Methodology described in this vignette is adapted from the article “BIGL: Biochemically Intuitive Generalized Loewe null model for prediction of the expected combined effect compatible with partial agonism and antagonism” (2017) by K. Van der Borght, A. Tourny, R. Bagdziunas, O. Thas, M. Nazarov, H. Turner, B. Verbist and H. Ceulemans (doi:10.1038/s41598-017-18068-5) as well as its technical supplement. We advise the reader to consult it for a deeper understanding of the procedure described next.
Further chapters were added as extensions on top of the original article regarding variance heterogeneity, Bliss independence and alternative Loewe generalization.
First, a monotherapy model is described by the following equation.
\[ y\left(d\right) = b + \dfrac{m - b}{1 + \left(\frac{\operatorname{EC50}}{d}\right)^{|h|}} \]
where \(y\) is the response (or effect), \(d\) is the dose (or concentration) of the compound, \(h\) is the Hill’s coefficient and \(b\) and \(m\) are respectively baseline and maximum response for that compound. Lastly, \(\textrm{EC50}\) stands for the dose level of the compound needed to attain the midpoint effect, i.e. \[y\left(\textrm{EC50}\right) = b + \frac{m - b}{2}\]
Note that \(m > b\) if and only if the response is increasing with the dose of the compound. If the response is decreasing, then \(m < b\).
This monotherapy equation is estimated for both compounds with the constraint that \(b\), the baseline level, is shared across compounds. This baseline level is denoted by b
in the parameter vector. Additionally, m1
and m2
in the parameter vector stand for estimates of maximal responses \(m_{1}\) and \(m_{2}\), respectively, whereas h1
and h2
are Hill’s coefficients (slope) of the monotherapy curve for each compound. Lastly, e1
and e2
are log-transformed inflection points, i.e. e1
\(= \log\left(\textrm{EC50}_{1}\right)\) and e2
\(= \log\left(\textrm{EC50}_{2}\right)\).
Define the occupancy level \(\textrm{occup}\), i.e. the fractional (enzymatic) effect or observed effect relative to maximal effect, for both compounds at given dose levels as \[ \textrm{occup}_{1}\left(d_{1}\right) = \frac{1}{1 + \left(\frac{\operatorname{EC50}_{1}}{d_{1}}\right)^{h_{1}}} \] \[ \textrm{occup}_{2}\left(d_{2}\right) = \frac{1}{1 + \left(\frac{\operatorname{EC50}_{2}}{d_{2}}\right)^{h_{2}}} \] Alternatively, the above equations can be rearranged to express dose in terms of occupancy so that \[ d_{1} = \operatorname{EC50}_{1} \left(\frac{1}{\operatorname{occup_{1}}} - 1 \right)^{-1/h_{1}} \] \[ d_{2} = \operatorname{EC50}_{2} \left(\frac{1}{\operatorname{occup_{2}}} - 1 \right)^{-1/h_{2}} \] Although the occupancy was considered here in the marginal case, it is equally well-defined when compounds are combined and is understood as the fraction of enzyme bound to any compound. It can thus be used to re-express classical Loewe additivity equations.
In the classical Loewe model where both marginal models share upper \((m)\) and lower \((b)\) asymptotes, occupancy is defined as the solution to this additivity equation for each dose combination \((d_{1}, d_{2})\), namely \[\frac{d_1\left(\textrm{occup}^{-1} - 1\right)^{1/h_{1}}}{\textrm{EC50}_{1}}+ \frac{d_2\left(\textrm{occup}^{-1} - 1\right)^{1/h_{2}}}{\textrm{EC50}_{2}} = 1\]
Once occupancy is computed, in the classical Loewe model the predicted response at dose combination \((d_{1}, d_{2})\) can be calculated to be \[\begin{equation} \begin{split} y & = b + \left(m - b\right) \times \textrm{occup} = \\ & = b + \left(m - b\right) \times \textrm{occup} \times \left[\frac{d_{1}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{1}}}{\textrm{EC50}_{1}} + \frac{d_{2}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{2}}}{\textrm{EC50}_{2}}\right] = \\ & = b + \textrm{occup} \times \left[\frac{ \left(m - b\right) d_{1}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{1}}}{\textrm{EC50}_{1}} + \frac{ \left(m - b\right) d_{2}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{2}}}{\textrm{EC50}_{2}}\right] \end{split} \end{equation}\]
Generalized Loewe model extends the classical Loewe model by allowing compounds to have different upper asymptotes so that when adjusted, the above predicted response is written instead as \[ y = b + \textrm{occup} \times \left[\frac{\left(m_{1} - b\right) d_{1}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{1}}}{\textrm{EC50}_{1}} + \frac{\left(m_{2} - b\right) d_{2}\left(\textrm{occup}^{-1} - 1\right)^{1/h_{2}}}{\textrm{EC50}_{2}}\right]\]
In particular, if \(m_{1} = m_{2}\), then generalized Loewe is equivalent to the classical Loewe.
A null model based on the Highest Single Agent (HSA) model does not attempt to model interaction effects at all and the predicted effect of a combination is either the minimum (if marginal curves are decreasing) or the maximum (if marginal curves are increasing) of both monotherapy curves.
Bliss independence implies that two agents do not cooperate, i.e. act independently of each other. Additionally, the assumption is that a decreasing monotherapy curves express the fractions of unaffected control populations, while increasing curves express the fractions of affected control populations.
Bliss independence model is formulated for the fractional responses \(f\) (“fraction affected”), where the predicted response \(f_{12}\) at dose combination \((d_{1}, d_{2})\) is defined as:
\[ f_{12}(d_1, d_2) = f_1(d_1) + f_2(d_2) - f_1(d_1)f_2(d_2), \]
with \[f_1(d_1) = \frac{y\left(d_1\right) - b}{m_1 - b} = \frac{1}{1 + \left(\frac{\operatorname{EC50}_{1}}{d_{1}}\right)^{|h_{1}|}}\] \[f_2(d_2) = \frac{y\left(d_2\right) - b}{m_2 - b} = \frac{1}{1 + \left(\frac{\operatorname{EC50}_{2}}{d_{2}}\right)^{|h_{2}|}}\] In the classical Bliss independence model, marginal models share baseline and maximum response.
To allow the compounds to have different maximal responses, the fractional responses are rescaled to the maximum range (i.e. absolute difference between baseline and maximal response). Then the predicted response is defined as:
\[
y = b + (m_{max}-b) \left[ \tilde{f_1}(d_1) + \tilde{f_2}(d_2) - \tilde{f_1}(d_1)\tilde{f_2}(d_2) \right],
\] where \(m_{max}\) is one of \(m_1\) or \(m_2\), for which the value of \(|m_i - b|\) is larger, and \[ \tilde{f_i} = f_i\frac{m_i-b}{m_{max}-b}~~\text{for}~~i = 1, 2.\]
This implementation of Bliss independence supports both compounds with decreasing and increasing monotherapy profiles. However using one compound with a decreasing profile and another with an increasing profile in combination is not supported.
An alternative generalization of Loewe Additivity for the case of different asymptotes can be defined as a combination of Loewe and HSA approaches as follows:
In a classical Loewe equation, predicted response \(y\) at a given dose combination \((d_1, d_2)\) can be found by solving the equation:
\[ \frac{d_1}{D_1(y)} + \frac{d_2}{D_2(y)} = 1, \]
where \(D_i(y) = \operatorname{EC50}_{i}\left(\frac{y-b}{m_i-y}\right)^{\frac{1}{|h_i|}}\), for \(i = 1, 2\) is the dose of the \(i\)-th compound that gives response \(y\). Note that here \(D_i\) is properly defined only if \(y\) is between \(b\) and \(m_i\).
For the case of different asymptotes, say when \(y > m_1\) (increasing curve) or \(y < m_1\) (decreasing curve), we set \(D_1(y) = +\infty,\) so that the \(y\) is determined from the equation \(d_2 = D_2(y)\), replicating what is done in the HSA approach.
In order to evaluate any of the null models described above, the fitSurface
function will use the monotherapy parameter estimates from the previous step. The idea is if there are synergistic or antagonistic effects, then administration of both compounds will lead to important deviations from what combined monotherapy data would suggest according to the null model. Routines within fitSurface
function do essentially the following.
Synergy is evaluated for all off-axis dose combinations, i.e. dose combinations that are not used in the monotherapy curve estimation. Synergy evaluation depends on the underlying null model and any of the above models, i.e. generalized or classical Loewe or Highest Single Agent, can be used for this purpose. We provide here a brief summary of both statistical tests. Technical derivations and further details are available in the article cited at the beginning of the document.
To define test statistics, the following notations are used.
We construct a vector \(R = (r_{1}, ..., r_{k})\) which represents mean deviation from the predicted effect. In particular, \[ r_{k} = \frac{1}{n_{k}} \sum_{i = 1}^{n_{k}} y_{ki} - p_{k} \]
With the help of bootstrapping, the covariance matrix of \(R\) can be estimated under the null hypothesis of no synergy so that \(\operatorname{Var}\left(R\right) = \sigma^{2}\left(D + C_{p}\right)\) where \(D\) is a diagonal matrix with \(1 / n_{i}\) in the \(i\)-th position and \(C_{p}\) is the covariance matrix obtained from bootstrap.
meanR
The meanR
test will evaluate whether the null model globally fits well the observed data. It is derived using a lack-of-fit sum of squares technique. In particular, the test statistic is given by \[
\operatorname{TestStat} = \frac{R^{T}\left(D + C_{p}\right)^{-1}R}{n_{1}\sigma^{2}}
\] Assuming that residuals from the generalized Loewe model are normally distributed, it can be shown that this statistic follows an \(F_{n_{1}, \operatorname{df}_{0}}\) distribution under the null. If these assumptions are not satisfied, the null distribution can be approximated by bootstrapping.
maxR
The maxR
test evaluates whether the null model locally fits the observed data. In particular, it provides a test score for each off-axis combination. Based on the sign of this score, it can be determined whether synergy or antagonism is more likely and a formal test can be constructed. Under the null hypothesis of no lack-of-fit and normally distributed effects, \[
\max \left| R^{T}\left(D + C_{p}\right)^{-1/2} \right| / \sigma \sim \max \left| Z_{1}, \dots, Z_{k} \right|
\] where \(Z_{j} \sim N\left(0,1\right)\). More particularly, the test statistic for the \(k\)-th off-axis dose combination \((d_{1}, d_{2})\) is computed as \[
\operatorname{TestStat}\left(d_{1}, d_{2}\right) = \left[\left| R^{T}\left(D + C_{p}\right)^{-1/2} \right| / \sigma\right]_{k}
\] where \(\left[\cdot\right]_{k}\) indicates the \(k\)-th coordinate. This test statistic is then compared either to the null distribution based on normal approximation or a bootstrapped approximation.
In the methodology described above one important assumption is made regarding the variance of the on- and off-axis dose combinations. It is considered to be equal across all points. This assumption is also mentioned in the original article and its technical supplement.
In reality it is often seen that the variance of the monotherapies is not equal to the variance of the off-axis combinations. The assumption of equal variances is thus not always valid. That is why the meanR
and maxR
test-statistics can also estimate the variances for on-axis (monotherapies) and off-axis dose-combinations separately. Two extra methods are described below: the unequal
method (Separated variance) and the model
method (Modeled variance). For both methods replicates are required and no variance-stabilizing transformations are required. The latter is often necessary when assuming equal variances.
meanR
The adapted meanR
test uses two separate variance estimates for (a) the monotherapies (= \(\sigma^{2}_{0}\)) and (b) the dose combinations (= \(\Sigma_{1}\), a diagonal matrix). The notation for both unequal
as model
will be the same, but the estimation of \(\Sigma_{1}\) will be different. The variance of the monotherapies \(\sigma^{2}_{0}\) is estimated as \(\sigma^{2}\) above by taking the MSE of the null model. The test statistic is given by:
\[ \operatorname{TestStat} = \frac{R^{T}\left(\Sigma_{1}D + \sigma^{2}_{0}C_{p}\right)^{-1}R}{n_{1}} \]
unequal
method: The variance for the dose combinations is estimated by taking the variance in each dose combination and then taking the mean of all these variances, thus \(\Sigma_{1} = \sigma^2_1 I_{n_1}\). The downside of this method is that the variance for all combinations is assumed to be equal. In reality the variance often depends on the mean effect. This is taken into account in the model
method.
model
method: In this method the diagonal elements of \(\Sigma_{1}\) are no longer estimated as single number but rather as a vector of variances. Each off-axis point has now its own variance. A linear model is fitted on the original dataset, modeling the variance of each off-axis point as a function of its mean effect. The estimated model parameters are then used to predict the variance for the corresponding mean effect measured for that dose combination. These predicted variances are placed in the diagonal of \(\Sigma_{1}\). Modelling the variance with a linear model may require a transformation, to achieve a better fit and to avoid negative variances being modelled. A log-transformation often makes a good impression.
maxR
The same approach is taken for the adapted maxR
test statistic. Instead of using one estimated variance for both on- and off-axis points, two separate estimates are used. The estimates for \(\Sigma_{1}\) are different depending on the method used (unequal
or model
). The methodology of estimating the variance is the same as was described in the “Adapted meanR
” section above.
The maxR
test becomes
\[ \max \left| R^{T}\left(\Sigma_{1} D + \sigma^{2}_{0} C_{p}\right)^{-1/2} \right| \sim \max \left| Z_{1}, \dots, Z_{k} \right| \]
where \(Z_{j} \sim N\left(0,1\right)\). In particular, the test statistic for the \(k\)-th off-axis dose combination \((d_{1}, d_{2})\) is computed as \[ \operatorname{TestStat}\left(d_{1}, d_{2}\right) = \left[\left| R^{T}\left(\Sigma_{1} D + \sigma^{2}_{0} C_{p}\right)^{-1/2} \right| \right]_{k} \] where \(\left[\cdot\right]_{k}\) indicates the \(k\)-th coordinate.
In case of the unequal
variance assumption, the bootstrap proceeds as before, with the off-axis residuals being pooled and resampled. With the model
assumption, the resampling is more complicated, as the residuals are no longer exchangeable. One option is to rescale the observed residuals according to the mean-variance model (i.e. dividing them by their standard deviations), resample from this pool of standardized residuals, and then scale back to the true variance (by multiplying by the standard deviation). Yet this approach has proven to be unstable as it leads to extreme observations. An alternative (the default) is to generate zero-mean normal data with the modelled variances (see the rescaleResids
argument in fitSurface()
).
unequal
and model
methods compared to assumption of equal variancesThe assumption of equal variances between monotherapies and off-axis dose-combinations fails to control the type I error rate around pre-specified level, when the variance of off-axis points increases (natural variance or outliers). This results in false positive synergy calls when in reality there were none. Both the unequal
and the model
methods control the type I error rate far better, with slightly better results obtained by the model
method.
Furthermore, the sensitivity and specificity of the maxR
test statistics are higher with the methods assuming variance heterogeneity compared to the methods where equal variances are assumed.
As with many statistical tests, the researcher may not only be interested in a measure of significance (e.g. a p-value), but also in a measure of effect size, and a measure of the imprecision of this estimated effect size. Here we develop confidence intervals for two types of effect sizes. The first is a pointwise effect size, which is defined at every off axis point as the difference between the true mean response and the expected response under additivity. It is estimated as \(E_{i} = \frac{1}{n_i}\sum_{j=1}^{n_i}(R_{ij}-\hat{R}_i)\) with \(j=1, ..., n_i\), for every off-axis point \(i=1, ..., n_1\), whereby we strive to achieve a simultaneous coverage for all off-axis points of 95%.
Let \(e_i\) denote the true effect size on off axis point \(i\), and call \(E_{i}\) its estimate based on the data. Relying on the asymptotic normality of the estimator, an approximate (asymptotic) confidence interval would be formed as the set:
\[\begin{equation} \left\{ e: \left\vert \frac{E_{i}-e_i}{\hat{s}_i} \right\vert < z_{\alpha/2} \right\} \end{equation}\]
with \(\hat{s}_i\) the estimated standard error of \(E_i\), and \(z_{\alpha/2}\) the \(1-\alpha/2\) quantile of the standard normal distribution.
We know, however, from the meanR and maxR tests that the asymptotic distributions provide poor approximations. Therefore, we use the bootstrap here too to build the confidence intervals.
For every bootstrap instance, bootstrap observations are sampled for on- as well as off axis points. For the on-axis points, a parametric bootstrap based on the estimated monotherapy curves is used, as for the calculation of the meanR and maxR statistics. Based on these on-axis bootstrap samples, new monotherapy curves are fitted with resulting residual variances bootstrap variance \(MSE_0^b\), and corresponding response surfaces with expected outcomes $_i^b $ are derived. For the off-axis points, with \(n_i\) replicates at a given point, \(A_{ij} = R_{ij} - \bar{R}_i\) are the pointwise residuals \(j = 1, ..., n_i\). Here \(R_{ij}\) is the observed outcome and \(\bar{R}_i\), the average outcome at point \(i\), serves as an unbiased estimator of the true response. Note that these residuals are different from the residuals \(E_i = \bar{R}_i-\hat{R}_i\) used to construct the test statistics; for \(A_{ij}\) the departure with respect to the mean outcome at that off-axis point is used. These residuals are resampled with replacement from the observed residuals, possibly using rescaling as explained below. The resampled residuals are then added to the estimated effect sizes to obtain bootstrapped observations \(R_{ij}^b = \bar{R}_i + A_{ij}^b\), with \(b = 1, ...,B\) denoting the bootstrap instance.
An extra option of using the wild bootstrap is also available. In this method, a new response variable is calculated by multiplying the sampled residuals \(R_i\) with yet another random variable \(\upsilon_{ij}\) so that the bootstrapped observations are given by
\[R_{ij}^b = \bar{R}_i + A_{ij}^b \upsilon_{ij}\]
where \(v_{ij}\) are independent random variables with mean zero and variance 1, and can be sampled from a normal, gamma, rademacher or two-point distributions.
This leads to the bootstrap effect sizes \(E^b_i = \bar{R}_i^b-\hat{R}_i^b\) and test statistics \(\left\vert \frac{E^b_i -E_i}{\hat{s}^b_i} \right\vert\), using the standard deviations \(\hat{s}_i^b\) from the bootstrap.
Over all bootstrap instances, we then find the distribution of
\[\begin{equation} T = \max_i \left\vert \frac{E^b_i -E_i}{\hat{s}^b_i} \right\vert \end{equation}\]
Call \(t_\alpha\) the threshold such that \[\begin{equation} \text{P}\left\{T>t_\alpha\right\} = \alpha \end{equation}\]
Finally, we find for every off-axis point the confidence interval as the collection:
\[\begin{equation} \left\{ e: \left\vert \frac{E^b_i -E_i}{\hat{s}^b_i} \right\vert < t_\alpha \right\} \end{equation}\]
As an estimate of the standard error we use
\[\begin{equation} \hat{s}_i^b = \sqrt{\text{diag}(\boldsymbol{F}^b+\text{MSE}_0^b \boldsymbol{C}_p)_i}, \label{eq:confIntSe} \end{equation}\]
with \(\boldsymbol{F}^b\) equal to \(\text{MSE}_0^b\boldsymbol{D}\), \(\text{MSE}_1^b\boldsymbol{D}\) or \(\boldsymbol{S}^b\), depending on which variance model is used. This standard error resembles the variance estimators of the meanR and maxR statistics discussed there.
By using only the diagonal elements of \(\boldsymbol{F}^b\), we ignore the covariance between test statistics. We use the studentised-range concept (which is also central to Tukey’s method for multiple testing) for controlling the family-wise error rate (FWER) as default. Other available options are false coverage rate (FCR) and directional false coverage rate (dFCR). For the covariance matrix \(\boldsymbol{C}_p\) we use the one estimated for the observed data. This matrix turns out to be quite stable over the bootstrap runs; moreover the calculation of the matrix for each bootstrap sample would imply a time-consuming nested bootstrap procedure. On the other hand, \(MSE_0^b\) is re-estimated with each bootstrap sample. Also \(\boldsymbol{F}^b\) is re-estimated based on the bootstrapped data.
Researchers may also want to have a single measure for the strength of the synergy for a single experiment, e.g. in view of ranking compound combinations according to their synergistic effect. For this we calculate the average of the pointwise off-axis effect sizes. This is estimated as \(\bar{E} = \frac{1}{\sum_{i= 1}^{n_1}n_i }\sum_{i=1}^{n_1}\sum_{j= 1}^{n_i}(R_{ij}-\hat{R}_i)\). It may be considered as a measure of the “volume” between the expected and observed response surfaces, similar to the “integrated synergy” of . Note that this effect size may cause synergistic and antagonistic points to cancel out against one another, but we believe this scenario is unlikely. As before we would like a measure of imprecision for this effect size.
The construction of the bootstrap confidence interval for the single effect size follows the general procedure for bootstrap-t confidence intervals . Let \(\boldsymbol{F}\) denote the estimated covariance matrix of the raw residuals as before.
Using Equation \(\eqref{Eq_Var}\) in the main text and the fact that
\[\begin{equation} \mbox{Var}\left\{\bar{E}\right\} = \mbox{Var}\left\{\frac{1}{n_1}\sum_{i=1}^{n_1} E_i\right\} = \frac{1}{n_1^2}\left(\sum_{i=1}^{n_1} \mbox{Var}\left\{E_i\right\} + \sum_{i=1}^{n_1}\sum_{j=1}^{n_1}\mbox{Cov}\left\{E_i, E_j\right\}\right), \label{eq:varE} \end{equation}\]
the standard error of \(\bar{E}\) is \(se(\bar{E}) = \frac{1}{n_1}\sqrt{\sum_{f \in \boldsymbol{F}} f}\). We obtain bootstrapped data for on- and off-axis points for bootstrap instances \(b=1, ..., B\), and calculate the corresponding mean residual and standard error \(\bar{E}_b\) and \(se(\bar{E}_b)\). Then define the statistic
\[\begin{equation} Q_b = \frac{\bar{E}_b-\bar{E}}{se(\bar{E}_b)} \label{eq:confIntSingle} \end{equation}\]
Note that \(se(\bar{E}_b)\) relies on the bootstrap covariance matrix \(\boldsymbol{F}^b\). Call (\(q_{\alpha/2}\), \(q_{1-\alpha/2}\)) the quantiles of the bootstrap distribution such that \[\begin{equation} \text{P}\left\{Q_b<q_{\alpha/2}\right\} = \text{P}\left\{Q_b>q_{1-\alpha/2} \right\} = \alpha/2 \end{equation}\]
Finally, we find the confidence interval as
\[\begin{equation} \bar{E} - se(\bar{E}_b)q_{\alpha/2}, \bar{E} + se(\bar{E}_b)q_{1-\alpha/2} \end{equation}\]
Of course, this procedure can easily be adapted to find the sum of all raw residuals, but the mean may be better comparable across experiments with different designs.
Depending on the mean-variance structure in the data, residuals are resampled differently. The same strategies are used for resampling 1) residuals with respect to the expected response surface \(R_{ij}\) under the null hypothesis for the meanR and maxR statistics as for 2) residuals \(A_{ij}\) with respect to the average at the off-axis point under the alternative hypothesis for constructing the confidence intervals. In the description below, we use \(U_{ij}\) as generic notation for either \(R_{ij}\) or \(A_{ij}\).
In case of constant variability within the off-axis points, the residuals \(U_{ij}\) can simply be pooled and resampled with replacement.
When a linear mean-variance structure is assumed, one option is to rescale the pointwise residuals first to \(b_{ij} = \frac{U_{ij}}{\sqrt{v^{-1}(\beta_0+\beta_1\mu_i)}}\), then pool and resample them, and then scale them back to \(b_{ij}\sqrt{v^{-1}(\beta_0+\beta_1\mu_i)}\) according to their new position \(i\). Yet in practice this leads to extreme observations, which destabilizes the fitting procedure. A second option is to use random draws from a zero-mean normal distribution with the modelled variance \(v^{-1}(\beta_0+\beta_1\mu_i)\) to generate new \(U_{ij}\)’s. This latter option was found to be more stable and is used as a default in the BIGL package.