def measure(self, position_root, timepoint, annotations, before, after):
print(f'Measuring position {position_root.name} - {timepoint}')
measures = {}
derived_root = position_root.parent / 'derived_data'
mask = self.get_mask(position_root, derived_root, timepoint,
annotations)
if mask is None:
return [numpy.nan] * len(self.feature_names)
measures['mask_area'] = mask.sum() * self.microns_per_pixel**2
moments = ski_measure.moments(mask, order=1)
centroid = numpy.array(
[moments[1, 0] / moments[0, 0], moments[0, 1] / moments[0, 0]])
centroid_distances = []
for adjacent in (before, after):
if adjacent is not None:
adj_mask = self.get_mask(position_root, derived_root,
adjacent['timepoint'], annotations)
if adj_mask is None:
centroid_distances.append(numpy.nan)
break
adj_moments = ski_measure.moments(adj_mask, order=1)
adj_centroid = numpy.array([
adj_moments[1, 0] / adj_moments[0, 0],
adj_moments[0, 1] / adj_moments[0, 0]
])
adj_dist = ((centroid - adj_centroid)**2).sum()**0.5
centroid_distances.append(adj_dist)
measures['mask_centroid_dist'] = numpy.sum(
centroid_distances) * self.microns_per_pixel
return [measures[feature] for feature in self.feature_names]
def test_scale_phosphene():
img = np.zeros((200, 200), dtype=np.double)
img[90:110, 70:90] = 1
img_area = skim.moments(img, order=0)
for scale in [0.9, 1, 1.5, 2, 4]:
scaled = imgproc.scale_phosphene(img, scale)
scaled_area = skim.moments(scaled, order=0)
npt.assert_almost_equal(scaled_area, img_area * scale**2)
def transform_rot(image):
# Need black background (0 boundary condition)
# for rotational transform
# Thats why Sobel or inverse transformation here
#image_ref = filters.sobel(image)
image_ref = 1.0 - image
# Center of mass to be used as rotation center
m = moments(image_ref,order=1)
cx = m[1, 0]/m[0, 0]
cy = m[0, 1]/m[0, 0]
com = cx, cy
# This next step is perfect in the math but the rotation angle
# it generates varies drastically with changes in the watch image
# thus its not robust enough for universal alignment.
# Therefore we add an extra rotation step after it.
# Ascertaining rotation angle from FFT transform
ind1 = np.arange(image.shape[0],dtype=float)
ind2 = np.arange(image.shape[1],dtype=float)[:,None]
angle = \
np.angle(ind1-com[0]+1j*(ind2-com[1]))
exp_theta = np.exp(1j*angle)
angle_rot = np.angle(np.sum(np.sum(image_ref*exp_theta,axis=1)),deg=True)
# Creating temporary rotated version of input image
image_rot_aux = \
transform.rotate(image,angle_rot,resize=False,center=com,mode='nearest')
# Second rotation step based on Inertia tensor
# Again need 0 boundary condition away from object and
# thus Sobel or inverse transform
#image_ref = filters.sobel(image_rot_aux)
image_ref = 1.0 - image_rot_aux
m = moments(image_ref,order=2)
Ixx = m[2, 0]/m[0, 0] - np.power(cx,2)
Iyy = m[0, 2]/m[0, 0] - np.power(cy,2)
Ixy = m[1, 1]/m[0, 0] - cx*cy
inertia = [[Ixx, Ixy],[Ixy, Iyy]]
w, v = np.linalg.eig(inertia)
idx = w.argsort()[::-1]
w = w[idx]
v = v[:,idx]
cross = np.cross(v[:,0],v[:,1])
# Ensuring eigenvectors satisfy right-hand rule
if (cross < 0):
v[:,1] *= -1
# Ascertaining rotation angle from inertia tensor eigenvectors
angle_rad = np.arctan2(v[1,0],v[0,0]) + np.pi/2
angle_rot = np.degrees(angle_rad)
# Creating final rotated version of input image
image_rot = \
transform.rotate(image_rot_aux,angle_rot,resize=False,center=com,mode='nearest')
return image_rot
def modified_hausdorff(image1, image2, metric=cv2.NORM_L2):
''' Compute the Modified Hausdorff distance. '''
# Align center with centroids
h1, w1 = image1.shape
h2, w2 = image2.shape
m1 = measure.moments(image1, order=1)
m2 = measure.moments(image2, order=1)
xc1, yc1 = int(m1[1, 0] / m1[0, 0]), int(m1[0, 1] / m1[0, 0])
xc2, yc2 = int(m2[1, 0] / m2[0, 0]), int(m2[0, 1] / m2[0, 0])
dx1, dy1 = (xc1 - w1 / 2), (yc1 - h1 / 2)
dx2, dy2 = (xc2 - w2 / 2), (yc2 - h2 / 2)
# Contour extraction
_, contours1, hierarchy1 = cv2.findContours(image1.copy(), cv2.RETR_CCOMP,
cv2.CHAIN_APPROX_SIMPLE)
_, contours2, hierarchy2 = cv2.findContours(image2.copy(), cv2.RETR_CCOMP,
cv2.CHAIN_APPROX_SIMPLE)
# Contours drawing
padded1 = np.zeros_like(image1)
padded2 = np.zeros_like(image2)
idx = 0
while idx >= 0:
padded1 = cv2.drawContours(padded1, contours1, idx, (255, 255, 255))
idx = hierarchy1[0][idx][0]
idx = 0
while idx >= 0:
padded2 = cv2.drawContours(padded2, contours2, idx, (255, 255, 255))
idx = hierarchy2[0][idx][0]
# Padding
padded1 = np.pad(padded1, ((max(0, -dy1), max(0, dy1)),
(max(0, -dx1), max(0, dx1))),
mode='constant',
constant_values=0)
padded2 = np.pad(padded2, ((max(0, -dy2), max(0, dy2)),
(max(0, -dx2), max(0, dx2))),
mode='constant',
constant_values=0)
# Distance computations
h1, w1 = padded1.shape
h2, w2 = padded2.shape
h, w = max(h1, h2) + 2, max(w1, w2) + 2
dx1, dy1 = (w - w1) / 2, (h - h1) / 2
dx2, dy2 = (w - w2) / 2, (h - h2) / 2
base1 = np.zeros((h, w), dtype=np.uint8)
base2 = np.zeros((h, w), dtype=np.uint8)
base1[dy1:dy1 + h1, dx1:dx1 + w1] = padded1
base2[dy2:dy2 + h2, dx2:dx2 + w2] = padded2
dist1 = cv2.distanceTransform(255 - base1, metric, cv2.DIST_MASK_PRECISE)
dist2 = cv2.distanceTransform(255 - base2, metric, cv2.DIST_MASK_PRECISE)
h12 = dist1[base2 == 255].mean()
h21 = dist2[base1 == 255].mean()
return max(h12, h21)
def test_rotation():
(trainX, trainY), (testX, testY) = mnist.load_data()
fig, ax = plt.subplots(4, 10, figsize=(16, 10))
index = 10
for i in range(index, index + 10):
M_norot = moments(trainX[i], order=1)
trainX[i] = rotate(trainX[i], 90, order=1, reshape=False)
M_rot = moments(trainX[i], order=1)
print("avant", M_norot[1, 0] / M_norot[0, 0],
M_norot[0, 1] / M_norot[0, 0])
print("apres", M_rot[1, 0] / M_rot[0, 0], M_rot[0, 1] / M_rot[0, 0])
ax[0][i - index].imshow(trainX[i])
plt.show()
def centroid_com(data, data_mask=None):
"""
Calculate the centroid of an array as its center of mass determined
from image moments.
Parameters
----------
data : array_like
The image data.
data_mask : array_like, bool, optional
A boolean mask with the same shape as `data`, where a `True`
value indicates the corresponding element of `data` is invalid.
Returns
-------
centroid : tuple
(x, y) coordinates of the centroid.
"""
from skimage.measure import moments
if data_mask is not None:
if data.shape != data_mask.shape:
raise ValueError('data and data_mask must have the same shape')
data[data_mask] = 0.
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return xcen, ycen
def huMoment(self, img):
h = 1 - img
m = moments(h)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(h, cr, cc)
return mu
def fitOnImageEllipse(data):
'''
Returns the length of the long and short axis and the angle measure
of the long axis to the horizontal of the best fit ellipsebased on
image moments.
usage: longAxis, shortAxis, angle = fitEllipse(N_by_M_image_as_array)
'''
# source:
# Kieran F. Mulchrone, Kingshuk Roy Choudhury,
# Fitting an ellipse to an arbitrary shape:
# implications for strain analysis, Journal of
# Structural Geology, Volume 26, Issue 1,
# January 2004, Pages 143-153, ISSN 0191-8141,
# <http://dx.doi.org/10.1016/S0191-8141(03)00093-2.>
# Lourena Rocha, Luiz Velho, Paulo Cezar P. Carvalho
# Image Moments-Based Structuring and Tracking of
# Objects, IMPA-Instituto Nacional de Matematica Pura
# e Aplicada. Estrada Dona Castorina, 110, 22460
# Rio de Janeiro, RJ, Brasil,
# <http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1167130>
m = moments(data, 2) # super fast compated to anything in pure python
xc = m[1, 0] / m[0, 0]
yc = m[0, 1] / m[0, 0]
a = (m[2, 0] / m[0, 0]) - (xc**2)
b = 2 * ((m[1, 1] / m[0, 0]) - (xc * yc))
c = (m[0, 2] / m[0, 0]) - (yc**2)
theta = .5 * (np.arctan2(b, (a - c)))
w = np.sqrt(6 * (a + c - np.sqrt(b**2 + (a - c)**2)))
l = np.sqrt(6 * (a + c + np.sqrt(b**2 + (a - c)**2)))
return l, w, theta
def centroid_com(data, mask=None):
"""
Calculate the centroid of a 2D array as its center of mass
determined from image moments.
Parameters
----------
data : array_like or `~astropy.nddata.NDData`
The 2D array of the image.
mask : array_like, bool, optional
A boolean mask with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is
invalid. If ``mask`` is input it will override ``data.mask``
for `~astropy.nddata.NDData` inputs.
Returns
-------
xcen, ycen : tuple of floats
(x, y) coordinates of the centroid.
"""
from skimage.measure import moments
data = _convert_image(data, mask=mask)
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return xcen, ycen
def centroid_com(data, mask=None):
"""
Calculate the centroid of a 2D array as its center of mass
determined from image moments.
Parameters
----------
data : array_like or `~astropy.nddata.NDData`
The 2D array of the image.
mask : array_like, bool, optional
A boolean mask with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is
invalid. If ``mask`` is input it will override ``data.mask``
for `~astropy.nddata.NDData` inputs.
Returns
-------
xcen, ycen : tuple of floats
(x, y) coordinates of the centroid.
"""
from skimage.measure import moments
data = _convert_image(data, mask=mask)
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return xcen, ycen
def fitOnImageEllipse(data):
'''
Returns the length of the long and short axis and the angle measure
of the long axis to the horizontal of the best fit ellipsebased on
image moments.
usage: longAxis, shortAxis, angle = fitEllipse(N_by_M_image_as_array)
'''
# source:
# Kieran F. Mulchrone, Kingshuk Roy Choudhury,
# Fitting an ellipse to an arbitrary shape:
# implications for strain analysis, Journal of
# Structural Geology, Volume 26, Issue 1,
# January 2004, Pages 143-153, ISSN 0191-8141,
# <http://dx.doi.org/10.1016/S0191-8141(03)00093-2.>
# Lourena Rocha, Luiz Velho, Paulo Cezar P. Carvalho
# Image Moments-Based Structuring and Tracking of
# Objects, IMPA-Instituto Nacional de Matematica Pura
# e Aplicada. Estrada Dona Castorina, 110, 22460
# Rio de Janeiro, RJ, Brasil,
# <http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1167130>
m = moments(data, 2) # super fast compated to anything in pure python
xc = m[1,0] / m[0,0]
yc = m[0,1] / m[0,0]
a = (m[2,0] / m[0,0]) - (xc**2)
b = 2 * ((m[1,1] / m[0,0]) - (xc * yc))
c = (m[0,2] / m[0,0]) - (yc**2)
theta = .5 * (np.arctan2(b, (a - c)))
w = np.sqrt(6 * (a + c - np.sqrt(b**2 + (a-c)**2)))
l = np.sqrt(6 * (a + c + np.sqrt(b**2 + (a-c)**2)))
return l, w, theta
def get_moments(image):
''' Image moments does not perform well in this scenario, I didn't
investigated the source
'''
order = 7
imm = measure.moments(image, order=order)
return imm
def centroid_com(data, mask=None):
"""
Calculate the centroid of a 2D array as its center of mass
determined from image moments.
Parameters
----------
data : array_like
The 2D array of the image.
mask : array_like (bool), optional
A boolean mask, with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is masked.
Returns
-------
xcen, ycen : float
(x, y) coordinates of the centroid.
"""
from skimage.measure import moments
data = _convert_image(data, mask=mask)
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return xcen, ycen
def get_hu_moments(samples):
print "getting hu moments..."
features = []
for sample in samples:
'''
sample = np.array(sample)
th = 200
img_binary = (sample < th).astype(np.double)
img_label = label(img_binary, background=255)
regions = regionprops(img_label)
if regions == []:
print "no regions"
for props in regions:
minr, minc, maxr, maxc = props.bbox
roi = img_binary[minr:maxr, minc:maxc]
'''
sample = np.array(sample)
sample = sample.astype(np.double)
m = moments(sample)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(sample, cr, cc)
nu = moments_normalized(mu)
hu = moments_hu(nu)
features.append(hu)
return features
def calculateCentroid(self, mask, bbox):
m = measure.moments(mask)
c = np.array((m[0, 1] / m[0, 0], m[1, 0] / m[0, 0]))
#centroid is (x, y) while measure returns (y,x and bbox is yx)
self.centroid = np.array((c[0] + bbox[1], c[1]+ bbox[0]))
self.blob_name = "c-{:d}-{:.1f}x-{:.1f}y".format(self.id, self.centroid[0], self.centroid[1])
def decision(fruit1, avg_momnt1, avg_momnt2, type_sample="Testing"):
"""
Decision which fruit fits each image and calculate error
ARGS:
fruit1 - name of 1st fruit
avg_moment1 - average moment value of dataset[fruit1]
avg_moment2 - average moment value of dataset[fruit2]
type_sample - name of root folder (Training or Testing)
RETURN VALUE:
list with error for each image
(If wrong decision: value error have minus)
"""
os.chdir(type_sample + "/" + fruit1)
img_list = os.listdir(path=os.getcwd())
decision_list = []
for img in img_list:
image = io.imread(img)
img_grayscale = color.rgb2gray(image)
edges = filters.sobel(img_grayscale) # FILTER
cur_moment = float(moments(edges, order=0))
err1 = abs(cur_moment - avg_momnt1)
err2 = abs(cur_moment - avg_momnt2)
if err1 < err2:
decision_list.append(err1)
else:
decision_list.append(-1 * err2)
os.chdir(os.getcwd() + "/../../")
return decision_list
def bscan_cut(bscans, onh_ybox=[-1, -1]):
if onh_ybox != [-1, -1]:
#either no coordinates were entered, or they weren't detected
cut_scans = bscans[onh_ybox[0]:onh_ybox[1], :, :]
else:
cut_scans = bscans[120:136, :, :]
avg_scans = np.mean(cut_scans, axis=0)
#Email from Mayank to Eric on 8-15-2015 on Mayank and Robert's formula to resize bscans to 1 px**2
#height = y_height*0.84
#width = 1600 px
height = np.round(avg_scans.shape[1] * 0.84)
width = 1600
scan = tf.resize(avg_scans, (height, width), order=3, mode="reflect")
#drop to 8 bit, otherwise the averaging takes a very long time. Which seems strange...
scan_s = scan.astype("uint8")
scan_m = sf.rank.mean(scan_s, selem=mp.disk(50))
#Worried there are issues with top hat. May smear in noise that becomes part of the center of mass computation.
scan_b = mp.white_tophat(scan_m, selem=mp.square(500))
m = sm.moments(scan_b, order=1)
y = int(np.round(m[0, 1] / m[0, 0]))
ymin = y - 300
ymax = y + 300
cut_scan = scan[ymin:ymax, :]
return cut_scan.astype("float32")
def centroid_com(data, mask=None):
"""
Calculate the centroid of a 2D array as its center of mass
determined from image moments.
Parameters
----------
data : array_like
The 2D array of the image.
mask : array_like (bool), optional
A boolean mask, with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is masked.
Returns
-------
xcen, ycen : float
(x, y) coordinates of the centroid.
"""
from skimage.measure import moments
data = _convert_image(data, mask=mask)
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return xcen, ycen
def get_hu_moment_from_image(image):
"""
Compute the 7 Hu's moments from an image.
This set of moments is proofed to be translation, scale and rotation invariant.
Parameters
----------
image: array-like
a 2d array of double or uint8 corresponding to an image
Returns
-------
(7, 1) array of double
7 Hu's moments
References
----------
http://scikit-image.org/docs/dev/api/skimage.measure.html#skimage.measure.moments
"""
order = 7
raw_moments = moments(image, order=order)
cr = raw_moments[0, 1] / raw_moments[0, 0]
cc = raw_moments[1, 0] / raw_moments[0, 0]
central_moments = moments_central(image, cr, cc, order=order)
normalized_moments = moments_normalized(central_moments, order)
hu_moments = moments_hu(normalized_moments)
return hu_moments
def extract_features(roi, props):
features = []
m = moments(roi)
# print(m)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(roi, (cr, cc))
nu = moments_normalized(mu)
#finding Seven Features
hu = moments_hu(nu)
# seven features to be put into feature list
features.extend(hu)
# print(features)
features.append(roi.shape[1]/roi.shape[0])
features.append(props.eccentricity)
features.append(props.convex_area/props.area)
features.append(props.orientation)
features.append(props.euler_number)
return np.array([features])
def collect(path, mean, std):
img = io.imread('./images/' + path + '.bmp')
hist = exposure.histogram(img)
th = get_threshold('./images/' + path + '.bmp')
img_binary = (img < th).astype(np.double)
img_label = label(img_binary, background=0)
regions = regionprops(img_label)
boxes = []
features = []
for props in regions:
box = []
minr, minc, maxr, maxc = props.bbox
if maxc - minc < 10 or maxr - minr < 10 or maxc - minc > 120 or maxr - minr > 120:
continue
box.append(minr)
box.append(maxr)
box.append(minc)
box.append(maxc)
boxes.append(box)
roi = img_binary[minr:maxr, minc:maxc]
m = moments(roi)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(roi, cr, cc)
nu = moments_normalized(mu)
hu = moments_hu(nu)
features.append(hu)
feature_arr = normalize(features, mean, std)
return (boxes, feature_arr)
def extract_features(path, show, tag):
img = io.imread('./images/' + path + '.bmp')
hist = exposure.histogram(img)
th = get_threshold('./images/' + path + '.bmp')
img_binary = (img < th).astype(np.double)
img_label = label(img_binary, background=0)
# Show images
if show == 1:
io.imshow(img)
plt.title('Original Image')
io.show()
plt.bar(hist[1], hist[0])
plt.title('Histogram')
plt.show()
io.imshow(img_binary)
plt.title('Binary Image')
io.show()
io.imshow(img_label)
plt.title('Labeled Image')
io.show()
regions = regionprops(img_label)
if show == 1:
io.imshow(img_binary)
ax = plt.gca()
features = []
for props in regions:
minr, minc, maxr, maxc = props.bbox
if maxc - minc < 10 or maxr - minr < 10 or maxc - minc > 120 or maxr - minr > 120:
continue
if show == 1:
ax.add_patch(
Rectangle((minc, minr),
maxc - minc,
maxr - minr,
fill=False,
edgecolor='red',
linewidth=1))
roi = img_binary[minr:maxr, minc:maxc]
m = moments(roi)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(roi, cr, cc)
nu = moments_normalized(mu)
hu = moments_hu(nu)
features.append(hu)
if (len(path) == 1):
tag.append(ord(path))
if show == 1:
plt.title('Bounding Boxes')
io.show()
return features
def test_moments(anisotropic):
image = np.zeros((20, 20), dtype=np.float64)
image[14, 14] = 1
image[15, 15] = 1
image[14, 15] = 0.5
image[15, 14] = 0.5
if anisotropic:
spacing = (1.4, 2)
else:
spacing = (1, 1)
if anisotropic is None:
m = moments(image)
else:
m = moments(image, spacing=spacing)
assert_equal(m[0, 0], 3)
assert_almost_equal(m[1, 0] / m[0, 0], 14.5 * spacing[0])
assert_almost_equal(m[0, 1] / m[0, 0], 14.5 * spacing[1])
def MM_area(im1):
import numpy as np
from skimage.measure import moments
I = np.array(im1, dtype=np.double)
M = moments(I)
area = M[0, 0]
return area
def compute_hu_moments(i):
b = cells_aligned_padded[i].astype(np.uint8)
m = moments(b, order=1)
hu = moments_hu(
moments_normalized(
moments_central(b, cc=m[0, 1] / m[0, 0],
cr=m[1, 0] / m[0, 0])))
return hu
def calculateCentroid(self, mask):
m = measure.moments(mask)
c = np.array((m[0, 1] / m[0, 0], m[1, 0] / m[0, 0]))
#centroid is (x, y) while measure returns (y,x and bbox is yx)
self.centroid = np.array((c[1] + self.bbox[1], c[0] + self.bbox[0]))
self.blob_name = "coral-" + str(self.centroid[0]) + "-" + str(
self.centroid[1])
def test_moments_coords():
image = np.zeros((20, 20), dtype=np.double)
image[13:17, 13:17] = 1
mu_image = moments(image)
coords = np.array([[r, c] for r in range(13, 17) for c in range(13, 17)],
dtype=np.double)
mu_coords = moments_coords(coords)
assert_almost_equal(mu_coords, mu_image)
def test_moments_coords():
image = np.zeros((20, 20), dtype=np.double)
image[13:17, 13:17] = 1
mu_image = moments(image)
coords = np.array([[r, c] for r in range(13, 17)
for c in range(13, 17)], dtype=np.double)
mu_coords = moments_coords(coords)
assert_almost_equal(mu_coords, mu_image)
def testKNN():
trainFeatures, trainLebels = extractFeatures()
knn = neighbors.KNeighborsClassifier()
knn.fit(trainFeatures, trainLebels)
#score = knn.score(trainFeatures, trainLebels)
testNames = ['test1', 'test2']
#testNames = ['test2']
testFeatures = []
testLabels = []
testTruth = []
correct = 0
#textPosition = []
for i in range(len(testNames)):
classes, locations = readPkl(testNames[i])
img = io.imread(testNames[i] + '.bmp')
#testTruth = ['a']*7+['d']*7+['m']*7+['n']*7+['o']*7+['p']*7+['q']*7+['r']*7+['u']*7+['w']*7
ret, binary = cv.threshold(img, 0, 255, cv.THRESH_BINARY | cv.THRESH_OTSU)
#ret, binary = cv.threshold(img, 0, 255, cv.THRESH_BINARY | cv.THRESH_TRIANGLE)
th = ret
img_binary = (img < th).astype(np.double)
img_dilation = morphology.binary_dilation(img_binary, selem=None)
img_erosion = morphology.binary_erosion(img_binary, selem=None)
img_label = label(img_binary, background=0)
regions = regionprops(img_label)
io.imshow(img_binary)
ax = plt.gca()
thresholdR = 15
thresholdC = 15
for props in regions:
minr, minc, maxr, maxc = props.bbox
# Computing Hu Moments and Removing Small Components
if (maxr - minr) >= thresholdR and (maxc - minc) >= thresholdC:
#textPosition.append((maxc, minr))
roi = img_binary[minr:maxr, minc:maxc]
m = moments(roi)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(roi, cr, cc)
nu = moments_normalized(mu)
hu = moments_hu(nu)
testFeatures.append(hu)
testLabels.append(knn.predict([testFeatures[-1]]))
indexFix = locationFix(locations, minr, minc, maxr, maxc)
if indexFix is not None:
if testLabels[-1] == classes[indexFix]:
correct += 1
plt.text(maxc, minr, testLabels[-1][0], bbox=dict(facecolor='white', alpha=0.5))
ax.add_patch(Rectangle((minc, minr), maxc - minc, maxr - minr, fill=False, edgecolor='red', linewidth=1))
plt.title('Bounding Boxes')
io.show()
print correct, len(testLabels)
correctRate = correct / len(testLabels)
print correctRate
def extractFeature(name, showall, showbb, flag):
(img, regions, ax, rthre, cthre) = extractImage(name, showall, showbb,
flag)
Features = []
boxes = []
for props in regions:
tmp = []
minr, minc, maxr, maxc = props.bbox
if maxc - minc < cthre or maxr - minr < rthre or maxc - minc > cthre * 9 or maxr - minr > rthre * 9:
continue
tmp.append(minr)
tmp.append(minc)
tmp.append(maxr)
tmp.append(maxc)
boxes.append(tmp)
if showbb == 1:
ax.add_patch(
Rectangle((minc, minr),
maxc - minc,
maxr - minr,
fill=False,
edgecolor='red',
linewidth=1))
# computing hu moments and removing small components
roi = img[minr:maxr, minc:maxc]
m = moments(roi)
cr = m[0, 1] / m[0, 0]
cc = m[1, 0] / m[0, 0]
mu = moments_central(roi, cr, cc)
nu = moments_normalized(mu)
hu = moments_hu(nu)
area = (maxr - minr) * (maxc - minc)
# add convexity
p = perimeter(img[minr:maxr, minc:maxc])
con = (area / (p * p)) * 4 * math.pi
convex = np.array([con])
hu = np.concatenate((hu, convex))
# add density
den = area / float(props.convex_area)
dense = np.array([den])
hu = np.concatenate((hu, dense))
Features.append(hu)
# print boxes
plt.title('Bounding Boxes')
if showbb == 1:
io.show()
return Features, boxes,
def test_moments():
image = np.zeros((20, 20), dtype=np.double)
image[14, 14] = 1
image[15, 15] = 1
image[14, 15] = 0.5
image[15, 14] = 0.5
m = moments(image)
assert_equal(m[0, 0], 3)
assert_almost_equal(m[1, 0] / m[0, 0], 14.5)
assert_almost_equal(m[0, 1] / m[0, 0], 14.5)
def get_inertia(mask, mu=None):
"""compute inertia tensor and eigenvalues from mask, if moments are give the function is much faster"""
if mu is None:
mu = measure.moments(mask)
inertia_tensor = measure.inertia_tensor(mask, mu)
inertia_eigen = measure.inertia_tensor_eigvals(mask,
mu=mu,
T=inertia_tensor)
return inertia_tensor, inertia_eigen
def find_centroid(pic):
from skimage.measure import moments
import numpy as np
if len(pic.shape) > 2:
pic = np.copy(pic).reshape(list(pic.shape)[:-1])
M = moments(pic)
centroid = (M[1, 0] / M[0, 0], M[0, 1] / M[0, 0])
return centroid
def test_moments():
image = np.zeros((20, 20), dtype=np.double)
image[14, 14] = 1
image[15, 15] = 1
image[14, 15] = 0.5
image[15, 14] = 0.5
m = moments(image)
assert_equal(m[0, 0], 3)
assert_almost_equal(m[0, 1] / m[0, 0], 14.5)
assert_almost_equal(m[1, 0] / m[0, 0], 14.5)
def getcentroid(filename, box):
ia.open(filename)
imgdataraw = ia.getregion()
headerlist = ia.summary()
ia.close()
x0,x1,y0,y1 = box
imgdata = np.squeeze(imgdataraw) #in units of Jy/beam
xpix = imgdata.shape[0] #confirmed that imgdata is x,y
ypix = imgdata.shape[1]
xcen, ycen = headerlist['refpix'][0], headerlist['refpix'][1]
RA0, DEC0 = headerlist['refval'][0], headerlist['refval'][1]
deltaRA, deltaDEC = headerlist['incr'][0], headerlist['incr'][1]
bminor = headerlist['restoringbeam']['minor']['value']
bmajor = headerlist['restoringbeam']['major']['value']
ang = headerlist['restoringbeam']['positionangle']['value']
beamsize = np.pi*bminor*bmajor/(4*np.log(2)) #in arcsec^2
print "The beam shape is %.3f, %.3f, %.3f" % (bmajor, bminor, ang)
cellsize = headerlist['incr'][1]*206265 #in arcsec
print "The image size is %d pixels" % imgdata.shape[0]
#background calculations
bg1 = imgdata[50:xpix-50 ,50:150]
bg2 = imgdata[50:xpix - 50, ypix - 150:ypix - 50]
bgmean = 0.5*(np.mean(bg1)+np.mean(bg2))
rms = np.sqrt(np.sum((bg1-bgmean)**2+(bg2-bgmean)**2)/(float(bg1.size)+float(bg2.size)))
print "The image rms is %.3e" % rms
#m = moments(image = imgdata[xpix/2-75:xpix/2+75,ypix/2-75:ypix/2+75], order = 1)
#print "The image centroid is (%.3f, %.3f)" % (xpix/2-75+m[0,1]/m[0,0], ypix/2-75+m[1,0]/m[0,0])
m = moments(image = imgdata[x0:x1,y0:y1], order = 1)
print "The image centroid is (%.3f, %.3f)" % (x0+m[0,1]/m[0,0], y0+m[1,0]/m[0,0])
centroidRA = (RA0+deltaRA*(x0+m[0,1]/m[0,0]-xcen))*180/np.pi*1/15.
centroidDEC = (DEC0+deltaDEC*(y0+m[1,0]/m[0,0]-ycen))*180/np.pi
ra = np.zeros(3)
ra[0] = int(centroidRA)
ra[1] = np.abs(int((centroidRA - ra[0])*60))
ra[2] = (np.abs(centroidRA)-np.abs(ra[0])-ra[1]/60.)*3600
dec = np.zeros(3)
dec[0] = int(centroidDEC)
dec[1] = np.abs(int((centroidDEC - dec[0])*60))
dec[2] = (np.abs(centroidDEC)-np.abs(dec[0])-dec[1]/60.)*3600
print "The coordinates are RA %d:%d:%.3f, DEC %d:%d:%.3f" % (ra[0], ra[1], ra[2], dec[0], dec[1], dec[2])
def test_moments_central_deprecated():
image = np.zeros((20, 20), dtype=np.double)
image[5:-5, 5:-5] = np.random.random((10, 10))
center = moments(image, 1)[[1, 0], [0, 1]]
cr, cc = center
with expected_warnings(['deprecated 2D-only']):
mu0 = moments_central(image, cr, cc)
mu1 = moments_central(image, cr=cr, cc=cc)
mu_ref = moments_central(image, center)
assert_almost_equal(mu0.T, mu_ref)
assert_almost_equal(mu1.T, mu_ref)
def _irafstarfind_moments(imgcutout, kernel, sky):
"""
Find the properties of each detected source, as defined by IRAF's
``starfind``.
Parameters
----------
imgcutout : `_ImgCutout`
The image cutout for a single detected source.
kernel : `_FindObjKernel`
The convolution kernel. The dimensions should match those of
``imgcutout``. ``kernel.gkernel`` should have a peak pixel
value of 1.0 and not contain any masked pixels.
sky : float
The local sky level around the source.
Returns
-------
result : dict
A dictionary of the object parameters.
"""
from skimage.measure import moments, moments_central
result = defaultdict(list)
img = np.array((imgcutout.data - sky) * kernel.mask)
img = np.where(img > 0, img, 0) # starfind discards negative pixels
if np.count_nonzero(img) <= 1:
return {}
m = moments(img, 1)
result['xcentroid'] = m[1, 0] / m[0, 0]
result['ycentroid'] = m[0, 1] / m[0, 0]
result['npix'] = float(np.count_nonzero(img)) # float for easier testing
result['sky'] = sky
result['peak'] = np.max(img)
flux = img.sum()
result['flux'] = flux
result['mag'] = -2.5 * np.log10(flux)
mu = moments_central(
img, result['ycentroid'], result['xcentroid'], 2) / m[0, 0]
musum = mu[2, 0] + mu[0, 2]
mudiff = mu[2, 0] - mu[0, 2]
result['fwhm'] = 2.0 * np.sqrt(np.log(2.0) * musum)
result['sharpness'] = result['fwhm'] / kernel.fwhm
result['roundness'] = np.sqrt(mudiff**2 + 4.0*mu[1, 1]**2) / musum
pa = 0.5 * np.arctan2(2.0 * mu[1, 1], mudiff) * (180.0 / np.pi)
if pa < 0.0:
pa += 180.0
result['pa'] = pa
result['xcentroid'] += imgcutout.x0
result['ycentroid'] += imgcutout.y0
return result
def test_moments_central_deprecated():
image = np.zeros((20, 20), dtype=np.double)
image[5:-5, 5:-5] = np.random.random((10, 10))
center = moments(image, 1)[[1, 0], [0, 1]]
cr, cc = center
with expected_warnings(['deprecated 2D-only']):
mu0 = moments_central(image, cr, cc)
mu1 = moments_central(image, cr=cr, cc=cc)
mu_ref = moments_central(image, center)
assert_almost_equal(mu0.T, mu_ref)
assert_almost_equal(mu1.T, mu_ref)
def main(raw_images,ntrans,Phi,coords_r,coords_c):
import w_subimg
lines = ntrans * ['line_id']
epoch = Phi
nepoch = len(Phi)
# centroid position for each transition and epoch and blob
# (middle col refers to the blobs and last col refers to x,y)
centroid_array = np.zeros((ntrans*nepoch,2,2))
flux_array = np.zeros((ntrans*nepoch,2))
for j in range(2):
coord1_r, coord2_r = coords_r[2*j:2*(j+1)]
coord1_c, coord2_c = coords_c[2*j:2*(j+1)]
for i in range(ntrans*nepoch):
if raw_images[i][1] == 'zero.fits':
raw_images[i][2] = raw_images[i][2] * 0
# call the sub-image function
subimg = w_subimg.main(raw_images[i][2],raw_images[i][5],coord1_r,coord1_c,coord2_r,coord2_c)
subim_r, extent = subimg[0:2]
row1, row2, col1, col2 = subimg[2:]
# extracting the subimage
img = subim_r.astype('double')
if raw_images[i][1] != 'zero.fits':
# pos = feature.blob_dog(img, threshold=1e-14, min_sigma=1.5, max_sigma=2.0, overlap=0.5)
pos = feature.peak_local_max(img, threshold_abs=1e-14, min_distance=1)
mom = measure.moments(img)
'''
The following properties can be calculated from raw image moments:
Area as: m[0, 0].
Centroid as: {m[0, 1] / m[0, 0], m[1, 0] / m[0, 0]}.
'''
centroid = [mom[0,1] / mom[0,0], mom[1,0] / mom[0,0]]
# centroid2 = get_centroid(img)
# center of img
center = (((raw_images[i][2]).shape)[0] - 1) / 2
cent_col = (center - (col1+centroid[1])) * raw_images[i][5]
cent_row = (row1+centroid[0] - center) * raw_images[i][5]
centroid_array[i,j,:] = [cent_row,cent_col]
# *REMOVING* THE FLUX CONSERVATION *PER PIXEL* CORRECTION FACTOR
flux_array[i,j] = np.sum(img) * (raw_images[i][5] / 0.1)**2
if pos.shape[0] != 0:
pos_col = (center - (col1+pos[:,1]).flatten()) * raw_images[i][5]
pos_row = ((row1+pos[:,0]).flatten() - center) * raw_images[i][5]
return centroid_array
def extract_features(img):
# This function extract our features out of an image. It basically
# computes the 8 (and not 7) Hu geometrical moments. To do this we
# first compute the moments, centralize and normalize them before
# computing Hu moments
m = moments(img)
cr = m[0,1] / m[0,0]
cc = m[1,0] / m[0,0]
mc = moments_central(img, cr, cc)
mn = moments_normalized(mc)
hu = moments_hu(mn)
i8 = mn[1, 1] * ( (mn[3, 0] + mn[1, 2])**2 - (mn[0,3]+mn[2,1])**2 ) - (mn[2,0] - mn[0,2]) * (mn[3,0] + mn[1,2]) * (mn[0,3] + mn[2,1])
return append(hu, [i8])
def centroid_com(data, mask=None):
"""
Calculate the centroid of a 2D array as its "center of mass"
determined from image moments.
Invalid values (e.g. NaNs or infs) in the ``data`` array are
automatically masked.
Parameters
----------
data : array_like
The 2D array of the image.
mask : array_like (bool), optional
A boolean mask, with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is masked.
Returns
-------
centroid : `~numpy.ndarray`
The ``x, y`` coordinates of the centroid.
"""
from skimage.measure import moments
data = np.ma.asanyarray(data)
if mask is not None and mask is not np.ma.nomask:
mask = np.asanyarray(mask)
if data.shape != mask.shape:
raise ValueError('data and mask must have the same shape.')
data.mask |= mask
if np.any(~np.isfinite(data)):
data = np.ma.masked_invalid(data)
warnings.warn('Input data contains input values (e.g. NaNs or infs), '
'which were automatically masked.', AstropyUserWarning)
# Convert the data to a float64 (double) `numpy.ndarray`,
# which is required for input to `skimage.measure.moments`.
# Masked values are set to zero.
data = data.astype(np.float)
data.fill_value = 0.
data = data.filled()
m = moments(data, 1)
xcen = m[1, 0] / m[0, 0]
ycen = m[0, 1] / m[0, 0]
return np.array([xcen, ycen])
def momentos_hu(self):
"""
Calcula os 7 momentos de Hu
"""
m = measure.moments(self.imagemTonsDeCinza)
row = m[0, 1] / m[0, 0]
col = m[1, 0] / m[0, 0]
mu = measure.moments_central(self.imagemTonsDeCinza,row,col)
nu = measure.moments_normalized(mu)
hu = measure.moments_hu(nu)
valores = list(hu)
nomes = [m+n for m,n in zip(['hu_'] * len(valores),map(str,range(0,len(valores))))]
tipos = [numerico] * len(nomes)
return nomes, tipos, valores
def get_moments(self):
"""
Return moments from frame
Returns
-------
moments : pandas Series object with the following keys
- m10 : row position of centroid
- m01 : col position of centroid
- mupr20 : higher moments
- mupr02 : higher moments
- mupr11 : higher moments
"""
frame = ma.masked_invalid(self)
frame.fill_value = 0
frame = frame.filled()
frame *= self.ap_weights # Multiply frame by aperture weights
# Compute the centroid
m = measure.moments(frame)
m10=m[1,0]
m01=m[0,1]
moments = np.array([m10,m01])
moments /= m[0,0]
# Compute central moments (second order)
mu = measure.moments_central(frame,moments[0],moments[1])
mupr20 = mu[2,0]
mupr02 = mu[0,2]
mupr11 = mu[1,1]
c_moments = np.array([mupr20,mupr02,mupr11])
c_moments/=mu[0,0]
moments = np.hstack([moments,c_moments])
return moments
def shape_params(data, data_mask=None):
"""
Calculate the centroid and shape parameters for an object using
image moments.
Parameters
----------
data : array_like
The 2D image data.
data_mask : array_like, bool, optional
A boolean mask with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is
invalid.
Returns
-------
dict : A dictionary containing the object shape parameters:
* ``xcen, ycen``: object centroid (zero-based origin).
* ``major_axis``: length of the major axis
* ``minor_axis``: length of the minor axis
* ``eccen``: eccentricity. The ratio of half the distance
between its two ellipse foci to the length of the the
semimajor axis.
* ``pa``: position angle of the major axis. Increases
clockwise from the positive x axis.
* ``covar``: corresponding covariance matrix for a 2D Gaussian
* ``linear_eccen`` : linear eccentricity is the distance between
the object center and either of its two ellipse foci.
"""
from skimage.measure import moments, moments_central
if data_mask is not None:
if data.shape != data_mask.shape:
raise ValueError('data and data_mask must have the same shape')
data[data_mask] = 0.
result = {}
xcen, ycen = centroid_com(data)
m = moments(data, 1)
mu = moments_central(data, ycen, xcen, 2) / m[0, 0]
result['xcen'] = xcen
result['ycen'] = ycen
# musum = mu[2, 0] + mu[0, 2]
mudiff = mu[2, 0] - mu[0, 2]
pa = 0.5 * np.arctan2(2.0*mu[1, 1], mudiff) * (180.0 / np.pi)
if pa < 0.0:
pa += 180.0
result['pa'] = pa
covar = np.array([[mu[2, 0], mu[1, 1]], [mu[1, 1], mu[0, 2]]])
result['covar'] = covar
eigvals, eigvecs = np.linalg.eigh(covar)
majsq = np.max(eigvals)
minsq = np.min(eigvals)
result['major_axis'] = np.sqrt(majsq)
result['minor_axis'] = np.sqrt(minsq)
# if True: # equivalent calculation
# tmp = np.sqrt(4.0*mu[1,1]**2 + mudiff**2)
# majsq = 0.5 * (musum + tmp)
# minsq = 0.5 * (musum - tmp)
# result['major_axis2'] = np.sqrt(majsq)
# result['minor_axis2'] = np.sqrt(minsq)
result['eccen'] = np.sqrt(1.0 - (minsq / majsq))
result['linear_eccen'] = np.sqrt(majsq - minsq)
return result
NewXs=np.arange(PosMinCtr-ExtSrch,PosMinCtr+ExtSrch,10)
#[a,b,c]=np.polyfit(FitXs,FitPnts,2)
#Xmax=
FitPnts=SegmntSMPadd[PosMaxCtr-ExtSrch:PosMaxCtr+ExtSrch]
Col=ss.medfilt(ZProjLog.max(axis=0),25)
MaxPos=Col.argmax()
scipy.misc.imsave('ZProjLog.jpg', ZProjLog)
scipy.misc.imsave('ZProj.jpg', ZProj)
#HoughRadii=np.arange(MaxPos-MaxHough,MaxPos+MaxHough,5)
#hough_res = hough_circle(ZProj, HoughRadii)
M=meas.moments(ZProj.astype('uint8'))
cx = M[0, 1] / M[0, 0]
cy = M[1, 0] / M[0, 0]
[cxc,cyc]=ZProj.shape
yCorr=int(cy-cyc/2)
xCorr=int(cx-cxc/2)
ZProj1=np.roll(ZProj,-xCorr,axis=0)
ZProj2=np.roll(ZProj1,-yCorr,axis=1)
pp.matshow(ZProj2)
Col=ss.medfilt(Img.max(axis=0),5)
Row=ss.medfilt(Img.max(axis=1),5)
MR=np.median(Row)
def geom_moments_sk(self, order):
return measure.moments(self.image, order=order)
imshow(imgLabel, cmap = cm.Greys_r, interpolation = 'none')
# Assignment 4 - Morphology # - not done yet
img = array(Image.open('figure_problem_set_4.tiff'))
img = 1 * (img > 1)
imshow(img, cmap = cm.Greys_r, interpolation = 'none')
equivTable, imgLabel = regionLabel(img)
imshow(imgLabel, cmap = cm.Greys_r, interpolation = 'none')
# HOMEWORK 6
# Assignment 3 - calculate moments
img = skimageIO.imread('img_moment.tif').astype(float)
imshow(img, cmap = cm.Greys_r, interpolation = 'none')
moments_deg1 = skimageMeasure.moments(img, order = 1)
x0 = moments_deg1[0, 1] / moments_deg1[0, 0]
y0 = moments_deg1[1, 0] / moments_deg1[0, 0]
momentsCentral_deg2 = skimageMeasure.moments_central(img, x0, y0, order = 2)
m00 = momentsCentral_deg2[0, 0]
m11 = momentsCentral_deg2[1, 1]
m02 = momentsCentral_deg2[0, 2]
m20 = momentsCentral_deg2[2, 0]
orientation = degrees(arctan2(2 * m11, (m20 - m02)) / 2)
# HOUGH TRANSFORM HOMEWORK
img = skimageIO.imread('img_hough_circle.tiff').astype(float)
# Enhance edges by Sobel operator
h1 = array([[1, 2, 1], [0, 0, 0], [-1, -2, -1]])
imgH1 = convolve2d(img, h1)
def compute_hu_moments(i):
b = cells_aligned_padded[i].astype(np.uint8)
m = moments(b, order=1)
hu = moments_hu(moments_normalized(moments_central(b, cc=m[0,1]/m[0,0], cr=m[1,0]/m[0,0])))
return hu
def shape_params(data, mask=None):
"""
Calculate the centroid and shape parameters of a 2D array (e.g., an
image cutout of an object) using image moments.
Parameters
----------
data : array_like or `~astropy.nddata.NDData`
The 2D array of the image.
mask : array_like, bool, optional
A boolean mask with the same shape as ``data``, where a `True`
value indicates the corresponding element of ``data`` is
invalid. If ``mask`` is input it will override ``data.mask``
for `~astropy.nddata.NDData` inputs.
Returns
-------
params : dict
A dictionary containing the object shape parameters:
* ``xcen, ycen``: The object centroid (zero-based origin).
* ``major_axis``: The length of the major axis of the ellipse
that has the same second-order moments as the input image.
* ``minor_axis``: The length of the minor axis of the ellipse
that has the same second-order moments as the input image.
* ``eccen``: The eccentricity of the ellipse that has the same
second-order moments as the input image. The eccentricity is
the ratio of half the distance between the two ellipse foci to
the length of the semimajor axis.
* ``angle``: Angle in radians between the positive x axis and
the major axis of the ellipse that has the same second-order
moments as the input image. The angle increases
counter-clockwise.
* ``covar``: The covariance matrix of the ellipse that has the
same second-order moments as the input image.
* ``linear_eccen`` : The linear eccentricity of the ellipse that
has the same second-order moments as the input image. Linear
eccentricity is the distance between the ellipse center and
either of its two foci.
"""
from skimage.measure import moments, moments_central
data = _convert_image(data, mask=mask)
xcen, ycen = centroid_com(data)
m = moments(data, 1)
mu = moments_central(data, ycen, xcen, 2) / m[0, 0]
result = {}
result['xcen'] = xcen
result['ycen'] = ycen
mudiff = mu[2, 0] - mu[0, 2]
angle = 0.5 * np.arctan2(2.0 * mu[1, 1], mudiff) * (180.0 / np.pi)
if angle < 0.0:
angle += np.pi
result['angle'] = angle
covar = np.array([[mu[2, 0], mu[1, 1]], [mu[1, 1], mu[0, 2]]])
result['covar'] = covar
eigvals, eigvecs = np.linalg.eigh(covar)
majsq = np.max(eigvals)
minsq = np.min(eigvals)
result['major_axis'] = np.sqrt(majsq)
result['minor_axis'] = np.sqrt(minsq)
# equivalent calculation of major/minor axes:
# tmp = np.sqrt(4.0*mu[1,1]**2 + mudiff**2)
# musum = mu[2, 0] + mu[0, 2]
# majsq = 0.5 * (musum + tmp)
# minsq = 0.5 * (musum - tmp)
# result['major_axis2'] = np.sqrt(majsq)
# result['minor_axis2'] = np.sqrt(minsq)
result['eccen'] = np.sqrt(1.0 - (minsq / majsq))
result['linear_eccen'] = np.sqrt(majsq - minsq)
return result
def position(data, coords_row, coords_col):
import numpy as np
import w_subimg
import copy
from skimage import measure
from skimage import feature
ntrans = len(np.unique(data['lineID']))
nepoch = len(np.unique(data['JD']))
Phi = np.unique(data['Phi'])
# http://www.python-course.eu/passing_arguments.php
# https://jeffknupp.com/blog/2012/11/13/is-python-callbyvalue-or-callbyreference-neither/
dic = copy.deepcopy(data) # <- THIS IS VERY IMPORTANT! KEEP copy.deepcopy()!
dic['coords'] = [] # new key: centroid coordinates (x,y)
dic['dist'] = [] # new key: centroid position
dic['pa'] = [] # new key: position angle E from N
raw_images = [
data['fileName'],
data['image'],
data['pixScale']
]
for j in range(ntrans):
for i in range(nepoch):
index = i + j * nepoch
# print(j, i, index, raw_images[0][index], coords_row, coords_col)
if raw_images[0][index] == 'zero.fits':
raw_images[1][index] = raw_images[1][index] * 0
# call the sub-image function
subimg = w_subimg.main(raw_images[1][index],
raw_images[2][index],
coords_row[0], coords_col[0],
coords_row[1], coords_col[1])
subim_r, extent = subimg[0:2]
row1, row2, col1, col2 = subimg[2:]
# extracting the subimage
img = subim_r.astype('double')
mom = measure.moments(img)
'''
The following properties can be calculated from raw image moments:
Area as: m[0, 0].
Centroid as: {m[0, 1] / m[0, 0], m[1, 0] / m[0, 0]}.
'''
centroid = [mom[0,1] / mom[0,0], mom[1,0] / mom[0,0]]
# centroid2 = get_centroid(img)
# center of img
center = (((raw_images[1][index]).shape)[0] - 1) / 2
cent_col = (center - (col1+centroid[1])) * raw_images[2][index]
cent_row = (row1+centroid[0] - center) * raw_images[2][index]
# position angle measured E from N
dist = np.sqrt(cent_col**2 + cent_row**2)
pa = (2. * np.pi - np.arctan(cent_col/cent_row)) / np.pi * 180.
dic["dist"].append(dist)
dic["coords"].append([cent_row,cent_col])
dic["pa"].append(pa)
return dic
def estimate_params(self, detrenddata=False):
"""
Estimate the parameters that best model the data using it's moments
Parameters
----------
detrenddata : bool
a keyword that determines whether data should be detrended first.
Detrending takes *much* longer than not. Probably only useful for
large fields of view.
Returns
-------
params : array_like
params[0] = amp
params[1] = x0
params[2] = y0
params[3] = sigma_x
params[4] = sigma_y
params[5] = rho
params[6] = offset
Notes
-----
Bias is removed from data using detrend in the util module.
"""
# initialize the parameter array
params = np.zeros(7)
# iterate at most 10 times
for i in range(10):
# detrend data
if detrenddata:
# only try to remove a plane, any more should be done before
# passing object instatiation.
data, bg = detrend(self._data.copy(), degree=1)
offset = bg.mean()
amp = data.max()
else:
data = self._data.astype(float)
offset = data.min()
amp = data.max() - offset
# calculate the moments up to second order
M = moments(data, 2)
# calculate model parameters from the moments
# https://en.wikipedia.org/wiki/Image_moment# Central_moments
xbar = M[1, 0] / M[0, 0]
ybar = M[0, 1] / M[0, 0]
xvar = M[2, 0] / M[0, 0] - xbar**2
yvar = M[0, 2] / M[0, 0] - ybar**2
covar = M[1, 1] / M[0, 0] - xbar * ybar
# place the model parameters in the return array
params[:3] = amp, xbar, ybar
params[3] = np.sqrt(np.abs(xvar))
params[4] = np.sqrt(np.abs(yvar))
params[5] = covar / np.sqrt(np.abs(xvar * yvar))
params[6] = offset
if abs(params[5]) < 1 or not detrenddata:
# if the rho is valid or we're not detrending data,
# break the loop.
break
# save estimate for later use
self._guess_params = params
# return parameters to the caller as a `copy`, we don't want them to
# change the internal state
return params.copy()
def properties(self):
"""Return a set of metrics on the masks with units of distance """
imgH, imgW = self.image.shape # Image height, width
# Don't overemphasize one dimension over the other by setting the max
# dimenstion to equal 1
imgL = np.max([imgH, imgW])
imgA = imgH * imgW # Total number of pixels
if self._properties is None:
# Must load contour into single variable before checking self.hasmask
# If mask exists, only then can we access x,y components of contour
C = self.contour
if self.hasmask:
D = {}
D['hasmask'] = True
# Area metric is normalize to number of image pixels. Sqrt
# converts units to distance
D['maskarea'] = np.sqrt(np.count_nonzero(self.image)/imgA)
# Contour-derived values
x, y = C
D['contxmin'] = np.min(x)/imgL
D['contxmax'] = np.max(x)/imgL
D['contymin'] = np.min(y)/imgL
D['contymax'] = np.max(y)/imgL
D['contW'] = D['contxmax'] - D['contxmin']
D['contH'] = D['contymax'] - D['contymin']
# Image moments
m = measure.moments(self.image, order=5)
D['moments'] = m
D['centrow'] = (m[0, 1]/m[0, 0])/imgL
D['centcol'] = (m[1, 0]/m[0, 0])/imgL
# Hu, scale, location, rotation invariant (7, 1)
mHu = measure.moments_hu(m)
for i, Ii in enumerate(mHu):
D['moment_hu_I{}'.format(i)] = Ii
# Contour SVD is converted to two coordinates
# First normalize and centre the contours
D['contour'] = self.contour
contour = (self.contour.T/imgL - [D['centrow'], D['centcol']]).T
D['unitcontour'] = contour
_, s, v = np.linalg.svd(contour.T)
D['svd'] = s*v
D['svdx0'] = D['svd'][0,0]
D['svdx1'] = D['svd'][0,1]
D['svdy0'] = D['svd'][1,0]
D['svdy1'] = D['svd'][1,1]
# Width by medial axis
skel, distance = morphology.medial_axis(self.image,
self.image,
return_distance=True)
self.skel = skel
self.distance = distance
#
D['skelpixels'] = np.sqrt((np.sum(skel)/imgA)) # number of pixels
# distances should be restricted to within mask to avoid over-
# counting the zeros outside the mask
distances = distance[self.image>0]/imgL
q = [10, 25, 50, 75, 90]
keys = ['skeldist{:2d}'.format(n) for n in q]
vals = np.percentile(distances, q)
D.update(dict(zip(keys, vals)))
D['skelavgdist'] = np.mean(distances)
D['skelmaxdist'] = np.max(distances)
self._properties = D
return self._properties
def moments(self):
"""Spatial moments up to 3rd order of the source."""
from skimage.measure import moments
return moments(self._data_cutout_maskzeroed_double, 3)
def hu_feature(gray):
moments = measure.moments(gray)
hu = measure.moments_hu(moments)
return normalize(hu)
def moments(self, order=3):
'''see skimage.measure.moments'''
return measure.moments(self, order)
def get_centroid(image):
m = measure.moments(image)
return m[0, 1] / m[0, 0], m[1, 0] / m[0, 0]
def getHuMoments(image):
img = image.copy()
return measure.moments_hu(measure.moments(img))