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Approximate Bayesian Computation for State Space Models Worapree (Ole) Maneesoonthorn Melbourne Business School, The University of Melbourne Joint work with Gael M. Martin, Brendan C.P. McCabe & Christian Robert December 2014 Thailand Development Research Institute Maneesoonthorn () ABC for state space models December 2014 Thailand Development Resear / 36

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Page 1: Approximate Bayesian Computation for State Space Modelstdri.or.th/wp-content/uploads/2014/12/Maneesoonthorn_ABC_TDRI.pdf · Approximate Bayesian Computation for State Space Models

Approximate Bayesian Computation for StateSpace Models

Worapree (Ole) ManeesoonthornMelbourne Business School, The University of Melbourne

Joint work withGael M. Martin, Brendan C.P. McCabe & Christian Robert

December 2014Thailand Development Research Institute

Maneesoonthorn () ABC for state space modelsDecember 2014 Thailand Development Research Institute 1

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Presentation outline

Presentation outline

• State space models and Bayesian inference• Approximate Bayesian Computation (ABC)• Our framework• Illustration using stochastic volatility models• Conclusions

Maneesoonthorn () ABC for state space models TDRI 2014 2 / 36

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State space models

State space models

• Structural time series model with hidden/unobserved components• Simplest form - linear-Gaussian model• Example:

yt = Trendt + etTrendt = β0 + β1Trendt−1 + ut

• Observed component: yt ; unobserved component: Trendt• Random components: et ∼ N

(0, σ2e

)and ut ∼ N

(0, σ2u

)• Inference about φ = (β0, β1, σu)

/ via maximum likelihood

• ⇒Kalman filter to obtain closed-form

Maneesoonthorn () ABC for state space models TDRI 2014 3 / 36

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State space models

State space models

• In general, the state space model can be written as

yt = f (xt , et , φ)

xt = g (xt−1, ut , φ)

where φ denotes a vector of static parameters

• f (.) and g (.) are potentially nonlinear• Densities p (et ) and p (ut ) are potentially non-Gaussian

• Example: stochastic volatility with student-t error

yt =√xtet

xt = β0 + β1xt−1 + σu√xt−1ut

where et ∼ tν (0, 1) and ut ∼ TN (0, 1)

Maneesoonthorn () ABC for state space models TDRI 2014 4 / 36

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State space models

State space models

• Inference of nonlinear/non-Gaussian state space models - diffi cult!• Likelihood cannot be evaluated in closed form

p (y1, ..., yT |φ) =T

∏t=1p (yt |y1, ..., yt−1,φ)

• with

p (yt |y1, ..., yt−1,φ) =∫p(yt |xt , y1, ..., yt−1, φ)p (xt |y1, ..., yt−1, φ) dxt

Maneesoonthorn () ABC for state space models TDRI 2014 5 / 36

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State space models

State space models

Inference of nonlinear/non-Gaussian state space model:

• Working with approximations• INLAR approximations• Mixtures of linear-Gaussians• ⇒estimate the approximating model

• Simulation based methods• Simulated maximum likelihood• Particle filtering

• Bayesian updating schemes• Simulating from proposed (approximating) model• Correct the draw via an updating scheme based on posterior densities

Maneesoonthorn () ABC for state space models TDRI 2014 6 / 36

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Bayesian inference

Classical vs Bayesian inference

• Classical frequentist inference• Latent state variable to be integrated out• Point estimates of parameters φ + Central Limit Theorem from MLEtheory

• Dynamic state - implied by parameter estimates

• Bayesian inference• Possible to estimate all unknowns - parameters φ + states x• Data-based inference via posterior distributions• Integration - by simulation

Maneesoonthorn () ABC for state space models TDRI 2014 7 / 36

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Bayesian inference

Bayesian inference

• Objective is to estimate

p (φ, x |y) = p (y |x , φ) p (x |φ) p (φ)p (y)

By sampling model unknowns iteratively the Markov chain from• φ ∼ p (φ|x , y)• x ∼ p (x |φ, y)

• Posterior in inference

p (φ|y) =∫p (φ, x |y) dx

p (x |y) =∫p (φ, x |y) dφ

by numerical integration

Maneesoonthorn () ABC for state space models TDRI 2014 8 / 36

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Bayesian inference

Bayesian inference

• Vast literature on Bayesian inference in state space setting• Markov chain Monte Carlo (MCMC), Particle MCMC, sequentialMonte Carlo (SMC)...

• However, these methods are not black box• High level expertise to develop• Convergence issues• Time consuming• Not widely applied by non-technical experts

• We propose a simpler alternative based on Approximate BayesianComputation (ABC)• Producing simulation-based estimate of an approximation to p (φ, x |y)

Maneesoonthorn () ABC for state space models TDRI 2014 9 / 36

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ABC

Approximate Bayesian computation - in brief

Aim:

• Produce i.i.d. draws from an approximation to p (φ, x |y)• Use draws to estimate that approximation• Employing a simple accept/reject algorithm

Need:

• To be able to simulate from p (x |φ) exactly• To be able to simulate from p (y |x , φ) exactly

Recent review: Marin, Publo, Robert & Ryder (2011)

Maneesoonthorn () ABC for state space models TDRI 2014 10 / 36

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ABC

Approximate Bayesian computation - in brief

Steps: for i = 1, ...,R

1 Simulate φi from p (φ)

2 Simulate x i from p(x |φi

)3 Simulate psuedo-data z i from the conditional likelihood p

(z |x i , φi

)4 Select

(x i , φi

)such that

d

η (y) , η(z i)≤ ε

where

• η (.) is a vector of summary statistics,• d. is a distance criterion• ε is an arbitrarily small tolerance

Maneesoonthorn () ABC for state space models TDRI 2014 11 / 36

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ABC

Approximate Bayesian computation - in brief

When η (.) is suffi cient and ε→ 0

• ⇒selected draws of(x i , φi

)⇒ p (φ, x |y)

• ... giving exact inference, up to simulation erro

When η (.) is not suffi cient

• ⇒selected draws of(x i , φi

)⇒ p (φ, x |η (y)) only

Choice of η (.) is usually problem-specific - still an open topic

• Joyce & Marjoram, 2008; Blum, 2010; Fearnhead & Prangle, 2012;Gleim & Pigorsch, 2013

• No general discussion in a state space setting

Maneesoonthorn () ABC for state space models TDRI 2014 12 / 36

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ABC

ABC and suffi ciency

How to render η(.) ‘close to’suffi cient in a state space model (SSM)setting?

• Linear Gaussian SSM ≡ ARMA model• ⇒ no reduction to suffi cient statistics (due to MA component)• ⇒ would not expect ABC based on arbitrary summary statistics(calculated from y) to perform well

Confirmed by numerical experimentation

• signal to noise ratio playing a role• dimension of η(.) also a problem (the ‘multiple matching’problem)

Maneesoonthorn () ABC for state space models TDRI 2014 13 / 36

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Our framework

Our approach to ABC

• In the spirit of indirect inference:• Gourieroux et al, 1993; Heggland and Frigessi, 2004

• think about a model that approximates the true (analyticallyintractable) SSM

• with associated likelihood function: LA(β; y)• Apply maximum likelihood estimation to LA(β; .) to produce β

• β asymptotically suffi cient for β in the approximate model• (β also asymptotically suffi cient for φ in the true model if true ∈approximate)

• If approximating model is ‘accurate’enough• β may be ‘close to’being suffi cient for φ in the true model

Maneesoonthorn () ABC for state space models TDRI 2014 14 / 36

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Our framework

Our approach to ABC

• Setting η(.) = β is computationally burdensome (optimizationrequired at each iteration of ABC.......)

• Instead, in the spirit of effi cient method of moments

• Gallant and Tauchen, 1996; Gallant and Long, 1997

• construct summary statistic as the score:

η(.) = S(β; .)|β=β(y) = T−1 ∂ ln LA(β; .)

∂β

∣∣∣∣β=β(y)

• Select ABC draws (φi , x i ) such that:

dη(y)︸︷︷︸=0

, η(z i ) ≤ ε,

• Does the ‘approx. asy. suffi ciency’of β⇒ S(β; .)|β=β(y)?

Maneesoonthorn () ABC for state space models TDRI 2014 15 / 36

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Our framework

• We show that:

dη(y), η(z i ) =√[

S(β(y); z i )]′

Σ[S(β(y); z i )

]≤ ε

and

dη(y), η(z i ) =√[

β(y)− β(z i )]′

Ω[

β(y)− β(z i )]≤ ε

• (for any p.d weighting matrices Σ and Ω)• ⇒ the same selected φi for ε→ 0

• ⇒ same estimate of p(φ|y)• For both:

• exactly identified (dim(β) = dim(φ)) case• over-identified (dim(β) > dim(φ)) case

• Estimates of p(φ|y) ≈ for small enough ε

Maneesoonthorn () ABC for state space models TDRI 2014 16 / 36

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Our framework

Our approach to ABC

• Also show that, for both criteria, (under regularity, and for ε→ 0)

• as T → ∞, p(φ|y) collapses onto the true φ0

• because we will only ever accept draws arbitrarily close to φ0

• ⇒ MLE- (or score-) based inference is (Bayesian) consistent

Maneesoonthorn () ABC for state space models TDRI 2014 17 / 36

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Our framework

Our approach to ABC

• Link between indirect inference and ABC already ackowledged; e.g.• Drovandi et al. (2011) - specific biological model• Drovandi and Pettitt (unpublished, 2013)

• Gleim and Pigorsch (unpublished, 2013) - SSM

• Use a semi-parametric approximating model based on a Hermiteexpansion - Gallant and Tauchen (1989)

• highly parameterized (by construction) - 12 parameters - and tunedto problem at hand

• Our aim is to produce a simple and generic algorithm suitable toany SSM

• Using an easily computed, parsimonious approximating model

Maneesoonthorn () ABC for state space models TDRI 2014 18 / 36

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Our framework

Our approach to ABC

• Steps:1 Define a non-linear/non-Gaussian (discrete time) state space model(SSM) of some sort

2 Apply the (augmented) unscented Kalman filter (AUKF) (Julier,Uhlmann, and Durrant-Whyte, 2000) to evaluate the likelihood:LA(β; y)

3 ⇒ use

η(.) = S(β; .)|β=β(y) = T−1 ∂ ln LA(β; .)

∂β

∣∣∣∣β=β(y)

as the matching statistic in the ABC algorithm

• Key point: computation burden of AUKF ≈ Kalman filter• ⇒ computationally feasible within ABC

Maneesoonthorn () ABC for state space models TDRI 2014 19 / 36

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Illustration

Illustration: Heston (CIR) SV model

• Assume:

rt =√xt εt ; εt ∼ i .i .d .N(0, 1)

dxt = (δ− αxt ) dt + σv√xtdWt ,

• rt = (demeaned) daily log return (observed discretely)• xt = latent variance (evolving continuously)

• Set parameters ⇒ rt and xt that ‘match’returns and realizedvolatility on S&P500 over 2003-2004 period

• Deliberately chose a tranquil period as:• not modelling price (and/or volatility) jumps• adopting conditional Gaussianity for returns

Maneesoonthorn () ABC for state space models TDRI 2014 20 / 36

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Illustration

Illustration: Heston (CIR) SV model

• Transition densities are known:

xt |xt−1 ∼ Non− Central χ2(2cxt ; 2q + 2, 2u)

• Use the exact transitions to produce an exact comparator for theABC estimate

• Applying a grid-based non-linear filtering method of Ng, Forbes,Martin and McCabe (2013)

• (Appropriate for low-dimensional/SSM’s for which xt can be solvedfrom measurement equation)

• ⇒ exact p(φ|y) (up to numerical integration error)• where φ = (k = 1− α, δ, σ2v )

Maneesoonthorn () ABC for state space models TDRI 2014 21 / 36

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Illustration

Illustration: Heston (CIR) SV model

Compare ABC score-based approx. of p(φ|y) with

1 Exact p(φ|y) (produced via grid-based non-linear filter)

2 Euler approximation to p(φ|y) (also produced via grid-basednon-linear filter)

3 AUKF approx. of p(φ|y)

Maneesoonthorn () ABC for state space models TDRI 2014 22 / 36

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Illustration

Illustration: Heston (CIR) SV model

Also of interest to compare ABC score-based approx. of p(φ|y) with

4. ABC approx. of p(φ|y) based on the use of 5 arbitrary summarystatistics

• s1 =T−1∑t=2

yt , s2 =T−1∑t=2

y2t , s3 =T∑t=2ytyt−1, s4 = y1+ yT ,

s5 = y21+ y2T

• suffi cient for an observed AR(1)

Maneesoonthorn () ABC for state space models TDRI 2014 23 / 36

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Illustration

4a. Use Euclidean distance:

dη(y), η(z i ) = [5∑j=1(s ij − sobsj )2/var(sj )]1/2

4b. Use dimension reduction method of Fearnhead and Prangle (2012).Steps:

1 For each scalar parameter φk regress φik on si =

[s i1, s

i2, s

i3, s

i4, s

i5]for

i = 1, 2, ...,R ⇒(a, b)

2 Define:

η(zi ) = E (φk |zi ) = a+ si bη(y) = E (φk |y) = a+ sobs b

3 And use:

dη(y), η(zi ) = abs(E (φk |y)− E (φk |zi ))

as the distance measure

Maneesoonthorn () ABC for state space models TDRI 2014 24 / 36

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Illustration

Illustration: Heston SV model: results

Fix all parameters other than k = 1− α (volatility persistence): p(k |y)

Maneesoonthorn () ABC for state space models TDRI 2014 25 / 36

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Illustration

To summarize so far.....

Key insights thus far are:

1 finite sample suffi ciency unattainable in SSMs (even in LG case)• ⇒ ABC based on arbitrary summary statistics ; p(φ|y)

2 asymptotic suffi ciency obtained via MLE/score• ‘approximate’suffi ciency accessible only in general non-linear (incl.latent diffusion) SSMs

3 even an inaccurate approximating model can produce an accurate

p(φ|y) via ABC/score

Maneesoonthorn () ABC for state space models TDRI 2014 26 / 36

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Illustration

To summarize so far.....

However......

4. dimensionality of the matching statistics is critical

• if dim(η(.)) = m, ⇒ accuracy of p(φ|η(y)) declines with m (Blum,JASA, 2010)

• in addition to any difference between p(φ|η(y)) and p(φ|y)• Complexity of approximating model increases dimension of η(y)• Hence our focus on a parsimoneous approximation

5. Advocate use of integrated likelihood in multiple parameter settings• ⇒ uni-dimensional score statistic (m = 1) for each parameter φj• Only makes sense dimension of approx. model = dimension of truemodel

Maneesoonthorn () ABC for state space models TDRI 2014 27 / 36

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Illustration

Multiple parameter case: linear Gaussian model

yt = xt + ηt ηt ∼ i .i .d .N(0, σ2η)xt = d + kxt−1 + vt vt ∼ i .i .d .N(0, σ2v )

• φ = (d , k , σ2v ); (σ2η fixed to control signal to noise)

• Use the exact (KF) likelihood to generate score

• ⇒ Enables us to measure gain from exploiting asymptoticsuffi ciency via the likelihood function

• Compared with use of arbitrary (non-suffi cient) summary statistics

• Without the confounding effect of a (potentially inaccurate)approximating model

• Plus gain from moving from joint score ⇒ marginal score(dimension reduction)

Maneesoonthorn () ABC for state space models TDRI 2014 28 / 36

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Illustration

Multiple parameter case: LG model

• Estimates of exact p(k |y) based on:• 1) joint score; 2) marg. score; 3) AR(1) stats (Euclid. distance); 4)AR(1) stats (FP distance)

Maneesoonthorn () ABC for state space models TDRI 2014 29 / 36

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Illustration

Multiple parameter case: LG model

Estimates of exact p(σv |y)

Maneesoonthorn () ABC for state space models TDRI 2014 30 / 36

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Illustration

Multiple parameter case: LG model

Estimates of exact p(d |y)

Maneesoonthorn () ABC for state space models TDRI 2014 31 / 36

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Illustration

Multiple parameter case: LG model

• Box plots (for estimates of p(k |y)) for 100 runs of ABC• High signal to noise:

• Clear ranking: 1) marginal score; 2) joint score; 3) summ. stats (FP);4) summ. stats (Euclidean)

• Marginal score method extremely accurateManeesoonthorn () ABC for state space models TDRI 2014 32 / 36

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Illustration

Multiple parameter case: LG model

• Score methods robust to signal to noise (exact likelihood stillaccessed)

• Two other parameters (σv and d):

• Main ranking still clear:

• 1) marginal score.......... 4) summ. stats (Euclidean)

• No uniform (intermediate) ranking for joint score/FP

• ⇒ shows the tension between the quest for asymptotic suffi ciency(via the joint score) and the quest for dimension reduction (via theFP regression method)

Maneesoonthorn () ABC for state space models TDRI 2014 33 / 36

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Illustration

Multiple parameter case: SQ model

φ = (k = 1− α, δ) (Hold σ2ν fixed)

Maneesoonthorn () ABC for state space models TDRI 2014 34 / 36

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Conclusion

To Conclude.....

• Use of (the score of) an auxilliary model to generate summarystatistics for ABC in an SSM setting seems promising

• Given that finite sample suffi ciency is unattainable

• (Approximate) asymptotic suffi ciency is a good goal to aim for

• Know that (Bayesian) consistency is also achievable

• Accuracy of the approximating model is always important (as it is inII/EMM)

Maneesoonthorn () ABC for state space models TDRI 2014 35 / 36

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Conclusion

To Conclude.....

• However, for auxiliary models with higher dimension

• ⇒ the closer is p(φ|η(y)) to p(φ|y)

• ⇒ the more inaccurate is the ABC estimate of p(φ|η(y))!

• ⇒ marginal score approach may reap benefits

• If not too compromised by the inaccuracy of the auxilliary model

Maneesoonthorn () ABC for state space models TDRI 2014 36 / 36