Abstract
Developing genomic selection (GS) models is an important step in applying GS to accelerate the rate of genetic gain in grain yield in plant breeding. In this study, seven genomic prediction models under two cross-validation (CV) scenarios were tested on 287 advanced elite spring wheat lines phenotyped for grain yield (GY), thousand-grain weight (GW), grain number (GN), and thermal time for flowering (TTF) in 18 international environments (year-location combinations) in major wheat-producing countries in 2010 and 2011. Prediction models with genomic and pedigree information included main effects and interaction with environments. Two random CV schemes were applied to predict a subset of lines that were not observed in any of the 18 environments (CV1), and a subset of lines that were not observed in a set of the environments, but were observed in other environments (CV2). Genomic prediction models, including genotype × environment (G×E) interaction, had the highest average prediction ability under the CV1 scenario for GY (0.31), GN (0.32), GW (0.45), and TTF (0.27). For CV2, the average prediction ability of the model including the interaction terms was generally high for GY (0.38), GN (0.43), GW (0.63), and TTF (0.53). Wheat lines in site-year combinations in Mexico and India had relatively high prediction ability for GY and GW. Results indicated that prediction ability of lines not observed in certain environments could be relatively high for genomic selection when predicting G×E interaction in multi-environment trials.
Keywords: genomic prediction, pedigree-based prediction, WAMI, spring wheat, GBLUP, genomic selection, GenPred, Shared Data Resources
Wheat is the most widely cultivated cereal crop in the world, and provides 20% of the protein and calories consumed by the world population (FAOSTAT). Several studies have reported that the present rate of genetic gain in spring wheat is <1% yr−1 (Aisawi et al. 2015; Sayre et al. 1997; Manes et al. 2012; Lopes et al. 2012); that rate needs to improve to meet future wheat demand (Reynolds et al. 2012). This can be done through improvements in plant structure and reproduction, and in crop physiology (radiation use efficiency), as well as improved genotyping or phenotyping methods, increased genetic diversity of breeding germplasm, or through the use of complementary genomic selection approaches in plant breeding (Reynolds et al. 2009; Tester and Langridge 2010).
Traditional breeders use the pedigree selection method for breeding most crops, which requires several generations of testing and advancing the lines. An alternative method is marker-assisted selection (MAS), where markers associated with genes of major effect are used (Spindel et al. 2015). The first to propose predicting breeding values of complex traits for unobserved phenotypes using all available high density markers were Meuwissen et al. (2001). This initial study was followed, in plants, by Bernardo and Yu (2007), who demonstrated, by simulation, that whole genome regression predicts complex traits more accurately than using only a few markers. These seminal investigations led to the application of different statistical parametric and nonparametric genomic models with pedigree information in different crops (Crossa et al. 2010, 2014; Jarquin et al. 2014; Pérez-Rodríguez et al. 2015; Velu et al. 2016; de los Campos et al. 2013; de los Campos and Pérez-Rodríguez 2013; Arruda et al. 2015).
All the initial genomic prediction models were developed for single-environment prediction. However, GS can accelerate genetic gains in wheat breeding, especially when multi-environment testing of lines is routine in their development and release (Braun et al. 2010). Multi-environment testing is prone to high levels of genotype × environment (G×E) interaction due to varying climatic zones, dynamic weather parameters, and different management factors. Burgueño et al. (2012) were the first to use marker- and pedigree-based Best Linear Unbiased Predictor (BLUP) models for assessing G×E under genomic prediction; these models account for correlated environmental structures, and thus predict performance of unobserved phenotypes in several environments. Heslot et al. (2014) incorporated crop modeling data for studying genomic G×E, and Jarquín et al. (2014) proposed a random effect genomic BLUP (GBLUP) model, where the main effect and the G×E interaction effects of markers and environmental covariates are introduced via covariance structures of markers and environmental covariables in a reaction norm model.
The reaction norm model of Jarquín et al. (2014) has been widely used in multi-environment data of different crops, including wheat data with pedigree and genomic information and their interaction with environments (Pérez-Rodríguez and de los Campos 2014; Crossa et al. 2016; Velu et al. 2016). This model is flexible and allows the incorporation of highly dimensional environmental covariable data. Furthermore, a similar genomic G×E model was recently developed and used on wheat breeding data, with the novelty that it decomposes the total marker × environment effect into a marker main effect across all the environments, and a marker-specific effect for each environment (López-Cruz et al. 2015). A recent study by Crossa et al. (2015) showed how the marker × environment model can be used both as a prediction model, by means of shrinkage regression, and/or as a variable selection to estimate marker effects.
Previous genomic and pedigree studies on assessing the prediction ability of G×E have considered a very limited number of environments; they usually included combinations of sites under a few agronomic management systems (i.e., levels of managed drought and heat stress). In the present study, we assess the genomic prediction ability of several models within the framework of the reaction norm model of Jarquín et al. (2014) using the Wheat Association Mapping Initiative (WAMI) panel-designed to evaluate G×E for grain yield (GY), while avoiding the confounding effects of extreme phenology (Lopes et al. 2015). The main objective of this study was to detect prediction ability of different international sites established in different years, with the objective of examining and identifying possible key testing sites to be further used in a genomic-assisted breeding program. A total of 287 spring wheat lines included in the WAMI data were grown in international multi-environment trials in 18 site-year combinations in South and West Asia, North Africa, and Mexico. Traits included in this study are grain yield (GY), grain number (GN), thousand-grain weight (GW) and thermal time for flowering (TTF).
The WAMI panel used in this study is very appropriate for studying genomic and pedigree prediction because its lines were phenotyped under a very diverse set of environments around the world. Also, the WAMI panel has already been studied for several complex traits: adaptation to plant density (Sukumaran et al. 2015b), grain yield and yield components (Sukumaran et al. 2015a), drought stress (Edae et al. 2014), and earliness per se (Sukumaran et al. 2016).
Materials and Methods
The genetic material
The WAMI population was assembled from the elite advanced wheat nurseries distributed through the International Wheat Improvement Network (IWIN). It consists of 287 diverse elite lines selected from nurseries bred for high yield potential environments (Lopes et al. 2015; Sukumaran et al. 2015a,b).
Phenotyping and genotyping
The WAMI population was phenotyped in major wheat-growing areas of India, Pakistan, Nepal, Bangladesh, Iran, Egypt, Sudan, and Mexico. These growing environments are diverse in terms of rainfall, heat stress, drought stress, and solar radiation patterns. Phenotyping was conducted at the following locations: Bangladesh Agricultural Research Institute (BARI), Joydebpur, Bangladesh (BGLD J); Indian Agricultural Research Institute (IARI), Delhi (India D); University of Agricultural Sciences, Dharwad, Karnataka (India H); Indian Institute of Wheat and Barley Research, Karnal, India (India K); Punjab Agricultural University, Ludhiana, India (India L); Darab Hassan Abad, Fars, Iran (Iran D); Banaras Hindu University, Varanasi (India V); National Wheat Research Program, Bhairahawa, Rupandehi (Nepal B); and National Agricultural Research Centre, Islamabad (PAK I). In addition, phenotyping was done under four different treatments at the Norman Borlaug Experiment Station, Cd. Obregon, Sonora, Mexico: irrigated yield potential (Mex I), heat stress (Mex H), drought stress (Mex D), and heat and drought stress (Mex HD) (Figure 1). Table 1 shows the countries, locations, and abbreviations used in this study, as well as the four traits that were recorded and analyzed: GY per square meter, GN per square meter, GW estimated using standard protocols (Sayre et al. 1997), and TTF estimated based on a base temperature of zero and the sowing date. Minimum and maximum temperatures, and the coordinates of the environments, were described in an earlier publication (Sukumaran et al. 2016).
Table 1. Descriptive statistics of the wheat association mapping initiative (WAMI) panel grown in several international environments.
Country | Location | Abbreviation | GY (Tons/Ha) | GN (Number) | GW | TTF |
---|---|---|---|---|---|---|
Bangladesh | Joydebpur | BGLD J10 | 2.2 ± 0.3 | 7314 ± 1249 | 30.9 ± 4.1 | 1260 ± 54 |
BGLD J11 | 3.4 ± 0.5 | 11,326 ± 1807 | 31.1 ± 4.1 | 1261 ± 64 | ||
India | Delhi | India D10 | 3.8 ± 0.6 | 11,520 ± 2018 | 33.6 ± 2.3 | 1343 ± 22 |
Dharwad | India H10 | 3.1 ± 0.4 | 11,415 ± 1914 | 27.6 ± 3.1 | 1336 ± 13 | |
Indore | India I11 | 5.7 ± 0.9 | 17,542 ± 3125 | 32.7 ± 3.7 | 1304 ± 46 | |
Karnal | India K10 | 4.2 ± 0.7 | 11,729 ± 2185 | 36.5 ± 4.1 | 1223 ± 46 | |
Ludhiana | India L11 | 4.3 ± 0.7 | 11,386 ± 1502 | 38.3 ± 2.8 | 1422 ± 64 | |
Varanasi | India V10 | 3.2 ± 0.6 | 14,189 ± 3079 | 23.2 ± 2.3 | 1242 ± 25 | |
Mexico | Droughta | Mex D10 | 3.7 ± 0.4 | 9902 ± 1204 | 37.7 ± 4.5 | 1175 ± 45 |
Heata | Mex H10 | 4.0 ± 0.4 | 13,341 ± 1849 | 30.5 ± 3.5 | 976 ± 41 | |
Heat droughta | Mex HD10 | 3.4 ± 0.4 | 11,831 ± 1931 | 29.2 ± 4.2 | 959 ± 32 | |
Irrigateda | Mex I10 | 7.0 ± 0.3 | 15,032 ± 1201 | 43.4 ± 4.5 | 1339 ± 33 | |
Nepal | Bhairahawa | Nepal B10 | 2.7 ± 0.5 | 8654 ± 1958 | 31.9 ± 4.4 | 1435 ± 45 |
Nepal B11 | 2.5 ± 0.5 | 7770 ± 1618 | 32.9 ± 4.3 | 1377 ± 49 | ||
Pakistan | Islamabad | Pak I10 | 3.2 ± 0.9 | 10,836 ± 3158 | 29.8 ± 3.1 | 1204 ± 74 |
Pak I11 | 6.9 ± 2.0 | 21,920 ± 6417 | 31.8 ± 3.0 | 1105 ± 38 | ||
Iran | Darab | Iran D10 | 5.3 ± 0.9 | 16,299 ± 2690 | 33.0 ± 3.3 | 1343 ± 22 |
Sudan | Wad Medani | Sudan W10 | 2.9 ± 0.4 | 8534 ± 1664 | 34.7 ± 3.9 | 1474 ± 99 |
Campo Experimental Norman E. Borlaug (CENEB), Mexico, different environments.
The WAMI panel was genotyped using 90K Illumina SNPs array (Sukumaran et al. 2015a). From the polymorphic SNPs after using a minor allele frequency cut-off of 5%, 15K SNPs were used for genomic prediction. The population structure associated with the 1B.1R translocation was described in earlier publications (Lopes et al. 2015; Sukumaran et al. 2015a).
Statistical models
The Best Linear Unbiased Estimators (BLUEs) were computed for mixed model analysis for each of the traits in each environment. The model used to calculate BLUEs for each environment is
where is the phenotypic response value for the specific trait measured on the jth line of the mth incomplete block within the kth replicate, is a fixed effect of the jth wheat line, is the random effect of the kth replicate assumed independent and identically multivariate normally distributed (iid) N(0, ) (where I is the identity matrix, and is the variance of replicate), denotes the random effect of the mth incomplete block within the kth replicate assumed independent and identically distributed (iid) with N(0, ), where is the variance of the incomplete block, is the random error associated to the trait measured on the jth line of the mth incomplete block within the kth replicate, and assumed iid with N(0, ), where denotes the error variance.
Broad-sense heritability (H2) for each environment was computed on an entry mean basis as where is the wheat line variance, r is the number of replicates, and is the error variance. Heritability estimates across environments were also estimated using the following formula,
where s is the number of environments, and is the variance of the wheat line × environment obtained from the combined analyses across environments.
For GS, we used the reaction norm model that is an extension of the random effect Genomic Best Linear Unbiased Predictor (GBLUP) model, where the main effect of lines, the main effect of environments, the main effect of markers, the main effect of pedigree, and their interactions with environments, are modeled using random covariance structures that are functions of marker or pedigree genotypes and environmental covariates (Jarquín et al. 2014). Brief descriptions of the baseline model, as well as the reaction norm models with G×E, are given below.
Baseline model
The response of the phenotypes () defined by random baseline model is
where is the overall mean, is the random effect of the ith environment, is the random effect of the jth line, is the interaction between the ith environment and the jth line, and is the random error term. All random effects follow a iid multivariate normal distribution such that and where and are the environment, line, and line × environment variances, respectively.
In the model above, the random effect of the line () can be replaced by which is an approximation of the genetic value of the jth line from the genomic relationship matrix. Also, the effects of the line () can be replaced by which is the additive effect obtained from the pedigree information. In the models described below, we used either or both and , as well as their interactions with environment Full descriptions of the different reaction norm models can be found in Jarquín et al. (2014) and Zhang et al. (2014), among others. Below, we give a brief description of the different reaction norm models that were fitted using pedigree and genomic information.
Reaction norm models
We fitted seven different models (M1–M7) with different components including E = environments, L = line, A = pedigree, G = genomic, AE = pedigree × environment interaction, GE = genomic × environment interaction, and e = residual error.
M1: Environment and line main effects (Y = E + L + e)
The response of the phenotypes () from the baseline model, but excluding the interaction term, is described as
(1) |
M2: Environment, line, and pedigree main effects (Y = E + L + A + e)
By adding the random effect that incorporates pedigree information by means of the numerical relationship matrix (A) to M1, we get model M2, defined as
(2) |
where is a random additive effect of the line, which, in this case accounts for pedigree-relationships, where contains the pedigree values of all the lines, and is assumed to follow a multivariate normal density with zero mean and covariance matrix where A is the numerical relationship matrix, and is the additive genetic variance. The random effects are correlated such that model M2 allows borrowing of information across lines based on the numerical relationship matrix (A) computed from the pedigree information.
M3: Environment, line, and genomic main effects (Y = E + L + G + e)
Model M3 is fitted by adding the genomic random effect of the line to M1, which is an approximation of the genetic value of the jth line, and is defined by the regression on marker covariates where is the genotype of the jth line at the lth marker, and is the effect of the lth marker assuming iid (l=1,…,p), and is the variance of the marker effects. The vector contains the genomic values of all the lines, and is assumed to follow a multivariate normal density with zero mean and covariance matrix where G is the genomic relationship matrix computed as suggested by VanRaden (2008) (i.e., with as the centered and standardized matrix of molecular markers and the frequency of the lth marker); and is the genomic variance. Thus, model M3 is
(3) |
with The random effects are correlated such that model M3 allows borrowing information across lines.
M4: Environment, line, pedigree, and pedigree × environment interaction effects (Y = E + L + A + AE + e)
By adding the interaction between the additive relationship matrix and environments () to model M2, model M4 becomes
(4) |
where the term is the interaction between the additive value of the ith genotype in the jth environment and Matrices and are the incidence matrices for the effects of the additive genetic values of genotypes and environments, respectively, is the variance component of the interaction term , and “” stands for Hadamart product between two matrices.
M5: Environments, lines, genomic, genomic × environment interaction effect (genomic × environment) (Y = E + L + G + GE + e)
By adding the interaction between markers and environments () to model M3, model M5 becomes
(5) |
where the term is the interaction between the genetic value of the ith genotype in the jth environment; then Matrices and are the incidence matrices for the effects of the genetic values of the genotypes and the environments, respectively, is the variance component of the interaction term
M6: Environment, line, pedigree, and genomic main effects (Y = E + L + A + G + e)
We added both the pedigree and genomic effects of the lines ( and ) to model M1, so that it contains the genomic random vector and the pedigree random vector Therefore, model M6 is
(6) |
M7: Environment, line, pedigree, genomic, pedigree × environment interaction and genomic × environment interaction effects (M7 = E + L + A + G + AE + GE + e)
By adding both the interaction between pedigree and environment (), and the interaction between markers (genomic) and environments () to model M6, model M7 becomes
(7) |
All the terms in this model have already been defined above.
Prediction assessment by cross-validation
Two distinct cross-validation (CV) schemes were used. The first, CV1, evaluates the prediction ability of models when a set of lines has not been evaluated in any of the environments (Burgueño et al. 2012). Predictions derived using CV1 are based entirely on phenotypic records of other lines. The second scheme, CV2, evaluates the prediction ability of models when some lines have been evaluated in some environments, but not in others. In CV2 prediction, information from related lines and the correlated environments is used, and prediction assessment benefits from borrowing information between lines within an environment, between lines across environments, and among correlated environments (Burgueño et al. 2012). Prediction ability is the Pearson correlation coefficient between the observed and predicted values for each genotype.
In both CV1 and CV2, a fivefold cross-validation scheme was used to generate the training (TRN) and testing (TST) sets, and to assess the prediction ability of each testing set. The data were divided randomly into five subsets, with 80% of the lines assigned to the training set and 20% assigned to the testing set. Four subsets were combined to form the training set, and the remaining subset was used as the validation set. Permutation of five subsets led to five possible training and validation data sets. This procedure was repeated 20 times, and a total of 100 runs was performed on each population for each trait-environment combination. The same partitions were analyzed with all models. The average value of the correlations between the phenotype and the genomic estimated breeding values from 100 runs was calculated in each population for each trait-environment combination, and was defined as the prediction ability.
Software
The genomic prediction analyses were computed using R, and the models were fitted using the BGLR package (de los Campos et al. 2013; de los Campos and Pérez-Rodríguez 2013). The ANOVA was performed in the SAS 9.2 (SAS Institute Inc 2010) program, and the boxplots created in R. Tukey’s test for significant differences between the models’ predictions (correlations) were generated in the SAS 9.2 (SAS Institute Inc 2010) program.
Data availability
All the phenotypic data for each environment and trait, as well as the genomic data, can be downloaded from the link http://hdl.handle.net/11529/10714.
Results
Variation in the studied traits
The WAMI panel was grown in seven countries, comprising a total of 18 environments (site-year combinations). India had the largest number of environments (6) followed by Mexico (4), and Bangladesh, Nepal, Pakistan, Iran, and Sudan with one site each. The ANOVA showed significant differences between the wheat lines and environments (Table A1, Appendix A). Environment Mex 110 was the highest yielding environment (7.02 ton/ha), followed by Pak I11 (6.9 ton/ha). The lowest yield was obtained in BGLD J10 (2.2 ton/ha) with a GW value of 30.9. The highest GW value was recorded in Mex I10 (43.4), followed by India L11 (38.3), and the lowest was India H10 (27.6). TTF ranged from 976°D in Mex H10 to 1474°D in Sudan W. The highest GN was recorded in Pak I11 (21920), followed by Iran D10 (Table 1). Heritability estimates of individual and combined environments for each trait were also calculated. Trait GW (0.74) had the highest H2 values, followed by GN (0.51), TTF (0.48), and GY (0.41) (Table A1, Appendix A). A box plot of the data at the individual locations indicated TTF had the highest variation and the lowest G × E was observed for GW (Figure 2 and Figure 3).
Prediction ability of different models for international sites
We used seven models (M1–M7) to predict the lines that were not observed under CV1 and CV2 scenarios. For GY, prediction ability values for individual sites ranged from −0.05 (M1) to 0.52 (M6) (Table 2). The highest value obtained for CV1 was in Mex D10 (0.52). The models’ average prediction abilities were −0.08, 0.11, 0.21, 0.22, 0.22, 0.29, and 0.31 for M1–M7, respectively. Models 6 and 7 had the highest significant prediction ability, followed by models 3, 4, and 5 (Figure 4). For CV2, the values ranged from 0.10 (Sudan W10) to 0.54 (India D10, India V10). On average, the CV2 correlation values for each model were 0.31, 0.31, 0.32, 0.32, 0.35, 0.37, and 0.38 for M1–M7, respectively (Table 2). Tukey’s test identified that M5–M7 had significantly higher prediction accuracies than the other models for CV2 (Figure 4).
Table 2. Correlations (mean ± SD) between the observed and predicted values for GY under CV1 and CV2 CV schemes for seven prediction models (M1–M7).
CV1 | CV2 | H2 | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Env\Model | M1a | M2 | M3 | M4 | M5 | M6 | M7 | M1 | M2 | M3 | M4 | M5 | M6 | M7 | |
BGLD J10b | −0.06 ± 0.05 | 0.04 ± 0.02 | 0.09 ± 0.02 | 0.09 ± 0.02 | 0.22 ± 0.03 | 0.16 ± 0.02 | 0.21 ± 0.03 | 0.21 ± 0.01 | 0.20 ± 0.01 | 0.20 ± 0.01 | 0.20 ± 0.01 | 0.26 ± 0.02 | 0.24 ± 0.02 | 0.26 ± 0.02 | 0.20 |
BGLD J11 | −0.08 ± 0.07 | 0.00 ± 0.03 | 0.05 ± 0.02 | 0.06 ± 0.02 | 0.22 ± 0.03 | 0.29 ± 0.02 | 0.30 ± 0.03 | 0.30 ± 0.01 | 0.30 ± 0.01 | 0.29 ± 0.01 | 0.29 ± 0.01 | 0.38 ± 0.01 | 0.42 ± 0.01 | 0.43 ± 0.01 | 0.67 |
India D10 | −0.09 ± 0.08 | 0.13 ± 0.05 | 0.21 ± 0.03 | 0.22 ± 0.03 | 0.24 ± 0.03 | 0.30 ± 0.03 | 0.30 ± 0.03 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.54 ± 0.01 | 0.54 ± 0.01 | 0.54 ± 0.01 | 0.55 |
India H10 | −0.06 ± 0.06 | −0.11 ± 0.04 | −0.05 ± 0.02 | 0.14 ± 0.03 | 0.20 ± 0.03 | −0.06 ± 0.03 | 0.21 ± 0.03 | 0.07 ± 0.02 | 0.07 ± 0.01 | 0.07 ± 0.01 | 0.16 ± 0.02 | 0.19 ± 0.02 | 0.07 ± 0.01 | 0.20 ± 0.02 | 0.13 |
India I11 | −0.10 ± 0.05 | 0.18 ± 0.06 | 0.32 ± 0.03 | 0.32 ± 0.03 | 0.23 ± 0.02 | 0.31 ± 0.02 | 0.30 ± 0.02 | 0.39 ± 0.02 | 0.40 ± 0.02 | 0.41 ± 0.02 | 0.41 ± 0.02 | 0.40 ± 0.02 | 0.42 ± 0.02 | 0.41 ± 0.02 | 0.44 |
India K10 | −0.08 ± 0.05 | 0.05 ± 0.03 | 0.16 ± 0.04 | 0.15 ± 0.03 | 0.18 ± 0.03 | 0.28 ± 0.02 | 0.26 ± 0.02 | 0.15 ± 0.02 | 0.16 ± 0.02 | 0.17 ± 0.02 | 0.17 ± 0.02 | 0.23 ± 0.02 | 0.31 ± 0.02 | 0.29 ± 0.02 | 0.28 |
India L11 | −0.10 ± 0.05 | 0.04 ± 0.04 | 0.20 ± 0.03 | 0.19 ± 0.03 | 0.19 ± 0.04 | 0.26 ± 0.03 | 0.29 ± 0.03 | 0.36 ± 0.02 | 0.36 ± 0.02 | 0.37 ± 0.02 | 0.36 ± 0.02 | 0.41 ± 0.01 | 0.41 ± 0.02 | 0.43 ± 0.02 | 0.79 |
India V10 | −0.09 ± 0.05 | 0.14 ± 0.05 | 0.21 ± 0.03 | 0.22 ± 0.03 | 0.24 ± 0.03 | 0.29 ± 0.04 | 0.29 ± 0.03 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.52 ± 0.01 | 0.54 ± 0.01 | 0.53 ± 0.01 | 0.53 ± 0.02 | 0.55 |
Iran D10 | −0.10 ± 0.06 | 0.06 ± 0.08 | 0.03 ± 0.01 | 0.04 ± 0.04 | 0.18 ± 0.04 | 0.24 ± 0.01 | 0.26 ± 0.03 | 0.11 ± 0.02 | 0.12 ± 0.02 | 0.11 ± 0.02 | 0.12 ± 0.02 | 0.19 ± 0.02 | 0.26 ± 0.02 | 0.27 ± 0.02 | 0.97 |
Mex D10 | −0.05 ± 0.07 | 0.29 ± 0.03 | 0.48 ± 0.02 | 0.48 ± 0.02 | 0.39 ± 0.02 | 0.52 ± 0.02 | 0.51 ± 0.02 | 0.43 ± 0.01 | 0.44 ± 0.01 | 0.46 ± 0.01 | 0.46 ± 0.01 | 0.50 ± 0.01 | 0.54 ± 0.01 | 0.53 ± 0.01 | 0.68 |
Mex H10 | −0.06 ± 0.06 | 0.18 ± 0.05 | 0.36 ± 0.02 | 0.35 ± 0.02 | 0.21 ± 0.05 | 0.41 ± 0.03 | 0.41 ± 0.03 | 0.44 ± 0.01 | 0.44 ± 0.01 | 0.45 ± 0.01 | 0.45 ± 0.01 | 0.44 ± 0.01 | 0.48 ± 0.01 | 0.48 ± 0.02 | 0.76 |
Mex HD10 | −0.07 ± 0.08 | 0.16 ± 0.04 | 0.30 ± 0.02 | 0.30 ± 0.02 | 0.21 ± 0.04 | 0.34 ± 0.03 | 0.35 ± 0.03 | 0.39 ± 0.02 | 0.40 ± 0.02 | 0.41 ± 0.02 | 0.41 ± 0.02 | 0.41 ± 0.02 | 0.43 ± 0.02 | 0.43 ± 0.02 | 0.60 |
Mex I10 | −0.08 ± 0.05 | 0.24 ± 0.03 | 0.34 ± 0.03 | 0.35 ± 0.03 | 0.29 ± 0.02 | 0.43 ± 0.03 | 0.43 ± 0.03 | 0.35 ± 0.01 | 0.36 ± 0.01 | 0.37 ± 0.01 | 0.37 ± 0.01 | 0.39 ± 0.01 | 0.43 ± 0.01 | 0.43 ± 0.01 | 0.74 |
Nepal B10 | −0.08 ± 0.04 | 0.20 ± 0.03 | 0.28 ± 0.02 | 0.29 ± 0.02 | 0.17 ± 0.03 | 0.26 ± 0.02 | 0.28 ± 0.02 | 0.33 ± 0.02 | 0.34 ± 0.02 | 0.34 ± 0.02 | 0.35 ± 0.02 | 0.33 ± 0.02 | 0.35 ± 0.02 | 0.36 ± 0.02 | 0.41 |
Nepal B11 | −0.08 ± 0.06 | 0.15 ± 0.03 | 0.24 ± 0.02 | 0.25 ± 0.02 | 0.31 ± 0.02 | 0.33 ± 0.03 | 0.36 ± 0.03 | 0.44 ± 0.01 | 0.44 ± 0.01 | 0.44 ± 0.01 | 0.45 ± 0.01 | 0.49 ± 0.01 | 0.50 ± 0.01 | 0.51 ± 0.01 | 0.55 |
Pak I10 | −0.09 ± 0.06 | 0.08 ± 0.04 | 0.21 ± 0.03 | 0.20 ± 0.03 | 0.10 ± 0.03 | 0.23 ± 0.02 | 0.20 ± 0.03 | 0.26 ± 0.02 | 0.27 ± 0.02 | 0.27 ± 0.02 | 0.27 ± 0.01 | 0.26 ± 0.02 | 0.30 ± 0.02 | 0.28 ± 0.02 | 0.33 |
Pak I11 | −0.10 ± 0.06 | 0.02 ± 0.08 | 0.12 ± 0.06 | 0.13 ± 0.06 | 0.10 ± 0.04 | 0.17 ± 0.04 | 0.16 ± 0.03 | 0.16 ± 0.03 | 0.17 ± 0.03 | 0.18 ± 0.03 | 0.18 ± 0.03 | 0.16 ± 0.02 | 0.20 ± 0.03 | 0.19 ± 0.03 | 0.26 |
Sudan W10 | −0.07 ± 0.06 | 0.13 ± 0.03 | 0.15 ± 0.02 | 0.16 ± 0.02 | 0.31 ± 0.03 | 0.38 ± 0.02 | 0.38 ± 0.02 | 0.10 ± 0.02 | 0.11 ± 0.02 | 0.11 ± 0.02 | 0.12 ± 0.02 | 0.21 ± 0.02 | 0.27 ± 0.02 | 0.27 ± 0.02 | 0.30 |
Average | −0.08 | 0.11 | 0.21 | 0.22 | 0.22 | 0.29 | 0.31 | 0.31 | 0.31 | 0.32 | 0.32 | 0.35 | 0.37 | 0.38 |
Broad-sense heritability H2 of GY in each environment.
Models: M1 Y = E+L+e; M2 Y= E+L+A+e; M3 Y= E+L+G+e; M4 Y= E+L+A+AE+e; M5 Y= E+L+G+GE+e; M6 Y= E+L+G+A+e; M7 Y= E+L+G+A+GE+AE+e.
Names of the environments are given in Table 1.
For CV1, 28 environment-model combinations had prediction ability values above 0.30 for GY. Among the sites, when using M7, Mexican environments (Mex I10, Mex D10, and Mex H10) had high prediction ability values (>0.41) for CV1 using M6 and M7. CV2 values were above 0.40 for 52 site-model combinations. For India V10 and India D10, prediction ability was above 0.5 for all models. In the CV1 scenario, 14 sites had the highest values when M6 and M7 were used (Table 2).
Trait GN mostly followed a similar pattern as that shown for GY but the CV1 values ranged from −0.05 (BGLD J10) to 0.56 (Mex I10). Forty-three environment-model combinations had CV1 values >0.30. Models 6 and 7 had five sites with CV1 values >0.4. Two sites (Sudan W10 and Mex I10) had CV1 values > 0.4 for six models. Models 6 and 7 had CV1 values > 0.50 for four environments (Mex H10, Mex HD10, Sudan W10, and Mex I10). On average, the highest CV1 values were recorded for M5 (0.32) and M7 (0.32) (Table 3). Tukey’s test also grouped M5 and M7 with the highest prediction ability models for CV1 and CV2 scenarios (Figure 5).
Table 3. Correlations (mean ± SD) between the observed and predicted values for GN under CV1 and CV2 schemes for seven prediction models (M1–M7).
CV1 | CV2 | H2 | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Env\Model | M1a | M2 | M3 | M4 | M5 | M6 | M7 | M1 | M2 | M3 | M4 | M5 | M6 | M7 | |
BGLD J10b | −0.05 ± 0.05 | 0.07 ± 0.01 | 0.13 ± 0.01 | 0.01 ± 0.03 | 0.09 ± 0.04 | 0.13 ± 0.02 | 0.10 ± 0.04 | 0.26 ± 0.01 | 0.26 ± 0.01 | 0.26 ± 0.01 | 0.26 ± 0.02 | 0.25 ± 0.01 | 0.26 ± 0.01 | 0.25 ± 0.01 | 0.26 |
BGLD J11 | −0.07 ± 0.06 | 0.15 ± 0.01 | 0.22 ± 0.01 | 0.12 ± 0.02 | 0.21 ± 0.02 | 0.22 ± 0.01 | 0.20 ± 0.03 | 0.43 ± 0.01 | 0.42 ± 0.01 | 0.42 ± 0.01 | 0.42 ± 0.01 | 0.43 ± 0.01 | 0.42 ± 0.01 | 0.42 ± 0.01 | 0.68 |
India D10 | −0.08 ± 0.06 | 0.23 ± 0.03 | 0.31 ± 0.01 | 0.25 ± 0.03 | 0.32 ± 0.03 | 0.31 ± 0.01 | 0.33 ± 0.03 | 0.42 ± 0.01 | 0.43 ± 0.01 | 0.43 ± 0.01 | 0.44 ± 0.01 | 0.43 ± 0.01 | 0.43 ± 0.01 | 0.44 ± 0.01 | 0.50 |
India H10 | −0.06 ± 0.07 | 0.22 ± 0.02 | 0.30 ± 0.02 | 0.30 ± 0.02 | 0.37 ± 0.02 | 0.29 ± 0.02 | 0.38 ± 0.03 | 0.35 ± 0.01 | 0.36 ± 0.01 | 0.37 ± 0.01 | 0.42 ± 0.01 | 0.43 ± 0.01 | 0.37 ± 0.01 | 0.44 ± 0.01 | 0.40 |
India I11 | −0.08 ± 0.07 | −0.08 ± 0.02 | −0.05 ± 0.02 | 0.17 ± 0.04 | 0.21 ± 0.03 | −0.05 ± 0.02 | 0.20 ± 0.03 | 0.04 ± 0.02 | 0.04 ± 0.02 | 0.04 ± 0.02 | 0.17 ± 0.03 | 0.21 ± 0.02 | 0.04 ± 0.02 | 0.22 ± 0.03 | 0.40 |
India K10 | −0.08 ± 0.06 | 0.15 ± 0.03 | 0.23 ± 0.02 | 0.14 ± 0.03 | 0.21 ± 0.03 | 0.22 ± 0.02 | 0.20 ± 0.03 | 0.39 ± 0.02 | 0.39 ± 0.02 | 0.39 ± 0.02 | 0.37 ± 0.02 | 0.37 ± 0.02 | 0.39 ± 0.02 | 0.36 ± 0.03 | 0.28 |
India L11 | −0.09 ± 0.05 | −0.14 ± 0.01 | −0.02 ± 0.01 | 0.10 ± 0.04 | 0.21 ± 0.03 | −0.04 ± 0.01 | 0.23 ± 0.03 | 0.06 ± 0.01 | 0.04 ± 0.01 | 0.05 ± 0.01 | 0.14 ± 0.02 | 0.17 ± 0.02 | 0.05 ± 0.01 | 0.19 ± 0.02 | 0.72 |
India V10 | −0.06 ± 0.05 | 0.20 ± 0.02 | 0.27 ± 0.02 | 0.24 ± 0.02 | 0.32 ± 0.02 | 0.27 ± 0.02 | 0.32 ± 0.02 | 0.37 ± 0.01 | 0.38 ± 0.01 | 0.38 ± 0.01 | 0.39 ± 0.01 | 0.41 ± 0.02 | 0.38 ± 0.01 | 0.41 ± 0.01 | 0.48 |
Iran D10 | −0.10 ± 0.06 | 0.21 ± 0.04 | 0.29 ± 0.02 | 0.25 ± 0.03 | 0.30 ± 0.03 | 0.29 ± 0.02 | 0.31 ± 0.03 | 0.40 ± 0.01 | 0.40 ± 0.01 | 0.41 ± 0.01 | 0.42 ± 0.01 | 0.41 ± 0.02 | 0.41 ± 0.01 | 0.41 ± 0.02 | 0 |
Mex D10 | −0.02 ± 0.06 | 0.30 ± 0.02 | 0.40 ± 0.01 | 0.32 ± 0.02 | 0.42 ± 0.01 | 0.40 ± 0.01 | 0.43 ± 0.01 | 0.60 ± 0.01 | 0.61 ± 0.01 | 0.61 ± 0.01 | 0.61 ± 0.01 | 0.62 ± 0.01 | 0.61 ± 0.01 | 0.63 ± 0.01 | 0.74 |
Mex H10 | −0.06 ± 0.04 | 0.36 ± 0.02 | 0.51 ± 0.01 | 0.37 ± 0.01 | 0.52 ± 0.01 | 0.50 ± 0.01 | 0.51 ± 0.01 | 0.66 ± 0.01 | 0.67 ± 0.01 | 0.68 ± 0.01 | 0.67 ± 0.01 | 0.69 ± 0.01 | 0.68 ± 0.01 | 0.69 ± 0.01 | 0.84 |
Mex HD10 | −0.07 ± 0.06 | 0.38 ± 0.02 | 0.51 ± 0.01 | 0.42 ± 0.01 | 0.53 ± 0.01 | 0.50 ± 0.01 | 0.53 ± 0.01 | 0.65 ± 0.01 | 0.66 ± 0.01 | 0.67 ± 0.01 | 0.68 ± 0.01 | 0.69 ± 0.01 | 0.67 ± 0.01 | 0.69 ± 0.01 | 0.74 |
Mex I10 | −0.05 ± 0.05 | 0.41 ± 0.02 | 0.53 ± 0.01 | 0.43 ± 0.02 | 0.56 ± 0.01 | 0.53 ± 0.01 | 0.56 ± 0.01 | 0.64 ± 0.01 | 0.65 ± 0.01 | 0.66 ± 0.01 | 0.66 ± 0.01 | 0.69 ± 0.01 | 0.66 ± 0.01 | 0.68 ± 0.01 | 0.83 |
Nepal B10 | −0.07 ± 0.05 | 0.31 ± 0.02 | 0.32 ± 0.01 | 0.29 ± 0.01 | 0.32 ± 0.02 | 0.34 ± 0.01 | 0.34 ± 0.01 | 0.46 ± 0.01 | 0.47 ± 0.01 | 0.47 ± 0.01 | 0.46 ± 0.01 | 0.47 ± 0.02 | 0.47 ± 0.01 | 0.47 ± 0.01 | 0.48 |
Nepal B11 | −0.06 ± 0.06 | 0.14 ± 0.01 | 0.08 ± 0.01 | 0.27 ± 0.02 | 0.20 ± 0.03 | 0.11 ± 0.02 | 0.24 ± 0.03 | 0.44 ± 0.01 | 0.43 ± 0.01 | 0.41 ± 0.01 | 0.49 ± 0.01 | 0.50 ± 0.01 | 0.42 ± 0.01 | 0.51 ± 0.01 | 0.50 |
Pak I10 | −0.08 ± 0.07 | 0.09 ± 0.02 | 0.15 ± 0.02 | 0.10 ± 0.03 | 0.20 ± 0.02 | 0.14 ± 0.02 | 0.18 ± 0.02 | 0.28 ± 0.01 | 0.28 ± 0.01 | 0.28 ± 0.01 | 0.28 ± 0.02 | 0.31 ± 0.02 | 0.28 ± 0.01 | 0.29 ± 0.02 | 0.36 |
Pak I11 | −0.10 ± 0.06 | 0.02 ± 0.05 | 0.06 ± 0.04 | 0.08 ± 0.04 | 0.12 ± 0.04 | 0.06 ± 0.04 | 0.11 ± 0.04 | 0.08 ± 0.02 | 0.08 ± 0.02 | 0.09 ± 0.02 | 0.11 ± 0.03 | 0.13 ± 0.02 | 0.08 ± 0.02 | 0.12 ± 0.02 | 0.25 |
Sudan W10 | −0.07 ± 0.07 | 0.45 ± 0.02 | 0.53 ± 0.01 | 0.45 ± 0.02 | 0.56 ± 0.01 | 0.53 ± 0.01 | 0.55 ± 0.01 | 0.51 ± 0.01 | 0.53 ± 0.01 | 0.54 ± 0.01 | 0.56 ± 0.01 | 0.60 ± 0.01 | 0.54 ± 0.01 | 0.60 ± 0.01 | 0.59 |
Average | −0.07 | 0.19 | 0.27 | 0.24 | 0.32 | 0.26 | 0.32 | 0.39 | 0.39 | 0.40 | 0.42 | 0.43 | 0.40 | 0.43 |
Broad-sense heritability H2 of GN in each environment.
Models: M1 Y = E+L+e; M2 Y= E+L+A+e; M3 Y= E+L+G+e; M4 Y= E+L+A+AE+e; M5 Y= E+L+G+GE+e; M6 Y= E+L+G+A+e; M7 Y= E+L+G+A+GE+AE+e.
Names of the environments are given in Table 1.
For CV2, 36 environment-model combinations had GN values >0.5. The values ranged from 0.08 (Iran D10) to 0.69 (Mex HD10). Five environments (Mex D10, Mex H10, Mex HD10, Sudan W10, and Mex I10) had values >0.5 for all models. On average, the increase in CV2 values from M1 to M7 was 0.04, with M5 and M7 recording the highest average increases (0.43) (Table 3).
Trait GW had the highest prediction values in CV1 (0.72, Iran D10) and CV2 (0.88, Iran D10) scenarios. Models 6 and 7 had eight environments with prediction values in CV1 >0.5. Thirty-six environment-model combinations had prediction values for CV1 >0.50, with M6 and M7 predicting the values for CV1 of five sites with correlation >0.6. On average, the model with the highest CV1 values was M3, followed by M7. Mex I10 and Mex D10 had the highest CV1 (0.72 for both M6 and M7) and CV2 values (0.88 for M6 and M7) (Table 4). Tukey’s test group showed models M3 and M7 as the most significant models with the highest prediction ability in the CV1 scenario (Figure 6). In the CV2 scenario, all models had the same prediction ability (0.63) (Figure 6 and Table 4).
Table 4. Correlations (mean ± SD) between the observed and predicted values for GW under CV1 and CV2 schemes for seven prediction models (M1–M7).
CV1 | CV2 | H2 | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Env\Model | M1a | M2 | M3 | M4 | M5 | M6 | M7 | M1 | M2 | M3 | M4 | M5 | M6 | M7 | |
BGLD J10b | −0.06 ± 0.05 | 0.28 ± 0.02 | 0.39 ± 0.01 | 0.35 ± 0.02 | 0.45 ± 0.02 | 0.41 ± 0.02 | 0.46 ± 0.02 | 0.65 ± 0.01 | 0.65 ± 0.01 | 0.65 ± 0.01 | 0.69 ± 0.01 | 0.68 ± 0.01 | 0.65 ± 0.01 | 0.68 ± 0.01 | 0.69 |
BGLD J11 | −0.06 ± 0.07 | 0.34 ± 0.01 | 0.60 ± 0.01 | 0.36 ± 0.01 | 0.43 ± 0.02 | 0.39 ± 0.01 | 0.45 ± 0.02 | 0.61 ± 0.01 | 0.61 ± 0.01 | 0.61 ± 0.01 | 0.63 ± 0.01 | 0.64 ± 0.01 | 0.61 ± 0.01 | 0.64 ± 0.01 | 0.84 |
India D10 | −0.04 ± 0.07 | 0.06 ± 0.01 | 0.09 ± 0.01 | 0.02 ± 0.04 | 0.03 ± 0.04 | 0.09 ± 0.01 | 0.03 ± 0.04 | 0.20 ± 0.01 | 0.20 ± 0.01 | 0.19 ± 0.01 | 0.20 ± 0.01 | 0.18 ± 0.01 | 0.19 ± 0.01 | 0.18 ± 0.01 | 0 |
India H10 | −0.06 ± 0.07 | 0.28 ± 0.02 | 0.45 ± 0.01 | 0.27 ± 0.02 | 0.29 ± 0.02 | 0.34 ± 0.01 | 0.29 ± 0.02 | 0.47 ± 0.01 | 0.47 ± 0.01 | 0.47 ± 0.01 | 0.46 ± 0.01 | 0.44 ± 0.02 | 0.47 ± 0.01 | 0.44 ± 0.02 | 0.69 |
India I11 | −0.05 ± 0.06 | 0.40 ± 0.02 | 0.59 ± 0.01 | 0.41 ± 0.02 | 0.51 ± 0.02 | 0.51 ± 0.01 | 0.51 ± 0.02 | 0.78 ± 0.00 | 0.78 ± 0.00 | 0.78 ± 0.00 | 0.77 ± 0.01 | 0.77 ± 0.01 | 0.78 ± 0.00 | 0.77 ± 0.01 | 0.79 |
India K10 | −0.06 ± 0.07 | 0.47 ± 0.02 | 0.51 ± 0.01 | 0.49 ± 0.01 | 0.59 ± 0.01 | 0.59 ± 0.01 | 0.59 ± 0.01 | 0.80 ± 0.00 | 0.80 ± 0.00 | 0.80 ± 0.00 | 0.79 ± 0.00 | 0.80 ± 0.00 | 0.80 ± 0.00 | 0.80 ± 0.00 | 0.77 |
India L11 | −0.04 ± 0.06 | 0.21 ± 0.02 | 0.09 ± 0.01 | 0.23 ± 0.03 | 0.18 ± 0.03 | 0.19 ± 0.01 | 0.20 ± 0.03 | 0.22 ± 0.01 | 0.22 ± 0.01 | 0.22 ± 0.01 | 0.21 ± 0.01 | 0.21 ± 0.01 | 0.22 ± 0.01 | 0.21 ± 0.01 | 0.51 |
India V10 | −0.04 ± 0.07 | 0.06 ± 0.01 | 0.14 ± 0.01 | 0.04 ± 0.04 | 0.04 ± 0.04 | 0.09 ± 0.01 | 0.05 ± 0.03 | 0.20 ± 0.01 | 0.19 ± 0.01 | 0.19 ± 0.01 | 0.20 ± 0.01 | 0.19 ± 0.01 | 0.19 ± 0.01 | 0.20 ± 0.01 | 0 |
Iran D10 | −0.06 ± 0.07 | 0.55 ± 0.02 | 0.64 ± 0.01 | 0.61 ± 0.01 | 0.72 ± 0.01 | 0.68 ± 0.01 | 0.72 ± 0.01 | 0.84 ± 0.01 | 0.85 ± 0.01 | 0.85 ± 0.01 | 0.87 ± 0.00 | 0.88 ± 0.00 | 0.85 ± 0.01 | 0.88 ± 0.00 | 0.05 |
Mex D10 | −0.04 ± 0.07 | 0.49 ± 0.01 | 0.59 ± 0.01 | 0.50 ± 0.02 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.88 ± 0.00 | 0.88 ± 0.00 | 0.88 ± 0.00 | 0.88 ± 0.00 | 0.88 ± 0.00 | 0.88 ± 0.00 | 0.88 ± 0.01 | 0.22 |
Mex H10 | −0.06 ± 0.07 | 0.45 ± 0.02 | 0.66 ± 0.01 | 0.47 ± 0.02 | 0.61 ± 0.01 | 0.59 ± 0.01 | 0.61 ± 0.02 | 0.81 ± 0.01 | 0.81 ± 0.01 | 0.81 ± 0.00 | 0.81 ± 0.01 | 0.82 ± 0.01 | 0.81 ± 0.00 | 0.82 ± 0.01 | 0.92 |
Mex HD10 | −0.08 ± 0.06 | 0.53 ± 0.02 | 0.61 ± 0.01 | 0.57 ± 0.01 | 0.68 ± 0.01 | 0.66 ± 0.01 | 0.68 ± 0.01 | 0.87 ± 0.00 | 0.87 ± 0.00 | 0.87 ± 0.00 | 0.87 ± 0.00 | 0.88 ± 0.00 | 0.87 ± 0.00 | 0.88 ± 0.00 | 0.9 |
Mex I10 | −0.05 ± 0.06 | 0.43 ± 0.02 | 0.48 ± 0.01 | 0.45 ± 0.01 | 0.64 ± 0.01 | 0.61 ± 0.01 | 0.64 ± 0.01 | 0.81 ± 0.01 | 0.81 ± 0.01 | 0.81 ± 0.01 | 0.80 ± 0.01 | 0.82 ± 0.01 | 0.81 ± 0.01 | 0.82 ± 0.01 | 0.92 |
Nepal B10 | −0.05 ± 0.08 | 0.36 ± 0.02 | 0.45 ± 0.01 | 0.36 ± 0.01 | 0.48 ± 0.02 | 0.48 ± 0.01 | 0.49 ± 0.02 | 0.78 ± 0.01 | 0.78 ± 0.01 | 0.78 ± 0.01 | 0.77 ± 0.01 | 0.76 ± 0.01 | 0.78 ± 0.01 | 0.76 ± 0.01 | 0.95 |
Nepal B11 | −0.06 ± 0.07 | 0.40 ± 0.01 | 0.29 ± 0.01 | 0.42 ± 0.01 | 0.46 ± 0.02 | 0.46 ± 0.01 | 0.47 ± 0.02 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.65 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.78 |
Pak I11 | −0.03 ± 0.04 | 0.18 ± 0.02 | 0.35 ± 0.01 | 0.15 ± 0.03 | 0.29 ± 0.03 | 0.29 ± 0.01 | 0.28 ± 0.03 | 0.30 ± 0.00 | 0.30 ± 0.00 | 0.30 ± 0.00 | 0.27 ± 0.01 | 0.28 ± 0.02 | 0.30 ± 0.00 | 0.28 ± 0.02 | 0.77 |
PakI10 | −0.06 ± 0.07 | 0.40 ± 0.02 | 0.85 ± 0.00 | 0.43 ± 0.01 | 0.54 ± 0.01 | 0.52 ± 0.01 | 0.54 ± 0.01 | 0.72 ± 0.01 | 0.72 ± 0.01 | 0.72 ± 0.01 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.72 ± 0.01 | 0.74 ± 0.01 | 0.70 |
Sudan W10 | −0.06 ± 0.05 | 0.28 ± 0.02 | 0.39 ± 0.01 | 0.35 ± 0.02 | 0.45 ± 0.02 | 0.41 ± 0.02 | 0.46 ± 0.02 | 0.65 ± 0.01 | 0.65 ± 0.01 | 0.65 ± 0.01 | 0.69 ± 0.01 | 0.68 ± 0.01 | 0.65 ± 0.01 | 0.68 ± 0.01 | 0.23 |
Average | −0.05 | 0.34 | 0.45 | 0.36 | 0.45 | 0.44 | 0.45 | 0.62 | 0.62 | 0.62 | 0.63 | 0.63 | 0.62 | 0.63 |
Broad-sense heritability H2 of GW in each environment.
Models: M1 Y = E+L+e; M2 Y= E+L+A+e; M3 Y= E+L+G+e; M4 Y= E+L+A+AE+e; M5 Y= E+L+G+GE+e; M6 Y= E+L+G+A+e; M7 Y= E+L+G+A+GE+AE+e.
Names of the environments are given in Table 1.
For TTF, the prediction ability in the CV1 scenario ranged from −0.11 (India L11, M1) to 0.44 (India K11, M5). A total of 29 model-site combinations had CV1 values >0.3, with M7 predicting eight sites with correlations >0.3. Mex I10 had five models predicting the sites with >0.3 for CV1, followed by Nepal. On average, M5 had the highest CV1 values (0.28) when compared with other models (Table 5). For CV2, values ranged from 0.40 (Mex H10) to 0.80 (BGLDJ10). All sites had correlation values >0.3, and 85 environment-model combinations had correlation values >0.50. Thirty-five sites (31%) had CV2 values >0.7 (Table 5). On average, correlations for M5–M7 for CV1 were 0.28, 0.24, and 0.27, respectively, and prediction ability values for M5–M7 for CV2 were 0.54, 0.52, and 0.53, respectively. Tukey’s test groups indicated that M5–M7 were the best predictive models for CV1, while for CV2 all models had the same prediction ability (Figure 7).
Table 5. Correlations (mean ± SD) between the observed and predicted values for TTF under CV1 and CV2 schemes for seven prediction models (M1–M7).
CV1 | CV2 | H2 | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Env\Models | M1a | M2 | M3 | M4 | M5 | M6 | M7 | M1 | M2 | M3 | M4 | M5 | M6 | M7 | |
BGLD J10b | −0.03 ± 0.06 | 0.05 ± 0.02 | 0.15 ± 0.02 | 0.07 ± 0.05 | 0.27 ± 0.02 | 0.14 ± 0.02 | 0.21 ± 0.04 | 0.80 ± 0.01 | 0.80 ± 0.01 | 0.80 ± 0.01 | 0.78 ± 0.01 | 0.80 ± 0.01 | 0.80 ± 0.01 | 0.79 ± 0.01 | 0.97 |
BGLD J11 | −0.05 ± 0.08 | 0.26 ± 0.04 | 0.33 ± 0.02 | 0.33 ± 0.01 | 0.41 ± 0.02 | 0.35 ± 0.02 | 0.41 ± 0.02 | 0.72 ± 0.01 | 0.72 ± 0.01 | 0.72 ± 0.01 | 0.68 ± 0.01 | 0.67 ± 0.01 | 0.72 ± 0.01 | 0.67 ± 0.01 | 0.84 |
India D10 | −0.05 ± 0.05 | 0.09 ± 0.02 | 0.16 ± 0.02 | −0.03 ± 0.04 | 0.10 ± 0.04 | 0.16 ± 0.01 | 0.07 ± 0.04 | 0.48 ± 0.01 | 0.48 ± 0.01 | 0.48 ± 0.01 | 0.51 ± 0.01 | 0.55 ± 0.01 | 0.48 ± 0.01 | 0.53 ± 0.01 | 0.53 |
India H10 | −0.07 ± 0.06 | 0.09 ± 0.03 | 0.15 ± 0.02 | 0.31 ± 0.02 | 0.36 ± 0.02 | 0.16 ± 0.02 | 0.36 ± 0.02 | 0.60 ± 0.01 | 0.60 ± 0.01 | 0.60 ± 0.01 | 0.61 ± 0.01 | 0.61 ± 0.02 | 0.61 ± 0.01 | 0.62 ± 0.02 | 0.98 |
India I11 | −0.07 ± 0.06 | 0.24 ± 0.04 | 0.27 ± 0.03 | 0.31 ± 0.02 | 0.35 ± 0.02 | 0.30 ± 0.02 | 0.37 ± 0.02 | 0.45 ± 0.01 | 0.45 ± 0.01 | 0.45 ± 0.01 | 0.49 ± 0.01 | 0.47 ± 0.01 | 0.45 ± 0.01 | 0.48 ± 0.01 | 0.79 |
India K11 | −0.06 ± 0.06 | 0.24 ± 0.04 | 0.39 ± 0.02 | 0.25 ± 0.02 | 0.44 ± 0.02 | 0.39 ± 0.02 | 0.42 ± 0.02 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.62 ± 0.01 | 0.64 ± 0.01 | 0.64 ± 0.01 | 0.63 ± 0.01 | 0.84 |
India L11 | −0.11 ± 0.06 | 0.22 ± 0.08 | 0.21 ± 0.05 | 0.41 ± 0.02 | 0.39 ± 0.03 | 0.24 ± 0.05 | 0.43 ± 0.02 | 0.40 ± 0.01 | 0.40 ± 0.01 | 0.39 ± 0.01 | 0.39 ± 0.01 | 0.39 ± 0.02 | 0.40 ± 0.01 | 0.39 ± 0.02 | 0.98 |
India V10 | −0.05 ± 0.07 | 0.15 ± 0.02 | 0.26 ± 0.02 | 0.15 ± 0.03 | 0.29 ± 0.02 | 0.26 ± 0.02 | 0.28 ± 0.03 | 0.57 ± 0.01 | 0.57 ± 0.01 | 0.57 ± 0.01 | 0.60 ± 0.01 | 0.62 ± 0.01 | 0.57 ± 0.01 | 0.61 ± 0.01 | 0.70 |
Iran D10 | −0.04 ± 0.05 | −0.01 ± 0.03 | 0.11 ± 0.02 | −0.02 ± 0.04 | 0.05 ± 0.04 | 0.08 ± 0.02 | 0.07 ± 0.04 | 0.19 ± 0.01 | 0.19 ± 0.01 | 0.18 ± 0.01 | 0.26 ± 0.01 | 0.30 ± 0.01 | 0.18 ± 0.01 | 0.31 ± 0.01 | 0.21 |
Mex D10 | −0.03 ± 0.06 | 0.08 ± 0.03 | 0.18 ± 0.02 | 0.08 ± 0.04 | 0.29 ± 0.03 | 0.18 ± 0.02 | 0.23 ± 0.05 | 0.69 ± 0.01 | 0.69 ± 0.01 | 0.69 ± 0.01 | 0.72 ± 0.01 | 0.75 ± 0.01 | 0.69 ± 0.01 | 0.74 ± 0.01 | 0.92 |
Mex H10 | −0.06 ± 0.06 | 0.24 ± 0.03 | 0.25 ± 0.02 | 0.19 ± 0.03 | 0.25 ± 0.03 | 0.28 ± 0.02 | 0.24 ± 0.03 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.75 ± 0.01 | 0.75 ± 0.01 | 0.74 ± 0.01 | 0.76 ± 0.01 | 0.83 |
Mex HD10 | −0.04 ± 0.06 | 0.05 ± 0.02 | 0.15 ± 0.02 | 0.08 ± 0.04 | 0.28 ± 0.02 | 0.14 ± 0.02 | 0.22 ± 0.03 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.73 ± 0.01 | 0.71 ± 0.01 | 0.74 ± 0.01 | 0.72 ± 0.01 | 0.20 |
Mex I10 | −0.06 ± 0.06 | 0.23 ± 0.03 | 0.26 ± 0.02 | 0.23 ± 0.03 | 0.22 ± 0.03 | 0.29 ± 0.02 | 0.27 ± 0.04 | 0.51 ± 0.01 | 0.51 ± 0.01 | 0.50 ± 0.01 | 0.51 ± 0.01 | 0.49 ± 0.01 | 0.50 ± 0.01 | 0.49 ± 0.01 | 0.82 |
Nepal B10 | −0.04 ± 0.07 | 0.04 ± 0.02 | 0.17 ± 0.01 | −0.07 ± 0.04 | 0.09 ± 0.03 | 0.14 ± 0.02 | 0.04 ± 0.02 | 0.56 ± 0.01 | 0.56 ± 0.01 | 0.56 ± 0.01 | 0.57 ± 0.01 | 0.58 ± 0.01 | 0.56 ± 0.01 | 0.57 ± 0.01 | 0.61 |
Nepal B11 | −0.05 ± 0.08 | 0.23 ± 0.03 | 0.32 ± 0.02 | 0.25 ± 0.03 | 0.35 ± 0.03 | 0.32 ± 0.02 | 0.34 ± 0.03 | 0.53 ± 0.01 | 0.53 ± 0.01 | 0.53 ± 0.01 | 0.55 ± 0.01 | 0.58 ± 0.01 | 0.53 ± 0.01 | 0.57 ± 0.01 | 0.77 |
Pak I10 | −0.03 ± 0.07 | 0.20 ± 0.02 | 0.28 ± 0.02 | 0.11 ± 0.04 | 0.22 ± 0.03 | 0.28 ± 0.01 | 0.21 ± 0.03 | −0.02 ± 0.01 | −0.02 ± 0.01 | −0.03 ± 0.01 | −0.08 ± 0.02 | 0.02 ± 0.03 | −0.02 ± 0.01 | −0.03 ± 0.03 | 0.65 |
Pak I11 | −0.07 ± 0.07 | 0.16 ± 0.02 | 0.30 ± 0.02 | 0.25 ± 0.03 | 0.42 ± 0.02 | 0.30 ± 0.02 | 0.40 ± 0.03 | −0.01 ± 0.01 | −0.01 ± 0.01 | −0.01 ± 0.01 | −0.01 ± 0.01 | −0.03 ± 0.02 | −0.01 ± 0.01 | −0.01 ± 0.01 | 0 |
Sudan W10 | −0.08 ± 0.06 | 0.20 ± 0.04 | 0.31 ± 0.02 | 0.21 ± 0.03 | 0.31 ± 0.03 | 0.32 ± 0.02 | 0.30 ± 0.03 | 0.74 ± 0.01 | 0.74 ± 0.01 | 0.75 ± 0.01 | 0.70 ± 0.02 | 0.75 ± 0.01 | 0.75 ± 0.01 | 0.74 ± 0.01 | 0.83 |
Average | −0.06 | 0.15 | 0.24 | 0.17 | 0.28 | 0.24 | 0.27 | 0.52 | 0.52 | 0.52 | 0.52 | 0.54 | 0.52 | 0.53 |
Broad-sense heritability H2 of TTF in each environment.
Models: M1 Y = E+L+e; M2 Y= E+L+A+e; M3 Y= E+L+G+e; M4 Y= E+L+A+AE+e; M5 Y= E+L+G+GE+e; M6 Y= E+L+G+A+e; M7 Y= E+L+G+A+GE+AE+e.
Names of the environments are given in Table 1.
In summary, for the complex trait GY, M6 and M7 with interactions had the highest average prediction ability across environments for CV1 (0.29 and 0.31, respectively), and for CV2 (0.37 and 0.38, respectively). For the less complex trait GW, M3 and M7 showed the highest mean prediction ability for CV1 (0.45), and it was around 0.63 for all models in CV2. For grain number (GN) (which is a GY component and a complex trait), M5 and M7 gave the highest prediction ability for CV1 (0.32) and CV2 (0.43). For trait TTF, M5–M7 (0.28, 0.24, and 0.27, respectively) were the best for CV1; all models performed similarly for CV2 (0.52–0.53).
Trends in prediction ability vs. heritability
The best model for GY was M7 and, for CV1, it showed increasing values of environment heritability with their corresponding prediction accuracies, whereas M1 prediction ability was not related to heritability values (Figure B1-A, Appendix B). For GY in the CV2 scenario, the best and worst models had similar prediction ability, and showed an increasing trend of up to H2 = 0.50; values decreased thereafter (Figure B1-B, Appendix B). For trait GW in the CV1 scenario, a positive trend of increased prediction ability with increased H2 values was observed for the best model (M3), which had no interaction terms. The worst model (M1) did not show a response with increased H2 values (Figure B2-A, Appendix B). For the CV2 scenario, the best and worst models showed increased correlation values, and an increase in H2 values (Figure B2-B, Appendix B).
For GN, the correlations and H2 values of the best model (M7) showed a positive trend in the CV1 scenario, whereas the basic model (M1) showed no association with H2 values (Figure B3-A, Appendix B). Similar to GY, the best and basic models showed very close prediction ability and H2 values for environments in the CV2 scenario for GN (Figure B3-B, Appendix B). For TTF, the best model (M5) did not show greater prediction ability, the positive trend was lower (R2 = 0.12), and the basic model M1 showed no association with H2 values (R2 = 0.08) (Figure B4-A, Appendix B). In the CV2 scenario, the best and basic model for TTF did not show high association between prediction values and H2 estimates, with some sites with high heritability estimates showing lower prediction values (Fig. B4-B, Appendix B).
Discussion
The WAMI panel has been extensively studied for several complex traits: adaptation to density (Sukumaran et al. 2015b), GY and yield components (Sukumaran et al. 2015a), drought stress (Edae et al. 2013, 2014), and earliness per se (Sukumaran et al. 2016). Since it was also phenotyped under diverse environments around the world, it is a perfect panel for testing some of the genomic and pedigree selection models. Data from these testing sites were used routinely to select lines for release as varieties, and for crossing them to generate new prebreeding lines (Reynolds and Langridge 2016). Physiological breeding is aimed at improving wheat productivity through complex physiological traits. These traits are often controlled by genes with small effects; if they can be proven to be of value in the breeding program, they are more effectively selected using genomic selection methods than using MAS.
Several models have been proposed for the genomic prediction schemes; however, it is important to test them on diverse environmental data before using them in the breeding program. Models 6 and 7 were the best models, for they had the highest average prediction ability values for the CV1 and CV2 scenarios for GY among all environments. Here, we evaluated seven models (some with the G×E term), and concluded that these models can predict GY with moderate to high levels of prediction ability, whereas less complex traits, such as GW, can be predicted without including any interaction terms in the model.
The results of this study agree with those of a recent study on Zn and Fe grain concentration in spring wheat (Velu et al. 2016). Models that include G×E interaction terms showed higher prediction accuracies. Also, prediction ability was generally associated with trait heritability, as in earlier reports (Muranty et al. 2015). The highest prediction ability was for GW, which is a high heritability trait in the WAMI panel (Sukumaran et al. 2015a). Another observation was that, for some environments, M3 gave high prediction ability for GW in the CV1 scenario, whereas model M2 was the best in CV2. In this study, we evaluated the correlation between genomic- and pedigree-based estimated breeding values, with phenotypic data from field trials. With a reasonable number of molecular markers, and incorporating G×E terms in the models, higher prediction ability was obtained for the “genomic” component when compared to pedigree-based prediction models (Burgueño et al. 2011). This was also dependent on trait heritability, as GW had higher prediction ability values even when using M3 (Muranty et al. 2015).
Genotypic values of lines in several environments were predicted using genomic prediction models; when compared across environments, the highest prediction ability was recorded at environments in Cd. Obregon (Mexico) for GY, GN, GW, and TTF. Relatively good climate, as well as optimal management of the Cd. Obregon site, are big factors influencing heritability of yield and prediction ability; sites with high heritability have higher prediction ability. However, our analysis also showed that there is no linear association between heritability and prediction ability values; nevertheless, prediction ability could be a function of H2 values and other parameters (Spindel et al. 2015). Another factor that could increase genomic prediction ability is incorporating high-dimensional environmental covariates (Jarquin et al. 2014; Pérez-Rodríguez et al. 2015). Recent studies on wheat have shown that GS selection could reshape wheat breeding because it produces higher genetic gains than conventional breeding (Bassi et al. 2016).
Conclusions
Genotype × environment prediction models in genomic selection and pedigree-based selection can help accelerate breeding cycles for complex traits such as grain yield in multi-environmental trials. Traditionally, breeders have depended on phenotypic selection for generation advancement. Results of the present study show that GS is a complementary method to phenotypic selection with medium-to-high prediction ability values. Genomic prediction of GY, and other traits in spring wheat lines evaluated in a large and diverse number of international environments, indicated that sites in Mexico and India could be key sites for genomic-assisted breeding. A set of wheat lines not observed in several site-year combinations were predicted with correlations of 0.3–0.5 in Mexico and India (CV1) for models that included genomic and pedigree interaction with environments. When some of these lines were observed in some environments, this correlation increased to 0.45–0.53 (CV2).
For less complex traits, such as GW, the prediction ability of lines not observed in sets of environments increased to about 0.6 for Mexican environments (CV1). Sets of wheat lines observed in some environments, but not in others, were predicted with correlations of up to 0.8 in Mexican and India environments (CV2) for genomic-enabled prediction models including (or not) genomic and pedigree interactions with environments.
Acknowledgments
The authors acknowledge the staff at research stations where the field experiments were conducted. They also acknowledge the financial support of the International Wheat Yield Partnership, Mexico’s Secretariat of Agriculture, Livestock, Rural Development, Fisheries and Food, and Arcadia Biosciences. We appreciate the help of Jose Manual Mendoza for the use of Arcmap software.
APPENDIX A
Table A1. ANOVA of the 18 environments for GY, GN, GW, and TTF.
Source | GY | GN | GW | TTTF | ||||
---|---|---|---|---|---|---|---|---|
df | MS | df | MS | df | MS | df | MS | |
Env | 17 | 1621.45*** | 17 | 10,710,471,211 | 17 | 12,355.91 | 16 | 186,946,414. |
Rep (Env) | 18 | 5.09*** | 18 | 91,729,154.79 | 18 | 138.41 | 17 | 646,553.8 |
Entry | 293 | 3.89*** | 293 | 51,442,282.18 | 293 | 233.89 | 287 | 12,232,101 |
Env*Entry | 4981 | 1.24*** | 4981 | 12,314,123.59 | 4981 | 15.90 | 4592 | 29,846,089 |
Error | 5236 | 0.90 | 5236 | 9,058,283.004 | 5241 | 7.67 | 5051 | 8,835,189 |
Model R-square | 0.88 | 0.84 | 0.90 | 0.96 | ||||
Coefficient of variation | 22.7 | 23.65 | 8.41 | 3.33 | ||||
Mean | 4.17 (ton/ha) | 12,727.66 (number) | 32.91 (gms) | 1255.1 (°D) | ||||
Broad-sense heritability (H2) | 0.41 | 0.51 | 0.74 | 0.48 |
df, degrees of freedom, MS mean squares, Env, environment; Rep, replication; °D, degree days.
*** significant at α = 0.001 level of significance.
APPENDIX B
Footnotes
Communicating editor: E. Huang
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Associated Data
This section collects any data citations, data availability statements, or supplementary materials included in this article.
Data Availability Statement
All the phenotypic data for each environment and trait, as well as the genomic data, can be downloaded from the link http://hdl.handle.net/11529/10714.