Bayesian Inference II: Fitting a Straight Line

Phil Marshall, Daniel Foreman-Mackey and Dustin Lang

Astro Hack Week, New York, September 2015

This is AstroHackWeek/inference/straightline.ipynb

Goals:

• Check models, with posterior predictive distributions of test statistics
• Suggest some simple hacks to get some practice with Bayesian inference


In [1]:

from __future__ import print_function
import numpy as np

import matplotlib.pyplot as plt
%matplotlib inline

plt.rcParams['figure.figsize'] = (6.0, 6.0)
plt.rcParams['savefig.dpi'] = 100




In [2]:

from straightline_utils import *



The Data

• Let's generate a simple dataset: observations of $y$ with reported uncertainties $\sigma_y$, at given $x$ values.
• Yours will look different to mine, as your random seed will be different. That's good - we can do some (completely unrealistic) comparisons over datasets.


In [3]:

(x,y,sigmay) = generate_data()

plot_yerr(x, y, sigmay)






Least-squares Straight Line Fit

• An industry standard: find the slope and intercept of a straight line that minimizes the mean square residual. Since the predicted data depend linearly on the parameters, the least squares solution can be found by a matrix inversion and multiplication, conveneniently packed in numpy.linalg.
• Suppose that the $y$ values are related to the $x$ values by $y = m x + b$, where $x$ and $y$ are "vectors" (numpy arrays). We might say that we want to find $m$ and $b$ that minimize

$W^2 = \sum_k \frac{(y_k - m x_k - b)^2}{\sigma_k^2}$

• Here, $1/\sigma_k^2$ is a sensible weighting factor that reduces the influence of $y_k$ values with large uncertainty $\sigma_k$
• Differentiating $W^2$ with respect to $m$ and $b$ and setting the result to zero leads to a matrix equation that can be solved - this is what np.linalg.lstsq is doing.


In [4]:

# Linear algebra to implement weighted least squares.
N = len(x)
A = np.zeros((N,2))
A[:,0] = 1. / sigmay
A[:,1] =  x / sigmay
yy = y / sigmay

theta,nil,nil,nil = np.linalg.lstsq(A,yy)

b_ls,m_ls = theta
print('Weighted least-squares estimated b,m:', b_ls,m_ls)

plot_yerr(x, y, sigmay)
plot_line(m_ls, b_ls);




Weighted least-squares estimated b,m: 116.70256265 0.120979422132



Probabilistic Fitting

• The Bayesian answer to the question "What are the values of $b$ and $m$ in a straight line model for the above data?" is the posterior PDF for those parameters, ${\rm Pr}(m,b|y)$
• The posterior PDF doesn't tell us the best-fit parameter combination - it gives us the means to simulate all plausible parameter combinations, given the data.
• Let's derive this posterior PDF, starting with a probabilistic graphical model.


In [5]:

# import straightline_pgm
# straightline_pgm.draw();

from IPython.display import Image
Image(filename="straightline_pgm.png",width=600)




Out[5]:


• The PGM illustrates the forward problem of simulating a dataset $\{y_k\}$ by drawing random numbers from conditional probability distributions, which are depicted by the nodes. The conditional dependences are depicted by the edges.
• The PGM is a complete description of the forward problem: it is a representation of the joint PDF for all our variables, ${\rm Pr}(m,b,\{y_k\},\{y^{\rm true}_k\}\,|\,\{x_k\},\{\sigma_k\})$, factorized such that we can simulate data:

${\rm Pr}(m,b,\{y_k\},\{y^{\rm true}_k\}\,|\,\{x_k\},\{\sigma_k\},H_1) = \prod_k {\rm Pr}(y_k\,|\,y^{\rm true}_k,\sigma_k,H_1) \;{\rm Pr}(y^{\rm true}_k\,|\,x_k,m,b,H_1) \;\;\;{\rm Pr}(m,b\,|\,H_1)$

Questions:

1. Where did that product come from? What assumption does it encode?

2. Why are the $\{x_k\}$ and the $\{\sigma_k\}$ always on the right hand side of the bar, but $\{y_k\}$ is sometimes on the left?

3. What is the meaning of "$H_1$"? Hint: notice that it too is always on the right hand side of the bar.

4. What functional form does the conditional PDF ${\rm Pr}(y^{\rm true}_k\,|\,x_k,m,b,H_1)$ have?

5. What functional form do you think we should assume for the sampling distribution, ${\rm Pr}(y_k\,|\,y^{\rm true}_k,x_k,\sigma_k,H_1)$? Hint: imagine you were generating mock data.

6. What functional form should we assume for ${\rm Pr}(m,b\,|\,H_1)$?

Talk to your neighbor(s) for 5 minutes about these, note down some brief answers, and be prepared to provide them when called upon.



In [6]:



The Inverse Problem

• Let's simplify our joint probability expression a bit, by marginalizing out the latent variables $\{y^{\rm true}_k\}$, and absorbing the $\{x_k\}$ and $\{\sigma_k\}$ into $H_1$ wherever it's helpful.

${\rm Pr}(m,b,\{y_k\}|H_1) = \int\, \prod_k {\rm Pr}(y_k\,|\,y^{\rm true}_k,H_1) \;{\rm Pr}(y^{\rm true}_k\,|\,m,b,H_1) \;\;\;{\rm Pr}(m,b\,|\,H_1) \; d y^{\rm true}_k$

$\longrightarrow {\rm Pr}(m,b,\{y_k\}|H_1) = \prod_k {\rm Pr}(y_k\,|\,(m x_k + b),H_1) \;\;\;{\rm Pr}(m,b\,|\,H_1)$

• Now we just factorize the left hand side and rearrange (like Bayes did), to get:

${\rm Pr}(m,b\,|\,\{y_k\},H_1) = \frac{1}{Z} \prod_k {\rm Pr}(y_k\,|\,(m x_k + b),H_1) \;\;\;{\rm Pr}(m,b\,|\,H_1)$

• Here, $Z = {\rm Pr}(\{y_k\}\,|\,H_1)$, and is known as the "evidence" for $H_1$. It also goes by the name "Fully Marginalized Likelihood" because

$Z = {\rm Pr}(\{y_k\}\,|\,H_1) = \int \prod_k {\rm Pr}(y_k\,|\,(m x_k + b),H_1) \;{\rm Pr}(m,b\,|\,H_1)\;dm\,db$

and $\prod_k {\rm Pr}(y_k\,|\,(m x_k + b),H_1)$ is the joint likelihood for the parameters. ${\rm Pr}(m,b\,|\,H_1)$ is the prior PDF for the parameters.

Evaluating the posterior PDF on a grid

• For simple, 2-dimensional parameter spaces like this one, evaluating on a grid is not a bad way to go. We'll see that the least squares solution lies at the peak of the posterior PDF - for a certain set of assumptions about the data and the model.
• To compute the evidence $Z$ and normalize the posterior PDF, we need to be able to integrate the likelihood function over the prior - on a grid, we can do this numerically, to normlize the posterior PDF.
• Un-normalized, the likelihood function can take very small values, so we usually work with the log likelihood instead.

Exercise:

With your neighbors, upgrade my log likelihood function below so that it a) gives sensible values and b) runs faster, and you get a plot of the posterior PDF for $m$ and $b$ without having to wait.



In [7]:

def straight_line_log_likelihood(theta, x, y, sigmay):
'''
Returns the log-likelihood of drawing data values *y* at
known values *x* given Gaussian measurement noise with standard
deviation with known *sigmay*, where the "true" y values are
*y_t = m * x + b*

x: list of x coordinates
y: list of y coordinates
sigmay: list of y uncertainties
m: scalar slope
b: scalar line intercept

and the parameter vector theta = (m,b).

Returns: scalar log likelihood
'''

m,b = theta

L = 1.0
for k in range(len(y)):
L *= np.exp(-(y[k] - m*x[k] - b)**2/(2.0*sigmay[k]**2))
L /= np.sqrt(2.0 * np.pi * sigmay[k]**2)

return np.log(L)




In [9]:

def straight_line_log_likelihood(theta, x, y, sigmay):
'''
Returns the log-likelihood of drawing data values *y* at
known values *x* given Gaussian measurement noise with standard
deviation with known *sigmay*, where the "true" y values are
*y_t = m * x + b*

x: list of x coordinates
y: list of y coordinates
sigmay: list of y uncertainties
m: scalar slope
b: scalar line intercept

Returns: scalar log likelihood
'''
m,b = theta
return (np.sum(np.log(1./(np.sqrt(2.*np.pi) * sigmay))) +
np.sum(-0.5 * (y - (m*x + b))**2 / sigmay**2))




In [10]:

def straight_line_log_prior(theta, theta_limits):
m, b = theta
mlimits, blimits = theta_limits

# Uniform in m:
if (m < mlimits[0]) | (m > mlimits[1]):
log_m_prior = -np.inf
else:
log_m_prior = np.log(1.0/(mlimits[1] - mlimits[0]))
# Uniform in b:
if (b < blimits[0]) | (b > blimits[1]):
log_b_prior = -np.inf
else:
log_b_prior = np.log(1.0/(blimits[1] - blimits[0]))

return log_m_prior + log_b_prior

def straight_line_log_posterior(theta, x, y, sigmay, theta_limits):
return (straight_line_log_likelihood(theta, x, y, sigmay) +
straight_line_log_prior(theta, theta_limits))




In [11]:

# Evaluate log P(m,b | x,y,sigmay) on a grid.

# Define uniform prior limits, enforcing positivity in both parameters:
mlimits = [0.0, 2.0]
blimits = [0.0, 200.0]
theta_limits = (mlimits, blimits)

# Set up grid:
mgrid = np.linspace(mlimits[0], mlimits[1], 101)
bgrid = np.linspace(blimits[0], blimits[1], 101)
log_posterior = np.zeros((len(mgrid),len(bgrid)))

# Evaluate log posterior PDF:
for im,m in enumerate(mgrid):
for ib,b in enumerate(bgrid):
theta = (m,b)
log_posterior[im,ib] = straight_line_log_posterior(theta, x, y, sigmay, theta_limits)

# Convert to probability density and plot, taking care with very small values:

posterior = np.exp(log_posterior - log_posterior.max())

plt.imshow(posterior, extent=[blimits[0],blimits[1],mlimits[0],mlimits[1]],cmap='Blues',
interpolation='none', origin='lower', aspect=(blimits[1]-blimits[0])/(mlimits[1]-mlimits[0]),
vmin=0, vmax=1)
plt.contour(bgrid, mgrid, posterior, pdf_contour_levels(posterior), colors='k')

i = np.argmax(posterior)
i,j = np.unravel_index(i, posterior.shape)
print('Grid maximum posterior values (m,b) =', mgrid[i], bgrid[j])

plt.title('Straight line: posterior PDF for parameters');
plt.plot(b_ls, m_ls, 'r+', ms=12, mew=4);
plot_mb_setup(*theta_limits);




Grid maximum posterior values (m,b) = 0.12 116.0



MCMC Sampling

• In problems with higher dimensional parameter spaces, we need a more efficient way of approximating the posterior PDF - both when characterizing it in the first place, and then when doing integrals over that PDF (to get the marginalized PDFs for the parameters, or to compress them in to single numbers with uncertainties that can be easily reported).
• In most applications it's sufficient to approximate a PDF with a (relatively) small number of samples drawn from it; MCMC is a procedure for drawing samples from PDFs.
• The following piece of code implements the Metropolis algorithm, whose derivation can be read in many textbooks. You can read a brief justification aimed at Phil's grad student self in Chapter 2 of Phil's thesis, for example.


In [12]:

def metropolis(log_posterior, theta, theta_limits, stepsize, nsteps=10000):
'''
log_posterior: function of theta
theta_limits:  uniform prior ranges
stepsize:      scalar or vector proposal distribution width
nsteps:        desired number of samples
'''

log_prob = log_posterior(theta, x, y, sigmay, theta_limits)

# Store Markov chain as an array of samples:
chain = np.empty((nsteps, len(theta)))
log_probs = np.empty(nsteps)

# Count our accepted proposals:
naccept = 0

for i in range(nsteps):

theta_new = theta + stepsize * np.random.randn(len(theta))
log_prob_new = log_posterior(theta_new, x, y, sigmay, theta_limits)

if np.log(np.random.rand()) < (log_prob_new - log_prob):
# accept, and move to the proposed position:
theta = theta_new
log_prob = log_prob_new
naccept += 1

else:
# reject, and store the same sample as before:
pass

chain[i] = theta
log_probs[i] = log_prob

acceptance_rate = naccept/float(nsteps)

return chain,log_probs,acceptance_rate




In [17]:

# Initialize m, b at the center of prior:
m = 0.5*(mlimits[0]+mlimits[1])
b = 0.5*(blimits[0]+blimits[1])
theta = np.array([m,b])

# Step sizes, 2% or 5% of the prior
mstep = 0.02*(mlimits[1]-mlimits[0])
bstep = 0.05*(blimits[1]-blimits[0])
stepsize = np.array([mstep,bstep])

# How many steps?
nsteps = 10000

print('Running Metropolis Sampler for', nsteps, 'steps...')

chain, log_probs, acceptance_rate = metropolis(
straight_line_log_posterior, theta, theta_limits, stepsize, nsteps=nsteps
)

print('Acceptance fraction:', acceptance_rate)




Running Metropolis Sampler for 10000 steps...
Acceptance fraction: 0.1697




In [18]:

# Pull m and b arrays out of the Markov chain and plot them:
mm = [m for m,b in chain]
bb = [b for m,b in chain]

# Traces, for convergence inspection:
plt.figure(figsize=(8,5))
plt.subplot(2,1,1)
plt.plot(mm, 'k-')
plt.ylim(mlimits)
plt.ylabel('m')
plt.subplot(2,1,2)
plt.plot(bb, 'k-')
plt.ylabel('Intercept b')
plt.ylim(blimits)




Out[18]:

(0.0, 200.0)


• This looks pretty good: no plateauing, or drift.
• A more rigorous test for convergence is due to Gelman & Rubin, and involves comparing the intrachain variance with the inter-chain variance in an ensemble. It's worth reading up on.
• Foreman-Mackey & Hogg recommend looking at the autocorrelation length, and whether it stablizes during the run.
• Note that we kept all the samples, and did not discard any at the beginning of the run as "burn-in". Nor did we thin the chain at all. Both of these are good ideas.
• Now let's look at the samples in parameter space, overlaid on our gridded posterior.


In [19]:

# First show contours from gridding calculation:
plt.contour(bgrid, mgrid, posterior, pdf_contour_levels(posterior), colors='k')
plt.gca().set_aspect((blimits[1]-blimits[0])/(mlimits[1]-mlimits[0]))

# Scatterplot of m,b posterior samples, overlaid:
plt.plot(bb, mm, 'b.', alpha=0.01)
plot_mb_setup(mlimits,blimits)






Multi-dimensional Visualization

• For a better view of a set of posterior samples, let's make a corner plot that shows all 1D and 2D marginalized distributions.


In [20]:

!pip install --upgrade --no-deps corner




Requirement already up-to-date: corner in /Users/pjm/lsst/DarwinX86/anaconda/2.1.0-4-g35ca374/lib/python2.7/site-packages




In [23]:

import corner
corner.corner(chain[5000:], labels=['m','b'], range=[mlimits,blimits],quantiles=[0.16,0.5,0.84],
show_titles=True, title_args={"fontsize": 12},
plot_datapoints=True, fill_contours=True, levels=[0.68, 0.95],
color='b', bins=80, smooth=1.0);






Exercise:

Now that you have seen the Metropolis sampler in action, let's try and break it.

With your neighbor(s), see if you can change the control parameters (ie. not the priors) to make the sampler fail in various ways - and be ready to report back in 5 minutes.

Anyway:

With a well-tuned sampler:

• It looks like we made a nice, precise measurement!
• Our next step is to check our model for accuracy.

Model Checking

• How do we know if our model is any good? There are two properties that "good" models have: the first is accuracy, and the second is efficiency. We'll return to th equestion of efficiency below.
• Accurate models generate data that is like the observed data. What does this mean? First we have to define what similarity is, in this context. Visual impression is one very important way, that's usually best done first.
• Test statistics that capture relevant features of the data are another. We'll look at the posterior predictive distributions for the datapoints, and for a particularly interesting test statistic, the reduced chi-squared.

Visual Model Checking

• Plot posterior predictions, in data space.


In [24]:

# Generate a straight line model for each parameter combination, and plot:
X = np.linspace(xlimits[0],xlimits[1],50)
for i in (np.random.rand(100)*len(chain)).astype(int):
m,b = chain[i]
plt.plot(X, b+X*m, 'b-', alpha=0.1)
plot_line(m_ls, b_ls)

# Overlay the data, for comparison:
plot_yerr(x, y, sigmay);






Posterior Predictive Model Checking

• If our model is the true one, then replica data generated by it should look like the one dataset we have. This means that summaries of both the real dataset, $T(d)$, and the replica datasets, $T(d^{\rm rep})$, should be drawn from the same distribution.
• If the real dataset was not generated with our model, then its summary may be an outlier from the distribution of summaries of replica datasets.
• We can account for our uncertainty in the parameters $\theta$ by marginalizing them out, which can be easily done by just making the histogram of $T(d^{\rm rep}(\theta))$ from our posterior samples, after drawing one replica dataset $d^{\rm rep}$ from the model sampling distribution ${\rm Pr}(d^{\rm rep}\,|\,\theta)$ for each one.
• Then, we can ask: what is the posterior probability for the summary $T$ to be greater than the observed summary $T(d)$? If this is very small or very large, we should be suspicious of our model - because it is not predicting the data very accurately.

${\rm Pr}(T(d^{\rm rep})>T(d)\,|\,d) = \int I(T(d^{\rm rep})>T(d))\,{\rm Pr}(d^{\rm rep}\,|\,\theta)\,{\rm Pr}(\theta\,|\,d)\;d\theta\,dd^{\rm rep}$

• Here $I$ is the "indicator function" - 1 or 0 according to the condition.


In [25]:

# Test statistics: functions of the data, not the parameters.

# 1) Reduced chisq for the best fit model:
# def test_statistic(x,y,sigmay,b_ls,m_ls):
#   return np.sum((y - m_ls*x - b_ls)**2.0/sigmay**2.0)/(len(y)-2)

# 2) Reduced chisq for the best fit m=0 model:
# def test_statistic(x,y,sigmay,dummy1,dummy2):
#    return np.sum((y - np.mean(y))**2.0/sigmay**2.0)/(len(y)-1)

# 3) Weighted mean y:
# def test_statistic(x,y,sigmay,dummy1,dummy2):
#    return np.sum(y/sigmay**2.0)/np.sum(1.0/sigmay**2.0)

# 4) Variance of y:
# def test_statistic(x,y,sigmay,dummy1,dummy2):
#    return np.var(y)

# 5) Correlation coefficient:
import scipy.stats
def test_statistic(x,y,dummy1,dummy2,dummy3):
'''
Pearson r correlation coefficient:
r12 = \sum [(xi - xbar)*(yi - ybar)] / [\sum (xi - xbar)^2 * \sum (yi - ybar)^2]^1/2
'''
r12 = np.sum((x - np.mean(x))*(y - np.mean(y))) / \
np.sqrt(np.sum((x - np.mean(x))**2) * np.sum((y - np.mean(y))**2))
return r12

# Approximate the posterior predictive distribution for T,
# by drawing a replica dataset for each sample (m,b) and computing its T:
T = np.zeros(len(chain))
for k,(m,b) in enumerate(chain):
yrep = b + m*x + np.random.randn(len(x)) * sigmay
T[k] = test_statistic(x,yrep,sigmay,b_ls,m_ls)

# Compare with the test statistic of the data, on a plot:
Td = test_statistic(x, y, sigmay, b_ls, m_ls)

plt.hist(T, 100, histtype='step', color='blue', lw=2, range=(0.0,np.percentile(T,99.0)))
plt.axvline(Td, color='black', linestyle='--', lw=2)
plt.xlabel('Test statistic')
plt.ylabel('Posterior predictive distribution')

# What is Pr(T>T(d)|d)?

greater = (T > Td)
P = 100*len(T[greater])/(1.0*len(T))
print("Pr(T>T(d)|d) = ",P,"%")




Pr(T>T(d)|d) =  57.93 %


• If our model is true (and we're just uncertain about its parameters, given the data), we can compute the probability of getting a $T$ less than that observed, where T is the reduced chisq relative to a straight line with some reference $(m,b)$.
• Note that we did not have to look up the "chi squared distribution" - we can simply compute the posterior predictive distribution given our generative model.
• Still, this test statistic looks a little bit strange: it's computed relative to the best fit straight line - which is a sensible reference but somehow not really in the spirit of fitting the data...
• Instead, lets look at a discrepancy measure $T(d,\theta)$ that is a function of both the data and the parameters, and compute the posterior probability of getting $T(d^{\rm rep},\theta) > T(d,\theta)$:

${\rm Pr}(T(d^{\rm rep},\theta)>T(d,\theta)\,|\,d) = \int I(T(d^{\rm rep},\theta)>T(d,\theta))\,{\rm Pr}(d^{\rm rep}\,|\,\theta)\,{\rm Pr}(\theta\,|\,d)\;d\theta\,dd^{\rm rep}$



In [26]:

# Discrepancy: functions of the data AND parameters.

# 1) Reduced chisq for the model:
def test_statistic(x,y,sigmay,b,m):
return np.sum((y - m*x - b)**2.0/sigmay**2.0)/(len(y)-2)

# Approximate the posterior predictive distribution for T,
# by drawing a replica dataset for each sample (m,b) and computing its T,
# AND ALSO its Td (which now depends on the parameters, too):
T = np.zeros(len(chain))
Td = np.zeros(len(chain))
for k,(m,b) in enumerate(chain):
yrep = b + m*x + np.random.randn(len(x)) * sigmay
T[k] = test_statistic(x,yrep,sigmay,b,m)
Td[k] = test_statistic(x,y,sigmay,b,m)

# Compare T with Td, on a scatter plot - how often is T>Td?

plt.scatter(Td, T, color='blue',alpha=0.1)
plt.plot([0.0, 100.0], [0.0, 100.], color='k', linestyle='--', linewidth=2)
plt.xlabel('Observed discrepancy $T(d,\\theta)$')
plt.ylabel('Replicated discrepancy $T(d^{\\rm rep},\\theta)$')
plt.ylim([0.0,np.percentile(Td,99.0)])
plt.xlim([0.0,np.percentile(Td,99.0)])




Out[26]:

(0.0, 1.316011856756593)




In [27]:

# Histogram of differences:

diff = T-Td
plt.hist(diff, 100, histtype='step', color='blue', lw=2, range=(np.percentile(diff,1.0),np.percentile(diff,99.0)))
plt.axvline(0.0, color='black', linestyle='--', lw=2)
plt.xlabel('Difference $T(d^{\\rm rep},\\theta) - T(d,\\theta)$')
plt.ylabel('Posterior predictive distribution')

# What is Pr(T>T(d)|d)?

greater = (T > Td)
Pline = 100*len(T[greater])/(1.0*len(T))
print("Pr(T>T(d)|d) = ",Pline,"%")




Pr(T>T(d)|d) =  73.29 %


• The conclusion drawn from the discrepancy is more interesting, in this case. All our $\theta = (m,b)$ samples are plausible, so replica datasets generated by them should also be plausible. The straight line defined by each $(m,b)$ should go through the real data points as readily (on average) as it does its replica dataset.
• Do our posterior predictive $p-$values suggest we need to improve our model? What about the visual check?
• The reduced chi-squared is actually not such an interesting test statistic - because we already used it in the likelihood! Better discrepancy measures would stress-test different aspects of the model - such as the correlations between datapoints, or the behavior of the model in particular places, etc.

Model Expansion

• Maybe I see some curvature in the data - or maybe I have a new astrophysical idea for how this data was generated. Let's try adding an extra parameter to the model, to make a quadratic function:

$y = m x + b + q x^2$

• The coefficient $q$ is probably pretty small (we were originally expecting to only have to use a straight line model for these data!), so I guess we can assign a fairly narrow prior, centered on zero.


In [28]:

def quadratic_log_likelihood(theta, x, y, sigmay):
'''
Returns the log-likelihood of drawing data values y at
known values x given Gaussian measurement noise with standard
deviation with known sigmay, where the "true" y values are
y_t = m*x + b + q**2

x: list of x coordinates
y: list of y coordinates
sigmay: list of y uncertainties
m: scalar slope
b: scalar line intercept
q: quadratic term coefficient

where theta = (m, b, q)

Returns: scalar log likelihood
'''
m, b, q = theta
return (np.sum(np.log(1./(np.sqrt(2.*np.pi) * sigmay))) +
np.sum(-0.5 * (y - (m*x + b + q*x**2))**2 / sigmay**2))

m, b, q = theta
mlimits, blimits, qpars = theta_limits

# m and b:
log_mb_prior = straight_line_log_prior(np.array([m,b]), np.array([mlimits, blimits]))
# q:
log_q_prior = np.log(1./(np.sqrt(2.*np.pi) * qpars[1])) - \
0.5 * (q - qpars[0])**2 / qpars[1]**2
return log_mb_prior + log_q_prior

def quadratic_log_posterior(theta, x, y, sigmay, theta_limits):
return (quadratic_log_likelihood(theta, x, y, sigmay) +




In [29]:

# Define uniform prior limits, enforcing positivity in m and b:
mlimits = [0.0, 2.0]
blimits = [0.0, 200.0]
# Define Gaussian prior centered on zero for q:
qpars = [0.0,0.003]

# Initialize m, b at the center of prior:
m = 0.5*(mlimits[0]+mlimits[1])
b = 0.5*(blimits[0]+blimits[1])
q = qpars[0]

# Arrays to pass to the sampler:
qtheta = np.array([m,b,q])
qtheta_limits = (mlimits, blimits, qpars)

# Step sizes, small fractions of the prior width:
mstep = 0.02*(mlimits[1]-mlimits[0])
bstep = 0.05*(blimits[1]-blimits[0])
qstep = 0.02*qpars[1]
stepsize = np.array([mstep,bstep,qstep])

# How many steps?
nsteps = 10000

print('Running Metropolis Sampler for', nsteps, 'steps...')

qchain, log_probs, acceptance_rate = metropolis(
quadratic_log_posterior, qtheta, qtheta_limits, stepsize, nsteps=nsteps
)

print('Acceptance fraction:', acceptance_rate)




Running Metropolis Sampler for 10000 steps...
Acceptance fraction: 0.1536




In [30]:

# Pull m, b and q arrays out of the Markov chain and plot them:
mm = [m for m,b,q in qchain]
bb = [b for m,b,q in qchain]
qq = [q for m,b,q in qchain]

# Traces, for convergence inspection:
plt.figure(figsize=(8,5))
plt.subplot(3,1,1)
plt.plot(mm, 'k-')
plt.ylim(mlimits)
plt.ylabel('Slope m')
plt.subplot(3,1,2)
plt.plot(bb, 'k-')
plt.ylim(blimits)
plt.ylabel('Intercept b')
plt.subplot(3,1,3)
plt.plot(qq, 'k-')
plt.ylim([qpars[0]-3*qpars[1],qpars[0]+3*qpars[1]])




Out[30]:

<matplotlib.text.Text at 0x1076a1d90>




In [31]:

corner.corner(qchain, labels=['m','b','q'], range=[mlimits,blimits,(qpars[0]-3*qpars[1],qpars[0]+3*qpars[1])],quantiles=[0.16,0.5,0.84],
show_titles=True, title_args={"fontsize": 12},
plot_datapoints=True, fill_contours=True, levels=[0.68, 0.95],
color='green', bins=80, smooth=1.0);





• All parameters are again precisely constrained.
• The gradient and intercept $m$ and $b$ are significantly different from before, though...

Checking the Quadratic Model



In [32]:

# Posterior visual check, in data space:
X = np.linspace(xlimits[0],xlimits[1],100)
for i in (np.random.rand(100)*len(chain)).astype(int):
m,b,q = qchain[i]
plt.plot(X, b + X*m + q*X**2, 'g-', alpha=0.1)
plot_line(m_ls, b_ls);
plot_yerr(x, y, sigmay)







In [33]:

# Discrepancy: functions of the data AND parameters.

# 1) Reduced chisq for the model:
def test_statistic(x,y,sigmay,m,b,q):
return np.sum((y - m*x - b - q*x**2)**2.0/sigmay**2.0)/(len(y)-3)

# 2) Some other discrepancy measure:

# Approximate the posterior predictive distribution for T,
# by drawing a replica dataset for each sample (m,b) and computing its T,
# AND ALSO its Td:
T = np.zeros(len(qchain))
Td = np.zeros(len(qchain))
for k,(m,b,q) in enumerate(qchain):
yp = b + m*x + q*x**2 + sigmay*np.random.randn(len(x))
T[k] = test_statistic(x,yp,sigmay,m,b,q)
Td[k] = test_statistic(x,y,sigmay,m,b,q)

# Histogram of differences:
diff = T - Td
plt.hist(diff, 100, histtype='step', color='green', lw=2, range=(np.percentile(diff,1.0),np.percentile(diff,99.0)))
plt.axvline(0.0, color='black', linestyle='--', lw=2)
plt.xlabel('Difference $T(d^{\\rm rep},\\theta) - T(d,\\theta)$')
plt.ylabel('Posterior predictive distribution')

# What is Pr(T>T(d)|d)?
greater = (T > Td)
print("Pr(T>T(d)|d,quadratic) = ",Pquad,"%, cf. Pr(T>T(d)|d,straightline) = ",Pline,"%")




Pr(T>T(d)|d,quadratic) =  92.55 %, cf. Pr(T>T(d)|d,straightline) =  73.29 %


• How do the two models compare? Which one matches the data better?

All of the above discussion was about model checking - assessment of the ability of a model to make accurate predictions.

• We used replicated data, drawn from the model assuming it was true, and then looked at the probability of getting (a summary of) the data, given this assumption.
• Note the parallel with frequentist hypothesis testing:

Frequentist: assume the null hypothesis $H_0$, and calculate the probability of getting the test statistic (designed according to the alternative hypothesis $H_1$) larger than the observed one, by studying the distribution of a test statistic over a large ensemble of replica datasets (which under certain assumptions is a standard distribution).

Bayesian: assume the alternative hypothesis $H_1$, and calculate the posterior predictive probability distribution for the test statistic given the data, relative to the one test statistic we observed, marginalizing over the model parameters. In general this distribution will be non-standard, but we can often draw samples from the posterior PDF anyway.

• The Bayesian posterior predictive check is fairly conservative, by comparison with tests that focus on the best-fit parameters. This can be a good thing, to err on the side of caution.

Model Comparison with the Bayesian Evidence

• The evidence for model $H$, ${\rm Pr}(d\,|\,H)$, enables a form of Bayesian hypothesis testing via the evidence ratio (or "Bayes Factor"):

$R = \frac{{\rm Pr}(d\,|\,H_1)}{{\rm Pr}(d\,|\,H_0)}$

• This quantity is similar to a likelihood ratio, but it's a fully marginalized likelihood ratio - which is to say that it takes into account our uncertainty about values of the parameters of each model by integrating over them all.
• As well as predictive accuracy, the other virtue a model can have is efficiency. The evidence summarizes all the information we put into our model inferences, via both the data and our prior beliefs. You can see this by inspection of the integrand of the fully marginalized likelihood (#FML) integral:

${\rm Pr}(d\,|\,H) = \int\;{\rm Pr}(d\,|\,\theta,H)\;{\rm Pr}(\theta\,|\,H)\;d\theta$

• The consequence of this is that the evidence depends on both model accuracy (goodness of fit, ability to predict data) and efficiency (not over-fitting by having implausible flexibility).

• The following figure might help illustrate how the evidence depends on both goodness of fit (through the likelihood) and the complexity of the model (via the prior). In this 1D case, a Gaussian likelihood (red) is integrated over a uniform prior (blue): the evidence can be shown to be given by $E = f \times L_{\rm max}$, where $L_{\rm max}$ is the maximum possible likelihood, and $f$ is the fraction of the blue dashed area that is shaded red. $f$ is 0.31, 0.98, and 0.07 in each case.



In [34]:

from IPython.display import Image
Image('evidence.png')




Out[34]:



The illustration above shows us a few things:

1) The evidence can be made arbitrarily small by increasing the prior volume: the evidence is more conservative than focusing on the goodness of fit ($L_{\rm max}$) alone. Of course if you assign a prior you don't believe, then you should not expect to get out a meaningful answer for ${\rm Pr}(d\,|\,H)$.

2) The evidence is linearly sensitive to prior volume ($f$), but exponentially sensitive to goodness of fit ($L_{\rm max}$). It's still a likelihood, after all.

• The odds ratio can, in principle, be combined with the ratio of priors for each model to give us the relative probability for each model being true, given the data:

$\frac{{\rm Pr}(H_1|d)}{{\rm Pr}(H_0|d)} = \frac{{\rm Pr}(d|H_1)}{{\rm Pr}(d|H_0)} \; \frac{{\rm Pr}(H_1)}{{\rm Pr}(H_0)}$

• Prior probabilities are very difficult to assign in most practical problems (notice that no theorist ever provides them). So, one way to interpret the evidence ratio is to note that:

• If you think that having seen the data, the two models are still equally probable,
• then the evidence ratio in favor of $H_1$ is you the odds that you would have had to have been willing to take against $H_1$, before seeing the data.
• That is: the evidence ratio updates the prior ratio into a posterior one - as usual.

Calculating the Evidence

• The FML is in general quite difficult to calculate, since it involves averaging the likelihood over the prior. MCMC gives us samples from the posterior - and these cannot, it turns out, be reprocessed so as to estimate the evidence stably.
• A number of sampling algorithms have been developed that do calculate the evidence, during the process of sampling. These include:

• Nested Sampling (including MultiNest and DNest)
• Parallel Tempering, Thermodynamic Integration
• ...
• If we draw samples from the prior, we can then estimate the evidence via the usual sum over samples,

${\rm Pr}(d\,|\,H) \approx \frac{1}{N_s} \sum_k\;{\rm Pr}(d\,|\,\theta_s,H)$

Simple Monte Carlo:

Consider the simplest possbile posterior inference, the mean of parameter $\theta$: $\bar{\theta} = \int\,\theta\,{\rm Pr}(\theta\,|\,d,H)\,d\theta$

This is approximated by an average over posterior samples:

$\bar{\theta} \approx \frac{1}{N_s}\,\sum_s\,\theta_s$

Now replace the posterior PDF with Bayes' Theorem:

$\bar{\theta} = \frac{1}{Z} \int\,\theta\,{\rm Pr}(d\,|\,\theta,H)\,{\rm Pr}(\theta\,|\,H)\,d\theta$

and the posterior samples with prior samples:

$\bar{\theta} \approx \frac{1}{(Z N_s)}\,\sum_s\,\theta_s\,{\rm Pr}(d\,|\,\theta_s,H)$

This is a weighted mean - if we don't want $Z$, we just define weights $w_s = {\rm Pr}(d\,|\,\theta_s,H)$ compute the approximate posterior mean as the likelihood-weighted prior mean:

$\bar{\theta} \approx \frac{\sum_s\,w_s\,\theta_s}{\sum_s\,w_s}$

To compute Z, we multiply both sides by $Z$ and replace $\theta$ with 1:

$Z \approx \frac{1}{N_s} \sum_s\,\,w_s$

• Simple Monte Carlo works well in certain low-dimensional situations, but in general it is very inefficient (at best).
• Still, let's give it a try on our two models, and attempt to compute the Bayes Factor

$R = \frac{{\rm Pr}(d\,|\,{\rm quadratic})}{{\rm Pr}(d\,|\,{\rm straight line})}$



In [35]:

# Draw a large number of prior samples and calculate the log likelihood for each one:
N = 50000

# Set the priors:
mlimits = [0.0, 2.0]
blimits = [0.0, 200.0]
qpars = [0.0,0.003]

# Sample from the prior:
mm = np.random.uniform(mlimits[0],mlimits[1], size=N)
bb = np.random.uniform(blimits[0],blimits[1], size=N)
qq = qpars[0] + qpars[1]*np.random.randn(N)

# We'll store the posterior samples as a "chain" again
schain = []

log_likelihood_straight_line = np.zeros(N)
for i in range(N):
theta = np.array([mm[i], bb[i]])
log_likelihood_straight_line[i] = straight_line_log_likelihood(theta, x, y, sigmay)
qtheta = np.array([mm[i], bb[i], qq[i]])

schain.append((mm[i],bb[i],qq[i]))



Now that we have the log likelihood for each sample, let's check that we did actually sample the posterior well. Here are the corner plots (note that for plotting, the weights don't need to be correctly normalized - and also that we do not want to plot the points as well as the contours, since the points are prior samples not posterior ones!):



In [36]:

# Unnormalized likelihoods for plotting:

unnormalized_likelihood_straight_line = np.exp(log_likelihood_straight_line - log_likelihood_straight_line.max())




In [37]:

corner.corner(schain, labels=['m','b','q'], range=[mlimits,blimits,(qpars[0]-3*qpars[1],qpars[0]+3*qpars[1])],quantiles=[0.16,0.5,0.84],
weights=unnormalized_likelihood_straight_line,
show_titles=True, title_args={"fontsize": 12},
plot_datapoints=False, fill_contours=True, levels=[0.68, 0.95],
color='blue', bins=80, smooth=1.0);