本文整理汇总了Python中numpy.floor函数的典型用法代码示例。如果您正苦于以下问题:Python floor函数的具体用法?Python floor怎么用?Python floor使用的例子?那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。
在下文中一共展示了floor函数的20个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于我们的系统推荐出更棒的Python代码示例。
示例1: solve
def solve(self, pixel=None, solver='cvxopt.coneqp'):
'''
Solves minimization problem using quadratic program formulation.
'''
n, m = self.image.shape
if not pixel:
i, j = floor(n/2), floor(m/2)
else:
i, j = pixel
r, p, q = self.psf_tensor.shape
psf_bbox = (max(0, p/2-i), max(0, q/2-j),
min(p, p/2-i+n), min(q, q/2-j+m))
img_bbox = (max(0, i-n/2), max(0, j-q/2),
min(n, i+n/2), min(m, j+m/2))
self.A = self._compute_A(psf_bbox)
self.normalization_factor = self._compute_normalization(psf_bbox)
self.y = self._compute_y(img_bbox)
Q = self._compute_Q()
p = self._compute_p()
G = self._compute_G()
h = self._compute_h()
result = cvxopt.solvers.qp(Q, p, G, h)
self.result = result
self.x = result['x']
return result['status']
开发者ID:bwallin,项目名称:edfm,代码行数:28,代码来源:inversion.py
示例2: svd_example
def svd_example():
a = np.floor(np.random.rand(4, 4)*20-6)
logger.info("Matrix A:\n %s", a)
b = np.floor(np.random.rand(4, 1)*20-6)
logger.info("Matrix B:\n %s", b)
u, s, v_t = np.linalg.svd(a) # SVD decomposition of A
logger.info("Matrix U:\n %s", u)
logger.info("Matrix S:\n %s", s)
logger.info("Matrix V(transpose:\n %s", u)
logger.info("Computing inverse using linalg.pinv")
# Computing the inverse using pinv
inv_pinv = np.linalg.pinv(a)
logger.info("pinv:\n %s", inv_pinv)
# Computing inverse using matrix decomposition
logger.info("Computing inverse using svd matrix decomposition")
inv_svd = np.dot(np.dot(v_t.T, np.linalg.inv(np.diag(s))), u.T)
logger.info("svd inverse:\n %s", inv_svd)
logger.info("comparing the results from pinv and svd_inverse:\n %s",
np.allclose(inv_pinv, inv_svd))
logger.info("Sol1: Solving x using pinv matrix... x=A^-1 x b")
result_pinv_x = np.dot(inv_pinv, b)
logger.info("Sol2: Solving x using svd_inverse matrix... x=A^-1 x b")
result_svd_x = np.dot(inv_svd, b)
if not np.allclose(result_pinv_x, result_svd_x):
raise ValueError('Should have been True')
开发者ID:pramitchoudhary,项目名称:Concepts-Simplified,代码行数:31,代码来源:svd.py
示例3: __init__
def __init__(self, filepath, qually, mode='444'):
'''
'''
imOrig = cv2.imread(filepath,1)
self.filepath = filepath
self.mode = mode
#Taxa de compressão e Redundancia
self.CRate = 0; self.Redunc = 0
self.avgBits = 0
#Qualidade
self.qually = qually
#Dimensões da imagem original
self.Mo, self.No, self.Do = imOrig.shape
self.r, self.c = [8, 8] #DIMENSAO DOS BLOCOS
#TRATA AS DIMENSOES DA IMAGEM
(self.M, self.N, self.D), self.img = h.adjImg(imOrig)
#NUMERO DE BLOCOS NA VERTICAL E HORIZONTAL
self.nBlkRows = int(np.floor(self.M/self.r))
self.nBlkCols = int(np.floor(self.N/self.c))
#Gera Tabela de Qunatizaçao
self.Z = h.genQntb(self.qually)
#TRANSFORMA DE RGB PARA YCbCr
self.Ymg = cv2.cvtColor(self.img, cv2.COLOR_BGR2YCR_CB)
self.NumBits = 0
if self.Do == 2:
self.NCHNL = 1
elif self.Do == 3:
self.NCHNL = 3
# self.OUTCOMES = self._run_()
self._run_()
开发者ID:LuanAGoncalves,项目名称:mpeg2_luan,代码行数:31,代码来源:entropyCoding.py
示例4: connect_composition_III
def connect_composition_III(self):
synapse_list = []
Mt3v_list = self.non_columnar_neurons['Mt3v']
Mt3h_list = self.non_columnar_neurons['Mt3h']
for neuron in Mt3v_list:
neuron.assign_pos(0., 0.)
for neuron in Mt3h_list:
neuron.assign_pos(0., 0.)
rule3synapsesv = self.other_synapse_dict[self.other_synapse_dict['postname'] == 'Mt3v']
rule3synapsesh = self.other_synapse_dict[self.other_synapse_dict['postname'] == 'Mt3h']
dtnames = rule3synapsesv.dtype.names
for cartridge in self.cartridges:
synapse = Synapse(dict(zip(dtnames, [np.asscalar(p) for p in rule3synapsesv[0]])))
mtn = int(np.floor(cartridge.neurons['L2'].ypos / ((self.hexarray.Y[-1][-1]+1)/4)))
synapse.link(cartridge.neurons['L2'], Mt3v_list[mtn])
synapse_list.append(synapse)
synapse = Synapse(dict(zip(dtnames, [np.asscalar(p) for p in rule3synapsesh[0]])))
mtn = int(np.floor(cartridge.neurons['L2'].xpos / ((self.hexarray.X[-1][-1]+1)/4)))
synapse.link(cartridge.neurons['L2'], Mt3h_list[mtn])
synapse_list.append(synapse)
self.composition_rules.append({'synapses': synapse_list})
开发者ID:neurokernel,项目名称:sensory_int,代码行数:25,代码来源:vision_configuration.py
示例5: _find_tails
def _find_tails(self, mag, rounding=True, half=5, full=10, flag=50):
'''
Find how many of each of the tail pieces is necessary. Flag
specifies the increment for a flag, barb for a full barb, and half for
half a barb. Mag should be the magnitude of a vector (ie. >= 0).
This returns a tuple of:
(*number of flags*, *number of barbs*, *half_flag*, *empty_flag*)
*half_flag* is a boolean whether half of a barb is needed,
since there should only ever be one half on a given
barb. *empty_flag* flag is an array of flags to easily tell if
a barb is empty (too low to plot any barbs/flags.
'''
#If rounding, round to the nearest multiple of half, the smallest
#increment
if rounding:
mag = half * (mag / half + 0.5).astype(np.int)
num_flags = np.floor(mag / flag).astype(np.int)
mag = np.mod(mag, flag)
num_barb = np.floor(mag / full).astype(np.int)
mag = np.mod(mag, full)
half_flag = mag >= half
empty_flag = ~(half_flag | (num_flags > 0) | (num_barb > 0))
return num_flags, num_barb, half_flag, empty_flag
开发者ID:AmitAronovitch,项目名称:matplotlib,代码行数:31,代码来源:quiver.py
示例6: interp
def interp(pic,flow):
ys=np.arange(pic.shape[0]*pic.shape[1])/pic.shape[1]
ud=(flow[:,:,0].reshape(-1)+ys)%pic.shape[0]
xs=np.arange(pic.shape[0]*pic.shape[1])%pic.shape[1]
lr=(flow[:,:,1].reshape(-1)+xs)%pic.shape[1]
u=np.int32(np.floor(ud))
d=np.int32(np.ceil(ud))%pic.shape[0]
udiffs=ud-u
udiffs=np.dstack((udiffs,udiffs,udiffs))
l=np.int32(np.floor(lr))
r=np.int32(np.ceil(lr))%pic.shape[1]
ldiffs=lr-l
ldiffs=np.dstack((ldiffs,ldiffs,ldiffs))
ul=pic[u,l,:]
ur=pic[u,r,:]
dl=pic[d,l,:]
dr=pic[d,r,:]
udl=ul*(1-udiffs)+dl*udiffs
udr=ur*(1-udiffs)+dr*udiffs
ans=np.zeros(pic.shape)
ans[ys,xs,:]=udl*(1-ldiffs)+udr*ldiffs
return ans
开发者ID:solomongarber,项目名称:texture_sampler,代码行数:26,代码来源:controller.py
示例7: getRowCol
def getRowCol(self,lat,lon,returnFloat=False):
"""Return data row and column from given geographic coordinates (lat/lon decimal degrees).
:param lat:
Input latitude.
:param lon:
Input longitude.
:param returnFloat:
Boolean indicating whether floating point row/col coordinates should be returned.
:returns:
Tuple of row and column.
"""
ulx = self._geodict['xmin']
uly = self._geodict['ymax']
xdim = self._geodict['xdim']
ydim = self._geodict['ydim']
#check to see if we're in a scenario where the grid crosses the meridian
if self._geodict['xmax'] < ulx and lon < ulx:
lon += 360
col = (lon-ulx)/xdim
row = (uly-lat)/ydim
if returnFloat:
return (row,col)
return (np.floor(row).astype(int),np.floor(col).astype(int))
开发者ID:mhearne-usgs,项目名称:grid,代码行数:25,代码来源:grid2d.py
示例8: solver_dt
def solver_dt(t0, y0, f, dt, tk, method='expl_RK4', tuning='', v=0, outform='arr'):
step=methods[method]
#we calculate number of steps
if np.abs(t0-tk/dt)-np.floor(np.abs(t0-tk/dt)) >= 0.5:
nos = int(np.ceil(np.abs(t0-tk)/dt))
else:
nos = int(np.floor(np.abs(t0-tk)/dt))
if v==2: print "Number of steps I`ll take is "+str(nos)
#in solver_nos above code will be changed!
soln = [[t0, y0]]
for i in range(nos-1):
tmp1, tmp2 = step(f, soln[i][1], soln[i][0], dt, tuning=tuning)
soln.append([tmp1, tmp2])
if v>=1: print "solved. Took "+str(nos)+" steps to solve on interval ["+str(t0)+";"+str(tk)+"]"
if v==2: print "solve method was "+method+". Additional tweaks for this solver were:"+tuning
if v==2: print "output form was "+outform+"(arr- numpy array such that arr[i] = [t, y1, ..., yn], list - nested list list[i]=[t, array(y)])"
if outform=='arr':
return np.array([[i[0]]+ ([a for a in i[1]] if type(i[1])==np.ndarray else [i[1]]) for i in soln])
elif outform=='list':
return soln
开发者ID:picalke,项目名称:NumerkiII,代码行数:28,代码来源:numerical1.py
示例9: get_border_to_nucleus_properties
def get_border_to_nucleus_properties(segment):
pts = np.array(segment. isotropic_border_coords)
res = min([segment.xres, segment.yres, segment.zres])
centroid = np.floor(np.mean(pts,0))
centroid_with_offset = np.floor(np.mean(segment.border_coords,0) + np.array([segment.bounding_box.xmin, segment.bounding_box.ymin, segment.bounding_box.zmin]))
centroid_by_res = centroid_with_offset * np.array([segment.xres, segment.yres, segment.zres])
# if centroid_with_offset[2] == 26:
# pdb.set_trace()
dists = ((pts[:,0] - centroid[0])**2 + (pts[:,1] - centroid[1])**2 + (pts[:,2] - centroid[2])**2 ) **0.5
max_dist = dists.max()
dists = dists/max_dist
bins = np.arange(0, 1.05, 0.05)
dist_hist = histogram(dists, bins = bins) [0]
segment.add_feature("centroid_res", tuple(centroid_by_res))
segment.add_feature("border_to_nucleus_dist_hist", dist_hist)
segment.add_feature("border_to_nucleus_dist_mean", np.mean(dists))
segment.add_feature("border_to_nucleus_dist_std", np.std(dists))
segment.add_feature("distance_to_border_scale_factor", max_dist)
pts = np.array(segment.border_coords)
segment.add_feature("centroid", tuple(centroid_with_offset.astype("int")))
开发者ID:ddiana,项目名称:CellECT,代码行数:31,代码来源:segment_features.py
示例10: calc_slit_box_aps_1id
def calc_slit_box_aps_1id(slit_box_corners, inclip=(1, 10, 1, 10)):
"""
Calculate the clip box based on given slip corners.
Parameters
----------
slit_box_corners : np.ndarray
Four corners of the slit box as a 4x2 matrix
inclip : tuple, optional
Extra inclipping to avoid clipping artifacts
Returns
-------
Tuple:
Cliping indices as a tuple of four
(clipFromTop, clipToBottom, clipFromLeft, clipToRight)
"""
return (
np.floor(slit_box_corners[:, 0].min()).astype(
int) + inclip[0], # clip top row
np.ceil(slit_box_corners[:, 0].max()).astype(
int) - inclip[1], # clip bottom row
np.floor(slit_box_corners[:, 1].min()).astype(
int) + inclip[2], # clip left col
np.ceil(slit_box_corners[:, 1].max()).astype(
int) - inclip[3], # clip right col
)
开发者ID:tekinbicer,项目名称:tomopy,代码行数:28,代码来源:alignment.py
示例11: build_X
def build_X(bids, bot_or_human):
X = bot_or_human
X = X.drop("payment_account", 1)
X = X.drop("address", 1)
bids["day"] = np.floor((bids["time"] - startt) / one_day)
bids["week"] = np.floor(bids["day"] / 7.0)
# print bids.bidder_id[0]
print "starting ips"
X = ip(X, bids)
print "starting bid order"
X = bid_order(X, bids)
print "starting dt"
X = dt(X, bids)
print "startin day"
X = day(X, bids)
print "starting n_bids"
X = n_bids(X, bids)
print "starting urls"
X = urls(X, bids)
# print 'starting bid order'
# X = bid_order(X, bids)
print "starting countries"
X = user_countries_per_auction(X, bids)
print "starting merch"
X = merch(X, bids)
return X
开发者ID:advnturecaptlst,项目名称:kaggle_archive,代码行数:29,代码来源:facebook_auction.py
示例12: check_orbits
def check_orbits(p1, t1, p2, t2, tmn, tmx, tol):
n1 = t1 + p1 * np.arange(np.floor((tmn-t1)/p1), np.ceil((tmx-t1)/p1))
n1 = n1[(tmn <= n1) * (n1 <= tmx)]
n2 = t2 + p2 * np.arange(np.floor((tmn-t2)/p2), np.ceil((tmx-t2)/p2))
n2 = n2[(tmn <= n2) * (n2 <= tmx)]
delta = np.fabs(n1[:, None] - n2[None, :])
return max(len(n1), len(n2)) == np.sum(delta < tol)
开发者ID:dfm,项目名称:ketu,代码行数:7,代码来源:feature_extract.py
示例13: multilook_attributes
def multilook_attributes(atr_dict,lks_az,lks_rg):
#####
atr = dict()
for key, value in atr_dict.iteritems(): atr[key] = str(value)
##### calculate new data size
length = int(atr['FILE_LENGTH'])
width = int(atr['WIDTH'])
length_mli = int(np.floor(length/lks_az))
width_mli = int(np.floor(width/lks_rg))
##### Update attributes
atr['FILE_LENGTH'] = str(length_mli)
atr['WIDTH'] = str(width_mli)
try:
atr['Y_STEP'] = str(lks_az*float(atr['Y_STEP']))
atr['X_STEP'] = str(lks_rg*float(atr['X_STEP']))
except: pass
try:
atr['AZIMUTH_PIXEL_SIZE'] = str(lks_az*float(atr['AZIMUTH_PIXEL_SIZE']))
atr['RANGE_PIXEL_SIZE'] = str(lks_rg*float(atr['RANGE_PIXEL_SIZE']))
except: pass
try:
atr['ref_y'] = str(int(int(atr['ref_y'])/lks_az))
atr['ref_x'] = str(int(int(atr['ref_x'])/lks_rg))
except: pass
try:
atr['subset_y0'] = str(int(int(atr['subset_y0'])/lks_az))
atr['subset_y1'] = str(int(int(atr['subset_y1'])/lks_az))
atr['subset_x0'] = str(int(int(atr['subset_x0'])/lks_rg))
atr['subset_x1'] = str(int(int(atr['subset_x1'])/lks_rg))
except: pass
return atr
开发者ID:yunjunz,项目名称:PySAR,代码行数:35,代码来源:multi_looking.py
示例14: __init__
def __init__(self, hipparcos, symbad, intervals):
self.hipparcos = hipparcos
self.symbad = symbad
self.ra_min = min(hipparcos['RA_J2000'])
self.ra_max = max(hipparcos['RA_J2000'])
self.de_min = min(hipparcos['DE_J2000'])
self.de_max = max(hipparcos['DE_J2000'])
self.intervals = intervals
self.ra_dif = self.ra_max - self.ra_min
self.de_dif = self.de_max - self.de_min
self.ra_sp = self.ra_dif/(self.intervals-1)
self.de_sp = self.de_dif/(self.intervals-1)
# set the position at the space grid for hipparcos catalog
self.stars = pandas.DataFrame(
numpy.zeros((len(self.hipparcos),2)), columns=['rec','dec'])
self.stars['rec'] = numpy.floor(
(self.hipparcos['RA_J2000'] - self.ra_min) / self.ra_sp) + 1
self.stars['dec'] = numpy.floor(
(self.hipparcos['DE_J2000'] - self.de_min) / self.de_sp) + 1
# set the position at the space grid for symbad catalog
self.symbad['rac'] = numpy.floor(
(self.symbad['RA_J2000'] - self.ra_min) / self.ra_sp) + 1
self.symbad['dec'] = numpy.floor(
(self.symbad['DE_J2000'] - self.de_min) / self.de_sp) + 1
开发者ID:nemiliani,项目名称:DMCyT,代码行数:26,代码来源:match_stars.py
示例15: _get_interv_graticule
def _get_interv_graticule(self,pmin,pmax,dpar,mmin,mmax,dmer,verbose=True):
def set_prec(d,n,nn=2):
arcmin=False
if d/n < 1.:
d *= 60
arcmin = True
nn = 1
x = d/n
y = nn*x
ex = np.floor(np.log10(y))
z = np.around(y/10**ex)*10**ex/nn
if arcmin:
z = 1./np.around(60./z)
return z
max_n_par = 18
max_n_mer = 36
n_par = (pmax-pmin)/dpar
n_mer = (mmax-mmin)/dmer
if n_par > max_n_par:
dpar = set_prec((pmax-pmin)/dtor,max_n_par/2)*dtor
if n_mer > max_n_mer:
dmer = set_prec((mmax-mmin)/dtor,max_n_mer/2,nn=1)*dtor
if dmer/dpar < 0.2 or dmer/dpar > 5.:
dmer = dpar = max(dmer,dpar)
vdeg = np.floor(np.around(dpar/dtor,10))
varcmin = (dpar/dtor-vdeg)*60.
if verbose: print "The interval between parallels is %d deg %.2f'."%(vdeg,varcmin)
vdeg = np.floor(np.around(dmer/dtor,10))
varcmin = (dmer/dtor-vdeg)*60.
if verbose: print "The interval between meridians is %d deg %.2f'."%(vdeg,varcmin)
return dpar,dmer
开发者ID:montefra,项目名称:healpy,代码行数:31,代码来源:projaxes.py
示例16: plot_scatter_with_histograms
def plot_scatter_with_histograms(xvals, yvals, colour='k', oneToOneLine=True, xlabel=None, ylabel=None, title=None):
gs = gridspec.GridSpec(5, 5)
xmin = np.floor(min(xvals))
xmax = np.ceil(max(xvals))
ymin = np.floor(min(yvals))
ymax = np.ceil(max(yvals))
plt.subplot(gs[1:, 0:4])
plt.plot(xvals, yvals, 'o', color=colour)
if xlabel is not None:
plt.xlabel(xlabel)
if ylabel is not None:
plt.ylabel(ylabel)
if oneToOneLine:
oneToOneMax = max([max(xvals),max(yvals)])
plt.plot([0,oneToOneMax],[0,oneToOneMax],'b--')
plt.xlim(xmin,xmax)
plt.ylim(ymin,ymax)
plt.subplot(gs[0, 0:4])
plt.hist(xvals, np.linspace(xmin,xmax,50))
plt.axis('off')
plt.subplot(gs[1:,4])
plt.hist(yvals, np.linspace(ymin,ymax,50), orientation='horizontal')
plt.axis('off')
if title is not None:
plt.suptitle(title)
开发者ID:sjara,项目名称:jaratest,代码行数:25,代码来源:compute_cell_stats.py
示例17: qwtCanvasClip
def qwtCanvasClip(canvas, canvasRect):
x1 = np.ceil(canvasRect.left())
x2 = np.floor(canvasRect.right())
y1 = np.ceil(canvasRect.top())
y2 = np.floor(canvasRect.bottom())
r = QRect(x1, y1, x2-x1-1, y2-y1-1)
return canvas.borderPath(r)
开发者ID:petebachant,项目名称:python-qwt,代码行数:7,代码来源:plot_renderer.py
示例18: PlotErrBoxPlot
def PlotErrBoxPlot(x, y, delta, ax, showXTicks):
if x.size < 1:
return
ids = np.floor((x)/delta).astype(np.int)
data = []
for i in range(ids.min(), ids.max()+1):
if (ids==i).any():
data.append(y[ids==i])
bp = plt.boxplot(data)
# plt.plot(x,y,'.', color=c1, alpha=0.3)
# set xticks
if showXTicks:
ticks = np.floor((np.arange(ids.min(), ids.max()+1)+0.5)*delta).astype(np.int)
if np.unique(ticks).size < ticks.size:
ticks = np.floor((np.arange(ids.min(), ids.max()+1)+0.5)*delta*10.)/10.
xtickNames = plt.setp(ax, xticklabels=ticks)
plt.setp(xtickNames, rotation=45)
else:
plt.setp(ax.get_xticklabels(), visible=False)
for box in bp["boxes"]:
box.set(color=c1)
#box.set(facecolor=c1)
for whisker in bp["whiskers"]:
whisker.set(color=c1)
for cap in bp["caps"]:
cap.set(color=c1)
for median in bp["medians"]:
median.set(color=c2)
for flier in bp["fliers"]:
flier.set(color=c3, marker=".", alpha=0.15) #,s=6)
开发者ID:tunino91,项目名称:dpOptTrans,代码行数:30,代码来源:plotResults.py
示例19: _search_fine
def _search_fine(sino, srad, step, init_cen, ratio, drop):
"""
Fine search for finding the rotation center.
"""
Nrow, Ncol = sino.shape
centerfliplr = (Ncol + 1.0) / 2.0 - 1.0
# Use to shift the sinogram 2 to the raw CoR.
shiftsino = np.int16(2 * (init_cen - centerfliplr))
_copy_sino = np.roll(np.fliplr(sino[1:]), shiftsino, axis=1)
lefttake = 0
righttake = Ncol - 1
if init_cen <= centerfliplr:
lefttake = np.ceil(srad + 1)
righttake = np.floor(2 * init_cen - srad - 1)
else:
lefttake = np.ceil(
init_cen - (Ncol - 1 - init_cen) + srad + 1)
righttake = np.floor(Ncol - 1 - srad - 1)
Ncol1 = righttake - lefttake + 1
mask = _create_mask(2 * Nrow - 1, Ncol1, 0.5 * ratio * Ncol, drop)
numshift = np.int16((2 * srad + 1.0) / step)
listshift = np.linspace(-srad, srad, num=numshift)
listmetric = np.zeros(len(listshift), dtype='float32')
num1 = 0
for i in listshift:
_sino = ndimage.interpolation.shift(
_copy_sino, (0, i), prefilter=False)
sinojoin = np.vstack((sino, _sino))
listmetric[num1] = np.sum(np.abs(np.fft.fftshift(
pyfftw.interfaces.numpy_fft.fft2(
sinojoin[:, lefttake:righttake + 1]))) * mask)
num1 = num1 + 1
minpos = np.argmin(listmetric)
return init_cen + listshift[minpos] / 2.0
开发者ID:JStuckner,项目名称:tomopy,代码行数:35,代码来源:rotation.py
示例20: errorScalingFactor
def errorScalingFactor(observable, beta):
"""
Look up the numerical factors to apply to the sky averaged parallax error in order to obtain error
values for a given astrometric parameter, taking the Ecliptic latitude and the number of transits into
account.
Parameters
----------
observable - Name of astrometric observable (one of: alphaStar, delta, parallax, muAlphaStar, muDelta)
beta - Values(s) of the Ecliptic latitude.
Returns
-------
Numerical factors to apply to the errors of the given observable.
"""
if isscalar(beta):
index=int(floor(abs(sin(beta))*_numStepsSinBeta))
if index == _numStepsSinBeta:
return _astrometricErrorFactors[observable][_numStepsSinBeta-1]
else:
return _astrometricErrorFactors[observable][index]
else:
indices = array(floor(abs(sin(beta))*_numStepsSinBeta), dtype=int)
indices[(indices==_numStepsSinBeta)] = _numStepsSinBeta-1
return _astrometricErrorFactors[observable][indices]
开发者ID:agabrown,项目名称:PyGaia,代码行数:27,代码来源:astrometric.py
注:本文中的numpy.floor函数示例由纯净天空整理自Github/MSDocs等源码及文档管理平台,相关代码片段筛选自各路编程大神贡献的开源项目,源码版权归原作者所有,传播和使用请参考对应项目的License;未经允许,请勿转载。 |
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