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inverse_tools.py
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inverse_tools.py
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"""Statistical model and fitter for occurrence rates."""
import warnings
import emcee
import numpy as np
from numpy import random
import pymc3 as pm
import pandas as pd
import matplotlib.pyplot as plt
import matplotlib.ticker as ticker
from mpl_toolkits.axes_grid1 import make_axes_locatable
from corner import corner
from . import vislib
# Jeffreys prior for a Poisson rate parameter:
#
# p(rate) = sqrt(1/rate)
#
# Or equivalently, sqrt(rate) has an unnormalised uniform distribution
#
# See:
# PAPERS
# https://en.wikipedia.org/wiki/Jeffreys_prior relevant section
#
# When transformed to log_rate, then it is:
#
# p(rate) = rate**(-3/2)
#
# TODO: more accurate name is OccurrenceModel or OccurrenceModelPoisson
# update this in analysis and other places too
class ObservableOccurrenceBasic(object):
"""Probability object defines the observable occurrence pdf.
The completeness is treated as binned in a set number of bins
in period and planet radius. The true occurence is treated as
binned only in radius in a set number of intervals.
NOTE: regarding logP vs P; this object doesn't care, at least
in the calculations. That's an outside consideration.
NOTE: regarding log_occr, the only place where this is considered
is during sampling. Thus, likelihood and probability
calculations will switch between taking log_occr or just
occr. Everywhere else (i.e volumise_occr), the parameter
is the occr, and never log_occr.
Additionally, all output, including MCMC samples, and
sample_storage, are always in normal form (occr). Never
in log form. So log_occr only affects the sampling. Really
apart from potentially convergence issues, it should be
completely the same.
TODO: potentially source of error, what happens outside of our grid.
For example, what if I give an event value outside our grid,
or in general it would be nice if there was an outside value.
"""
def __init__(self, R_boundaries, P_boundaries, cpf_value_grid,
N_stars, planets=None, fit_log_occr=False,
log_p=True, log_r=False):
"""Creates the probability from array of completeness values.
Completeness grid has a N x M dimension; with N R-bins,
and M P-bins.
Occurence rate is binned in radius, in 1 Rj intervals,
for now.
Args:
R_boundaries (np.array, (N+1)-dim): the boundaries of
the bins in R space (inclusive of top bound)
P_boundaries (np.array, (M+1)-dim): the boundaries of
the bins in P space (inclusive of top bound)
cpf_value_grid (np.ndarray, shape: NxM): the values of the
*completeness* in each bin,
[i,j]: i indexes radii, j index period
N_stars
planets
fit_log_occr
log_p
log_r
"""
grid_shape = (len(R_boundaries) - 1, len(P_boundaries) - 1)
self._R_boundaries = np.array(R_boundaries)
self._P_boundaries = np.array(P_boundaries)
self._N_stars = N_stars
self._grid_shape = grid_shape
self._log_p_flag = log_p
self._log_r_flag = log_r
self._log_occr_flag = fit_log_occr
# Enter completeness array
if np.shape(cpf_value_grid) == grid_shape:
self._cpf_grid = np.array(cpf_value_grid)
elif np.shape(cpf_value_grid.T) == grid_shape:
print("Reshaping completeness array.")
self._cpf_grid = np.array(cpf_value_grid.T)
else:
raise ValueError("Array shape of completeness_value_grid "
"doesn't match the expected internal shape "
"based on the bin boundary values.")
# Check that shape of completeness grid is the same as grid_shape
if not all(dim in np.shape(self._cpf_grid) for dim in self.shape):
raise ValueError("The completeness grid doesn't match "
"the grid shape.")
# Initiate the occurrence rate in same bins of R as cpf
# NOTE: never start them at zero, it will crash
# This initialisation isn't checked for shape
self.occr_array = np.ones(np.shape(self))
# Flag; if True, the parameters have been unchanged since
# the last time the rate integral was calculated; therefore
# the cached integral is safe to use.
self._int_cache_flag = False
self._int_cache = 0.0
self._sample_storage = None
# If uncertainties are given, bootstrap the events and reduce
# the weights
if np.ndim(planets) == 2 and np.shape(planets)[1] == 2:
# Where only hard values are given
event_weight = 1
event_values = planets
else:
# Otherwise, we need a df in the form:
# R_p, R_p_err_low, R_p_err_high, P, P_err (optional)
N_s = 1000
event_weight = 1/N_s
planet_samples = []
for idx in planets.index:
radii, periods = [], []
if 'P_err' not in planets or planets.P_err.isnull()[idx]:
periods = N_s * [planets.loc[idx, 'P']]
else:
periods = random.randn(N_s) * planets.loc[idx, 'P_err']
periods += planets.loc[idx, 'P']
# The radii are taken from a "split" normal
radii = random.randn(N_s)
radii[radii >= 0] *= planets.loc[idx, 'R_p_err_high']
radii[radii < 0] *= planets.loc[idx, 'R_p_err_low']
radii += planets.loc[idx, 'R_p']
planet_samples.append(np.column_stack([radii, periods]))
event_values = np.concatenate(planet_samples)
# event_values must not be a pandas DataFrame
self._event_values = event_values
self._event_weights = event_weight
# if event_values is None or len(event_values) == 0:
# self._event_values = event_values
# else:
# filtered_events = []
# for i in range(len(event_values)):
# if (self._R_boundaries[0] < event_values[i][0])
# and (event_values[i][0] < self._R_boundaries[-1]):
# filtered_events.append(event_values[i])
# self._event_values = np.concatenate(filtered_events)
# this may be un-necessary. Avoid using this and perhaps delete it.
# It's entirely ambiguous what the object call should really return.
def __call__(self, *args, **kwargs):
"""Calculates the value of the likelihood.
Args:
event_values (np.array or float): the R, P pairs to calculate
the likelihood. If None or empty, calculates it
assuming zero events. Otherwise, expects a single
(R, P) coordinate, or N values of (R, P), i.e
shape (N x 2).
"""
return self.log_likelihood(*args, **kwargs)
# Properties and internals
# ------------------------
@property
def shape(self):
"""Gives the shape of the completeness array."""
# TODO: perhaps this should be a list? That's what the shape
# normally is.
return np.array([len(self._R_boundaries)-1, len(self._P_boundaries)-1])
@property
def occr_r_names(self):
"""The string names (ranges) of the radius bins."""
occr_names = []
for i in range(len(self._R_boundaries) - 1):
occr_names.append("{} - {}".format(self._R_boundaries[i],
self._R_boundaries[i+1]))
return occr_names
@property
def occr_p_names(self):
"""The string names (ranges) of the period bins."""
occr_names = []
for i in range(len(self._P_boundaries) - 1):
occr_names.append("{:.3g} - {:.3g}".format(
self._P_boundaries[i], self._P_boundaries[i+1]))
return occr_names
def get_occr(self):
return self.occr_array
def set_occr(self, array):
if not np.array_equal(np.shape(array), np.shape(self)):
# np.all(np.shape(array) == np.shape(self)):
import pdb; pdb.set_trace()
raise ValueError("Input array is the wrong shape.")
elif (array < 0.0).any():
raise InvalidOccurrenceRate("Negative occurrence rate is invalid.")
self._int_cache_flag = False
self.occr_array = array
def get_log_occr(self):
return np.log10(self.occr_array)
def set_log_occr(self, array):
if not np.array_equal(np.shape(array), np.shape(self)):
# np.all(np.shape(array) == np.shape(self)):
import pdb; pdb.set_trace()
raise ValueError("Input array is the wrong shape.")
elif not np.isfinite(array).all():
raise InvalidOccurrenceRate("Negative occurrence rate is invalid.")
self._int_cache_flag = False
self.occr_array = 10**array
def get_event_values(self):
return self._event_values
def set_event_values(self, array):
self._int_cache_flag = False
if array is None:
self._event_values = None
elif np.ndim(array) == 1:
self._event_values = np.array(array).reshape([1, 2])
elif (np.ndim(array) == 2) and (np.shape(array)[1] == 2):
self._event_values = np.array(array)
else:
raise ValueError('Invalid entry to event values '
'(check the shape).')
occr = property(get_occr, set_occr)
log_occr = property(get_log_occr, set_log_occr)
event_values = property(get_event_values, set_event_values)
# Probabilistic methods
# ---------------------
def likelihood(self, occr_array=None, event_values=None):
"""Calculates the value of the likelihood.
NOTE: likelihood, not log-likelihood
Args:
occr_array (np.array): occurrence rates. If _log_occr_flag
then give them as log occurrence rates.
event_values (np.array or float): the R, P pairs to calculate
the likelihood. If None or empty, calculates it
assuming zero events. Otherwise, expects a single
(R, P) coordinate, or N values of (R, P), i.e
shape (N x 2).
"""
# BUG UPDATE
if occr_array is not None and not self._log_occr_flag:
# Normal occurrence rates
try:
self.occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return 0.0
elif occr_array is not None and self._log_occr_flag:
# Log occurrence
try:
self.log_occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return 0.0
# if occr_array is not None and not (occr_array < 0.0).any():
# self.occr = occr_array
# elif occr_array is not None and (occr_array < 0.0).any():
# # Prevent it at this stage so we don't trying an error
# return 0.0
if event_values is not None:
self.event_values = event_values
I = self.calc_integral() * self._N_stars
# Case of no events
if self.event_values is None or \
not hasattr(self.event_values, '__len__'):
value = np.exp(-I)
else:
value = np.exp(-I) * np.prod(self.rate_density(self.event_values))
# BUG
if np.isnan(value):
import pdb; pdb.set_trace()
# A nan value is possible when some of the occr are too high
return value if not np.isnan(value) else 0.0
def log_likelihood(self, occr_array=None, event_values=None):
"""Calculates the value of the likelihood.
Args:
occr_array (np.array): occurrence rates. If _log_occr_flag
then give them as log occurrence rates.
event_values (np.array or float): the R, P pairs to calculate
the likelihood. If None or empty, calculates it
assuming zero events. Otherwise, expects a single
(R, P) coordinate, or N values of (R, P), i.e
shape (N x 2).
"""
# BUG UPDATE
if occr_array is not None and not self._log_occr_flag:
# Normal occurrence rates
try:
self.occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return -np.inf
elif occr_array is not None and self._log_occr_flag:
# Log occurrence
try:
self.log_occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return -np.inf
# if occr_array is not None and not (occr_array < 0.0).any():
# self.occr = occr_array
# elif occr_array is not None and (occr_array < 0.0).any():
# # Prevent it at this stage so we don't try an error
# return - np.inf
if event_values is not None:
self.event_values = event_values
I = self.calc_integral() * self._N_stars
# Case of no events
if self.event_values is None or \
not hasattr(self.event_values, '__len__'):
value = - I
else:
value = np.sum(np.log(self.rate_density(self.event_values))) - I
# BUG
if np.isnan(value):
import pdb; pdb.set_trace()
return value if not np.isnan(value) else -np.inf
def prior(self, occr_array=None):
"""Calculates the prior pdf of the occurrence rates.
Automatically transforms in the case where log_occr is used.
Args:
occr_array (np.array): occurrence rates. If _log_occr_flag
then give them as log occurrence rates.
"""
# Deal with the actual input/read it
if occr_array is not None and not self._log_occr_flag:
# Normal occurrence rates
try:
self.occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return 0.0
elif occr_array is not None and self._log_occr_flag:
# Log occurrence
try:
self.log_occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return 0.0
if not self._log_occr_flag:
return np.prod(np.sqrt(1/self.occr))
else:
# Written in terms of occr for ease, also same as:
# sqrt(occr) = sqrt(10**self.log_occr)
return np.prod(np.sqrt(self.occr))
def log_prior(self, occr_array=None):
"""Calculates the prior pdf of the occurrence rates.
Automatically transforms in the case where log_occr is used.
Args:
occr_array (np.array): occurrence rates. If _log_occr_flag
then give them as log occurrence rates.
"""
# Deal with the actual input/read it
if occr_array is not None and not self._log_occr_flag:
# Normal occurrence rates
try:
self.occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return -np.inf
elif occr_array is not None and self._log_occr_flag:
# Log occurrence
try:
self.log_occr = occr_array
except InvalidOccurrenceRate:
# Catch invalid occurrence rates for zero likelihood
return -np.inf
if not self._log_occr_flag:
# NOTE: Ah ah ah! We take log10 for log_occr, but log
# for the log of a prior or probability density function
return np.sum(-0.5*np.log(self.occr))
else:
# Written in terms of occr for ease.
value = np.sum(0.5*np.log(self.occr))
# At this point, it's still possible for occr to be so
# small that it's underflowing, where value will be nan
# This should not be possible if _log_occr_flag = False
return value if not np.isnan(value) else -np.inf
def log_posterior(self, occr_array=None, event_values=None,
flattened_occr=False):
"""Calculates the log posterior of a value array of occr.
occr_array can be normal or log, which must be reflected in
self._log_occr_flag
occr_array can also be flattened so that emcee can use it,
however we then need to set flattened_occr to True.
Args:
occr_array: can be normal or log, which must be reflected in
self._log_occr_flag. Can also be flattened so that
emcee can use it, however we then need to set
flattened_occr to True.
event_values (np.array or float): the R, P pairs to calculate
the likelihood. If None or empty, calculates it
assuming zero events. Otherwise, expects a single
(R, P) coordinate, or N values of (R, P), i.e
shape (N x 2).
flattened_occr (bool=False): if True, it will assume that
that passed occr was flattened, and will attempt to
unflatted (ravel) it, through np.reshape.
Returns:
log(p(occr|data))
"""
if flattened_occr and occr_array is not None:
# Unflatten it into the occurrence rate grid
occr_array = np.reshape(occr_array, np.shape(self.occr))
# Let the likelihood and prior actually sub the values in
log_likelihood = self.log_likelihood(occr_array)
log_prior = self.log_prior(occr_array)
# BUG:
if np.isnan(log_likelihood + log_prior) \
or (log_likelihood + log_prior) is None:
import pdb; pdb.set_trace()
return log_likelihood + log_prior
# Calculations
# ------------
def calc_integral(self):
"""Calculates the in TODO"""
# Return the cached value if possible
if self._int_cache_flag:
return self._int_cache
#I = np.sum(self.occr * np.sum(self._cpf_grid*self.calc_bin_volumes(),
# axis=1))
I = np.sum(self.volumise_occr() * self._cpf_grid)
self._int_cache_flag = True
self._int_cache = I
return I
def calc_bin_volumes(self):
"""Calculates the array of areas (Lebesque measure) per bin.
If logP, the volume will be in log-space for P.
"""
if self._log_p_flag:
P_diffs = np.diff(np.log10(self._P_boundaries))
else:
P_diffs = np.diff(self._P_boundaries)
if self._log_r_flag:
R_diffs = np.diff(np.log10(self._R_boundaries))
else:
R_diffs = np.diff(self._R_boundaries)
return np.outer(R_diffs, P_diffs)
# return np.outer(np.diff(self._R_boundaries),
# np.diff(np.log10(self._P_boundaries)))
#else:
# return np.outer(np.diff(self._R_boundaries),
# np.diff(self._P_boundaries))
# TODO: should this take occr as a parameter and should it be
# allowed to take log_occr
def volumise_occr(self, occr=None):
"""Integrates the occurrence rate over volume.
NOTE:should be the only thing that's changed between,
different hyperparametrisations.
Returns:
volumised_occr: must be the same shape as the grid shape.
"""
occr = self.occr if occr is None else occr
volumised_occr = occr * self.calc_bin_volumes()
assert np.all(np.shape(volumised_occr)[-2:] == self.shape)
assert np.array_equal(np.shape(volumised_occr)[-2:], np.shape(self))
return volumised_occr
def integrate_over_volume(self, value_array):
"""Multiplies input by self.calc_bin_volumes.
TODO: currently do not use, DEPRECATED."""
return value_array * self.calc_bin_volumes()
def rate_density(self, value):
"""Returns the rate density at a particular value of (R, P).
Returns: occurrence rate x completeness
"""
# TODO: analyse for certain that log units cancel out
# with the change in occr
if value.ndim == 2:
value = value.T
# The transpose kind of "switches" the R, P index
# even though planets is in [[P_i, R_i], [...], ...]
R_i = np.digitize(value[0], self._R_boundaries) - 1
P_i = np.digitize(value[1], self._P_boundaries) - 1
# Remove the ones out of bounds (oob_mask = out of bounds mask)
oob_mask = np.zeros_like(R_i, dtype=bool)
oob_mask = oob_mask | ((R_i < 0) | (R_i >= np.shape(self.occr)[0]))
oob_mask = oob_mask | ((P_i < 0) | (P_i >= np.shape(self.occr)[1]))
R_i = R_i[~oob_mask]
P_i = P_i[~oob_mask]
return self.occr[R_i, P_i] * self._cpf_grid[R_i, P_i]
# Estimators
# ----------
def predict_rate_grid(self, occr=None, N_stars=None,
expected_detection=False):
"""Predicts the rate at each cpf-grid bin."""
occr = self.occr if occr is None else occr
N_stars = self._N_stars if N_stars is None else N_stars
if expected_detection:
# Includes detection sensitivity and geometric transit,
# i.e the entire completeness
rate_grid = self.volumise_occr(occr) * self._cpf_grid
#rate_grid = (self._cpf_grid * self.calc_bin_volumes()).T * occr
else:
rate_grid = self.volumise_occr(occr)
return N_stars * rate_grid
def marginalise_occr_period(self, occr=None):
"""Marginalises the occurence rate over the range of periods."""
occr = self.occr if occr is None else occr
#return occr * self.calc_bin_volumes().sum(axis=1)
# TODO: check if this is True.
# i.e: in an inhomogeneous Poisson process, is the total
# rate in a volume of the space equal to the integral
# of the rate-function across that volume of space?
return self.volumise_occr(occr).sum(axis=-1)
# Sampling and inversion
# ----------------------
def sample_occr(self, burn=2000, iters=2000, nwalkers=None,
save=True, plot=False):
flat_shape = np.prod(np.shape(self.occr))
nwalkers = 2*(flat_shape+1) if nwalkers is None else nwalkers
occr_initial = random.rand(nwalkers, flat_shape)
if self._log_occr_flag:
occr_initial = np.log10(occr_initial)
sampler = emcee.EnsembleSampler(nwalkers=nwalkers,
dim=flat_shape,
lnpostfn=self.log_posterior,
kwargs={'event_values':None,
'flattened_occr':True})
# Burn
pos, _, _ = sampler.run_mcmc(occr_initial, N=burn)
sampler.reset()
# BUG
print("Burn complete without error.")
# Run
pos, _, _ = sampler.run_mcmc(pos, N=iters)
# BUG
print("Run complete without error.")
# Extract chains
#samples = sampler.chain[:, burn:, :].reshape((-1, len(self.occr)))
samples = sampler.flatchain
# Need to reshape back into the occr shape
samples = np.reshape(samples, (-1, *np.shape(self.occr)))
# Crucial: the samples and output are always in normal form,
# never in log form
if self._log_occr_flag:
samples = 10**samples
if save:
self._sample_storage = samples
# TODO: rmeove this.
if plot:
medians = np.median(samples, axis=0)
hfig = corner(samples, labels=self.occr_r_names, truths=medians)
hfig.suptitle("Occurrence hyperparameters")
hfig.show()
# The occurrences marginalised over period bins
moccr_samples = self.volumise_occr(samples).sum(axis=-1)
moccr_medians = np.median(moccr_samples, axis=0)
mfig = corner(moccr_samples, labels=self.occr_r_names,
truths=moccr_medians)
mfig.suptitle("Marginalised occurrences")
mfig.show()
return samples
def sample_occr_individual(self, iters=2000, nwalkers=2,
save=True, plot=False):
"""Samples the occurrence rates individually in each bin."""
# TODO: make an invert_poisson function that does the MCMC.
# will need to be transposed to samples of 2d grid
# But this shape will make it easier to sub the data in
samples = np.zeros([np.shape(self)[0],
np.shape(self)[1],
iters*nwalkers])
volumised_cpf = self._cpf_grid * self.calc_bin_volumes()
for ix, iy in np.ndindex(*np.shape(self)):
rm = volumised_cpf[ix, iy] * self._N_stars
if self._event_values is not None:
nevents = np.sum(
(self._event_values.T[0] > self._R_boundaries[ix]) \
& (self._event_values.T[0] < self._R_boundaries[ix+1]) \
& (self._event_values.T[1] > self._P_boundaries[iy]) \
& (self._event_values.T[1] < self._P_boundaries[iy+1]))
else:
nevents = 0
samples[ix, iy, :] = sample_poisson_rate_pymc(rate_multiplier=rm,
num_events=nevents,
iters=iters,
nchains=nwalkers)
samples = samples.swapaxes(0, -1).swapaxes(-1, 1)
if save:
self._sample_storage = samples
if plot:
medians = np.median(samples, axis=0)
hfig = corner(samples, labels=self.occr_r_names, truths=medians)
hfig.suptitle("Occurrence hyperparameters")
hfig.show()
# The occurrences marginalised over period bins
moccr_samples = self.volumise_occr(samples).sum(axis=-1)
moccr_medians = np.median(moccr_samples, axis=0)
mfig = corner(moccr_samples, labels=self.occr_r_names,
truths=moccr_medians)
mfig.suptitle("Marginalised occurrences")
mfig.show()
return samples
# Plotting and additional
# -----------------------
def plot_2d_occr(self, samples=None, show=True, percentage_flag=True,
**sampler_kwargs):
"""Plots the 2d occurrence rate. Focus on the distribution.
Args:
samples (np.ndarray=None)
show (bool=True)
upper_limits (bool=True)
print_mode (str='dist'): What to print on the array
None, 'none', False: nothing is printed
'dist', 'norm', 'uncertainties': gaussian uncertainties
'detail', 'full', 'predict': paper plot, prints
predicted detections, 95% limit, etc...
Returns:
fig, ax
"""
# We still get this error:
# TypeError: Dimensions of C (5, 11) are incompatible with X (6) and/or Y (12); see help(pcolormesh)
# ~/invocc/inverse_tools.py in plot_2d_occr(self, samples, show, **sampler_kwargs)
# 681 else:
# 682 im = ax.pcolormesh(self._P_boundaries, self._R_boundaries,
# --> 683 occr_grid.T)
# 684 ax.set_xscale('log')
#
# TODO: for that, check how it's done in vislib, perhaps we need
# one less boundary at the end for example.
#
# TODO: in any case, update this to use vislib
#
# TODO: one option is: to plot the upper bounds or the median
# this should be an argument
# Multiplies by 100 to get percentages
pfac = 100 if percentage_flag else 1
if percentage_flag:
cbar_text = 'occurrence rate limit (%)'
pfac = 100
else:
cbar_text = 'occurrence rate limit'
pfac = 1
if samples is None and self._sample_storage is not None:
samples = self._sample_storage
elif samples is None:
samples = self.sample_occr(**sampler_kwargs)
occr_median = self.predict_rate_grid(np.median(samples, axis=0),
N_stars=1,
expected_detection=False)
occr_lower = self.predict_rate_grid(np.percentile(samples, 16, axis=0),
N_stars=1,
expected_detection=False)
occr_upper = self.predict_rate_grid(np.percentile(samples, 84, axis=0),
N_stars=1,
expected_detection=False)
occr_limit = self.predict_rate_grid(np.percentile(samples, 95, axis=0),
N_stars=1,
expected_detection=False)
ax = vislib.plot_grid(grid_values=occr_limit*pfac,
x_edges=self._P_boundaries,
y_edges=self._R_boundaries,
log_x=self._log_p_flag,
log_values=True,
value_label=cbar_text,
print_values=False,
show=False,
truncated_cmap=True)
# Add the text
# ------------
# Upper limits
ulim_text = np.empty_like(occr_limit, dtype=object)
for ix, iy in np.ndindex(*np.shape(ulim_text)):
# ulim_text[ix, iy] = r"{:.2g}".format(occr_limit[ix, iy]*pfac)
ulim_text[ix, iy] = np.format_float_positional(
occr_limit[ix, iy]*pfac, precision=2, fractional=False)
vislib.add_text_grid(ulim_text,
self._P_boundaries,
self._R_boundaries,
ax=ax, square_offset=[0.98, 0.95],
horizontalalignment='right',
verticalalignment='top',
size_factor=1,
color='red')
# Median
med_text = np.empty_like(occr_median, dtype=object)
for ix, iy in np.ndindex(*np.shape(med_text)):
# med_text[ix, iy] = r"{:.2g}".format(occr_median[ix, iy]*pfac)
med_text[ix, iy] = np.format_float_positional(
occr_median[ix, iy]*pfac, precision=2, fractional=False)
vislib.add_text_grid(med_text,
self._P_boundaries,
self._R_boundaries,
ax=ax, square_offset=[0.45, 0.05],
horizontalalignment='right',
verticalalignment='bottom',
size_factor=1)
# +-
pm_text = np.empty_like(occr_upper, dtype=object)
for ix, iy in np.ndindex(*np.shape(pm_text)):
pm_text[ix, iy] = r"$^{{\,+{}}} _{{\,-{}}}$".format(
np.format_float_positional(occr_upper[ix, iy]*pfac,
precision=1, fractional=False),
np.format_float_positional(occr_lower[ix, iy]*pfac,
precision=1, fractional=False))
vislib.add_text_grid(pm_text,
self._P_boundaries,
self._R_boundaries,
ax=ax, square_offset=[0.42, 0.01],
horizontalalignment='left',
verticalalignment='bottom',
size_factor=1*1)
# Predicted detections with occr=1
pred_text = np.empty_like(occr_median, dtype=object)
for ix, iy in np.ndindex(*np.shape(pred_text)):
# pred_text[ix, iy] = r"{:.2g}".format(
# self._cpf_grid[ix, iy]*self._N_stars)
pred_text[ix, iy] = np.format_float_positional(
self._cpf_grid[ix, iy]*self._N_stars,
precision=2, fractional=False)
vislib.add_text_grid(pred_text,
self._P_boundaries,
self._R_boundaries,
ax=ax, square_offset=[0.03, 0.95],
horizontalalignment='left',
verticalalignment='top',
size_factor=1)
# occr_text = np.empty_like(occr_median, dtype=object)
# for ix, iy in np.ndindex(*np.shape(occr_text)):
# occr_text[ix, iy] = r"${:.2g} ^{{\,{:.1g}}} _{{\,{:.1g}}}$".format(
# occr_median[ix, iy], occr_upper[ix, iy], occr_lower[ix, iy])
# vislib.add_text_grid(occr_text,
# self._P_boundaries,
# self._R_boundaries,
# ax=ax, square_offset=[0.1, 0.05])
# Additional aesthetics
ax.set_xlabel('Period, days')
ax.set_ylabel(r'Radius, $R_\oplus$')
fig = ax.figure
if show:
plt.show()
else:
fig.show()
return fig, ax
def plot_2d_occr_detail(self, samples=None, show=True,
upper_limits=True, **sampler_kwargs):
"""Plots the 2d occurrence rate with different details.
Focus on upper limit, expected number of detections, etc...
Returns:
fig, ax
"""
# We still get this error:
# TypeError: Dimensions of C (5, 11) are incompatible with X (6) and/or Y (12); see help(pcolormesh)
# ~/invocc/inverse_tools.py in plot_2d_occr(self, samples, show, **sampler_kwargs)
# 681 else:
# 682 im = ax.pcolormesh(self._P_boundaries, self._R_boundaries,
# --> 683 occr_grid.T)
# 684 ax.set_xscale('log')
#
# TODO: for that, check how it's done in vislib, perhaps we need
# one less boundary at the end for example.
#
# TODO: in any case, update this to use vislib
#
# TODO: one option is: to plot the upper bounds or the median
# this should be an argument
if samples is None and self._sample_storage is not None:
samples = self._sample_storage
elif samples is None:
samples = self.sample_occr(**sampler_kwargs)
occr_median = np.median(samples, axis=0)
occr_lower = np.percentile(samples, 16, axis=0)
occr_upper = np.percentile(samples, 84, axis=0)
occr_limit = np.percentile(samples, 95, axis=0)
occr_grid = self.predict_rate_grid(occr_median,
N_stars=1,
expected_detection=False)
fig, ax = plt.subplots()
if not self._log_p_flag:
im = ax.matshow(occr_grid, origin='lower',
extent=(self._P_boundaries[0],
self._P_boundaries[-1],
self._R_boundaries[0],
self._R_boundaries[-1]))
else:
import pdb; pdb.set_trace()
im = ax.pcolormesh(self._P_boundaries, self._R_boundaries,
occr_grid)
ax.set_xscale('log')
# Colour bar
divider = make_axes_locatable(ax)
cax = divider.append_axes("right", size="6%", pad=0.3)
cbar = fig.colorbar(im, cax=cax)
cbar.set_label("occurrence rate")
fig.suptitle('Occurrence rate (within bin)')
#ax.set_xticklabels(self._R_boundaries - 0.25)
#ax.set_yticklabels(self._P_boundaries - 2.50)
ax.set_xlabel('Period, days')
ax.set_ylabel(r'Radius, $R_\oplus$')
ax.set_aspect('auto')
ax.tick_params('both', reset=True, which='major', direction='inout',
bottom=True, top=False, left=True, right=False,
length=12, width=1, zorder=10)
ax.tick_params('both', reset=True, which='minor', direction='inout',
bottom=True, top=False, left=True, right=False,
length=8, width=0.5, zorder=10)
ax.xaxis.set_major_formatter(ticker.FormatStrFormatter('%.1f'))
if show:
plt.show()
else:
fig.show()
return fig, ax
def plot_marg_occr(self, samples=None, show_95=True,
show=True, fix_limits=True,
print_values=True, **sampler_kwargs):
"""Plots the marginalised occurrence rate in R-space.
Returns:
fig, ax
"""
if samples is None and self._sample_storage is not None:
samples = self._sample_storage
elif samples is None:
samples = self.sample_occr(**sampler_kwargs)
#moccr_samples = samples * self.calc_bin_volumes().sum(axis=1)
moccr_samples = self.volumise_occr(samples).sum(axis=-1)
# better way
moccr_samples = self.marginalise_occr_period(samples)