Last updated: 2018-05-15
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html
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e05bc83
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LSun
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2018-05-12
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Update to 1.0
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rmd
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cc0ab83
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Lei Sun
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2018-05-11
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update
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html
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LSun
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2018-02-01
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knockoff
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2018-02-01
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knockoff comparison
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4491358
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LSun
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2018-01-30
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linear regression
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rmd
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c17f67c
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2018-01-30
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wflow_publish(c(“analysis/index.rmd”, “analysis/knockoff.rmd”, “analysis/knockoff_2.rmd”, “analysis/knockoff_3.rmd”))
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rmd
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56957bd
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LSun
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2018-01-27
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Sigma betahat
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56957bd
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2018-01-27
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Sigma betahat
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Introduction
Similar to previous simulations, only that the design matrix \(X\) is simulated such that \(\Sigma_{\hat\beta} = \sigma_e^2(X^TX)^{-1}\) has non negligible off-diagnoal correlations.
\(d\) and \(\Sigma_{\hat\beta}\)
Let \(\Sigma_{\hat\beta} / \sigma_e^2 = B_{p \times d} \cdot B_{p \times d}^T + I\), where \(B_{i, j} \stackrel{\text{iid}}{\sim} N(0, 1)\). Then rescale the matrix such that the mean of its diagnal \(= 1\). Generate \(X_{n \times p}\) such that \((X^TX)^{-1} = \Sigma_{\hat\beta} / \sigma_e^2\).
Recall that the random coefficient of the second order of Gaussian deviative with the empirical distribution of correlated null \(W_2\) has the property \[
Var(W_2) = \bar{\rho_{ij}^2}
\] We take a look at how \(d\) is related to this quantity.
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\(\eta \in \{0.5, 0.6, 0.7, 0.8, 0.9\}\), \(\sigma_\beta / \sigma_e = 3\), \(d \sim Unif\{1, 2, \cdots, 50\}\)
Overall FDR and Power comparison
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FDR and Power at low sparsity: \(50\%\) true signal
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FDR and Power at high sparsity: \(10\%\) true signal
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\(\eta \in \{0.75, 0.80, 0.85, 0.90, 0.95\}\), \(\sigma_\beta / \sigma_e = 3\), \(d \sim Unif\{1, 2, \cdots, 20\}\)
Overall FDR and Power comparison
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FDR and Power at low sparsity: \(20\%\) true signal
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FDR and Power at high sparsity: \(10\%\) true signal
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