AN ABSTRACT OF THE THESIS OF Robert C. Gaynor for the degree of Master of Science in Crop Science presented on May 27, 2010. Title: Quantitative Trait Loci Mapping of Yield, its Related Traits, and Spike Morphology Factors in Winter Wheat (Triticum aestivum L.). Abstract approved: _____________________________________________________________________ C. James Peterson Increasing grain yield in wheat (Triticum aestivum L.) is a challenging task, because yield is a complex trait controlled by many genes and highly influenced by environmental factors. The genetic control of yield components and other traits associated with yield may be less complex and thus more manageable for breeding. This study seeks to identify quantitative trait loci (QTLs) for these traits. Two new genetic linkage maps were constructed from recombinant inbred lines (RILs) derived from crosses between the Oregon soft white winter wheat variety Tubbs and a Western European hard red winter wheat variety, Einstein. A third linkage map was constructed from RILs from a cross with Tubbs and a Western European experimental hard red winter wheat line. A combination of Diversity Arrays Technology (DArT), Simple Sequence Repeat (SSR), orw5, and B1 markers were used to construct genetic linkage maps. Two replications of the RIL populations were grown in yield trial sized plots at Corvallis, OR and Pendleton, OR in 2009. The RILs were evaluated for grain yield, spikes per m2, fertile spikelets per spike, sterile spikelets per spike, seeds per spike, seeds per fertile spikelet, average seed weight, growing degree days (GDD) to flowering, GDD to physiological maturity, GDD of grain fill, plant height, test weight, and percent grain protein. Composite interval mapping (CIM) detected 146 QTLs for these traits spread across all chromosomes except for 6D. Thirty six percent of all of the QTLs detected were in close proximity to four loci: Rht-B1, Rht-D1, B1, and Xgwm372. The use of factor analysis to aid in QTL mapping for correlated traits related to spike morphology was explored. Quantitative trait loci mapping of factor scores for these traits potentially showed an increase in statistical power to detect QTLs and a decrease in the probability of type I error over mapping the traits individually. ©Copyright by Robert C. Gaynor May 27, 2010 All Rights Reserved Quantitative Trait Loci Mapping of Yield, its Related Traits, and Spike Morphology Factors in Winter Wheat (Triticum aestivum L.) by Robert C. Gaynor A THESIS submitted to Oregon State University in partial fulfillment of the requirements for the degree of Master of Science Presented May 27, 2010 Commencement June 2011 Master of Science thesis of Robert C. Gaynor presented on May 27, 2010. APPROVED: _____________________________________________________________________ Major Professor, representing Crop Science _____________________________________________________________________ Head of the Department of Crop and Soil Science _____________________________________________________________________ Dean of the Graduate School I understand that my thesis will become part of the permanent collection of Oregon State University libraries. My signature below authorizes release of my thesis to any reader upon request. _____________________________________________________________________ Robert C. Gaynor, Author ACKNOWLEDGEMENTS I would like to thank Adam Heesacker for his work in constructing the genetic linkage maps used in this study. Thanks to Mark Larson, Eddie Simons, Mary Verhoeven, Dolores Vasquez, and the wheat project’s summer crew for helping collect data. I would also like to thank Lan Xue, Oscar Riera-Lizarazu, Mike Flowers, Jim Peterson, and Jeff Leonard for advising on technical aspects of this research. Finally, I would like to thank Jeffery Stone for serving as a graduate council representative on my committee. TABLE OF CONTENTS Page 1. INTRODUCTION.....................................................................................................1 2. LITERATURE REVIEW.........................................................................................6 2.1. Yield Components and Crop Ideotype........................................................6 2.2. Donald's Ideotype......................................................................................10 2.3. Genetic Markers........................................................................................12 2.4. Linkage Analysis.......................................................................................15 2.5. QTL Mapping............................................................................................17 2.6. Factor Analysis..........................................................................................22 2.7. Crop Models..............................................................................................26 3. MATERIALS AND METHODS............................................................................28 3.1. Plant Populations.......................................................................................28 3.2. Data Collection and Summary Statistics...................................................29 3.3. Linkage and QTL Mapping.......................................................................30 3.4. Factor Analysis..........................................................................................32 4. RESULTS AND DISCUSSION.............................................................................34 4.1. Genetic Linkage Maps...............................................................................45 4.2. QTL Mapping............................................................................................45 4.3. Factor Analysis..........................................................................................56 5. CONCLUSION.......................................................................................................64 6. BIBLIOGRAPHY...................................................................................................66 TABLE OF CONTENTS (Continued) Page 7. APPENDICES.........................................................................................................73 LIST OF TABLES Table Page Table 1 Measured traits.................................................................................................31 Table 2 Least square means for parents and RILs in TxN population..........................36 Table 3 Least square means for parents and RILs in ExT1 population........................37 Table 4 Least square means for parents and RILs in ExT2 population........................38 Table 5 Summary of across location analyzes for the three populations of RILs........39 Table 6 Pearson product-moment correlations for the Tubbs x NSA 98-0995 RILs...41 Table 7 Pearson product-moment correlations for the ExT1 population......................42 Table 8 Pearson product-moment correlations for the ExT2 population......................43 Table 9 QTLs for yield, grain protein, test weight, and spikes per m2.........................46 Table 10 QTLs for flowering, ripening, and grain fill duration....................................47 Table 11 QTLs for plant height and seeds per spike.....................................................48 Table 12 QTLs for fertile spikelets per spike and sterile spikelets per spike...............49 Table 13 QTLs for seeds per fertile spikelet and seed weight......................................50 Table 14 Pearson product-moment correlations between initial factors and yield, grain protein, and test weight........................................................................................57 Table 15 Factor loadings for rotated spike morphology traits......................................59 Table 16 QTLs for spike morphology factors...............................................................60 LIST OF APPENDIX FIGURES Figure Page Figure 1 Genetic linkage map for the Tubbs x NSA 98-0995 population (TxN) with QTL positions.......................................................................................................74 Figure 2 Genetic linkage map for the larger Einstein x Tubbs population (ExT1) with QTL positions.......................................................................................................78 Figure 3 Genetic linkage map for the smaller Einstein x Tubbs population (ExT2) with QTL positions.......................................................................................................82 Quantitative Trait Loci Mapping of Yield, its Related Traits, and Spike Morphology Factors in Winter Wheat (Triticum aestivum L.) 1. INTRODUCTION Increasing grain yield is a primary goal of wheat (Triticum aestivum L.) breeders. Accomplishing this goal is a challenging task due to the complexity of the trait. Grain yield is a complex trait, because it is controlled by many genes and its expression is heavily influenced by environmental factors. Wheat breeders produce large numbers of crosses every year to develop higher yielding varieties. These crosses are in turn used to generate numerous inbred lines with unknown yield potential that have to be evaluated for a litany of agronomic and quality traits before any of these lines can become eligible for release as a variety. For example, Oregon State University's (OSU) wheat breeding program typically generates over 600 crosses and evaluates around 40 thousand F4 and F5 rows of inbred lines each year. Accurately measuring yield of these lines is only possible in subsequent generations when there is sufficient seed to plant replicated yield trials at multiple locations. Thus, several cycles of selection have to be carried out on those lines before they are ever evaluated for yield. Once sufficient seed is generated, the high cost of running yield 2 trials severely limits the number of lines that can be evaluated. At OSU, less than 300 of the initial 40 thousand rows will be screened for yield in replicated trials. Many of these lines will prove to have insufficient yields to be candidates for variety release. Finding a way to screen lines earlier and at a lower cost could vastly improve a breeder's ability to generate higher yielding varieties. Marker assisted selection (MAS) is a potential method for selecting for yield at early generations. This method uses genetic markers to select for favorable plants based on knowledge of associations between those markers and traits. Genetic markers only require a small sample of DNA, so limited quantities of seed are not a problem. Screening a line with genetic markers is also significantly cheaper than screening that line in a replicated yield trial. However, there are several limitations to MAS that have to be addressed first. The most common way of finding markers for MAS is to identify quantitative trait loci (QTLs) using QTL mapping (Lande and Thompson, 1990). Statistical limitations of QTL mapping for complex traits, like yield, can make such an approach impractical (Doerge, 2002). However, QTL mapping for traits that influence yield may be more successful, because they often have simpler genetic control and are less influenced by environment (Yin et al., 2000). MAS for traits that influence yield may then be an indirect means of applying early generation selection for yield. The traits that influence yield include disease resistance, stress tolerance, maturity, and plant architecture. A great deal of research has gone into elucidating the 3 genetic control for disease resistance (e.g. Singh et al., 2000), stress tolerance (e.g. Zhou et al., 2007), maturity (e.g. Yan et al., 2003) and plant architecture, particularly yield components (e.g. Li et al., 2007). This has lead to successful, albeit limited, implementation of MAS techniques for disease and stress response in wheat (e.g. Murphy et al., 2009; Baerstmayr et al., 2009; Kumar et al., 2010). Markers are available for vernalization genes, genes that partially influence maturity, which can be used in MAS (e.g. Sherman et al., 2004). Dwarfing genes, major determinants of plant height, also have markers that can be used for MAS (Ellis et al., 2002). Besides plant height, there is little literature to suggest that successful MAS strategies for yield components and other architectural traits have been implemented. Successfully incorporating QTLs for these traits into a MAS program will likely not be accomplished by simply pyramiding genes. This is due to the lack of an obvious “more is better” philosophy for these traits that is present with disease resistance and stress tolerance. Breeders will instead have to manipulate QTLs for yield components and other architectural traits to achieve a crop ideotype. An ideotype is an idealized structure of a plant that obtains the maximum performance under production conditions. Finding optimum values for yield components and architectural traits that obtain this ideotype will require consideration of their interactions with each other, related traits, and the environment (Loomis et al., 1979). Combining knowledge of these interactions with knowledge of the QTLs that control these traits can be accomplished with “QTL-based ecophysiological modeling” (Yin et 4 al., 2003). This approach uses a statistical model to estimate yield of a variety based on its composition of QTLs and the environmental and production conditions that variety is grown under. Before such an approach can be considered, markers for QTLs that are relevant to germplasm that a breeder is using have to be available. The QTLs that have already been identified may not be relevant to OSU's germplasm. These QTLs may simply not be present in the germplasm. QTL effects are dependent on genetic background, so the QTLs already identified may perform very differently in OSU's germplasm than they did in the studies that identified them (Babu et al., 2004). This could mean that the already identified QTLs for traits related to yield have no practical value to OSU's breeding project. The goal of this study is to identify QTLs for traits related to yield in crosses that are representative of elite germplasm in OSU’s wheat breeding program. The genetic mapping populations used herein contained crosses with an Oregon variety, Tubbs, and varieties from Nickerson, a private breeding program based in Western Europe. Material from Nickerson has been a source of well adapted lines for enhancing germplasm at OSU and has also been a source of lines for direct release as varieties. Knowledge of important QTLs in the genetic background of these crosses could be applicable to a wide range of crosses in OSU’s wheat breeding program. Furthermore, this study examines using QTL mapping of factor scores as a way of dealing with numerous correlated traits in QTL analyzes. The use of factor 5 scores would create new variables that are not correlated and can reduce the number of variables that are analyzed with QTL mapping. This should result in a reduction of type I error compared to analyzing traits individually. It may also be possible to increase the power to detect QTLs with this method. Factor scores will be calculated for traits related to spike morphology. The results of QTL mapping for these factors will be compared to mapping done on the original traits to see if any of these potential benefits are realized. 6 2. LITERATURE REVIEW 2.1. Yield Components and Crop Ideotype The study of yield in cereals has often been based on exploring the relationships between yield and other traits. In particular, traits that are referred to as yield components have been the subject of considerable study. Engledow and Wadham (1923) may have been the first to partition the yield of cereal crops into its components. Their list of components included, among others: plants per unit area, number of ears per plant, number of grains per ear, and weight per grain. They proposed that if the favorable combinations of these traits were known, producing higher yielding lines is possible by generating crosses that obtain these combinations. Although they didn't phrase it as such, this favorable combination of traits can be considered an ideotype. An ideotype simply refers to the idealized appearance of a plant variety. Subsequent research has produced some support for Engledow and Wadham's proposal by showing evidence that changes in the distribution of yield components in the highest yielding varieties can partially explain increases in yield over time (Calderini, 1995). Changes in maturity and plant height have also been attributed to increased yield and were the driving forces behind the “Green 7 Revolution” (Borlaug, 1983). Thus, determining a wheat ideotype requires consideration of various components of plant architecture and maturity. Varieties are ultimately judged on their performance in production settings. Therefore, studies that evaluate performance in markedly different conditions may not be meaningful for determining an ideotype (Donald, 1968). For example, many studies on yield components and plant architecture have been conducted on individual plants or thinly seeded plots (e.g. Quarrie et al., 2006; Li et al., 2006). The performance of these individual plants and thinly seeded plots is not likely to be representative of how the plants will perform under production settings (Nerson, 1980). For this reason, these studies may have limited to no applicability when it comes to constructing an ideotype. Only studies of yield components as they behave in a community of plants are likely to further the creation of a crop ideotype. It is widely known that the optimum maturity for wheat in one environment can be different in another environment. Thus, the ideotype for one region can be different from the ideotype in another region. This difference may extend beyond maturity. For example, seeds per m2 and tillering have been shown to be the two most correlated components with yield in a study conducted in Kansas (Donmez et al., 2001). This is consistent with the widely accepted view that gains in yield are primarily due to increases in seeds per unit area (Slafer et al., 1996). However, selection based on kernel weight has been shown to be a more effective way of breeding for higher yielding lines in a study conducted in Oklahoma (Alexander et al., 8 1984). Calderini et al. (1995) examined a historical accession of varieties in Argentina and found an increase in seeds per unit area as the driving force for increasing yield in varieties released before 1987 and found seed weight to be more important in varieties released after 1987. These discrepancies could be the product of the different populations studied, but it may also represent differences in ideotypes for these regions. If that is the case, findings from one region may not be of any value to another region. In addition to variation between environments there is also variation between years that have to be considered. The variation in wheat yields from one year to the next in one field can be large (Washmon et al., 2002). Thus, data from a single year may not be representative of an average year. This year to year variation will have to be taken into account when formulating an ideotype. First, care must be taken to not give too much weight to a single year’s data. The ability of an ideotype to have stable yields over multiple years will have to be considered. Large degrees of correlation between yield components and other traits such as maturity and height have been observed in several studies (e.g. Li et al., 2007; Kato et al., 2000). These correlations can impact studies that attempt to determine the structure of an ideotype. For example, multiple regression of yield on its components is an approach that previously was often used for studying yield components (Walton, 1971). The results from these analyzes may be misleading, because the interpretation of the calculated coefficients is how much a change in one trait will change yield when 9 all other traits are held constant. Since the traits are correlated, it is not likely and perhaps not possible to change just one while keeping the others constant. Furthermore, the estimates of standard errors for those coefficients are not accurate when traits are correlated. Thus, consideration of these correlations is crucial. This has lead to research into yield components that include a statistical analysis involving the correlation matrix such as path analysis (e.g. Fonseca and Patterson, 1968) or factor analysis (e.g. Walton, 1971). These sorts of analyzes give information on how changing one yield component effects yield and the other traits simultaneously. How much an individual trait can be manipulated and how consistent the effects of those manipulations are over a large range of changes is not determined with these analyzes. This drastically limits the ability of these approaches to predict the performance of varieties not studied. More recent studies into yield components to identify QTLs have largely ignored correlations between traits (e.g. Börner et al., 2002; Marza et al., 2005). Even when the correlations are considered, the extent of the examination is often limited to reporting a correlation matrix and suggesting that collocated QTLs for different traits represent close linkage or pleiotropy (e.g. Kato et al., 2000; Li et al., 2007; Cuthbert et al., 2008). These correlations could partially be examined with multiple-trait QTL analyzes, and such an approach would increase the power of QTL detection (Mi et al., 2008). The massive computational requirement of analyzing many traits at once has been a limiting factor to the adoption of this technique. An alternative is to use 10 principal component analysis to reduce the correlated traits into latent, uncorrelated variables. This approach has been used with tassel morphology in maize (Upadyayula et al., 2006) and for morphological factors in wheat (Addisu et al., 2009). The study on tassel morphology found QTLs for the principal components that were not identified with single trait analysis. This might have represented increased power from the use of principal components. The study in wheat didn’t find any additional QTLs. This could be due to the inclusion of too many traits in the principal component analysis. This large number of traits were probably controlled by many genes, so there was no realized benefit of increased statistical power. 2.2. Donald's Ideotype Donald (1968) presented a model for a wheat ideotype in an article titled “The Breeding of Crop Ideotypes”. He attempted to draw on the research available at the time to predict what a wheat ideotype would look like. His proposed ideotype would have short, strong stems to withstand lodging. He pointed to the work being done by others with dwarfing genes and the general trend towards shorter wheat as evidence supporting this view. The subsequent “Green Revolution” in wheat that is in large part attributed to the introduction of dwarfing genes verifies Donald's conclusion (Borlaug, 1983). Donald's ideotype also had erect leaves to allow for maximum 11 illumination of the photosynthetic surfaces. The plant would have a few small leaves. Small leaves were deemed better than large leaves, because they are more likely to be erect. He also noted that theoretical work suggested that an arrangement of several uniformly dispersed small leaves was better at capturing light than a few large leaves. Donald proposed that the ear should be large to assure an adequate sink for photosynthates and to allow for high levels of grain production. The ear should also be erect and have awns to allow for maximum capture of light. A high proportion of seminal roots were deemed desirable for gathering soil nutrients. Donald also stated that the degree to which tillering is desirable is a product of production practices. He suggested that it would be best to grow an ideotype that only had a single culm, because the production of tillers is wastes a plant's resources when it results in overproduction of tillers that are subsequently aborted. Changing the production practices, namely seeding rate, would then be needed to best fit this plant type. The main characteristic of Donald's ideotype, as proposed by him, is that the variety should be a poor competitor. Donald argued that varieties that are strong competitors use their resources to out compete their neighbors. In a well managed production setting, those neighbors are primarily plants of the same variety. Thus, there is no benefit to the yield of the crop when the plants spend resources trying to out-compete other plants that also contribute to the overall yield. Therefore, it would be better to have a variety that more efficiently use those resources for the production of yield. This trait of Donald’s ideotype is probably the most important for breeders, 12 because early generation selections are likely to favor strong competitors. For example, F3 generation plants are typically grown in bulk plots in breeding projects. Under these conditions each plant will have neighbors of different genetic composition next to them. The strongest competitors will out compete their weak neighbors. Thus, the stronger competitors will yield more and appear to have a more favorable phenotype than the weak competitors. This will likely bias the breeder towards selecting for the strong competitors. It may therefore be more prudent for breeders to select plants that don't necessarily look the best at these generations. These plants may actually produce higher yielding varieties according to Donald. 2.3. Genetic Markers Understanding the genetic control of yield components and other traits related to yield requires the use of genetic markers. Genetic markers are powerful tools for exploring the genetic composition of organisms. They can be used to construct genetic maps that can subsequently be used to locate genes controlling various traits within an organism. They can also be used by breeders for identifying favorable genotypes in MAS. For genetic markers to be useful, they have to be able to distinguish between different alleles at a locus. When this is the case, a genetic marker is said to be 13 polymorphic. The ability of a marker to detect polymorphisms can be classified as either dominate or co-dominate. Dominate markers have a binary response; they are either expressed or not expressed. These types of markers are only able to detect the presence of one particular allele at a locus, and they cannot definitely distinguish between homozygous and heterozygous individuals. Negative results (lack of expression) are not very informative with these markers, because there are potentially multiple genotypes that cause this result. Thus, two individuals that share a positive result can be said to share at least one allele at a locus. Two individuals that share a negative result can’t be considered a match, unless it is known that there are only two alleles present at that locus. Co-dominate markers are more informative than dominate markers. These types of markers are able to distinguish between multiple alleles at a locus. This gives these markers the ability to detect heterozygotes and they are more frequently polymorphic than dominate markers (Paux and Sourdille, 2009). The majority of genetic markers use at least one of two important biotechnological tools (Paux and Sourdille, 2009). These tools are restriction endonucleases (or restriction enzymes) and polymerase chain reaction (PCR). Restriction enzymes cleave double stranded DNA at specific recognition sites. These recognition sites are short sequences of DNA that are interspersed in plant and animal DNA (Voet and Voet, 2004). Markers that utilize restriction enzymes detect polymorphisms based on differences in the locations of these recognition sites (Paux and Sourdille, 2009). PCR is a technique that amplifies DNA using a set of genetic 14 probes called primers and a heat stable polymerase. The polymerase is used to exponentially increase the number of copies of DNA in regions that are flanked by primers. Correct primer selection allows polymorphic regions of DNA to be amplified and used as genetic markers (Voet and Voet, 2004). Primers can also be chosen to amplify fragments created using restriction enzymes. This can be accomplished by ligating a piece of DNA, called an adapter, to the end of these fragments that contains a sequence of DNA that the primers bind to (Voet and Voet, 2004). The most commonly used genetic markers for constructing wheat genetic linkage maps are Amplification Fragment Length Polymorphisms (AFLPs), Simple Sequence Repeats (SSRs), and the proprietary Diversity Array Technology (DArT) markers (Paux and Sourdille, 2009). AFLPs are dominate markers that are generated by cutting DNA with two restriction enzymes, ligating DNA to the end of the fragments, and amplifying fragments with PCR. The main benefit of these markers is that they don’t require any development. SSRs are codominate makers that amplify regions of the genome that contain short, repeated sequences of DNA. These markers are highly polymorphic and fairly high throughput, but they are very expensive to develop. DArTs are dominate markers that are used in large capacity microarrays to screen fragments of DNA for hybridization with probes. These markers are ultrahigh throughput. On a per marker basis they are inexpensive, but thousands of markers are screened at once making them expensive to use. 15 2.4. Linkage Analysis To improve the usefulness of genetic markers, it is best to know where those markers are located in the genome. The method for determining this is linkage analysis. Linkage refers to the tendency of genes to be inherited together. This occurs when they are located on the same chromosome and in relatively close proximity to each other. Linkage can also be observed between marker loci. The examination of linkage through linkage analysis is the foundation for constructing genetic maps (Wu et al., 2007). Traits that are inherited qualitatively and by only one gene can be directly incorporated into those genetic maps using linkage analysis (Kaeppler et al., 1993). Wheat is an allohexaploid, so many of its qualitative traits are controlled by three genes. Thus, if more than one of those genes are segregating in a population this method cannot be used for mapping the trait. The real power in genetic maps is the ability to place quantitative traits on those maps using QTL analysis (Wu et al., 2007). Genetic maps that contain the locations of important traits can then be used by breeders for identifying markers for MAS. The first step in linkage analysis is obtaining a population of individuals that share the same parents. Either F2, backcross, doubled haploid (DH), or recombinant inbred line (RIL) populations are typically used. The DH and RIL populations are the most common, because subsequent generations can be obtained through self-crossing 16 that will not differ genetically. This makes it easy to repeat experiments using these populations in additional years. All of these populations allow for the measurement of linkage between sets of markers that are polymorphic in the parents (Wu el al., 2007). If the loci are unlinked, equal proportions of the parental, non-recombinant, and nonparental, recombinant, pairings of marker alleles would be expected. The lower the proportion of recombinants between two loci, the higher the linkage between them is likely to be. The greater the linkage between loci the closer they are in terms of genetic distance. It is thus a matter of ordering loci according to their linkage to find where they fit on a genetic map. In theory, finding the optimum order of loci can be determined simultaneously by maximizing the likelihood function for all possible orders. In practice there are x!/2 orders for x loci, so the number of calculations that are required with an actual set of markers would be impractical for current computing technology (Wu et al., 2007). To overcome this limitation, the order of loci is determined using sets of only two or three loci at a time (Wu et al., 2007). After considering many of these sets it is possible to determine an overall order for all loci. The distance between these loci is a function of the recombination rates between them. Recombination rates are not additive, so for the purpose of creating a linkage map the recombination rates are transformed to additive measures of genetic distance called Morgans. This transformation is performed using one of several available mapping functions. The most popular mapping functions are Haldane and Kosambi (Wu et al., 2007). The 17 difference between these functions is how they handle the occurrence of crossover events between two markers. Haldane’s original formula called for a parameter that controls the occurrence of crossovers called coincidence (1919). The mapping function known as Haldane’s mapping function sets this parameter to one (Crow and Dove, 1990). This means the function assumes that crossovers occur randomly and independently of each other, so they can be modeled using a Poisson distribution (Wu et al., 2007). Kosambi (1944) introduced a function that assumes the coefficient of coincidence is proportional to the recombination rate between the markers. This results in interference at short distances that diminishes as the distance increases (Crow and Dove, 1990). 2.5. QTL Mapping After constructing genetic maps, the next step for locating areas of the genome that control a trait of interest is QTL mapping. QTL mapping is a statistical method that aims to find associations between traits and regions of DNA. The regions that associate with the trait are known as QTLs. Markers that are closely linked to these QTLs are commonly used in MAS to select for the desired allele of the target QTL. Many methods for conducting QTL mapping have been proposed. 18 The simplest technique for QTL mapping is Single Marker Analysis (SM). This technique tests if different marker alleles at a locus are associated with different values of the phenotype. This technique doesn't require a genetic map and there can be multiple marker alleles tested at once (Wu et al., 2007). Analysis of variance (ANOVA) is used to test the significance of the different marker alleles. This approach has severe limitations. First, estimation of the QTL’s effect is confounded with the genetic distance between the marker and the QTL (Lander and Botstein, 1989). That is, the less linkage the marker has with the QTL, the more the effect of the QTL will be underestimated. Multiple comparisons are also problematic for single marker analysis. Due to the large number of markers that are commonly tested, a large number of type I errors are expected (Jansen, 1994). Multiple comparison techniques can be used to reduce the incidence of type I error, but they will also reduce the power of the test. Performing SM in a genetic mapping population can offer some graphical tools that can help interpreting the results. In a genetic mapping population there are only two alleles possible at each locus, so a t-test is used to test the significance of different alleles. The genetic map also allows for the t-values to be plotted according to their map position. Then multiple markers that test significant for a QTL and are located next to each other on the genetic map can be assumed to be measuring a single QTL. This makes using a genetic map with SM a better way of interpreting the results when it comes to estimating how many QTLs are present and their locations. 19 Another way of using markers to find QTLs would be to use them as predictors in a multiple regression model. However, simultaneously estimating the partial regression coefficients is statistically challenging, because the number of markers may be greater than the number of individuals and many of the coefficients are close to zero (Wu et al., 2007). Xu (2003) proposed using a Bayesian approach to estimating the coefficients when marker density is high to cope with this simultaneous estimation problem. His approach is referred to as whole-genome marker analysis. Compared to SM this approach gives fewer significant peaks, and better estimates the effects and locations of the QTLs (Xu, 2003). Lander and Botstein (1989) formulated a QTL mapping approach that is referred to as Interval Mapping (IM). This approach utilizes a genetic map in performing the calculations for detecting QTLs. The genetic map allows IM to test for the presence of a QTL in the intervals between markers. This is accomplished by maximizing the likelihood function for QTL effect with given values of the flanking markers, considered random variables, and constant values for recombination frequencies between the QTL and each marker. A likelihood ratio (LR) is then constructed comparing this model to the model that assumes there is no QTL present. Traditionally the expectation-maximization algorithm developed by Dempster et al. in 1977 is used, but a regression approximation to the LR statistic that is computationally simpler can be used as an alternative (Haley and Knott, 1992). The procedure is repeated at multiple locations and the resulting LR statistics are plotted against their 20 location on the genetic map. With either method, significance of the LR statistics can be tested using a permutation test that calculates the experiment-wise error (Churchill and Doerge, 1994). Peaks on the map that surpass the significance threshold are used as estimates for QTL locations and effects. A permutation test for significance that sets levels differently for major and minor QTLs has been proposed, but has not been widely adopted (Doerge and Churchill, 1996). IM only tests for the presence of one QTL at a time, so the presence of multiple QTLs can impact the accuracy of the estimates for location and effect of a QTL (Zeng, 1993). Like SM, IM is prone to type I and type II error (Jansen, 1994). Zeng (1994) along with Jansen and Stam (1994) independently proposed a QTL mapping technique that is called Composite Interval Mapping (CIM). This approach expands IM to include covariates chosen from markers outside the test interval. The covariates work to offset the impact that QTLs outside of the test interval have on the performing the likelihood test. There are several methods for choosing markers as covariates available. Zeng (1994) originally tested using all unlinked markers or all markers. Using all unlinked markers gave greater power and using all markers gave better estimates of QTL effects. An additional method using multiple regression modeling techniques of forward, reverse, or forward-reverse selection to choose markers has become popular. These techniques chose from markers not used in the test site and outside of a certain distance from the test site. They are chosen at a distance from the test site to prevent from eliminating the QTL 21 signal. Viewing results and determining significance in CIM is conducted in a similar fashion as with IM. Jiang and Zeng (1994) proposed an extension of CIM to handle more than one trait that is called Multiple-Trait Composite Interval Mapping (MT-CIM). This test only tests one site at a time and uses covariates like CIM, but it looks at more than one trait at a time. This approach offers greater power to detect QTLs when traits are inversely correlated. It also provides a mechanism to test a site that has effects on more than one trait for pleiotropy or close linkage. This can be a valuable tool to breeders, because it allows them to assess if it is possible to break unfavorable combinations of traits. Permutation tests can be used to set significance thresholds as in CIM, but there is some debate as to what is an appropriate null model. A null model that assumes evenly spaced QTLs for the traits might be more favorable than a model that assumes there are no QTLs. In practice, MT-CIM is severely limited by the computational difficulty of handling many traits at one time. Multiple Interval Mapping (MIM) provides a mechanism for testing multiple QTLs simultaneously (Kao et al., 1999). This allows for interactions between QTLs, epistasis, to be examined. However, the level of computation required for this analysis is greater than those previously mentioned. Thus, putative QTLs detected using another method, such as CIM, are best used in the first steps of model building in MIM (Hackett et al., 2000). The models can then be further refined by optimizing the positions and effects of the QTLs and testing for interactions (Kao et al., 1999). A 22 permutation test for determining significance levels doesn't exist for this method. Thus, minimizing a model selection criterion is the preferred method for fitting models (Hackett et al., 2000). However, this method is not able to fully protect against over fitting a model, so other factors such as not exceeding the heritability of a trait are often considered. MIM can be expanded to consider multiple traits. 2.6. Factor Analysis There are two ways to deal with multiple correlated traits in QTL mapping: map each trait separately or use a multiple-trait mapping procedure. Both approaches have disadvantages. Mapping single traits inflates type I error, because multiple analyzes are being performed. Multiple-trait analyzes have greater power to detect QTLs than single trait analyzes, but they are computationally prohibitive and there is no universally accepted model for determining significance of a QTL. Combining factor analysis, a multivariate dimension reduction analysis, with QTL mapping may be a beneficial alternative to those two methods. Factor analysis would reduce the number of variables to be studied and those variables would be uncorrelated. The beginnings of factor analysis date back to attempts by Karl Pearson, Charles Spearman, and others in the early 20th century to quantify intelligence (Johnson and Wichern, 2007). The technique has been used by cereal breeders and 23 agronomists as a way of examining correlated traits such as yield components (e.g. Walton, 1971). The intent of factor analysis is to explain inter-correlations between a set of variables as coming from a few underlying latent variables called common factors. The analysis uses the covariance matrix resulting from this set of variables or its standardized version the correlation matrix. The factors are then extracted by one of three methods: principle component, common factor, or maximum likelihood. The number of factors to be considered is determined and then their coefficients are either examined directly, or after an orthogonal or oblique factor rotation. Factor scoring coefficients can also be calculated. These can be used to determine the factor values of individuals for use in subsequent analyzes. The principle component method for factor extraction is the most popular (Johnson and Wichern, 2007). The first factor is extracted by finding a linear combination of the variables that explains as much of the total variance as possible. The second factor is then determined by finding a linear combination of the variable that is orthogonal to the first and explains as much of the remaining variance as possible. This is process is then iterated until the desired number of factors are obtained, to a maximum of a number of factors equal to the number of variables. The researcher can use multiple methods for determining how many factors to retain. The eigenvalue greater than unity and the scree test are the most popular, but are not necessarily the most accurate (Tanguma, 2000). Parallel analysis is widely considered the most accurate method for selecting the number of factors to retain (Hayton et al., 24 2004). This method compares the eigenvalues of the observed factors to those of randomly generated data to determine if a factor should be retained. Since the principal component method uses all of the variance and not just the shared variance to extract factors it is not considered a true method of factor analysis (Costello and Osborne, 2005). That is, it is really a method of data reduction and not a method for identifying latent variables. A true factor analysis can be performed with the common factor method. The common factor method is performed on a reduced correlation matrix (Johnson and Wichern, 2007). This reduced correlation matrix has the variance that is specific to a variable removed from the diagonal of the matrix. Thus, the matrix only represents the variance shared between variables. There are multiple methods for determining what values should be used for the diagonals. After one of these methods is chosen, the factor solution is then obtained iteratively. However, using the reduced matrix now makes it possible to obtain negative eigenvalues for some of the factors since the reduced matrix doesn't represent all of the variance. The common factor method more accurately reproduces population patterns than the principal component method, but these differences converge when the number of variables is large and the loading patterns increase (Snook and Gorsuch, 1989). The maximum likelihood method is another form of a true factor analysis that assumes the common and specific factors are normally distributed (Johnson and Wichern, 2007). This method can give fairly different results from the common factor 25 method. It is also possible to perform hypothesis tests for the adequacy of the number of factors retained when the assumptions of the maximum likelihood method are met. This gives an additional tool to researcher for deciding how many factors to retain. However, the normal distribution restriction can make the maximum likelihood method unusable for some sets of data. Factor rotation is often applied to aid in the interpretation of factors. The mathematical justification for factor rotation is that orthogonally rotated factors will explain the covariance just as well as the original factors, so there is no unique solution for finding factors (Johnson and Wichern, 2007). The varimax rotation, the most common orthogonal rotation, seeks a rotation that makes as many coefficients close to zero as possible (Kaiser, 1957). The resulting rotated factors can then be easier to interpret than the originals, because individual factors have fewer variables making large contributions to them. In cases where the underlying factors are not assumed to be independent, oblique rotations may be more appropriate (Johnson and Wichern, 2007). These types of rotations seek to explain variables with as few factors as possible. Even after performing one of these types of rotations there can still be a good deal of ambiguity in the interpretation of the factors. The researcher has to rely on his experience to make sense of the factors. The lack of uniqueness in the factor solution that allows for rotation is also a reason that many researchers are opposed to using factor analysis (Kaiser, 1957). The large number of subjective decisions that a researcher has to make can bias the results 26 of the analysis. These biases can have the greatest impact when it comes to selecting the number of factors to retain and interpreting the resulting factor coefficients (Costello and Osborne, 2005). Overall, factor analysis can appear to be more of an art than a science and great care should be taken when interpreting the results (Johnson and Wichern, 2007). 2.7. Crop Models Simply finding QTLs for a trait is of no use unless it is known what the ideal value for that trait is. A method for determining the optimum values for yield components and other traits related to yield is using crop models. Crop models are statistical models that are typically used to predict the yield of a crop. They use predictors based on weather patterns, production practices, nutrient levels, and components known as genetic coefficients (Loomis et al., 1979). Crop models can potentially be used to assist in the design of crop ideotypes by maximizing the contribution from genetic coefficients (Haverkort and Kooman, 1997). The main benefit of this approach is that it can be used to manipulate the genetic coefficients to test plant types not currently available to the breeder (Loomis et al., 1979). Some estimates of genetic coefficients are actually based on observed phenotypic values, so they may really be measuring genotype by environment (GxE) interactions and not 27 actual genetics (Baenziger et al., 2004). For models to have a useful role in structuring a crop ideotype, they have to have input parameters that are firmly based on real genetics. If the parameters are not based on genetics, breeding will not easily be able to produce plants with the desired phenotypic values of those parameters, because it is based on the manipulation of genetics (Baenziger et al., 2004). A recent approach to crop modeling called “QTL-based ecophysiological modeling” has replaced genetic coefficients with QTLs in crop models to incorporate actual genetics into them (Yin et al., 2003). QTLs are regions of DNA that are associated with one or more traits. A QTL is often thought of as a gene, but that is not necessarily the case. A QTL can be a gene, a group of genes, or some other part of DNA that influences the trait. The effects of individual QTLs can be highly dependent on GxE interactions (Jansen et al., 1995). This is particularly the case for complex traits such as yield (Campbell et al., 2003). To overcome this, QTL-based ecophysiological modeling uses QTLs for the component traits of yield which are likely to be less impacted by GxE interactions (Yin et al., 2000). The effects of those QTLs on yield and how the environment influences yield are then considered in the framework of a crop model to produce an estimate for yield. The first attempt at this approach was made in barley with poor results, because the model lacked the power to distinguish small changes in yield (Yin et al., 2000). However, success using the same modeling approach for less complex traits suggests that this approach may be successful for yield in the future (Buck-Sorlin, 2002; Yin et al., 2005). 28 3. MATERIALS AND METHODS 3.1. Plant Populations The populations used for linkage mapping and QTL analysis were obtained by randomly selecting heads from two F2 populations in OSU's wheat breeding program. One population consisted of a cross between Tubbs, an awned, soft white winter wheat variety widely grown in Oregon, and NSA 98-0995, an awnless experimental hard red winter wheat line from the Nickerson breeding program. 280 F5 derived RILs were generated from this population. The other population was a cross of Einstein, an awnless, hard red winter wheat variety from Nickerson that is widely grown in Western Europe, and Tubbs. 276 F5 derived RILs were produced from this population. OSU's wheat breeding program produced these populations by combining two separate crosses. Each individual cross is typically only pollinated with one spike, but a second spike may be used when low levels of pollen are obtained. No record is kept of the precise individuals used in these crosses; just what lines they came from. Thus, it is possible for there to actually be up to four true populations within a nominal population and up to six separate parents. However, only one female plant and one or two males are typically used to create a population. To account for this, the segregation of multi-allelic loci was examined in these populations in an attempt to 29 determine the number of true populations present in each nominal population. This information was used to divide the RILs into “true” populations if necessary and possible. Lines that could not be assigned to a population with confidence were discarded. 3.2. Data Collection and Summary Statistics The ExT and TxN RILs were grown in separate experiments with local varieties to serve as agronomic checks and their parent lines. Since actual parents weren't known, the parental varieties were used in their place. Each experiment was grown at two locations with two replications in a randomized complete block design planted in the fall of 2008. Each replication was planted in a plot that was 1.52 m wide by 4.27 m long using about 90 grams of seed. The two locations were Corvallis, OR and Pendleton, OR. The Corvallis plots contained six evenly spaced rows and the Pendleton plots had seven rows. These locations represent two of the highest yielding locations in Oregon. Each location was managed according to standard fertility and weed control practices in their respective locations. All seed was treated with a fungicidal seed treatment prior to planting. No subsequent fungicides or insecticides were used. 30 Fourteen traits were measured on each plot. A list of those traits and the methods used to measure them are presented in table 1. Each trait was analyzed separately in each population using the general linear model procedure in the SAS software package (The SAS Institute, Cary, NC). Environment was considered a fixed effect and genotype was considered a random effect. Type III sum of squares were used to test significance of the terms in the model. Least square means of RILs were calculated on a location basis for subsequent use in determining Pearson productmoment correlation coefficients and for QTL mapping. Heritabilities for each trait were calculated across locations on a plot mean basis using the sum of squares from the ANOVA output as outlined by Bernardo (2002). 3.3. Linkage and QTL Mapping Each population was screened with one STS (orw5), 123 SSR, and 6,500 DArT markers. Markers that were polymorphic were used with the phenotypic marker for the awn repressor gene, B1, to create genetic linkage maps. The regression mapping algorithm in JoinMap 4.0 was used to generate linkage maps (Van Ooijen and Voorrips, 2006). Large clusters of markers were replaced with “delegate” markers to keep from exceeding resolution power and causing unreliable mapping (Korol et al., 2009). 31 Table 1 Measured traits. Grain Fill Duration Height Ripening minus Flowering Distance from ground to top of an average spike in the plot. Measured no earlier than two weeks before physiological maturity. Yield Weight of grain harvest in a plot divided by area of a plot. Test Weight Sample of grain from a plot analyzed with an automated test weight machine (model GAC 2100b, Dickey-John, St. Louis, MO) Grain Protein Sample of grain from a plot analyzed using NIR-spectroscopy (model InfratecTM 1241 Gain Analyzer, Foss, Laurel, MD) Spikes / m2 Measured from a 0.5 meter section of row at Corvallis and two 0.5 meter sections at Pendleton. Fertile Spikelets / Spike The average of 10 randomly chosen spikes in a plot. Sterile Spikelets / Spike The average of the same 10 randomly chosen spikes in a plot. The 10 randomly chosen spikes were threshed, the seed counted, and divided by the total number of fertile spikelets on those spikes. Seeds / Fertile Spikelet Seeds / Spike The 10 randomly chosen spikes were threshed, the seed counted, and divided by 10. Seed Weight The seed from the 10 randomly chosen spikes was weighed and divided by the number of seeds counted. "GDD" stands for Celsius growing degree days. [----Spike Fertility----] GDD from planting to 50% of flag leaves have senesced (physiological maturity). [-----------Spike Morphology Traits-----------] Ripening Trait Categories [Maturity Traits] Method of Measurement GDD from planting to 50% of spikes have extruded anthers. [---------------------Yield Components---------------------] Trait Flowering 32 Linkage groups were assigned to their appropriate chromosome based on marker locations documented at the public source website Grain Genes 2.0 (http://wheat.pw.usda.gov/GG2). Multiple linkage groups that were attributed to the same chromosome were joined on a single linkage group by relaxing criterion for joining if possible. QTL mapping was conducted in Windows QTL Cartographer using the composite interval mapping procedure (Wang et al., 2010). Each location was analyzed separately using the least square means of the RILs. Covariates were selected using forward-reverse regression with a probability of 0.1 for adding to and removing from the model. Covariates were excluded if they were within 10 cM of the test site to prevent elimination of the QTL signal at that site. The significance threshold for declaring a QTL was set to 0.05 using 1000 permutations. QTLs were scanned for automatically with the requirement that they are at least 5 cM apart and there is at least a 1 LOD drop between peak and trough. QTLs that appeared to be detected due to incorrectly ordered loci in the genetic map were removed. 3.4. Factor Analysis Factor analysis was performed on the spike morphology traits (Table 1) in the TxN population using the factor procedure in the SAS software package (The SAS 33 Institute, Cary, NC). Each location was analyzed separately. The principal component method was used to extract factors from the correlation matrix. The number of factors retained was determined by looking at correlations between factors and grain yield, test weight, and grain protein. The smallest number of factors possible was chosen such that a factor with a significant correlation with grain yield, test weight, or grain protein was not discarded. Extracted factors were rotated with the varimax function to aid in interpretation. Scoring coefficients were calculated for each factor and used to determine factor scores for the RILs. These factor scores were used for QTL mapping. QTL mapping of factor scores was performed using the same methods as QTL mapping of the original traits. 34 4. RESULTS AND DISCUSSION The TxN RILs showed no marker loci with more than two alleles, so all 280 lines in the population were considered to have come from a single true population (results not shown). Three alleles were present at some marker loci in the ExT RILs. The segregation pattern of those alleles suggested there were two populations with a common Einstein parent and different Tubbs parents in this cross (results not shown). RILs from this cross were divided into two populations, ExT1 and ExT2. ExT1 included 153 RILs and ExT2 included 87 RILs. The remaining 36 lines were not analyzed due to lack of sufficient marker data to assign them to a population, or they had alleles that appeared to come from two different Tubbs parents at a locus. The latter occurrence could be an indication of out-crossing in this population. Lines lacking sufficient seed for the field trial were included in linkage mapping and not QTL mapping. This brought the total lines for QTL mapping to 271, 142, and 81 in the TxN, ExT1, and ExT2 populations respectively. The accuracy of population assignments is critical to the resulting linkage and QTL mapping procedures. Individuals incorrectly assigned to populations, could generate outliers that bias linkage and QTL maps. For this reason, all results obtained from these populations must be interpreted with caution. This is particularly the case for those from the ExT populations, because a high number of lines couldn't be 35 assigned to a population. Further examination of codominate markers in these lines is needed to split them into their appropriate populations. This would increase the sizes of these populations and add statistical power to the subsequent linkage and QTL mappings. The range of phenotypic values for RILs in each population was broad and transgressive segregates were present for all traits (Tables 2, 3, and 4). The broad range of these values should give good statistical power to detect QTLs, if the complexity of the trait is low. The presence of transgressive segregates indicates that QTLs with positive contributions to these traits are present in both parents or epistatic interactions between QTLs exist. The majority of traits showed significant GxE interactions (Table 5). The genotype term was significant with a probability less than 0.001 for all traits and in all populations except for grain fill duration in the ExT2 population which has a p-value of 0.019 (data not shown). A large number of degrees of freedom were used to test these terms, so significant results don’t necessarily indicate the presence of a meaningful effect. Correlations between locations and estimates of heritability may give better indications of meaningful GxE interactions (Table 5). For example, plant height showed significant or suggestive GxE interactions in all populations, but the correlations between locations (0.82-0.96) and heritability estimates (0.89-0.97) were high in those populations. This indicates that the GxE interactions are probably not very meaningful compared to the simple effect of genotype. 36 Table 2 Least square means for parents and recombinate inbred lines (RILs) in the Tubbs x NSA 98-01995 population (TxN). Trait Parents NSA 98-0995 Tubbs Corvallis Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) 1610 2200 590 94 74.6 10.4 8.3 Spikes / m2 289 22.4 1.2 2.9 43 66 Fertile Spikelets / Spike Sterile Spikelets / Spike Seeds / Fertile Spikelet Seed Weight (mg) Seeds / Spike Range RILs Mean Std. Err. 1589 2217 628 113 74.1 9.9 8.3 1541-1681 2173-2347 554-701 75-140 67.5-78.3 8.5-14.7 4.4-9.6 1600 2215 615 100 73.7 10.5 7.8 8 20 20 3 0.4 0.6 0.3 339 19.1 2.7 2.9 49 56 217-449 17.1-25.2 0.4-3.6 2.2-3.6 33-57 42-77 321 20.9 1.6 2.9 46 61 35 0.5 0.2 0.1 2 3 1403-1538 2017-2249 556-739 63-108 67.1-77.5 7.6-12.7 3.2-6.9 1458 2126 669 83 73.2 9.6 5.3 12 22 20 3 0.7 0.6 0.4 Pendleton Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) Spikes / m2 1469 2127 659 77 73.1 9.4 5.5 1448 2099 651 94 74.6 8.9 6.0 369 415 276-526 397 44 Fertile Spikelets / Spike 21.4 16.8 15.1-21.8 18.9 0.5 Sterile Spikelets / Spike 1.3 3.6 0.6-4.1 2.0 0.3 Seeds / Fertile Spikelet 2.6 2.8 2.1-3.2 2.7 0.2 Seed Weight (mg) 37 43 32-52 40 1 Seeds / Spike 55 47 38-64 50 4 "Std. Err." refers to the standard error of a RIL least square mean assuming no missing data. "GDD" refers to Celsius growing degree days. 37 Table 3 Least square means for parents and recombinate inbred lines (RILs) in the larger Einstein x Tubbs population (ExT1). Trait Parents Einstein Tubbs Corvallis Range Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) 1580 2219 639 86 74.3 10.3 9.0 1591 2227 637 112 75.2 10.1 8.7 1541-1690 2173-2457 575-776 58-160 70.7-80.1 9.3-15.1 3.3-9.8 1602 2247 645 100 75.9 11.1 7.8 8 16 17 4 0.4 0.5 0.3 Spikes / m2 322 21.2 1.9 3.1 47 66 315 19.6 2.5 3.0 48 59 228-472 17.3-24.5 0.9-4 1.4-3.5 35-58 31-75 329 20.8 2.4 2.7 46 57 36 0.6 0.3 0.2 1 4 1412-1582 2004-2317 584-795 48-123 69.4-78.3 7.5-13.7 1.6-6.6 1475 2163 688 81 74.5 9.2 4.9 14 30 29 3 0.4 0.5 0.5 Fertile Spikelets / Spike Sterile Spikelets / Spike Seeds / Fertile Spikelet Seed Weight (mg) Seeds / Spike ExT1 RILs Mean Std. Err. Pendleton Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) Spikes / m2 1484 2140 656 68 73.3 8.4 5.2 1455 2117 662 91 75.1 8.2 5.5 351 356 223-462 330 42 Fertile Spikelets / Spike 20.4 16.9 15.6-22.3 18.8 0.6 Sterile Spikelets / Spike 2.5 3.6 1.3-4.8 2.8 0.4 Seeds / Fertile Spikelet 2.5 2.8 0.9-3.2 2.5 0.2 Seed Weight (mg) 39 43 32-46 39 1 Seeds / Spike 51 47 18-63 48 3 "Std. Err." refers to the standard error of a RIL least square mean assuming no missing data. "GDD" refers to Celsius growing degree days. 38 Table 4 Least square means for parents and recombinate inbred lines (RILs) in the smaller Einstein x Tubbs population (ExT2). Trait Parents Einstein Tubbs Corvallis Range Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) 1580 2219 639 86 74.3 10.3 9.0 1591 2227 637 112 75.2 10.1 8.7 1561-1713 2173-2362 534-711 65-138 70.3-78.9 8.7-11.9 5.6-9.9 1605 2239 634 103 75.0 10.5 8.4 8 16 17 3 0.5 0.6 0.4 Spikes / m2 322 21.2 1.9 3.1 47 66 315 19.6 2.5 3.0 48 59 220-492 16.5-23.3 0.9-4 2.3-4 38-58 44-83 347 20.2 2.5 2.9 47 58 36 0.7 0.4 0.2 2 4 1431-1654 2012-2317 551-725 58-118 70.3-78 7.3-11.1 3.3-6.5 1490 2164 675 85 73.9 8.6 5.1 18 36 37 3 0.6 0.5 0.5 Fertile Spikelets / Spike Sterile Spikelets / Spike Seeds / Fertile Spikelet Seed Weight (mg) Seeds / Spike ExT2 RILs Mean Std. Err. Pendleton Flowering (GDD) Ripening (GDD) Grain Fill Duration (GDD) Plant Height (cm) Test Weight (kg/hL) Grain Protein (% on dry basis) Yield (metric tons/ha) Spikes / m2 1484 2140 656 68 73.3 8.4 5.2 1455 2117 662 91 75.1 8.2 5.5 351 356 225-434 331 47 Fertile Spikelets / Spike 20.4 16.9 15.8-21.4 18.8 0.5 Sterile Spikelets / Spike 2.5 3.6 1.2-5.1 3.1 0.3 Seeds / Fertile Spikelet 2.5 2.8 1.7-3.4 2.7 0.1 Seed Weight (mg) 39 43 32-47 40 1 Seeds / Spike 51 47 32-70 50 3 "Std. Err." refers to the standard error of a RIL least square mean assuming no missing data. "GDD" refers to Celsius growing degree days. *** * * ns *** ** *** Flowering Ripening Grain Fill Duration Plant Height Test Weight Grain Protein Yield 0.72*** 0.60*** 0.38*** 0.82*** 0.74*** 0.29*** 0.45*** 0.98 0.89 0.80 0.93 0.92 0.71 0.93 Correlation R2 2 0.84 0.75 0.54 0.89 0.85 0.44 0.60 h *** *** ** *** *** *** *** GxE 0.72*** 0.61*** 0.31*** 0.95*** 0.83*** 0.55*** 0.58*** 0.98 0.88 0.76 0.97 0.96 0.88 0.95 Correlation R2 0.82 0.73 0.45 0.96 0.90 0.71 0.72 2 h Larger Einstein x Tubbs Population (ExT1) ** ns ns * *** ns ** GxE 0.64*** 0.58*** 0.12 0.96*** 0.77*** 0.26* 0.54*** 0.96 0.80 0.65 0.97 0.93 0.83 0.95 Correlation R2 0.78 0.74 0.28 0.97 0.87 0.52 0.69 2 h Smaller Einstein x Tubbs Population (ExT2) Spikes / m ns 0.28*** 0.69 0.44 ns 0.32*** 0.65 0.45 ns 0.24* 0.67 0.47 Fertile Spikelets / Spike *** 0.69*** 0.90 0.80 ** 0.76*** 0.90 0.85 ns 0.76*** 0.87 0.87 Sterile Spikelets / Spike ** 0.65*** 0.81 0.79 ** 0.60*** 0.81 0.75 ** 0.65*** 0.84 0.78 Seeds / Fertile Spikelet *** 0.43*** 0.78 0.60 *** 0.48*** 0.85 0.68 ns 0.58*** 0.80 0.74 Seed Weight *** 0.67*** 0.91 0.78 *** 0.73*** 0.94 0.82 ns 0.60*** 0.92 0.70 Seeds / Spike *** 0.51*** 0.84 0.67 *** 0.45*** 0.88 0.63 *** 0.53*** 0.82 0.78 "GxE" is the probability of a genotype by environment interaction from the ANOVA. *, **, and *** represent 0.05, 0.01, and 0.001 significance levels, respectively. "ns" stands for not significant. "Correlation" is the Pearson product-moment correlations between RIL means at Pendleton and Corvallis. "R2" is the coefficient of determination from the ANOVA. "h2" is the across location narrow sense heritability estimates for the RILs on a plot mean basis. 2 GxE Trait Tubbs x NSA 98-0995 Population (TxN) Table 5 Summary of across location analyzes for the three populations of recombinate inbred lines (RILs). 39 40 Under these conditions, QTLs detected at one location should have a high degree of correspondence with QTLs detected at the other location. Low correlations and heritability estimates with a lack of a significant GxE interaction indicates that a trait was measured with low precision. A low coefficient of determination also indicates this (Table 5). Spikes per m2 is an examples of such a trait. QTL mapping for these traits is unreliable due to a lack of statistical power. The relatively low heritabilties and coefficients of determination for grain protein are likely due to environmental variability within each test location. Correlations between traits are presented in tables 6, 7, and 8 for the TxN, ExT1, and ExT2 populations respectively. The relationships between these traits may not be strictly linear, so the correlation coefficients won’t accurately represent the relatedness between these traits. That is because correlation coefficients make the assumption that traits are linearly related. Even if the relationship is linear, the simple correlations between traits may not fully represent relatedness between the traits (Fonseca and Patterson, 1968). The relationship between height and yield in the ExT populations does not appear to be linear. Biplots of the traits suggest an increase in yield as height increase until the highest values of height (results not shown). At these higher values, there appears to be a decrease in yield. Thus, the height to yield correlations in the ExT populations can be misleading. -0.23*** 0.12* -0.24*** Height Test Weight Grain Protein Yield -0.17** 0.01 -0.22*** 0.11 Sterile Spikelets / Spike Seeds / Fertile Spikelet Seed Weight Seeds / Spike 0.18** -0.24*** 0.11 -0.16** 0.18** -0.09 -0.13* 0.21*** -0.10 0.11 0.72*** 0.67*** 0.13* -0.08 0.12* -0.04 0.06 -0.00 0.04 0.15* 0.07 0.19** 0.68*** -0.09 -0.09 0.23*** -0.10 0.22*** -0.00 0.01 0.17** 0.03 0.06 0.24*** 0.10 -0.11 Height *, **, and *** represent 0.05, 0.01, and 0.001 significance levels, respectively 0.19** Spikes / m Fertile Spikelets / Spike -0.16* -0.09 Grain Fill Duration 2 0.58*** -0.13* Ripening Flowering Flowering Ripening Grain Fill Duration -0.04 0.07 0.06 0.25*** -0.15* -0.13* -0.14* 0.30*** 0.29*** 0.13* -0.16** -0.35*** Test Weight -0.10 -0.01 -0.00 0.03 -0.18** -0.03 -0.20** 0.33*** 0.03 0.30*** 0.16** -0.09 Grain Protein 0.25*** 0.16** 0.21*** 0.04 0.15* 0.13* -0.19** 0.02 0.35*** 0.09 -0.06 -0.17** Yield -0.20*** -0.22*** -0.17** -0.13* -0.13* 0.05 0.15* 0.05 -0.08 0.11 0.06 -0.03 m 2 Spikes / 0.60*** -0.09 0.08 -0.40*** -0.11 0.09 -0.12 -0.22*** 0.01 0.09 0.35*** 0.39*** -0.39*** 0.40*** -0.22*** -0.15* -0.07 -0.14* -0.14* 0.14* 0.11 -0.10 0.03 0.14* 0.85*** -0.19** -0.29*** -0.03 -0.22*** 0.23*** -0.24*** -0.10 0.02 -0.09 -0.24*** -0.24*** Fertile Sterile Seeds / Spikelets / Spikelets / Fertile Spike Spike Spikelet -0.20*** -0.13* 0.10 -0.33*** -0.20*** 0.18** 0.18** 0.34*** 0.19** -0.04 -0.25*** -0.30*** Seed Weight -0.30*** 0.80*** -0.33*** 0.57*** -0.24*** 0.24*** -0.27*** -0.22*** 0.01 -0.02 0.00 0.02 Seeds / Spike Table 6 Pearson product-moment correlations for recombinate inbred lines in the Tubbs x NSA 98-0995 population (TxN). Corvallis correlations are above the diagonal and Pendleton correlations are below the diagonal. 41 -0.11 -0.35*** Test Weight Yield -0.22** Seeds / Spike -0.19* -0.04 -0.24** -0.20* 0.06 0.42*** -0.02 -0.37*** -0.25** -0.43*** 0.83*** 0.70*** -0.09 -0.07 -0.12 -0.10 0.03 0.32*** 0.01 -0.24** -0.23** -0.31*** 0.63*** -0.11 0.03 0.28*** 0.18* 0.30*** -0.25** -0.26** -0.16 0.37*** 0.41*** -0.28*** -0.38*** -0.23** Height *, **, and *** represent 0.05, 0.01, and 0.001 significance levels, respectively -0.25** 0.01 Seed Weight Sterile Spikelets / Spike Seeds / Fertile Spikelet 0.07 -0.23** Fertile Spikelets / Spike 0.33*** Grain Protein -0.05 -0.34*** Height 2 0.11 Grain Fill Duration Spikes / m 0.64*** Ripening Flowering Flowering Ripening Grain Fill Duration -0.32*** 0.16 -0.21* 0.15 -0.20* 0.24** -0.19* -0.16 0.58*** -0.09 -0.18* -0.15 Test Weight 0.49*** 0.05 0.53*** 0.22** -0.06 -0.55*** 0.29*** 0.16 0.41** -0.09 -0.38*** -0.41*** Yield 0.04 -0.31*** 0.07 -0.03 -0.06 -0.19* 0.09 0.03 -0.08 0.13 0.01 -0.11 m 2 Spikes / -0.48*** 0.04 -0.50*** -0.11 0.03 -0.04 -0.49*** 0.26** -0.07 0.38*** 0.41*** 0.18* Grain Protein 0.24** -0.09 -0.26** -0.28*** -0.03 -0.20* 0.04 -0.24** -0.08 0.11 0.09 0.01 -0.27** 0.41*** -0.13 -0.25** -0.12 0.06 0.09 0.36*** 0.32*** -0.08 -0.02 0.04 0.86*** -0.25** -0.18* -0.14 -0.48*** -0.08 0.58*** -0.10 0.14 -0.20* -0.46*** -0.40*** Fertile Sterile Seeds / Spikelets / Spikelets / Fertile Spike Spike Spikelet -0.30*** -0.14 0.22** -0.11 0.07 -0.34*** 0.01 0.27*** 0.37*** -0.25** -0.09 0.11 Seed Weight -0.17* 0.84*** -0.29*** 0.42*** -0.48*** -0.19* 0.56*** -0.22** 0.09 -0.14 -0.38*** -0.37*** Seeds / Spike Table 7 Pearson product-moment correlations for recombinate inbred lines in the larger Einstein x Tubbs population (ExT1). Corvallis correlations are above the diagonal and Pendleton correlations are below the diagonal. 42 -0.37*** -0.15 -0.40*** Height Test Weight Yield 0.14 0.00 -0.08 0.27* 0.19 -0.15 -0.07 -0.15 0.05 Grain Protein Fertile Spikelets / Spike Sterile Spikelets / Spike Seeds / Fertile Spikelet Seed Weight Seeds / Spike -0.16 0.09 0.08 0.08 0.02 0.05 -0.10 -0.20 -0.07 -0.10 0.06 0.64*** -0.20 0.21 -0.09 0.30** -0.17 0.12 -0.12 0.22 0.46*** -0.04 -0.26* -0.29** Height *, **, and *** represent 0.05, 0.01, and 0.001 significance levels, respectively 0.12 -0.11 0.22 -0.20 -0.39*** -0.21 -0.25* 0.64*** 0.66*** -0.05 2 -0.20 Grain Fill Duration Spikes / m 0.61*** Ripening Flowering Flowering Ripening Grain Fill Duration -0.25* 0.26* -0.22 0.27* -0.12 0.48*** -0.13 -0.02 0.64*** 0.05 -0.22 -0.33** Test Weight 0.25* 0.02 0.34** 0.05 -0.06 -0.28* 0.36*** 0.07 0.09 0.28* -0.00 -0.28* Yield 2 -0.10 -0.04 0.01 0.01 -0.21 -0.13 0.19 -0.10 -0.06 0.19 0.11 -0.04 m Spikes / -0.26* 0.07 -0.34** 0.06 0.03 -0.01 -0.08 0.37*** 0.26* 0.37*** 0.24* -0.05 Grain Protein 0.51*** -0.40*** -0.03 -0.45*** 0.04 -0.11 -0.17 -0.16 -0.09 0.18 0.18 0.06 -0.45*** 0.24* -0.25* -0.32** 0.26* 0.10 0.06 0.37*** 0.28* 0.08 0.02 -0.05 0.84*** -0.07 -0.12 -0.29** -0.24* -0.13 0.35** -0.23* -0.05 -0.16 -0.22* -0.13 Fertile Sterile Seeds / Spikelets / Spikelets / Fertile Spike Spike Spikelet -0.28* 0.08 0.06 -0.24* -0.14 -0.34** 0.22 0.26* 0.45*** -0.11 -0.13 -0.06 Seed Weight Table 8 Pearson product-moment correlations for recombinate inbred lines in the smaller Einstein x Tubbs population (ExT2). Corvallis correlations are above the diagonal and Pendleton correlations are below the diagonal. -0.09 0.74*** -0.33** 0.41*** -0.20 -0.22 0.21 -0.33** -0.12 -0.02 -0.08 -0.09 Seeds / Spike 43 44 All other traits appear to be at least close to linearly related over the ranges measured (not shown). However, it should not be assumed that these relationships will occur beyond the ranges measured. The correlations between the spike fertility traits, seeds per fertile spikelet and seeds per spike, were consistently the strongest across all locations and populations. Mathematically, fertile spikelets per spike multiplied by seeds per fertile spikelet equals seeds per spike. Thus, it is expected that the spike fertility traits are under vary similar genetic control. The correlations between other traits depended to a large degree on the population and the location where they were measured. Thus, there may be different genes segregating in the different populations and/or the presence of gene by environment interactions. There is a lack of consistently strong correlations between yield and any of the other traits in all populations at every location (Tables 6, 7, and 8). Generally, yield is correlated with the spike fertility traits and inversely correlated with flowering. In the TxN population no trait has a correlation with yield stronger than 0.35. However, correlations greater than 0.5 for the spike fertility traits with yield are present in the ExT1 population. This lack of consistently strong correlations makes identifying traits to manipulate for increased yield difficult. Ultimately, selection of QTLs for these traits will require considerable knowledge of the genetic backgrounds that they are in. 45 4.1. Genetic Linkage Maps The TxN population mapped 373 markers on 21 linkage groups. This map covered 1387.6 cM, 1245.5 cM and 1163 cM for the A, B, and D genomes respectively. The ExT1 population mapped 353 markers on 22 linkage groups covering 1318.6 cM, 1552.5 cM, and 1444.7 cM for the A, B, and D genomes. The ExT2 population mapped 358 markers on 22 linkage groups covering 1548.9 cM, 1423.9 cM, and 955.2 cM for the three genomes. All chromosomes were represented in each population. Relaxing criterion for merging linkage groups from the same chromosome resulted in only two gaps in all three maps. However, there were 57 marker intervals that were greater than 50 cM. Seven of those intervals were over 100 cM. Any QTLs detected in these intervals need to be interpreted with care, because the markers are nearly unlinked at these distances. 4.1. QTL Mapping Multiple QTLs were detected for all traits for a total of 146 QTLs (Tables 9, 10, 11, 12, and 13). Grain protein (Table 9), seed weight (Table 13), and spikes per m2 (Table 9) had at least one population that failed to identify QTLs for that trait. 46 Table 9 QTLs for yield, grain protein, test weight, and spikes per m2 Trait Yield Grain Protein Test Weight 2 Spikes / m Pop. Chrom. Loc. ExT1 4D Corv 7A Corv ExT2 2B Pend TxN 2B Pend ExT2 3D Pend 6B Pend TxN 4A Corv ExT1 4A Corv 4A Pend 4B Corv 5A-2 Corv 5B Corv 6B Corv ExT2 4D Corv 5A Pend TxN 5A Corv 5A Pend 5A Pend 6B Pend 7D Pend Nearest Marker wPt-0472cluster wPt-0031 wPt-2110 wPt-2327cluster wPt-6066 381509cluster wmc617 wPt-4544 wPt-1007cluster barc90cluster wPt-7061 348314cluster wPt-6441 wPt-3058 gwm291 B1 barc330 B1 barc79cluster cfd14 Position LOD (cM) Score Add. E. 20.8 3.296 0.31682 20.5 4.84 -0.3644 184.1 3.387 0.2889 90.9 4.342 0.17337 114 5.012 0.398 48.7 3.179 -0.2728 14.9 3.188 -0.2622 93.5 3.877 1.14463 151.7 6.197 0.72838 138.9 4.054 -0.58725 4.2 3.64 0.57225 74.6 3.588 0.51 216 3.623 1.13775 0 4.686 0.815 155.3 3.669 1.24788 136.4 3.356 0.41863 42.2 3.622 0.47363 134.4 7.617 0.63588 80.1 4.932 0.49213 170.3 3.882 -0.631 R2 0.1 0.13 0.16 0.07 0.23 0.12 0.08 0.28 0.14 0.08 0.08 0.07 0.31 0.15 0.18 0.05 0.06 0.11 0.06 0.1 ExT2 3A Corv wPt-0714 184.8 3.743 23.7785 0.15 3D Pend gdm72 95.2 4.952 25.5167 0.24 4B Corv barc90cluster 150.4 3.315 -21.45 0.12 5D-1 Corv wPt-1197 89.5 3.749 34.8061 0.34 7A Pend wPt-3425 251.1 4.144 -28.7746 0.18 TxN 1A Corv wmc278 96.1 5.102 13.3076 0.09 1A Pend wPt-4765cluster 116 6.092 24.3792 0.28 "Pop." refers to mapping population. "TxN" refers to Tubbs x NSA 98-0995 population. "ExT1" and "ExT2" refer to the large and small Einstein by Tubbs populations respectively. "Chom." is chromosome. "Loc." is location. "Add. E." is the additive effect for replacing an allele from a Nickerson parent with an allele from Tubbs. "R2" is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. 47 Table 10 QTLs for flowering, ripening, and grain fill duration. Position LOD Score Add. E. R2 Pop. Chrom. Loc. Nearest Marker (cM) ExT1 1B Corv wPt-6690 104.9 3.48 8.6361 0.07 3A Corv tPt-1143 166.8 4.897 11.9123 0.12 3A Pend tPt-1143 164.8 7.312 12.9231 0.18 4D Corv wPt-0472cluster 20.8 5.12 -11.3638 0.13 5B Corv barc4cluster 56.7 5.989 -12.2117 0.13 ExT2 5A Pend wPt-4419 56.6 2.799 -11.0962 0.11 TxN 5B Corv wPt-1895cluster 122.7 5.396 -7.4737 0.08 5B Pend wPt-1895cluster 122.7 7.742 -11.4246 0.11 7A Corv wPt-1928 99.1 7.018 -8.4414 0.1 Ripening ExT1 1B Corv wPt-6690 104.3 4.751 12.7814 0.09 3A Corv gwm666 168.8 3.957 13.5863 0.1 3B Corv 381874cluster 154.6 4.153 11.5948 0.08 ExT2 4B Corv tPt-0602 154.8 3.905 -14.7623 0.12 4B Pend gwm251 158.8 4.106 -19.7188 0.18 4D Corv wPt-3058 0 4.628 -15.0344 0.14 6B Corv barc101cluster 55.8 3.233 11.748 0.09 TxN 4A Corv wPt-7924 66.9 3.473 13.4196 0.14 4A Pend wPt-7924 62.9 3.853 15.0062 0.16 5B Corv 303931cluster 119.2 4.501 -12.0272 0.08 5B Corv wPt-9467 77.8 4.581 14.0095 0.07 6A Pend wPt-7063 74.7 3.857 9.3901 0.06 Grain Fill Duration ExT1 1A Pend wPt-3904 31 5.129 16.0089 0.14 ExT2 1B Pend barc8cluster 35.1 3.459 15.7915 0.15 4B Pend gwm251 161.2 3.746 -15.1368 0.16 5B Corv wPt-1881 100.1 4.277 -11.3228 0.15 TxN 2A Corv gwm312 145.5 4.635 7.2015 0.07 2B Corv wPt-8760 211.1 3.711 6.1693 0.05 3B Pend wPt-3107 110.3 5.293 9.4677 0.1 5B Corv 311648cluster 248.8 3.167 5.776 0.04 7D Pend cfd14 166 4.17 -9.2513 0.09 "Pop." refers to mapping population. "TxN" refers to Tubbs x NSA 98-0995 population. "ExT1" and "ExT2" refer to the large and small Einstein by Tubbs populations respectively. "Chom." is chromosome. "Loc." is location. "Add. E." is the additive effect for replacing an allele from a Nickerson parent with an allele from Tubbs. "R2" is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. Trait Flowering 48 Table 11 QTLs for plant height and seeds per spike. Position LOD Score Add. E. R2 Pop. Chrom. Loc. Nearest Marker (cM) ExT1 1D Pend barc229cluster 66 3.42 3.5724 0.05 2A Pend wPt-7024 212.8 3.182 3.4297 0.04 4B Corv barc20cluster 143 15.44 -11.6664 0.27 4B Pend barc20cluster 143.6 17 -9.6777 0.31 4D Corv wPt-0472cluster 20.8 24.08 16.2917 0.52 4D Pend wPt-0472cluster 18.8 26.89 13.904 0.64 5A-1 Corv wPt-4419 102.4 3.483 4.4523 0.05 ExT2 2B Corv wmc175 234 5.241 6.8583 0.13 2B Pend wmc175 234 5.437 5.6995 0.13 4B Corv barc20cluster 146.2 8.395 -9.3857 0.2 4B Pend barc20cluster 146.2 7.61 -7.1513 0.18 4D Corv wPt-0472cluster 14.7 9.64 11.3276 0.3 4D Pend wPt-0472cluster 14.7 8.467 9.0307 0.29 7A Corv wPt-0961cluster 243.8 5.826 6.9774 0.15 7A Pend wPt-0961cluster 245.2 6.142 5.4881 0.14 7B Corv tPt-8569cluster 26.2 4.315 5.7242 0.1 TxN 2A Pend gwm515 98.2 3.759 2.0655 0.09 4B Corv gwm513 36.2 3.868 -2.0761 0.06 4B Pend gwm513 36.2 6.203 -2.1745 0.1 5A Corv barc330 40.2 5.992 2.6729 0.1 5A Pend barc330 38.2 4.531 1.9373 0.08 5B Pend 305092cluster 124.2 4.159 1.6379 0.06 Seeds per Spike ExT1 2A Corv wPt-1142cluster 171.8 6.066 -3.2037 0.15 3B Corv wPt-3041 7.7 5.428 3.4932 0.18 5A-1 Corv barc186 56.2 3.298 2.498 0.09 ExT2 3A Pend wPt-3697cluster 73.4 3.015 2.4179 0.11 4A Pend wPt-2301 199.5 3.142 -2.2382 0.1 4B Pend wPt-0391 179.6 6.654 4.3063 0.39 TxN 2A Corv gwm372cluster 110.7 12.37 -2.8105 0.18 2A Pend wPt-1142cluster 115.8 11.01 -2.1352 0.17 4A Corv rPt-2478cluster 116 4.39 1.5737 0.05 5B Corv 310624 71.3 3.078 -1.298 0.04 "Pop." refers to mapping population. "TxN" refers to Tubbs x NSA 98-0995 population. "ExT1" and "ExT2" refer to the large and small Einstein by Tubbs populations respectively. "Chom." is chromosome. "Loc." is location. "Add. E." is the additive effect for replacing an allele from a Nickerson parent with an allele from Tubbs. "R2" is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. Trait Plant Height 49 Table 12 QTLs for fertile spikelets per spike and sterile spikelets per spike. Position LOD Score Add. E. R2 Pop. Chrom. Loc. Nearest Marker (cM) ExT1 2A Corv gwm372cluster 175.2 6.7 -0.5348 0.11 2A Pend wPt-1142cluster 173.8 6.864 -0.4372 0.12 4A Corv wPt-6757 55.5 5.307 -0.473 0.08 4B Pend gwm149 5.8 3.54 -0.413 0.09 5A-2 Pend wPt-1200 0 3.591 -0.3091 0.06 7A Corv wPt-5987 190.5 16.26 0.8717 0.29 7A Pend wPt-5987 191.5 14.12 0.6934 0.29 7B Corv gwm111 136.8 6.445 -0.5216 0.1 ExT2 5A Corv gwm666 16.3 5.252 -0.7029 0.2 7A Corv wPt-5987 225.8 13.3 1.01 0.4 7B Corv gwm111 83.2 4.237 -0.5263 0.11 TxN 2A Corv 348413cluster 117.8 9.019 -0.4952 0.13 2A Pend gwm95 108.4 8.312 -0.363 0.12 3B Corv wPt-0280cluster 179.8 3.198 0.2744 0.04 4B Pend gwm251 41.5 3.925 -0.2389 0.05 5A Pend B1 136.4 4.573 -0.2656 0.06 5B Corv wPt-2273cluster 93 4.018 -0.3364 0.06 5B Pend wPt-2273cluster 90.1 4.184 -0.2404 0.05 Sterile Spikelets ExT1 2A Pend wPt-0094cluster 205.5 4.108 0.2084 0.09 per Spike 5A-2 Corv wPt-7061 4.2 5.097 0.2326 0.14 5A-2 Pend wPt-7061 4.2 7.46 0.3165 0.2 ExT2 2D Pend wPt-9580 5.9 5.248 0.3206 0.14 3A Pend wmc11 214.4 3.959 -0.2741 0.11 4B Corv rPt-6847 167.6 5.42 -0.2985 0.21 4B Pend rPt-6847 171.6 5.514 -0.4274 0.25 5A Corv B1 156.7 6.631 0.2995 0.23 5A Pend B1 156.7 6.206 0.3669 0.19 TxN 2D Corv cfd51cluster 8.2 5.667 -0.1537 0.08 2D Pend gwm296 2.2 3.797 -0.1414 0.05 4D Corv wmc473cluster 11 7.313 0.1861 0.11 4D Pend wmc473cluster 13 10.78 0.2503 0.17 5A Corv B1 134.4 11.01 0.2221 0.17 5A Pend B1 134.4 9.663 0.2097 0.12 "Pop." refers to mapping population. "TxN" refers to Tubbs x NSA 98-0995 population. "ExT1" and "ExT2" refer to the large and small Einstein by Tubbs populations respectively. "Chom." is chromosome. "Loc." is location. "Add. E." is the additive effect for replacing an allele from a Nickerson parent with an allele from Tubbs. "R2" is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. Trait Fertile Spikelets per Spike 50 Table 13 QTLs for seeds per fertile spikelet and seed weight. Position LOD Score Add. E. R2 Pop. Chrom. Loc. Nearest Marker (cM) ExT1 3B Corv wPt-3041 11.7 6.021 0.1531 0.17 4A Pend wPt-1007cluster 153.7 4.725 -0.1164 0.12 5A-1 Corv barc186 56.2 3.212 0.1082 0.09 ExT2 4A Pend wPt-6900 198.3 5.252 -0.129 0.17 4B Pend wPt-0391 179.6 3.925 0.1443 0.21 6A Corv tPt-6278 135.3 3.269 -0.1058 0.12 6A Pend tPt-6278 135.3 3.254 -0.1005 0.1 TxN 2A Corv gwm372cluster 110.7 3.268 -0.0609 0.06 2A Pend wPt-1142cluster 112.7 3.823 -0.053 0.06 3A Pend gwm2 161.9 3.864 -0.0604 0.07 5A Pend wPt-4203cluster 138.4 4.213 0.0553 0.06 Seed Weight ExT1 1A Pend barc83cluster 58.8 3.451 -0.8668 0.08 5A-2 Pend wPt-7061 2.2 3.416 0.822 0.07 7A Corv gwm332 202.4 5.306 -1.7144 0.17 7B Corv wPt-1266 132.6 4.423 1.3819 0.11 7B Pend wPt-4258cluster 128.2 6.272 1.1377 0.14 TxN 2B Corv wPt-4417cluster 115.7 3.356 0.8225 0.05 4A Corv 311358cluster 98.7 7.414 -1.2428 0.1 4D Corv wmc331 15 7.699 1.5327 0.16 4D Pend wmc331 15 5.61 0.8952 0.1 5A Pend gwm291 130.4 3.487 0.5972 0.04 5B Corv wPt-3457cluster 137.2 6.937 1.5656 0.16 5B Corv barc4cluster 67.5 4.122 0.8847 0.05 5B Pend wPt-3329 149.2 5.66 1.2411 0.19 "Pop." refers to mapping population. "TxN" refers to Tubbs x NSA 98-0995 population. "ExT1" and "ExT2" refer to the large and small Einstein by Tubbs populations respectively. "Chom." is chromosome. "Loc." is location. "Add. E." is the additive effect for replacing an allele from a Nickerson parent with an allele from Tubbs. "R2" is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. Trait Seeds per Fertile Spikelet 51 Significant differences existed between RILs for grain protein, seed weight and spikes per m2. Thus, the failure to detect QTLs for these traits is likely the result of a lack of statistical power. For spikes per m2, the lack of statistical power is probably the result of a lack of precision in the measurement of that trait. The relatively few (81) RILs mapped in the ExT2 population could explain the failure to detect QTLs for seed weight in that population. A smaller number of lines used in QTL mapping results in less statistical power (Zeng, 1994). It is not immediately clear why QTLs weren’t mapped for grain protein in the ExT1 population. Grain protein had higher heritability in the ExT1 population than it did in the other two populations (Table 5). Since power to detect QTLs is inversely proportional to heritability, this should have been the population that had the greatest power to detect QTLs for grain protein (Beavis, 1994). The best explanation for the failure to detect these QTLs is that genetic control of grain protein is complex or that it is more heavily influenced by environment than genetics. QTLs for a trait that occur at nearly the same position on the genetic map for both locations likely represent a single QTL that is effective across those locations (Jiang and Zeng, 1995). These QTLs are useful to breeders, because they can be selected for with minimal consideration of GxE interactions. QTLs of this type were detected for all traits except for grain fill duration, grain protein, and yield. The lack of across location QTLs detected for grain fill duration may be attributed to the high standard error of the RIL means relative to their spread (Tables 2, 3, and 4). This high 52 relative standard error indicates that the measured values for this trait are too inaccurate for consistent QTL mapping. Grain protein is highly influenced by environmental factors (Gonzalez-Hernandez et al., 2004). Failure to account for in field variability of those environmental factors could be limiting the ability to detect QTLs for grain protein. For yield, the lack of across environment QTLs is probably attributable to GxE interactions and complex genetic control of the trait. The genetic control of this trait may poorly fit the additive genetic model that is assumed by QTL analysis using CIM (Zeng, 1994). Techniques that allow for epistatic interactions, such as MIM, could have greater power to detect QTLs for yield (Kao et al., 1999). However, an overall lack of statistical power to detect sufficient quantities of QTLs to explain a meaningful percent of variation for yield will probably still exist. There are several instances of QTLs occurring on the same chromosome for a particular trait in more than one population. This may indicate that a single QTL occurs in more than one population. If this is the case, it would provide some measure of conformation for that QTL. Such an assumption should be made with great care, because of the large differences between linkage maps of different populations and the sparseness of those maps. However, these finding at least show that one chromosome is important to a trait in more than one population. Examples of this include 7A for fertile spikelets per spike in ExT1 and ExT2 populations and 2D for sterile spikelets per spike in the ExT2 and TxN populations (Table 12). Finer mapping is needed to determine if only one QTL is actually present in those populations. 53 There are four loci that show close linkage or pleiotropy with 36% of the detected QTLs. These loci are Rht-B1, Rht-D1, B1, and Xgwm372 on chromosomes 4B, 4D, 5A, and 2A respectively. The large numbers of QTLs found at these loci indicates that they are strong determinants of the variability present in these populations and further examination is warranted. Rht-B1 and Rht-D1 are the loci for the two major dwarfing genes in these populations. Since the ExT populations are segregating for dwarfing alleles at Rht-B1 and Rht-D1, the strong QTLs for height on 4B and 4D can be explained by the dwarfing genes (Table 11). The TxN population is fixed at these loci, so the QTL for height on 4B in that population represents a minor QTL for height. This QTL appears to be closed linked to Rht-B1, because its nearest marker, gwm513, maps closely to the QTLs for Rht-B1 in both ExT populations. The height QTLs account for 10 of the 28 QTLs detected in close proximity to these loci. Pleiotropy may explain the occurrence of many of the other QTLs. If the other QTLs are not due to pleiotropy, it may be possible to break unfavorable linkages between QTLs. Finer mapping of these chromosomes combined with multiple-trait QTL mapping would be able to better position the QTLs on these chromosomes and be able to distinguish between pleiotropy and close linkage (Jiang and Zeng, 1995). This is needed to determine how useful the QTLs detected at these loci are to breeders. Pleiotropic effects are probably not very useful, unless they indicate that one dwarfing gene is more favorable than the other. 54 The B1 locus is the location of the awn inhibitor gene that is segregating in all of the populations. A total of 15 QTLs showed pleiotropy or close linkage with this gene. The awned allele is associated with more sterile spikelets and fewer fertile spikelets. For sterile spikelets per spike there are QTLs at both locations for all three populations at the B1 locus (Table 12). QTLs for fertile spikelets per spike are present at Corvallis for the TxN and ExT1 populations and Pendleton for the ExT2 population near the B1 locus (Table 12). Based on QTLs detected for seed weight (Table 13) and test weight (Table 9) close to B1, it appears that awned varieties have higher seed weights and greater test weights. Laperche et al. (2007) also detected QTLs for seed weight at the B1 locus. However, they found greater seed weight for awned varieties at low soil nitrogen levels and greater seed weight for awnless varieties at high soil nitrogen levels. Thus, the effects of these QTLs appear to depend on production and environmental practices. As with the Rht-B1 and Rht-D1 loci, finer linkage mapping and multiple-trait QTL mapping can be used to find more precise positions of these QTLs and test for pleiotropic effects (Jiang and Zeng, 1995). If the QTLs prove to be pleiotropic, then it appears that there is a trade-off of number of fertile spikelets for greater seed weight when choosing awned varieties under the conditions studied. These findings indicate that selection of an awned or awnless variety is not trivial, but it is not obvious if one type is universally preferred over the other. A preference for awned wheat has been shown in studies in the Great Plains, attributed to awns the available photosynthetic 55 area of a variety (Donald, 1968). However, it has been suggested that the awnless trait makes varieties less prone to pre-harvest sprouting and thus preferable in regions prone to pre-harvest sprouting (King and Richards, 1984). Further examination is needed to identify which plant type is preferable for Oregon. Another 8 QTLs were detected on 5A in the general vicinity of Xbarc330. When combined with the QTLs detected at B1, at least one QTL was mapped on chromosome 5A for sterile spikelets per spike, fertile spikelets per spike, flowering, height, seed weight, seeds per fertile spikelet, seeds per spike, and test weight. Other researchers have also observed QTLs for yield and yield components on chromosome 5A (Kato et al., 1998). This indicates that 5A is a good candidate for further research. Important genes that have been mapped to this chromosome include Vrn-A1, a gene that controls vernalization requirement; and Rht12, a dwarfing gene that is thought to be tightly linked with B1 (Worland et al., 2006). Nothing is known about the allelic variation of these loci in the populations. Thirteen QTLs were detected near the Xgwm372 locus in the TxN and ExT1 populations. It is not immediately apparent what gene or genes are responsible for these QTLs. QTLs found near this locus include those for seeds per fertile spikelet (Table 13), seeds per spike (Table 11), and fertile spikelets per spike (Table 12). These spike fertility traits are the yield components that are most consistently correlated with yield (Tables 6, 7, and 8), so these QTLs might be useful for increasing yield. It appears that all of the favorable alleles are coming from the 56 Nickerson parent in their respective populations. Thus, it is only of minor consequence if the QTLs are pleiotropic or closely linked. Selecting for the favorable allele at the Xgwm372 locus could provide a bump to yield. However, no QTLs for yield were detected at this locus. Thus, a better understanding of the interactions with this locus and others is probably needed to maximize any potential gain. 4.2. Factor Analysis Four factors were retained for the Corvallis spike morphology traits and three factors were retained for the Pendleton traits based on significant correlations with yield, test weight, or grain protein (Table 14). This criterion for selecting the number of factors was used to guard against throwing out potentially informative factors. Selection of factors based on the proportion of variation explained can result in disregarding a factor that only explains a small portion of the total variation, but is important for explaining the economically important traits: yield, test weight, and protein. The significant correlation criterion is quite conservative, because the many degrees of freedom used to test correlations can identify correlations as significant that may not be very meaningful. 57 Table 14 Pearson product-moment correlations between initial factors and yield, grain protein, and test weight. Factor Yield Corvallis Test weight Protein F1 F2 F3 F4 F5 -0.22*** 0.04 -0.30*** -0.01 0.06 0.19** 0.20** -0.04 0.22*** -0.03 -0.28*** 0.19** 0.01 0.15* 0.09 Pendleton F1 0.16** -0.09 -0.12 F2 0.27*** -0.00 0.20*** F3 0.12* -0.15* -0.12 F4 0.01 -0.08 0.12 F5 -0.05 0.03 -0.01 *, **, and *** represent 0.05, 0.01, and 0.001 significance levels, respectively 58 After rotation, Corvallis factors three and four are essentially factors for single traits (Table 15). These traits are seed weight for factor three and sterile spikelets for factor four. Since QTL mapping was already carried out for these traits individually, these factors were not considered further. The remaining three spike morphology traits primarily loaded on the first two factors (Table 15). Factor one can be thought of as a factor for the seeds per fertile spikelet contribution to seeds per spike and factor two can be thought of as a factor for the fertile spikelets per spike contribution to seeds per spike. Using this reasoning, the QTLs detected for factor one would be expected to be the same as those for seeds per fertile spikelet. The QTLs detected for factor two would be expected to be the same as those for fertile spikelets per spike. One QTL was detected for factor one at Corvallis (Table 16) and that QTL was found at the same site as the only QTL detected for seeds per fertile spikelet at that location (Table 13). Three QTLs were detected for factor two (Table 16) and three QTLs were detected for fertile spikelets per spike (Table 12). Each had matching QTLs on 2A and 5B, but the third QTL differed in the two traits. The LOD threshold for declaring a QTL significant was 3.1 for both of these traits. On 3B, the LOD score for seeds per fertile spikelet exceeded this threshold by a score less than 0.1 LOD over and factor two was below the threshold by a score less than 0.1 LOD under (results not shown). Thus, QTL mapping of these traits at that locus was essentially the same. On chromosome 3A a significant QTL was found for factor two (Table 16), but none was found for fertile spikelets per spike (Table 12). 59 Table 15 Factor loadings for rotated spike morphology traits. fertile sterile seeds / spikelets spikelets fertile seed seeds / variance Factor / spike / spike spikelet weight spike explained Corvallis 1 2 3 4 Communuality 0.06 0.98 -0.16 -0.07 1.00 -0.16 -0.07 0.04 0.98 1.00 0.98 -0.11 -0.05 -0.14 1.00 -0.09 -0.16 0.98 0.04 1.00 0.84 0.50 -0.14 -0.15 1.00 34.40% 25.05% 20.26% 20.23% 100% Pendleton 1 0.14 -0.11 0.99 -0.11 0.87 35.42% 2 0.95 -0.52 -0.03 0.06 0.48 28.31% 3 -0.03 0.66 -0.12 0.92 -0.12 26.37% Communuality 0.93 0.73 0.99 0.86 0.99 90.11% "Communuality" represents proportion of the variation for that variable explained by the factors. 60 Table 16 QTLs for spike morphology factors. Position LOD 2 Score Add. E. R Factor Chrom. Nearest Marker (cM) Corvallis 1 2 2A 2A 3A 5B gwm372cluster 348413cluster barc346 wPt-2273cluster 110.7 117.8 145.5 93 5.391 -0.296 0.086 8.753 -0.365 0.132 3.482 0.3069 0.094 3.449 -0.23 0.051 Pendleton 1 2A wPt-1142cluster 113.8 4.616 -0.255 0.063 3A gwm2 161.9 3.27 -0.248 0.061 5A wPt-4203cluster 138.4 6.068 0.3005 0.088 2 2A gwm95 108.4 6.139 -0.296 0.087 5A B1 136.4 8.067 -0.345 0.117 1B rPt-9074 147.5 3.184 0.2203 0.047 4B gwm513 36.2 3.374 -0.221 0.047 5B 378650cluster 88.1 3.005 -0.195 0.037 6B wmc494cluster 59.7 3.071 -0.197 0.038 3 5A B1 134.4 6.618 0.2897 0.083 5B wPt-3329 149.2 5.099 0.4005 0.159 4D wmc331 15 9.329 0.3989 0.155 "Factor" corresponds to factors in table 14. "Chom." is chromosome. "Add. E." is the additive effect for replacing an allele 2 from a Nickerson parent with an allele from Tubbs. "R " is the coefficient of determination for how the QTL explains the residuals after accounting for the covariates. 61 Overall, the two Corvallis factors detected or nearly detected the same significant QTLs that were found for seeds per fertile spikelet and fertile spikelets per spike as expected. The factors also identified an additional QTL not found mapping the individual traits. These results indicate that factor analysis may have increased power to detect QTLs. However, there was a QTL for seeds per spike on 4A that didn’t show up with the factors or the other traits (Table 11). This could indicate that the factor analysis didn’t account for some of the genetic variation in seeds per spike. On the other hand, it is possible that this QTL is false. Analyzing seeds per spike for QTLs after already scanning the two traits that should account for all of its variation inflates the probability of type I error (Jiang and Zeng, 1995). It is important to know which of the QTLs detected were real and which are false positives in order to adequately rate the benefits of using the factor analysis approach. The best way to do this is to collect more years of data and compare the results of multiple years. The rotated factors for Pendleton didn’t show single trait factors like Corvallis (Table 15). Factor one can be considered a factor for the seeds per fertile spikelet contribution to seeds per spike just like factor one at Corvallis. Factor two can be considered the fertile spikelets per spike contribution to seeds per spike, but it also has a meaningful negative loading of sterile spikelets per spike. Biologically this could make sense. The number of total spikelets per spike is determined at an early growth stage and when the plant experiences stress at a later growth stage it will abort some of these spikelets (Acevedo et al., 2002). The abortion of spikelets results in sterile 62 spikelets. There is a higher proportion of sterile spikelets to fertile spikelets at Pendleton than there is at Corvallis (Table 2). This is probably explained by greater water and heat stress at Pendleton that caused the formation of sterile spikelets. It may be that lines that produced more spikelets per spike were also less likely to abort those spikelets. This reasoning is supported by the significant inverse correlation between fertile spikelets per spike and sterile spikelets per spike that was observed at Pendleton (Table 6). Factor three loaded seed weight and sterile spikelets per spike (Table 15). The biological explanation for this factor could be that lines that aborted more spikelets had relatively less seeds to act as a sink for photosynthates compared to their production of photosynthates. Thus, these lines produced larger seeds on average. For the sake of comparing the QTL mappings of the Pendleton factors to those of the single traits, factor one QTLs are compared to QTLs for seeds per fertile spikelet, factor two is compared to fertile spikelets per spike, and factor three is compared to seed weight. Factor one mapped QTLs (Table 16) that were essentially the same as those for seeds per fertile spikelet (Table 13). Factor two mapped QTLs (Table 16) that included essentially the same QTLs that were mapped for fertile spikelets per spike (Table 12). Factor two also identified QTLs on 4B and 6B that were not identified by fertile spikelets per spike. Factor three found QTLs (Table 16) that were essentially the same as those for seed weight (Table 13). Pendleton factors one and three behaved the same as their equivalent single traits. Factor two appeared to have greater power to detect QTLs than its equivalent 63 single trait. The increased power may be attributable to considering multiple traits at once with the factor scores. In particular, the inverse correlation of sterile spikelets per spike with fertile spikelets per spike may be increasing detection power in a similar way to the power increase observed in multiple-trait QTL analysis (Jiang and Zeng, 1994). There is a lack of conclusive evidence supporting using factor analysis as a method for improved QTL mapping. However, the method did find QTLs that weren’t previously detected. This provides some anecdotal evidence that the procedure has merit. Without knowing the true composition of QTLs for these traits, it cannot be determined if this is the result of increased power or simply error. Ultimately, the best way of analyzing this method is through simulation studies were the true distribution of QTLs is known. The results in this study indicate that such a simulation study should be performed. If the simulation study does show increased power and reduce error using factor analysis, the results from this method are probably more useful than those gathered using the traits individually. 64 5. CONCLUSION A large number of QTLs were detected for traits related to yield in three genetic mapping populations representative of populations that produce elite germplasm in OSU's wheat breeding program. These QTLs may eventually be useful for developing MAS procedures for lines in OSU's program. For example, selection for the favorable allele at the Xgwm372 locus can be implemented in relatively short order. This should result in wheat that has greater spike fertility, and more fertile spikelets. However, greater understanding of all of the detected QTLs and how they are interrelated is needed to maximize the effectiveness of a MAS program. This greater understanding includes finer genetic mapping to identify genetic markers that are more closely linked to the identified QTLs and are inexpensive to use. Additional years of data are also needed to expand the scope of inference for this study. More complicated analyzes could also improve the usefulness of the data collected. Multiple-trait QTL mapping can be used to distinguish between pleiotropy and close linkage of QTLs (Zeng, 1994). This would allow a breeder to determine if it is possible to break unfavorable linkages. The impact of epistasis on these traits also needs to be examined and can be accomplished using MIM (Kao et al., 1999). These two techniques would greatly enhance understanding of genetic control of the examined traits in these populations. 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Molecular Breeding 19:153-16 73 APPENDICES 74 1A gwm636 tPt-2481 wPt-5245 345256cluster barc124cluster FS/S-C S/S-P S/FS-P S/FS-C S/S-C wPt-1596cluster wPt-1888cluster gwm666 wmc169 305077cluster wPt-2698cluster wPt-2127 127.5 wPt-8658 157.6 161.9 168.0 196.4 204.0 206.2 218.1 229.0 237.0 244.9 barc346 gwm2 barc356 344008cluster wPt-0797cluster wPt-1652cluster wPt-2866 wmc11 wPt-1111 345152cluster S/FS-P GFD-C wPt-6711cluster wPt-5029cluster wPt-1657 gwm515 gwm95 gwm372cluster wPt-1142cluster 348413cluster gwm294 gwm312 wPt-7024 381146 wPt-9277cluster wPt-1615cluster wPt-9797 wPt-1499cluster wPt-6687cluster 0.0 9.6 29.6 35.2 38.6 56.7 68.4 FS/S-P 74.3 81.0 86.2 107.4 108.4 110.7 113.8 120.6 142.9 145.5 146.8 155.7 191.0 201.9 202.2 204.0 208.6 3A HT-P wPt-0164cluster wPt-5577 345666cluster wPt-5316 cfa2147 0.0 1.3 3.1 3.7 4.6 S/M2-P 191.5 199.9 214.7 217.8 223.9 gdm33cluster wPt-6358 304069cluster 344950cluster 377889cluster 378503 cfd15cluster 304991cluster wPt-7326 wPt-3904 barc148 cfd59 wmc278 gwm357 wPt-4765cluster S/M2-C 0.0 19.8 31.2 32.9 35.7 39.3 44.0 47.9 54.8 77.5 91.7 95.1 96.1 97.9 99.9 2A Figure 1 Genetic linkage map for the Tubbs x NSA 98-0995 population (TxN) with QTL positions. Distances are in Kosambi cM. “Cluster” at the end of a marker name denotes the use of a delegate marker. Solid boxes indicate the position of a QTL that has a positive additive effect for the Tubbs allele. Open boxes indicate a negative additive effect for the Tubbs allele. The trait abbreviations are “YLD” for grain yield, “PROT” for grain protein, “TWT” for test weight, “FLW” for growing degree days to flowering, “RIPE” for growing degree days to ripening, “GFD” for growing degree days of grain fill duration, “HT” for height, “S/M2” for spikes per square meter, “FS/S” for fertile spikelets per spike, “SS/S” for sterile spikelets per spike, “S/FS” for seeds per fertile spikelet, “S/S” for seeds per spike, and “SW” for seed weight. At the end of the trait abbreviations “-C” indicates the QTL is for Corvallis and “-P” indicates the QTL is for Pendleton. 75 4A 5A 196.1 200.4 217.8 306004cluster wPt-0687cluster 312808cluster 234.0 wPt-6768 255.6 gwm332 0.0 5.2 7.9 9.0 10.8 12.1 80.9 81.4 82.8 104.2 107.1 131.0 136.4 139.9 140.9 146.4 149.4 174.9 177.9 194.6 196.1 202.1 212.6 215.2 217.1 221.9 344418cluster wPt-0049cluster 343718cluster 305231 379274cluster wPt-0471 wPt-0047 305461cluster 348369 wPt-0950cluster wPt-0189cluster 345055 wPt-2430 wPt-5044 wPt-2327cluster wPt-4417cluster wPt-6471 345421cluster wPt-3561 wPt-9668 wPt-0746cluster wPt-8760 wPt-0477cluster wPt-1813 gwm614 wPt-0100cluster SW-C 348652cluster tPt-1772cluster barc156cluster wPt-1500 wPt-1568 wPt-0983cluster wPt-2654cluster wPt-0044cluster 372565 wPt-2859cluster barc8cluster 344609cluster 345641 344206cluster barc119.1 wPt-0441cluster wPt-1684cluster gwm413cluster wmc216 wPt-6690 wPt-2315 wPt-3579 wPt-0705 wPt-1403 rPt-9074 wPt-0944cluster 345746 wPt-1973 303896cluster 304031cluster 378539 GFD-C 143.5 2B YLD-P wPt-1928 wPt-7785 barc127cluster barc222 S/FS-P 97.1 100.0 107.4 125.6 0.0 1.0 2.2 4.2 7.3 8.7 12.3 15.9 18.2 32.8 36.5 60.2 62.8 67.2 71.5 75.2 77.8 93.8 106.7 111.0 111.2 112.3 137.5 152.5 154.2 163.4 192.3 194.6 197.5 198.5 TWT-C gwm666 wPt-0031 wPt-9255 tPt-6794cluster wPt-0008cluster 343497cluster wPt-8418cluster gwm635 305067cluster wPt-4835cluster FS/S-P 0.0 6.9 10.1 13.5 15.1 16.0 17.7 22.0 28.5 37.8 TWT-P SS/S-C Figure 1 Continued TWT-P gwm427cluster 344553 wPt-3247cluster wPt-2216cluster SS/S-P 164.1 164.7 170.7 171.5 1B FLW-C wPt-1377cluster 346131 tPt-6710 wPt-4270 wPt-0832 gwm334 wPt-0689cluster wPt-9759 wPt-8266 wPt-3965cluster wPt-0259cluster 375954cluster wPt-7063 gwm518 348276 303843 RIPE-P 0.0 0.9 2.0 3.7 5.6 20.0 23.4 26.6 28.3 33.3 34.6 35.2 74.7 78.0 93.8 96.2 HT-C 7A SW-P RIPE-C S/S-C RIPE-P SW-C 6A wPt-0373cluster 349403 gwm666 barc151 wPt-4262 345676 barc330 gwm186 373063 wPt-7769 348090cluster tPt-9702cluster wPt-3884cluster tPt-6183cluster barc56 barc186 gwm293 gwm304 wPt-4131 tPt-4184cluster gwm291 B1 wPt-4203cluster wPt-7061 HT-P PROT-C wPt-2788 wmc617 wPt-7924 wPt-0817cluster wPt-7939 wPt-6997 377680 311358cluster wPt-5124cluster wPt-2301 wPt-2291cluster rPt-2478cluster 373576 wPt-1007cluster wPt-6900 wPt-3491cluster wPt-0610 wPt-7590 wPt-0032cluster wPt-4620cluster 0.0 10.9 78.4 79.5 81.5 85.6 89.3 98.7 99.8 108.3 109.7 115.9 118.7 120.7 122.2 122.5 122.7 123.5 124.0 141.3 0.0 6.5 10.3 16.6 19.7 27.6 38.1 44.1 45.4 54.4 57.0 63.0 65.0 66.4 67.0 67.5 67.8 73.7 122.9 130.4 134.4 140.0 141.8 76 3B 4B HT-P gwm296 cfd51cluster SS/S-C wPt-3738 wPt-5320 gwm337 gwm458 wPt-3743 gwm642 0.0 8.2 SS/S-P 379913 wPt-4647cluster gdm33cluster wmc432cluster cfd15 FLW-C 2D FS/S-C FLW-P wPt-6156 wPt-3086cluster 78.2 83.1 88.5 97.1 99.5 102.6 S/S-C 159.7 160.3 0.0 2.7 25.2 37.4 41.4 RIPE-C RIPE-C wPt-8920 wPt-6936 orw5 tPt-8569cluster wPt-0577cluster wPt-5377 375919 wPt-5138cluster wPt-0217cluster SW-P 0.0 3.1 11.9 14.2 15.5 17.4 18.5 22.0 27.6 FS/S-P 1D GFD-C wPt-1261cluster wmc149cluster wPt-0708cluster wPt-1302 wPt-0419cluster wPt-1784 barc4cluster 303942 310624 wPt-0318cluster wPt-9467 378650cluster wPt-2273cluster wPt-0103cluster 349448 303987 303931cluster wPt-1895cluster 305092cluster wPt-3457cluster wPt-3329 tPt-1253 wPt-3204cluster wPt-4418 346078cluster 345374cluster 304364 311893cluster 311648cluster wPt-0837 SW-C TWT-P Figure 1 Continued 0.0 1.1 20.6 22.8 24.2 27.1 39.1 72.6 78.9 80.7 123.4 125.7 127.1 128.7 136.3 140.9 144.9 159.8 162.0 172.1 175.6 178.6 180.0 182.4 188.7 199.8 224.7 232.9 235.6 249.9 SW-C FS/S-C 7B wPt-5234cluster 348774 wPt-1547cluster 344152cluster wPt-3116 wPt-1241 wPt-5256cluster wPt-0293cluster 381509cluster wmc494cluster 343986cluster wPt-8721 377899 346705 wPt-3657 gwm608 gwm193 wPt-2726 barc79cluster wPt-4924 wPt-3581cluster tPt-4990 wPt-8554 tPt-3689 wPt-9270 wPt-1048 cfd45 wPt-0696cluster 344410cluster wPt-0171cluster FS/S-P HT-C wmc617 348732 wPt-4535 barc90cluster tPt-0602 gwm513 gwm495 gwm251 304777 wPt-0391 344980cluster 0.0 7.2 34.2 34.8 38.1 40.1 43.4 46.1 55.8 68.8 76.3 6B 0.0 1.3 3.3 7.0 7.9 35.6 38.2 47.0 54.3 59.7 61.4 64.2 65.3 70.6 72.5 74.5 75.2 78.1 81.7 85.0 85.5 87.8 91.3 93.2 101.1 103.8 128.1 147.3 156.3 156.8 5B HT-P GFD-P wPt-7984 wPt-1867cluster wPt-3921cluster wPt-9066 wPt-5064 wPt-0013cluster wPt-0688cluster 348055cluster wPt-6239 wPt-6945 wPt-4209 381874cluster wPt-5390 304025cluster wPt-1171 wPt-3107 wPt-4428 wmc326cluster wPt-4933 wPt-2491 wPt-8206 wPt-6834 gwm547cluster wPt-0280cluster wPt-1311 gwm247 0.0 2.7 3.7 11.9 21.1 36.1 36.2 50.1 54.7 57.0 58.6 63.1 64.6 66.9 92.9 104.2 118.8 135.5 137.6 141.5 171.1 174.6 177.0 179.8 180.2 181.8 77 3D 4D wmc11 gwm161cluster wPt-1034cluster gwm533cluster 246.5 barc71 333.1 336.9 wmc656 barc42 cfd14 gdm46 barc97cluster wPt-0695cluster wPt-0493 265.6 wPt-3018cluster 289.2 301.3 303.8 wPt-0827cluster wPt-3923cluster wPt-5674cluster Figure 1 Continued TWT-P 123.5 139.3 140.4 144.3 161.4 GFD-P wPt-1080cluster gwm350cluster gwm635 cfd31 gwm44 gwm111 gwm473 6D 0.0 gwm583 16.9 barc144 63.4 72.6 77.1 80.6 88.9 gwm272 wPt-0400cluster 347042 wPt-5870 gdm63 192.0 7D 0.0 1.2 3.2 4.1 5.8 9.1 15.3 SW-C 167.4 171.4 173.1 175.2 wmc720 wmc473cluster wmc331 gdm125 wPt-4572 53.6 54.7 68.3 72.4 75.7 SW-P gdm99 wPt-1994 wPt-8130 wPt-8463 wPt-6066 wPt-8356 wPt-2013cluster gdm72 barc356 SS/S-P 57.0 63.0 63.6 67.9 69.3 70.2 71.6 92.2 103.5 barc217 0.0 SS/S-C wPt-5313 0.0 5D wmc357 0.0 65.6 70.1 wPt-1695 wmc773cluster gwm469 121.1 gdm36 143.8 cfd45 78 1A 2A 57.7 cfd59 RIPE-C FLW-C tPt-6376 wPt-1888cluster wPt-1036 305077cluster wmc169 gwm666 wPt-5173 wPt-3697cluster wPt-2127 wPt-1562cluster tPt-3563cluster wPt-11619 wPt-0714 wPt-2910cluster gwm2 barc346 tPt-1143 gwm6661 barc356 FLW-P gwm294 wPt-7024 gwm312 wPt-3244 FS/S-C 200.9 203.6 203.9 213.2 0.0 0.3 4.3 7.9 11.1 16.9 32.2 58.2 61.8 81.6 98.0 114.1 119.0 139.6 142.3 144.9 151.4 167.8 169.1 HT-P wPt-1615cluster wPt-1499cluster wPt-6775 wPt-2696 wPt-1657 wPt-6711cluster tPt-9405cluster wPt-0003cluster cfd36cluster wPt-5738cluster barc124cluster wPt-0128cluster 345256cluster gwm636 wPt-1142cluster gwm372cluster gwm95 gwm515 wPt-0094cluster FS/S-P wmc278 gwm357 barc83cluster wPt-8797 wPt-9757 wPt-4384 wPt-5316 345666cluster wPt-8016 wPt-4399 wPt-7339 wPt-5577 0.0 0.2 0.4 1.4 7.7 33.3 36.6 38.0 39.4 105.7 106.2 107.4 109.9 113.1 113.6 119.9 126.8 132.3 143.1 S/S-C SS/S-P 100.4 101.6 112.4 116.4 121.5 128.0 128.3 144.7 160.6 164.2 168.8 173.3 SW-P 377889cluster 304991cluster wPt-2150 wPt-7326 wPt-3904 GFD-P 0.0 18.2 22.9 24.1 28.9 3A Figure 2 Genetic linkage map for the larger Einstein x Tubbs population (ExT1) with QTL positions. Distances are in Kosambi cM. “Cluster” at the end of a marker name denotes the use of a delegate marker. Solid boxes indicate the position of a QTL that has a positive additive effect for the Tubbs allele. Open boxes indicate a negative additive effect for the Tubbs allele. The trait abbreviations are “YLD” for grain yield, “PROT” for grain protein, “TWT” for test weight, “FLW” for growing degree days to flowering, “RIPE” for growing degree days to ripening, “GFD” for growing degree days of grain fill duration, “HT” for height, “S/M2” for spikes per square meter, “FS/S” for fertile spikelets per spike, “SS/S” for sterile spikelets per spike, “S/FS” for seeds per fertile spikelet, “S/S” for seeds per spike, and “SW” for seed weight. At the end of the trait abbreviations “-C” indicates the QTL is for Corvallis and “-P” indicates the QTL is for Pendleton. 79 4A 5A wPt-2788 55.5 wPt-6748cluster tPt-1772cluster wPt-1568 wPt-2654cluster wPt-8627 wPt-0983cluster wPt-0044cluster wPt-2859cluster wPt-3465 344609cluster wPt-4574 barc8cluster wPt-0441cluster barc1191 gwm413cluster wPt-2461 wPt-6690 wPt-2315 wPt-0705 wPt-1201cluster FLW-C FS/S-P Figure 2 Continued wPt-4229cluster wPt-4445 wPt-3247cluster tPt-4178cluster wPt-5310 gwm518 2B RIPE-C 0.0 7.9 11.6 14.2 16.1 39.4 41.9 48.6 80.9 87.7 91.4 97.4 105.3 107.2 112.5 113.4 116.1 118.5 SW-C FS/S-C gwm635 304885cluster gwm666 343497cluster wPt-8418cluster tPt-6794cluster wPt-1885 wPt-0008cluster wPt-9255 wPt-6959 wPt-0031 wPt-9651 barc70cluster wPt-1179cluster wPt-0321 barc127cluster wPt-1446 barc222 117416cluster wPt-0514 wPt-3992cluster wPt-0433 wPt-5987 gwm332 wPt-11723 wPt-4831cluster wPt-3425 wPt-1976cluster wPt-0687cluster 306004cluster YLD-C 0.0 1.4 4.9 53.5 54.6 55.3 64.2 75.1 77.7 122.1 125.2 130.4 151.2 171.0 171.3 184.9 225.7 228.1 230.0 245.2 249.1 251.5 255.0 255.4 255.9 256.4 258.6 259.4 261.9 265.7 1B wPt-1285 wPt-4047 tPt-6710 wPt-1664cluster wPt-4270 117493cluster gwm334 wPt-0689cluster wPt-9759 wPt-8266 tPt-6278 TWT-C 7A SS/S-P wPt-1200 wPt-4203cluster wPt-7061 gwm291 B1 SS/S-C 0.0 1.5 2.2 8.8 14.4 84.6 85.3 85.5 87.9 111.7 132.8 SW-P wPt-0373cluster FS/S-P 154.4 0.0 4.1 5.8 9.0 12.8 14.4 15.6 17.4 24.0 HT-C S/FS-P TWT-P wPt-4544 rPt-2478cluster wPt-6757 wPt-0421cluster wPt-1007cluster wPt-2291cluster 311358cluster wPt-7096cluster wPt-5124cluster wPt-2301 wPt-6900 wPt-0610 tPt-9948cluster wPt-7590 wPt-3491cluster wPt-0032cluster 107.1 127.9 143.3 143.6 153.6 155.4 161.3 161.5 163.7 171.9 173.3 173.4 175.8 195.5 195.7 wPt-1165 wPt-4131 barc186 barc56 gwm293 wPt-3884cluster gwm304 gwm186 rPt-3563 wPt-3187 barc330 wPt-4419 wPt-0707cluster barc151 wPt-4262 gwm666 S/S-C 21.6 0.0 16.2 21.1 23.1 50.9 52.0 53.3 59.8 60.2 61.3 90.0 91.1 93.0 96.2 99.6 111.7 S/FS-C wmc617 FS/S-C TWT-C 0.0 6A 0.0 17.1 20.8 53.9 59.4 83.0 86.7 88.6 89.0 90.0 108.1 109.9 112.6 113.8 117.6 128.7 142.9 159.3 166.8 173.2 182.3 193.9 205.7 208.5 214.7 215.6 226.6 251.1 259.3 273.6 wPt-5017 343718cluster wPt-6643 wPt-0471 gwm526cluster wPt-0694cluster wPt-9257 wPt-0697 wPt-3383cluster wPt-0473 wPt-8460 wPt-0489cluster wPt-0189cluster wPt-0950cluster wmc175 wPt-2327cluster wPt-2110 wPt-4417cluster wPt-6471 wPt-2314 wPt-0408 wPt-7715 345421cluster wPt-3561 wPt-1489cluster wPt-8349 tPt-4627cluster wPt-9859 wPt-0746cluster wPt-0100cluster 80 3B 4B 7B wPt-3284 wPt-4388cluster wPt-2564 wPt-3309cluster wPt-4119 wPt-1241 rPt-0029 wPt-6441 269.1 272.8 wPt-3657 gwm608 Figure 2 Continued 2D 0.0 5.8 wPt-2026 38.4 64.3 66.0 75.4 wPt-6963 barc229cluster cfd92 FS/S-C 239.6 0.0 SW-C wPt-3207cluster wPt-9256 wPt-1541cluster 344410cluster wPt-1264cluster wPt-7636 TWT-C 168.1 168.9 171.8 172.6 173.0 188.0 1D wPt-6936 wPt-8920 wPt-0837cluster orw5 tPt-8569cluster wPt-5216cluster wPt-4620cluster wPt-5377 wPt-0577cluster wPt-5138cluster wPt-4054 wPt-0217cluster wPt-7720 wPt-8040 wPt-3939 wPt-2356 wPt-0194cluster wPt-4258cluster wPt-1266 gwm111 wPt-3723 wPt-1826 SW-P 0.0 1.0 2.8 56.8 65.0 66.9 75.2 81.5 82.5 85.6 86.2 91.1 93.4 109.4 112.1 123.1 125.6 128.2 130.6 136.7 142.0 143.8 TWT-C gwm251 wPt-1261cluster wmc149cluster rPt-6127 barc216cluster wPt-1784 barc4cluster wPt-0318cluster wPt-1505 348314cluster 378650cluster wPt-0419cluster wPt-6878cluster 305092cluster wPt-1895cluster wPt-3457cluster wPt-9454 wPt-6014 wPt-3030cluster wPt-1304 wPt-3204cluster wPt-1881 wPt-0935cluster tPt-1253 wPt-3329 wPt-2514cluster wPt-7006 220.6 wPt-3855 295.3 cfd48 gwm296 gwm261cluster gwm6 HT-P 0.0 6.9 10.8 22.9 38.6 39.4 55.5 165.9 0.0 28.9 32.5 35.7 43.2 44.7 48.3 51.8 62.8 63.1 82.8 89.5 94.8 97.7 112.1 134.6 158.0 176.2 182.9 190.2 192.1 198.8 202.9 211.6 219.8 250.8 FLW-C 6B rPt-6847 HT-P wPt-8021cluster wPt-0367 wmc326cluster 140.1 HT-C wPt-3342cluster 300.5 313.4 327.1 gwm149 gwm664 wmc617 barc90cluster wPt-3991 wPt-8397 barc20cluster tPt-0602 gwm513 gwm495 TWT-C 285.1 0.0 4.8 14.9 17.0 20.3 22.8 23.9 26.3 27.0 65.4 FS/S-P wPt-8910 wPt-0013cluster wPt-0688cluster wPt-6945 wPt-4209 wPt-6020 381874cluster 348055cluster barc068 tPt-4541cluster wPt-7158 gwm547cluster wPt-6834 wPt-8206 S/FS-C 141.6 166.0 172.5 179.4 186.7 187.4 204.7 205.8 211.0 240.1 245.5 248.1 251.5 255.5 RIPE-C wmc11 wPt-3041 wPt-4352 barc57cluster wPt-1867cluster wPt-7984 wPt-3921cluster barc133 wPt-9066 S/S-C 0.0 24.6 38.1 43.6 59.6 68.4 70.0 71.5 71.9 5B 110.6 wPt-0638cluster 152.1 163.0 wmc18 wPt-0298 81 3D 4D gwm3 261.4 barc323 7D 0.0 11.7 barc126cluster gwm44 87.0 88.3 gwm473 wPt-7508 123.0 136.1 146.1 GDM99 GDM67 wPt-1859 216.3 wPt-1080cluster 237.0 gwm635 285.0 cfd31 Figure 2 Continued wPt-0472cluster HT-C 242.3 23.2 YLD-C gwm161cluster gwm533cluster wPt-1034cluster wmc11 wmc473cluster wPt-3058 FLW-C 144.1 146.4 147.1 148.7 0.0 0.7 HT-P gwm52 GDM72 wPt-8356 wPt-1994 wPt-2013cluster wPt-6066 wPt-8130 wPt-7847 0.0 23.8 40.6 43.4 44.4 45.2 59.5 5D 6D 0.0 5.7 12.0 gwm583 wPt-2256 cfd8 65.2 GDM63 109.8 gwm292 173.5 174.8 wmc161 wPt-9169 wPt-0162 244.7 249.6 264.4 gwm272 wPt-0400cluster wPt-1197 0.0 0.6 152.4 GDM127 cfd33 cfd49 82 1A 377889cluster 304991cluster wPt-2150 wPt-7326 wPt-3904 wmc278 cfd59 gwm357 wPt-8797 barc83cluster wPt-9757 wPt-4384 113.7 wPt-5316 139.4 145.8 148.1 150.5 345666cluster wPt-4399 wPt-8016 wPt-7339 wPt-5577 wPt-0164cluster gwm636 tPt-2481 345256cluster wPt-6711cluster wPt-5029cluster 88.1 92.3 94.2 96.0 116.3 119.5 128.8 129.4 gwm95 gwm515 wPt-1142cluster gwm372cluster gwm294 gwm312 wPt-7024 wPt-0094cluster 159.2 wPt-1499cluster 174.7 wPt-1615cluster 225.3 230.0 236.2 wPt-9797 wPt-6687cluster wPt-7009 gwm666 wPt-1036 wPt-1888cluster tPt-6376 wmc169 305077cluster wPt-2698cluster wPt-1277 wPt-3697cluster wPt-2127 wPt-1562cluster tPt-3563cluster wPt-11619 gwm2 barc346 barc356 gwm6661 rPt-9057 tPt-1143 wPt-2910cluster wPt-0714 wPt-1652cluster wPt-1111 wPt-2866 wmc11 wPt-4352 345152cluster barc57cluster SS/S-P 24.8 27.4 30.7 34.0 0.0 18.5 19.8 27.9 32.7 38.0 52.1 57.5 83.8 92.3 93.3 95.2 95.5 95.9 101.3 119.2 120.6 147.3 156.9 170.1 175.9 176.4 200.6 203.8 219.1 220.6 238.4 242.3 S/M2-C 183.2 187.5 0.0 3A S/S-P 0.0 3.0 5.8 8.8 21.9 44.4 46.4 53.6 57.4 61.9 70.4 71.1 2A Figure 3 Genetic linkage map for the smaller Einstein x Tubbs population (ExT2) with QTL positions. Distances are in Kosambi cM. “Cluster” at the end of a marker name denotes the use of a delegate marker. Solid boxes indicate the position of a QTL that has a positive additive effect for the Tubbs allele. Open boxes indicate a negative additive effect for the Tubbs allele. The trait abbreviations are “YLD” for grain yield, “PROT” for grain protein, “TWT” for test weight, “FLW” for growing degree days to flowering, “RIPE” for growing degree days to ripening, “GFD” for growing degree days of grain fill duration, “HT” for height, “S/M2” for spikes per square meter, “FS/S” for fertile spikelets per spike, “SS/S” for sterile spikelets per spike, “S/FS” for seeds per fertile spikelet, “S/S” for seeds per spike, and “SW” for seed weight. At the end of the trait abbreviations “-C” indicates the QTL is for Corvallis and “-P” indicates the QTL is for Pendleton. 83 4A 5A wPt-2301 171.8 wPt-5124cluster 208.9 311358cluster 6A 0.0 gwm291 B1 wPt-1200 wPt-4203cluster wPt-7061 tPt-4184cluster 151.2 156.7 166.4 167.8 170.5 186.3 SS/S-P 144.7 SS/S-C wPt-0610 TWT-P 117.3 FLW-P wPt-6900 FS/S-C 90.6 wPt-0373cluster gwm666 wPt-0707cluster barc330 wPt-4419 gwm186 wPt-3187 rPt-3563 barc186 348090cluster tPt-6183cluster tPt-9702cluster gwm304 wPt-4131 wPt-3884cluster gwm293 barc56 0.0 16.3 54.8 55.7 56.6 66.2 66.8 70.1 85.1 87.2 89.8 90.7 92.6 94.7 96.9 99.3 S/S-P wmc617 wPt-2788 wPt-6748cluster wPt-7096cluster wPt-4544 rPt-2478cluster wPt-2291cluster wPt-1007cluster wPt-0032cluster wPt-7590 wPt-3491cluster tPt-9948cluster S/FS-P 0.0 2.0 9.4 10.6 11.3 14.0 14.4 15.3 20.4 22.3 55.3 7A wPt-5310 wPt-2582 tPt-6661 wPt-3247cluster wPt-4229cluster 93.5 wPt-4445 gwm518 S/M2-P wPt-0008cluster tPt-6794cluster wPt-8418cluster wPt-1885 343497cluster wPt-0031 wPt-6959 wPt-9255 gwm635 gwm666 304885cluster wPt-9651 wPt-6824 wPt-1179cluster wPt-4835cluster wmc283cluster barc127cluster wPt-1446 barc222 wPt-0321 117416cluster wPt-3992cluster wPt-0514 wPt-0433 wPt-5987 wPt-0961cluster wPt-3425 wPt-6768 gwm332 HT-P 52.2 53.5 54.6 55.2 56.6 60.3 63.2 64.5 71.0 72.4 73.3 91.2 98.1 98.5 105.2 133.7 136.7 139.0 162.6 173.2 191.1 195.5 200.3 221.0 225.8 245.1 249.1 259.6 273.4 0.0 19.9 36.8 39.3 41.8 42.4 57.2 86.5 92.1 98.6 119.8 127.2 130.8 133.7 141.8 142.4 145.7 148.0 148.4 149.2 154.5 154.9 HT-C Figure 3 Continued 306004cluster wPt-0687cluster wPt-1976cluster FS/S-C 214.3 S/FS-P tPt-6278 wPt-0689cluster wPt-8266 gwm334 tPt-6710 wPt-4047 wPt-1285 wPt-1664cluster wPt-4270 117493cluster wPt-9759 S/FS-C 135.3 142.4 144.6 150.0 152.6 158.0 160.2 163.7 165.7 170.0 0.0 1.8 7.1 barc156cluster wPt-1500 wPt-0983cluster wPt-2654cluster wPt-8627 wPt-1568 tPt-1772cluster wPt-2859cluster wPt-0044cluster 344609cluster wPt-4574 wPt-3465 barc8cluster gwm413cluster wPt-0441cluster barc1191 wmc216 wPt-6690 wPt-2315 wPt-3579 wPt-1201cluster wPt-0944cluster rPt-9074 wPt-4651 GFD-P 54.5 61.5 66.4 69.8 1B 84 2B 3B 0.0 22.7 24.0 28.6 32.3 35.9 45.1 47.2 48.3 67.0 77.2 88.4 92.8 94.3 wPt-0049cluster 343718cluster wPt-5017 0.0 5.2 15.1 wPt-0391 HT-C HT-P wPt-8206 wPt-7158 wPt-6834 gwm547cluster wPt-0280cluster 6B wPt-2514cluster 348314cluster Figure 3 Continued wPt-2175 wPt-0293cluster cfd1cluster 381509cluster wmc494cluster gwm518 barc101cluster wPt-7489 wPt-2726 tPt-3689 wPt-8554 wPt-4924 wPt-3581cluster tPt-4990 wPt-9231 barc79cluster wPt-3657 gwm193 gwm608 wPt-6441 344410cluster wPt-0171cluster 0.0 17.8 22.2 27.5 31.5 33.6 37.3 38.0 39.5 40.8 47.4 49.2 57.6 60.8 64.1 72.8 75.8 79.2 88.4 164.8 165.4 166.9 wPt-6936 wPt-8920 wPt-0837cluster FS/S-C 171.9 181.9 132.4 150.7 151.2 152.7 157.6 159.6 162.9 165.7 169.5 171.6 171.7 173.8 176.9 178.4 179.3 184.0 189.1 192.4 197.3 226.7 232.7 1D wPt-4620cluster wPt-5216cluster orw5 tPt-8569cluster wPt-5377 wPt-0577cluster wPt-5138cluster wPt-4054 wPt-7720 wPt-0217cluster wPt-8040 wPt-3939 wPt-2356 wPt-0194cluster wPt-1266 wPt-3723 wPt-1826 gwm111 wPt-4258cluster HT-C wPt-1302 barc232cluster wPt-1304 wPt-0935cluster wPt-1881 wPt-1547cluster wPt-3774cluster RIPE-C 72.6 81.8 82.8 86.2 96.9 0.0 1.8 7B PROT-P wPt-0708cluster GFD-C 0.0 S/M2-C 189.6 GFD-P rPt-6847 SS/S-C 164.5 SS/S-P gwm251 RIPE-C 114.9 S/S-P gwm495 RIPE-P 91.6 HT-P gwm149 gwm664 wmc617 wPt-0246cluster wPt-8397 barc20cluster wPt-3991 barc90cluster tPt-0602 gwm513 wPt-0065 YLD-P 5B 212.4 217.9 223.2 224.6 233.6 0.0 26.4 31.9 33.5 34.3 34.7 39.2 42.4 43.4 44.5 S/FS-P 139.4 barc068 wPt-6945 wPt-4209 wPt-6020 381874cluster 348055cluster wPt-8910 wPt-0688cluster wPt-0013cluster wPt-9066 barc133 wPt-7984 wPt-3921cluster wPt-1867cluster HT-C wPt-0100cluster wPt-0746cluster wPt-9859 tPt-4627cluster wPt-1489cluster wPt-3561 wPt-9668 345421cluster wPt-7715 wPt-2110 wPt-0408 wPt-2314 wPt-6471 wPt-4417cluster wPt-2327cluster wmc175 wPt-0189cluster wPt-0489cluster wPt-0950cluster wPt-8460 wPt-9257 wPt-0697 wPt-0473 wPt-0694cluster 86.1 97.4 107.3 122.7 136.0 143.0 146.1 153.0 161.4 180.1 191.7 199.0 204.5 211.4 226.7 232.0 237.4 239.4 247.3 249.5 259.3 260.6 264.3 4B 0.0 15.8 17.1 wPt-2026 wPt-6963 barc229cluster 67.1 cfd92 85 2D 3D gwm3 220.6 barc323 237.5 barc71 268.4 cfd60 5D 6D wPt-2256 32.9 42.2 43.5 cfd8 gwm583 gwm292 76.5 gwm272 108.6 109.8 111.5 0.0 1.8 wPt-0400cluster wPt-1197 GDM63 0.0 1.9 S/M2-C 0.0 7D GDM127 cfd33 0.0 8.0 barc126cluster gwm44 34.3 44.7 46.0 gwm111 gwm473 cfd14 71.9 73.8 82.5 95.7 GDM46 GDM99 GDM67 wPt-1859 183.5 gwm635 212.0 222.5 226.9 cfd31 wmc463 wPt-1100cluster 269.0 270.8 274.7 275.9 278.1 282.4 wPt-3923cluster wPt-5674cluster wPt-0493 wPt-3018cluster wPt-0695cluster barc97cluster wmc161 wPt-9169 wPt-0162 Figure 3 Continued HT-C 206.5 TWT-C wPt-0619cluster wPt-0638cluster gwm52 GDM72 wPt-8356 wPt-1994 wPt-2013cluster wPt-6066 wPt-8130 wPt-7847 wPt-3058 wmc473cluster wPt-0472cluster HT-P 201.0 205.2 81.9 95.2 106.3 109.6 110.7 112.0 116.0 130.8 0.0 0.6 16.9 RIPE-C wPt-4691cluster wPt-9580 gwm161cluster wmc11 gwm533cluster wPt-1034cluster PROT-P 91.3 98.9 0.0 4.6 6.6 7.2 S/M2-P gwm261cluster gwm296 wmc18 wPt-0298 gwm608 SS/S-P 0.0 2.7 5.9 6.1 10.4 4D