Why Family QTL Power Depends on Design
A family QTL study seeks evidence that relatives’ phenotypes share covariance attributable to a genomic region. Its power is not determined by the number of people alone. Relatives differ in how much genetic information they share; markers differ in how well they reveal that sharing; and a QTL effect can be difficult to distinguish from other sources of familial resemblance. Families selected because of their phenotypes also require an analysis that accounts for selection.
Design calculations connect these features to a test’s ability to detect a nonzero QTL variance component. The calculations below use a local, score-based approximation to make the role of information explicit. It is a planning tool, not a substitute for a model that matches the proposed sampling and analysis.
The entries of \(\Pi\) depend on the family relationships and on the IBD information used by the model. With uncertain IBD, the likelihood accounts for that uncertainty rather than treating an unobserved sharing state as known. In a design calculation, marker informativeness therefore affects how much covariance information is available, not merely how many markers are counted.
Information and a Local Power Approximation
First suppose the null covariance \(V_0\) is specified and positive definite. Let \(P=V_0^{-1}-V_0^{-1}X(X^\mathsf{T}V_0^{-1}X)^{-1}X^\mathsf{T}V_0^{-1}\), assuming the columns of \(X\) are linearly independent. This matrix removes the fitted mean directions: \(PX=0\), and \(PV_0P=P\). The restricted-likelihood score for \(\tau\) at zero is
The quadratic term is effectively based on the mean-adjusted phenotype: because \(PX=0\), \(Py=P(y-X\beta)\). This matters when the mean is not zero; using an uncentered quadratic form without removing the fitted mean would generally produce a nonzero expected score under the null.
A short justification
Under \(H_0\), \(E(y)=X\beta\) and \(\operatorname{Cov}(y)=V_0\). Since \(PX\beta=0\),
Thus \(E(U)=0\); under the Gaussian model its null variance is \(I_{\tau\tau}\). Under the alternative with the same mean and covariance \(V_0+\tau\Pi\), the mean term still vanishes after projection, and
Consequently, \(E_\tau(U)=\tau I_{\tau\tau}\). For small alternatives and enough independent family units for a normal approximation, \(U/\sqrt{I_{\tau\tau}}\) has approximate mean \(\tau\sqrt{I_{\tau\tau}}\) and variance near one. For a one-sided score test at significance level \(\alpha\), approximate power is
Here \(\Phi_N\) is the standard normal cumulative distribution function, \(z_c\) is its \(c\)-quantile, \(1-\beta\) is target power, and \(n\) is the number of independent families when their per-family information is equal. The sample-size expression rearranges the approximation; it is not exact, especially for small numbers of pedigrees or alternatives far from zero.
In practice, nuisance covariance components are often estimated too. Their score can carry information that overlaps with the QTL score. For covariance derivatives \(A_j\) of nuisance parameters \(\lambda_j\), define score information \(I_{ab}=\tfrac12\operatorname{tr}(P A_a P A_b)\), with \(A_\tau=\Pi\). The information for \(\tau\) after accounting for nuisance covariance parameters is the efficient information \(I_{\tau\cdot\lambda}=I_{\tau\tau}-I_{\tau\lambda}I_{\lambda\lambda}^{-1}I_{\lambda\tau}\), when \(I_{\lambda\lambda}\) is invertible. Use this adjusted information in planning rather than treating a confounded component as known.
Worked Example: Comparing Pedigree Structures
Consider hypothetical, mean-centered phenotypes with covariance \(V_0=\sigma^2 I\), where the baseline variance \(\sigma^2\) is a nuisance parameter. Set \(\sigma^2=1\) for the calculation. Compare a four-member family with two independent two-member families, using the same total of four people. Suppose the QTL covariance derivative has diagonal entries 1 and off-diagonal entries \(r=0.5\) within each family. Assume the same \(r\) applies to each pair in the four-member family.
For a four-member family, \(\operatorname{tr}(\Pi)=4\). Its squared trace is \(4+12(0.5)^2=7\): four diagonal squares and twelve ordered off-diagonal squares. The information before adjusting for \(\sigma^2\) is \(\tfrac12(7)=3.5\). The nuisance-variance information is \(\tfrac12\operatorname{tr}(I^2)=2\), and the cross-information is \(\tfrac12\operatorname{tr}(\Pi I)=2\). Therefore,
For two independent pairs, the block-diagonal \(\Pi\) has \(\operatorname{tr}(\Pi)=4\) and \(\operatorname{tr}(\Pi^2)=2\{2+2(0.5)^2\}=5\). The unadjusted information is \(2.5\), and the nuisance-variance adjustment is again \(2^2/2=2\), giving \(I_{\tau\cdot\sigma^2}=0.5\). Under these deliberately simplified covariance assumptions, the four-member structure provides more information about this QTL covariance pattern than two separate pairs with the same number of people. Real designs must use their actual relationship and baseline covariance matrices; larger pedigrees are not automatically more informative if their additional covariance is poorly distinguished from nuisance components.
Marker Information and Target Sample Size
Marker informativeness affects the precision of the IBD information used to construct the linkage likelihood. Better information can sharpen the distinction between the covariance under linkage and the null, but its effect is model- and pedigree-dependent. A scalar “reliability” is useful only as a transparent approximation; it does not replace integrating uncertain IBD probabilities in the actual analysis.
Worked Example: Marker Informativeness and Required Families
For planning, approximate each hypothetical two-person family’s covariance derivative by \(\Pi_q=\begin{pmatrix}1&qr\\qr&1\end{pmatrix}\), where \(r=0.8\) is the underlying off-diagonal sharing contrast and \(q=0.75\) is a design approximation to how much of that contrast is resolved by the marker data. Let \(V_0=\sigma^2 I\), with unknown \(\sigma^2\), and use \(\sigma^2=1\) as the scale. There are no other nuisance covariance components in this illustration.
For one pair, \(\operatorname{tr}(\Pi_q^2)=2+2(qr)^2\), while \(\operatorname{tr}(\Pi_q)=2\). The raw information for \(\tau\) is \(1+(qr)^2\); the information for \(\sigma^2\) and their cross-information are both 1. Adjusting for the baseline variance gives
Suppose the QTL variance is \(\tau=0.25\) in units of the baseline phenotypic variance, the target power is 80%, and \(\alpha=0.05\) for a one-sided score test. Using \(z_{0.95}=1.645\) and \(z_{0.80}=0.842\),
The approximation suggests at least 275 independent, analyzable pairs under these assumptions. If the sharing contrast were fully resolved (\(q=1\)), information per family would be \(0.8^2=0.64\), and the same calculation would require about \(6.185/\{0.0625(0.64)\}=155\) pairs. This comparison is illustrative: a real marker panel should be evaluated using its expected IBD probabilities and the planned likelihood.
QTL Effect Size, Ascertainment, and Practical Design
Because the local noncentrality is \(\tau\sqrt{I}\), effect size and information have distinct roles. For a fixed design, halving \(\tau\) approximately halves the noncentrality; maintaining the same power then requires about four times as much information. Increasing family count generally increases information nearly linearly for independent families, while changing relationship structure can alter information per family. The latter depends on the full covariance pattern, including how well the QTL component is separated from polygenic, environmental, and residual components.
Ascertainment can change the distribution of observed families. If families are selected based on their phenotypes, an ordinary likelihood for an unselected sample may not describe the sampling process. Power should then be evaluated using an ascertainment-corrected or conditional likelihood consistent with the selection rule. A design calculation that ignores selection can misstate both the null calibration and the alternative distribution. When selection is complex, simulate the full process: generate pedigrees and phenotypes, apply the selection rule, generate or condition on marker information, and analyze each simulated sample with the intended corrected procedure.
The same principle applies to incomplete phenotypes, departures from the assumed covariance model, and unequal pedigree sizes. A simple information formula is useful for screening candidate designs, but final planning should reflect the expected number of usable relatives, actual marker informativeness, nuisance parameters, and the exact test calibration. Parametric simulation is especially valuable when the boundary at \(\tau=0\), small family counts, or ascertainment makes a normal approximation unreliable.
Worked Example: Translating an Effect-Size Change Into Design
Suppose a hypothetical design has efficient information \(I_{\text{per family}}=0.36\), and the target is 80% power at a one-sided 5% level. If the anticipated QTL variance is \(\tau=0.25\), the preceding calculation gives about 275 families. If the true planning value is instead \(\tau=0.125\), while all other assumptions remain fixed, the required count is
Thus about 1,100 independent families would be required by this approximation, four times the earlier count because the effect was halved. This is not evidence that the smaller effect is absent; it shows that a smaller covariance component is harder to distinguish at a fixed information level. A proposed study should justify its effect-size assumption and assess power across a range of plausible values.
Common Pitfalls and Design Checks
- Counting people instead of covariance information. The same number of participants can yield different power when pedigree relationships differ. Compare covariance information after nuisance components are accounted for.
- Treating marker uncertainty as if IBD were observed. Use the information implied by marker data and the planned IBD treatment; do not assume perfect sharing information unless the design supports it.
- Ignoring the fitted mean. A score quadratic must remove fixed-effect means. With \(PX=0\), \(Py=P(y-X\beta)\); an uncentered score without this projection can have a nonzero null expectation.
- Using raw information when nuisance components are estimated. Overlap between QTL and baseline covariance patterns reduces efficient information and can substantially lower power.
- Applying an unselected-sample calculation to selected families. Phenotype-based ascertainment must be reflected in the likelihood and in power evaluation.
A defensible design starts with a plausible QTL variance, the family structures that can be recruited, expected marker information, and a covariance model that includes relevant nuisance components. Use local information calculations to compare options, then verify the selected design by simulation under the actual ascertainment and analysis procedures when those features are consequential.
Check Your Understanding
Use the definitions and approximations in this tutorial to answer the following questions.
- Why does the restricted score remove \(X\beta\), and what can go wrong if a nonzero mean is ignored?
- In the local power approximation, what happens to the required number of families if the anticipated QTL variance is halved while other quantities stay fixed?
- Why can a larger pedigree provide more linkage information than several smaller pedigrees with the same number of people, and why is that not guaranteed in every model?
- In the pair example, how did adjustment for the unknown baseline variance change the information attributable to the QTL covariance pattern?
- What features of the study should be reproduced in a simulation when families are selected based on their phenotypes?