def calculate_normalised_xsection(inputs,
bin_widths,
normalise_to_one=False,
covariance_matrix=None,
inputMC_covariance_matrix=None):
"""
Calculates normalised average x-section for each bin: 1/N *1/bin_width sigma_i
There are two ways to calculate this
1) N = sum(sigma_i)
2) N = sum(sigma_i/bin_width)
The latter one will normalise the total distribution to 1
@param inputs: list of value-error pairs
@param bin_widths: bin widths of the inputs
"""
values = [u.ufloat(i[0], i[1]) for i in inputs]
norm_cov_matrix = None
norm_corr_matrix = None
inputMC_norm_cov_matrix = None
if not covariance_matrix is None and not normalise_to_one:
values_correlated = u.correlated_values(
[v.nominal_value for v in values], covariance_matrix.tolist())
norm = sum(values_correlated)
norm_values_correlated = []
# Loop over unfolded number of events with correlated uncertainties
# And corresponding bin width
# Calculate normalised cross section, with correctly correlated uncertainty
for v, width in zip(values_correlated, bin_widths):
norm_values_correlated.append(v / width / norm)
# Get covariance and correlation matrix for normalised cross section
norm_cov_matrix = matrix(u.covariance_matrix(norm_values_correlated))
norm_corr_matrix = matrix(u.correlation_matrix(norm_values_correlated))
result = [(v.nominal_value, v.std_dev) for v in norm_values_correlated]
# Get Covariance Matrix for input MC
if not inputMC_covariance_matrix is None:
inputMC_values_correlated = u.correlated_values(
[v.nominal_value for v in values],
inputMC_covariance_matrix.tolist())
inputMC_norm = sum(inputMC_values_correlated)
inputMC_norm_values_correlated = []
for v, width in zip(inputMC_values_correlated, bin_widths):
inputMC_norm_values_correlated.append(v / width / inputMC_norm)
inputMC_norm_cov_matrix = matrix(
u.covariance_matrix(inputMC_norm_values_correlated))
else:
normalisation = 0
if normalise_to_one:
normalisation = sum([
value / bin_width
for value, bin_width in zip(values, bin_widths)
])
else:
normalisation = sum(values)
xsections = [(1 / bin_width) * value / normalisation
for value, bin_width in zip(values, bin_widths)]
result = [(xsection.nominal_value, xsection.std_dev)
for xsection in xsections]
return result, norm_cov_matrix, norm_corr_matrix, inputMC_norm_cov_matrix
def test_correlated_values():
"Correlated variables."
u = uncertainties.ufloat((1, 0.1))
cov = uncertainties.covariance_matrix([u])
# "1" is used instead of u.nominal_value because
# u.nominal_value might return a float. The idea is to force
# the new variable u2 to be defined through an integer nominal
# value:
u2, = uncertainties.correlated_values([1], cov)
expr = 2 * u2 # Calculations with u2 should be possible, like with u
####################
# Covariances between output and input variables:
x = ufloat((1, 0.1))
y = ufloat((2, 0.3))
z = -3 * x + y
covs = uncertainties.covariance_matrix([x, y, z])
# "Inversion" of the covariance matrix: creation of new
# variables:
(x_new, y_new, z_new) = uncertainties.correlated_values(
[x.nominal_value, y.nominal_value, z.nominal_value], covs, tags=["x", "y", "z"]
)
# Even the uncertainties should be correctly reconstructed:
assert matrices_close(numpy.array((x, y, z)), numpy.array((x_new, y_new, z_new)))
# ... and the covariances too:
assert matrices_close(numpy.array(covs), numpy.array(uncertainties.covariance_matrix([x_new, y_new, z_new])))
assert matrices_close(numpy.array([z_new]), numpy.array([-3 * x_new + y_new]))
####################
# ... as well as functional relations:
u = ufloat((1, 0.05))
v = ufloat((10, 0.1))
sum_value = u + 2 * v
# Covariance matrices:
cov_matrix = uncertainties.covariance_matrix([u, v, sum_value])
# Correlated variables can be constructed from a covariance matrix, if
# NumPy is available:
(u2, v2, sum2) = uncertainties.correlated_values([x.nominal_value for x in [u, v, sum_value]], cov_matrix)
# matrices_close() is used instead of _numbers_close() because
# it compares uncertainties too:
assert matrices_close(numpy.array([0]), numpy.array([sum2 - (u2 + 2 * v2)]))
def calculate_xsection(inputs,
bin_widths,
luminosity,
efficiency=1.,
covariance_matrix=None,
inputMC_covariance_matrix=None):
'''
BUG: this doesn't work unless the inputs are unfolded!
inputs = list of value-error pairs
luminosity = integrated luminosity of the measurement
'''
abs_cov_matrix = None
abs_corr_matrix = None
inputMC_abs_cov_matrix = None
result = []
add_result = result.append
values = [u.ufloat(i[0], i[1]) for i in inputs]
if not covariance_matrix is None:
values_correlated = u.correlated_values(
[v.nominal_value for v in values], covariance_matrix.tolist())
abs_values_correlated = []
# Loop over unfolded number of events with correlated uncertainties
# And corresponding bin width
# Calculate absolute cross section, with correctly correlated uncertainty
for v, width in zip(values_correlated, bin_widths):
abs_values_correlated.append(v / width / luminosity / efficiency)
# Get covariance and correlation matrix for absolute cross section
abs_cov_matrix = matrix(u.covariance_matrix(abs_values_correlated))
abs_corr_matrix = matrix(u.correlation_matrix(abs_values_correlated))
result = [(v.nominal_value, v.std_dev) for v in abs_values_correlated]
# Get Covariance Matrix for input MC
if not inputMC_covariance_matrix is None:
inputMC_values_correlated = u.correlated_values(
[v.nominal_value for v in values],
inputMC_covariance_matrix.tolist())
inputMC_abs_values_correlated = []
for v, width in zip(inputMC_values_correlated, bin_widths):
inputMC_abs_values_correlated.append(v / width / luminosity /
efficiency)
inputMC_abs_cov_matrix = matrix(
u.covariance_matrix(inputMC_abs_values_correlated))
else:
for valueAndErrors, binWidth in zip(inputs, bin_widths):
value = valueAndErrors[0]
error = valueAndErrors[1]
xsection = value / (luminosity * efficiency * binWidth)
xsection_error = error / (luminosity * efficiency * binWidth)
add_result((xsection, xsection_error))
return result, abs_cov_matrix, abs_corr_matrix, inputMC_abs_cov_matrix
def linear_regression_u(x, y, uncert_x=None, uncert_y=None):
"""
Linear regression with uncertainties in both directions, returning
UncertainVariables from the uncertainties package.
Parameters
----------
x : array_like
x-values
y : array_like
y-values
uncert_x : array_like or None
uncertainty of x-values
uncert_y : array_like
uncertainty of y-values
Takes two arrays for x-values and y-values and optional two arrays of
uncertainties. The uncertainty arguments are default to None, which is
treated as a zero uncertainty in every value.
Fits a function y=m*x+c to the values and returns the results for m and c
as UncertainVariables from the package uncertainties (considering their
correlation), and the chisquared of the fit. It returns a tuple containing:
m, c, chisquared
If both uncertainties are unequal zero, the calculation can not be
performed analytically and the package scipy.odr is used.
"""
m,sigma_m,c,sigma_c,corr,chisq = linear_regression(x,y,uncert_x, uncert_y)
cov = sigma_m * sigma_c * corr
cov_mat = [[sigma_m**2, cov],[cov, sigma_c**2]]
m2, c2 = uncertainties.correlated_values([m, c], cov_mat)
return m2, c2, chisq
def set_parameters(self, pars, cov):
"""
Sets patameters and their covariance matrix
Args:
pars: dictionary
cov: np.cov
"""
if len(pars) < len(self.param_names):
raise ValueError("Provide all parameters!")
if len(cov) < len(self.param_names) or len(cov[0]) < len(
self.param_names):
raise ValueError("Wrong dimensions of covariance matrix")
self.params_C = cov
self.params = {}
for par_name in self.param_names:
self.params[par_name] = pars[par_name]
# set uparams once for all
if self.param_names is None or self.params is None or self.params_C is None:
return None
par_values = uncertainties.correlated_values(
[self.params[par_name] for par_name in self.param_names],
self.params_C)
self.uparams = {}
for i in range(len(self.param_names)):
self.uparams[self.param_names[i]] = par_values[i]
def auswerten(name, d, n, t, z, V_mol, eps, raw):
d *= 1e-3
N = unp.uarray(n/t, np.sqrt(n)/t) - N_u
if name=="Cu":
tools.table((raw[0], raw[1], N), ("D/mm", "n", "(N-N_U)/\per\second"), "build/{}.tex".format(name), "Messdaten von {}.".format(name), "tab:daten{}".format(name), split=2, footer=r"$\Delta t = \SI{60}{s}$")#"(N-N_U)/\per\second"
else:
tools.table((raw[0], raw[1], raw[2], N), ("D/mm", "n", "\Delta t/s", "(N-N_U)/\per\second"), "build/{}.tex".format(name), "Messdaten von {}.".format(name), "tab:daten{}".format(name), split=2)
mu = z * const.N_A / V_mol * 2 * np.pi * (const.e**2 / (4 * np.pi * const.epsilon_0 * const.m_e * const.c**2))**2 * ((1+eps)/eps**2 * ((2 * (1+eps))/(1+2*eps) - 1/eps * np.log(1+2*eps)) + 1/(2*eps) * np.log(1+ 2*eps) - (1+ 3*eps)/(1+2*eps)**2)
params, pcov = curve_fit(fit, d, unp.nominal_values(N), sigma=unp.std_devs(N))
params_ = unc.correlated_values(params, pcov)
print("{}: N(0) = {}, µ = {}, µ_com = {}".format(name, params_[0], -params_[1], mu))
sd = np.linspace(0, .07, 1000)
valuesp = (fit(sd, *(unp.nominal_values(params_) + 10*unp.std_devs(params_)))).astype(float)
valuesm = (fit(sd, *(unp.nominal_values(params_) - 10*unp.std_devs(params_)))).astype(float)
#plt.xlim(0,7)
plt.xlabel(r"$D/\si{mm}$")
plt.ylabel(r"$(N-N_U)/\si{\per\second}$")
plt.plot(1e3*sd, fit(sd, *params), 'b-', label="Fit")
plt.fill_between(1e3*sd, valuesm, valuesp, facecolor='blue', alpha=0.125, edgecolor='none', label=r'$1\sigma$-Umgebung ($\times 10$)')
plt.errorbar(1e3*d, unp.nominal_values(N), yerr=unp.std_devs(N), fmt='rx', label="Messdaten")
plt.legend(loc='best')
plt.yscale('linear')
plt.tight_layout(pad=0)
plt.savefig("build/{}.pdf".format(name))
plt.yscale('log')
plt.savefig("build/{}_log.pdf".format(name))
plt.clf()
def FitModel(self, model, x, y):
# Fitting the Model to the Data
popt, pcov = curve_fit(model, x, y)
params = popt
errors = np.sqrt(np.diag(pcov))
ymodel = model(x, *params)
DoF = len(x) - len(params)
chiSq = round(
self.ChiSq(y, ymodel),
1 - int(math.floor(math.log10(abs(self.ChiSq(y, ymodel))))) - 1)
rChiSq = round(chiSq / DoF,
1 - int(math.floor(math.log10(abs(chiSq / DoF)))) - 1)
a, b = unc.correlated_values(popt, pcov)
xp = np.linspace(min(x), max(x), 1000)
yp = a * xp + b
nom = unp.nominal_values(yp)
std = unp.std_devs(yp)
# Calculating CI
lpb, upb = self.predband(xp, x, y, params, model, conf=0.95)
print(
'ChiSquared: {} \n Reduced ChiSquare: {} \n Fitted Parameters: {}, {} \n Parameter Errors: {}, {}'
.format(chiSq, rChiSq, *np.round(params, 2), *np.round(errors, 2)))
print('---------------------------------')
confidence95 = [xp, nom - 1.96 * std, nom + 1.96 * std]
confidenceInterval = [xp, lpb, upb]
fit = [xp, ymodel, params]
return fit, confidence95, confidenceInterval
def plot_lightyield_vs_dose(d, title=''):
print(" Calculating D for " + title)
plt.figure()
y = d['Bi207AveragePE']
yerr = 0.7 # for some reason if I use 0.05*y, the plt.errorbar crashes with the contains N2 condition above...?
x = d['Dose (Mrad)']
names = d['TileName']
print(d[[
'TileName', 'SampleRun', 'Dose (Mrad)', 'Comment', 'DoseRate (rad/h)',
'Bi207AveragePE'
]])
#plt.plot(x, y, linewidth=2.0, linestyle='-', color='black', marker='o', markerfacecolor='r', markersize=5.2)
plt.errorbar(x,
y,
yerr=yerr,
linestyle='None',
ecolor='k',
marker='o',
markerfacecolor='black',
markersize=5.2,
label='Tile')
for i in range(0, len(names)):
plt.text(x.values[i],
y.values[i],
names.values[i],
fontsize=12,
color='g')
fitres = optimize.curve_fit(func_nexp,
x,
y,
sigma=yerr,
full_output=True,
absolute_sigma=True)
popt = fitres[0]
pcov = fitres[1]
# Need to use correlated errors to draw sigma bands
a, b = unc.correlated_values(popt, pcov)
print('Fit results: \na = {0:.3f} \nb = {1:.3f}'.format(a, b))
redchisq = (fitres[2]['fvec']**
2).sum() / (len(fitres[2]['fvec']) - len(popt))
print("chi2/Ndof = %6.3f" % redchisq)
#print len(fitres[2]['fvec'])
finex = np.arange(min(x), max(x), 0.2)
plt.plot(
finex,
func_nexp(finex, *popt),
'b-',
linewidth=2,
label=r'Fit: $y={0:.2f}e^{{-x/{1:.2f}}}$'.format(*popt)) # fit line
plt.legend(loc='upper right', frameon=False, framealpha=1, numpoints=1)
plt.xscale('log') # make it log scale!
plt.xlim([5.e-2, 20.])
plt.title(title)
plt.ylabel(r"Bi207 Source [# PE]")
plt.xlabel(r"Dose d [Mrad]")
plt.grid()
plt.savefig("SourcePELightYield_vs_Dose" + title + ".png")
return a, b
def get_covariance_matrix(self):
'''
Get the covariance matrix from all contributions
https://root.cern.ch/doc/master/classTUnfoldDensity.html#a7f9335973b3c520e2a4311d2dd6f5579
'''
import uncertainties as u
from numpy import array, matrix, zeros
from numpy import sqrt as np_sqrt
if self.unfolded_data is not None:
# Calculate the covariance from TUnfold
covariance = asrootpy(
self.unfoldObject.GetEmatrixInput('Covariance'))
# Reformat into a numpy matrix
zs = list(covariance.z())
cov_matrix = matrix(zs)
# Just the unfolded number of events
inputs = hist_to_value_error_tuplelist(self.unfolded_data)
nominal_values = [i[0] for i in inputs]
# # Unfolded number of events in each bin
# # With correlation between uncertainties
values_correlated = u.correlated_values( nominal_values, cov_matrix.tolist() )
corr_matrix = matrix(u.correlation_matrix(values_correlated) )
return cov_matrix, corr_matrix
else:
print("Data has not been unfolded. Cannot return unfolding covariance matrix")
return
def model_with_uncertainties(self):
"""Best fit model with uncertainties
The parameters on the model will be in units ``keV``, ``cm``, and
``s``. Thus, when evaluating the model energies have to be passed in
keV and the resulting flux will be in ``cm-2 s-1 keV-1``. The
covariance matrix passed on initialization must also have these units.
TODO: This is due to sherpa units, make more flexible
TODO: Add to gammapy.spectrum.models
This function uses the uncertainties packages as explained here
https://pythonhosted.org/uncertainties/user_guide.html#use-of-a-covariance-matrix
Examples
--------
TODO
"""
import uncertainties
pars = self.model.parameters
# convert existing parameters to ufloats
values = [pars[_].value for _ in self.covar_axis]
ufloats = uncertainties.correlated_values(values, self.covariance)
upars = dict(zip(self.covar_axis, ufloats))
# add parameters missing in covariance
for name in pars:
upars.setdefault(name, pars[name].value)
return self.model.__class__(**upars)
def iterated_fit(
f,
X,
Y,
p0 = None,
df = None,
absolute_sigma = False,
convergence_condition = DEFAULT_CONVERGENCE_CONDITION,
max_iterations = DEFAULT_MAX_ITERATION,
):
"""
Iterated fit that propagates the errors on the X on the Y to account the x-axis
error.
If p0 is None is calculated with ucurve_fit without X error.
If df is None it is used the numeric derivative from scipy. Not always work.
"""
if df is None:
raise NotImplementedError("Numeric derivatived not implemented yet!")
else:
@wraps(df)
def dmodel(x, *pars):
return unumpy.nominal_values(df(x, *pars))
@wraps(f)
def model(x, *pars):
return unumpy.nominal_values(f(x, *pars))
x, ux = unpack_unarray(X)
y, uy = unpack_unarray(Y)
# Now we can work with normal numpy functions, without unceraties
par, cov = curve_fit(model, x, y, sigma = uy, p0 = p0, absolute_sigma = absolute_sigma)
while --max_iterations:
dif_y = numpy.sqrt(uy**2 + (dmodel(x, *par) * ux)**2)
npar, ncov = curve_fit(
model,
x,
y,
sigma = dif_y,
p0 = par,
absolute_sigma = absolute_sigma
)
perror = numpy.abs(npar - par) / npar
cerror = numpy.abs(ncov - cov) / ncov
if (perror < convergence_condition).all() and (cerror < convergence_condition).all():
break
par = npar
cov = ncov
if max_iterations == 0:
raise Warning("iterated_fit termined because max_iterations was reached.")
return unc.correlated_values(par, cov)
def get_estimates_from_bootstrap(params, daily_installs, observed_days,
conversion_rate, free_trial_conversion, N):
model = BGModel(penalizer_coef=0.01)
Ts = reduce(
lambda x, y: x + y,
[[(observed_days - day) / 7] *
int(math.floor(installs * conversion_rate * free_trial_conversion))
for day, installs in enumerate(daily_installs)])
Ts = filter(lambda x: x > 0, Ts)
gen_data = gen.bgext_model(Ts, params['alpha'], params['beta'])
data = comp.compress_bgext_data(gen_data)
model.fit(frequency=data["frequency"],
T=data["T"],
N=data["N"],
bootstrap_size=N)
exs = []
for i in range(N):
a = model.sampled_parameters[i]['alpha']
b = model.sampled_parameters[i]['beta']
cov = model.params_C
[a, b] = uncertainties.correlated_values([a, b], cov)
Ex = model.wrapped_static_expected_number_of_purchases_up_to_time(
a, b, 52) + 1
if not math.isnan(Ex.n) and not math.isinf(Ex.n):
print((i, Ex))
exs.append(Ex)
return exs, model.expected_number_of_purchases_up_to_time(52) + 1
def model_with_uncertainties(self):
"""Best fit model with uncertainties
The parameters on the model will have the units of the model attribute.
The covariance matrix passed on initialization must also have these
units.
TODO: Add to gammapy.spectrum.models
This function uses the uncertainties packages as explained here
https://pythonhosted.org/uncertainties/user_guide.html#use-of-a-covariance-matrix
Examples
--------
TODO
"""
import uncertainties
pars = self.model.parameters
# convert existing parameters to ufloats
values = [pars[_].value for _ in self.covar_axis]
ufloats = uncertainties.correlated_values(values, self.covariance)
upars = dict(zip(self.covar_axis, ufloats))
# add parameters missing in covariance
for name in pars:
upars.setdefault(name, pars[name].value)
return self.model.__class__(**upars)
def model_with_uncertainties(self):
"""Best fit model with uncertainties
The parameters on the model will have the units of the model attribute.
The covariance matrix passed on initialization must also have these
units.
TODO: Add to gammapy.spectrum.models
This function uses the uncertainties packages as explained here
https://pythonhosted.org/uncertainties/user_guide.html#use-of-a-covariance-matrix
Examples
--------
TODO
"""
if self.covariance is None:
raise ValueError('covariance matrix not set')
import uncertainties
pars = self.model.parameters
# convert existing parameters to ufloats
values = [pars[_].value for _ in self.covar_axis]
ufloats = uncertainties.correlated_values(values, self.covariance)
upars = dict(zip(self.covar_axis, ufloats))
# add parameters missing in covariance
for par in pars.parameters:
upars.setdefault(par.name, par.value)
return self.model.__class__(**upars)
def plot_ratio(xvals, ratio, error, p, plotname, cov=None):
result = "{:.2e} t^2 + {:.2e} t + {:.2e}".format(*p)
result = result.replace("e-0", "e-")
print("Fit result:", result)
if plotname:
result = re.sub(r"e(\S+?)(\s|$)", r" \\times {10}^{\1} ", result)
fig, ax = plt.subplots()
ax.errorbar(xvals, ratio, yerr=error, fmt="k.")
ax.plot(xvals, np.polyval(p, xvals))
ax.text(0.1,
0.85,
"${}$".format(result),
transform=ax.transAxes,
fontsize=16)
if cov is not None and unc is not None:
p_unc = unc.correlated_values(p, cov)
y = np.polyval(p_unc, xvals)
ax.fill_between(
xvals,
unumpy.nominal_values(y) - unumpy.std_devs(y),
unumpy.nominal_values(y) + unumpy.std_devs(y),
alpha=0.5,
facecolor="b",
)
fig.savefig(plotname)
def calc_KMCP(temp=25, sal=35, mode='dickson'):
"""
K2 of MCP dye.
Either calculated using equation 8 of SOP 6b in Dickson,
Sabine & Christian (2007, ISBN:1-897176-07-4), or calculated
using in-house measurements of Tris-buffered artificial seawater.
Parameters
----------
temp : array_like
Temperature in Celcius
sal : array_like
Salinity
mode : str
'dickson' or 'tris'
Returns
-------
array_like : K2 of MCP dye
"""
if mode == 'tris':
p = un.correlated_values(
[8.81873900e-12, -5.00996717e-11, 5.95759909e-09],
[[5.72672924e-24, -2.56643258e-22, 2.80811298e-21],
[-2.56643258e-22, 1.15587639e-20, -1.27159130e-19],
[2.80811298e-21, -1.27159130e-19, 1.40773494e-18]])
return np.polyval(p, temp)
elif mode == 'dickson':
tempK = temp + 273.15
pK = 1245.69 / tempK + 3.8275 + 0.00211 * (35 - sal)
return 10**-pK
else:
raise ValueError('Please specify `mode` as `tris` or `dickson`')
def main():
data = pd.read_csv(
'data/messwerte_2.csv',
skiprows=(1, 2, 3, 4, 5),
)
data['T'] = data['T'].apply(const.C2K)
func = partial(linear, x0=data['t'].mean())
params, cov = curve_fit(func, data['t'], data['T'])
a, b = unc.correlated_values(params, cov)
print('Rate = {} Kelvin per minute'.format(a))
with open('build/rate.tex', 'w') as f:
f.write(r'b = \SI{{{a.n:1.2f} +- {a.s:1.2f}}}{{\kelvin\per\minute}}'.format(a=a))
T_max = 289.95 * u.kelvin
relaxation_time = (
(u.boltzmann_constant * T_max**2) /
(0.526 * u.eV * a * u.kelvin / u.minute) *
np.exp(-0.526 * u.eV / (u.boltzmann_constant * T_max))
)
print(relaxation_time.to(u.second))
t = np.linspace(0, 60, 2)
plt.plot(t, func(t, *params), label='Ausgleichsgerade', color='gray')
plt.plot(data['t'], data['T'], 'x', ms=3, label='Messwerte')
plt.xlabel(r'$t \mathbin{/} \si{\minute}$')
plt.ylabel(r'$T \mathbin{/} \si{\kelvin}$')
plt.legend(loc='lower right')
plt.tight_layout(pad=0)
plt.savefig('build/rate.pdf')
def plot_confintervals(ax_obj, optpar, covpar, xarr, fcolor='grey'):
"""
Plots 3-Sigma Confidence Intervals in Fits of SN Parameters.
Args:
ax_obj : Axes object on which the confidence interval is to be plotted
optpar : Optimised Parameters of the Fit
covpar : Covariance Parameters of the Fit
xarr : Array of X-Values over which confidence intervals are to be plotted
fcolor : Fill color for the confidence intervals
Returns:
None
"""
coeff = unc.correlated_values(optpar, covpar)
func = ls.legval(xarr, coeff)
fit = unp.nominal_values(func)
sigma = unp.std_devs(func)
fitlow = fit - 3 * sigma
fithigh = fit + 3 * sigma
ax_obj.plot(xarr,
fitlow,
ls='-.',
c='k',
lw=0.7,
alpha=0.3,
label='_nolegend_')
ax_obj.plot(xarr,
fithigh,
ls='-.',
c='k',
lw=0.7,
alpha=0.3,
label='_nolegend_')
ax_obj.fill_between(xarr, fitlow, fithigh, facecolor=fcolor, alpha=0.3)
def Plot(x=[], y=[], limx=None, limy=None, xname='', yname='', name='', markername='Wertepaare', marker='rx', linear=True, linecolor='b-', linename='Ausgleichsgerade', xscale=1, yscale=1, save=True, Plot=True):
uParams = None
if(Plot):
dx = abs(x[-1]-x[0])
if(limx==None):
xplot = np.linspace((x[0]-0.05*dx)*xscale,(x[-1]+0.05*dx)*xscale,1000)
else:
xplot = np.linspace(limx[0]*xscale,limx[1]*xscale,1000)
if(save):
plt.cla()
plt.clf()
plt.errorbar(noms(x)*xscale, noms(y)*yscale, xerr=stds(x)*xscale, yerr=stds(y)*yscale, fmt=marker, markersize=6, elinewidth=0.5, capsize=2, capthick=0.5, ecolor='g',barsabove=True ,label=markername)
if(linear == True):
params, covar = curve_fit(Line, noms(x), noms(y))
uParams=uncertainties.correlated_values(params, covar)
if(Plot):
plt.plot(xplot*xscale, Line(xplot, *params)*yscale, linecolor, label=linename)
if(Plot):
if(limx==None):
plt.xlim((x[0]-0.05*dx)*xscale,(x[-1]+0.05*dx)*xscale)
else:
plt.xlim(limx[0]*xscale,limx[1]*xscale)
if(limy != None):
plt.ylim(limy[0]*yscale,limy[1]*yscale)
plt.xlabel(xname)
plt.ylabel(yname)
plt.legend(loc='best')
plt.tight_layout(pad=0, h_pad=1.08, w_pad=1.08)
if(save):
plt.savefig('build/'+name+'.pdf')
if(linear):
return(uParams)
def integral():
x1 = uc.ufloat( 20 /2 *10**(-3) , 1*10**(-3))
x2 = uc.ufloat( 150/2 *10**(-3) , 1*10**(-3))
L = uc.ufloat( 175 *10**(-3) , 1*10**(-3))
l = uc.ufloat( 150 *10**(-3) , 1*10**(-3))
I = uc.ufloat(10 , 0.1)
N = 3600
A = N / (2 *L * (x2-x1))
factor = (x2 * (sqrt( x2**2 + ((L+l)/2)**2)- sqrt( x2**2 + ((L-l)/2)**2) ) \
-x1 * (sqrt( x1**2 + ((L+l)/2)**2)- sqrt( x1**2 + ((L-l)/2)**2) ) \
+ (((L+l)/2)**2* log((x2 + sqrt(((L+l)/2)**2 + x2**2))/ (x1 + sqrt(((L+l)/2)**2 + x1**2)) ) \
-((L-l)/(4))**2* log((x2 + sqrt(((L-l)/2)**2 + x2**2))/ (x1 + sqrt(((L-l)/2)**2 + x1**2)) )))
print(factor)
print(A * factor)
a = np.load(input_dir +"a_3.npy")
I = np.load(input_dir + "i_3.npy")
I_fit = np.linspace(min(I),max(I),100)
S_a = 0.2
S_I = 0.05
weights = a*0 + 1/S_a
p, cov= np.polyfit(I,a, 1, full=False, cov=True, w=weights)
(p1, p2) = uc.correlated_values([p[0],p[1]], cov)
print(p1 / (A*factor))
print(p1/2556/100 *oe *60)
def salt2mu_aberr(x1=None,x1err=None,
c=None,cerr=None,
mb=None,mberr=None,
cov_x1_c=None,cov_x1_x0=None,cov_c_x0=None,
alpha=None,beta=None,
alphaerr=None,betaerr=None,
M=None,x0=None,sigint=None,z=None,peczerr=0.0005):
from uncertainties import ufloat, correlated_values, correlated_values_norm
alphatmp,betatmp = alpha,beta
alpha,beta = ufloat(alpha,alphaerr),ufloat(beta,betaerr)
sf = -2.5/(x0*np.log(10.0))
cov_mb_c = cov_c_x0*sf
cov_mb_x1 = cov_x1_x0*sf
mu_out,muerr_out = np.array([]),np.array([])
for i in range(len(x1)):
covmat = np.array([[mberr[i]**2.,cov_mb_x1[i],cov_mb_c[i]],
[cov_mb_x1[i],x1err[i]**2.,cov_x1_c[i]],
[cov_mb_c[i],cov_x1_c[i],cerr[i]**2.]])
mb_single,x1_single,c_single = correlated_values([mb[i],x1[i],c[i]],covmat)
mu = mb_single + x1_single*alpha - beta*c_single + 19.36
if sigint: mu = mu + ufloat(0,sigint)
zerr = peczerr*5.0/np.log(10)*(1.0+z[i])/(z[i]*(1.0+z[i]/2.0))
mu = mu + ufloat(0,np.sqrt(zerr**2. + 0.055**2.*z[i]**2.))
mu_out,muerr_out = np.append(mu_out,mu.n),np.append(muerr_out,mu.std_dev)
return(mu_out,muerr_out)
def ucurve_fit(model,
X,
Y,
p0=None,
absolute_sigma=True,
check_finite=True,
bounds=(-numpy.inf, +numpy.inf),
method=None,
jac=None):
x, ux = unpack_unarray(X)
y, uy = unpack_unarray(Y)
p, cov = curve_fit(model,
x,
y,
sigma=uy,
p0=p0,
absolute_sigma=absolute_sigma,
check_finite=check_finite,
bounds=bounds,
method=method,
jac=jac)
return unc.correlated_values(p, cov)
def _scp_error_curve_fit(f, x, y, *args, **kwargs):
if not 'sigma' in kwargs:
kwargs['sigma'] = unp.std_devs(y)
if not 'absolute_sigma' in kwargs:
kwargs['absolute_sigma'] = True
result = scp.optimize.curve_fit(f, unp.nominal_values(x),
unp.nominal_values(y), *args, **kwargs)
return uc.correlated_values(*result)
def ucurve_fit(f, x, y, **kwargs):
if np.any(unp.std_devs(y) == 0):
sigma = None
else:
sigma = unp.std_devs(y)
popt, pcov = scipy.optimize.curve_fit(f, x, unp.nominal_values(y), sigma=sigma, **kwargs)
return unc.correlated_values(popt, pcov)
def MLS(model,
d_model,
X,
Y,
convergence_condition=1e-7,
max_iterations=20,
p0=None,
absolute_sigma=True,
verbose=False):
if type(p0) != 'numpy.ndarray':
try:
p0, up0 = unpack_unarray(p0)
except TypeError:
pass
x, ux = unpack_unarray(X)
y, uy = unpack_unarray(Y)
# Primo step curve fit
par, cov = curve_fit(model,
x,
y,
sigma=uy,
p0=p0,
absolute_sigma=absolute_sigma)
# Procedimento iterato
while --max_iterations:
dif_y = numpy.sqrt(uy**2 + (d_model(x, *par) * ux)**2)
npar, ncov = curve_fit(model,
x,
y,
sigma=dif_y,
p0=par,
absolute_sigma=absolute_sigma)
if verbose:
print(npar)
print(ncov)
perror = numpy.abs(npar - par) / npar
cerror = numpy.abs(ncov - cov) / ncov
if (perror < convergence_condition).all() and (
cerror < convergence_condition).all():
if verbose:
print("MLS Convergence")
break
par = npar
cov = ncov
return unc.correlated_values(npar, ncov)
def pH_from_spectrum(wavelength, spectrum, dye='BPB', sigma=None, temp=25., sal=35., **kwargs):
pe = un.correlated_values(*unmix_spectra(wavelength, spectrum, dye, sigma))
F = pe[1] / pe[0]
dyeK = dyes.K_handler(dye, temp=temp, sal=sal, **kwargs)
return pH_from_F(F=F, K=dyeK)
def ucurve_fit(f, x, y, **kwargs):
if np.any(unp.std_devs(y) == 0):
sigma = None
else:
sigma = unp.std_devs(y)
popt, pcov = scipy.optimize.curve_fit(f, x, unp.nominal_values(y), sigma=sigma, **kwargs)
return unc.correlated_values(popt, pcov)
def CdTe_Am():
detector_name = "CdTe"
sample_name = "Am"
suff = "_" + sample_name + "_" + detector_name
npy_file = npy_dir + "spectra" + suff + ".npy"
n = np.load(npy_file)[:500]
s_n = np.sqrt(n)
x = np.arange(len(n))
# only fit
p0 = [250000, 250, 25]
red = (x > 235) * (x < 270)
n_red = n[red]
x_red = x[red]
s_n_red = s_n[red]
fit, cov_fit = curve_fit(gauss, x_red, n_red, p0=p0, sigma=s_n_red)
fit = np.abs(fit)
fit_corr = uc.correlated_values(fit, cov_fit)
s_fit = un.std_devs(fit_corr)
# chi square
n_d = 4
chi2 = np.sum(((gauss(x_red, *fit) - n_red) / s_n_red) ** 2 )
chi2_test = chi2/n_d
fit_r, s_fit_r = err_round(fit, cov_fit)
fit_both = np.array([fit_r, s_fit_r])
fit_both = np.reshape(fit_both.T, np.size(fit_both))
As[2], mus[2], sigmas[2] = fit
s_As[2], s_mus[2], s_sigmas[2] = un.std_devs(fit_corr)
all = np.concatenate((fit_both, [chi2_test]), axis=0)
def plot_two_gauss():
fig1, ax1 = plt.subplots(1, 1)
if not save_fig:
fig1.suptitle("Detector: " + detector_name + "; sample: " + sample_name)
plot1, = ax1.plot(x, n, '.', alpha=0.3) # histo plot
ax1.errorbar(x, n, yerr=s_n, fmt=',', alpha=0.99, c=plot1.get_color(), errorevery=10) # errors of t are not changed!
ax1.plot(x_red, gauss(x_red, *fit))
ax1.set_xlabel("channel")
ax1.set_ylabel("counts")
textstr = 'Results of fit:\n\
\\begin{eqnarray*}\
A &=& (%.0f \pm %.0f) \\\\ \
\mu &=& (%.1f \pm %.1f) \\\\ \
\sigma&=& (%.1f \pm %.1f) \\\\ \
\chi^2 / n_d &=& %.1f\
\end{eqnarray*}'%tuple(all)
ax1.text(0.65, 0.95, textstr, transform=ax1.transAxes, va='top', bbox=props)
if show_fig:
fig1.show()
if save_fig:
file_name = "detector" + suff
fig1.savefig(fig_dir + file_name + ".pdf")
fig1.savefig(fig_dir + file_name + ".png")
return 0
plot_two_gauss()
return fit, s_fit
def poly_fit(x, y_e, x_range, p0):
x_min, x_max = x_range
mask = (x > x_min) * (x < x_max)
x_fit = x[mask]
y_fit = un.nominal_values(y_e[mask])
y_sigma = np.sqrt(un.std_devs(y_e[mask]))
coeff, cov = curve_fit(poly, x_fit, y_fit, p0=p0,
sigma=y_sigma, absolute_sigma=True)
c = uc.correlated_values(coeff, cov)
return c
def _fit_odr(datax, datay, function, params=None, yerr=None, xerr=None):
model = Model(lambda p, x: function(x, *p))
realdata = RealData(datax, datay, sy=yerr, sx=xerr)
odr = ODR(realdata, model, beta0=params)
out = odr.run()
# This was the old wrong way! Now use correct co. matrix through unc-package!
# Note Issues on scipy odr and curve_fit, regarding different definitions/namings of standard deviation or error and covaraince matrix
# https://github.com/scipy/scipy/issues/6842
# https://github.com/scipy/scipy/pull/12207
# https://stackoverflow.com/questions/62460399/comparison-of-curve-fit-and-scipy-odr-absolute-sigma
return unc.correlated_values(out.beta, out.cov_beta)
def plot_fits(country, df, exp_popt, exp_pcov, log_popt, log_pcov,
inflection_p_idx, case):
plt.figure(figsize=(10, 5))
firstday = 0
lastday = df[country].dropna().shape[0]
xdata = df['Day'][(df['Day'] >= firstday) & (df['Day'] < lastday)]
ydata = df[country][(df['Day'] >= firstday) & (df['Day'] < lastday)]
x = np.linspace(firstday, lastday + 10, 100)
plt.plot(xdata, ydata, 'k.', label='data')
plt.plot(x, exponential(x, *exp_popt), 'r-', label="Exponential fit")
plt.plot(x, logistic(x, *log_popt), 'b-', label='Logistic fit')
ae, be, ce = unc.correlated_values(exp_popt, exp_pcov)
py = ae * unp.exp(be * x) + ce
nom = unp.nominal_values(py)
std = unp.std_devs(py)
plt.fill_between(x,
nom + 2 * std,
nom - 2 * std,
facecolor="red",
alpha=.2)
al, bl, cl, dl, el = unc.correlated_values(log_popt, log_pcov)
py = al / (1 + bl * unp.exp(-cl * (x - dl))) + el
nom = unp.nominal_values(py)
std = unp.std_devs(py)
plt.fill_between(x,
nom + 2 * std,
nom - 2 * std,
facecolor="blue",
alpha=.2)
plt.plot(x[inflection_p_idx],
logistic(x, *log_popt)[inflection_p_idx],
'oy',
label='inflection point')
plt.legend()
if case == "confirmed":
set_cases_labels()
elif case == "deaths":
set_deaths_labels()
plt.ylim(-ydata.max() / 10., 2 * ydata.max())
plt.title(country, loc='center')
plt.show()
def linleastsquares(functions, x_values, y_values):
y = unp.nominal_values(y_values)
Z = np.linalg.inv(unc.covariance_matrix(y_values))
A = np.column_stack([f(x_values) for f in functions])
invATA = np.linalg.inv(A.T @ Z @ A)
params = invATA @ A.T @ Z @ y
cov = invATA
return unc.correlated_values(params.flat, cov)
def test_ucurve_fit_correlation():
def model(x, a, b):
return numpy.sqrt(a * x + b)
def umodel(x, a, b):
return unumpy.sqrt(a * x + b)
x = numpy.array([3., 41., 100.])
ux = x / 100.
y = numpy.array([5., 15., 25.])
uy = numpy.array([[0.01, 0.001, 0.01],
[0.001, 0.01, 0.02],
[0.01, 0.02, 0.05]])
p, cov = curve_fit(model, x, y, sigma=uy)
fitted1 = correlated_values(p, cov)
X = unarray(x, ux)
Y = correlated_values(y, uy)
fitted2 = ucurve_fit(umodel, X, Y)
assert(str(fitted1[0]) == str(fitted2[0]))
assert(str(fitted1[1]) == str(fitted2[1]))
def parabola_fit(points):
dims = points[0][0].shape[0]
x = np.array([p[0] for p in points])
f = np.array([p[1] for p in points])
A = build_design_matrix(x, f)
B = build_design_vector(f)[:, np.newaxis] # make column vector
# Compute best-fit parabola coefficients using a singular value
# decomposition.
U, w, V = np.linalg.svd(A, full_matrices=False)
V = V.T # Flip to convention used by Numerical Recipies
inv_w = 1.0 / w
inv_w[np.abs(w) < 1e-6] = 0.0
# Numpy version of Eq 15.4.17 from Numerical Recipies (C edition)
coeffs = np.zeros(A.shape[1])
for i in range(len(coeffs)):
coeffs += (np.dot(U[:, i], B[:, 0]) * inv_w[i]) * V[:, i]
# Chi2 and probability for best fit and quadratic coefficents
chi2_terms = np.dot(A, coeffs[:, np.newaxis]) - B
chi2 = (chi2_terms**2).sum()
ndf = len(points) - (1 + dims + dims * (dims + 1) / 2)
prob = ROOT.TMath.Prob(chi2, ndf)
# Covariance is from Eq 15.4.20
covariance = np.dot(V * inv_w**2, V.T)
# Pack the coefficients into ufloats
ufloat_coeffs = uncertainties.correlated_values(coeffs,
covariance.tolist())
# Separate coefficients into a, b, and c
a = ufloat_coeffs[0]
b = ufloat_coeffs[1:dims + 1]
c = np.zeros(shape=(dims, dims), dtype=object)
index = dims + 1
for i in range(dims):
for j in range(i, dims):
c[i, j] = ufloat_coeffs[index]
c[j, i] = ufloat_coeffs[index]
if j != i:
# We combined the redundant off-diagonal parts of c
# matrix, but now we have to divide by two to
# avoid double counting when c is used later
c[i, j] /= 2.0
c[j, i] /= 2.0
index += 1
return a, np.array(b), c, chi2, prob
def parabola_fit(points):
dims = points[0][0].shape[0]
x = np.array([p[0] for p in points])
f = np.array([p[1] for p in points])
A = build_design_matrix(x, f)
B = build_design_vector(f)[:,np.newaxis] # make column vector
# Compute best-fit parabola coefficients using a singular value
# decomposition.
U, w, V = np.linalg.svd(A, full_matrices=False)
V = V.T # Flip to convention used by Numerical Recipies
inv_w = 1.0/w
inv_w[np.abs(w) < 1e-6] = 0.0
# Numpy version of Eq 15.4.17 from Numerical Recipies (C edition)
coeffs = np.zeros(A.shape[1])
for i in xrange(len(coeffs)):
coeffs += (np.dot(U[:,i], B[:,0]) * inv_w[i]) * V[:,i]
# Chi2 and probability for best fit and quadratic coefficents
chi2_terms = np.dot(A, coeffs[:,np.newaxis]) - B
chi2 = (chi2_terms**2).sum()
ndf = len(points) - (1 + dims + dims * (dims + 1) / 2)
prob = ROOT.TMath.Prob(chi2, ndf)
# Covariance is from Eq 15.4.20
covariance = np.dot(V*inv_w**2, V.T)
# Pack the coefficients into ufloats
ufloat_coeffs = uncertainties.correlated_values(coeffs, covariance.tolist())
# Separate coefficients into a, b, and c
a = ufloat_coeffs[0]
b = ufloat_coeffs[1:dims+1]
c = np.zeros(shape=(dims,dims), dtype=object)
index = dims + 1
for i in xrange(dims):
for j in xrange(i, dims):
c[i,j] = ufloat_coeffs[index]
c[j,i] = ufloat_coeffs[index]
if j != i:
# We combined the redundant off-diagonal parts of c
# matrix, but now we have to divide by two to
# avoid double counting when c is used later
c[i,j] /= 2.0
c[j,i] /= 2.0
index += 1
return a, np.array(b), c, chi2, prob
def verdet_constant():
a = np.load(input_dir +"a_3.npy")
I = np.load(input_dir + "i_3.npy")
I_fit = np.linspace(min(I),max(I),100)
S_a = 0.2
S_I = 0.05
weights = a*0 + 1/S_a
p, cov= np.polyfit(I,a, 1, full=False, cov=True, w=weights)
(p1, p2) = uc.correlated_values([p[0],p[1]], cov)
print(p1/2556)
print(p1/2556/100 *oe *60)
def to_uncertainties(self):
"""Convert to `uncertainties`_ objects.
The `uncertainties`_ package makes it easy to
do error propagation on derived quantities.
See :ref:`analyse-error`.
Returns
-------
tuple (length ``n``) of ``uncertainties.core.AffineScalarFunc``
"""
from uncertainties import correlated_values
return correlated_values(self.mean, self.cov)
def fitSpectrum(self):
K = K_handler(self.mode, self.data['temp'], self.sal)
p, cov = unmix_spectra(self.data['wv'], self.data['absorption'],
self.mode)
self.p = un.correlated_values(p, cov)
F = self.p[1] / self.p[0]
pH = pH_from_F(F, K)
self.storeResult(K, F, pH)
self.updateFitGraph()
def two_bw_fit(x, y_e, x_range, p0, fit=True):
x_min, x_max = x_range
mask = (x > x_min) * (x < x_max)
x_fit = x[mask]
y_fit = un.nominal_values(y_e[mask])
y_sigma = np.sqrt(un.std_devs(y_e[mask]))
if fit:
coeff, cov = curve_fit(two_breit_wigner, x_fit, y_fit, p0=p0,
sigma=y_sigma, absolute_sigma=True)
c = uc.correlated_values(coeff, cov)
fit_peak = two_breit_wigner(x_fit, *coeff)
else:
fit_peak = two_breit_wigner(x_fit, *p0)
c = un.uarray(p0, [0, 0, 0, 0])
return x_fit, fit_peak, c
def auswerten(param):
name, p0 = param
I1, U1 = np.genfromtxt('daten/' + name + '1.txt', unpack=True)
I2, U2 = np.genfromtxt('daten/' + name + '2.txt', unpack=True)
popt1, pcov1 = curve_fit(cauchy, I1, U1, maxfev=10000000, p0=p0)
popt2, pcov2 = curve_fit(cauchy, I2, U2, maxfev=10000000, p0=p0)
x = np.linspace(0, 950, 1000)
plt.xlim(0, 950)
plt.xlabel(r'$I/\mathrm{mA}$')
plt.ylabel(r'$U_B / \mathrm{mV}$')
plt.plot(x, cauchy(x, *popt1), 'C0', label="Fit (mod. Cauchy/Lorentz)")
plt.plot(x, cauchy(x, *popt2), 'C1', label="Fit (mod. Cauchy/Lorentz)")
plt.plot(I1, U1, 'x', label='Daten 1')
plt.plot(I2, U2, 'x', label='Daten 2')
plt.legend(loc='best')
plt.tight_layout(pad=0)
plt.savefig('build/' + name + '.pdf')
plt.close()
param1 = unc.correlated_values(popt1, pcov1)
param2 = unc.correlated_values(popt2, pcov2)
return param1[2], param2[2]
def plot_fit(f,
c,
fit_result,
xlimits,
ylimits,
disregard_correlation=False,
color='gray',
alpha=0.3,
fill_band=True,
npoints=100):
"""Plot the error butterfly.
Errors are propagated using the uncertainties module.
If disregard_correlation == True, the off-diagonal elements of the
covariance matrix are set to 0 before propagating the errors.
"""
import matplotlib.pylab as plt
import uncertainties
# Choose equal-log x spacing
logxlimits = np.log10(xlimits)
logx = np.linspace(logxlimits[0], logxlimits[1], npoints)
x = 10**logx
popt = fit_result[0]
pcov = fit_result[1]
if disregard_correlation:
pcov = set_off_diagonal_to_zero(pcov)
y = f(popt, c, x)
# Use uncertainties to compute an error band
p_wu = uncertainties.correlated_values(popt, pcov)
y_wu = f(p_wu, c, x)
y_val = np.empty_like(y_wu)
y_err = np.empty_like(y_wu)
for i in range(y_wu.size):
y_val[i] = y_wu[i].nominal_value
y_err[i] = y_wu[i].std_dev
# Need to clip values to frame so that no plotting artifacts occur
y1 = np.maximum(y - y_err, ylimits[0])
y2 = np.minimum(y + y_err, ylimits[1])
# Plot error band
if fill_band == True:
plt.fill_between(x, y1, y2, color=color, alpha=alpha)
else:
plt.plot(x, y1, color=color, alpha=alpha)
plt.plot(x, y2, color=color, alpha=alpha)
# Plot best-fit spectrum
plt.plot(x, y, color=color, alpha=alpha)
def fit_curve(df, country, status, start_date, end_date=None):
"""
Summary line.
Extended description of function.
Parameters:
arg1 (int): Description of arg1
Returns:
int: Description of return value
"""
# Select the data
slc_date = slice(start_date, end_date)
y_data = df.loc[(country, status), slc_date].groupby(
CTRY_K).sum().values[0]
# Generate a dummy x_data
x_data = np.arange(0, y_data.shape[0])
# Set initial guesses for the curve fit
x0_0 = x_data[np.where(y_data > 0)[0][0]] # Day of the first case
a_0 = y_data.max() # Current number of cases
b_0 = 0.1 # Arbitrary
p0 = [x0_0, a_0, b_0]
# Fit the curve
popt, pcov = opt.curve_fit(sig, x_data, y_data, p0=p0)
# Evaluate the curve fit to calculate the R²
y_fit = sig(x_data, *popt)
r2 = mt.r2_score(y_data, y_fit)
# Estimate the uncertainty of the obtained coefficients
x0, a, b, = unc.correlated_values(popt, pcov)
# Store the fit information
fit = {
"r2": r2,
"x0": x0,
"a": a,
"b": b,
"coef": popt,
"coef_cov": pcov,
"y_data": y_data,
"x_data": slc_date,
}
return x0, a, b, fit
def _fit_curvefit(datax, datay, function, params=None, yerr=None, **kwargs):
try:
pfit, pcov = \
optimize.curve_fit(function, datax, datay, p0=params,
sigma=yerr, epsfcn=util.get("epsfcn", kwargs, 0.0001), **kwargs, maxfev=util.get("maxfev", kwargs, 10000))
except RuntimeError as e:
debug.msg(str(e))
return params
error = []
for i in range(len(pfit)):
try:
error.append(np.absolute(pcov[i][i])**0.5)
except Exception as e:
warnings.warn(str(e))
error.append(0.00)
return unc.correlated_values(pfit, pcov)
def _ufloats(self):
"""Return dict of ufloats with covariance."""
from uncertainties import correlated_values
values = [_.value for _ in self.parameters]
try:
# convert existing parameters to ufloats
uarray = correlated_values(values, self.covariance)
except np.linalg.LinAlgError:
raise ValueError("Covariance matrix not set.")
upars = {}
for par, upar in zip(self.parameters, uarray):
upars[par.name] = upar
return upars
def plot_fit(f, c, fit_result, xlimits, ylimits,
disregard_correlation=False,
color='gray', alpha=0.3,
fill_band=True,
npoints=100):
"""Plot the error butterfly.
Errors are propagated using the uncertainties module.
If disregard_correlation == True, the off-diagonal elements of the
covariance matrix are set to 0 before propagating the errors.
"""
import matplotlib.pylab as plt
import uncertainties
# Choose equal-log x spacing
logxlimits = np.log10(xlimits)
logx = np.linspace(logxlimits[0], logxlimits[1], npoints)
x = 10 ** logx
popt = fit_result[0]
pcov = fit_result[1]
print pcov
if disregard_correlation:
pcov = set_off_diagonal_to_zero(pcov)
print pcov
y = f(popt, c, x)
# Use uncertainties to compute an error band
p_wu = uncertainties.correlated_values(popt, pcov)
y_wu = f(p_wu, c, x)
y_val = np.empty_like(y_wu)
y_err = np.empty_like(y_wu)
for i in range(y_wu.size):
y_val[i] = y_wu[i].nominal_value
y_err[i] = y_wu[i].std_dev
# Need to clip values to frame so that no plotting artifacts occur
y1 = np.maximum(y - y_err, ylimits[0])
y2 = np.minimum(y + y_err, ylimits[1])
# Plot error band
if fill_band == True:
plt.fill_between(x, y1, y2, color=color, alpha=alpha)
else:
plt.plot(x, y1, color=color, alpha=alpha)
plt.plot(x, y2, color=color, alpha=alpha)
# Plot best-fit spectrum
plt.plot(x, y, color=color, alpha=alpha)
def linleastsquares(functionlist, x_values, y_values):
y = np.matrix(unp.nominal_values(y_values)).T
Z = np.matrix(unc.covariance_matrix(y_values)).I
# N rows vor every value, p columns for every function
dim = (len(x_values), len(functionlist))
A = np.matrix(np.zeros(dim))
for i, func in enumerate(functionlist):
A[:, i] = func(x_values)[:, np.newaxis]
invATA = (A.T * Z * A).I
params = invATA * A.T * Z * y
cov = invATA
return (np.array(unc.correlated_values(params.flat, np.array(cov))))
def translate_fit_parameters(popt, pcov, P_detector0_raw, T=300*u.K):
"""Take the fit parameters and covariances, and converts them to
SI values and errors for f_c, k_c, Q.
Also makes sure all values are positive."""
pvals = correlated_values(popt, pcov)
punits = [u.nm**2 / u.Hz, u.Hz, u.dimensionless, u.nm**2 / u.Hz]
scales = [P_detector0_raw, 1, 1, P_detector0_raw]
def create_measurement(uncert_val, unit, scale):
return (uncert_val.n * unit).plus_minus(uncert_val.s) * scale
P_x0, f_c, Q, P_detector = [np.abs(
create_measurement(uncert_val, unit, scale)
) for
uncert_val, unit, scale in
zip(pvals, punits, scales)]
k_c = np.abs(calc_k_c(f_c, Q, P_x0, T))
return f_c, k_c, Q, P_detector
def ucurve_fit(f, x, y, **kwargs):
'''
Uncertainties wrapper around curve_fit
y can be a uarray with uncertainties
and the parameters are returned as uncertainties.correlated_values
'''
if np.any(unp.std_devs(y) == 0):
sigma = None
else:
sigma = unp.std_devs(y)
popt, pcov = scipy.optimize.curve_fit(
f,
x,
unp.nominal_values(y),
sigma=sigma,
absolute_sigma=True,
**kwargs,
)
return unc.correlated_values(popt, pcov)
def calibration(detector_name, mu, s_mu):
"""
does a linear fit fit three points !!!
"""
def lin_func(x, a, b):
return(a*x + b)
fit_, cov_fit_ = curve_fit(lin_func, Es, mu, p0=None, sigma=s_mu)
fit_corr_ = uc.correlated_values(fit_, cov_fit_)
fit_corr = np.array([1 / fit_corr_[0], - fit_corr_[1] / fit_corr_[0]])
fit = un.nominal_values(fit_corr)
cov_fit = uc.covariance_matrix(fit_corr)
s_fit = un.std_devs(fit_corr)
fit_r, s_fit_r = err_round(fit, cov_fit)
fit_both = np.array([fit_r, s_fit_r])
fit_both = np.reshape(fit_both.T, np.size(fit_both))
fig1, ax1 = plt.subplots(1, 1)
if not save_fig:
fig1.suptitle("Calibration: " + detector_name)
#plot1, = ax1.plot(mu, Es, '.', alpha=0.9)
mu_grid = np.linspace(0, 700, 100)
plot_fit, = ax1.plot(mu_grid, lin_func(mu_grid, *fit), alpha=0.5)
ax1.errorbar(mu, Es, xerr=s_mu, fmt='.', alpha=0.99, c=plot_fit.get_color()) # errors of t are not changed!
ax1.set_xlabel("channel")
ax1.set_ylabel("Energy / keV")
textstr = 'Results of linear fit for %s'%detector_name + ":\n"
textstr += '\\begin{eqnarray*}\
E(\mu)&=& a \mu + E_0 \\\\ \
a &=& (%.4f \pm %.4f)\, \mathrm{keV / ch} \\\\ \
E_0 &=& (%.1f \pm %.1f)\, \mathrm{keV} \\\\ \
\end{eqnarray*}'%tuple(fit_both)
ax1.text(0.1, 0.95, textstr, transform=ax1.transAxes, va='top', bbox=props)
if show_fig:
fig1.show()
if save_fig:
file_name = "detector_calibration_" + detector_name
fig1.savefig(fig_dir + file_name + ".pdf")
fig1.savefig(fig_dir + file_name + ".png")
return fit_corr[0]
def main():
data = pd.read_csv("build/data_corrected.csv")
data["invT"] = 1 / data["T"]
data["j"] = data["I_corrected"] / A
data["logj"] = np.log(data["j"])
fit_region = data.query("0.00345 < invT < 0.0037")
func = partial(linear, x0=fit_region.invT.mean())
params, cov = curve_fit(func, fit_region["invT"], fit_region["logj"])
a, b = unc.correlated_values(params, cov)
with open("build/fit_parameters_1.tex", "w") as f:
f.write(r"a &= {}".format(SI(a, r"\kelvin")))
f.write(" \\\\ \n ")
f.write(r"b &= {}".format(num(b)))
with open("build/activation_work_1.tex", "w") as f:
f.write("W = ")
f.write(SI(-a * const.k, r"\joule"))
f.write(" = ")
f.write(SI(-a * const.k / const.e, r"\electronvolt"))
px = np.linspace(3.335e-3, 3.7e-3, 2)
plt.plot(px, func(px, a.n, b.n), label="Ausgleichsgerade")
plt.plot(data.invT, data.logj, "+", ms=3, label="Nicht berücksichtigt", color="#949494")
plt.plot(fit_region.invT, fit_region.logj, "+", ms=3, label="Fit-Region")
plt.legend()
plt.xlabel(r"$T^{-1} \mathrel{/} \si{\per\kelvin}$")
plt.ylabel(r"$\ln(j \mathrel{/} \si{\pico\ampere})$")
plt.xlim(0.0031, 0.0038)
# plt.ylim(6, 8.1)
plt.tight_layout(pad=0)
plt.savefig("build/method1.pdf")
def plot_ratio(xvals, ratio, error, p, plotname, cov=None):
result = "{:.2e} t^2 + {:.2e} t + {:.2e}".format(*p)
result = result.replace('e-0','e-')
print("Fit result:", result)
if plotname:
result = re.sub(r'e(\S+?)(\s|$)', r' \\times {10}^{\1} ', result)
fig, ax = plt.subplots()
ax.errorbar(xvals, ratio, yerr=error, fmt='k.')
ax.plot(xvals, np.polyval(p, xvals))
ax.text(.1, .85, "${}$".format(result),
transform=ax.transAxes, fontsize=16)
if cov is not None and unc is not None:
p_unc = unc.correlated_values(p, cov)
y = np.polyval(p_unc, xvals)
ax.fill_between(xvals,
unumpy.nominal_values(y)-unumpy.std_devs(y),
unumpy.nominal_values(y)+unumpy.std_devs(y),
alpha=.5, facecolor='b')
fig.savefig(plotname)
header=2, names=['t', 'U'],
)
# embed()
df['t'] = (df.t - df.ix[df['U'].idxmax()].t)
plateau = df.query('t > -0.8e-6 & t < -0.1e-6')
u_1 = ufloat(plateau['U'].mean(), plateau['U'].std())
ax_1.axhline(u_1.n, color='#ababab')
ax_1.axhline(df['U'].max(), color='#ababab')
reflection_factor = (df['U'].max() / u_1)
R = - 50 * (1 + reflection_factor)/(1 - reflection_factor)
print('resistance is {}'.format(R))
df_fit = df.query('t > 0.4e-6 & t < 3e-6').dropna()
popt, pcov = opt.curve_fit(curve, df_fit['t'], df_fit['U'], [1, 1e-6, 1])
a_0, tau, u_0 = correlated_values(popt, pcov)
print('tau is {}'.format(tau))
L = tau * (50 + R)
print('L is {}'.format(L))
ax_1.plot(df['t']*1e6, df['U'], alpha=0.8, label='Gemessene Spannung')
ax_1.plot(df_fit['t']*1e6, curve(df_fit['t'], a_0.n, tau.nominal_value, u_0.n), linewidth=2, label='Fit mit Exponentialfunktion')
# ax_1.legend(loc='upper right')
ax_1.set_ylabel(r'$U \mathbin{/} \si{\volt}$')
ax_1.set_xlim(-2, 6)
capacity_tex = '\SI{{{:.0f} \pm {:.0f}}}{{\\micro\\henry}}'.format(L.n * 1e6, L.s* 1e6)
with open('build/k1a6_l.tex', 'w') as f:
f.write(capacity_tex)
def leastsq(self, scale_covar=True, **kws):
"""
use Levenberg-Marquardt minimization to perform fit.
This assumes that ModelParameters have been stored,
and a function to minimize has been properly set up.
This wraps scipy.optimize.leastsq, and keyword arguments are passed
directly as options to scipy.optimize.leastsq
When possible, this calculates the estimated uncertainties and
variable correlations from the covariance matrix.
writes outputs to many internal attributes, and
returns True if fit was successful, False if not.
"""
# print 'RUNNING LEASTSQ'
self.prepare_fit()
lskws = dict(full_output=1, xtol=1.0e-7, ftol=1.0e-7, gtol=1.0e-7, maxfev=2000 * (self.nvarys + 1), Dfun=None)
lskws.update(self.kws)
lskws.update(kws)
if lskws["Dfun"] is not None:
self.jacfcn = lskws["Dfun"]
lskws["Dfun"] = self.__jacobian
lsout = scipy_leastsq(self.__residual, self.vars, **lskws)
_best, _cov, infodict, errmsg, ier = lsout
self.residual = resid = infodict["fvec"]
self.ier = ier
self.lmdif_message = errmsg
self.message = "Fit succeeded."
self.success = ier in [1, 2, 3, 4]
if ier == 0:
self.message = "Invalid Input Parameters."
elif ier == 5:
self.message = self.err_maxfev % lskws["maxfev"]
else:
self.message = "Tolerance seems to be too small."
self.nfev = infodict["nfev"]
self.ndata = len(resid)
sum_sqr = (resid ** 2).sum()
self.chisqr = sum_sqr
self.nfree = self.ndata - self.nvarys
self.redchi = sum_sqr / self.nfree
# need to map _best values to params, then calculate the
# grad for the variable parameters
grad = ones_like(_best)
vbest = ones_like(_best)
for ivar, varname in enumerate(self.var_map):
par = self.params[varname]
grad[ivar] = par.scale_gradient(_best[ivar])
vbest[ivar] = par.value
# modified from JJ Helmus' leastsqbound.py
infodict["fjac"] = transpose(transpose(infodict["fjac"]) / take(grad, infodict["ipvt"] - 1))
rvec = dot(triu(transpose(infodict["fjac"])[: self.nvarys, :]), take(eye(self.nvarys), infodict["ipvt"] - 1, 0))
try:
cov = inv(dot(transpose(rvec), rvec))
except (LinAlgError, ValueError):
cov = None
for par in self.params.values():
par.stderr, par.correl = 0, None
self.covar = cov
if cov is None:
self.errorbars = False
self.message = "%s. Could not estimate error-bars"
else:
self.errorbars = True
if self.scale_covar:
self.covar = cov = cov * sum_sqr / self.nfree
for ivar, varname in enumerate(self.var_map):
par = self.params[varname]
par.stderr = sqrt(cov[ivar, ivar])
par.correl = {}
for jvar, varn2 in enumerate(self.var_map):
if jvar != ivar:
par.correl[varn2] = cov[ivar, jvar] / (par.stderr * sqrt(cov[jvar, jvar]))
# set uncertainties on constrained parameters.
# Note that first we set all named params to
# have values that include uncertainties, then
# evaluate all constrained parameters, then set
# the values back to the nominal values.
if HAS_UNCERT and self.covar is not None:
uvars = uncertainties.correlated_values(vbest, self.covar)
for v, nam in zip(uvars, self.var_map):
self.asteval.symtable[nam] = v
for pname, par in self.params.items():
if hasattr(par, "ast"):
try:
out = self.asteval.run(par.ast)
par.stderr = out.std_dev()
except:
pass
for v, nam in zip(uvars, self.var_map):
self.asteval.symtable[nam] = v.nominal_value
for par in self.params.values():
if hasattr(par, "ast"):
delattr(par, "ast")
return self.success
labels = ['435.8 nm', '546.1 nm', '577.1 nm', '579.1 nm']
for i, x_range, p0, label in enum(x_ranges, p0s, labels):
x_fit, fit_peak, c1 = bw_fit(x, y_e, x_range, p0, fit=True)
x0s.append(c1[0])
As.append(c1[2])
lits = [435.8, 546.1, 577.1, 579.1]
for i, x0, lit in enum(x0s, lits):
print("\cellcolor{LightCyan}$%i$ & $%s$ & $%.1f$ \\\\"%(
i+1, uc_str(x0), lit))
# Linear fit on peaks
x0 = un.nominal_values(x0s)
s_x0 = un.std_devs(x0s)
lit_peaks = np.array([435.8, 546.1, 577.1, 579.1])
coeff_lin, cov_lin = curve_fit(linear, lit_peaks, x0, p0=None,
sigma=np.sqrt(s_x0), absolute_sigma=True)
c_lin = uc.correlated_values(coeff_lin, cov_lin)
# Switch to lambda(x0) = lit_peak(x0)
d_lin = np.array([1 / c_lin[0], -c_lin[1] / c_lin[0]])
np.save(npy_dir + 'ccd_calibration', d_lin)
# Detection probability
filename = "ccd_white_pol0"
t, avg, x, y0, y_e0 = get_ccd_data(filename)
filename = "ccd_white_pol45"
t, avg, x, y45, y_e45 = get_ccd_data(filename)
filename = "ccd_white_pol90"
t, avg, x, y90, y_e90 = get_ccd_data(filename)
# Correlation factor:
corr0 = y45 / y0
corr90 = y45 / y90
# remove one outlier:
return np.arctan(f * 2 * np.pi * RC)
phi_ = a / (1 / f) * 2 * np.pi
A_ = U / U0
maketable(
(f.astype(int), unp.nominal_values(U), unp.nominal_values(U0), A_, unp.nominal_values(a * 1000), phi_),
"build/daten.txt",
)
paramsa, pcova = curve_fit(A, f, unp.nominal_values(A_), p0=[1 / 742], sigma=unp.std_devs(A_), absolute_sigma=True)
paramsb, pcovb = curve_fit(
phi, f, unp.nominal_values(phi_), p0=[1 / 742], sigma=unp.std_devs(phi_), absolute_sigma=True
)
paramsa_u = unc.correlated_values(paramsa, pcova)
paramsb_u = unc.correlated_values(paramsb, pcovb)
maketable([paramsa_u], "build/b1.txt", True)
maketable([paramsb_u], "build/b2.txt", True)
x = np.linspace(0.2, 10000, 100000)
# plt.fill_between(x, A(x, paramsa_u[0].n - paramsa_u[0].s*10), A(x, paramsa_u[0].n + paramsa_u[0].s*10), facecolor='blue', alpha=0.25, edgecolor='none', label=r'$1\sigma$-Umgebung ($\times 10$)')
plt.plot(x, A(x, *paramsa), "b-", label="Fit")
plt.errorbar(f, unp.nominal_values(A_), yerr=unp.std_devs(A_), fmt="rx", label="Messdaten")
plt.xlabel(r"$\nu/\si{\hertz}")
plt.ylabel(r"$U/U0$")
plt.xlim(4, 11000)
plt.legend(loc="best")
plt.xscale("log")
plt.savefig("build/b1.pdf")
def autobk(energy, mu=None, group=None, rbkg=1, nknots=None, e0=None,
edge_step=None, kmin=0, kmax=None, kweight=1, dk=0,
win='hanning', k_std=None, chi_std=None, nfft=2048, kstep=0.05,
pre_edge_kws=None, nclamp=4, clamp_lo=1, clamp_hi=1,
calc_uncertainties=False, _larch=None, **kws):
"""Use Autobk algorithm to remove XAFS background
Parameters:
-----------
energy: 1-d array of x-ray energies, in eV, or group
mu: 1-d array of mu(E)
group: output group (and input group for e0 and edge_step).
rbkg: distance (in Ang) for chi(R) above
which the signal is ignored. Default = 1.
e0: edge energy, in eV. If None, it will be determined.
edge_step: edge step. If None, it will be determined.
pre_edge_kws: keyword arguments to pass to pre_edge()
nknots: number of knots in spline. If None, it will be determined.
kmin: minimum k value [0]
kmax: maximum k value [full data range].
kweight: k weight for FFT. [1]
dk: FFT window window parameter. [0]
win: FFT window function name. ['hanning']
nfft: array size to use for FFT [2048]
kstep: k step size to use for FFT [0.05]
k_std: optional k array for standard chi(k).
chi_std: optional chi array for standard chi(k).
nclamp: number of energy end-points for clamp [2]
clamp_lo: weight of low-energy clamp [1]
clamp_hi: weight of high-energy clamp [1]
calc_uncertaintites: Flag to calculate uncertainties in
mu_0(E) and chi(k) [False]
Output arrays are written to the provided group.
Follows the 'First Argument Group' convention.
"""
msg = _larch.writer.write
if 'kw' in kws:
kweight = kws.pop('kw')
if len(kws) > 0:
msg('Unrecognized a:rguments for autobk():\n')
msg(' %s\n' % (', '.join(kws.keys())))
return
energy, mu, group = parse_group_args(energy, members=('energy', 'mu'),
defaults=(mu,), group=group,
fcn_name='autobk')
energy = remove_dups(energy)
# if e0 or edge_step are not specified, get them, either from the
# passed-in group or from running pre_edge()
group = set_xafsGroup(group, _larch=_larch)
if edge_step is None and isgroup(group, 'edge_step'):
edge_step = group.edge_step
if e0 is None and isgroup(group, 'e0'):
e0 = group.e0
if e0 is None or edge_step is None:
# need to run pre_edge:
pre_kws = dict(nnorm=3, nvict=0, pre1=None,
pre2=-50., norm1=100., norm2=None)
if pre_edge_kws is not None:
pre_kws.update(pre_edge_kws)
pre_edge(energy, mu, group=group, _larch=_larch, **pre_kws)
if e0 is None:
e0 = group.e0
if edge_step is None:
edge_step = group.edge_step
if e0 is None or edge_step is None:
msg('autobk() could not determine e0 or edge_step!: trying running pre_edge first\n')
return
# get array indices for rkbg and e0: irbkg, ie0
ie0 = index_of(energy, e0)
rgrid = np.pi/(kstep*nfft)
if rbkg < 2*rgrid: rbkg = 2*rgrid
irbkg = int(1.01 + rbkg/rgrid)
# save ungridded k (kraw) and grided k (kout)
# and ftwin (*k-weighting) for FT in residual
enpe = energy[ie0:] - e0
kraw = np.sign(enpe)*np.sqrt(ETOK*abs(enpe))
if kmax is None:
kmax = max(kraw)
else:
kmax = max(0, min(max(kraw), kmax))
kout = kstep * np.arange(int(1.01+kmax/kstep), dtype='float64')
iemax = min(len(energy), 2+index_of(energy, e0+kmax*kmax/ETOK)) - 1
# interpolate provided chi(k) onto the kout grid
if chi_std is not None and k_std is not None:
chi_std = np.interp(kout, k_std, chi_std)
# pre-load FT window
ftwin = kout**kweight * ftwindow(kout, xmin=kmin, xmax=kmax,
window=win, dx=dk)
# calc k-value and initial guess for y-values of spline params
nspl = max(4, min(128, 2*int(rbkg*(kmax-kmin)/np.pi) + 1))
spl_y, spl_k, spl_e = np.zeros(nspl), np.zeros(nspl), np.zeros(nspl)
for i in range(nspl):
q = kmin + i*(kmax-kmin)/(nspl - 1)
ik = index_nearest(kraw, q)
i1 = min(len(kraw)-1, ik + 5)
i2 = max(0, ik - 5)
spl_k[i] = kraw[ik]
spl_e[i] = energy[ik+ie0]
spl_y[i] = (2*mu[ik+ie0] + mu[i1+ie0] + mu[i2+ie0] ) / 4.0
# get spline represention: knots, coefs, order=3
# coefs will be varied in fit.
knots, coefs, order = splrep(spl_k, spl_y)
# set fit parameters from initial coefficients
params = Group()
for i in range(len(coefs)):
name = FMT_COEF % i
p = Parameter(coefs[i], name=name, vary=i<len(spl_y))
p._getval()
setattr(params, name, p)
initbkg, initchi = spline_eval(kraw[:iemax-ie0+1], mu[ie0:iemax+1],
knots, coefs, order, kout)
# do fit
fit = Minimizer(__resid, params, _larch=_larch, toler=1.e-4,
fcn_kws = dict(ncoefs=len(coefs), chi_std=chi_std,
knots=knots, order=order,
kraw=kraw[:iemax-ie0+1],
mu=mu[ie0:iemax+1], irbkg=irbkg, kout=kout,
ftwin=ftwin, kweight=kweight,
nfft=nfft, nclamp=nclamp,
clamp_lo=clamp_lo, clamp_hi=clamp_hi))
fit.leastsq()
# write final results
coefs = [getattr(params, FMT_COEF % i) for i in range(len(coefs))]
bkg, chi = spline_eval(kraw[:iemax-ie0+1], mu[ie0:iemax+1],
knots, coefs, order, kout)
obkg = np.copy(mu)
obkg[ie0:ie0+len(bkg)] = bkg
# outputs to group
group = set_xafsGroup(group, _larch=_larch)
group.bkg = obkg
group.chie = (mu-obkg)/edge_step
group.k = kout
group.chi = chi/edge_step
# now fill in 'autobk_details' group
params.init_bkg = np.copy(mu)
params.init_bkg[ie0:ie0+len(bkg)] = initbkg
params.init_chi = initchi/edge_step
params.knots_e = spl_e
params.knots_y = np.array([coefs[i] for i in range(nspl)])
params.init_knots_y = spl_y
params.nfev = params.fit_details.nfev
params.kmin = kmin
params.kmax = kmax
group.autobk_details = params
# uncertainties in mu0 and chi: fairly slow!!
if HAS_UNCERTAIN and calc_uncertainties:
vbest, vstd = [], []
for n in fit.var_names:
par = getattr(params, n)
vbest.append(par.value)
vstd.append(par.stderr)
uvars = uncertainties.correlated_values(vbest, params.covar)
# uncertainty in bkg (aka mu0)
# note that much of this is working around
# limitations in the uncertainty package that make it
# 1. take an argument list (not array)
# 2. work on returned scalars (but not arrays)
# 3. not handle kw args and *args well (so use
# of global "index" is important here)
nkx = iemax-ie0 + 1
def my_dsplev(*args):
coefs = np.array(args)
return splev(kraw[:nkx], [knots, coefs, order])[index]
fdbkg = uncertainties.wrap(my_dsplev)
dmu0 = [fdbkg(*uvars).std_dev() for index in range(len(bkg))]
group.delta_bkg = np.zeros(len(mu))
group.delta_bkg[ie0:ie0+len(bkg)] = np.array(dmu0)
# uncertainty in chi (see notes above)
def my_dchi(*args):
coefs = np.array(args)
b,chi = spline_eval(kraw[:nkx], mu[ie0:iemax+1],
knots, coefs, order, kout)
return chi[index]
fdchi = uncertainties.wrap(my_dchi)
dchi = [fdchi(*uvars).std_dev() for index in range(len(kout))]
group.delta_chi = np.array(dchi)/edge_step
save_tab = 1
plt.close('all')
fig_dir = '../figures/'
tab_dir = '../tables/'
tab_name = "b_I"
input_dir = "../data/"
output_dir = input_dir
colors = ['b', 'g', 'r', 'pink']
b, I = csv_to_npy(1)
b2, I2 = csv_to_npy(2)
# least square fit for b(I) (polyfit of deg = 1)
i_max = 8
coeff, cov = np.polyfit(I[:i_max], b[:i_max], deg=1, cov=True)
c = uc.correlated_values(coeff, cov)
Is = np.linspace(0, 6, 100)
f1 = open("coefficients.tex", "w+")
var_names = ["p_0", "p_1"]
la_coeff(f1, coeff, cov, var_names, additional_digits=2)
f1.close()
# plot B(I) with error bars
fig1, ax1 = plt.subplots(1,1, figsize = (8.09,5))
b_error = 5 # uncertainty on B measurement, taken to be the last significant digit
I_error = 0.01 # uncertainty in measuring the current I
ax1.fill_between(Is,
unv(np.polyval(c, Is)) + usd(np.polyval(c, Is)),
unv(np.polyval(c, Is)) - usd(np.polyval(c, Is)),
facecolor=colors[0], color=colors[0], alpha=0.2)
def f(a,b,c):
return ( b * a ) + c
parameters1, pcov = curve_fit(f, a, dx)
a_plot = np.linspace(0.02,0.18)
plt.xlim(0.02,0.18)
plt.plot(a_plot,f(a_plot,*parameters1), 'g-', label='Fit')
plt.plot(a,dx, 'rx', label='Messwerte')
plt.xlabel(r'$4 x^3 - 12 L x^2 + 9 L^2 x - L^3 / m^3$')
plt.ylabel(r'$D(x) / m$')
plt.tight_layout()
plt.legend(loc='best')
plt.savefig('stab1_beidseitig_rechts.pdf')
parameters1 = correlated_values(parameters1, pcov)
for param1 in parameters1:
print(param1)
print()
print(parameters1)
print(pcov)
#Ausgabe:
#0.01207+/-0.00006
#(4.8+/-0.8)e-05
#
#(0.012074401751652291+/-5.565018647514912e-05, 4.8030418172796886e-05+/-8.120504158407705e-06)
#[[ 3.09694325e-09 -4.34868178e-10]
# [ -4.34868178e-10 6.59425878e-11]]
#Elasitzitätsmodul:
def gaussian_sum_moments(F, sigma, x, y, cov_matrix, shift=0.5):
"""Compute image moments with uncertainties for sum of Gaussians.
The moments are computed analytically, the formulae are documented below.
Calls ``uncertainties.correlated_values`` to propagate the errors.
Parameters
----------
F : array
Integral norms of the Gaussian components.
sigmas : array
Widths of the Gaussian components.
x : array
x positions of the Gaussian components.
y : array
y positions of the Gaussian components.
cov_matrix : array
Covariance matrix of the parameters. The columns have to follow the order:
[sigma_1, x_1, y_1, F_1, sigma_2, x_2, y_2, F_2, ..., sigma_N, x_N, y_N, F_N]
shift : float (default = 0.5)
Depending on where the image values are given, the grid has to be
shifted. If the values are given at the center of the pixel
shift = 0.5.
Returns
-------
nominal_values : list
List of image moment nominal values:
[F_sum, x_sum, y_sum, x_sigma, y_sigma, sqrt(x_sigma * y_sigma)]
All values are given in pixel coordinates.
std_devs : list
List of image moment standard deviations.
Examples
--------
A simple example for an image consisting of three Gaussians
with zero covariance matrix:
>>> import numpy as np
>>> from gammapy.image.models.gauss import gaussian_sum_moments
>>> cov_matrix = np.zeros((12, 12))
>>> F = [100, 200, 300]
>>> sigma = [15, 10, 5]
>>> x = [100, 120, 70]
>>> y = [100, 90, 120]
>>> nominal_values, std_devs = gaussian_sum_moments(F, sigma, x, y, cov_matrix)
Notes
-----
The 0th moment (total flux) is given by:
.. math::
F_{\\Sigma} = \\int_{-\\infty}^{\\infty}f_{\\Sigma}(x, y)dx dy =
\\sum_i^N F_i
The 1st moments (position) are given by:
.. math::
x_{\\Sigma} = \\frac{1}{F_{\\Sigma}} \\int_{-\\infty}^{\\infty}x
f_{\\Sigma}(x, y)dx dy = \\frac{1}{F_{\\Sigma}}\\sum_i^N x_iF_i
y_{\\Sigma} = \\frac{1}{F_{\\Sigma}} \\int_{-\\infty}^{\\infty}y
f_{\\Sigma}(x, y)dx dy = \\frac{1}{F_{\\Sigma}}\\sum_i^N y_iF_i
The 2nd moments (extension) are given by:
.. math::
\\sigma_{\\Sigma_x}^2 = \\frac{1}{F_{\\Sigma}} \\sum_i^N F_i
\\cdot (\\sigma_i^2 + x_i^2) - x_{\\Sigma}^2
\\sigma_{\\Sigma_y}^2 = \\frac{1}{F_{\\Sigma}} \\sum_i^N F_i
\\cdot (\\sigma_i^2 + y_i^2) - y_{\\Sigma}^2
"""
import uncertainties
# Check input arrays
if len(F) != len(sigma) or len(F) != len(x) or len(F) != len(x):
raise Exception("Input arrays have to have the same size")
# Order parameter values
values = []
for i in range(len(F)):
values += [sigma[i], x[i], y[i], F[i]]
# Set up parameters with uncertainties
parameter_list = uncertainties.correlated_values(values, cov_matrix)
# Reorder parameters by splitting into 4-tuples
parameters = list(zip(*[iter(parameter_list)] * 4))
def zero_moment(parameters):
"""0th moment of the sum of Gaussian components."""
F_sum = 0
for component in parameters:
F_sum += component[3]
return F_sum
def first_moment(parameters, F_sum, shift):
"""1st moment of the sum of Gaussian components."""
x_sum, y_sum = 0, 0
for component in parameters:
x_sum += (component[1] + shift) * component[3]
y_sum += (component[2] + shift) * component[3]
return x_sum / F_sum, y_sum / F_sum
def second_moment(parameters, F_sum, x_sum, y_sum, shift):
"""2nd moment of the sum of Gaussian components."""
var_x_sum, var_y_sum = 0, 0
for p in parameters:
var_x_sum += ((p[1] + shift) ** 2 + p[0] ** 2) * p[3]
var_y_sum += ((p[2] + shift) ** 2 + p[0] ** 2) * p[3]
return var_x_sum / F_sum - x_sum ** 2, var_y_sum / F_sum - y_sum ** 2
# Compute moments
F_sum = zero_moment(parameters)
x_sum, y_sum = first_moment(parameters, F_sum, shift)
var_x_sum, var_y_sum = second_moment(parameters, F_sum, x_sum, y_sum, shift)
# Return values and stddevs separately
values = [F_sum, x_sum, y_sum, var_x_sum ** 0.5, var_y_sum ** 0.5, (var_x_sum * var_y_sum) ** 0.25]
nominal_values = [_.nominal_value for _ in values]
std_devs = [float(_.std_dev) for _ in values]
return nominal_values, std_devs