Although GLM are a natural choice for count data and have been successfully applied to address a broad range of questions in RNA-seq 32 (link),33 (link), a simpler alternative is to consider a linear model (LM) for some suitable transformation of the read counts (e.g., logarithmic transformation). Such an LM-based version of RUVg reduces to RUV-2 (refs. 19 (link),20 ). Additionally, using a linear model allows approaches such as RUV-4 and RUV-inv (ref. 20 ).
Supplementary Figures 19 and 20 show that LM-based RUVg on log counts does not perform as well as our proposed GLM-based RUVg. In particular, although LM-based RUVg seems effective at removing the unwanted variation (cf. uniform distribution of p-values in Supplementary Fig. 19 ), it does not yield enough power to detect any DE genes, neither when using a standard t-test nor when using an empirical Bayes moderated t-test (limma 34 ).
>
Phenomena
>
Natural Phenomenon or Process
>
Natural Selection
Natural Selection
Natural Selection is a fundamental process in evolutionary biology, in which organisms with favorable traits are more likely to survive and reproduce, passing on their genetic information to future generations.
This process drives the adaptation of species to their environment, leading to the emergence of new and diverse life forms over time.
Researchers utilize various methods, including computational modeling and experiments, to study the mechanisms and dynamics of natural selection, providing insights into the evolutionary history and future of living organisms.
PubCompare.ai's cutting-edge AI-powered tools can assist in this research by optimizing experimental protocols, comparing findings from literature, preprints, and patents, and identifying the most effective approaches to advancing the field of natural selection.
Explore the frontiers of this essential biological principle with the innovative technology of PubCompare.ai.
This process drives the adaptation of species to their environment, leading to the emergence of new and diverse life forms over time.
Researchers utilize various methods, including computational modeling and experiments, to study the mechanisms and dynamics of natural selection, providing insights into the evolutionary history and future of living organisms.
PubCompare.ai's cutting-edge AI-powered tools can assist in this research by optimizing experimental protocols, comparing findings from literature, preprints, and patents, and identifying the most effective approaches to advancing the field of natural selection.
Explore the frontiers of this essential biological principle with the innovative technology of PubCompare.ai.
Most cited protocols related to «Natural Selection»
Genes
Natural Selection
RNA-Seq
To characterize the data, we propose the following Bayesian hierarchical model, based on the beta-binomial distribution. Notation for our model is as follows: at the i-th CpG site, j-th group and k-th replicate, is the number of reads that show methylation, is the total number of reads that cover this position and is the underlying ‘true’ methylation proportion. Since the process of sequencing involves the random sampling of two kinds of reads—methylated or unmethylated, will follow a binomial distribution:
Since the true methylation proportions among replicates can be anywhere between 0 and 1, we assume that the proportions for each CpG site within each group of replicates follow a beta distribution. The beta distribution has long been a natural choice to model binomial proportions as it is a conjugate distribution of the binomial distribution and is the most flexible distribution with a support interval of [0,1].
Here the beta distribution is parameterized by mean (denoted by ) and dispersion (denoted by ). Compared with the traditional parameterization of the Beta ( ) distribution, the parameters have the following relationship:
In this hierarchical model, the biological variation among replicates is captured by the beta distribution and the variation due to the random sampling of DNA segments during sequencing is captured by the binomial distribution. The dispersion parameter captures the variation of a CpG site’s methylation proportion relative to the group mean. We allow each CpG site within a single condition (e.g. within cases, or controls) to have its own dispersion. This is a flexible assumption because it allows either different or common dispersions for both conditions; however, our software also includes an option to assume a common dispersion for cases and controls.
To combine information across all CpG sites, based on the observed distribution of dispersion from a publicly available RRBS dataset on mouse embryogenesis (21 (link)), we assumed the following prior on :
where and are mean and variance parameters that can be estimated from the data. For each CpG site in this dataset, we applied a method of moments (MOM) estimator to estimate the dispersion parameters. As shown inFigure 1 , the genome-wide distribution of logarithm dispersion parameter estimates is approximately Gaussian with mean = –3.39 and SD = 1.08, suggesting that the dispersion parameters can be well-described by a log-normal distribution. However, simulations using dispersions from different distributions also show that our proposed method is robust to violations of this log-normal assumption (Supplementary Figure S1 ).
![]()
Since the true methylation proportions among replicates can be anywhere between 0 and 1, we assume that the proportions for each CpG site within each group of replicates follow a beta distribution. The beta distribution has long been a natural choice to model binomial proportions as it is a conjugate distribution of the binomial distribution and is the most flexible distribution with a support interval of [0,1].
Here the beta distribution is parameterized by mean (denoted by ) and dispersion (denoted by ). Compared with the traditional parameterization of the Beta ( ) distribution, the parameters have the following relationship:
In this hierarchical model, the biological variation among replicates is captured by the beta distribution and the variation due to the random sampling of DNA segments during sequencing is captured by the binomial distribution. The dispersion parameter captures the variation of a CpG site’s methylation proportion relative to the group mean. We allow each CpG site within a single condition (e.g. within cases, or controls) to have its own dispersion. This is a flexible assumption because it allows either different or common dispersions for both conditions; however, our software also includes an option to assume a common dispersion for cases and controls.
To combine information across all CpG sites, based on the observed distribution of dispersion from a publicly available RRBS dataset on mouse embryogenesis (21 (link)), we assumed the following prior on :
where and are mean and variance parameters that can be estimated from the data. For each CpG site in this dataset, we applied a method of moments (MOM) estimator to estimate the dispersion parameters. As shown in
Histogram of the logarithm of estimated CpG-specific dispersion (
Biopharmaceuticals
Chromosomes
DNA Replication
Embryonic Development
Genome
Methylation
Mice, Laboratory
Natural Selection
All simulations were performed
in the isothermal–isobaric ensemble, NPT,
at a pressure of 1 atm. The pressure was held constant by using the
Parrinello–Rahman barostat77 with
a coupling constant of 10.0 ps with an isothermal compressibility
of 4.5 × 10–5 bar–1. For
the bulk liquids an isotropic pressure coupling was used and for the
bilayer simulations a semi-isotropic pressure coupling scheme was
used. The temperature was kept constant by the Nosé–Hoover
thermostat78 ,79 (link) with a coupling constant of 0.5 ps. The
lipid bilayer and water were coupled separately to the thermostat.
Long-range electrostatic interactions were treated by a particle-mesh
Ewald scheme80 ,81 with a real-space cutoff at 1.4
nm with a Fourier spacing of 0.10 nm and a fourth-order interpolation
to the Ewald mesh. Single-atom charge groups were used. van der Waals
interactions were truncated at 1.5 nm and treated with a switch function
from 1.4 nm. Long-range corrections for the potential and pressure
were added.51 The inclusion of long-range
corrections should eliminate the LJ cutoff dependency in the simulations.
Due to the fact that lipid bilayers are inhomogeneous systems the
method introduced by Lagüe et al.82 to add long-range corrections could be applied instead. Periodic
boundary conditions were imposed in every dimension. A time step of
2 fs was used with a Leap-Frog integrator. The LINCS algorithm83 was used to freeze all covalent bonds in the
lipid, and the analytical SETTLE84 method
was used to hold the bonds and angle in water constant. The TIP3P
water model85 was the water model of choice.
The choice of water model can be explained by the fact that TIP3P
is the default water model in major FFs such as AMBER and CHARMM and
since one of the aims of the work presented here was to create a lipid
FF compatible with AMBER this was a natural choice. Further, earlier
work of Högberg et al.31 (link) has shown
that there is flexibility in the choice of water model for AA simulations
of lipid bilayers. Atomic coordinates were saved every 1 ps and the
neighbor list was updated every 10th step.
Bulk liquids were
simulated with a simulation box consisting of 128 molecules for the
larger alkanes and 256 for the smaller alkanes (hexane and heptane)
at a temperature of 298.15 K. The lipid bilayer systems were prepared
using the CHARMM-GUI86 (link),87 (link) with 128 lipids in total, 64
in each leaflet. In order to achieve proper hydration, 30 TIP3P water
molecules were added per lipid. Three different lipid types were simulated,
DLPC (12:0/12:0), DMPC (14:0/14:0), and DPPC (16:0/16:0). These system
were investigated under a range of temperatures; see Table1 for an overview of all simulations performed. All
lipid bilayer systems were equilibrated for 40 ns before production
runs were initiated which lasted for 300–500 ns. All MD simulations
were performed with the Gromacs88 software
package (versions 4.5.3 and 4.5.4). All analysis were made with the
analysis tools that come with the MDynaMix software package.89 System snapshots were rendered and analyzed
with VMD.90 Neutron scattering form factors
were computed with the SIMtoEXP software.91 (link)The calculations of free energies of solvation in
water and cyclohexane
were performed by using thermodynamic integration over 35 λ
values in the range between 0 and 1. A soft core potential (SCP) was
used to avoid singularities when the solute is almost decoupled from
the solvent. The α-parameters used for the SCP and the simulation
workflow were set following the methodology described by Sapay and
Tieleman.92 (link) The amino acid analogues were
solvated with 512 and 1536 molecules of cyclohexane and water, respectively.
in the isothermal–isobaric ensemble, NPT,
at a pressure of 1 atm. The pressure was held constant by using the
Parrinello–Rahman barostat77 with
a coupling constant of 10.0 ps with an isothermal compressibility
of 4.5 × 10–5 bar–1. For
the bulk liquids an isotropic pressure coupling was used and for the
bilayer simulations a semi-isotropic pressure coupling scheme was
used. The temperature was kept constant by the Nosé–Hoover
thermostat78 ,79 (link) with a coupling constant of 0.5 ps. The
lipid bilayer and water were coupled separately to the thermostat.
Long-range electrostatic interactions were treated by a particle-mesh
Ewald scheme80 ,81 with a real-space cutoff at 1.4
nm with a Fourier spacing of 0.10 nm and a fourth-order interpolation
to the Ewald mesh. Single-atom charge groups were used. van der Waals
interactions were truncated at 1.5 nm and treated with a switch function
from 1.4 nm. Long-range corrections for the potential and pressure
were added.51 The inclusion of long-range
corrections should eliminate the LJ cutoff dependency in the simulations.
Due to the fact that lipid bilayers are inhomogeneous systems the
method introduced by Lagüe et al.82 to add long-range corrections could be applied instead. Periodic
boundary conditions were imposed in every dimension. A time step of
2 fs was used with a Leap-Frog integrator. The LINCS algorithm83 was used to freeze all covalent bonds in the
lipid, and the analytical SETTLE84 method
was used to hold the bonds and angle in water constant. The TIP3P
water model85 was the water model of choice.
The choice of water model can be explained by the fact that TIP3P
is the default water model in major FFs such as AMBER and CHARMM and
since one of the aims of the work presented here was to create a lipid
FF compatible with AMBER this was a natural choice. Further, earlier
work of Högberg et al.31 (link) has shown
that there is flexibility in the choice of water model for AA simulations
of lipid bilayers. Atomic coordinates were saved every 1 ps and the
neighbor list was updated every 10th step.
Bulk liquids were
simulated with a simulation box consisting of 128 molecules for the
larger alkanes and 256 for the smaller alkanes (hexane and heptane)
at a temperature of 298.15 K. The lipid bilayer systems were prepared
using the CHARMM-GUI86 (link),87 (link) with 128 lipids in total, 64
in each leaflet. In order to achieve proper hydration, 30 TIP3P water
molecules were added per lipid. Three different lipid types were simulated,
DLPC (12:0/12:0), DMPC (14:0/14:0), and DPPC (16:0/16:0). These system
were investigated under a range of temperatures; see Table
lipid bilayer systems were equilibrated for 40 ns before production
runs were initiated which lasted for 300–500 ns. All MD simulations
were performed with the Gromacs88 software
package (versions 4.5.3 and 4.5.4). All analysis were made with the
analysis tools that come with the MDynaMix software package.89 System snapshots were rendered and analyzed
with VMD.90 Neutron scattering form factors
were computed with the SIMtoEXP software.91 (link)The calculations of free energies of solvation in
water and cyclohexane
were performed by using thermodynamic integration over 35 λ
values in the range between 0 and 1. A soft core potential (SCP) was
used to avoid singularities when the solute is almost decoupled from
the solvent. The α-parameters used for the SCP and the simulation
workflow were set following the methodology described by Sapay and
Tieleman.92 (link) The amino acid analogues were
solvated with 512 and 1536 molecules of cyclohexane and water, respectively.
Alkanes
Amber
Amino Acids
ARID1A protein, human
Cyclohexane
Dietary Fiber
Dimyristoylphosphatidylcholine
Electrostatics
Freezing
Heptane
Lipid Bilayers
Lipids
Maritally Unattached
n-hexane
Natural Selection
Pressure
Rana
Solvents
A list of candidate genes for a particular disease can be gleaned from published association studies, gene expression studies, disease pathways and the specific interests of an investigator. Such lists may be very large, so we first filter the list against GWAS results as shown in Figure 1 . We use SNPs that have genotype data in dbSNP as our source of SNPs in and near a gene (for a user-specified flanking region around the gene). We keep a gene if it has at least one small P-value SNP (less than or equal to a user-specified threshold, T1) in the GWAS. We also keep genes that were not adequately represented by SNPs in the GWAS panel. The percent of common SNPs (within a gene and flanking region) in high LD (pairwise r2 ≥ a user-specified threshold) with any GWAS SNP (including GWAS SNPs outside the gene and flanking region) is calculated and genes with coverage less than a user-specified cutoff A% are retained. Genes that do not have SNPs with small P-value but do have sufficient coverage by GWAS SNPs are excluded from further analysis.
![]()
For the candidate genes that pass the above screen we extract SNPs from dbSNP and process this list as shown in Figure 1 . If a SNP was examined in the GWAS and had a P-value less than the user-specified threshold T1 it is retained. If a SNP was not in the GWAS but was in high LD with a GWAS SNP that had a P-value larger than T1 it is eliminated because we reason that it was adequately evaluated by the GWAS and found to have no association with disease. We then score all retained SNPs for functional significance and apply different minor allele frequency (MAF) filters depending on the functional category of the SNP. These user-specified MAF filters are provided because functionally important SNPs often have lower MAF due to natural selection (6 (link)) and we wish to provide extra flexibility to retain functional SNPs below the MAF filter being applied to SNPs without such function. The details of the functional predictions used in this and other pipelines are provided in a separate section below.
In the final processing step we select LD tag SNPs. Because there are certain advantages to having functional and small P-value SNPs directly assessed by the genotyping panel (instead of being indirectly assessed via LD) we provide for the assignment of user-specified weights for different categories of functional SNPs and small P-value SNPs. If weights are assigned the null value of 1, then tag SNPs are selected simply by rank order, so that SNPs that are in high LD with the largest number of SNPs are selected first and SNPs that tag only themselves (singleton tags) are selected last. If a functional SNP has a weight applied, then the weight act as multiplier of the actual number of SNPs tagged so that it is more likely to be selected early. For example, a functional SNP with a weight of two that is in LD with four SNPs (including itself) would have a weighted tag value of 2 × 4 = 8. Investigators may modify a variety of values (e.g. P-value threshold T1, LD threshold, or weights) to adjust selected SNP counts to fit their genotyping panel size and budget. We provide two options for additional SNP reduction that we think are useful: (i) Each SNP must be in LD with a user-specified minimum number of common SNPs (after multiplied by the user-assigned weights). For example, this option can be used to eliminate singleton SNPs. (ii) A user can also specify the maximum number of SNPs that are allowed for any one gene using a method which is similar to selecting the best N SNPs to optimize power (7 (link)). To insure that each gene has some coverage, we also provide a user-specified minimum number of best SNPs (in terms of number of SNPs captured at a specific LD threshold) that must be selected for each gene even if they do not meet the previous criterion for tag SNPs.
GenePipe: decision tree to prioritize SNPs for candidate genes based on GWAS results, SNP functional prediction characteristics and pair-wise LD. The six-sided boxes represent decision points and rectangles represent action steps or end points.
In the final processing step we select LD tag SNPs. Because there are certain advantages to having functional and small P-value SNPs directly assessed by the genotyping panel (instead of being indirectly assessed via LD) we provide for the assignment of user-specified weights for different categories of functional SNPs and small P-value SNPs. If weights are assigned the null value of 1, then tag SNPs are selected simply by rank order, so that SNPs that are in high LD with the largest number of SNPs are selected first and SNPs that tag only themselves (singleton tags) are selected last. If a functional SNP has a weight applied, then the weight act as multiplier of the actual number of SNPs tagged so that it is more likely to be selected early. For example, a functional SNP with a weight of two that is in LD with four SNPs (including itself) would have a weighted tag value of 2 × 4 = 8. Investigators may modify a variety of values (e.g. P-value threshold T1, LD threshold, or weights) to adjust selected SNP counts to fit their genotyping panel size and budget. We provide two options for additional SNP reduction that we think are useful: (i) Each SNP must be in LD with a user-specified minimum number of common SNPs (after multiplied by the user-assigned weights). For example, this option can be used to eliminate singleton SNPs. (ii) A user can also specify the maximum number of SNPs that are allowed for any one gene using a method which is similar to selecting the best N SNPs to optimize power (7 (link)). To insure that each gene has some coverage, we also provide a user-specified minimum number of best SNPs (in terms of number of SNPs captured at a specific LD threshold) that must be selected for each gene even if they do not meet the previous criterion for tag SNPs.
Gene Expression
Genes
Genes, vif
Genome-Wide Association Study
Natural Selection
Single Nucleotide Polymorphism
Matching on the propensity score was not dealt with in depth by any of the three papers. Zanutto simply stated that “it is less clear in this case [matching] how to incorporate the survey weights from a complex survey design” (page 69),5 while Ridgeway et al. did not consider matching on the propensity score. When using propensity score matching, DuGoff et al. suggested fitting a survey-weighted regression model in the propensity score matched sample. In their simulations, the continuous outcome variable was regressed on an indicator variable denoting treatment status and on the single baseline covariate, resulting in a conditional effect estimate within the matched sample. While this approach may be suitable when outcomes are continuous, such an approach is likely to be problematic when outcomes are binary or time-to-event in nature. The reason for this is that propensity score methods result in marginal estimates of effect, rather than conditional estimates of effect.8 When outcomes are continuous, a linear treatment effect is collapsible: the conditional and marginal estimates coincide. When the outcome is binary, regression adjustment in the propensity score matched sample will typically result in an estimate of the odds ratio. The odds ratio (like the hazard ratio) is not collapsible; thus the marginal and conditional estimates will not coincide.9 Prior research has demonstrated that propensity score matching results in biased estimation of both conditional and marginal odds ratios.10 (link),11 (link) Thus, the method proposed by DuGoff for use with propensity score matching may not perform well when outcomes are binary.
Prior to presenting alternate estimators, we briefly introduce the potential outcomes framework.12 Let Y(1) and Y(0) denote the potential outcomes observed under the active treatment (Z = 1) and the control treatment (Z = 0), respectively. The effect of treatment is defined as Y(1) − Y(0). The average treatment effect (ATE) is defined as . The average treatment effect in the treated (ATT) is defined as . Imai et al. distinguish between two different estimands: the sample average treatment effect (SATE) and the population average treatment effect (PATE).13 The former is the effect of treatment in the analytic sample, while the latter refers to the effect of treatment in the population from which the sample was drawn. The PATE is defined as , while the SATE is defined as , where and denote the number of subjects in the population and in the sample, respectively. We would argue that the population estimand is usually of greater interest than the sample estimand, as researchers typically want to make inferences about the larger population from which the sample was drawn. Typically, one uses a sample estimate to make inferences about a population parameter. In doing so, one must take appropriate analytic steps to ascertain that the estimate pertains to the target population. For this reason, all of the methods that we consider for estimating the effect of treatment in a matched sample will employ the survey weights.
There are a large number of possible algorithms for matching treated and control subjects on the propensity score.14 (link) Popular approaches include nearest neighbour matching (NNM) and NNM within specified calipers of the propensity score.15 ,16 (link) NNM selects a treated subject (typically at random, although one can sequentially select the treated subjects from highest to lowest propensity score) and then selects the control subject whose propensity score is closest to that of the treated subject. The most frequent approach is to use matching without replacement, in which each control is selected for matching to at most one treated subject. NNM within specified calipers of the propensity score is a refinement of NNM, in which a match is considered permissible only if the difference between the treated and control subjects’ propensity scores is below a pre-specified maximal difference (the caliper width). Optimal choice of calipers was studied elsewhere.17 (link) An alternative to these approaches is optimal matching, in which matched pairs are formed so as to minimize the average within-pair difference in the propensity score.18 When using propensity score matching, one is estimating the ATT. For each treated subject, the missing potential outcome under the control intervention is imputed by the observed outcome for the control subject to whom the treated subject was matched. By using the above estimate of the ATT, rather than fit an outcomes regression model in the matched sample, one can simply obtain a marginal estimate of the outcome in treated subjects and a marginal estimate of the outcome in control subjects. These are estimated as the mean outcome in treated and control subjects, respectively. The ATT can then be estimated as the difference in these two quantities.19 (link)As the research interest usually focusses on the population average treatment effect in the treated (PATT), rather than its sample analogue (SATT), the mean potential outcome under the active treatment can be estimated as , where denotes the observed outcome for the ith treated subject in the matched sample, denotes the sampling weight associated with this subject, and Nmatch is the number of matched pairs in the propensity score matched sample. Similarly, the mean potential outcome under the control condition can be estimated as . The PATT for both continuous and binary outcomes can then be estimated as . Failure to include the sampling weights in estimating the ATT would result in an estimate of the SATT, rather than the PATT.
An unaddressed question is which weights should be used for the matched control subjects. As noted above, Zanutto suggested that “it is less clear in this case [matching] how to incorporate the survey weights from a complex survey design” (page 69).5 In propensity score matching, one is attempting to create a control group that resembles the treated group. However, when using weighted survey data, there are two possible populations to which one can standardize the matched control subjects: (i) the population of control subjects that resemble the treated subjects; (ii) the population of treated subjects. The natural choice of weight to use for each control subject would be to use each control subject’s original sampling weight. In using these weights, one is weighting the control subjects to reflect the population of control subjects that resemble the population of treated subjects. An alternative choice would be to weight the matched control subjects using the population of treated subjects as the reference population. To do so, one would have each matched control subject inherit the weight of the treated subject to whom they were matched. Treated and control subjects with the same propensity score have observed baseline covariates that come from the same multivariable distribution.1 This suggests that if control subjects inherit the weight of the treated subject to whom they were matched, then the distribution of baseline covariates in the weighted sample will be similar between treated and control subjects, using the population of treated subjects as the reference population. In this paper, we use the term ‘natural weight’ when each matched control subject retains its own survey sampling weight, and the term ‘inherited weight’ when each matched control subject inherits the weight of the treated subject to whom it was matched.
Prior to presenting alternate estimators, we briefly introduce the potential outcomes framework.12 Let Y(1) and Y(0) denote the potential outcomes observed under the active treatment (Z = 1) and the control treatment (Z = 0), respectively. The effect of treatment is defined as Y(1) − Y(0). The average treatment effect (ATE) is defined as . The average treatment effect in the treated (ATT) is defined as . Imai et al. distinguish between two different estimands: the sample average treatment effect (SATE) and the population average treatment effect (PATE).13 The former is the effect of treatment in the analytic sample, while the latter refers to the effect of treatment in the population from which the sample was drawn. The PATE is defined as , while the SATE is defined as , where and denote the number of subjects in the population and in the sample, respectively. We would argue that the population estimand is usually of greater interest than the sample estimand, as researchers typically want to make inferences about the larger population from which the sample was drawn. Typically, one uses a sample estimate to make inferences about a population parameter. In doing so, one must take appropriate analytic steps to ascertain that the estimate pertains to the target population. For this reason, all of the methods that we consider for estimating the effect of treatment in a matched sample will employ the survey weights.
There are a large number of possible algorithms for matching treated and control subjects on the propensity score.14 (link) Popular approaches include nearest neighbour matching (NNM) and NNM within specified calipers of the propensity score.15 ,16 (link) NNM selects a treated subject (typically at random, although one can sequentially select the treated subjects from highest to lowest propensity score) and then selects the control subject whose propensity score is closest to that of the treated subject. The most frequent approach is to use matching without replacement, in which each control is selected for matching to at most one treated subject. NNM within specified calipers of the propensity score is a refinement of NNM, in which a match is considered permissible only if the difference between the treated and control subjects’ propensity scores is below a pre-specified maximal difference (the caliper width). Optimal choice of calipers was studied elsewhere.17 (link) An alternative to these approaches is optimal matching, in which matched pairs are formed so as to minimize the average within-pair difference in the propensity score.18 When using propensity score matching, one is estimating the ATT. For each treated subject, the missing potential outcome under the control intervention is imputed by the observed outcome for the control subject to whom the treated subject was matched. By using the above estimate of the ATT, rather than fit an outcomes regression model in the matched sample, one can simply obtain a marginal estimate of the outcome in treated subjects and a marginal estimate of the outcome in control subjects. These are estimated as the mean outcome in treated and control subjects, respectively. The ATT can then be estimated as the difference in these two quantities.19 (link)As the research interest usually focusses on the population average treatment effect in the treated (PATT), rather than its sample analogue (SATT), the mean potential outcome under the active treatment can be estimated as , where denotes the observed outcome for the ith treated subject in the matched sample, denotes the sampling weight associated with this subject, and Nmatch is the number of matched pairs in the propensity score matched sample. Similarly, the mean potential outcome under the control condition can be estimated as . The PATT for both continuous and binary outcomes can then be estimated as . Failure to include the sampling weights in estimating the ATT would result in an estimate of the SATT, rather than the PATT.
An unaddressed question is which weights should be used for the matched control subjects. As noted above, Zanutto suggested that “it is less clear in this case [matching] how to incorporate the survey weights from a complex survey design” (page 69).5 In propensity score matching, one is attempting to create a control group that resembles the treated group. However, when using weighted survey data, there are two possible populations to which one can standardize the matched control subjects: (i) the population of control subjects that resemble the treated subjects; (ii) the population of treated subjects. The natural choice of weight to use for each control subject would be to use each control subject’s original sampling weight. In using these weights, one is weighting the control subjects to reflect the population of control subjects that resemble the population of treated subjects. An alternative choice would be to weight the matched control subjects using the population of treated subjects as the reference population. To do so, one would have each matched control subject inherit the weight of the treated subject to whom they were matched. Treated and control subjects with the same propensity score have observed baseline covariates that come from the same multivariable distribution.1 This suggests that if control subjects inherit the weight of the treated subject to whom they were matched, then the distribution of baseline covariates in the weighted sample will be similar between treated and control subjects, using the population of treated subjects as the reference population. In this paper, we use the term ‘natural weight’ when each matched control subject retains its own survey sampling weight, and the term ‘inherited weight’ when each matched control subject inherits the weight of the treated subject to whom it was matched.
Natural Selection
Specimen Handling
Target Population
Training Programs
Most recents protocols related to «Natural Selection»
To understand the molecular evolution at the amino acid level and the intensity of natural selection acting on metabolism in a specific clade, we used a tree based on codon alignment produced by the maximum-likelihood method using the software EasyCodeML109 (link). We retrieved Coding Sequencing (CDS) sequences from TPS-b genes from A. thaliana, E. grandis, P. cattleyanum, V. vinifera and P. trichocarpa species in Phytozome v11 (http://phytozome.jgi.doe.gov/ ; last accessed November 2020), to use in positive selection analysis. The dataset included 76 sequences and 389 amino acids from five species. We performed statistical analysis using the CodeML program in PAML version 4.9 software using the site, branch, and branch-site models110 (link), implemented in EasyCodeML109 (link).
Parameter estimates (ω) and likelihood scores111 (link) were calculated for the three pairs of models. These were M0 (one-ratio, assuming a constant ω ratio for all coding sites) vs. M3 (discrete, allowed for three discrete classes of ω within the gene), M1a (nearly neutral, allowed for two classes of ω sites: negative sites with ω0 < 1 estimated from our data and neutral sites with ω1 = 1) vs. M2a (positive selection, added a third class with ω2 possibly > 1 estimated from our data), and M7 (beta, a null model in which ω was assumed to be beta-distributed among sites) vs. M8 (beta and ω, an alternative selection model that allowed an extra category of positively selected sites)112 (link).
A series of branch models and branch site models were tested: the one-ratio model for all lineages and the two-ratio model, where the original enzyme functional evolution occurred. The branch-site model assumes that the branches in the phylogeny are divided into the foreground (the one of interest for which positive selection is expected) and background (those not expected to exhibit positive selection).
Likelihood ratio tests (LRT) were conducted to determine which model measured the statistical significance of the data. The twice the log likelihood difference between each pair of models (2ΔL) follows a chi-square distribution with the number of degrees of freedom equal to the difference in the number of free parameters, resulting in a p-value for this113 (link). A significantly higher likelihood of the alternative model compared to the null model suggests positive selection. Positive sites with high posterior probabilities (> 0.95) were obtained using empirical Bayes analysis. If ω > 1, then there is a positive selection on some branches or sites, but the positive selection sites may occur in very short episodes or on only a few sites during the evolution of duplicated genes; ω < 1 suggests a purifying selection (selective constraints), and ω = 1 indicates neutral evolution. Finally, naive empirical Bayes (NEB) approaches were used to calculate the posterior probabilities that a site comes from the site class with ω > 1112 (link). The selected sites and images of protein topology were predicted using Protter114 (link).
Parameter estimates (ω) and likelihood scores111 (link) were calculated for the three pairs of models. These were M0 (one-ratio, assuming a constant ω ratio for all coding sites) vs. M3 (discrete, allowed for three discrete classes of ω within the gene), M1a (nearly neutral, allowed for two classes of ω sites: negative sites with ω0 < 1 estimated from our data and neutral sites with ω1 = 1) vs. M2a (positive selection, added a third class with ω2 possibly > 1 estimated from our data), and M7 (beta, a null model in which ω was assumed to be beta-distributed among sites) vs. M8 (beta and ω, an alternative selection model that allowed an extra category of positively selected sites)112 (link).
A series of branch models and branch site models were tested: the one-ratio model for all lineages and the two-ratio model, where the original enzyme functional evolution occurred. The branch-site model assumes that the branches in the phylogeny are divided into the foreground (the one of interest for which positive selection is expected) and background (those not expected to exhibit positive selection).
Likelihood ratio tests (LRT) were conducted to determine which model measured the statistical significance of the data. The twice the log likelihood difference between each pair of models (2ΔL) follows a chi-square distribution with the number of degrees of freedom equal to the difference in the number of free parameters, resulting in a p-value for this113 (link). A significantly higher likelihood of the alternative model compared to the null model suggests positive selection. Positive sites with high posterior probabilities (> 0.95) were obtained using empirical Bayes analysis. If ω > 1, then there is a positive selection on some branches or sites, but the positive selection sites may occur in very short episodes or on only a few sites during the evolution of duplicated genes; ω < 1 suggests a purifying selection (selective constraints), and ω = 1 indicates neutral evolution. Finally, naive empirical Bayes (NEB) approaches were used to calculate the posterior probabilities that a site comes from the site class with ω > 1112 (link). The selected sites and images of protein topology were predicted using Protter114 (link).
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Amino Acids
Biological Evolution
Codon
Enzymes
Evolution, Molecular
Evolution, Neutral
Exons
Genes
Metabolism
Natural Selection
Proteins
Trees
Sequence analysis included 80 nucleotide sequences of PfGARP from Thai isolates, one clinical isolate from Guinea (isolate MDCU32) and 18 publicly available complete gene sequences whose isolate names, country of origins and their GenBank accession numbers are as follows: 3D7 (Netherlands from West Africa, AL844501), CD01 (Congo, LR129686), Dd2 (Indochina, LR131290), FC27 (Papua New Guinea, J03998), FCC1/HN (Hainan in China, AF251290), GA01 (Gambia, LR131386), GB4 (Ghana, LR131402), KH1 (Cambodia, LR131418), KH2 (Cambodia, LR131306), HB3 (Honduras, LR131338), IGH-CR14 (India, GG6656811), IT (Brazil, LR131322), KE01 (Kenya, LR131354), ML01 (Mali, LR131481), SD01 (Sudan, LR131466), SN01 (Senegal, LR131434), TG01 (Togo, LR131450), and UGT5.1 (Vietnam, KE124372). Of these, the 3D7, FC27and FCC1/HN sequences were determined by Sanger dideoxy-chain termination method whereas the remaining isolates were assembled sequences from next-generation sequencing platforms (Supplemental Table S1 ). Sequence alignment was performed by using the CLUSTAL_X program, taken into account appropriate codon match in the coding region by manual adjustment to maintain the reading frame. The sequence from the FC27 strain was used as a reference6 (link). Searching for nucleotide repeats was performed by using the Tandem Repeats Finder version 4.0 program with the default option. Nucleotide diversity (π), the rate of synonymous substitutions per synonymous site (dS) and the rate of nonsynonymous substitutions per nonsynonymous site (dN) were determined from the average values of sequence differences in all pairwise comparison of each taxon and the standard error was computed from 1000 bootstrap pseudoreplicates implemented in the MEGA 6.0 program41 (link). Haplotype diversity and its sampling variance were computed by taking into account the presence of gaps in the aligned sequences using the DnaSP version 5.10 program42 (link). Natural selection on codon substitution was determined by using fast unconstrained Bayesian approximation (FUBAR) method in the Datamonkey Web-Server43 (link),44 (link). Neighbor-joining phylogenetic tree based on nucleotide sequences was constructed by using maximum composite likelihood parameter whereas maximum likelihood tree was built using Tamura-Nei model with the rate variation model allowed for some sites to be evolutionarily invariable. The Arlequin 3.5.2.2 software was deployed to determine genetic differentiation between populations, the fixation index (FST), using analysis of molecular variance approach (AMOVA) akin to the Weir and Cockerham’s method but taken into account the number of mutations between haplotypes45 (link). One hundred permutations were deployed to determine the significance levels of the fixation indices. Prediction of linear B cell epitopes in PfGARP was performed by using a sequence similarity to known experimentally verified epitopes from the Immune Epitope DataBase (IEDB) implemented in the BepiBlast Web Server11 (link). Furthermore, linear B cell epitopes were also predicted based on protein language models implemented in BepiPred-3.012 (link). Potential HLA-class II-binding peptides were analyzed by using the IEDB recommended 2.22 algorithm with a default 12–18 amino acid residues option. The predicted HLA-class II-binding peptides were predicted based on the percentile rank < 10 and the IC50 threshold for HLA binding affinity ≤ 1000 nM14 (link). The analysis mainly concerned the common HLA class II haplotypes among Thai populations with allele frequency > 0.113 (link).
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Amino Acids
Codon
Epitopes
Epitopes, B-Lymphocyte
Genes
Genetic Drift
Haplotypes
Hereditary Nonpolyposis Colorectal Cancer Type 1
Mutation
Natural Selection
Nucleotides
Peptides
Population Group
Proteins
Reading Frames
Sequence Alignment
Sequence Analysis
Strains
Tandem Repeat Sequences
Thai
Trees
We used a Bayesian latent hierarchical compositional manova with a multinomial observation model to determine how final proportional cover was affected by treatments. A manova is the obvious way to examine patterns in multiple species, and a compositional approach is needed because we have relative abundance data, for which the standard vector addition and scalar multiplication operations used in manova are not appropriate. Pawlowsky-Glahn, Egozcue & Tolosana-Delgado (2015) is a good introduction to compositional data analysis. A multinomial observation model is the obvious choice for data derived from point counts. We analyzed the pre-treatment data from the final photographic sampling date, and included only A. aurita growing directly on panels, bare panel and other taxa contributing at least 20 points to the point count data for at least one panel: Botrylloides spp., Bugula spp. and Molgula tubifera. Together, these five taxa accounted for 90–100 points out of 100 on every panel in the pre-treatment point count data from the final week, and no other taxon contributed more than seven points on any panel. Compositional data analysis is subcompositionally coherent (Egozcue & Pawlowsky-Glahn, 2011 , Section 2.3.2), which means that results for the subcomposition we studied do not depend on excluded taxa. We therefore analyzed final subcompositions of the form , where parts one to five represent A. aurita on panel, bare panel, Botrylloides spp., Bugula spp. and M. tubifera, respectively. We represented these final subcompositions in isometric logratio (ilr) coordinates (Egozcue et al., 2003 (link)) using the contrast matrix described in the supporting information, Section S1 .
Let be the vector of point count data for the single panel from depth , treatment , block , and let be the total number of points counted in this observation (between 90 and 100). We modelled these data using a Bayesian latent hierarchical compositional manova with a multivariate observation model:
Here, is the vector of expected relative abundances for the panel from depth , treatment , block . The isometric log transformation of is a vector in , formed from the sum of an overall mean vector , the effect of depth , the effect of treatment , the effect of the interaction between depth and treatment , the effect of block and the effect of the panel from depth , treatment , block . The block and panel effects are modelled hierarchically, drawn from 4-dimensional multivariate normal distributions with mean vector and covariance matrices and Σ respectively (independent of each other and of the explanatory variables). Note that can be written in the simplex as
where the primes indicate transformations of the corresponding parameters in 4, and denotes the perturbation operator (Aitchison, 1986 , p. 42). We coded treatment effects as described in the supporting information,Section S2 . Similar models have been used for effects of vegetation disturbance and predator manipulation on terrestrial arthropod communities (Billheimer, Guttorp & Fagan, 2001 (link)), effects of depth on community composition at our study site (Chong & Spencer, 2018 (link)), and effects of cyclones and bleaching on coral reef composition (Vercelloni et al., 2020 (link)).
We fitted the model using Bayesian estimation in cmdstan 2.23.0 (Carpenter et al., 2017 (link)), which implements a dynamic Hamiltonian Monte Carlo algorithm (Hoffman & Gelman, 2014 ). Details of priors are given in the supporting information,Section S3 . Details of fitting, checking and calibration are given in the supporting information, Section S4 .
We compared the ability to predict new observations between the full model and simpler models (without the interaction between depth and treatment, without depth, or without treatment) using leave-one-cluster-out cross-validation. The natural choice for “new observations” is a new block of panels, because a replication of the experiment would involve a new set of blocks, rather than new panels within existing blocks or new observations on existing panels. We therefore evaluated models based on marginal rather than conditional likelihoods with respect to block and panel effects (Merkle, Furr & Rabe-Hesketh, 2019 (link)). Details are in the supporting information,Section S5 .
Our primary interest is in responses of A. aurita, bare panel and potential competitors as a whole, rather than variation within the subcomposition of potential competitors. Visualizing is not easy, so we decomposed treatment effects into two orthogonal components, each of which can be represented in a ternary plot: effects on A. aurita, bare panel and potential competitors as a whole, and effects on the subcomposition of potential competitors (supporting information,Section S6 ).
We assessed the effects of potential competitors on A. aurita using differences in between potential competitor removal (O) and control (C) treatments. Similarly, we assessed the effects of A. aurita on potential competitors using differences in between A. aurita removal (A) and control (C) treatments, as described in the supporting information,Section S7 .
Let be the vector of point count data for the single panel from depth , treatment , block , and let be the total number of points counted in this observation (between 90 and 100). We modelled these data using a Bayesian latent hierarchical compositional manova with a multivariate observation model:
Here, is the vector of expected relative abundances for the panel from depth , treatment , block . The isometric log transformation of is a vector in , formed from the sum of an overall mean vector , the effect of depth , the effect of treatment , the effect of the interaction between depth and treatment , the effect of block and the effect of the panel from depth , treatment , block . The block and panel effects are modelled hierarchically, drawn from 4-dimensional multivariate normal distributions with mean vector and covariance matrices and Σ respectively (independent of each other and of the explanatory variables). Note that can be written in the simplex as
where the primes indicate transformations of the corresponding parameters in 4, and denotes the perturbation operator (Aitchison, 1986 , p. 42). We coded treatment effects as described in the supporting information,
We fitted the model using Bayesian estimation in cmdstan 2.23.0 (Carpenter et al., 2017 (link)), which implements a dynamic Hamiltonian Monte Carlo algorithm (Hoffman & Gelman, 2014 ). Details of priors are given in the supporting information,
We compared the ability to predict new observations between the full model and simpler models (without the interaction between depth and treatment, without depth, or without treatment) using leave-one-cluster-out cross-validation. The natural choice for “new observations” is a new block of panels, because a replication of the experiment would involve a new set of blocks, rather than new panels within existing blocks or new observations on existing panels. We therefore evaluated models based on marginal rather than conditional likelihoods with respect to block and panel effects (Merkle, Furr & Rabe-Hesketh, 2019 (link)). Details are in the supporting information,
Our primary interest is in responses of A. aurita, bare panel and potential competitors as a whole, rather than variation within the subcomposition of potential competitors. Visualizing is not easy, so we decomposed treatment effects into two orthogonal components, each of which can be represented in a ternary plot: effects on A. aurita, bare panel and potential competitors as a whole, and effects on the subcomposition of potential competitors (supporting information,
We assessed the effects of potential competitors on A. aurita using differences in between potential competitor removal (O) and control (C) treatments. Similarly, we assessed the effects of A. aurita on potential competitors using differences in between A. aurita removal (A) and control (C) treatments, as described in the supporting information,
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Arthropods
Cardiac Arrest
Cloning Vectors
Cyclonic Storms
DNA Replication
Natural Selection
Specimen Handling
The model of Pichancourt et al. (2014) (link) is primarily based on the life-history theory. According to this theory, biophysical constraints on the allocation of energy between reproduction, growth and self-maintenance are viewed as the primary explanation for why species do not possess arbitrary combinations of life-history traits (LHTs) between organs and life-stages, throughout the life cycle of the organism. These ultimately drive the population growth rate of species to adapt to their environmental conditions. To reflect this principle, the model is structured according to a multiple-tier approach to LHTs (Fig. 2 ).
The first tier of LHTs represents the specific vital rates of stage and size throughout the life cycle of a tree species (i.e., seed survival, germination, tree growth, survival and fertility). These traits are constrained by allometric traits that are assumed to be optimally defined by natural selection (the second tier of LHTs, as outlined by the scaling theory of ecology). Finally, the second tier of LHTs is itself constrained by the third tier—the metabolic LHTs—based on the different physiological processes, e.g., photosynthetic carbon assimilation, respiration, Vmax, Jmax, biomass turnover, water absorption, carbon biomass production (as outlined, e.g., by the metabolic theory of ecology).
For plant species, the theory also predicts that ~50% of the variability of most of the tree LHTs on Earth can ultimately be reduced to three ((van Bodegom, Douma & Verheijen, 2014 (link)): specific leaf area (SLA) (m2.kg−1); specific wood density (SWD) (kg.m−3); and seed size (SS) (kg)). Under this realistic assumption, species with similar values of these three LHTs share other similar 1–2- and 3-tier LHT and life-cycle strategies. Based on this organization, mathematical models can be developed to create a wide range of unique tree species life cycle strategies (see summary of models in Pichancourt et al. (2014) (link) and in van Bodegom, Douma & Verheijen (2014) (link)). In this article, computational capabilities limited our exploration to eight species, representing all the combinations between a range of extreme values of LHTs found in the literature (see Pichancourt et al., 2014 (link)): SLA (2.5–20 m2.kg−1); SWD (400–1,000 kg.m−3); and SS (10−7–10−3 kg per seed).
The first tier of LHTs represents the specific vital rates of stage and size throughout the life cycle of a tree species (i.e., seed survival, germination, tree growth, survival and fertility). These traits are constrained by allometric traits that are assumed to be optimally defined by natural selection (the second tier of LHTs, as outlined by the scaling theory of ecology). Finally, the second tier of LHTs is itself constrained by the third tier—the metabolic LHTs—based on the different physiological processes, e.g., photosynthetic carbon assimilation, respiration, Vmax, Jmax, biomass turnover, water absorption, carbon biomass production (as outlined, e.g., by the metabolic theory of ecology).
For plant species, the theory also predicts that ~50% of the variability of most of the tree LHTs on Earth can ultimately be reduced to three ((van Bodegom, Douma & Verheijen, 2014 (link)): specific leaf area (SLA) (m2.kg−1); specific wood density (SWD) (kg.m−3); and seed size (SS) (kg)). Under this realistic assumption, species with similar values of these three LHTs share other similar 1–2- and 3-tier LHT and life-cycle strategies. Based on this organization, mathematical models can be developed to create a wide range of unique tree species life cycle strategies (see summary of models in Pichancourt et al. (2014) (link) and in van Bodegom, Douma & Verheijen (2014) (link)). In this article, computational capabilities limited our exploration to eight species, representing all the combinations between a range of extreme values of LHTs found in the literature (see Pichancourt et al., 2014 (link)): SLA (2.5–20 m2.kg−1); SWD (400–1,000 kg.m−3); and SS (10−7–10−3 kg per seed).
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Carbon
Cell Respiration
Fertility
Germination
Life History Traits
Natural Selection
Photosynthesis
Physiological Processes
Plant Leaves
Plants
Reproduction
Trees
The energy of a state can also be extracted by tracking the global phase that it acquires during time propagation. This is given by the phase of the autocorrelation function, which is a discrete time series of the inner product between a propagated state and the initial state. Suppose that we time propagate an eigenstate Ψn of with energy En. The corresponding autocorrelation signal is where the absolute value ∣⟨Ψ(t = 0)∣Ψ(t)⟩∣ should be close to unity, and in this work, we use it as one measure of a simulation’s veracity.
On a quantum computer, this otherwise-unobservable global phase is efficiently extracted using phase estimation. Phase estimation through the use of ancilla qubits (67 ) is one of the fundamental techniques used in diverse applications of quantum computing, and its utility in the context of SO-QFT and first-quantized simulation is well recognized [see, e.g., (5 (link))].
In the IPE approach, even a single ancilla (8 , 68 ) is sufficient to learn this phase; a resource cost saving that will be welcome in the early fault-tolerant regime. The method is summarized on the left ofFig. 10 . We conditionally apply N SO-QFT steps UN(δt) controlled by an ancillary qubit in the ∣+⟩ state. At the Nth step, we measure the ancillary qubit in the ∣+⟩ basis, at which point the state is discarded. We see that for an eigenstate, the global phase information is encoded in the relative phase between the ∣0⟩ and ∣1⟩ state of the ancillary qubit
The probability of finding the ancillary qubit in state ∣+⟩ fluctuates as the phase. We use this to extract a periodic time signal a(t) where the frequency is proportional to the energy of the simulated wave function
Because the number of qubits that we can classically emulate is limited, using the single-ancilla IPE for our demonstrations here is a natural choice. We report the exact evolution of a(t) plotted at regular time points; this is straightforward since we use classically emulated quantum processors. On a real device, because the single-ancilla projection probability is statistical in nature, the time propagation and measurement will have to be repeated multiple times.
If more ancilla qubits are available, then this naturally extends to the standard Fourier phase estimation; for completeness, we include this in the Supplementary Materials, where we also note the use of classical Fourier analysis to extract features if the hardware is limited to a single ancilla.
On a quantum computer, this otherwise-unobservable global phase is efficiently extracted using phase estimation. Phase estimation through the use of ancilla qubits (67 ) is one of the fundamental techniques used in diverse applications of quantum computing, and its utility in the context of SO-QFT and first-quantized simulation is well recognized [see, e.g., (5 (link))].
In the IPE approach, even a single ancilla (8 , 68 ) is sufficient to learn this phase; a resource cost saving that will be welcome in the early fault-tolerant regime. The method is summarized on the left of
The probability of finding the ancillary qubit in state ∣+⟩ fluctuates as the phase. We use this to extract a periodic time signal a(t) where the frequency is proportional to the energy of the simulated wave function
Because the number of qubits that we can classically emulate is limited, using the single-ancilla IPE for our demonstrations here is a natural choice. We report the exact evolution of a(t) plotted at regular time points; this is straightforward since we use classically emulated quantum processors. On a real device, because the single-ancilla projection probability is statistical in nature, the time propagation and measurement will have to be repeated multiple times.
If more ancilla qubits are available, then this naturally extends to the standard Fourier phase estimation; for completeness, we include this in the Supplementary Materials, where we also note the use of classical Fourier analysis to extract features if the hardware is limited to a single ancilla.
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Biological Evolution
Medical Devices
Natural Selection
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