<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJS</journal-id><journal-title-group><journal-title>Open Journal of Statistics</journal-title></journal-title-group><issn pub-type="epub">2161-718X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojs.2013.32012</article-id><article-id pub-id-type="publisher-id">OJS-30323</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Minimum Description Length Methods in Bayesian Model Selection: Some Applications
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ohan</surname><given-names>Delampady</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Statistics and Mathematics Unit, Indian Statistical Institute, Bangalore, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>mohan.delampady@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>16</day><month>04</month><year>2013</year></pub-date><volume>03</volume><issue>02</issue><fpage>103</fpage><lpage>117</lpage><history><date date-type="received"><day>January</day>	<month>8,</month>	<year>2013</year></date><date date-type="rev-recd"><day>February</day>	<month>10,</month>	<year>2013</year>	</date><date date-type="accepted"><day>February</day>	<month>26,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   Computations involved in Bayesian approach to practical model selection problems are usually very difficult. Computational simplifications are sometimes possible, but are not generally applicable. There is a large literature available on a methodology based on information theory called Minimum Description Length (MDL). It is described here how many of these techniques are either directly Bayesian in nature, or are very good objective approximations to Bayesian solutions. First, connections between the Bayesian approach and MDL are theoretically explored; thereafter a few illustrations are provided to describe how MDL can give useful computational simplifications.
     
 
</p></abstract><kwd-group><kwd>Bayesian Analysis; Model Selection; Minimum Description Length; Hierarchical Bayes; Bayesian Computations</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Bayesian computations can be difficult, in particular those in model selection problems. For instance, it may be noted that learning the structure of Bayesian networks is in general of the computational complexity type NPcomplete ([1,2]). It is therefore meaningful to consider alternative computationally simpler solutions which are approximations to Bayesian solutions. Sometimes direct computational simplifications are possible, as shown, for example, in [<xref ref-type="bibr" rid="scirp.30323-ref3">3</xref>], but often approaches arising out of different methodologies are needed. We discuss some aspects of Minimum Description Length (MDL) methods with this point of view. Another important reason for exploring these methods is that there is a substantial literature on this topic available in engineering and computer science with potential applications in statistics. We will not, however, explore certain other aspects of MDL such as the “Normalized Maximum Likelihood (NML)” introduced by [<xref ref-type="bibr" rid="scirp.30323-ref4">4</xref>] which do not seem to be in the spirit of the Bayesian approach that we have taken here.</p><p>The discussion below is organized as follows. In Section 2 we briefly describe the MDL principle and then indicate in Sections 3 and 4 how it applies to model fitting and model checking. It is shown that a particular version of MDL is equivalent to the Bayes factor criterion of model selection. Since this is computationally difficult most often, some approximations are desirable, and it is next shown how a different version of MDL can provide such an approximation. Following this discussion, new applications are presented in Section 5. Specifically, MDL approach to step-wise regression in Section 5.1, wavelet thresholding in 5.2 and a change-point problem in 5.3 are described.</p></sec><sec id="s2"><title>2. Minimum Description Length Principle</title><p>The MDL approach to model fitting can be described as follows (see [5,6]). Suppose we have some data. Consider a collection of probability models for this set of data. A model provides a better fit if it can provide a more compact description for the data. In terms of coding, this means that according to MDL, the best model is the one which provides the shortest description length for the given data. The MDL approach as discussed here is also related to the Minimum Message Length (MML) approach of [<xref ref-type="bibr" rid="scirp.30323-ref7">7</xref>]. See [8,9] for connections to information theory and other related details.</p><p>If data <img src="5-1240178\10c957ab-748c-44ee-911a-d34196e6afb3.jpg" /> is known to arise from a probability density<img src="5-1240178\3ddfc6c4-0fbf-4372-83b5-c6027c835cc0.jpg" />, then (see [<xref ref-type="bibr" rid="scirp.30323-ref10">10</xref>] or [<xref ref-type="bibr" rid="scirp.30323-ref11">11</xref>]) the optimal code length (in an average sense) is given by<img src="5-1240178\144142ac-8920-408e-8201-672676c688d6.jpg" />. (Here <img src="5-1240178\0a6a5c93-9e5c-475f-81a0-babbf7a5d3f1.jpg" /> is logaritm to the base 2.) This is the link between description length and model fitting.</p><p>The optimal code length of <img src="5-1240178\aa5793bf-ba42-405b-9449-f50ba056fbd1.jpg" /> is valid only in the discrete case. To handle the continuous case later, discretize x and denote it by <img src="5-1240178\c054259d-3b33-4e45-9fb5-0b510f75fb5c.jpg" /> where <img src="5-1240178\8da6f4bc-d2dd-4e30-8de6-d90fa1a021fa.jpg" /></p><p>denotes the precision. In effect we will then be considering</p><p><img src="5-1240178\00544120-a749-43d1-be73-473baa7c6877.jpg" /></p><p>instead of <img src="5-1240178\de1d5c65-dbc4-4c78-b119-d78f6d44f0b5.jpg" /> itself as far as coding of x is considered when x is one-dimensional. In the r-dimensional case, we will replace the density <img src="5-1240178\e0ee6d51-65a2-412d-b08a-bdc69e6b6ccf.jpg" /> by the probability of the <img src="5-1240178\2bf36710-3c45-450e-8af0-8ab9b2d3cd67.jpg" />-dimensional cube of side <img src="5-1240178\3612c8f1-eb86-42bd-86d8-c04a920fc9d3.jpg" /> containing<img src="5-1240178\0683e733-018b-49bf-8148-c69a6aa2ea83.jpg" />, namely<img src="5-1240178\09d4e4c5-28f8-4177-b883-40a6c2929375.jpg" />, so that the optimal code length changes to<img src="5-1240178\580401a0-613d-4f80-b37d-c756d1c40eae.jpg" />.</p></sec><sec id="s3"><title>3. MDL for Estimation or Model Fitting</title><p>Consider data<img src="5-1240178\38e3f538-ce13-4d20-b118-471749ce982d.jpg" />, and suppose</p><p><img src="5-1240178\6a484dce-7ff5-4f4b-b192-00719d828269.jpg" /></p><p>is the collection of models of interest. Further, let <img src="5-1240178\2cbbe53c-d7c3-42fa-b6a0-576d8e130401.jpg" /> be a prior density for<img src="5-1240178\3db24a00-84d7-469b-844f-600ca4038b84.jpg" />. Given a value of <img src="5-1240178\9e79e41c-68c7-4e70-a634-0a4616fac28c.jpg" /> (or a model), the optimal code length for describing <img src="5-1240178\8f60d2d9-afcf-4ee7-80c0-19fd727b7035.jpg" /> is<img src="5-1240178\866de672-2ab4-4848-9623-cd24863dd274.jpg" />, but since <img src="5-1240178\862b94c5-6578-4fe5-b39a-456d4880b95d.jpg" /> is unknown, its description requires a further <img src="5-1240178\272e8603-1246-4025-b802-f2f22ac09fe5.jpg" /> bits on average. Therefore the optimal code length is obtained upon minimizing</p><disp-formula id="scirp.30323-formula105183"><label>(1)</label><graphic position="anchor" xlink:href="5-1240178\61d8e61c-7156-48ef-90ae-c8c30ea0c346.jpg"  xlink:type="simple"/></disp-formula><p>so that MDL amounts to seeking that model which minimizes the sum of</p><p>• the length, in bits, of the description of the model, and</p><p>• the length, in bits, of data when encoded with the help of the model.</p><p>Now note that the posterior density of <img src="5-1240178\0fb78dc6-1ff0-4aab-91dd-907bc621b9c9.jpg" /> given the data <img src="5-1240178\467930d0-9827-4306-a83d-4461a478692a.jpg" /> is</p><disp-formula id="scirp.30323-formula105184"><label>(2)</label><graphic position="anchor" xlink:href="5-1240178\653b2cf5-c947-4052-8a36-8c16fa1212a0.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\2648e02f-4b91-4ce2-b35c-8375a6960738.jpg" /> is the marginal or predictive density. Therefore, minimizing</p><p><img src="5-1240178\14acff47-b238-4392-a54b-bb0f4bbc43fb.jpg" /></p><p>over <img src="5-1240178\9ff0453a-a9b1-41fe-91fa-d7a16bac9768.jpg" /> is equivalent to maximizing<img src="5-1240178\68756fa2-cf27-4a3b-ac90-7cffdf45503d.jpg" />. Thus MDL for estimation or model fitting is equivalent to finding the highest posterior density (HPD) estimate of<img src="5-1240178\3aeeb283-0da9-4a1d-a777-125df86ddf6d.jpg" />. Note, however, that a prior <img src="5-1240178\fec2ad93-a356-4f74-bc1c-0e374e85f0ac.jpg" /> is needed for these calculations. The approach that a Bayesian adopts in specifying the prior is not, in general, what is accepted by practitioners of the MDL approach. Therefore, the equivalence of MDL and HPD approaches is either subject to accepting the same prior, or as an asymptotic or similar approximation. MDL mostly prefers an approximately uniform prior when <img src="5-1240178\44a97bc9-a355-45c2-abe5-d0e8cce620ef.jpg" /> for some fixed <img src="5-1240178\de23ec5e-57f6-434a-8010-c79286551a48.jpg" /> (same <img src="5-1240178\47151c27-2fbd-41e7-9b18-43e15b2e896b.jpg" /> across all models), leading to the maximum likelihood estimate (MLE). The case of <img src="5-1240178\c184c69a-35b2-4a8b-9c4d-e89814e9b0cb.jpg" /> having model parameters of different dimensions is different and is interesting. This can be easily seen in the continuous case upon discretization. Now denote <img src="5-1240178\1fc82bfb-dfab-463b-989a-ae5cd4339fad.jpg" /> by <img src="5-1240178\10485a0d-d6e2-4067-9c9d-cb9b242092d6.jpg" /> and <img src="5-1240178\32a02c14-24ef-4309-800d-72e6678cd021.jpg" /> by<img src="5-1240178\b33b0bf1-4672-4687-a772-d9e7b0dff87c.jpg" />. Then</p><p><img src="5-1240178\3ce65558-0c8b-4528-8619-f1874fc56f69.jpg" /></p><p>Here <img src="5-1240178\58f764ce-75c8-4756-aefc-32b484f633a1.jpg" /> and <img src="5-1240178\91f57621-c535-4b61-83e3-9b70593ad92f.jpg" /> are the precisions required to discretize <img src="5-1240178\f6ac5b6e-b5f7-4ffa-bb5b-69e4166b4816.jpg" /> and<img src="5-1240178\c0fdf219-cced-44d6-804c-857ea4800beb.jpg" />, respectively. Note that the term <img src="5-1240178\b05f512e-0673-49cc-ab14-7b9981444ed6.jpg" /> is common across all models, so it can be ignored. However, the term <img src="5-1240178\fe316db2-70b3-40f8-8b98-1d305a3e911c.jpg" /> which involves the dimension of <img src="5-1240178\5f050384-145b-4f02-83f9-bc6473f134d4.jpg" /> in the model varies and is influential. According to [6,12], <img src="5-1240178\63813f3d-2a69-48bd-8c23-0b5f058fbbd7.jpg" />is optimal (see [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>] for details), in which case</p><disp-formula id="scirp.30323-formula105185"><label>(3)</label><graphic position="anchor" xlink:href="5-1240178\c0f20a96-308e-471e-9c02-1c8d8a5963c8.jpg"  xlink:type="simple"/></disp-formula><p>Minimizing this will not lead to MLE even when π(θ<sup>k</sup>) is assumed to be approximately constant. In fact, [<xref ref-type="bibr" rid="scirp.30323-ref12">12</xref>] proceeds further and argues that the correct precision <img src="5-1240178\4ece38a6-c766-4545-9f98-b98a00de3511.jpg" /> should depend on the Fisher information matrix. This amounts to using a prior which is similar in nature to the Jeffreys’ prior on<img src="5-1240178\65dbbb00-cca8-4b11-b02c-7e4df1d148c9.jpg" />. Jeffreys prior is an objective choice and thus this approach to MDL can then be considered a default Bayesian approach.</p><p>In spite of these desirable properties, however, MDL leads to the HPD estimate of<img src="5-1240178\c578d5c5-e457-40b0-a02c-1d9d623407d5.jpg" />, which is not the usual Bayes estimate. Posterior mean is what is generally preferred, so that the error in estimation has an immediate simple answer in the posterior standard deviation. In summary, therefore, the Bayesian approach doesn’t seem to find attractive solutions in the MDL approach as far as estimation or model fitting is concerned unless the models under consideration are hierarchical having parameters of varying dimension. On the other hand, when such hierarchical models are of interest the inference problem usually involves model selection in addition to model fitting. Thus the possible gains from studying the MDL approach are in the context of model selection as described below.</p></sec><sec id="s4"><title>4. Model Selection Using MDL</title><p>Let us recall the Bayesian approach to model selection and express it in the following form. Let</p><p><img src="5-1240178\b1f7d7ca-3fa2-40fd-954c-06b376d7e09b.jpg" />. Suppose</p><p><img src="5-1240178\725ebe69-96fa-403a-b04a-3465679a3fb0.jpg" />. Consider testing</p><disp-formula id="scirp.30323-formula105186"><label>(4)</label><graphic position="anchor" xlink:href="5-1240178\8bdcf436-9706-4d48-b3b6-605b316a826e.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="5-1240178\c372ef03-1377-4c9c-8eed-0e4bb1980292.jpg" />, for some<img src="5-1240178\b905e325-c393-4b04-855b-80d07c80fee5.jpg" /> and<img src="5-1240178\59246657-4244-4354-bc30-e83502a83de6.jpg" />. Let <img src="5-1240178\2ff9b19c-bba3-4526-ba71-96ffd6cbd494.jpg" /> be a prior on<img src="5-1240178\f46ce463-468b-41f6-b428-f0fa634f8562.jpg" />. Then <img src="5-1240178\c7f20a48-41f6-47fb-a660-b2901767a63c.jpg" /> can be expressed as</p><disp-formula id="scirp.30323-formula105187"><label>(5)</label><graphic position="anchor" xlink:href="5-1240178\25983961-25a7-4c30-b4a8-838bcdd8050e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\c45fae30-c7d6-409b-b8cd-09169a9247fd.jpg" /> and <img src="5-1240178\692fd8c9-82b1-4792-a748-f50959db4a65.jpg" /> and <img src="5-1240178\2888e535-3edb-4858-a3c2-2d707306ab7a.jpg" /> are the conditional densities (with respect to some dominating <img src="5-1240178\fbcfca27-dbd3-4406-a9ed-25d81fdee9e3.jpg" />- finite measure) of <img src="5-1240178\ed1ccf37-db1d-4b83-8be5-c3dbd15cf5b3.jpg" /> under <img src="5-1240178\386ecbb6-8189-424f-be37-f2d7fc1736a2.jpg" /> and <img src="5-1240178\8abcd44a-a545-4880-9f7c-429197a488c8.jpg" /> respectively. Then</p><disp-formula id="scirp.30323-formula105188"><label>(6)</label><graphic position="anchor" xlink:href="5-1240178\2ec26a18-9dfb-48ab-ba0c-1fb91013e000.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.30323-formula105189"><label>(7)</label><graphic position="anchor" xlink:href="5-1240178\ced55cc8-d497-4081-8d72-cb41a7a42368.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.30323-formula105190"><label>(8)</label><graphic position="anchor" xlink:href="5-1240178\90b8126d-b18e-4422-9846-8063028b4ffc.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.30323-formula105191"><label>(9)</label><graphic position="anchor" xlink:href="5-1240178\5a97eeca-303f-4228-8ce2-5d2da89ee542.jpg"  xlink:type="simple"/></disp-formula><p>Note that <img src="5-1240178\c82e7361-979b-43a4-8193-62ffa32bf12b.jpg" /> is simply the marginal or predictive density of <img src="5-1240178\42702749-e504-4478-9d2e-b38f41a8cda9.jpg" /> under <img src="5-1240178\88298428-07e7-410c-abb5-7ae1734e57b3.jpg" /> and <img src="5-1240178\5f3aec5d-89ae-4a4a-a31c-d5f454af9c21.jpg" /> is the unconditional predictive density obtained upon averaging <img src="5-1240178\bdb6d15f-0b5c-4a7a-995a-36476580caaf.jpg" /> and<img src="5-1240178\2f189d9f-4aa3-4624-8dc8-acc4ee77d467.jpg" />. Consequently, the posterior odds ratio of <img src="5-1240178\4d278b1c-12cd-491d-9658-e04b20ba1db9.jpg" /> relative to <img src="5-1240178\b946b6bd-a80a-4158-8f81-51f7e2453b18.jpg" /> is,</p><disp-formula id="scirp.30323-formula105192"><label>(10)</label><graphic position="anchor" xlink:href="5-1240178\09f7aac1-141e-4d52-a852-4fbbf55a7c38.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="5-1240178\1b835d61-ac4b-4890-ae94-87db6ad151d9.jpg" /> denoting the Bayes factor of <img src="5-1240178\759adc9f-0a80-4711-a300-41e07c7ec364.jpg" /> relative to<img src="5-1240178\084e12df-730d-4642-8b8f-69093923414c.jpg" />. When we compare two competing models <img src="5-1240178\e3a1e562-e56a-41f4-ad21-c66950cff592.jpg" /> and<img src="5-1240178\4e21c9f7-a5e5-4cad-a08a-bd29bc137f1b.jpg" />, we usually take<img src="5-1240178\b0ade44e-f964-4146-a91c-670982781097.jpg" />, and hence settle upon the Bayes factor <img src="5-1240178\6bfb6445-fede-4201-ba21-73c826e6e3e3.jpg" /> as the model selection tool. This agrees well with the intuitive notion that the model yielding a better predictive ability must be a better model for the given data.</p><sec id="s4_1"><title>4.1. Mixture MDL and Stochastic Complexity</title><p>Let us consider the MDL principle now for model selection between <img src="5-1240178\3f09cc78-1714-4727-9c5d-f6ad60acdea8.jpg" /> and<img src="5-1240178\f56824d0-6490-4cda-8aca-870086641c82.jpg" />. Once the conditional prior densities <img src="5-1240178\4b083ec7-7f71-4054-923a-b2307c8ed88e.jpg" /> and <img src="5-1240178\b30914b7-4fc4-456c-8021-f2e49b52dfcf.jpg" /> are agreed upon, MDL will select that model <img src="5-1240178\f70c9816-2fc9-4d7e-bac7-99ca83e55c24.jpg" /> which obtains a smaller value for the code length, <img src="5-1240178\d128f98c-67af-4bd9-b0ac-e50c7127879b.jpg" />, between the two. This is clearly equivalent to using Bayes factor as the model selection tool, and hence this version of MDL is equivalent to the Bayes factor criterion. In the MDL literature, this version of MDL is known as “mixture MDL”, and is distinguished from the “two-stage MDL” which separately codes the model and the prior. The two-stage MDL can be derived as an approximation to the mixture MDL as discussed later. See [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>] for further details and other interesting comparisons and discussion. Let us consider a few examples before examining the need for other versions of MDL.</p><p>Example 1. Suppose X<sup>n</sup> is a random sample from</p><p><img src="5-1240178\bcfccd03-1b65-4a39-941a-ca8187b50c37.jpg" />with known<img src="5-1240178\fb2ef67e-7ad6-47cd-b8a9-6c35cf484b46.jpg" />. We want to test</p><p><img src="5-1240178\246ddef5-7f08-4dee-bf10-036aba341d63.jpg" /></p><p>Consider the <img src="5-1240178\66fc7947-507e-4ef0-b84b-c4acbf6ef0c1.jpg" /> prior on <img src="5-1240178\9807d928-f543-4a60-97ad-ca5949431f61.jpg" /> with known <img src="5-1240178\fe2eba3e-e299-4e21-ac46-b4006a876b99.jpg" /> under<img src="5-1240178\f92980e2-e049-4043-a7b1-6d17d32b62cb.jpg" />. Then the marginal distribution of <img src="5-1240178\600a1db6-6c1e-44b1-8fb6-cbad295e2747.jpg" /> is</p><p><img src="5-1240178\8a2261c9-bbf9-464f-bb94-daf3c0cca1a3.jpg" />under <img src="5-1240178\87947a9b-bcaa-42d1-b013-2b0b8e97bb65.jpg" /> and under <img src="5-1240178\1a6502db-2da2-4325-8e32-776b6dfe3d42.jpg" /> it is</p><p><img src="5-1240178\8cbb3511-9ef9-479a-a355-ad3eb5f7079d.jpg" />. A continuous model and a continuous prior is considered here. Since the precision of the prior parameter is the same across all models upon discretization we will ignore the distinction and proceed with densities. Then, both the Bayes factor criterion and the MDL principle will select <img src="5-1240178\98c1e99b-fc56-40ba-925e-63de8f3be91f.jpg" /> over <img src="5-1240178\87c3d86b-15c0-436c-b204-9e0e721e832c.jpg" /> if and only if</p><p><img src="5-1240178\4cd38704-38db-4fed-a265-102dda3f065c.jpg" /></p><p>where <img src="5-1240178\b36a17c8-9eb0-40bf-a62b-62d407b0dab6.jpg" /> and <img src="5-1240178\32c47154-9917-453b-9e18-dc1a7727ecf3.jpg" /> are the corresponding densities. Since we are comparing two logarithms, let us switch to natural logarithms. Then</p><p><img src="5-1240178\542ba3ac-e9c8-49e8-8fe9-5e4ae01ad901.jpg" />and</p><p><img src="5-1240178\7c57d8e8-061b-4394-953e-f67cf1bce203.jpg" /></p><p>Noting that</p><p><img src="5-1240178\4e2d639d-7e04-4081-8201-0c91bb450b5e.jpg" /></p><p>and</p><p><img src="5-1240178\a3889ab7-7211-4789-8339-99041b0959b8.jpg" /></p><p>we obtain</p><p><img src="5-1240178\d3002ee9-2b8e-4240-bb44-b3120f6da3a0.jpg" /></p><p>Therefore <img src="5-1240178\85780ede-0510-4758-ad54-2fcdfdd2dde2.jpg" /> is preferred over <img src="5-1240178\a0ec1f7d-e813-42c1-a214-9463140b66b7.jpg" /> either by the Bayes factor or by the mixture MDL if and only if</p><p><img src="5-1240178\ca601ef1-0c8f-4a24-bb58-30f9f4ebcce3.jpg" /></p><p>Example 2. Let us consider the previous example with unknown <img src="5-1240178\427b9e3d-0549-43c1-8798-6914636a6d39.jpg" /> now. Suppose the prior on <img src="5-1240178\016822df-048c-405b-8606-63c601af5eb2.jpg" /> is the default <img src="5-1240178\e071d931-4be5-45d7-a24f-7054d659df1c.jpg" /> under both models. The prior on <img src="5-1240178\92ec3bb0-05f8-4f2d-8966-41f400fe7cc1.jpg" /> under <img src="5-1240178\2bcad21f-6821-4680-b252-a5314312122d.jpg" /> is now assumed to depend on<img src="5-1240178\a8c05802-6800-4bb1-8f06-8a04cbb4ce07.jpg" />, i.e., <img src="5-1240178\a823d1e3-f91f-48c9-b6a3-940338a86c73.jpg" />, where <img src="5-1240178\b6db7f86-b123-4464-9eda-ab419c092487.jpg" /> is assumed to be a known constant for now. Then, provided<img src="5-1240178\2daf780b-36b3-41f5-bd85-d3f601573780.jpg" />,</p><p><img src="5-1240178\4df03c72-3d6b-4eae-9cb9-cb1a581450d8.jpg" /></p><p>and letting<img src="5-1240178\80816152-da73-47a7-ac04-009eb5e31f76.jpg" />, and <img src="5-1240178\4da8661b-df99-4621-bea0-232943e7acec.jpg" /> denote the marginal density of <img src="5-1240178\539daf91-c883-4977-b870-adf9e7958ff5.jpg" /> given <img src="5-1240178\929201c4-40e1-4f65-8647-204f8afafe40.jpg" /> and<img src="5-1240178\768bb46f-9d44-424b-80da-82e77218635f.jpg" />,</p><p><img src="5-1240178\6b6e3398-517d-4845-9db2-5abd678a3283.jpg" /></p><p>Thus</p><p><img src="5-1240178\d86a6910-e74d-4f25-858b-388510193628.jpg" /></p><p>Therefore, the Bayes factor criterion or the mixture MDL reduces to a criterion which is very similar to that given in the previous example, except that <img src="5-1240178\d6bd5a8f-0c6d-4e10-9e7f-846a1f3ffcdb.jpg" /> is now replaced by an estimator.</p><p>Example 3. (Jeffreys’ Test) This is similar to the problem discussed above, except that<img src="5-1240178\961ccda9-b3a5-40da-b931-ee15109b3739.jpg" />, with density</p><p><img src="5-1240178\bb8881e8-54b4-436e-9f30-bbd6bf27bc0c.jpg" /></p><p>the Cauchy prior. The prior on <img src="5-1240178\a29fd8f4-0f12-4571-9991-e092c1994be7.jpg" /> is the same as before under both models:<img src="5-1240178\70b3d55f-f224-4ce4-8c81-c0b856fc1e14.jpg" />. This approach suggested by Jeffreys ([<xref ref-type="bibr" rid="scirp.30323-ref14">14</xref>]) is important. It explains how one should proceed when the hypotheses which describe the model selection problem involve only some of the parameters and the remaining parameters are considered to be nuisance parameters. Then Jeffreys suggestion is to employ the same noninformative prior on the nuisance parameters under both models, and a proper prior with low level of information on the parameters of interest. Details on this problem along with this choice of prior can be found in Section 2.7 of [<xref ref-type="bibr" rid="scirp.30323-ref15">15</xref>].</p><p>Note that <img src="5-1240178\3e21dad9-47db-4a34-a00a-706c14525678.jpg" /> is the same as in the previous example, namely</p><p><img src="5-1240178\eb21c596-b116-47fa-b3c3-b2102b2970e2.jpg" /></p><p>whereas</p><p><img src="5-1240178\37a92765-da33-4695-aa14-8b270293e930.jpg" /></p><p>No closed form is available for m<sub>1</sub>(x<sup>n</sup>) in this case. To calculate this one can proceed as follows as indicated in Section 2.7 of [<xref ref-type="bibr" rid="scirp.30323-ref15">15</xref>]. The Cauchy density <img src="5-1240178\cfcf4161-c018-41fa-9adc-8044662b85d6.jpg" /> can be expressed as a Gamma scale mixture of normals,</p><p><img src="5-1240178\4d555ef0-413b-464c-a6ac-aa6ff832fa86.jpg" /></p><p>where <img src="5-1240178\c55ac290-cbe7-4b33-b711-b19a07c0d4c6.jpg" /> is the mixing Gamma variable. Now one can integrate over <img src="5-1240178\e9c420b5-3a6e-40b9-bf9c-80f78f9825df.jpg" /> and <img src="5-1240178\8e67a351-71dc-48c9-b7c2-6366601ca56e.jpg" /> in closed form to simplify (m<sub>1</sub>x<sup>n</sup>). Finally, one has a one-dimensional integral over <img src="5-1240178\07144a29-5a31-4490-a651-594a84a5de99.jpg" /> left, which can be numerically computed whenever needed.</p><p>Now, let us note from the examples discussed above that an efficient computation of m<sub>i</sub>(x<sup>n</sup>) relies on having an explicit functional form for it. This is generally possible only when a conjugate prior is used as in Examples 1 and 2. For other priors, such as in Example 3, some numerical approximation will have to be employed. Thus we are lead to considering possible approximations to the mixture MDL technique, or equivalently to the Bayes factor,<img src="5-1240178\9eab06b4-5ea5-44fb-9ec0-5640ac1d3d4a.jpg" />.</p><p>From Sections 4.3.1 and 7.1 of [<xref ref-type="bibr" rid="scirp.30323-ref15">15</xref>], assuming that <img src="5-1240178\954e309f-a0aa-4e71-a60a-26e31585b311.jpg" /> and <img src="5-1240178\5d7c7524-309c-4d8a-98ee-8a5f392865e2.jpg" /> are smooth functions, we obtain, for large<img src="5-1240178\e48c4849-ceea-45d5-955a-e5d3b2e91c6d.jpg" />, the following asymptotic approximation for <img src="5-1240178\3767a3e0-29a9-433e-917d-db814a728d57.jpg" /> of equation (8). Let <img src="5-1240178\e61296ee-63ab-426d-ac2c-d45c21d986da.jpg" /> be the dimension of<img src="5-1240178\fa790353-404a-4494-b70f-5613f12aad15.jpg" />,</p><p><img src="5-1240178\add3abaa-81f2-4ea8-9c5f-f42cefe9fb55.jpg" />and <img src="5-1240178\b8945139-6742-485c-8f8c-0792b7802310.jpg" /> denote the Hessian of<img src="5-1240178\cea50372-659a-4291-bd93-d0c8b0ffffd4.jpg" />, i.e.,</p><p><img src="5-1240178\ccfb47fd-7c0b-464d-bc67-897ad9b4f23a.jpg" /></p><p>Also, let <img src="5-1240178\415d2e71-25b0-474e-b05a-660ff34e5424.jpg" /> denote either the MLE or the posterior mode. Then</p><disp-formula id="scirp.30323-formula105193"><label>(11)</label><graphic position="anchor" xlink:href="5-1240178\be35fb2c-40b6-499c-875e-8c2e5673fca7.jpg"  xlink:type="simple"/></disp-formula><p>so that</p><disp-formula id="scirp.30323-formula105194"><label>(12)</label><graphic position="anchor" xlink:href="5-1240178\d3434f53-128d-4cb5-87b8-3cbd8de33bc6.jpg"  xlink:type="simple"/></disp-formula><p>Ignoring terms that stay bounded as<img src="5-1240178\fd29e185-899b-4dc2-8687-ab662698ffc9.jpg" />, [<xref ref-type="bibr" rid="scirp.30323-ref12">12</xref>] suggests using the (approximate) criterion which Rissanen calls stochastic information complexity (or “stochastic complexity” for short),</p><disp-formula id="scirp.30323-formula105195"><label>(13)</label><graphic position="anchor" xlink:href="5-1240178\e0156f46-a23e-4c28-af62-c5e1372a4c9a.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.30323-formula105196"><label>(14)</label><graphic position="anchor" xlink:href="5-1240178\a6814b9a-0422-4121-949e-e89d0ea82089.jpg"  xlink:type="simple"/></disp-formula><p>for implementing MDL. See [12,16-18] for further details.</p><p>If <img src="5-1240178\2ceb016b-fbb3-431b-a615-54ea98eccb3e.jpg" /> are i.i.d. observations, then we have</p><p><img src="5-1240178\774f60ec-0420-44ea-a28c-67425eb065f1.jpg" /></p><p>where <img src="5-1240178\1a4de937-eff1-49c1-a289-2a41ff8c14ac.jpg" /> is the Fisher Information matrix and hence</p><disp-formula id="scirp.30323-formula105197"><label>(15)</label><graphic position="anchor" xlink:href="5-1240178\e9c6e578-bf5e-499c-8c81-3e124bac3ab6.jpg"  xlink:type="simple"/></disp-formula><p>Now ignoring terms that stay bounded as<img src="5-1240178\a7c9dd6b-e647-4f41-9837-6ee0f8bcb0f3.jpg" />, we obtain the Schwarz criterion ([<xref ref-type="bibr" rid="scirp.30323-ref19">19</xref>]), BIC, for <img src="5-1240178\29c00832-807a-4102-af26-b684a3b30d5d.jpg" /> given by</p><disp-formula id="scirp.30323-formula105198"><label>(16)</label><graphic position="anchor" xlink:href="5-1240178\b14595c8-84a5-4a37-9d39-6fbc0b998648.jpg"  xlink:type="simple"/></disp-formula><p>which can be seen to be asymptotically equivalent to SIC.</p><p>Example 4. [<xref ref-type="bibr" rid="scirp.30323-ref20">20</xref>] discusses a model selection problem for failure time data. The two models considered are exponential and Weibull:</p><p><img src="5-1240178\73b640c4-4d8c-4b51-a863-92f00b3d3261.jpg" /></p><p>versus</p><p><img src="5-1240178\84435b86-7101-48cc-a5ef-c5c5d3f200da.jpg" /></p><p>where <img src="5-1240178\5ec8bd49-e7ec-4857-ada0-e491b409b3ec.jpg" /> and<img src="5-1240178\dedbb711-fe7c-4ecc-a08a-c3524d131372.jpg" />. Model selection criterion of Rissanen is SIC as described in Equations (13) and (14). However, in this problem a better approximation is employed for the mixture MDL, the mixture being Jeffreys mixture, i.e., the conditional prior densities under <img src="5-1240178\c85d7b47-0e95-46c6-beb0-eab2e64a4480.jpg" /> for <img src="5-1240178\2dcaab65-6ff2-47cf-aab8-45bdfdc613c8.jpg" /> are given by</p><p><img src="5-1240178\9446c964-9ea9-48da-935a-ec5e17268bce.jpg" /></p><p>where <img src="5-1240178\47dac945-4d37-4c11-873a-c7d16f2d5ee1.jpg" /> is a compact subset of the relevant parameter space <img src="5-1240178\689b7752-335b-43a8-b3ca-12d3c20dd7da.jpg" /> and<img src="5-1240178\1d323b55-4a12-4d5b-ba0e-6132b70d591a.jpg" />. Consequentlyit follows that,</p><p><img src="5-1240178\10208f10-c03c-4b89-bfd4-222fc34c6889.jpg" /></p><p>where <img src="5-1240178\3ec8a0a9-f4fd-42b0-ba8b-fecdf47a4a1d.jpg" /> is the MLE of <img src="5-1240178\a5bc1752-c781-4c4d-a5d2-c21293be599c.jpg" /> under<img src="5-1240178\8509dc3c-c489-47db-af52-3f32a96eca16.jpg" />. This yields,</p><p><img src="5-1240178\4158e932-3e01-4662-9b21-a83d46fdb154.jpg" /></p><p>Compare this with (15) and note that the term involving <img src="5-1240178\5e1dc169-d804-4892-a36a-02f0a3793a5a.jpg" /> vanishes.</p><p>We would like to note here that many authors [21,22] define the MDL estimate to be the same as the HPD estimate with respect to the Jeffreys’ prior restricted to some compact set <img src="5-1240178\c38963dc-732c-4aa6-ab7f-18f178dd40aa.jpg" /> where its integral is finite:</p><p><img src="5-1240178\36813c7b-d4af-4f32-89c7-8bd051b5784d.jpg" /></p><p>which is the stochastic complexity approach advocated above.</p><p>It must be emphasized that proper priors are being employed to derive the SIC criterion, and hence indeterminacy and inconsistency problems faced by techniques employing improper priors are not a difficulty in this approach. Moreover, this approach can be viewed as an implementable approximation to an objective Bayesian solution.</p></sec><sec id="s4_2"><title>4.2. Two-Stage MDL</title><p>Now consider the two-stage MDL which codes the prior and the likelihood separately and adds the two description lengths. This approach is therefore similar to estimating the parameter <img src="5-1240178\c98859ef-3d86-4353-8b26-5e55699003af.jpg" /> with the HPD estimate when there is an informative prior, or with the MLE, but the resulting minimum description length does have interesting features. To see when and how this approach approximates the above mentioned model selection criterion, let us look at some of the specific details in the two stages of coding. See [12,13] for further details. Again, recall the setup in (4) and (5).</p><p>Stage 1. Let <img src="5-1240178\cbbead09-bf60-4a12-bc8d-9d930053ddd1.jpg" /> be an estimate of <img src="5-1240178\cbf0a420-4986-4359-ade1-085e91417bea.jpg" /> such as the posterior mean, HPD or MLE under<img src="5-1240178\579dc50a-758b-4442-8062-15802ff1a95d.jpg" />. This needs to be coded. Consider the prior density <img src="5-1240178\28c325fa-27e3-4950-9f41-107d707c0f97.jpg" /> conditional on <img src="5-1240178\f5bc360c-82a5-4983-ae14-672b3271d96e.jpg" /> being true. Usually MDL would choose a uniform density. Restrict <img src="5-1240178\aa2e4b23-ccd3-4a63-a9f2-c290e13f0591.jpg" /> to a large compact subset of the parameter space and discretize it as discussed in Section 3 with a precision of<img src="5-1240178\b5280981-efcd-41ba-b529-9c5ee45fa603.jpg" />. Then the codelength required for coding <img src="5-1240178\474a1253-2933-4e42-ba81-7cc45f5b4c13.jpg" /> is</p><disp-formula id="scirp.30323-formula105199"><label>(17)</label><graphic position="anchor" xlink:href="5-1240178\9016b4c6-7573-4329-ab01-e1071fa5e944.jpg"  xlink:type="simple"/></disp-formula><p>Stage 2. Now the data <img src="5-1240178\626d26eb-4c9f-44b1-bb2b-d95cf52a4ef2.jpg" /> is coded using the model density<img src="5-1240178\404189b4-cba5-4701-8399-801336890156.jpg" />. Discretization may again be neededsay with precision<img src="5-1240178\07ac9c2b-899d-41ab-99d1-7c2aef4e4ea1.jpg" />. Thus the description length for coding <img src="5-1240178\c80a6856-9055-4620-a64b-079fde03cf21.jpg" /> will be</p><disp-formula id="scirp.30323-formula105200"><label>(18)</label><graphic position="anchor" xlink:href="5-1240178\8b610282-e90e-411b-bd9d-12c39463652a.jpg"  xlink:type="simple"/></disp-formula><p>Summing these two codelengths, therefore, we obtain a total description length of</p><disp-formula id="scirp.30323-formula105201"><label>(19)</label><graphic position="anchor" xlink:href="5-1240178\f470969e-8917-474b-9eaf-0fc963f62355.jpg"  xlink:type="simple"/></disp-formula><p>Since the second term above, <img src="5-1240178\5487e735-6aea-4e54-85bb-9b35fbf62175.jpg" />, is constant over both M<sub>0</sub> and<img src="5-1240178\108e64e6-e3a2-454a-b0c7-47baf4eafc71.jpg" />, and the third term stays bounded as <img src="5-1240178\9923c635-acdc-4715-937d-434177ab1b06.jpg" /> increases, these two terms are dropped from the MDL two-stage coding criterion. Thus, for regular parametric models, the two-stage MDL simplifies to the same criterion (for<img src="5-1240178\65a72de3-893b-482c-9614-8c2186325631.jpg" />) as BIC, namely,</p><disp-formula id="scirp.30323-formula105202"><label>(20)</label><graphic position="anchor" xlink:href="5-1240178\64237c9c-69f9-494b-8745-da2ac8b46549.jpg"  xlink:type="simple"/></disp-formula><p>In more complicated model selection problems, the two-stage MDL will involve further steps and may differ from BIC.</p><p>It may also be seen upon comparing (19) with (15) that the performance of SIC based MDL should be superior to the simplified two-stage MDL for moderate <img src="5-1240178\75dd49f9-b9ef-493d-9fe4-a19047bf57e3.jpg" /> since SIC uses a better precision for coding the parameter, namely, one based on the Fisher information.</p></sec></sec><sec id="s5"><title>5. Regression and Function Estimation</title><p>Model selection is an important part of parametric and nonparametric regression and smoothing. Variable selection problems in multiple linear regression, order of the spline to fit and wavelet thresholding are some such areas. We will briefly consider these problems to see how MDL methods can provide computationally attractive approximations to the respective Bayesian solutions.</p><sec id="s5_1"><title>5.1. Variable Selection in Linear Regression</title><p>Variable selection is an important and well studied problem in the context of normal linear models. Literature includes [23-32]. We will only touch upon this area with the specific intention of examining useful and computationally attractive approximations to some of the Bayesian methods.</p><p>Suppose we have an observation vector y<sup>n</sup> on a response variable Y and also measurements <img src="5-1240178\43c73146-6c43-4515-bb88-de790e7d5d57.jpg" /> on a set of potential explanatory variables (or regressors). Following [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>], we associate with each regressor<img src="5-1240178\716ffe49-a84c-4fad-9164-94c62180b288.jpg" />, a binary variable<img src="5-1240178\74c3e232-073b-4b15-b8af-6aaf07d02ab5.jpg" />. Then the set of available linear models is</p><disp-formula id="scirp.30323-formula105203"><label>(21)</label><graphic position="anchor" xlink:href="5-1240178\1d8bd768-f2c9-4345-ac04-783660a53b8e.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="5-1240178\b659f7c0-b19f-4623-8d5c-58e400f976ae.jpg" />. Note that <img src="5-1240178\d9274003-1ba5-488c-a151-35bb32907dd1.jpg" /> is, then, a Bernoulli sequence associated with the set of regression coefficients, <img src="5-1240178\dabecff5-5d4e-4dba-b5c3-2f17bd1ea90c.jpg" />also. Let <img src="5-1240178\20eec1b4-bc79-4690-82f6-9c7a92393339.jpg" /> denote the vector of non-zero regression coefficients corresponding to<img src="5-1240178\5b620bab-9d0c-4acf-9ef9-dfe13fad4ee4.jpg" />, and <img src="5-1240178\94948656-6c1a-45c1-9a41-d3eb31986a67.jpg" /> the corresponding design matrix, which results in the model</p><p><img src="5-1240178\3329b26a-5734-4546-afd0-6cee60d35759.jpg" /></p><p>Selecting the best model, then, is actually an estimation problem, i.e., find the HPD estimate of <img src="5-1240178\21809f82-3e5b-4b5c-a712-b4e05cc08520.jpg" /> starting with a prior <img src="5-1240178\63b36a28-4276-436b-a0bb-bd7136ab3284.jpg" /> on <img src="5-1240178\3b1f27c4-d715-49b5-9676-f44f16fcb5a3.jpg" /> and a prior <img src="5-1240178\d272463c-eb61-4560-9686-c7be2d09c33a.jpg" /> on <img src="5-1240178\ad2d74f6-be8c-4b24-91d3-bb428041b035.jpg" /> given<img src="5-1240178\7dc3c536-d305-4669-b738-655da6449af6.jpg" />. The two-stage MDL, which is the simplest, uses the criterion of minimizing</p><disp-formula id="scirp.30323-formula105204"><label>(22)</label><graphic position="anchor" xlink:href="5-1240178\b397acfc-63f8-4a1c-942c-f51fc44d7ede.jpg"  xlink:type="simple"/></disp-formula><p>MLE for <img src="5-1240178\a03d1efe-b3de-4e57-9acb-3f19cebdd335.jpg" /> and <img src="5-1240178\7765e912-b093-4ca5-80ab-02b186dbaae6.jpg" /> given <img src="5-1240178\a5978e02-d19f-496d-b4ab-9466288d7dbc.jpg" /> are easily available:</p><disp-formula id="scirp.30323-formula105205"><label>(23)</label><graphic position="anchor" xlink:href="5-1240178\01e258fb-b032-4771-934d-d1f2b0651d63.jpg"  xlink:type="simple"/></disp-formula><p>Consider the uniform prior on<img src="5-1240178\9d0a1471-0c1c-43e8-b0f7-158051be778b.jpg" />, all <img src="5-1240178\1e553b77-7035-4d9a-9d83-3423fb5c6c00.jpg" /> values receiving the same weight<img src="5-1240178\ba4619ff-16a8-492b-9f93-9bd00abf177d.jpg" />. Using these, we can re-write the MDL criterion as the one which minimizes (as in Example 2)</p><disp-formula id="scirp.30323-formula105206"><label>(24)</label><graphic position="anchor" xlink:href="5-1240178\1520e439-02cf-4430-9fb4-830db0e0d91f.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\27d9b83d-2b78-4fcb-9a2b-68aea124e8ea.jpg" /> is the number of<img src="5-1240178\c125786f-d83d-4790-b4d3-3c0e93e55445.jpg" />.</p><p>We can also derive the mixture MDL or stochastic complexity of a given model<img src="5-1240178\a80cb323-b96c-4b22-830a-828aa0a1c963.jpg" />. If <img src="5-1240178\29eed900-34ac-494c-bcd0-df1cfa8d2324.jpg" /> is the prior density under<img src="5-1240178\3abe3984-2dc4-443a-ac59-7b8f37b393bc.jpg" />,</p><disp-formula id="scirp.30323-formula105207"><label>(25)</label><graphic position="anchor" xlink:href="5-1240178\457c15d5-1ef0-4340-894d-6fe027d510b3.jpg"  xlink:type="simple"/></disp-formula><p>Applying (13), (14) after evaluating the information matrix of the parameters <img src="5-1240178\73c395c1-e74a-4384-95ee-f8b37aa0164d.jpg" /> and ignoring terms that are irrelevant for model selection, one obtains (see [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>]),</p><disp-formula id="scirp.30323-formula105208"><label>(26)</label><graphic position="anchor" xlink:href="5-1240178\274d2285-3463-4d31-a0d7-6d12b4d90beb.jpg"  xlink:type="simple"/></disp-formula><p>If <img src="5-1240178\cad3523f-ff01-47e4-a92f-bd7b2aa3ac2e.jpg" /> is chosen to be the conjugate prior density, then the marginal density <img src="5-1240178\8fbfe29d-5be1-4fd1-ac2d-d8c3d7c499a4.jpg" /> can be explicitly derived. Details on this and further simplifications obtained upon using Zellner’s g-prior can be found in [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>]. (See also [33,34].)</p><p>This method is only useful if one is interested in comparing a few of these models, arising out of some pre-specified subsets. Comparing all <img src="5-1240178\0c700eba-9d9c-44eb-b563-995f50b9f03a.jpg" /> models is not a computationally viable option for even moderate values of<img src="5-1240178\7863fbd4-3fc7-461b-844a-b274027d8f8b.jpg" />, since for each model, <img src="5-1240178\20b0a91e-bfac-42a8-abee-f79b195df64f.jpg" />, one has to compute the corresponding <img src="5-1240178\55cb3b72-e1f0-42c0-82ef-fdd20f613367.jpg" /> and<img src="5-1240178\3e8d559c-b929-4938-994a-f0ba4dcb61f3.jpg" />.</p><p>We are more interested in a different problem, namely, whether an extra regressor should be added to an already determined model. This is the idea behind the step-wise regression, forward selection method. In this set-up, the model comparison problem can be stated as comparing</p><p><img src="5-1240178\2fae26cd-6e44-4014-a330-d20f123e249d.jpg" /></p><p>versus</p><p><img src="5-1240178\9ce9bb6b-17d8-4e38-8116-23ba48883bff.jpg" /></p><p>This is actually a model building method, so we assume that<img src="5-1240178\9e0ef2dc-de67-4a9e-a192-c5e550d02d19.jpg" />, and hence <img src="5-1240178\067a2340-cbb7-4d6f-9b6c-c52315874405.jpg" /> is the intercept which gives the starting model. Then we decide whether this model needs to be expanded by adding additional regressors. Thus, at step<img src="5-1240178\cdbdbc50-7edd-4aa2-b110-295f6ae797cb.jpg" />, we have an existing model with regressors <img src="5-1240178\e4628b88-e117-450b-a515-cab0484729ea.jpg" /> and we fix <img src="5-1240178\fdddb5ec-5aa0-4dcd-b0e6-017c19082c74.jpg" /> to be one of the remaining <img src="5-1240178\137a9554-f92a-4061-8b02-7985a21c65f4.jpg" /> regressors as the candidate for possible selection. Now the two-stage MDL approach is straight forward. From (22) and (24), we note that <img src="5-1240178\08441fe8-8e4c-4dba-82c1-6698915aaa11.jpg" /> is to be selected if and only if</p><disp-formula id="scirp.30323-formula105209"><label>(27)</label><graphic position="anchor" xlink:href="5-1240178\876b3aa0-6df8-43ad-abf2-889d0b0bcf90.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\b8b24151-9806-4557-9528-422c0d5b0352.jpg" /> is the description length of the model with regressors <img src="5-1240178\b340c538-e5c0-48ff-9d45-3b6eca1dd00f.jpg" /> and <img src="5-1240178\7041ce0c-e35c-4692-b6f1-6a2278f48716.jpg" /> is its residual sum of squares as given in (23). A closer look at (27) reveals certain interesting facts. We need the following additional notations involving design matrices and the corresponding projection matrices. We assume that the required matrix inverses exist.</p><p><img src="5-1240178\eba5a99d-6cff-4c9b-b15a-58dab47a90ad.jpg" /></p><p>Then we note the following result which may be found, for example, in [<xref ref-type="bibr" rid="scirp.30323-ref35">35</xref>].</p><disp-formula id="scirp.30323-formula105210"><label>(28)</label><graphic position="anchor" xlink:href="5-1240178\5480b0dc-3c79-43f2-b6ac-c39f630d82a2.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="5-1240178\45dbeda7-7503-4c08-9e95-a6a7322457cc.jpg" /></p><p>It then follows that</p><p><img src="5-1240178\053b4734-3dac-4cdb-aec8-d85b8cbbcd2b.jpg" /></p><p>and hence</p><p><img src="5-1240178\e5f40b99-a65f-4a8e-a822-93ff6618a019.jpg" /></p><p>and</p><p><img src="5-1240178\0d7e6403-736c-4e29-ade8-2e98270ca0b1.jpg" /></p><p>where <img src="5-1240178\78230ea5-94e5-4e74-ac07-32ba723ec3b4.jpg" /> is simply the partial correlation coefficient between <img src="5-1240178\5d4ea21f-37fb-4dfc-9715-d0682a1d06e6.jpg" /> and <img src="5-1240178\52faa49e-2d4c-4375-b89b-d716f72103a6.jpg" /> conditional on<img src="5-1240178\4076a602-4785-410f-9be7-b90bed77d8a9.jpg" />. Substituting these in (27), we see that</p><disp-formula id="scirp.30323-formula105211"><label>(29)</label><graphic position="anchor" xlink:href="5-1240178\8c78639f-bd30-4a35-ac76-ca556c5ea0ef.jpg"  xlink:type="simple"/></disp-formula><p>Therefore,</p><p><img src="5-1240178\17bf6107-697c-4395-b4c8-7151c5e590ec.jpg" />if and only if</p><p><img src="5-1240178\eeb2e7b2-74fe-4270-9117-0d5b8093fda6.jpg" />if and only if</p><disp-formula id="scirp.30323-formula105212"><label>(30)</label><graphic position="anchor" xlink:href="5-1240178\22727ebc-30ed-42ff-a77f-f09db17db85e.jpg"  xlink:type="simple"/></disp-formula><p>This method does have some appeal, in that at each step, it tries to select that variable which has the largest partial correlation with the response (conditional on the variables which are already in the model), just like the step-wise regression method. However, unlike the stepwise regression method it does not require any stopping rule to decide whether the candidate should be added. It relies on the magnitude of the partial correlation instead.</p><p>One can also apply the stochastic complexity criterion given in (26) above. Then we obtain,</p><p><img src="5-1240178\3225cbcf-4cff-4f0d-b00c-225f236f1a43.jpg" /></p><p>(31)</p><p>which is related to the step-wise regression approach, but uses more information than just the partial correlation.</p><p>A full-fledged Bayesian approach using the g-prior can also be implemented as shown below. Note that</p><p><img src="5-1240178\9a3e7a38-b3f8-4891-8659-a4ea83b61935.jpg" /></p><p>and</p><disp-formula id="scirp.30323-formula105213"><label>(32)</label><graphic position="anchor" xlink:href="5-1240178\447c59d4-74f0-4da1-aba0-1897003de2bf.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\579c6042-aa1b-4a89-87c6-eec595f1ed53.jpg" /> and<img src="5-1240178\e8ae6cf1-eb22-4f14-b4ab-510489fca708.jpg" />, respectively, are the prior densities under <img src="5-1240178\10469a22-81bb-4e4e-9d87-95a1e677f153.jpg" /> and<img src="5-1240178\dc25d166-2bd6-4871-84d7-32beb54fcad5.jpg" />. Taking these priors to be g-priors, namely,</p><p><img src="5-1240178\f85003f7-3bcd-4ff1-9ac6-fe1bff593917.jpg" /></p><p>along with the density <img src="5-1240178\ae9d6b47-06b5-43e0-baf9-517d18bb1b6c.jpg" /> for<img src="5-1240178\e018e555-89d3-463f-a8be-4316e18e062a.jpg" />, a (proper prior) density <img src="5-1240178\984ca00b-97ff-48b5-b774-069d49fbe41b.jpg" /> for the hyperparameter<img src="5-1240178\3f99cc8c-ecdb-4db4-b225-06c79d1abfad.jpg" />, we obtain,</p><disp-formula id="scirp.30323-formula105214"><label>(33)</label><graphic position="anchor" xlink:href="5-1240178\8edd51fd-fdd5-4029-bea4-d6c8d5a8bed7.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.30323-formula105215"><label>(34)</label><graphic position="anchor" xlink:href="5-1240178\be106fb7-43a7-479f-bcb8-f089a9e46560.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="5-1240178\076c1053-d1a9-4759-a9e4-7672abadce9f.jpg" /> and<img src="5-1240178\d2fa0b49-a8ce-4390-ac78-4132cf2c6db6.jpg" />.</p><p>The one-dimensional integrals in (33), however, cannot be obtained in closed form. One could also approximate</p><p><img src="5-1240178\ce04a350-8a19-4d84-b343-4302e7b36796.jpg" />with<img src="5-1240178\51081c98-326e-44a4-bd83-5c0acf04b31c.jpg" />, where <img src="5-1240178\348e44de-5235-4dbb-bad4-92a284319576.jpg" /> are the ML-II (cf. [<xref ref-type="bibr" rid="scirp.30323-ref36">36</xref>]) estimates of<img src="5-1240178\a750c057-aa18-4734-a0b7-3d28194e2259.jpg" />. See [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>] for details.</p><p>Example 5. We illustrate the MDL approach to stepwise regression by applying it to the Iowa-corn-yielddata (see [37,38]). We have not included “year” as a regressor (which is a proxy for technological advance) and instead have considered only the weather-related regressors.</p><p>In this data set the variables are: X<sub>1</sub> = Year, 1 denoting 1930, X<sub>2</sub> = Pre-season precipitation, X<sub>3</sub> = May temperature, X<sub>4</sub> = June rain, X<sub>5</sub> = June temperature, X<sub>6</sub> = July rain, X<sub>7</sub> = July temperature, X<sub>8</sub> = August rain, X<sub>9</sub> = August temperature, and Y = X<sub>10</sub> = Corn Yield.</p><p>As mentioned earlier, we always keep the intercept and check whether this regression should be enlarged by adding more regressors. We first apply the Two-stage MDL criterion. From (30), at step<img src="5-1240178\f4de8209-68e2-4301-97bf-5a54639ac6a4.jpg" />, we consider only those regressors (which are not already in the model and)</p><p>which satisfy <img src="5-1240178\390bc407-4313-4cda-8f0e-0998822280a9.jpg" /> (=0.1005 in this example). From this set we pick the one with the largest</p><p><img src="5-1240178\8522e701-6c65-4746-93cf-7b019a9c1e26.jpg" />. The values of <img src="5-1240178\e10bb557-f4ee-470b-93cc-083a943758f0.jpg" /> for the relevant steps are listed below.</p><p><img src="5-1240178\3287118f-bc7a-4ff0-9451-288e17b34022.jpg" /></p><p>According to our procedure we select <img src="5-1240178\96017e16-a544-478e-8e85-217f8024caff.jpg" /> first, followed by <img src="5-1240178\936118ab-fb4b-48f4-b9f2-f73936f7ecc9.jpg" /> and the selection ends there.</p><p>We consider the SIC criterion next. From (31), at step<img src="5-1240178\e8b10408-4aca-46b2-946f-896017099ddc.jpg" />, we pick the regressor <img src="5-1240178\d7fba2b7-f9d0-461f-a2f9-dfc4f68c7271.jpg" /> with the largest value for</p><p><img src="5-1240178\63b23bce-0e30-48f6-8bff-5074f8ac5ca2.jpg" /></p><p>provided it is positive. The values of <img src="5-1240178\c1545f10-2da2-4fa3-8449-f732540f20e4.jpg" /> for the relevant steps are given below.</p><p><img src="5-1240178\5061a709-d31c-42d1-be80-894eeb80a12f.jpg" /></p><p>According to SIC our order of selection is<img src="5-1240178\b1dcbd45-1319-4d9f-97bd-cd25414ba4ec.jpg" />.</p></sec><sec id="s5_2"><title>5.2. Wavelet Thresholding</title><p>Consider the nonparametric regression problem where we have the following model for the noisy observations<img src="5-1240178\7b8ccf65-6186-43e8-9f33-38e1d4549536.jpg" />:</p><disp-formula id="scirp.30323-formula105216"><label>(35)</label><graphic position="anchor" xlink:href="5-1240178\37f630d6-8453-4240-9cf4-070963122f05.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\86d135ef-a04a-43c6-ad80-ee641c52bf8b.jpg" /> are i.i.d. <img src="5-1240178\0241f97d-c06f-40d7-a1e1-30f5faede83a.jpg" />errors with unknown error variance<img src="5-1240178\fff4b07a-1d3f-44af-b0f6-04d83a3a0cce.jpg" />, and <img src="5-1240178\f51359eb-577c-492a-9e11-d7d78c09a2a1.jpg" /> is a function (or signal) defined on some interval<img src="5-1240178\4bf64106-c440-435a-86e9-2247be898f38.jpg" />. Assuming s is a smooth function satisfying certain regularities (see [15,39,40]), we have the wavelet decomposition of<img src="5-1240178\2c389f69-fa32-4706-8e3b-7e094beaad4b.jpg" />:</p><disp-formula id="scirp.30323-formula105217"><label>(36)</label><graphic position="anchor" xlink:href="5-1240178\033230a3-d515-47b3-afc7-10a71d9d85e5.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="5-1240178\4c48e0e5-bcae-491b-89c2-6a53f9eb3b3e.jpg" /> are the wavelet functions and</p><p><img src="5-1240178\eafdef23-4f74-4cf9-84df-0fdaad1376a2.jpg" />is the corresponding vector of wavelet coefficients. We assume that the normally infinite sum in (36) can be taken to be a finite sum (or at least a very good approximation) as indicated in [<xref ref-type="bibr" rid="scirp.30323-ref39">39</xref>].</p><p>Upon applying the discrete wavelet transform (DWT) to<img src="5-1240178\d469c6cf-038b-4d33-85ba-4045df83e60b.jpg" />, we get the estimated wavelet coefficients,<img src="5-1240178\1117c4b5-6718-4a58-a57e-360169a0281e.jpg" />. Consider now the equivalent model:</p><p><img src="5-1240178\11b13cbd-66fb-4a78-bc60-5890c05e290e.jpg" /></p><p>where<img src="5-1240178\08f73e8f-631b-4601-b8f8-6a64cd42ea5c.jpg" />.</p><p>The model selection problem here involves determining the number of non-zero wavelet coefficients:</p><p><img src="5-1240178\1aae6373-9d0d-4688-a795-2b9fac567d47.jpg" /></p><p>versus</p><p><img src="5-1240178\a84787fb-5778-4f6e-a4e2-f56cd503cdcf.jpg" /></p><p>where <img src="5-1240178\ae286f3a-ff58-4a7f-89bd-a90cdf987951.jpg" /> are the number of wavelet coefficients of interest.</p><p>The prior distribution on the non-zero <img src="5-1240178\ec2583fb-5372-4adc-977d-fb3adfa8ccc7.jpg" /> is assumed to be i.i.d. <img src="5-1240178\dc5ec9ab-dc47-435f-b42e-0982daeee1d3.jpg" />under<img src="5-1240178\57bce424-29b7-4ba8-bf4b-94285b2c3b4d.jpg" />.</p><p>Since we have not identified the locations (indices) of the non-zero wavelet coefficients, <img src="5-1240178\4d8c40db-c960-4cee-b9d7-f2cbf537b00c.jpg" />, we proceed as follows to describe the prior structure. With each <img src="5-1240178\7dbf157a-c419-41fe-abdd-86625cc5fa05.jpg" /> we associate a binary variable <img src="5-1240178\a37da56f-a36e-482e-b59d-3c29b34666d0.jpg" /> as in [<xref ref-type="bibr" rid="scirp.30323-ref41">41</xref>] for wavelet regression or as in [<xref ref-type="bibr" rid="scirp.30323-ref13">13</xref>] for variable selection in regression. Then <img src="5-1240178\966f8f24-a34e-475c-97e9-d24b0adb8b99.jpg" /> is a Bernoulli sequence associated with the set of regression coefficients,<img src="5-1240178\bdbdc2fb-1bf0-4d8f-9725-e3532188c886.jpg" />. Let</p><p><img src="5-1240178\32ea7657-15e3-405a-ac95-93f1d9015ee5.jpg" /></p><p>Finally, we let <img src="5-1240178\fe791969-47cb-4457-8cf2-3d5476d0fbda.jpg" /> be i.i.d. <img src="5-1240178\9196be6a-b5fd-42ac-b51f-5e98f76a1d63.jpg" />(<img src="5-1240178\315dbf24-d4f8-4c0d-9bf4-158e58cffed4.jpg" />be the corresponding joint density), and define the following structure under<img src="5-1240178\39633511-6df4-4177-bdbe-28d4b0b95464.jpg" />.</p><disp-formula id="scirp.30323-formula105218"><label>(37)</label><graphic position="anchor" xlink:href="5-1240178\ab36ec06-ec48-4f3b-8ed6-5ec1bf1e6df5.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.30323-formula105219"><label>(38)</label><graphic position="anchor" xlink:href="5-1240178\3257c6a9-9b1d-4fdf-a28d-1c6c433f9488.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.30323-formula105220"><label>(39)</label><graphic position="anchor" xlink:href="5-1240178\b2ac2f5e-b259-4d7f-873c-d1053d892e0f.jpg"  xlink:type="simple"/></disp-formula><p>The nuisance parameter <img src="5-1240178\28fa828f-7536-466a-98d1-d1f4b7667d8d.jpg" /> which is common under both models is given the prior density<img src="5-1240178\b34d2176-9f40-46d0-b7b6-c250aca3ef70.jpg" />. Then it follows that</p><disp-formula id="scirp.30323-formula105221"><label>(40)</label><graphic position="anchor" xlink:href="5-1240178\ee630719-9873-4bdc-831b-0ab73cbbfbfe.jpg"  xlink:type="simple"/></disp-formula><p>Note that only those <img src="5-1240178\1ea52a25-955d-42fc-a3f0-15b4ae5d627d.jpg" /> for which <img src="5-1240178\b8ed3e8a-2e50-449d-9298-e7622d3f4666.jpg" /> appear in the integral above.</p><p>The Two-stage MDL approach is clearly the easiest to take in this problem. As described earlier, it approximates <img src="5-1240178\b464ff34-483f-487f-a47f-b15296c551d7.jpg" /> by coding the prior and the likelihood (both evaluated at an estimate) separately and sums the codelengths to obtain the description length. In this case, discretizing <img src="5-1240178\039f4f5c-5ee6-4063-87d1-c119f11602af.jpg" /> and <img src="5-1240178\14734b41-7f12-4c90-b29d-ebabc81c3875.jpg" /> to a precision of <img src="5-1240178\5989f0b0-7b44-4cb4-b912-fe8253747c5f.jpg" /> and ignoring terms that stay bounded as <img src="5-1240178\1fc5122c-a80d-4241-8854-a418d991ee99.jpg" /> increases, this amounts to</p><disp-formula id="scirp.30323-formula105222"><label>(41)</label><graphic position="anchor" xlink:href="5-1240178\65c26550-77fd-47eb-a4b1-e2898726167d.jpg"  xlink:type="simple"/></disp-formula><p>where the first term is obtained from Stirling’s approximation, the second term <img src="5-1240178\7b4f8dbc-4bce-43cc-af5e-3c695ff1a945.jpg" /> is for coding the <img src="5-1240178\3db95066-f8af-4d1e-a554-dd54cfa147a6.jpg" /> non-zero<img src="5-1240178\29b79cd5-bfea-425e-af61-d245c745a444.jpg" />’s and <img src="5-1240178\6148caaf-85cb-496a-b522-f84a1558d3df.jpg" /> is an estimate such as the MLE. On the other hand, computing SIC or <img src="5-1240178\27d7fc77-bcb0-48c0-b283-8af7c4e8f63a.jpg" /> is not an impossible task either. In fact, to integrate out the <img src="5-1240178\240132cd-8f72-4877-b1cb-12d8c65489ef.jpg" /> in <img src="5-1240178\daace493-df88-4c75-bcbf-d5f0ec3ac09e.jpg" /> of Equation (40) we argue as follows.</p><p><img src="5-1240178\488f67f7-5902-49bf-a81b-cdef28d80ffe.jpg" />and</p><p><img src="5-1240178\9ff98f54-7c45-449a-81b6-d63ffb0c0e37.jpg" /></p><p>Now, as we argued in Jeffreys test, we take<img src="5-1240178\04b7d588-d521-45ab-b7c1-4f16bf297cc5.jpg" />, and integrate out <img src="5-1240178\925f6bbc-053e-4935-af8b-9e8c45063c48.jpg" /> also. This leaves us with the following expression where we have a sum over<img src="5-1240178\9579f63b-0819-480e-9712-c61d4b5dd469.jpg" />.</p><disp-formula id="scirp.30323-formula105223"><label>(42)</label><graphic position="anchor" xlink:href="5-1240178\8f6c054f-03ae-4d1a-897d-fcc45fea0804.jpg"  xlink:type="simple"/></disp-formula><p>The term <img src="5-1240178\8eaa6207-7113-4230-bf38-bb26894404ca.jpg" /> is interesting. Most of the contribution to this sum is expected from <img src="5-1240178\94b59d15-1d5a-4ccf-9714-77265cb87cc8.jpg" /> with <img src="5-1240178\9c14a766-161f-4f00-b249-58859f10b1c3.jpg" /> corresponding to the largest <img src="5-1240178\3e2acdde-9fa0-49a0-9467-bf1a2e1b0ae3.jpg" /> of the<img src="5-1240178\ece41da7-21e4-4ae4-ba5a-022d6dab6705.jpg" />, which yields the MLE of <img src="5-1240178\a38d2882-ca1b-4406-b5ab-6a98d19625aa.jpg" /> upon normalization. The Bayes estimate, on the other hand, will arise from a weighted average of all the sums, with weights depending on the posterior probabilities of the corresponding<img src="5-1240178\5e8a4ced-66a4-4e82-b4e2-4a18eae61958.jpg" />. As is clear, weighted average over the space <img src="5-1240178\33698be2-a604-43dc-8da5-8ec41809df2b.jpg" /> is computationally very intensive when <img src="5-1240178\6a0d7327-3eaa-4a8a-9676-f9bcc09ed926.jpg" /> and <img src="5-1240178\8d1fb9d7-f107-4be6-a0f0-d64c7f93a129.jpg" /> are large. An appropriate approximation is indeed necessary, and MDL is important in that sense.</p><p>Even though we have justified the two-stage MDL for wavelet thresholding by showing that it is an approximation to a mixture MDL corresponding to a certain prior, a few questions related to this prior remain. First of all, the prior assumption that <img src="5-1240178\07eed14a-4ad9-484c-a53c-02cfc96e6107.jpg" /> are i.i.d. <img src="5-1240178\12cedde4-ba6c-4bee-9881-f531fecdad44.jpg" />is unreasonable; wavelet coefficients corresponding to wavelets at different levels of resolution must be modeled with different variances. Specifically they should decrease as the resolution level increases to indicate their decreasing importance (see [40,42,43]). Secondly, wavelet coefficients tend to cluster according to resolution levels (see [<xref ref-type="bibr" rid="scirp.30323-ref44">44</xref>]), so instead of independent normal priors, a multivariate normal prior with an appropriate dependence structure must be employed. These modifications can be easily implemented in the Bayesian approach, except that the resulting computational requirements may be substantial.</p></sec><sec id="s5_3"><title>5.3. Change Point Problem</title><p>We shall now consider MDL methods for a problem which attempts to decide whether there is a change-point in a given time series data. We use the data on British road casualties available in [<xref ref-type="bibr" rid="scirp.30323-ref45">45</xref>], which examines the effects on casualty rates of the seat belt law introduced on 31 January 1983 in Great Britain.</p><p>We follow the approach of [<xref ref-type="bibr" rid="scirp.30323-ref46">46</xref>]. Let <img src="5-1240178\eac65c3f-4448-4381-a8e5-82f43977eb48.jpg" /> be independent Poisson counts with<img src="5-1240178\35c469c4-ca0d-410a-be81-2af404f95dbb.jpg" />. <img src="5-1240178\5077175f-e3b3-4408-b568-9e9eb6c1ad5f.jpg" />are a priori considered related, and a joint multivariate normal prior distribution on their logarithm is assumed. Specifically, let <img src="5-1240178\ec6a3c74-61c5-4a66-981d-8569198f0947.jpg" /> be the <img src="5-1240178\7d098650-5103-4423-ac45-3ef86626496d.jpg" />th element of <img src="5-1240178\088eb125-9928-4dfb-8997-e87d38c3e4d2.jpg" /> and suppose</p><p><img src="5-1240178\afd8b487-ec66-40c1-adcb-61ba54a794b2.jpg" /></p><p>We model the change-point as the model selection problem:</p><p><img src="5-1240178\d49f7c59-0d1b-4b87-acdd-014d0c8d5504.jpg" /></p><p>versus</p><p><img src="5-1240178\fc718ed3-41b2-4202-a705-53cbd57d601a.jpg" /></p><p><img src="5-1240178\4531d602-d1c7-44a0-8298-953cf494208d.jpg" /></p><p>where <img src="5-1240178\d1c13d21-9f25-4891-8352-97f3397ffcd2.jpg" /> is the possible change-point. We further let <img src="5-1240178\1bb16302-832a-4468-abe9-5b355c754668.jpg" /> be i.i.d.<img src="5-1240178\8abd61b0-566d-4c7e-b5f7-fd3f9e928259.jpg" />. Note that <img src="5-1240178\2aec6b11-2432-4732-8f2e-58abb7c16796.jpg" /> and <img src="5-1240178\ca8c4d6b-3747-429b-9a36-988c31e56bfe.jpg" /> are hyperparameters.</p><p>First, we approximate the likelihood function assuming <img src="5-1240178\c518433d-503f-4990-8ce9-912c3203715c.jpg" /> as follows.</p><p><img src="5-1240178\70468ea7-396e-4c30-b18d-fec48268a170.jpg" /></p><p>(43)</p><p>where<img src="5-1240178\7b3ff74a-7a17-4d64-b6ec-87606197bdab.jpg" />. Expanding (43) about<img src="5-1240178\1819ec75-0923-4c84-9dcf-c1f3bcac4f79.jpg" />, its maximum, in Taylor series and ignoring higher order terms in<img src="5-1240178\35500924-5326-4664-b6c5-5bb0fa352705.jpg" />, we obtain</p><disp-formula id="scirp.30323-formula105224"><label>(44)</label><graphic position="anchor" xlink:href="5-1240178\5d2151ab-e6c3-46aa-851d-0ea0b4b9d185.jpg"  xlink:type="simple"/></disp-formula><p>What is appealing and useful about (44) is that it is proportional to the multivariate normal likelihood function (for<img src="5-1240178\4de3a2ea-da8d-4ceb-8d23-0347dd950368.jpg" />) with mean vector x and covariance matrix <img src="5-1240178\08674d14-0261-40c3-80b3-05285ccb5678.jpg" /> where</p><p><img src="5-1240178\98e96c78-a000-46cf-8e4d-04159b69846a.jpg" />and</p><p><img src="5-1240178\8d9b977d-facf-4779-b0c8-16319f08bc91.jpg" /></p><p>Thus hierarchical Bayesian analysis of multivariate normal linear models is applicable (see [15,36,47]). We note that the hyper-parameters <img src="5-1240178\b9cb83a5-15eb-499b-ad9c-66e1c50e2063.jpg" /> and <img src="5-1240178\b7298b29-90b3-462a-8316-71293c0ef252.jpg" /> do not have substantial influence and hence treat them as fixed constants (to be chosen based on some sensitivity analysis) in the following discussion. Consequently, denoting by <img src="5-1240178\0d086314-68bd-4ea0-a778-d8b96a42fc17.jpg" /> and <img src="5-1240178\f453fa81-ed88-44b7-9ccd-e3590de62034.jpg" /> the respective prior densities under <img src="5-1240178\661602be-cca3-47b6-83e4-6e50d4ff7677.jpg" /> and<img src="5-1240178\7de630fe-e7dd-41dc-8bbe-2ae6d619e001.jpg" />,</p><disp-formula id="scirp.30323-formula105225"><label>(45)</label><graphic position="anchor" xlink:href="5-1240178\26d3ad3a-cc6f-49b7-bf6a-2d3e45a98289.jpg"  xlink:type="simple"/></disp-formula><p>Now, from multivariate normal theory, observe that</p><disp-formula id="scirp.30323-formula105226"><label>(46)</label><graphic position="anchor" xlink:href="5-1240178\a2a98dbc-e08c-46fc-8ead-9f17bcebc5fb.jpg"  xlink:type="simple"/></disp-formula><p>and subsequently that, <img src="5-1240178\279fa4fb-2a98-4ad7-83b6-69d8d87ccdf1.jpg" />can be integrated out as in Example 2. Thus,</p><disp-formula id="scirp.30323-formula105227"><label>(47)</label><graphic position="anchor" xlink:href="5-1240178\c03b70cc-cb49-46d3-9328-3e4153f78200.jpg"  xlink:type="simple"/></disp-formula><p>Expression (47) is not available, in general, in closed form. Approaching it from the MDL technique, we look for a subsequent approximation employing an ML-II type estimator (cf. [<xref ref-type="bibr" rid="scirp.30323-ref36">36</xref>]) for<img src="5-1240178\657b4eeb-f11f-461b-9f56-a619396d2db6.jpg" />. Again, from (47), an ML-II likelihood for <img src="5-1240178\f264a413-9698-456a-9e91-2b07805cce72.jpg" /> is given by <img src="5-1240178\f640f011-d733-4112-87c4-8fcff8cfc483.jpg" /> which maximizes</p><p><img src="5-1240178\c6ba892d-458b-4686-8890-1edd0d4329d8.jpg" /></p><p>For fixed <img src="5-1240178\b901e255-1e69-4961-9667-805369552588.jpg" /> and <img src="5-1240178\b9ad9408-3d05-46f4-9373-e10f56e450c5.jpg" /> this involves only examining a smooth function of a single variable, <img src="5-1240178\bdffafb1-be4a-43fe-8f92-77b6d40b41a4.jpg" />, which is a simple computational task.</p><p>We proceed exactly as above to derive <img src="5-1240178\379fc88d-5027-4951-9cba-a6fdc1e3d9e1.jpg" /> also. Partition the required vectors and matrices as follows.</p><p><img src="5-1240178\a5c995a9-027a-48b1-8d44-011c6705ef37.jpg" /></p><p>Then we have</p><p><img src="5-1240178\726f05f1-3b66-4478-8f3a-6b38a0ba7728.jpg" /></p><p>(48)</p><p>As before, the MDL technique invloves deriving the ML-II estimator of <img src="5-1240178\98facf0f-0cd3-4f66-9ad1-7de95934336b.jpg" /> from<img src="5-1240178\c675951d-2026-4f6b-a00f-a4b1c748b627.jpg" />, for fixed <img src="5-1240178\b8a53728-e023-4c53-b86d-ed18947b542f.jpg" /> and<img src="5-1240178\5b971a69-a5c1-4d84-b550-ae480f1554a9.jpg" />. Obtaining <img src="5-1240178\72453f4a-ec83-4041-8254-d121564758cd.jpg" /> (for fixed <img src="5-1240178\85f047f3-d021-47ff-a4c7-24db5f062fc3.jpg" /> and</p><p><img src="5-1240178\a21a3c74-e551-4557-9c5d-5922750366d5.jpg" />) which maximizes <img src="5-1240178\d3d3ce1a-4ff8-4a6b-ae08-f3e37faf2ab2.jpg" /> is very similar to that for<img src="5-1240178\c4077ec1-47dd-4ca9-8a70-6a5bfd0296e8.jpg" />.</p><p>We have applied this technique to analyze the British Road Casualties data. Figures 1(a) and (b) show</p><p><img src="5-1240178\f571d7d0-ce63-4268-b17e-7b3b0c19efbb.jpg" />and <img src="5-1240178\72238f48-28f2-4c59-a2a6-b2e72bd8eae1.jpg" /> as a function of <img src="5-1240178\922aa745-d32f-463f-844f-70620b967b0c.jpg" /> for <img src="5-1240178\bf9528dc-4b7d-445e-b7d1-8784097d1bb3.jpg" /> and<img src="5-1240178\67e68b4e-d91c-483e-9a68-9183cee2d403.jpg" />, for the LGV and HGV data, respectively. As mentioned previously, <img src="5-1240178\2cea7f8c-0eca-4f68-802c-6f1a72c8a64c.jpg" />and <img src="5-1240178\c81ce8fb-729a-4905-bccb-24d01c6e41aa.jpg" /> do not seem to play any influential role; any reasonably small value of <img src="5-1240178\c9e74179-0cd9-42b5-ab81-2aadac3f00fa.jpg" /> seems to yield similar results, and any <img src="5-1240178\927727bb-b9fb-4faa-8368-80f9656b9659.jpg" /> which is not too close to 0 behaves similarly.</p><p>There seems to be strong evidence for a change-point in the intensity rate of casualties (induced by the ‘seatbelt law’) in the case of the LGV data, whereas this is absent in the case of the HGV data. This is evident from the very high value of <img src="5-1240178\ac74b618-5a59-45a6-a443-cdf180868e85.jpg" /> near the ML-II estimate of <img src="5-1240178\fc1c0a4b-3357-4c9a-b14d-c9fbe537eba0.jpg" /> for the LGV data.</p><p>There is a vast literature related to MDL, mostly in engineering and computer science. See [<xref ref-type="bibr" rid="scirp.30323-ref48">48</xref>] and the references listed there for the latest developments. See also [<xref ref-type="bibr" rid="scirp.30323-ref49">49</xref>]. [<xref ref-type="bibr" rid="scirp.30323-ref50">50</xref>] provides a review of MDL and SIC, and claim that SIC is the solution to “optimal universal coding problems”. MDL techniques have not become very popular in statistics, but they seem to be quite useful in many applications.</p></sec></sec><sec id="s6"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.30323-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">N. B. Asadi, T. H. Meng and W. H. 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