User:Timothee Flutre/Notebook/Postdoc/2011/11/10
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(→Bayesian model of univariate linear regression for QTL detection: finish posterior tau) |
(→Bayesian model of univariate linear regression for QTL detection: fix typo) |
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| - | * '''Data''': let's assume that we obtained data from N individuals. We note <math>y_1,\ldots,y_N</math> the (quantitative) phenotypes (e.g. expression | + | * '''Data''': let's assume that we obtained data from N individuals. We note <math>y_1,\ldots,y_N</math> the (quantitative) phenotypes (e.g. expression levels at a given gene), and <math>g_1,\ldots,g_N</math> the genotypes at a given SNP (encoded as allele dose: 0, 1 or 2). |
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| - | * '''Likelihood''': <math>\forall i \in \{1,\ldots,N\}, \; y_i = \mu + \beta_1 g_i + \beta_2 \mathbf{1}_{g_i=1} + \epsilon_i \text{ with } \epsilon_i \overset{i.i.d}{\sim} \mathcal{N}(0,\tau^{-1})</math> | + | * '''Likelihood''': we start by writing the usual linear regression for one individual |
| + | |||
| + | <math>\forall i \in \{1,\ldots,N\}, \; y_i = \mu + \beta_1 g_i + \beta_2 \mathbf{1}_{g_i=1} + \epsilon_i \text{ with } \epsilon_i \overset{i.i.d}{\sim} \mathcal{N}(0,\tau^{-1})</math> | ||
where <math>\beta_1</math> is in fact the additive effect of the SNP, noted <math>a</math> from now on, and <math>\beta_2</math> is the dominance effect of the SNP, <math>d = a k</math>. | where <math>\beta_1</math> is in fact the additive effect of the SNP, noted <math>a</math> from now on, and <math>\beta_2</math> is the dominance effect of the SNP, <math>d = a k</math>. | ||
| - | Let's now write in matrix notation: | + | Let's now write the model in matrix notation: |
<math>Y = X B + E \text{ where } B = [ \mu \; a \; d ]^T</math> | <math>Y = X B + E \text{ where } B = [ \mu \; a \; d ]^T</math> | ||
| - | + | This gives the following [http://en.wikipedia.org/wiki/Multivariate_normal_distribution multivariate Normal distribution] for the phenotypes: | |
| - | <math>Y | X | + | <math>Y | X, \tau, B \sim \mathcal{N}(XB, \tau^{-1} I_N)</math> |
The likelihood of the parameters given the data is therefore: | The likelihood of the parameters given the data is therefore: | ||
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<math>\mathcal{L}(\tau, B) = \mathsf{P}(Y | X, \tau, B)</math> | <math>\mathcal{L}(\tau, B) = \mathsf{P}(Y | X, \tau, B)</math> | ||
| - | <math>\mathcal{L}(\tau, B) = \left(\frac{\tau}{2 \pi}\right)^{N | + | <math>\mathcal{L}(\tau, B) = \left(\frac{\tau}{2 \pi}\right)^{\frac{N}{2}} exp \left( -\frac{\tau}{2} (Y - XB)^T (Y - XB) \right)</math> |
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<math>\mathsf{P}(\tau, B) = \mathsf{P}(\tau) \mathsf{P}(B | \tau)</math> | <math>\mathsf{P}(\tau, B) = \mathsf{P}(\tau) \mathsf{P}(B | \tau)</math> | ||
| + | |||
| + | A [http://en.wikipedia.org/wiki/Gamma_distribution Gamma distribution] for <math>\tau</math>: | ||
<math>\tau \sim \Gamma(\kappa/2, \, \lambda/2)</math> | <math>\tau \sim \Gamma(\kappa/2, \, \lambda/2)</math> | ||
| + | |||
| + | which means: | ||
| + | |||
| + | <math>\mathsf{P}(\tau) = \frac{\frac{\lambda}{2}^{\kappa/2}}{\Gamma(\frac{\kappa}{2})} \tau^{\frac{\kappa}{2}-1} e^{-\frac{\lambda}{2} \tau}</math> | ||
| + | |||
| + | And a multivariate Normal distribution for <math>B</math>: | ||
<math>B | \tau \sim \mathcal{N}(\vec{0}, \, \tau^{-1} \Sigma_B) \text{ with } \Sigma_B = diag(\sigma_{\mu}^2, \sigma_a^2, \sigma_d^2)</math> | <math>B | \tau \sim \mathcal{N}(\vec{0}, \, \tau^{-1} \Sigma_B) \text{ with } \Sigma_B = diag(\sigma_{\mu}^2, \sigma_a^2, \sigma_d^2)</math> | ||
| + | |||
| + | which means: | ||
| + | |||
| + | <math>\mathsf{P}(B | \tau) = \left(\frac{\tau}{2 \pi}\right)^{\frac{3}{2}} |\Sigma_B|^{-\frac{1}{2}} exp \left(-\frac{\tau}{2} B^T \Sigma_B^{-1} B \right)</math> | ||
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Again, we use the priors and likelihoods specified above (but everything inside the integral is kept inside it, even if it doesn't depend on <math>B</math>!): | Again, we use the priors and likelihoods specified above (but everything inside the integral is kept inside it, even if it doesn't depend on <math>B</math>!): | ||
| - | <math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} \int \tau^{ | + | <math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} \int \tau^{3/2} \tau^{N/2} exp(-\frac{\tau}{2} B^T \Sigma_B^{-1} B) exp(-\frac{\tau}{2} (Y - XB)^T (Y - XB)) \mathsf{d}B</math> |
As we used a conjugate prior for <math>\tau</math>, we know that we expect a Gamma distribution for the posterior. | As we used a conjugate prior for <math>\tau</math>, we know that we expect a Gamma distribution for the posterior. | ||
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We also factorize inside the exponential: | We also factorize inside the exponential: | ||
| - | <math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{N+\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} \int \tau^{ | + | <math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{N+\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} \int \tau^{3/2} exp \left[-\frac{\tau}{2} \left( (B - \Omega X^T Y)^T \Omega^{-1} (B - \Omega X^T Y) - Y^T X \Omega X^T Y + Y^T Y \right) \right] \mathsf{d}B</math> |
We recognize the conditional posterior of <math>B</math>. | We recognize the conditional posterior of <math>B</math>. | ||
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<math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{N+\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} exp\left[-\frac{\tau}{2} (Y^T X \Omega X^T Y + Y^T Y) \right]</math> | <math>\mathsf{P}(\tau | Y, X) \propto \tau^{\frac{N+\kappa}{2} - 1} e^{-\frac{\lambda}{2} \tau} exp\left[-\frac{\tau}{2} (Y^T X \Omega X^T Y + Y^T Y) \right]</math> | ||
| - | We finally recognize | + | We finally recognize a Gamma distribution, allowing us to write the posterior as: |
<math>\tau | Y, X \sim \Gamma \left( \frac{N+\kappa}{2}, \; \frac{1}{2} (Y^T X \Omega X^T Y + Y^T Y + \lambda) \right)</math> | <math>\tau | Y, X \sim \Gamma \left( \frac{N+\kappa}{2}, \; \frac{1}{2} (Y^T X \Omega X^T Y + Y^T Y + \lambda) \right)</math> | ||
Revision as of 22:24, 21 November 2012
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Bayesian model of univariate linear regression for QTL detectionSee Servin & Stephens (PLoS Genetics, 2007).
where β1 is in fact the additive effect of the SNP, noted a from now on, and β2 is the dominance effect of the SNP, d = ak. Let's now write the model in matrix notation:
This gives the following multivariate Normal distribution for the phenotypes:
The likelihood of the parameters given the data is therefore:
A Gamma distribution for τ:
which means:
And a multivariate Normal distribution for B:
which means:
Here and in the following, we neglect all constants (e.g. normalization constant, YTY, etc):
We use the prior and likelihood and keep only the terms in B:
We expand:
We factorize some terms:
Let's define
This now becomes easy to factorizes totally:
We recognize the kernel of a Normal distribution, allowing us to write the conditional posterior as:
Similarly to the equations above:
But now, to handle the second term, we need to integrate over B, thus effectively taking into account the uncertainty in B:
Again, we use the priors and likelihoods specified above (but everything inside the integral is kept inside it, even if it doesn't depend on B!):
As we used a conjugate prior for τ, we know that we expect a Gamma distribution for the posterior. Therefore, we can take τN / 2 out of the integral and start guessing what looks like a Gamma distribution. We also factorize inside the exponential:
We recognize the conditional posterior of B. This allows us to use the fact that the pdf of the Normal distribution integrates to one:
We finally recognize a Gamma distribution, allowing us to write the posterior as:
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the (quantitative) phenotypes (e.g. expression levels at a given gene), and
the genotypes at a given SNP (encoded as allele dose: 0, 1 or 2).
. We can see that


