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398 andrew gelman stats-2010-11-06-Quote of the day


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Introduction: “A statistical model is usually taken to be summarized by a likelihood, or a likelihood and a prior distribution, but we go an extra step by noting that the parameters of a model are typically batched, and we take this batching as an essential part of the model.”


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Introduction: “A statistical model is usually taken to be summarized by a likelihood, or a likelihood and a prior distribution, but we go an extra step by noting that the parameters of a model are typically batched, and we take this batching as an essential part of the model.”

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Introduction: Mike McLaughlin writes: Consider the Seeds example in vol. 1 of the BUGS examples. There, a binomial likelihood has a p parameter constructed, via logit, from two covariates. What I am wondering is: Would it be legitimate, in a binomial + logit problem like this, to allow binomial p[i] to be a function of the corresponding n[i] or would that amount to using the data in the prior? In other words, in the context of the Seeds example, is r[] the only data or is n[] data as well and therefore not permissible in a prior formulation? I [McLaughlin] currently have a model with a common beta prior for all p[i] but would like to mitigate this commonality (a kind of James-Stein effect) when there are lots of observations for some i. But this seems to feed the data back into the prior. Does it really? It also occurs to me [McLaughlin] that, perhaps, a binomial likelihood is not the one to use here (not flexible enough). My reply: Strictly speaking, “n” is data, and so what you wa

3 0.16858289 779 andrew gelman stats-2011-06-25-Avoiding boundary estimates using a prior distribution as regularization

Introduction: For awhile I’ve been fitting most of my multilevel models using lmer/glmer, which gives point estimates of the group-level variance parameters (maximum marginal likelihood estimate for lmer and an approximation for glmer). I’m usually satisfied with this–sure, point estimation understates the uncertainty in model fitting, but that’s typically the least of our worries. Sometimes, though, lmer/glmer estimates group-level variances at 0 or estimates group-level correlation parameters at +/- 1. Typically, when this happens, it’s not that we’re so sure the variance is close to zero or that the correlation is close to 1 or -1; rather, the marginal likelihood does not provide a lot of information about these parameters of the group-level error distribution. I don’t want point estimates on the boundary. I don’t want to say that the unexplained variance in some dimension is exactly zero. One way to handle this problem is full Bayes: slap a prior on sigma, do your Gibbs and Metropolis

4 0.16237609 1474 andrew gelman stats-2012-08-29-More on scaled-inverse Wishart and prior independence

Introduction: I’ve had a couple of email conversations in the past couple days on dependence in multivariate prior distributions. Modeling the degrees of freedom and scale parameters in the t distribution First, in our Stan group we’ve been discussing the choice of priors for the degrees-of-freedom parameter in the t distribution. I wrote that also there’s the question of parameterization. It does not necessarily make sense to have independent priors on the df and scale parameters. In some sense, the meaning of the scale parameter changes with the df. Prior dependence between correlation and scale parameters in the scaled inverse-Wishart model The second case of parameterization in prior distribution arose from an email I received from Chris Chatham pointing me to this exploration by Matt Simpson of the scaled inverse-Wishart prior distribution for hierarchical covariance matrices. Simpson writes: A popular prior for Σ is the inverse-Wishart distribution [ not the same as the

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Introduction: David Hogg points me to this discussion: Martin Strasbourg and I [Hogg] discussed his project to detect new satellites of M31 in the PAndAS survey. He can construct a likelihood ratio (possibly even a marginalized likelihood ratio) at every position in the M31 imaging, between the best-fit satellite-plus-background model and the best nothing-plus-background model. He can make a two-dimensional map of these likelihood ratios and show a the histogram of them. Looking at this histogram, which has a tail to very large ratios, he asked me, where should I put my cut? That is, at what likelihood ratio does a candidate deserve follow-up? Here’s my unsatisfying answer: To a statistician, the distribution of likelihood ratios is interesting and valuable to study. To an astronomer, it is uninteresting. You don’t want to know the distribution of likelihoods, you want to find satellites . . . I wrote that I think this makes sense and that it would actualy be an interesting and useful rese

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Introduction: “A statistical model is usually taken to be summarized by a likelihood, or a likelihood and a prior distribution, but we go an extra step by noting that the parameters of a model are typically batched, and we take this batching as an essential part of the model.”

2 0.80507606 1474 andrew gelman stats-2012-08-29-More on scaled-inverse Wishart and prior independence

Introduction: I’ve had a couple of email conversations in the past couple days on dependence in multivariate prior distributions. Modeling the degrees of freedom and scale parameters in the t distribution First, in our Stan group we’ve been discussing the choice of priors for the degrees-of-freedom parameter in the t distribution. I wrote that also there’s the question of parameterization. It does not necessarily make sense to have independent priors on the df and scale parameters. In some sense, the meaning of the scale parameter changes with the df. Prior dependence between correlation and scale parameters in the scaled inverse-Wishart model The second case of parameterization in prior distribution arose from an email I received from Chris Chatham pointing me to this exploration by Matt Simpson of the scaled inverse-Wishart prior distribution for hierarchical covariance matrices. Simpson writes: A popular prior for Σ is the inverse-Wishart distribution [ not the same as the

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Introduction: Mike McLaughlin writes: Consider the Seeds example in vol. 1 of the BUGS examples. There, a binomial likelihood has a p parameter constructed, via logit, from two covariates. What I am wondering is: Would it be legitimate, in a binomial + logit problem like this, to allow binomial p[i] to be a function of the corresponding n[i] or would that amount to using the data in the prior? In other words, in the context of the Seeds example, is r[] the only data or is n[] data as well and therefore not permissible in a prior formulation? I [McLaughlin] currently have a model with a common beta prior for all p[i] but would like to mitigate this commonality (a kind of James-Stein effect) when there are lots of observations for some i. But this seems to feed the data back into the prior. Does it really? It also occurs to me [McLaughlin] that, perhaps, a binomial likelihood is not the one to use here (not flexible enough). My reply: Strictly speaking, “n” is data, and so what you wa

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Introduction: A student writes: I have a question about an earlier recommendation of yours on the election of the prior distribution for the precision hyperparameter of a normal distribution, and a reference for the recommendation. If I recall correctly I have read that you have suggested to use Gamma(1.4, 0.4) instead of Gamma(0.01,0.01) for the prior distribution of the precision hyper parameter of a normal distribution. I would very much appreciate if you would have the time to point me to this publication of yours. The reason is that I have used the prior distribution (Gamma(1.4, 0.4)) in a study which we now revise for publication, and where a reviewer question the choice of the distribution (claiming that it is too informative!). I am well aware of that you in recent publications (Prior distributions for variance parameters in hierarchical models. Bayesian Analysis; Data Analysis using regression and multilevel/hierarchical models) suggest to model the precision as pow(standard deviatio

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