def test_simulate_highest_outlier_works(self):
m = 1
nfreq = 100000
seed = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(seed)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
nsim = 10
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
s_all = np.atleast_2d(np.ones(nsim) * 2.0).T
pe = PSDParEst(ps)
res = pe.fit(loglike, [2.0], neg=True)
maxpow_sim = pe.simulate_highest_outlier(s_all, loglike, [2.0],
max_post=False, seed=seed)
assert maxpow_sim.shape[0] == nsim
assert np.all(maxpow_sim > 20.00) and np.all(maxpow_sim < 31.0)
def test_calibrate_highest_outlier_works_with_mvn(self):
m = 1
nfreq = 10000
seed = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(seed)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
nsim = 10
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
pe = PSDParEst(ps)
pval = pe.calibrate_highest_outlier(loglike, [2.0], sample=None,
max_post=False, seed=seed,
nsim=nsim)
assert pval > 0.001
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.arange(nfreq)
noise = np.random.exponential(size=nfreq)
power = noise * 2.0
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude": p_amplitude}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power, cls.model,
m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
def test_compute_highest_outlier_works(self):
mp_ind = 5
max_power = 1000.0
ps = Powerspectrum()
ps.freq = np.arange(10)
ps.power = np.ones_like(ps.freq)
ps.power[mp_ind] = max_power
ps.m = 1
ps.df = ps.freq[1]-ps.freq[0]
ps.norm = "leahy"
model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=1.0, scale=1.0).pdf(
amplitude)
priors = {"amplitude": p_amplitude}
lpost = PSDPosterior(ps.freq, ps.power, model, 1)
lpost.logprior = set_logprior(lpost, priors)
pe = PSDParEst(ps)
res = pe.fit(lpost, [1.0])
res.mfit = np.ones_like(ps.freq)
max_y, max_x, max_ind = pe._compute_highest_outlier(lpost, res)
assert np.isclose(max_y[0], 2*max_power)
assert np.isclose(max_x[0], ps.freq[mp_ind])
assert max_ind == mp_ind
def test_calibrate_lrt_works_with_mvn(self):
m = 1
nfreq = 10000
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(100)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
model2 = models.PowerLaw1D() + models.Const1D()
model2.x_0_0.fixed = True
loglike2 = PSDLogLikelihood(ps.freq, ps.power, model2, 1)
pe = PSDParEst(ps)
pval = pe.calibrate_lrt(loglike, [2.0], loglike2,
[2.0, 1.0, 2.0], sample=None,
max_post=False, nsim=10,
seed=100)
assert pval > 0.001
def test_generate_data_produces_correct_distribution(self):
model = models.Const1D()
model.amplitude = 2.0
p = model(self.ps.freq)
seed = 100
rng = np.random.RandomState(seed)
noise = rng.exponential(size=len(p))
power = noise*p
ps = Powerspectrum()
ps.freq = self.ps.freq
ps.power = power
ps.m = 1
ps.df = self.ps.freq[1]-self.ps.freq[0]
ps.norm = "leahy"
lpost = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
pe = PSDParEst(ps)
rng2 = np.random.RandomState(seed)
sim_data = pe._generate_data(lpost, [2.0], rng2)
assert np.allclose(ps.power, sim_data.power)
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.arange(nfreq)
noise = np.random.exponential(size=nfreq)
power = noise * 2.0
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude": p_amplitude}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power,
cls.model, m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [2.0]
cls.neg = True
cls.opt = scipy.optimize.minimize(cls.lpost, cls.t0,
method=cls.fitmethod,
args=cls.neg, tol=1.e-10)
def setup_class(cls):
cls.m = 10
nfreq = 1000000
freq = np.arange(nfreq)
noise = scipy.stats.chi2(2.*cls.m).rvs(size=nfreq)/np.float(cls.m)
power = noise
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = cls.m
ps.df = freq[1]-freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude":p_amplitude}
def test_calibrate_lrt_works_with_sampling(self):
m = 1
nfreq = 10000
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(100)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
lpost = PSDPosterior(ps.freq, ps.power, model, m=1)
p_amplitude_1 = lambda amplitude: \
scipy.stats.norm(loc=2.0, scale=1.0).pdf(amplitude)
p_alpha_0 = lambda alpha: \
scipy.stats.uniform(0.0, 5.0).pdf(alpha)
p_amplitude_0 = lambda amplitude: \
scipy.stats.norm(loc=self.a2_mean, scale=self.a2_var).pdf(
amplitude)
priors = {"amplitude": p_amplitude_1}
priors2 = {"amplitude_1": p_amplitude_1,
"amplitude_0": p_amplitude_0,
"alpha_0": p_alpha_0}
lpost.logprior = set_logprior(lpost, priors)
model2 = models.PowerLaw1D() + models.Const1D()
model2.x_0_0.fixed = True
lpost2 = PSDPosterior(ps.freq, ps.power, model2, 1)
lpost2.logprior = set_logprior(lpost2, priors2)
pe = PSDParEst(ps)
pval = pe.calibrate_lrt(lpost, [2.0], lpost2,
[2.0, 1.0, 2.0], sample=None,
max_post=True, nsim=10, nwalkers=100,
burnin=100, niter=20,
seed=100)
assert pval > 0.001
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.arange(nfreq)
noise = np.random.exponential(size=nfreq)
power = noise * 2.0
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(
amplitude)
cls.priors = {"amplitude": p_amplitude}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power,
cls.model, m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [2.0]
cls.neg = True
pe = ParameterEstimation()
res = pe.fit(cls.lpost, cls.t0)
cls.nwalkers = 100
cls.niter = 200
np.random.seed(200)
p0 = np.array(
[np.random.multivariate_normal(res.p_opt, res.cov) for
i in range(cls.nwalkers)])
cls.sampler = emcee.EnsembleSampler(cls.nwalkers,
len(res.p_opt), cls.lpost,
args=[False], threads=1)
_, _, _ = cls.sampler.run_mcmc(p0, cls.niter)
def test_plotfits_log_pow(self):
ps = Powerspectrum()
ps.freq = self.ps.freq
ps.power = self.ps.power
ps.m = self.ps.m
ps.df = self.ps.df
ps.norm = "none"
pe = PSDParEst(ps)
t0 = [2.0, 1, 1, 1]
res = pe.fit(self.lpost, t0)
pe.plotfits(res, res2=res, save_plot=True, log=True)
assert os.path.exists("test_ps_fit.png")
os.unlink("test_ps_fit.png")
def test_find_highest_outlier_works_as_expected(self):
mp_ind = 5
max_power = 1000.0
ps = Powerspectrum()
ps.freq = np.arange(10)
ps.power = np.ones_like(ps.freq)
ps.power[mp_ind] = max_power
ps.m = 1
ps.df = ps.freq[1]-ps.freq[0]
ps.norm = "leahy"
pe = PSDParEst(ps)
max_x, max_ind = pe._find_outlier(ps.freq, ps.power, max_power)
assert np.isclose(max_x, ps.freq[mp_ind])
assert max_ind == mp_ind
def test_fitting_with_ties_and_bounds(self, capsys):
double_f = lambda model : model.x_0_0 * 2
model = self.model.copy()
model += models.Lorentz1D(amplitude=model.amplitude_0,
x_0 = model.x_0_0 * 2,
fwhm = model.fwhm_0)
model.x_0_0 = self.model.x_0_0
model.amplitude_0 = self.model.amplitude_0
model.amplitude_1 = self.model.amplitude_1
model.fwhm_0 = self.model.fwhm_0
model.x_0_2.tied = double_f
model.fwhm_0.bounds = [0, 10]
model.amplitude_0.fixed = True
p = model(self.ps.freq)
noise = np.random.exponential(size=len(p))
power = noise*p
ps = Powerspectrum()
ps.freq = self.ps.freq
ps.power = power
ps.m = self.ps.m
ps.df = self.ps.df
ps.norm = "leahy"
pe = PSDParEst(ps, fitmethod="TNC")
llike = PSDLogLikelihood(ps.freq, ps.power, model)
true_pars = [self.x_0_0, self.fwhm_0,
self.amplitude_1,
model.amplitude_2.value,
model.fwhm_2.value]
res = pe.fit(llike, true_pars, neg=True)
compare_pars = [self.x_0_0, self.fwhm_0,
self.amplitude_1,
model.amplitude_2.value,
model.fwhm_2.value]
assert np.allclose(compare_pars, res.p_opt, rtol=0.5)
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.arange(nfreq)
noise = np.random.exponential(size=nfreq)
power = noise * 2.0
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude": p_amplitude}
cls.lpost = PSDPosterior(cls.ps.freq,
cls.ps.power,
cls.model,
m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [2.0]
cls.neg = True
cls.opt = scipy.optimize.minimize(cls.lpost,
cls.t0,
method=cls.fitmethod,
args=cls.neg,
tol=1.e-10)
def setup_class(cls):
m = 1
nfreq = 1000000
freq = np.arange(nfreq)
noise = np.random.exponential(size=nfreq)
power = noise * 2.0
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude": p_amplitude}
def test_simulate_lrts_works(self):
m = 1
nfreq = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(100)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
s_all = np.atleast_2d(np.ones(5) * 2.0).T
model2 = models.PowerLaw1D() + models.Const1D()
model2.x_0_0.fixed = True
loglike2 = PSDLogLikelihood(ps.freq, ps.power, model2, 1)
pe = PSDParEst(ps)
lrt_obs, res1, res2 = pe.compute_lrt(loglike, [2.0], loglike2,
[2.0, 1.0, 2.0], neg=True)
lrt_sim = pe.simulate_lrts(s_all, loglike, [2.0], loglike2,
[2.0, 1.0, 2.0],
seed=100)
assert (lrt_obs > 0.4) and (lrt_obs < 0.6)
assert np.all(lrt_sim < 10.0) and np.all(lrt_sim > 0.01)
def test_calibrate_lrt_works_as_expected(self):
m = 1
nfreq = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(100)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
s_all = np.atleast_2d(np.ones(10) * 2.0).T
model2 = models.PowerLaw1D() + models.Const1D()
model2.x_0_0.fixed = True
loglike2 = PSDLogLikelihood(ps.freq, ps.power, model2, 1)
pe = PSDParEst(ps)
pval = pe.calibrate_lrt(loglike, [2.0],
loglike2, [2.0, 1.0, 2.0],
sample=s_all,
max_post=False,
nsim=5,
seed=100)
assert pval > 0.001
def test_compute_lrt_works(self):
m = 1
nfreq = 100000
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(100)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
s_all = np.atleast_2d(np.ones(10) * 2.0).T
model2 = models.PowerLaw1D() + models.Const1D()
model2.x_0_0.fixed = True
loglike2 = PSDLogLikelihood(ps.freq, ps.power, model2, 1)
pe = PSDParEst(ps)
lrt_obs, res1, res2 = pe.compute_lrt(loglike, [2.0], loglike2,
[2.0, 1.0, 2.0], neg=True)
lrt_sim = pe.simulate_lrts(s_all, loglike, [2.0], loglike2,
[2.0, 1.0, 2.0],
seed=100)
assert (lrt_obs > 0.4) and (lrt_obs < 0.6)
assert np.all(lrt_sim < 10.0) and np.all(lrt_sim > 0.01)
def test_calibrate_highest_outlier_works_with_sampling(self):
m = 1
nfreq = 100000
seed = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(seed)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
nsim = 10
lpost = PSDPosterior(ps.freq, ps.power, model, m=1)
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=1.0, scale=1.0).pdf(
amplitude)
priors = {"amplitude": p_amplitude}
lpost.logprior = set_logprior(lpost, priors)
pe = PSDParEst(ps)
pval = pe.calibrate_highest_outlier(lpost, [2.0], sample=None,
max_post=True, seed=seed,
nsim=nsim, niter=20, nwalkers=100,
burnin=100)
assert pval > 0.001
def setup_class(cls):
cls.m = 10
nfreq = 1000000
freq = np.arange(nfreq)
noise = scipy.stats.chi2(2. * cls.m).rvs(size=nfreq) / np.float(cls.m)
power = noise
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = cls.m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.model = models.Const1D()
p_amplitude = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
cls.priors = {"amplitude": p_amplitude}
def test_simulate_highest_outlier_works(self):
m = 1
nfreq = 100000
seed = 100
freq = np.linspace(1, 10, nfreq)
rng = np.random.RandomState(seed)
noise = rng.exponential(size=nfreq)
model = models.Const1D()
model.amplitude = 2.0
p = model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
nsim = 10
loglike = PSDLogLikelihood(ps.freq, ps.power, model, m=1)
s_all = np.atleast_2d(np.ones(nsim) * 2.0).T
pe = PSDParEst(ps)
res = pe.fit(loglike, [2.0], neg=True)
maxpow_sim = pe.simulate_highest_outlier(s_all,
loglike, [2.0],
max_post=False,
seed=seed)
assert maxpow_sim.shape[0] == nsim
assert np.all(maxpow_sim > 20.00) and np.all(maxpow_sim < 31.0)
def setup_class(cls):
m = 1
nfreq = 100
freq = np.linspace(0, 10.0, nfreq + 1)[1:]
rng = np.random.RandomState(100) # set the seed for the random number generator
noise = rng.exponential(size=nfreq)
cls.model = models.Lorentz1D() + models.Const1D()
cls.x_0_0 = 2.0
cls.fwhm_0 = 0.05
cls.amplitude_0 = 1000.0
cls.amplitude_1 = 2.0
cls.model.x_0_0 = cls.x_0_0
cls.model.fwhm_0 = cls.fwhm_0
cls.model.amplitude_0 = cls.amplitude_0
cls.model.amplitude_1 = cls.amplitude_1
p = cls.model(freq)
np.random.seed(400)
power = noise*p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1]-freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.a2_mean, cls.a2_var = 100.0, 10.0
p_amplitude_1 = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
p_x_0_0 = lambda alpha: \
scipy.stats.uniform(0.0, 5.0).pdf(alpha)
p_fwhm_0 = lambda alpha: \
scipy.stats.uniform(0.0, 0.5).pdf(alpha)
p_amplitude_0 = lambda amplitude: \
scipy.stats.norm(loc=cls.a2_mean, scale=cls.a2_var).pdf(amplitude)
cls.priors = {"amplitude_1": p_amplitude_1,
"amplitude_0": p_amplitude_0,
"x_0_0": p_x_0_0,
"fwhm_0": p_fwhm_0}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power,
cls.model, m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "powell"
cls.max_post = True
cls.t0 = [cls.x_0_0, cls.fwhm_0, cls.amplitude_0, cls.amplitude_1]
cls.neg = True
# make compound model plc = pl + c # parameters for fake data. alpha = 2.0 amplitude = 5.0 white_noise = 2.0 freq = np.linspace(0.01, 10.0, int(10.0 / 0.01)) from astropy.modeling.fitting import _fitter_to_model_params _fitter_to_model_params(plc, [amplitude, alpha, white_noise]) psd_shape = plc(freq) powers = psd_shape * np.random.chisquare(2, size=psd_shape.shape[0]) / 2.0 ps = Powerspectrum() ps.freq = freq ps.power = powers ps.df = ps.freq[1] - ps.freq[0] ps.m = 1 loglike = PSDLogLikelihood(ps.freq, ps.power, plc, m=ps.m) test_pars = [1, 5, 100] parest = PSDParEst(ps, fitmethod="L-BFGS-B", max_post=True) # flat prior for the power law index p_alpha = lambda alpha: ((-1. <= alpha) & (alpha <= 5.)) # flat prior for the power law amplitude p_amplitude = lambda amplitude: ((0.01 <= amplitude) & (amplitude <= 10.0)) # normal prior for the white noise parameter p_whitenoise = lambda white_noise: scipy.stats.norm(2.0, 0.1).pdf(white_noise)
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.linspace(1, 1000, nfreq)
np.random.seed(100) # set the seed for the random number generator
noise = np.random.exponential(size=nfreq)
cls.model = models.PowerLaw1D() + models.Const1D()
cls.model.x_0_0.fixed = True
cls.alpha_0 = 2.0
cls.amplitude_0 = 100.0
cls.amplitude_1 = 2.0
cls.model.alpha_0 = cls.alpha_0
cls.model.amplitude_0 = cls.amplitude_0
cls.model.amplitude_1 = cls.amplitude_1
p = cls.model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.a2_mean, cls.a2_var = 100.0, 10.0
p_amplitude_1 = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
p_alpha_0 = lambda alpha: \
scipy.stats.uniform(0.0, 5.0).pdf(alpha)
p_amplitude_0 = lambda amplitude: \
scipy.stats.norm(loc=cls.a2_mean, scale=cls.a2_var).pdf(
amplitude)
cls.priors = {
"amplitude_1": p_amplitude_1,
"amplitude_0": p_amplitude_0,
"alpha_0": p_alpha_0
}
cls.lpost = PSDPosterior(cls.ps, cls.model)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [cls.amplitude_0, cls.alpha_0, cls.amplitude_1]
cls.neg = True
cls.opt = scipy.optimize.minimize(cls.lpost,
cls.t0,
method=cls.fitmethod,
args=cls.neg,
tol=1.e-5)
cls.optres = OptimizationResultsSubclassDummy(cls.lpost,
cls.opt,
neg=True)
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.linspace(1, 10.0, nfreq)
rng = np.random.RandomState(100) # set the seed for the random number generator
noise = rng.exponential(size=nfreq)
cls.model = models.Lorentz1D() + models.Const1D()
cls.x_0_0 = 2.0
cls.fwhm_0 = 0.1
cls.amplitude_0 = 100.0
cls.amplitude_1 = 2.0
cls.model.x_0_0 = cls.x_0_0
cls.model.fwhm_0 = cls.fwhm_0
cls.model.amplitude_0 = cls.amplitude_0
cls.model.amplitude_1 = cls.amplitude_1
p = cls.model(freq)
np.random.seed(400)
power = noise*p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1]-freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.a2_mean, cls.a2_var = 100.0, 10.0
p_amplitude_1 = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
p_x_0_0 = lambda alpha: \
scipy.stats.uniform(0.0, 5.0).pdf(alpha)
p_fwhm_0 = lambda alpha: \
scipy.stats.uniform(0.0, 0.5).pdf(alpha)
p_amplitude_0 = lambda amplitude: \
scipy.stats.norm(loc=cls.a2_mean, scale=cls.a2_var).pdf(amplitude)
cls.priors = {"amplitude_1": p_amplitude_1,
"amplitude_0": p_amplitude_0,
"x_0_0": p_x_0_0,
"fwhm_0": p_fwhm_0}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power,
cls.model, m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [cls.x_0_0, cls.fwhm_0, cls.amplitude_0, cls.amplitude_1]
cls.neg = True
def setup_class(cls):
m = 1
nfreq = 100000
freq = np.linspace(1, 1000, nfreq)
np.random.seed(100) # set the seed for the random number generator
noise = np.random.exponential(size=nfreq)
cls.model = models.PowerLaw1D() + models.Const1D()
cls.model.x_0_0.fixed = True
cls.alpha_0 = 2.0
cls.amplitude_0 = 100.0
cls.amplitude_1 = 2.0
cls.model.alpha_0 = cls.alpha_0
cls.model.amplitude_0 = cls.amplitude_0
cls.model.amplitude_1 = cls.amplitude_1
p = cls.model(freq)
power = noise * p
ps = Powerspectrum()
ps.freq = freq
ps.power = power
ps.m = m
ps.df = freq[1] - freq[0]
ps.norm = "leahy"
cls.ps = ps
cls.a_mean, cls.a_var = 2.0, 1.0
cls.a2_mean, cls.a2_var = 100.0, 10.0
p_amplitude_1 = lambda amplitude: \
scipy.stats.norm(loc=cls.a_mean, scale=cls.a_var).pdf(amplitude)
p_alpha_0 = lambda alpha: \
scipy.stats.uniform(0.0, 5.0).pdf(alpha)
p_amplitude_0 = lambda amplitude: \
scipy.stats.norm(loc=cls.a2_mean, scale=cls.a2_var).pdf(
amplitude)
cls.priors = {"amplitude_1": p_amplitude_1,
"amplitude_0": p_amplitude_0,
"alpha_0": p_alpha_0}
cls.lpost = PSDPosterior(cls.ps.freq, cls.ps.power,
cls.model, m=cls.ps.m)
cls.lpost.logprior = set_logprior(cls.lpost, cls.priors)
cls.fitmethod = "BFGS"
cls.max_post = True
cls.t0 = [cls.amplitude_0, cls.alpha_0, cls.amplitude_1]
cls.neg = True
cls.opt = scipy.optimize.minimize(cls.lpost, cls.t0,
method=cls.fitmethod,
args=cls.neg, tol=1.e-5)
cls.optres = OptimizationResultsSubclassDummy(cls.lpost, cls.opt,
neg=True)