W1':dW1, 'W2':dW2}
def H(s, tres, QAA, QFF, QAF, QFA, kF):
"""
Evaluate H(s) funtion (Eq. 54, HJC92).
HAA(s) = QAA + QAF * (s*I - QFF) ^(-1) * (I - exp(-(s*I - QFF) * tau)) * QFA
To evaluate HFF(s) exhange A by F and F by A in function call.
Parameters
----------
s : float
Laplace transform argument.
tres : float
Time resolution (dead time).
QAA : array_like, shape (kA, kA)
QFF : array_like, shape (kF, kF)
QAF : array_like, shape (kA, kF)
QFA : array_like, shape (kF, kA)
QAA, QFF, QAF, QFA - submatrices of Q.
kF : int
A number of shut states in kinetic scheme.
Returns
-------
H : ndarray, shape (kA, kA)
"""
IF = np.eye(kF)
XFF = s * IF - QFF
invXFF = nplin.inv(XFF)
expXFF = expQt(-XFF, tres)
H = QAA + np.dot(np.dot(np.dot(QAF, invXFF), IF - expXFF), QFA)
return H
def objective_gradient(self, X, J=None, return_K=False):
"""
Computes MPF objective gradient on input data X given coupling
strengths J.
Parameters
----------
X : numpy array
(M, N)-dim array of binary input patterns of length N,
where N is the number of nodes in the network
J : numpy array, optional
Coupling matrix of size N x N, where N denotes the number
of nodes in the network (default None)
return_K : bool, optional
Flag wether to return K (default False)
Returns
-------
dJ [, K] : numpy array [, numpy array]
Update to coupling matrix J [and K if return_K is True]
"""
if J is None:
J = self._J
J[np.eye(self._N, dtype=bool)] = -2 * self._theta
X = np.atleast_2d(X)
M, N = X.shape
S = 2 * X - 1
Kfull = np.exp(-S * np.dot(X, J.T) + .5 * np.diag(J)[None, :])
dJ = -np.dot(X.T, Kfull * S) + .5 * np.diag(Kfull.sum(0))
if self._symmetric is True:
dJ = .5 * (dJ + dJ.T)
if return_K:
return Kfull.sum() / M, dJ / M
else:
return dJ / M
def CHSvec(roots, tres, tcrit, QFA, kA, expQAA, phiF, R):
"""
Calculate initial and final CHS vectors for HJC likelihood function
(Eqs. 5.5 or 5.7, CHS96).
Parameters
----------
roots : array_like, shape (1, kA)
Roots of the asymptotic pdf.
tres : float
Time resolution (dead time).
tcrit : float
Critical time.
QFA : array_like, shape(kF, kA)
kA : int
expQAA : array_like, shape(kA, kA)
phiF : array_like, shape(1, kF)
R : array_like, shape(kF, kF, kF)
Returns
-------
start : ndarray, shape (1, kA)
CHS start vector (Eq. 5.11, CHS96).
end : ndarray, shape (kF, 1)
CHS end vector (Eq. 5.8, CHS96).
"""
H = HAF(roots, tres, tcrit, QFA, expQAA, R)
u = np.ones((kA, 1))
start = np.dot(phiF, H) / np.dot(np.dot(phiF, H), u)
end = np.dot(H, u)
return start, end
def phiSub(Q, k1, k2):
"""
Calculate initial vector for any subset.
Parameters
----------
mec : dcpyps.Mechanism
The mechanism to be analysed.
Returns
-------
phi : ndarray, shape (kA)
"""
u = np.ones((k2 - k1 + 1, 1))
p = pinf(Q)
p1, p2, p3 = np.hsplit(p,(k1, k2+1))
p1c = np.hstack((p1, p3))
#Q = Q.copy()
Q1, Q2, Q3 = np.hsplit(Q,(k1, k2+1))
Q21, Q22, Q23 = np.hsplit(Q2.transpose(),(k1, k2+1))
Q22c = Q22.copy()
Q12 = np.vstack((Q21.transpose(), Q23.transpose()))
nom = np.dot(p1c, Q12)
denom = np.dot(nom,u)
phi = nom / denom
return phi, Q22c
def phiHJC(eGAF, eGFA, kA):
"""
Calculate initial HJC vector for openings by solving
phi*(I-eGAF*eGFA)=0 (Eq. 10, HJC92)
For shuttings exhange A by F and F by A in function call.
Parameters
----------
eGAF : array_like, shape (kA, kF)
eGFA : array_like, shape (kF, kA)
kA : int
A number of open states in kinetic scheme.
kF : int
A number of shut states in kinetic scheme.
Returns
-------
phi : array_like, shape (kA)
"""
if kA == 1:
phi = np.array([1])
else:
Qsub = np.eye(kA) - np.dot(eGAF, eGFA)
u = np.ones((kA, 1))
S = np.concatenate((Qsub, u), 1)
phi = np.dot(u.transpose(), nplin.inv(np.dot(S, S.transpose())))[0]
return phi
def iGs(Q, kA, kB):
r"""
Calculate GBA and GAB matrices (Eq. 1.25, CH82).
Calculate also GFA and GAF if kF is given instead of kB.
.. math::
\bs{G}_\cl{BA} &= -\bs{Q}_\cl{BB}^{-1} \bs{Q}_\cl{BA} \\
\bs{G}_\cl{AB} &= -\bs{Q}_\cl{AA}^{-1} \bs{Q}_\cl{AB}
Parameters
----------
Q : array_like, shape (k, k)
kA : int
A number of open states in kinetic scheme.
kB : int
A number of short lived shut states in kinetic scheme.
Returns
-------
GAB : ndarray, shape (kA, kB)
GBA : ndarray, shape (kB, kA)
"""
kE = kA + kB
QBB = Q[kA:kE, kA:kE]
QBA = Q[kA:kE, 0:kA]
QAA = Q[0:kA, 0:kA]
QAB = Q[0:kA, kA:kE]
GAB = np.dot(nplin.inv(-1 * QAA), QAB)
GBA = np.dot(nplin.inv(-1 * QBB), QBA)
return GAB, GBA
def eGs(GAF, GFA, kA, kF, expQFF):
"""
Calculate eGAF, probabilities from transitions from apparently open to
shut states regardles of when the transition occurs. Thease are Laplace
transform of eGAF(t) when s=0. Used to calculat initial HJC vectors (HJC92).
eGAF*(s=0) = (I - GAF * (I - expQFF) * GFA)^-1 * GAF * expQFF
To caculate eGFA exhange A by F and F by A in function call.
Parameters
----------
GAF : array_like, shape (kA, kF)
GFA : array_like, shape (kF, kA)
kA : int
A number of open states in kinetic scheme.
kF : int
A number of shut states in kinetic scheme.
Returns
-------
eGAF : array_like, shape (kA, kF)
"""
temp = np.eye(kA) - np.dot(np.dot(GAF, np.eye(kF) - expQFF), GFA)
eGAF = np.dot(np.dot(nplin.inv(temp), GAF), expQFF)
return eGAF
def backprop(self, x, y):
activation = x
activations = [x]
zs = []
for weight, bias in zip(self.weights, self.biases):
z = np.dot(activation, weight)+bias
zs.append(z)
activation = sigmoid(z)
activations.append(activation)
delta = (activation-y)*sigmoid_prime(zs[-1])
nabla_weights = [np.zeros(w.shape) for w in self.weights]
nabla_biases = [np.zeros(b.shape) for b in self.biases]
nabla_weights[-1] = np.dot(activations[-2].transpose(), delta)
nabla_biases[-1] = delta
for l in xrange(2, len(self.layers)):
delta = np.dot(delta, self.weights[-l+1].transpose())*sigmoid_prime(zs[-l])
nabla_weights[-l] = np.dot(activations[-l-1].transpose(), delta)
nabla_biases[-l] = delta
return (nabla_weights, nabla_biases)
def read_abinit(filename):
with open(filename) as f:
abinit_in = AbinitIn(f.readlines())
tags = abinit_in.get_variables()
acell = tags['acell']
rprim = tags['rprim'].T
scalecart = tags['scalecart']
lattice = rprim * acell
if scalecart is not None:
for i in range(3):
lattice[i] *= scalecart[i]
if tags['xcart'] is not None:
pos_bohr = np.transpose(tags['xcart'])
positions = np.dot(np.linalg.inv(lattice), pos_bohr).T
elif tags['xangst'] is not None:
pos_bohr = np.transpose(tags['xangst']) / Bohr
positions = np.dot(np.linalg.inv(lattice), pos_bohr).T
elif tags['xred'] is not None:
positions = tags['xred']
numbers = [tags['znucl'][x - 1] for x in tags['typat']]
return Atoms(numbers=numbers,
cell=lattice.T,
scaled_positions=positions)
def vertex_transform1(vertex):
"""
This transform was applied on the original surface.
"""
return np.dot(rotation_matrix(np.array([0.0, 0.0, 1.0]), math.pi),
np.dot(rotation_matrix(np.array([1.0, 0.0, 0.0]), -math.pi / 1.6),
np.array([float(x) / 1.5 for x in vertex[:3]]) + np.array([0.0, -40.0, 20.0])))
def test_grid_search_precomputed_kernel():
"""Test that grid search works when the input features are given in the
form of a precomputed kernel matrix """
X_, y_ = make_classification(n_samples=200, n_features=100, random_state=0)
# compute the training kernel matrix corresponding to the linear kernel
K_train = np.dot(X_[:180], X_[:180].T)
y_train = y_[:180]
clf = SVC(kernel='precomputed')
cv = GridSearchCV(clf, {'C': [0.1, 1.0]})
cv.fit(K_train, y_train)
assert_true(cv.best_score_ >= 0)
# compute the test kernel matrix
K_test = np.dot(X_[180:], X_[:180].T)
y_test = y_[180:]
y_pred = cv.predict(K_test)
assert_true(np.mean(y_pred == y_test) >= 0)
# test error is raised when the precomputed kernel is not array-like
# or sparse
assert_raises(ValueError, cv.fit, K_train.tolist(), y_train)
def updateParameters(self, articlePicked, click, userID): self.counter +=1 self.Wlong = vectorize(self.W) featureDimension = len(articlePicked.featureVector) T_X = vectorize(np.outer(articlePicked.featureVector, self.W.T[userID])) self.A += np.outer(T_X, T_X) self.b += click*T_X self.AInv = np.linalg.inv(self.A) self.UserTheta = matrixize(np.dot(self.AInv, self.b), len(articlePicked.featureVector)) Xi_Matirx = np.zeros(shape = (featureDimension, self.userNum)) Xi_Matirx.T[userID] = articlePicked.featureVector W_X = vectorize( np.dot(np.transpose(self.UserTheta), Xi_Matirx)) self.batchGradient +=evaluateGradient(W_X, click, self.Wlong, self.lambda_, self.regu ) if self.counter%self.windowSize ==0: self.Wlong -= 1/(float(self.counter/self.windowSize)+1)*self.batchGradient self.W = matrixize(self.Wlong, self.userNum) self.W = normalize(self.W, axis=0, norm='l1') #print 'SVD', self.W self.batchGradient = np.zeros(self.userNum*self.userNum) # Use Ridge regression to fit W ''' plt.pcolor(self.W_b) plt.colorbar plt.show() ''' if self.W.T[userID].any() <0 or self.W.T[userID].any()>1: print self.W.T[userID] self.CoTheta = np.dot(self.UserTheta, self.W) self.BigW = np.kron(np.transpose(self.W), np.identity(n=len(articlePicked.featureVector))) self.CCA = np.dot(np.dot(self.BigW , self.AInv), np.transpose(self.BigW)) self.BigTheta = np.kron(np.identity(n=self.userNum) , self.UserTheta)
def fitToData(self, data):
'''
param data: numpy array where [:,0] is x and [:,1] is y
'''
x = data[:, 0][:, np.newaxis]
y = data[:, 1][:, np.newaxis]
D = np.hstack((x*x, x*y, y*y, x, y, np.ones_like(x)))
S = np.dot(D.T, D)
C = np.zeros([6, 6])
C[0, 2] = C[2, 0] = 2; C[1, 1] = -1
E, V = eig(np.dot(inv(S), C))
n = np.argmax(np.abs(E))
self.parameters = V[:, n]
axes = self.ellipse_axis_length()
self.a = axes[0]
self.b = axes[1]
self.angle = self.ellipse_angle_of_rotation()
if not self.a or not self.b or self.parameters == None or np.iscomplexobj(self.parameters) or \
math.isnan(self.a) or math.isnan(self.b) or math.isnan(self.ellipse_center()[0]) or \
np.iscomplex(self.ellipse_center()[0]) or np.iscomplex(self.a) or np.iscomplex(self.b) or \
np.iscomplexobj(self.angle):
self.a = 0
self.b = 0
self.parameters = [0.0, 0.0, 0.0, 0.0, 0.0, 0.0]
self.angle = 0
self.error = True
def test_primal_dual_relationship():
y = y_diabetes.reshape(-1, 1)
coef = _solve_cholesky(X_diabetes, y, alpha=[1e-2])
K = np.dot(X_diabetes, X_diabetes.T)
dual_coef = _solve_cholesky_kernel(K, y, alpha=[1e-2])
coef2 = np.dot(X_diabetes.T, dual_coef).T
assert_array_almost_equal(coef, coef2)
def EvaluatePolicy(s, w_pi, useRBFKernel = False):
# the value of the improved policy
value = np.zeros((len(s),1))
# the new policy
policy = [False] * len(s)
# iterate through every state,
for idx in range(len(s)):
# State-Action value function for actions 0.0 and 1.0
if useRBFKernel == True:
q0 = np.dot(computePhiRBF(s[idx], 0.0).T, w_pi)
q1 = np.dot(computePhiRBF(s[idx], 1.0).T, w_pi)
else:
q0 = np.dot(np.append(s[idx, 0],0.0), w_pi)
q1 = np.dot(np.append(s[idx, 0],1.0), w_pi)
# update the value
value[idx] = max(q0, q1)
# update the policy
policy[idx] = True if q1 > q0 else False
return (policy, value)
def Haffine_from_points(fp, tp):
'''计算仿射变换的单应性矩阵H，使得tp是由fp经过仿射变换得到的'''
if fp.shape != tp.shape:
raise RuntimeError('number of points do not match')
# 对点进行归一化
# 映射起始点
m = numpy.mean(fp[:2], axis=1)
maxstd = numpy.max(numpy.std(fp[:2], axis=1)) + 1e-9
C1 = numpy.diag([1/maxstd, 1/maxstd, 1])
C1[0, 2] = -m[0] / maxstd
C1[1, 2] = -m[1] / maxstd
fp_cond = numpy.dot(C1, fp)
# 映射对应点
m = numpy.mean(tp[:2], axis=1)
maxstd = numpy.max(numpy.std(tp[:2], axis=1)) + 1e-9
C2 = numpy.diag([1/maxstd, 1/maxstd, 1])
C2[0, 2] = -m[0] / maxstd
C2[1, 2] = -m[1] / maxstd
tp_cond = numpy.dot(C2, tp)
# 因为归一化之后点的均值为0，所以平移量为0
A = numpy.concatenate((fp_cond[:2], tp_cond[:2]), axis=0)
U, S, V = numpy.linalg.svd(A.T)
# 创建矩阵B和C
tmp = V[:2].T
B = tmp[:2]
C = tmp[2:4]
tmp2 = numpy.concatenate((numpy.dot(C, numpy.linalg.pinv(B)), numpy.zeros((2, 1))), axis=1)
H = numpy.vstack((tmp2, [0, 0, 1]))
H = numpy.dot(numpy.linalg.inv(C2), numpy.dot(H, C1)) # 反归一化
return H / H[2, 2] # 归一化，然后返回
def predict(self,samples):
# this function returns the output layer activations (estimates)
z2 = np.dot(samples,self.W1)+np.array([self.b1])
a2 = sigmoid(z2)
z3 = np.dot(a2,self.W2)+np.array([self.b2])
a3 = sigmoid(z3)
return a3
def runLabeling(file_path, gps_filename, output_name, frames_to_skip, final_frame, lp, rp, pickle_loc):
video_reader = WarpedVideoReader(file_path)
#video_reader.setSubsample(True)
video_reader.setPerspectives(pickle_loc)
gps_reader = GPSReader(gps_filename)
gps_dat = gps_reader.getNumericData()
cam = getCameraParams()
cam_to_use = cam[int(output_name[-1]) - 1]
lp = pixelTo3d(lp, cam_to_use)
rp = pixelTo3d(rp, cam_to_use)
tr = GPSTransforms(gps_dat, cam_to_use)
pitch = -cam_to_use['rot_x']
height = 1.106
R_camera_pitch = euler_matrix(cam_to_use['rot_x'], cam_to_use['rot_y'], cam_to_use['rot_z'], 'sxyz')[0:3, 0:3]
Tc = np.eye(4)
Tc[0:3, 0:3] = R_camera_pitch.transpose()
Tc[0:3, 3] = [-0.2, -height, -0.5]
lpts = np.zeros((lp.shape[0], 4))
rpts = np.zeros((rp.shape[0], 4))
for t in range(min(tr.shape[0], lp.shape[0])):
lpts[t, :] = np.dot(tr[t, :, :], np.linalg.solve(Tc, np.array([lp[t, 0], lp[t, 1], lp[t, 2], 1])))
rpts[t, :] = np.dot(tr[t, :, :], np.linalg.solve(Tc, np.array([rp[t, 0], rp[t, 1], rp[t, 2], 1])))
ldist = np.apply_along_axis(np.linalg.norm, 1, np.concatenate((np.array([[0, 0, 0, 0]]), lpts[1:] - lpts[0:-1])))
rdist = np.apply_along_axis(np.linalg.norm, 1, np.concatenate((np.array([[0, 0, 0, 0]]), rpts[1:] - rpts[0:-1])))
start_frame = frames_to_skip
runBatch(video_reader, gps_dat, cam_to_use, output_name, start_frame, final_frame, lpts, rpts, ldist, rdist, tr)
print "Done with %s" % output_name
def backprop(self, x, y):
"""Return a tuple ``(nabla_b, nabla_w)`` representing the
gradient for the cost function C_x. ``nabla_b`` and
``nabla_w`` are layer-by-layer lists of numpy arrays, similar
to ``self.biases`` and ``self.weights``."""
nabla_b = [np.zeros(b.shape) for b in self.biases]
nabla_w = [np.zeros(w.shape) for w in self.weights]
# feedforward
activation = x
activations = [x] # list to store all the activations, layer by layer
zs = [] # list to store all the z vectors, layer by layer
for b, w in zip(self.biases, self.weights):
z = np.dot(w, activation)+b
zs.append(z)
activation = sigmoid(z)
activations.append(activation)
# backward pass
delta = self.cost_derivative(activations[-1], y) * \
sigmoid_prime(zs[-1])
nabla_b[-1] = delta
nabla_w[-1] = np.dot(delta, activations[-2].transpose())
# Note that the variable l in the loop below is used a little
# differently to the notation in Chapter 2 of the book. Here,
# l = 1 means the last layer of neurons, l = 2 is the
# second-last layer, and so on. It's a renumbering of the
# scheme in the book, used here to take advantage of the fact
# that Python can use negative indices in lists.
for l in xrange(2, self.num_layers):
z = zs[-l]
sp = sigmoid_prime(z)
delta = np.dot(self.weights[-l+1].transpose(), delta) * sp
nabla_b[-l] = delta
nabla_w[-l] = np.dot(delta, activations[-l-1].transpose())
return (nabla_b, nabla_w)
def forward(self, X):
#Propogate inputs though network
self.z2 = np.dot(X, self.W1)
self.a2 = self.sigmoid(self.z2)
self.z3 = np.dot(self.a2, self.W2)
yHat = self.sigmoid(self.z3)
return yHat
def smooth_objective(self, x, mode='both', check_feasibility=False):
"""
Evaluate a smooth function and/or its gradient
if mode == 'both', return both function value and gradient
if mode == 'grad', return only the gradient
if mode == 'func', return only the function value
"""
x = self.apply_offset(x)
exp_x = np.exp(x)
#TODO: Using transposes to scale the rows of a 2d array - should we use an affine_transform to do this?
#JT: should be able to do this with np.newaxis
if mode == 'both':
ratio = ((self.trials/(1. + np.sum(exp_x, axis=1))) * exp_x.T).T
f, g = -2. * self.scale(np.sum(self.firstcounts * x) - np.dot(self.trials, np.log(1. + np.sum(exp_x, axis=1)))), - 2 * self.scale(self.firstcounts - ratio)
return f, g
elif mode == 'grad':
ratio = ((self.trials/(1. + np.sum(exp_x, axis=1))) * exp_x.T).T
f, g = None, - 2 * self.scale(self.firstcounts - ratio)
return g
elif mode == 'func':
f, g = -2. * self.scale(np.sum(self.firstcounts * x) - np.dot(self.trials, np.log(1. + np.sum(exp_x, axis=1)))), None
return f
else:
raise ValueError("mode incorrectly specified")
def InitialAlignment(self, scale = 0.15):
""" Compute SVD and align object to be in a certain coordinate frame.
Usage: model.InitialAlignment(scale)
Input:
scale - Desired scale for object. Scale is defined as the length
along the leading eigenvector, in meters.
"""
pts3D = self.pts3D
# Compute eigenvecs and rotate according to them
pc, evals, mean = utils.pca(pts3D, remove_mean = True)
pts3D_rot = np.dot(pc.T, pts3D)
# Find length according to max eigenvector
mins = np.min(pts3D_rot, axis=1)
maxs = np.max(pts3D_rot, axis=1)
max_length = maxs[0] - mins[0]
# Rotation matrix is the covariance matrix, but we want Z as the leading
# eigenvector:
rot = np.c_[-pc[2], pc[1], pc[0]]
# Transform model to have zero mean, reasonable scale and rotation.
self.transform(rot, np.dot(rot, -mean), float(scale) / max_length)
def get_corr_pred( self, sctx, u, du, tn, tn1,
u_avg = None,
B_mtx_grid = None,
J_det_grid = None,
ip_coords = None,
ip_weights = None ):
'''
Corrector and predictor evaluation.
@param u current element displacement vector
'''
if J_det_grid == None or B_mtx_grid == None:
X_mtx = sctx.X
show_comparison = True
if ip_coords == None:
ip_coords = self.ip_coords
show_comparison = False
if ip_weights == None:
ip_weights = self.ip_weights
### Use for Jacobi Transformation
n_e_dofs = self.n_e_dofs
K = zeros( ( n_e_dofs, n_e_dofs ) )
F = zeros( n_e_dofs )
sctx.fets_eval = self
ip = 0
for r_pnt, wt in zip( ip_coords, ip_weights ):
#r_pnt = gp[0]
sctx.r_pnt = r_pnt
#caching cannot be switched off in the moment
# if J_det_grid == None:
# J_det = self._get_J_det( r_pnt, X_mtx )
# else:
# J_det = J_det_grid[ip, ... ]
# if B_mtx_grid == None:
# B_mtx = self.get_B_mtx( r_pnt, X_mtx )
# else:
# B_mtx = B_mtx_grid[ip, ... ]
J_det = J_det_grid[ip, ... ]
B_mtx = B_mtx_grid[ip, ... ]
eps_mtx = dot( B_mtx, u )
d_eps_mtx = dot( B_mtx, du )
sctx.mats_state_array = sctx.elem_state_array[ip * self.m_arr_size: ( ip + 1 ) * self.m_arr_size]
#print 'elem state ', sctx.elem_state_array
#print 'mats state ', sctx.mats_state_array
sctx.r_ls = sctx.ls_val[ip]
sig_mtx, D_mtx = self.get_mtrl_corr_pred( sctx, eps_mtx, d_eps_mtx, tn, tn1 )
k = dot( B_mtx.T, dot( D_mtx, B_mtx ) )
k *= ( wt * J_det )
K += k
f = dot( B_mtx.T, sig_mtx )
f *= ( wt * J_det )
F += f
ip += 1
return F, K
def train(self, inp, out, training_weight=1.):
inp = np.mat(inp).T
out = np.mat(out).T
deriv = []
val = inp
vals = [val]
# forward calculation of activations and derivatives
for weight,bias in self.__weights:
val = weight*val
val += bias
deriv.append(self.__derivative(val))
vals.append(self.__activation(val))
deriv = iter(reversed(deriv))
weights = iter(reversed(self.__weights))
errs = []
errs.append(np.multiply(vals[-1]-out, next(deriv)))
# backwards propagation of errors
for (w,b),d in zip(weights, deriv):
errs.append(np.multiply(np.dot(w.T, errs[-1]), d))
weights = iter(self.__weights)
for (w,b),v,e in zip(\
self.__weights,\
vals, reversed(errs)):
e *= self.__learning_rate*training_weight
w -= e*v.T
b -= e
tmp = vals[-1]-out
return np.dot(tmp[0].T,tmp[0])*.5*training_weight
def top_eigenvector(A,niter=1000,force_iteration=False):
'''
assuming the LEFT invariant subspace of A corresponding to the LEFT
eigenvalue of largest modulus has geometric multiplicity of 1 (trivial
Jordan block), returns the vector at the intersection of that eigenspace and
the simplex
A should probably be a ROW-stochastic matrix
probably uses power iteration
'''
n = A.shape[0]
np.seterr(invalid='raise',divide='raise')
if n <= 25 and not force_iteration:
x = np.repeat(1./n,n)
x = np.linalg.matrix_power(A.T,niter).dot(x)
x /= x.sum()
return x
else:
x1 = np.repeat(1./n,n)
x2 = x1.copy()
for itr in xrange(niter):
np.dot(A.T,x1,out=x2)
x2 /= x2.sum()
x1,x2 = x2,x1
if np.linalg.norm(x1-x2) < 1e-8:
break
return x1
def test_dot():
# Test normal dot
a = np.random.uniform(-3, 3, (3, 4))
b = np.random.uniform(-3, 3, (4, 5))
c = np.dot(a, b)
A = mx.nd.array(a)
B = mx.nd.array(b)
C = mx.nd.dot(A, B)
assert reldiff(c, C.asnumpy()) < 1e-5
# Test dot with transpose kargs
a = np.random.uniform(-3, 3, (3, 4))
b = np.random.uniform(-3, 3, (3, 5))
c = np.dot(a.T, b)
A = mx.nd.array(a)
B = mx.nd.array(b)
C = mx.nd.dot(A, B, transpose_a=True)
assert reldiff(c, C.asnumpy()) < 1e-5
# Test dot with transpose kargs
a = np.random.uniform(-3, 3, (3, 4))
b = np.random.uniform(-3, 3, (5, 4))
c = np.dot(a, b.T)
A = mx.nd.array(a)
B = mx.nd.array(b)
C = mx.nd.dot(A, B, transpose_b=True)
assert reldiff(c, C.asnumpy()) < 1e-5
# Test dot with transpose kargs
a = np.random.uniform(-3, 3, (4, 3))
b = np.random.uniform(-3, 3, (5, 4))
c = np.dot(a.T, b.T)
A = mx.nd.array(a)
B = mx.nd.array(b)
C = mx.nd.dot(A, B, transpose_a=True, transpose_b=True)
assert reldiff(c, C.asnumpy()) < 1e-5
def test_grtm():
l = language(1000)
n_iter = 1000
KL_thresh = 0.3
mu = 0.
nu2 = 1.
np.random.seed(l['seed'])
H = np.random.normal(loc=mu, scale=nu2, size=(l['K'], l['K']))
zeta = pd.DataFrame([(i, j, np.dot(np.dot(l['thetas'][i], H),
l['thetas'][j]))
for i, j in product(range(l['D']), repeat=2)],
columns=('tail', 'head', 'zeta'))
zeta['y'] = (zeta.zeta >= 0).astype(int)
y = zeta[['tail', 'head', 'y']].values
skf = StratifiedKFold(y[:, 2], n_folds=100)
_, train_idx = next(iter(skf))
_K = l['K']
_alpha = l['alpha'][:_K]
_beta = np.repeat(0.01, l['V'])
_b = 1.
grtm = GRTM(_K, _alpha, _beta, mu, nu2, _b, n_iter, seed=l['seed'],
n_report_iter=l['n_report_iters'])
grtm.fit(l['doc_term_matrix'], y[train_idx])
assert_probablity_distribution(grtm.phi)
check_KL_divergence(l['topics'], grtm.phi, KL_thresh)
def ehist_equalize_melhist(d, sr, refMelHist, edges):
""" Modify a signal in the Mel domain
by equalizing the Mel-subband histograms to match
the passed-in ones """
# Calculate the (Mel) spectrograms, and histogram, and axes
melHist, edges, D, DmeldB, melmx, freqs = mel_hist(d, sr, edges=edges)
# Build mapping & modify mel spectrogram
histmaps = make_hist_maps(melHist, refMelHist, edges)
# for some reason, extrapolating madly below bottom edge - clip it
DmeldBmapped = np.maximum(edges[0],
np.minimum(edges[-1],
apply_hist_maps(DmeldB, histmaps)))
# Reconstruct audio based on mapped envelope
# We map both original and modified Mel envelopes to FFT domain
# then scale original STFT magnitudes by their ratio
DmelInFFT = np.dot(melmx.T, idB(DmeldB))
DmappedInFFT = np.dot(melmx.T, idB(DmeldBmapped))
# Zero values in denominator will match to zeros in numerator,
# so it's OK to drop them
Dmask = DmappedInFFT / (DmelInFFT + (DmelInFFT==0))
# Median filter to remove short blips in gain
medfiltwin = 7
DmaskF = median_filter(Dmask, size=(1, medfiltwin))
# Now scale each FFT val by their ratio
Dmod = D * DmaskF
# and resynthesize
nfft = 2*(np.size(D, axis=0)-1)
win = nfft
hop = win/4
dout = istft(Dmod.T, win, hop)
return dout
def tz(M):
mz = matrix_power(M,-1)
assert_almost_equal(identity(M.shape[0]), dot(mz,M))
def hinge_loss_gradient(w, x, y):
if np.dot(w, x) * y >= 1:
return 0
else:
return y * x
def propdown(self, h):
pre_activation = numpy.dot(h, self.W.T) + self.vbias
return pre_activation
def step_length(f, g, xk, alpha, pk, c2):
return interpolation(f, g, lambda alpha: f(xk + alpha * pk),
lambda alpha: np.dot(g(xk + alpha * pk), pk), alpha,
c2,
lambda f, g, alpha, c2: wolfe(f, g, xk, alpha, pk))
def gold_stein(f, g, xk, alpha, pk, c):
return (f(xk) +
(1 - c) * alpha * np.dot(g(xk), pk) <= f(xk + alpha * pk)) and (
f(xk + alpha * pk) <= f(xk) + c * alpha * np.dot(g(xk), pk))
def strong_wolfe(f, g, xk, alpha, pk, c2):
# typically, c2 = 0.9 when using Newton or quasi-Newton's method.
# c2 = 0.1 when using non-linear conjugate gradient method.
return wolfe(f, g, xk, alpha, pk) and abs(np.dot(
g(xk + alpha * pk), pk)) <= c2 * abs(np.dot(g(xk), pk))
def wolfe(f, g, xk, alpha, pk):
c1 = 1e-4
return f(xk + alpha * pk) <= f(xk) + c1 * alpha * np.dot(g(xk), pk)
def do(self, a, b):
a_ginv = linalg.pinv(a)
assert_almost_equal(dot(a, a_ginv), identity(asarray(a).shape[0]))
assert imply(isinstance(a, matrix), isinstance(a_ginv, matrix))
def do(self, a, b):
evalues, evectors = linalg.eig(a)
assert_almost_equal(dot(a, evectors), multiply(evectors, evalues))
assert imply(isinstance(a, matrix), isinstance(evectors, matrix))
def tz(M):
mz = matrix_power(M,2)
assert_equal(mz, dot(M,M))
assert_equal(mz.dtype, M.dtype)
# QR decomposition ensures that the columns of B are orthogonal
B, R = np.linalg.qr(B)
L = B.shape[1]
theta_old = theta[:nroot]
print("EOMCCSD: Iter # {:>6} L = {}".format(EOMCCSD_iter, L))
# Build up the matrix S, holding the products Hbar*B, aka sigma vectors
S = np.zeros_like(B)
for i in range(L):
B1 = B[:nov, i].reshape(ndocc, nvir).copy()
B2 = B[nov:, i].reshape(ndocc, ndocc, nvir, nvir).copy()
S1 = cceom.build_sigma1(B1, B2)
S2 = cceom.build_sigma2(B1, B2)
S[:nov, i] += S1.flatten()
S[nov:, i] += S2.flatten()
# Build the subspace Hamiltonian
G = np.dot(B.T, S)
# Diagonalize it, and sort the eigenvector/eigenvalue pairs
theta, alpha = np.linalg.eig(G)
idx = theta.argsort()[:nroot]
theta = theta[idx]
alpha = alpha[:, idx]
# This vector will hold the new guess vectors to add to our space
add_B = []
for j in range(nroot):
# Compute a residual vector "w" for each root we seek
# Note: for a more robust convergence criteria you can also check
# that the norm of the residual vector is below some threshold.
w = np.dot(S, alpha[:, j]) - theta[j] * np.dot(B, alpha[:, j])
# Precondition the residual vector to form a correction vector
q = w / (theta[j] - D[j])
def do(self, a, b):
u, s, vt = linalg.svd(a, 0)
assert_almost_equal(a, dot(multiply(u, s), vt))
assert imply(isinstance(a, matrix), isinstance(u, matrix))
assert imply(isinstance(a, matrix), isinstance(vt, matrix))
def _rotate_points(self, points):
_points = np.pad(points, [(0, 0), (0, 1)], 'constant')
_points[:, 2] = 1
_points = np.dot(self._mat, _points.T)
return _points.T.astype(points.dtype)
def do(self, a, b):
x = linalg.solve(a, b)
assert_almost_equal(b, dot(a, x))
assert imply(isinstance(b, matrix), isinstance(x, matrix))
def hessian(self, x=None, mean_output=False, mc_num=1, denormalize=False, method='exact'):
"""
| Calculate the hessian of output to input
|
| Please notice that the de-normalize (if True) assumes the output depends on the input data first orderly
| in which the hessians does not depends on input scaling and only depends on output scaling
|
| The hessians can be all zeros and the common cause is you did not use any activation or
| activation that is still too linear in some sense like ReLU.
:param x: Input Data
:type x: ndarray
:param mean_output: False to get all hessian, True to get the mean
:type mean_output: boolean
:param mc_num: Number of monte carlo integration
:type mc_num: int
:param denormalize: De-normalize diagonal part of Hessian
:type denormalize: bool
:param method: Either 'exact' to calculate numerical Hessian or 'approx' to approximate Hessian from Jacobian
:type method: str
:return: An array of Hessian
:rtype: ndarray
:History: 2018-Jun-14 - Written - Henry Leung (University of Toronto)
"""
if not mean_output:
print('only mean output is supported at this moment')
mean_output = True
if method == 'approx':
all_args = locals()
# remove unnecessary argument
all_args.pop('self')
all_args.pop('method')
jacobian = self.jacobian(**all_args)
hessians_master = np.stack([np.dot(jacobian[x_shape:x_shape + 1].T, jacobian[x_shape:x_shape + 1])
for x_shape in range(jacobian.shape[0])], axis=0)
return hessians_master
elif method == 'exact':
self.has_model_check()
if x is None:
raise ValueError('Please provide data to calculate the jacobian')
if mc_num < 1 or isinstance(mc_num, float):
raise ValueError('mc_num must be a positive integer')
if self.input_normalizer is not None:
x_data = self.input_normalizer.normalize(x, calc=False)
else:
# Prevent shallow copy issue
x_data = np.array(x)
x_data -= self.input_mean
x_data /= self.input_std
try:
input_tens = self.keras_model_predict.get_layer("input").input
output_tens = self.keras_model_predict.get_layer("output").output
input_shape_expectation = self.keras_model_predict.get_layer("input").input_shape
output_shape_expectation = self.keras_model_predict.get_layer("output").output_shape
except AttributeError:
input_tens = self.keras_model.get_layer("input").input
output_tens = self.keras_model.get_layer("output").output
input_shape_expectation = self.keras_model.get_layer("input").input_shape
output_shape_expectation = self.keras_model.get_layer("output").output_shape
except ValueError:
raise ValueError(
"astroNN expects input layer is named as 'input' and output layer is named as 'output', "
"but None is found.")
if len(input_shape_expectation) == 1:
input_shape_expectation = input_shape_expectation[0]
# just in case only 1 data point is provided and mess up the shape issue
if len(input_shape_expectation) == 3:
x_data = np.atleast_3d(x_data)
elif len(input_shape_expectation) == 4:
if len(x_data.shape) < 4:
x_data = x_data[:, :, :, np.newaxis]
else:
raise ValueError('Input data shape do not match neural network expectation')
total_num = x_data.shape[0]
hessians_list = []
for j in range(self._labels_shape):
hessians_list.append(tf.hessians(output_tens[:, j], input_tens))
final_stack = tf.stack(tf.squeeze(hessians_list))
# Looping variables for tensorflow setup
i = tf.constant(0)
mc_num_tf = tf.constant(mc_num)
# To store final result
l = tf.TensorArray(dtype=tf.float32, infer_shape=False, size=1, dynamic_size=True)
def body(i, l):
l = l.write(i, final_stack)
return i + 1, l
tf_index, loop = tf.while_loop(lambda i, *_: tf.less(i, mc_num_tf), body, [i, l])
loops = tf.cond(tf.greater(mc_num_tf, 1), lambda: tf.reduce_mean(loop.stack(), axis=0),
lambda: loop.stack())
start_time = time.time()
hessians = np.concatenate(
[get_session().run(loops, feed_dict={input_tens: x_data[i:i + 1], tfk.backend.learning_phase(): 0})
for i
in range(0, total_num)], axis=0)
if np.all(hessians == 0.): # warn user about not so linear activation like ReLU will get all zeros
warnings.warn(
'The hessians is detected to be all zeros. The common cause is you did not use any activation or '
'activation that is still too linear in some sense like ReLU.', UserWarning)
if mean_output is True:
hessians_master = np.mean(hessians, axis=0)
else:
hessians_master = np.array(hessians)
hessians_master = np.squeeze(hessians_master)
if denormalize: # no need to denorm input scaling because of we assume first order dependence
if self.labels_std is not None:
try:
hessians_master = hessians_master * self.labels_std
except ValueError:
hessians_master = hessians_master * self.labels_std.reshape(-1, 1)
print(f'Finished hessian ({method}) calculation, {(time.time() - start_time):.{2}f} seconds elapsed')
return hessians_master
else:
raise ValueError(f'Unknown method -> {method}')
def label_softmax_grad(X, dY):
dX = Y * 0.0
for i in range(n):
d = np.dot(Y[i, :], dY[i, :])
dX[i, :] = Y[i, :] * (dY[i, :] - d)
return [dX]
def calculate_nll(y, tx, w):
"""compute the cost by negative log likelihood."""
txw = np.dot(tx,w)
return np.sum(np.log(1+np.exp(txw)) - y*txw)
def dot(a,b): return np.dot(a,b)
def conjugate_gradient(
func,
x0,
args=(),
fprime=None,
alpha=0.5,
scaling_factor=0.8,
numIter=1e5,
norm_lim=1e-7,
epsilon=1e-10,
order=2,
disp=False,
period=10000):
"""
Conjugate descent algorithm to optimize the cost function using Fletcher-Reeves Update
Usage:
func : function
function to be optimized
x0 : list
initial guess
args :
other arguments to be passed to func
fprime : function
derivative or jacobian of func, if not passed then will be generated automatically
alpha : float
learning rate
scaling_factor : float
factor to multiply alpha with when doing line search
numIter : int
number of iterations
norm_lim : float
minimum value of norm
epsilon : float
delta x for calculting fprime
order : int
order of norm, max value = Inf
Example:
>>> def func(x):
return pow(x[0]-2,6.0)+pow(x[1]-3,6.0)
>>> x0 = [1,2]
>>> point_of_optima = conjugate_gradient(func,x0)
"""
if fprime is None:
fprime = hlp.compute_numerical_grad(func, len(x0), epsilon)
iters = 0
func_value = func(x0, *args)
gradient_prev = np.array(fprime(x0, *args))
norm_gradient = hlp.vecnorm(gradient_prev, order)
xPrev = np.array(x0)
pPrev = -gradient_prev
while norm_gradient > norm_lim and iters < numIter:
iters += 1
if disp and (iters % period == 0 or iters == 1):
print("Iter : %d | Function value : %f" % (iters, func_value))
alp = alpha
while func(xPrev + alp * pPrev, *args) > func(xPrev, *args):
alp *= scaling_factor
xUpdated = xPrev + alp * pPrev
gradient_updated = np.array(fprime(xUpdated, *args))
betaUpdated = np.dot(gradient_updated, gradient_updated) / \
np.dot(gradient_prev, gradient_prev)
pUpdated = -gradient_updated + betaUpdated * pPrev
func_value = func(xUpdated, *args)
norm_gradient = hlp.vecnorm(gradient_updated, order)
pPrev = pUpdated
gradient_prev = gradient_updated
xPrev = xUpdated
if disp and iters % period != 0:
print("Iter : %d | Function value : %f" % (iters, func_value))
return xUpdated
def compute_error(y, tx, w):
return y - np.dot(tx, w)
def simulate_eazy_sed(fieldidx='GOODS-S.21740', eazydata=None,
returnfluxunit='AB', returnwaveunit='nm',
limitwaverange=True, savetofile='',
headerstring='# wave flux\n'):
"""
Pull best-fit SED from eazy-py output files.
NB: Requires the eazy-py package to apply the IGM absorption!
(https://github.com/gbrammer/eazy-py)
Optional Args: returnfluxunit: ['AB', 'flambda'] TODO: add Jy
returnwaveunit: ['A' or 'nm'] limitwaverange: limit the output
wavelengths to the range covered by PFS savetofile: filename for saving
the output spectrum as a two-column ascii data file (suitable for use
with the SubaruPFS ETC from C. Hirata.
Returns
-------
templz : observed-frame wavelength, Angstroms or nm
tempflux : flux density of best-fit template, erg/s/cm2/A or AB mag
"""
fieldstr, idxstr = fieldidx.split('.')
field = fieldstr.lower().replace('-','')
idx = int(idxstr)
# TODO : this is a kludge. Should not assume only one eazypy.data.fits file per field
if eazydata is None:
fitsfilename = glob(
'3DHST/{0}_3dhst.*.eazypy.data.fits'.format(field))[0]
eazydata = EazyData(fitsfilename)
imatch = eazydata.ID == idx
if imatch.sum() == 0:
print('ID {0} not found.'.format(idx))
return None, None
ix = np.arange(len(imatch))[imatch][0]
z = eazydata.ZBEST[ix]
# the input data units are Angstroms for wavelength
# and cgs for flux: erg/cm2/s/Ang
templz = eazydata.TEMPL * (1 + z)
templf = np.dot(eazydata.COEFFS[ix, :], eazydata.TEMPF)
fnu_factor = 10 ** (-0.4 * (25 + 48.6))
flam_spec = 1. / (1 + z) ** 2
tempflux = templf * fnu_factor * flam_spec
try:
import eazy.igm
igmz = eazy.igm.Inoue14().full_IGM(z, templz)
tempflux *= igmz
except:
pass
if limitwaverange:
# to simplify things, we only write out the data over the Subaru PFS
# wavelength range, from 300 to 1300 nm (3000 to 13000 Angstroms)
ipfs = np.where((templz>2000) & (templz<25000))[0]
templz = templz[ipfs]
tempflux = tempflux[ipfs]
if returnfluxunit=='AB':
# convert from flux density f_lambda into AB mag:
mAB_from_flambda = lambda f_lambda, wave: -2.5 * np.log10(
3.34e4 * wave * wave * f_lambda / 3631)
tempflux = mAB_from_flambda(tempflux, templz)
if returnwaveunit=='nm':
templz = templz / 10.
if savetofile:
fout = open(savetofile, 'w')
fout.write(headerstring)
for i in range(len(templz)):
fout.write('{wave:.3e} {flux:.3e}\n'.format(
wave=templz[i], flux=tempflux[i]))
fout.close()
else:
return templz, tempflux
import pickle
import numpy as np
# db = pickle.load(open('bert_fine_tune.p', 'rb'))
from utils import Config, safe_pickle_dump, strip_version
db = pickle.load(open(Config.db_path, 'rb'))
orig = pickle.load(open('elmo_embed.p', 'rb'))
# db = pickle.load(open('bert_out.p', 'rb'))
# print(len(db))
# X = np.array(list(db.values()))
# normalization
X = orig / np.linalg.norm(orig, axis=1, keepdims=1)
# print(X.shape)
pids = list(db.keys())
# B = N
ds = -np.asarray(np.dot(X, X.T)) #NxD * DxB => NxB
# print(ds[0][0])
IX = np.argsort(ds, axis=0) # NxB
# pid = '1407.2515'
# pid = '1904.05856'
# pid = '1904.07460'
# ID = pids.index(pid)
# print(IX.shape)
ARXIV_PATH = 'https://arxiv.org/abs/'
# print(ARXIV_PATH + pids[ID])
# print(orig[ID])
# for i in range(0,6):
# # print(IX[ID][i])
# # print(orig[IX[i][ID]])
# # print(1+ds[ID][IX[i][ID]], end=' ')
# sim_pid = pids[IX[i][ID]]
# print(ARXIV_PATH + sim_pid)
def rgb2gray(self, rgb):
'''
take a numpy rgb image return a new single channel image converted to
greyscale
'''
return np.dot(rgb[...,:3], [0.299, 0.587, 0.114])
def simulate_eazy_sed_from_coeffs(
eazycoeffs, eazytemplatedata, z,
returnfluxunit='', returnwaveunit='A',
limitwaverange=True, savetofile='',
**outfile_kwargs):
"""
Generate a simulated SED from a given set of input eazy-py coefficients
and eazypy templates.
NB: Requires the eazy-py package to apply the IGM absorption!
(https://github.com/gbrammer/eazy-py)
Optional Args:
returnfluxunit: ['AB', 'flambda'] TODO: add Jy
'AB'= return log(flux) as AB magnitudes
'flambda' = return flux density in erg/s/cm2/A
returnwaveunit: ['A' or 'nm'] limitwaverange: limit the output
wavelengths to the range covered by PFS savetofile: filename for saving
the output spectrum as a two-column ascii data file (suitable for use
with the SubaruPFS ETC from C. Hirata.
Returns
-------
obswave : observed-frame wavelength, Angstroms or nm
obsflux : flux density of best-fit template, erg/s/cm2/A or AB mag
"""
# the input data units are Angstroms for wavelength
# and cgs for flux: erg/cm2/s/Ang
obswave = eazytemplatedata[0] * (1 + z)
obsfluxmatrix = eazytemplatedata[1:]
sedsimflux = np.dot(eazycoeffs, obsfluxmatrix)
fnu_factor = 10 ** (-0.4 * (25 + 48.6))
flam_spec = 1. / (1 + z) ** 2
obsflux = sedsimflux * fnu_factor * flam_spec
try:
import eazy.igm
igmz = eazy.igm.Inoue14().full_IGM(z, obswave)
obsflux *= igmz
except:
pass
if limitwaverange:
# to simplify things, we only write out the data over the Subaru PFS
# + WFIRST prism wavelength range, from 200 to 2500 nm
# (3000 to 25000 Angstroms)
iuvoir = np.where((obswave>2000) & (obswave<25000))[0]
obswave = obswave[iuvoir]
obsflux = obsflux[iuvoir]
if returnfluxunit=='AB':
# convert from flux density f_lambda into AB mag:
mAB_from_flambda = lambda f_lambda, wave: -2.5 * np.log10(
3.34e4 * wave * wave * f_lambda / 3631)
obsflux = mAB_from_flambda(obsflux, obswave)
if returnwaveunit=='nm':
obswave = obswave / 10.
if savetofile:
out_table = Table()
outcol1 = Column(data=obswave, name='wave')
outcol2 = Column(data=obsflux, name='flux')
out_table.add_columns([outcol1, outcol2])
out_table.write(savetofile, **outfile_kwargs)
return obswave, obsflux
def gv(w):
return av + np.dot(lv, w - cg_shift)
import numpy as np
A = np.array([[1,2,3],[4,5,6],[7,8,9]])
B = np.array([[1,2,3],[4,5,6],[7,8,9]])
newmatrix = []
i = 0
while i < len(A):
eachrow = [np.sum(A[i]*B[:,j]) for j in range(len(A))]
i += 1
newmatrix.append(eachrow)
print(np.array(newmatrix))
print(np.dot(A,B))
def _beta_divergence(X, W, H, beta, square_root=False):
"""Compute the beta-divergence of X and dot(W, H).
Parameters
----------
X : float or array-like of shape (n_samples, n_features)
W : float or array-like of shape (n_samples, n_components)
H : float or array-like of shape (n_components, n_features)
beta : float or {'frobenius', 'kullback-leibler', 'itakura-saito'}
Parameter of the beta-divergence.
If beta == 2, this is half the Frobenius *squared* norm.
If beta == 1, this is the generalized Kullback-Leibler divergence.
If beta == 0, this is the Itakura-Saito divergence.
Else, this is the general beta-divergence.
square_root : bool, default=False
If True, return np.sqrt(2 * res)
For beta == 2, it corresponds to the Frobenius norm.
Returns
-------
res : float
Beta divergence of X and np.dot(X, H)
"""
beta = _beta_loss_to_float(beta)
# The method can be called with scalars
if not sp.issparse(X):
X = np.atleast_2d(X)
W = np.atleast_2d(W)
H = np.atleast_2d(H)
# Frobenius norm
if beta == 2:
# Avoid the creation of the dense np.dot(W, H) if X is sparse.
if sp.issparse(X):
norm_X = np.dot(X.data, X.data)
norm_WH = trace_dot(np.linalg.multi_dot([W.T, W, H]), H)
cross_prod = trace_dot((X * H.T), W)
res = (norm_X + norm_WH - 2. * cross_prod) / 2.
else:
res = squared_norm(X - np.dot(W, H)) / 2.
if square_root:
return np.sqrt(res * 2)
else:
return res
if sp.issparse(X):
# compute np.dot(W, H) only where X is nonzero
WH_data = _special_sparse_dot(W, H, X).data
X_data = X.data
else:
WH = np.dot(W, H)
WH_data = WH.ravel()
X_data = X.ravel()
# do not affect the zeros: here 0 ** (-1) = 0 and not infinity
indices = X_data > EPSILON
WH_data = WH_data[indices]
X_data = X_data[indices]
# used to avoid division by zero
WH_data[WH_data == 0] = EPSILON
# generalized Kullback-Leibler divergence
if beta == 1:
# fast and memory efficient computation of np.sum(np.dot(W, H))
sum_WH = np.dot(np.sum(W, axis=0), np.sum(H, axis=1))
# computes np.sum(X * log(X / WH)) only where X is nonzero
div = X_data / WH_data
res = np.dot(X_data, np.log(div))
# add full np.sum(np.dot(W, H)) - np.sum(X)
res += sum_WH - X_data.sum()
# Itakura-Saito divergence
elif beta == 0:
div = X_data / WH_data
res = np.sum(div) - np.product(X.shape) - np.sum(np.log(div))
# beta-divergence, beta not in (0, 1, 2)
else:
if sp.issparse(X):
# slow loop, but memory efficient computation of :
# np.sum(np.dot(W, H) ** beta)
sum_WH_beta = 0
for i in range(X.shape[1]):
sum_WH_beta += np.sum(np.dot(W, H[:, i])**beta)
else:
sum_WH_beta = np.sum(WH**beta)
sum_X_WH = np.dot(X_data, WH_data**(beta - 1))
res = (X_data**beta).sum() - beta * sum_X_WH
res += sum_WH_beta * (beta - 1)
res /= beta * (beta - 1)
if square_root:
return np.sqrt(2 * res)
else:
return res
def f0(x):
ang = [x[0], x[1:a_in + 1], x[1 + a_in:]]
scr = angles2Score(device, ang, eta, vis)
return av_curr + np.dot(lv_curr, scr - cg_shift)
def _multiplicative_update_w(X,
W,
H,
beta_loss,
l1_reg_W,
l2_reg_W,
gamma,
H_sum=None,
HHt=None,
XHt=None,
update_H=True):
"""update W in Multiplicative Update NMF"""
if beta_loss == 2:
# Numerator
if XHt is None:
XHt = safe_sparse_dot(X, H.T)
if update_H:
# avoid a copy of XHt, which will be re-computed (update_H=True)
numerator = XHt
else:
# preserve the XHt, which is not re-computed (update_H=False)
numerator = XHt.copy()
# Denominator
if HHt is None:
HHt = np.dot(H, H.T)
denominator = np.dot(W, HHt)
else:
# Numerator
# if X is sparse, compute WH only where X is non zero
WH_safe_X = _special_sparse_dot(W, H, X)
if sp.issparse(X):
WH_safe_X_data = WH_safe_X.data
X_data = X.data
else:
WH_safe_X_data = WH_safe_X
X_data = X
# copy used in the Denominator
WH = WH_safe_X.copy()
if beta_loss - 1. < 0:
WH[WH == 0] = EPSILON
# to avoid taking a negative power of zero
if beta_loss - 2. < 0:
WH_safe_X_data[WH_safe_X_data == 0] = EPSILON
if beta_loss == 1:
np.divide(X_data, WH_safe_X_data, out=WH_safe_X_data)
elif beta_loss == 0:
# speeds up computation time
# refer to /numpy/numpy/issues/9363
WH_safe_X_data **= -1
WH_safe_X_data **= 2
# element-wise multiplication
WH_safe_X_data *= X_data
else:
WH_safe_X_data **= beta_loss - 2
# element-wise multiplication
WH_safe_X_data *= X_data
# here numerator = dot(X * (dot(W, H) ** (beta_loss - 2)), H.T)
numerator = safe_sparse_dot(WH_safe_X, H.T)
# Denominator
if beta_loss == 1:
if H_sum is None:
H_sum = np.sum(H, axis=1) # shape(n_components, )
denominator = H_sum[np.newaxis, :]
else:
# computation of WHHt = dot(dot(W, H) ** beta_loss - 1, H.T)
if sp.issparse(X):
# memory efficient computation
# (compute row by row, avoiding the dense matrix WH)
WHHt = np.empty(W.shape)
for i in range(X.shape[0]):
WHi = np.dot(W[i, :], H)
if beta_loss - 1 < 0:
WHi[WHi == 0] = EPSILON
WHi **= beta_loss - 1
WHHt[i, :] = np.dot(WHi, H.T)
else:
WH **= beta_loss - 1
WHHt = np.dot(WH, H.T)
denominator = WHHt
# Add L1 and L2 regularization
if l1_reg_W > 0:
denominator += l1_reg_W
if l2_reg_W > 0:
denominator = denominator + l2_reg_W * W
denominator[denominator == 0] = EPSILON
numerator /= denominator
delta_W = numerator
# gamma is in ]0, 1]
if gamma != 1:
delta_W **= gamma
return delta_W, H_sum, HHt, XHt
def _multiplicative_update_h(X, W, H, beta_loss, l1_reg_H, l2_reg_H, gamma):
"""update H in Multiplicative Update NMF"""
if beta_loss == 2:
numerator = safe_sparse_dot(W.T, X)
denominator = np.linalg.multi_dot([W.T, W, H])
else:
# Numerator
WH_safe_X = _special_sparse_dot(W, H, X)
if sp.issparse(X):
WH_safe_X_data = WH_safe_X.data
X_data = X.data
else:
WH_safe_X_data = WH_safe_X
X_data = X
# copy used in the Denominator
WH = WH_safe_X.copy()
if beta_loss - 1. < 0:
WH[WH == 0] = EPSILON
# to avoid division by zero
if beta_loss - 2. < 0:
WH_safe_X_data[WH_safe_X_data == 0] = EPSILON
if beta_loss == 1:
np.divide(X_data, WH_safe_X_data, out=WH_safe_X_data)
elif beta_loss == 0:
# speeds up computation time
# refer to /numpy/numpy/issues/9363
WH_safe_X_data **= -1
WH_safe_X_data **= 2
# element-wise multiplication
WH_safe_X_data *= X_data
else:
WH_safe_X_data **= beta_loss - 2
# element-wise multiplication
WH_safe_X_data *= X_data
# here numerator = dot(W.T, (dot(W, H) ** (beta_loss - 2)) * X)
numerator = safe_sparse_dot(W.T, WH_safe_X)
# Denominator
if beta_loss == 1:
W_sum = np.sum(W, axis=0) # shape(n_components, )
W_sum[W_sum == 0] = 1.
denominator = W_sum[:, np.newaxis]
# beta_loss not in (1, 2)
else:
# computation of WtWH = dot(W.T, dot(W, H) ** beta_loss - 1)
if sp.issparse(X):
# memory efficient computation
# (compute column by column, avoiding the dense matrix WH)
WtWH = np.empty(H.shape)
for i in range(X.shape[1]):
WHi = np.dot(W, H[:, i])
if beta_loss - 1 < 0:
WHi[WHi == 0] = EPSILON
WHi **= beta_loss - 1
WtWH[:, i] = np.dot(W.T, WHi)
else:
WH **= beta_loss - 1
WtWH = np.dot(W.T, WH)
denominator = WtWH
# Add L1 and L2 regularization
if l1_reg_H > 0:
denominator += l1_reg_H
if l2_reg_H > 0:
denominator = denominator + l2_reg_H * H
denominator[denominator == 0] = EPSILON
numerator /= denominator
delta_H = numerator
# gamma is in ]0, 1]
if gamma != 1:
delta_H **= gamma
return delta_H