depths = 2e-5 + (2e-4 - 2e-5) * np.random.rand(N)
durations = 0.3 + 0.2 * np.random.rand(N)
datasets = []
for t0, depth, duration in zip(t0s, depths, durations):
ds = deepcopy(dataset)
model = np.ones_like(ds.time)
model[(ds.time < t0+duration)*(ds.time > t0-duration)] *= 1.0 - depth
ds.flux *= model
datasets.append(ds)
[pl.plot(ds.time, ds.flux, ".") for ds in datasets]
pl.savefig("data.png")
# Compute the Gaussian processes on the dataset.
gp = GaussianProcess([1e-3, 3.0, 10.])
gp.compute(dataset.time, dataset.ferr)
# Loop over true epochs.
d = 0.2
correct = []
incorrect = []
for t0, depth, duration, data in zip(t0s, depths, durations, datasets):
null = gp.lnlikelihood(data.flux - 1.0)
# Compute the correct model.
model = np.ones_like(data.time)
model[(data.time < t0+duration)*(data.time > t0-duration)] *= 1.0 - 0.0001
correct.append(gp.lnlikelihood(data.flux - model) - null)
for i, t in enumerate(data.time):
if np.abs(t0 - t) < 2*d:
pl.savefig("data.png")
t = data.time
f = data.flux
d = 0.2
x = np.linspace(-6, 0, 10)
y = np.linspace(-1.0, 10, 12)
s2n = np.zeros((len(x), len(y)))
ll = np.zeros((len(x), len(y)))
delta_ll = np.zeros((len(x), len(y)))
for ix, a in enumerate(x):
for iy, l in enumerate(y):
gp = GaussianProcess([10 ** a, 10 ** l, 1e6])
gp.compute(data.time, data.ferr)
null = gp.lnlikelihood(f - 1.0)
results = []
for i, t0 in enumerate(t):
if np.abs(t0 - truth[2]) < 2*d:
continue
model = np.ones_like(f)
model[(t < t0+d) * (t > t0-d)] *= 1.0 - 0.0001
results.append((t0, gp.lnlikelihood(f - model)))
results = np.array(results)
model = np.ones_like(f)
model[(t < truth[2]+d) * (t > truth[2]-d)] *= 1.0 - 0.0001
ll_true = gp.lnlikelihood(f - model)
mu, std = np.mean(results[:, 1]), np.std(results[:, 1])
class GPLightCurve(LightCurve):
"""
An extension to :class:`LightCurve` with a Gaussian Process likelihood
function. This does various nice things like masking NaNs and Infs and
normalizing the fluxes by the median.
:param time:
The time series in days.
:param flux:
The flux measurements in arbitrary units.
:param ferr:
The error bars on ``flux``.
:param hyperpars:
The parameters for the ``GaussianProcess`` kernel.
:param texp: (optional)
The integration time (in seconds). (default: 1626.0… Kepler
long-cadence)
:param K: (optional)
The number of bins to use in the approximate exposure time integral.
(default: 3)
"""
def __init__(self, time, flux, ferr, hyperpars, jitter=0.0, **kwargs):
if GaussianProcess is None:
raise ImportError("You need to install george to use GPs")
super(GPLightCurve, self).__init__(time, flux, ferr, **kwargs)
self._hyperpars = hyperpars
self._gp = None
self._jitter = jitter
def __getstate__(self):
return dict([(k, v) for k, v in self.__dict__.items() if k != "_gp"])
def __setstate__(self, d):
for k, v in d.items():
setattr(self, k, v)
self._gp = None
@property
def gp(self):
if self._gp is None:
self._gp = GaussianProcess(ExpSquaredKernel(*self.hyperpars))
if not self._gp.computed:
std = np.sqrt(self.ferr**2 + self.jitter**2)
self._gp.compute(self.time, std)
return self._gp
@property
def jitter(self):
return self._jitter
@jitter.setter
def jitter(self, value):
self._gp = None
self._jitter = value
@property
def hyperpars(self):
return self._hyperpars
@hyperpars.setter
def hyperpars(self, value):
self._hyperpars = value
self._gp = None
# Helper functions for the individual hyperparameters.
@property
def alpha(self):
return self._hyperpars[0]
@alpha.setter
def alpha(self, value):
h = self._hyperpars
h[0] = value
self.hyperpars = h
@property
def scale(self):
return self._hyperpars[1]
@scale.setter
def scale(self, value):
h = self._hyperpars
h[1] = value
self.hyperpars = h
def optimize_hyperpars(self, n=None, **kwargs):
if n is None:
n = len(self.time)
gp = GaussianProcess(self.hyperpars)
flag, hyperpars = gp.optimize(self.time[:n], self.ferr[:n],
self.flux[:n]-1, **kwargs)
self.hyperpars = hyperpars
return flag, hyperpars
def lnlike(self, lc):
"""
Get the likelihood of this dataset given a particular :class:`Model`.
:param model:
The predicted light curve model evaluated at ``eval_time``.
"""
return self.gp.lnlikelihood(self.flux - lc)
def predict(self, lc, size=None, resample=None):
"""
Generate a sample from the light curve probability function for a
particular :class:`Model`.
:param model:
The predicted light curve model evaluated at ``eval_time``.
"""
if resample is None:
mu, cov = self.gp.predict(self.flux - lc, self.time)
return mu + lc
t = self.time[::resample]
mu, cov = self.gp.predict(self.flux - lc, t)
mu += lc[::resample]
return np.interp(self.time, t, mu)
# Generate some fake data.
period = 0.956
x = 10 * np.sort(np.random.rand(75))
yerr = 0.1 + 0.1 * np.random.rand(len(x))
y = gp.sample_prior(x)
y += 0.8 * np.cos(2 * np.pi * x / period)
y += yerr * np.random.randn(len(yerr))
# Set up a periodic kernel.
pk = ExpSquaredKernel(np.sqrt(0.8), 1000.0) * CosineKernel(period)
kernel2 = kernel + pk
gp2 = GaussianProcess(kernel2)
# Condition on this data.
gp2.compute(x, yerr)
# Compute the log-likelihood.
print("Log likelihood = {0}".format(gp2.lnlikelihood(y)))
# Compute the conditional predictive distribution.
t = np.linspace(0, 10, 200)
f = gp2.sample_conditional(y, t, size=500)
mu = np.mean(f, axis=0)
std = np.std(f, axis=0)
pl.errorbar(x, y, yerr=yerr, fmt=".k")
pl.plot(t, mu, "k", lw=2, alpha=0.5)
pl.plot(t, mu+std, "k", alpha=0.5)
pl.plot(t, mu-std, "k", alpha=0.5)
pl.savefig("periodic.png")
