Multivariate Analysis in Twins

1970 ◽  
Vol 19 (1-2) ◽  
pp. 150-154 ◽  
Author(s):  
E. Defrise-Gussenhoven

We present the results of a noncentral χ2 test applied to 63 like-sexed twin pairs.We have separated the pairs into two groups: 30 serologically identical and 33 serologically nonidentical pairs for nine sera of the blood groups ABO, MN, and Rh.The probabilities of monozygosity of the serologically identical pairs, calculated by the method of Maynard-Smith and Penrose, range from 0.83 to 0.92 — rather small values. With the help of Belgian frequencies of DZ and MZ twins, we could prove that there are about 50% chances of having less than two DZ pairs amongst the 30 serologically identicals.Consequently, our first group with 30 pairs is mostly MZ (less than 7 DZ pairs in 96% of the cases); while our second group, with 33 pairs, is completely DZ.We did not try to extract out of the 30 serologically identicals, such pairs that might “seem” DZ. For instance, we have kept in our first group two twins — one with blue and one with brown eyes — because the genetics of eye colour is not yet enough well-known to be safely used in twin-diagnosis; and also in memory of Madame de Sévigné, who had one brown and one blue eye. Imperfect as the composition of our sample is, we have avoided at least one mistake: adding, to surely DZ pairs, twins who are “seemingly” DZ, but not proven to be so.

1952 ◽  
Vol 17 (1) ◽  
pp. 175-182
Author(s):  
MOGENS HAUGE ◽  
HANS FR. HELWEG-LARSEN
Keyword(s):  
Red Hair ◽  

1971 ◽  
Vol 20 (1) ◽  
pp. 96-113 ◽  
Author(s):  
Charlotte C. Taylor

SummaryFifty marriages of twins to twins have been studied. Most of them have the characteristics of MZ twins. All have an identical outcome of their marriages within each set. This finding and others from the literature are consistent with the idea that marital stability depends in part upon one's original “blueprint” for physical and emotional health.Two findings in this study, and others from the literature, are consistent with the idea that similarities at the chemical level may in general tend to promote a better understanding of each other and hence more congenial relationships: (a) all but one of the twin foursomes have lived closeby; three-quarters of them share the same house, even after they have had children; and (b) there is some degree of similarity in the ABO and Rh blood groups between husbands and wives in this sample.The stably-married twins knew each other for an average of four years before marriage, whereas the divorced and annulled ones met only a few weeks or months before marriage.


1976 ◽  
Vol 25 (1) ◽  
pp. 164-166
Author(s):  
D.P. Pace ◽  
F. Saccucci ◽  
F. Britti ◽  
D. Casini

The distribution of A1A2BO, MN, and Rh-Hr blood groups, of salivary ABH substances, and of natural antibodies, was assessed in a sample of 47 MZ twin pairs. The resulting distribution provides indications as to the level of genetic control over the quantitative expression of these traits.


Author(s):  
José Antonio Sainz Bueno ◽  
Lucas Cerrillos González ◽  
Alejandra Abascal-Saiz ◽  
María Victoria Rodríguez Gallego ◽  
Rocío López Pérez ◽  
...  

1966 ◽  
Vol 24 ◽  
pp. 188-189
Author(s):  
T. J. Deeming

If we make a set of measurements, such as narrow-band or multicolour photo-electric measurements, which are designed to improve a scheme of classification, and in particular if they are designed to extend the number of dimensions of classification, i.e. the number of classification parameters, then some important problems of analytical procedure arise. First, it is important not to reproduce the errors of the classification scheme which we are trying to improve. Second, when trying to extend the number of dimensions of classification we have little or nothing with which to test the validity of the new parameters.Problems similar to these have occurred in other areas of scientific research (notably psychology and education) and the branch of Statistics called Multivariate Analysis has been developed to deal with them. The techniques of this subject are largely unknown to astronomers, but, if carefully applied, they should at the very least ensure that the astronomer gets the maximum amount of information out of his data and does not waste his time looking for information which is not there. More optimistically, these techniques are potentially capable of indicating the number of classification parameters necessary and giving specific formulas for computing them, as well as pinpointing those particular measurements which are most crucial for determining the classification parameters.


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