dump("sinfo2.numpoints")
res = f.fit()
if res.succeeded: print("Fit succeeded")
if not res.succeeded: print("**** ERRRR, the fit failed folks")
report("res.format()")
report("res")
from sherpa.plot import DataPlot, ModelPlot
dplot = DataPlot()
dplot.prepare(f.data)
mplot = ModelPlot()
mplot.prepare(f.data, f.model)
dplot.plot()
mplot.overplot()
savefig("data_model_c0_c2.png")
dump("f.method.name")
original_method = f.method
from sherpa.optmethods import NelderMead
f.method = NelderMead()
resn = f.fit()
print("Change in statistic: {}".format(resn.dstatval))
fit2 = Fit(d, mdl, method=NelderMead())
fit2.fit()
mdl.c1.thaw()
plt.plot(xmid, y2 / (xhi - xlo) / pha.exposure)
plt.xlabel('Energy (keV)')
plt.ylabel('Counts/sec/keV')
savefig('pha_eval_model_to_fit.png')
from sherpa.astro.plot import ModelHistogram
mplot = ModelHistogram()
mplot.prepare(pha, full)
mplot.plot()
savefig('pha_fullmodel_model.png')
from sherpa.fit import Fit
fit = Fit(pha, full)
res = fit.fit()
report('res.format()')
from sherpa.plot import ModelPlot
dplot.prepare(pha)
dplot.plot(xlog=True)
mplot2 = ModelPlot()
mplot2.prepare(pha, full)
mplot2.overplot()
savefig('pha_fullmodel_fit.png')
def multifit(star_name, data_list, model_list, silent=False):
"""A function that will fit 2 models to 2 spectra simultaneously.
This was created to fit the NaI doublets at ~3300 and ~5890 Angstroms.
:param star_name: Name of the target star
:type star_name: str
:param data_list: List of spectrum data in the form [(wave, flux), (wave, flux),...]
:type data_list: tuple
:param model_list: A list of unfit spectrum models
:type model_list: list
:param silent: If true, no plots will generate, defaults to False
:type silent: bool
:return: models that are fit to the data
:rtype: list
"""
wave1, flux1 = data_list[0]
wave2, flux2 = data_list[1]
model1 = model_list[0]
model2 = model_list[1]
name_1 = star_name + " 1"
name_2 = star_name + " 2"
d1 = Data1D(name_1, wave1, flux1)
d2 = Data1D(name_2, wave2, flux2)
dall = DataSimulFit("combined", (d1, d2))
mall = SimulFitModel("combined", (model1, model2))
# # ==========================================
# # Initial guesses
# Dataset 1
dplot1 = DataPlot()
dplot1.prepare(d1)
if silent is False:
dplot1.plot()
mplot1 = ModelPlot()
mplot1.prepare(d1, model1)
if silent is False:
dplot1.plot()
mplot1.overplot()
plt.show()
# Dataset 2
dplot2 = DataPlot()
dplot2.prepare(d2)
if silent is False:
dplot2.plot()
mplot2 = ModelPlot()
mplot2.prepare(d2, model2)
if silent is False:
dplot2.plot()
mplot2.overplot()
plt.show()
# # =========================================
# # Fitting happens here - don't break please
stat = LeastSq()
opt = LevMar()
opt.verbose = 0
opt.ftol = 1e-15
opt.xtol = 1e-15
opt.gtol = 1e-15
opt.epsfcn = 1e-15
print(opt)
vfit = Fit(dall, mall, stat=stat, method=opt)
print(vfit)
vres = vfit.fit()
print()
print()
print("Did the fit succeed? [bool]")
print(vres.succeeded)
print()
print()
print(vres.format())
# # =========================================
# # Plotting after fit
if silent is False:
# Dataset 1
fplot1 = FitPlot()
mplot1.prepare(d1, model1)
fplot1.prepare(dplot1, mplot1)
fplot1.plot()
# residual
title = "Data 1"
plt.title(title)
plt.plot(wave1, flux1 - model1(wave1))
plt.show()
# Dataset 2
fplot2 = FitPlot()
mplot2.prepare(d2, model2)
fplot2.prepare(dplot2, mplot2)
fplot2.plot()
# residual
title = "Data 2"
plt.title(title)
plt.plot(wave2, flux2 - model2(wave2))
plt.show()
# both datasets - no residuals
splot = SplitPlot()
splot.addplot(fplot1)
splot.addplot(fplot2)
plt.tight_layout()
plt.show()
return model_list
def fit(star_name, data, model, silent=False, breakdown=False):
"""A function that will fit a given multi-part model to a given spectrum.
:param star_name: Name of the target star
:type star_name: str
:param data: Spectrum data in the form (wave, flux)
:type data: tuple
:param model: An unfit spectrum model
:type model: object
:param silent: If true, no plots will generate, defaults to False
:type silent: bool
:return: model that is fit to the data
:rtype: object
"""
wave, flux = data
# %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
d = Data1D(star_name, wave, flux)
# ==========================================
# Initial guesses
# Dataset 1
dplot = DataPlot()
dplot.prepare(d)
if silent is False:
dplot.plot()
mplot = ModelPlot()
mplot.prepare(d, model)
if silent is False:
dplot.plot()
mplot.overplot()
plt.show()
# =========================================
# Fitting happens here - don't break please
start = time.time()
stat = LeastSq()
opt = LevMar()
opt.verbose = 0
opt.ftol = 1e-15
opt.xtol = 1e-15
opt.gtol = 1e-15
opt.epsfcn = 1e-15
if silent is False:
print(opt)
vfit = Fit(d, model, stat=stat, method=opt)
if silent is False:
print(vfit)
vres = vfit.fit()
if silent is False:
print()
print()
print(vres.format())
# =========================================
# Plotting after fit
# Dataset 1
if silent is False:
fplot = FitPlot()
mplot.prepare(d, model)
fplot.prepare(dplot, mplot)
fplot.plot()
# residual
plt.title(star_name)
plt.plot(wave, flux - model(wave))
# plt.xaxis(fontsize = )
plt.xlabel("Wavelength (AA)", fontsize=12)
plt.ylabel("Flux", fontsize=12)
plt.tick_params(axis="both", labelsize=12)
if silent is False:
duration = time.time() - start
print()
print("Time taken: " + str(duration))
print()
plt.show()
if breakdown is True:
params = []
cont = model[0]
if silent is False:
plt.scatter(wave, flux, marker=".", c="black")
plt.plot(wave, model(wave), c="C1")
for line in model:
if line.name[0] != "(":
if line.name == "Cont_flux":
if silent is False:
print(line)
plt.plot(wave, line(wave), linestyle="--")
else:
params.append(line)
if silent is False:
print()
print(line)
plt.plot(wave, line(wave) * cont(wave), linestyle="--")
plt.show()
return model, params
return model
# Note: can not print(dplot) as there is a problem with the fact
# the input to the data object is a list, not ndarray
# Sherpa 4.10.0
from sherpa.models.basic import Polynom1D
mdl = Polynom1D()
report("print(mdl)")
mdl.c2.thaw()
from sherpa.plot import ModelPlot
mplot = ModelPlot()
mplot.prepare(d, mdl)
dplot.plot()
mplot.overplot()
savefig("data_model_initial.png")
from sherpa.stats import LeastSq
from sherpa.optmethods import NelderMead
from sherpa.fit import Fit
f = Fit(d, mdl, stat=LeastSq(), method=NelderMead())
report("print(f)")
res = f.fit()
dump("res.succeeded")
report("res.format()")
report("res")
report("mdl")
